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+50.9 0 32 (dressed by 32\255bit clients.  It will also be possible to mount disks from 64\255bit systems on 32\255bit) W
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+79.6 0 32 (Programs that do not read or write data containing pointers or long variables will have a great) W
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+(duce or consume data for 32\255bit programs should run unchanged.) h
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+102.9 0 32 (definition changes.  Programs that must deal with data containing 32\255bit pointers may require) W
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+300 -6000 M
+300 -7400 M
+300 -9400 M
+300 -10836 M
+-7200 7200 T
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+
+showpage
+$P e
+
+%%Trailer
+$D restore
+end % DEC_WRITE_dict
+%%Pages: 8
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diff --git a/alpha_portability.ps b/alpha_portability.ps
new file mode 100644
index 0000000000000000000000000000000000000000..d6685d3db9caf75ad711bd18ed2d9906ffb06b15
--- /dev/null
+++ b/alpha_portability.ps
@@ -0,0 +1,2635 @@
+%!PS-Adobe-2.1
+%%Creator: DECwrite T2.0-IFT
+%%+Copyright (c) 1990 DIGITAL EQUIPMENT CORPORATION.  
+%%+All Rights Reserved.
+%%DocumentFonts: (atend)
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+getinterval putinterval}for pa py pw put}for}def/pat2{/pi exch def/cflag
+exch def save cflag 1 eq{eoclip}{clip}ifelse newpath{clippath
+pathbbox}stopped not{/ph exch def/pw exch def/py exch def/px exch def/px px
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+translate/pw pw px sub 3072 div floor 1 add cvi def/ph ph py sub 3072 div
+floor 1 add cvi def pw 3072 mul ph 3072 mul scale/pw pw 32 mul def/ph ph 32
+mul def/px 0 def/py 0 def pw ph pi[pw 0 0 ph 0 0]{pa py get/px px 32 add
+def px pw ge{/px 0 def/py py 1 add 8 mod def}if}pi type/booleantype
+eq{imagemask}{image}ifelse}if restore}def/PS{/_op exch def/_np 8 string def
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+11 3 13 5 9 1 14 6 10 2 12 4 8 0]exch get}def/FR{0.7200 0 $E defaultmatrix
+dtransform/yres exch def/xres exch def xres dup mul yres dup mul add
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+def/rm _sa $R rotate def/sm _cs dup $L scale def sm rm _mm _mm concatmatrix
+_mm concatmatrix pop 1 0 _mm dtransform/y1 exch def/x1 exch def/_vl x1 dup
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+_pn 0 _p1 putinterval _pn _p1 length _p2 putinterval _pn
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diff --git a/batch.txt b/batch.txt
new file mode 100644
index 0000000000000000000000000000000000000000..bcedc4e6a8807a468500ae17878be27419201791
--- /dev/null
+++ b/batch.txt
@@ -0,0 +1,321 @@
+Betreft:
+Batch processing in Newstar
+---------------------------
+
+Waarde heren,
+
+Ik heb wat details van DWARF opgespoord ten behoeve van automatische 
+processing. Hieronder volgt een voorlopig overzicht. Een aantal zaken 
+staat al in het Cookbook: Program Descriptions, Common.
+
+
+1e. DWARF Keywords, streams
+---------------------------
+
+Een gebruiker heeft invloed op de werking van een Newstar programma via
+de DWARF user-interface. Alle grootheden/parameters die een gebruiker
+in principe kan specificeren corresponderen met keywords, die een 
+waarde hebben. Die waarde kan op een aantal niveaus bepaald worden:
+
+   1e. Interne of program defaults:
+         De programmeur heeft een default waarde meegegeven bij de
+         definitie van het keyword (in de zgn. PIN-file). In een 
+         (beperkt) aantal gevallen staat er geen default in de PIN-file
+         maar geeft het programma zelf een default mee.
+
+   2e. Externe defaults:
+         De gebruiker heeft, buiten het programma om, een waarde 
+         gegeven aan het keyword door een DWARF symbool te definieren
+         (met dwspecify, met dwrestore, of door het programma eerder 
+         te gebruiken met de /SAVE switch)
+
+Voor een aantal algemene keywords wordt de externe default op twee 
+plaatsten gezocht: eerst in een tabel met defaults voor het programma
+(de "local" external default), als daar geen waarde staat in de algemene
+tabel (de external default van "NGEN").
+
+   3e. Het programma prompt de gebruiker voor het keyword en krijgt 
+       een waarde via toetsenbord of input-file. 
+
+Normaliter gaan de antwoorden die de user geeft op keyword prompts verloren
+wanneer het programma wordt verlaten. Er zijn twee manieren om een keyword
+te bewaren (alsof het met dwspecify was gegeven):
+
+   - Voor alle keywords de waarde bewaren: start programma met 
+         dwe <programma> /SAVE
+
+   - Voor individuele keywords de waarde bewaren: geef na de prompt
+         waarde /SAVE [/[NO]ASK]    (zie ook onder 3e)
+
+
+Op elk niveau kan een qualifier (switch) /ASK of /NOASK worden meegegeven.
+Deze bepaalt of de gebruiker voor het keyword geprompt wordt of niet
+(het opgeven van /[NO]ASK bij een prompt heeft alleen zin als ook de 
+/SAVE switch gegeven wordt).
+
+
+Met de /SAVE optie en dwspecify (= dws) kunnen vaste defaults voor een 
+programma worden gezet. Omdat het meestal wenselijk is verschillende 
+sets van defaults te gebruiken voor verschillende procedures kan een 
+programma in verschillende "streams" (wat was dat andere woord ook al 
+weer?) gestart worden. Elke "stream" heeft een eigen set defaults.
+
+Het commando om een programma te starten in een bepaalde "stream" is
+
+   dwe <programma>$<streamname>
+
+bv
+   dwe nscan$1
+   dwe nmap$standard
+   dwe nplot             default: stream 1
+
+Wanneer een keyword geen default heeft in de opgegeven stream wordt 
+een default in stream 0 gezocht, is daar ook niets dan blijft alleen
+de default van de PIN file over. Voor NGEN keywords wordt steeds zowel
+in de stream voor het programma als in de stream voor NGEN gezocht.
+
+ 
+
+2e. DWARF Symbols
+-----------------
+
+DWARF slaat externe defaults op als symbolen. Alle symbolen staan 
+fysiek in de file $DWARF_SYMBOLS (meestal ~/SYMBOL_DIR/SYMBOL.$$).
+
+Een DWARF keyword correspondeert met een symbool 
+
+     <Programma>$<Stream>_<Keyword>
+
+De waarde van het symbool is de character string die als default 
+gebruikt zal worden bij user-input, eventueel met de qualifier /ASK 
+of /NOASK er achter.
+
+Wanneer achter de waarde <space>/ASK staat, vervangt de waarde de default 
+van het programma, maar wordt de user toch geprompt voor het keyword.
+
+Wanneer achter de waarde <space>/NOASK staat, of wanneer er helemaal geen 
+qualifier staat, dan wordt de user niet meer voor het keyword geprompt.
+
+
+Naast deze keyword symbolen kunnen ook algemene symbolen gezet worden,
+die in antwoorden op prompts gebruikt kunnen worden, bv PI = 3.1415,
+NATUURLIJK = YES en zo voorts.
+
+
+De volgende utilities zijn beschikbaar om symbolen te manipuleren:
+
+
+ dwlet [symbol=value]  [/LOG[=long|short] [/NOLOG]   (= dwl)
+
+   Geef een waarde aan algemene symbolen. Kan niet gebruikt worden
+   om DWARF keywords te wijzigen.
+
+   Als er geen symbol=value wordt meegegeven wordt de standard input 
+   gelezen voor regels met "symbol=value", om te stoppen: lege regel 
+   of # of ^D.
+
+ dwspecify program[$stream] [/MENU] [/NOMENU]        (= dws)
+
+   Default stream is 1, default mode is /NOMENU.
+
+   Hiermee worden externe defautls voor DWARF keywords opgegeven.
+   Met /menu wordt voor elk keyword geprompt met de huidige 
+   (externe of interne) default, alleen wijzigingen worden in 
+   een symbool gezet. Met /nomenu worden van de standard input 
+   regels keyword=value gelezen.
+
+ dwclear [program[$stream]keyword,... [/CONFIRM] ...  (= dwc)
+
+   Verwijdert de definitie van de keywords, wildcards zijn toegestaan,
+   erg handig is bijvoorbeeld: dwclear nscan$*_*, om helemaal schoon
+   te beginnen.
+
+ dwsave  [program[$stream]keyword,... [/OUTPUT=file] [/CONFIRM] ... 
+
+   Default file is dwarfsave.sav, default extensie is sav
+
+   Schrijft de keywords en hun waarde in de genoemde (ASCII) file, 
+   wildcards zijn toegestaan. Default is *$*_*
+
+ dwrestore file [/CONFIRM] [/OVERWRITE]
+
+   Leest regels keyword=value van de genoemde file en definieert de
+   corresponderende symbolen.
+ 
+ dwview symbol,... [/EXTERN] [/GENERAL] [/INPUT=file] (=dwv)
+
+   Laat de waarde van symbolen zien:
+
+     Zonder /GENERAL en /INPUT:   
+       Symbols moeten de vorm [[program]$stream_]keyword hebben,
+       wildcards toegestaan. Laat zowel interne als externe defaults
+       zien, als /EXTERN alleen de externe (zowel "local" als "NGEN").
+
+     Met /INPUT:
+       Leest als dwrestore van de genoemde file, laat keywords zien      
+       die matchen met de genoemde symbols.
+
+     Met /GENERAL:   (optie gemaakt 28/07/93)
+       Symbols mag zowel DWARF keywords als algemene symbols bevatten,
+       wildcards toegestaan (bv: dwv /g *).
+       Voor keywords: alleen externde defaults worden getoond.
+       Als er precies een symbool is opgegeven is de uitvoer de 
+       waarde van dat symbool, anders regels symbol=value.
+
+
+Een typische manier om standard streams te gebruiken is dus:
+
+  dwe nscan$abc /save [/norun]       of   dws nscan$abc /menu
+  dwe nplot$abc /save [/norun]       
+
+  dwsave *$abc /output=abc
+
+Tenslotte commentaar invoegen in abc.sav, eventueel nog wat keywords 
+van de /ask switch voorzien.
+
+Dan bij gebruik:
+
+   dwrestore abc /override
+
+   dwe nscan$abc
+   dwe nplot$abc
+
+
+
+
+
+
+3e. Antwoorden op prompts
+-------------------------
+
+Het programma bepaalt (via de PIN file) wat voor antwoorden geldig zijn
+(character strings, numeric values). Binnen de grenzen van die geldigheid
+kunnen de volgende constructies worden opgegeven:
+
+   ?                     Geef online help
+
+   # of ^D               Exit (meestal: vraag vorige keyword)
+
+   ""                    Empty answer (meestal: by-pass option)
+ 
+   *                     Wildcard (meestal: take all)
+
+   ... ! Comment         Alles na een uitroepteken is commentaar
+
+   ...'Symbol'...        Het symbol wordt vertaald voor alle verdere 
+                           processing
+
+   (1=2)*4               Rekenkundige expressies worden uitgewerkt
+                           (alleen voor numerieke waarden, dus wel voor
+                            INPUT_LABELS, niet voor LOOPS)
+
+   99 TO 120 BY 2        Reeksen worden gegeven als begin TO eind BY stap
+                           (alleen voor numerieke waarden, dus wel voor
+                            INPUT_LABELS, niet voor LOOPS)
+
+   ... /SAVE [/[NO]ASK]  Bewaar deze waarde na afloop van het programma in
+                           een DWARF symbol. De qualifier /ASK of /NOASK
+                           wordt in het symbool bewaard (geen qualifier
+                           betekent in praktijk: /NOASK)
+
+   value1; value2; ...   Geef een reeks waardes op, de volgende keer dat
+                           het keyword wordt gevraagd neemt het programma
+                           de eerstvolgende waarde
+
+   value1,value2         Geef een vector op, alle waardes worden meteen
+                           naar het programma doorgegeven
+
+   /ASK=keyword          Wanneer het programma het opgegeven keyword 
+                           nodig heeft krijgt de gebruiker een prompt;
+ 			   als deze qualifier gegeven is wordt het 
+                           huidige keyword nog een keer gevraagd.
+
+
+
+Nota Bene: er is geen snelle manier om hidden keywords te zetten als
+           het programma al draait. Met dws is dat wel mogelijk.
+
+
+
+4e. Scripts en batch processing
+-----------------------------------------------
+
+Er zijn twee manieren om Newstar (of eigenlijk: DWARF) in batch mode
+te gebruiken. De simpelste manier lijkt me via shell scripts, waarin 
+keywords worden gelezen met dwrestore en vervolgens de nodige programma's
+worden gedraaid. 
+
+Er is (voor WENSS) een "Batch package" ontworpen om de interactie met
+de keyword files te vereenvoudigen. Voor zover ik kan zien is de enige
+functie het overnemen van de dwrestore en het zetten van /ASK achter
+een aantal keywords. Dit weegt denk ik niet op tegen de extra moeite om
+voor elk programma een "batch versie" te maken. Ik zal hier nog wat 
+beter naar kijken. Je hoort er nog van.
+ 
+
+5e. Voorstel voor wijzigingen en uitbreidingen
+----------------------------------------------
+
+De volgende wijzigingen in het huidige systeem lijken me wenselijk:
+
+  - Alternatieve specificatie voor streams omdat $ een Unix special 
+    character is. Ik stel voor om voor stream specificaties zowel
+    een $ als een . toe te staan (bv dwe nscan.test of dwe nscan$test).
+
+  - Van keywords die als symbol gedefinieerd zijn met /NOASK moet tijdens
+    de uitvoering van het programma het keyword en de waarde worden 
+    afgedrukt.
+
+
+Een "conditionele" batch processing kan vrij makkelijk worden gerealiseerd
+door de Newstar programma's bepaalde interne waarden in een (algemeen) 
+symbol te laten zetten. Die waarden kunnen dan in het shell script worden
+opgevraagd en getest. Bv: bij NSCAN kan het aantal Channels in symbol
+NCHAN worden gezet, in het shell script kan dan een test worden gedaan
+
+   if (`dwv /General nchan` == 128) then ...
+
+of de waarde kan in een shell variabele worden gezet
+
+   set channels=`dwv /g nchan`
+
+of de waarde kan worden toegekend aan een keyword voor een ander programma
+
+   dws nmap\$1 /NOMENU <_EOD_
+LOOPS='NCHAN',...1
+#
+_EOD_
+
+
+Wanneer jullie doorgeven op welke parameters je wilt testen is het een 
+kleine moeite die waarden in een symbol te zetten. Wanneer je een 
+programma met /SAVE draait zijn alle antwoorden van de user in elk
+geval beschikbaar in symbolen, dus daar kun je ook op testen.
+
+
+----------
+
+Tot zover maar weer even. Ik maak hier nog een fatsoenlijk (Engels) document
+van, maar hiermee kunnen jullie denk ik wel even vooruit.
+
+Hartelijk groeten,
+
+Marco.
+
+
+
+--
+
+
+ +--------------------------------------------------------------------------+
+ | NFRA/St. ASTRON      | eMail:  devoscm@astro.rug.nl         /  cccccccc  |
+ | P.O. Box 2           |  or:    devoscm@astron.nl            /   c m   m  c |
+ | NL-7900 AA Dwingeloo |                                  /    c m m m  c  |
+ |                      | ---------------------------------+  c  m   m  c   |
+ | Phone: +31 5219 7244  \  "If you reinvent the wheel,    |   v      v     |
+ | Fax:   +31 5219 7332   \  make sure yours will look     |    v   v       |
+ | Telex: 42043 rzm nl     | different..."                 |      v         |
+ +--------------------------------------------------------------------------+
+
+
+
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+Fb(Nature)f(..)i(p..)106 868 y(\(1981\))35 951 y([7])j(Corn)o(w)o(ell)
+14 b(T.J.)i Fd(...)f Fb(\(1983\))35 1034 y([8])21 b(Ek)o(ers)12
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+1897 y([...])41 b(...:)22 b Fd(...)935 2995 y Fa(1)p
+eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/bibliography/bibliography.html b/bibliography/bibliography.html
new file mode 100644
index 0000000000000000000000000000000000000000..b222798b7e059656301c114c28a5c013ac6d320e
--- /dev/null
+++ b/bibliography/bibliography.html
@@ -0,0 +1,87 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Bibliography</b>
+<P>
+ <P><H2>References</H2><P>
+<DL COMPACT>            <b><DT><A NAME=Brouw71><B>1</B></A><DD> Brouw W.N. <i>Data processing for the WSRT</i> PhD Thesis, Leiden (1971)
+<P>
+<DT><A NAME=Brouw72><B>2</B></A><DD> Brouw W.N. <i>Data processing for the WSRT</i> Handbook of Computational Physics (1972?)
+<P>
+<DT><A NAME=Hogbom74><B>3</B></A><DD> H&#246;gbom J.A.  <i>...</i> Astron.Astrophys.Suppl. 15, p417 (1974)
+<P>
+<DT><A NAME=Schwarz78><B>4</B></A><DD> Schwarz U.J.   <i>...</i> Astron.Astrophys. 65, p345 (1978)
+<P>
+<DT><A NAME=Clark80><B>5</B></A><DD>  Clark B.G.  <i>...</i> (1980)
+<P>
+<DT><A NAME=Noordam81><B>6</B></A><DD>  Noordam J.E. and De Bruyn A.G.  <i>High dynamic range observations of 3C84</i> Nature .. p.. (1981)
+<P>
+<DT><A NAME=Cornwell83><B>7</B></A><DD> Cornwell T.J.  <i>...</i> (1983)
+<P>
+<DT><A NAME=Ekers83><B>8</B></A><DD> Ekers R.D.  <i>The almost serendipitous discovery of SELFCAL</i> Proceedings of IAU Symposium nr ..., (&quot;Serendipitous discoveries in radio astronomy&quot;), K.Kellermann (ed), Green Bank U.S.A. (1983)
+<P>
+<DT><A NAME=Greve84><B>9</B></A><DD> Van Someren Greve H.W.  <i>...</i> NFRA Internal Technical Report 171 (1984)
+<P>
+<DT><A NAME=Spoelstra85><B>10</B></A><DD> Spoelstra T.A.Th.  <i>...</i> NFRA Note 477 (1985)
+<P>
+<DT><A NAME=Tan86><B>11</B></A><DD> Tan G.B.  <i>Multi Frequency Frontend (MFFE) receivers for the WSRT</i> (1986)
+<P>
+<DT><A NAME=Spoelstra88><B>12</B></A><DD> Spoelstra T.A.Th. <i>...</i> NFRA Note 429 (1988)
+<P>
+<DT><A NAME=DWARF><B>13</B></A><DD> Olnon F.M.  <i>DWARF Users Guide</i> (1991)
+<P>
+<DT><A NAME=Wieringa91><B>14</B></A><DD> Wieringa M. <i>327 MHz studies of the high redshift Universe and the galactic foreground</i> PhD Thesis, Leiden (1991)
+<P>
+<DT><A NAME=Brouw91c><B>15</B></A><DD> Brouw W.N. <i>The WNG programming environment, part 3: I/O (WNC, WNF, WND</i> NFRA ITR 197c (1991)
+<P>
+<DT><A NAME=...><B>...</B></A><DD>  ...: <i>...</i> 
+</b></DL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/bibliography/images.pl b/bibliography/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/bibliography/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/bibliography/labels.pl b/bibliography/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..d35805c9867870f3893b1bcdf95871618e8f6160
--- /dev/null
+++ b/bibliography/labels.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/bug_reports.txt b/bug_reports.txt
new file mode 100644
index 0000000000000000000000000000000000000000..0c65ed83723cb931125d341f93cfdd905f4af602
--- /dev/null
+++ b/bug_reports.txt
@@ -0,0 +1,434 @@
+Newstar Bug reporting procedure
+-------------------------------
+
+     bug_reports.txt  14/06/93 v1.0 CMV
+     bug_reports.txt  06/09/93 v1.2 CMV
+     JPH 940621	Add list of contents. Include bug_report.2 (=sec. 6.1)
+
+
+INHOUD
+======
+1. Inleiding
+2. Procedure
+3. Revisions en Releases
+4. Functionality Requests
+5. Implementatie: nbug
+6. Prioriteitsstelling
+6.1 Update on priorities
+7. Slotopmerkingen
+
+
+1. Inleiding
+------------
+
+Zolang een programmapakket door een beperkte groep gebruikt wordt, is
+er weinig noodzaak voor al te veel formele procedures. Naarmate het 
+pakket door een grotere groep, met een grotere geografische verspreiding
+wordt gebruikt werkt een aantal informele overlegcircuits niet meer en 
+moet er een aantal afspraken over tijdschema's en rapportage gemaakt worden.
+
+Die afspraken moeten het volgende garanderen:
+
+  1e. Gebruikers weten welke versie van het pakket voor hen draait,
+      en wat de (voornaamste) eigenschappen van die versie zijn.
+
+  2e. Gebruikers die een "bug" rapporteren worden regelmatig op de 
+      hoogte gehouden van de afhandeling van die bug.
+
+  3e. Programmeurs weten aan welke programma's gewerkt wordt.
+
+  4e. Er is een duidelijke prioriteitstelling voor de verschillende
+      onderhouds- en ontwikkelingstaken, waardoor niet onevenredig
+      veel tijd wordt besteed aan minder belangrijke klussen.
+
+  5e. Er zijn duidelijke overleg momenten, waardoor er doorlopend 
+      een optimale werkverdeling is.
+
+  6e. Er is een rapportage procedure, waardoor ervaring bij debugging 
+      voor het nageslacht bewaard blijft.
+
+Voor wat betreft Newstar zijn de meeste van die punten nu (informeel) 
+geregeld. Dit rapport probeert het geheel te structureren, uitgaande 
+van de afhandeling van bugs. Aangezien in mijn optiek missende
+functionaliteit ook een bug is (het jeukt net zo erg...) geldt het 
+verhaal in hoofdlijnen ook voor functionality requests.
+
+
+
+2. Procedure
+------------
+
+Afhandeling van een bug doorloopt de volgende fasen (tussen haakjes de
+status die na deze fase aan de fout wordt toegekend, zie sectie 5):
+
+ 1e. Ontvangst                                      (Received)
+ 2e. Prioriteitsstelling, toewijzing                (Assigned)
+ 3e. Bevestiging naar gebruiker                     (Confirmed)
+
+Tussen 1e. en 3e. mag hooguit twee dagen verstijken. De bevestiging kan 
+ook inhouden: dit heeft lage prioriteit, we houden u op de hoogte. Een 
+bevestiging kan ook plaatsvinden voor prioriteitsstelling.
+
+ 4e. Reproductie van de fout
+
+Als 4e. problemen geeft, wordt teruggekoppeld naar de gebruiker:
+architectuur/site specifieke problemen, kan gebruiker reproduceren?
+Wanneer dit onderdeel meer dan een dag in beslag neemt, moet de 
+prioriteitstelling opnieuw worden bekeken.
+
+ 5e. Analyse van de fout                            (Analysed)
+
+Hier wordt de set van modules/bestanden waar de fout in kan zitten 
+afgebakend: tracen van de fout, controleren van asynchrone effecten etc.
+Wanneer dit onderdeel meer dan een dag in beslag neemt, moet de 
+prioriteitstelling opnieuw worden bekeken. Afhankelijk van de locatie
+van de fout kan de bug worden doorgeschoven naar een andere programmeur
+(bv omdat die de modules geschreven of recent gewijzigd heeft).
+
+  6e. Formuleren van een oplossing of omleiding
+
+Wanneer dit onderdeel meer dan een week in beslag neemt, moet de
+prioriteitstelling opnieuw bekeken worden. Ook moet de gebruiker 
+een bericht krijgen dat de zaak wel eens wat langer kon duren.
+
+  7e. Implementeren van de oplossing of omleiding   (Solved)
+
+Als het implementeren van de geformuleerde oplossing langer dan een week
+duurt, moeten we terug naar 6e.
+
+  8e. Validatie van de oplossing of omleiding       (Tested)
+
+Eventueel worden de wijzigingen gecontroleerd door de oorspronkelijke
+auteur van de modules.
+De gebruiker wordt verzocht op zijn site een test te draaien met de
+gewijzigde modules (evt ftp van executable naar user systeem op die site).
+
+  9e. Afwikkeling van de fout                       (Released)
+
+De wijzigingen worden in de NFRA Master geupdate, inclusief wijzigingen
+van de documentatie.
+De gebruiker die de bug gemeld had, wordt op de hoogte gesteld,
+de master op zijn site wordt bijgewerkt. 
+Andere sites ontvangen een melding van de wijzigingen, en worden 
+eventueel bijgewerkt.
+
+
+3. Revisions en releases
+------------------------
+
+Bij wijzigingen in Newstar kunnen we twee gevallen onderscheiden:
+  - de wijziging heeft een minimale invloed op het gebruik van de 
+    programma's (afgezien van het ontbreken van crashes etc.); 
+    kleine toevoegingen in functionaliteit vallen hier ook onder
+  - de wijziging heeft invloed op het gebruik van de programma's
+    (veranderde keywords, noodzaak om SCN files te converteren etc)
+ 
+In het eerste geval spreken we van een revision van Newstar. Bij een 
+revision is het niet nodig dat elke gebruiker een melding van
+dit heuglijke feit ontvangt. Ook is het niet nodig dat alle sites
+een revision onmiddelijke ontvangen. Het exporteren van een revision
+gebeurt door een beperkt aantal bestanden over te zenden (via een
+revision groupfile: update retrieve .....grp)
+
+In het tweede geval spreken we van een release van Newstar.
+Een release wordt expliciet aangekondigd aan alle gebruikers (evt via
+locale Newstar managers). Een release wordt ge\"exporteerd naar alle
+sites. Voor een release wordt het volledige Master systeem van de site
+gecontroleerd: update retrieve all)
+
+
+4. Functionality requests
+-------------------------
+
+Voor functionality requests geldt in principe hetzelfde als voor bug,
+met dien verstande dat het reproduceren van de fout vervalt, en dat de
+overige stappen een langere tijdschaal hebben. 
+
+
+5. Implementatie: nbug
+----------------------
+
+In de NFRA Master staat een subdirectory $n_src/doc/bug waarin voor 
+elke bug een bestand wordt bijgehouden. Deze bestanden (project files)
+kunnen met de Hypertext browser worden bekeken via een aantal indexen. 
+Onderlinge verbindingen zijn mogelijk.
+
+Onafhankelijk van de manier waaop de bug binnenkomt (eMail, formulier AGB,
+telefonisch, wandelgangen) wordt een project file gemaakt. Als de bug 
+elektronisch gerapporteerd werd, kan het betreffende bestand aan de
+project file gekoppeld worden, anders moet de essentiele informatie 
+worden ingevoerd. 
+
+Wanneer nieuwe informatie beschikbaar komt (na toewijzing, bevestiging,
+oplossing etc) wordt die toegevoegd aan de project file, eventueel met 
+een gekoppeld tekstbestand.
+
+De bug-reports worden bijgehouden middels de utility "nbug", die een 
+hele reeks opties heeft. De meeste opties corresponderen met de diverse
+stadia die een bug in zijn carriere kan doorlopen.
+
+  add          Invoeren nieuwe bug (kent nummer toe, vraagt details)
+  confirm      Ontvangstbevestiging
+  priority     Prioriteitstelling (vraagt priority en assignment)
+  suspend      Wordt tijdelijk niet aan gewerkt (behoudt prioriteit)
+
+  analysed     Fout is gevonden
+  solved       Fout is opgelost
+  tested       Oplossing is getest
+
+  released     Nieuwe software is vrijgegeven (priority wordt -1)
+
+  feedback     Bevestiging van contact met melder
+  status       Vraagt status op van bepaalde bug (kan beter via hypertext)
+ 
+
+Bovenstaande opties vragen allemaal om een associated file en een
+comment, en geven de optie om de project file te editen (emacs of $EDITOR).
+Ze voeren ook automatisch een index commando uit. Indices kunnen op
+ieder moment gemaakt worden met de index optie:
+
+  index        Maakt de standard indexen voor de hypertext
+                 - Alle bugs op volgorde van nummer
+                 - Alle bugs op volgorde van prioriteit
+                 - Alle actieve bugs op volgorde van prioriteit
+
+Naast indices voor on-line toegang zijn (geprinte) lijsten vooralsnog
+van groot belang. De volgende lijsten kunnen met de ndoc optie "list"
+worden gemaakt:
+
+  list        Maakt lijsten voor printout
+    full        Alle bugs op volgorde van nummer
+    priority    Alle bugs op volgorde van prioriteit
+    active      Alle actieve bugs op volgorde van prioriteit
+    late        Alle "vertraagde" bugs, dat is: 
+                  - ontvangen en niet binnen twee dagen bevestigd 
+                  - niet suspended en geen feedback binnen twee weken 
+                  - suspended of released en geen feedback binnen twee dagen
+
+    user        Alle bugs van een bepaalde user (Pietje Puk etc)
+    programmer  Alle bugs van een bepaalde programmeur (HjV, WNB, ...)
+
+
+In de lijsten (en indices) verschijnt de bug als volgt:
+
+ID   Pr.ty Origin              Worker Status   Action/Feedback  Description
+------------------------------------------------------------------------------
+
+0024    10 verheijen           None   Confirmed  930806/930823  Gridding in ..
+0023   200 verheijen           CMV    Confirmed  930806/930823  NGIDS locks ..
+:
+0020     0 verheijen           None   Confirmed  930806/930823  NGIDS much t..
+0019   300 verheijen, WHISP    CMV    Confirmed  930806/930823  NGIDS flaggi..
+:
+
+De volgende bestanden zijn van belang voor nbug:
+ 
+   $n_src/doc/bug/n????.prj           Project file
+   $n_src/doc/bug/detail/n????.*      Alle overige documenten
+
+   $n_src/doc/bug/nbug.txt           "Home Page" met links naar indices
+   $n_src/doc/bug/nbug.idx            Index op nummer
+   $n_src/doc/bug/npriority.idx       Index op priority   
+   $n_src/doc/bug/nactive.idx         Index op priority voor actieve bugs
+   
+Al deze bestanden zijn normale ASCII file die naar believe kunnen worden
+bijgewerkt voor veranderingen die niet door nbug worden ondersteund.
+
+
+6. Prioriteitsstelling
+----------------------
+
+De voorlopige strategie voor de prioriteiten is als volgt:
+ 
+  - Prioriteiten lopen van 0 tot 900
+  - De honderdtallen doen dienst als grove prioriteitsklassen
+    Bugs uit 900-999 worden in principe het eerst aangepakt
+  - De tientallen doen dienst als een globaal werkschema binnen de
+    prioriteitsklassen. Bugs uit 990-999 worden in principe eerder
+    aangepakt dan bugs uit 980-989
+  - De eenheden zijn een kunstmatig middel om een bug omhoog te kunnen
+    schuiven zonder alle overige project files te moeten wijzigen.
+    Als een bug met prioriteit 700 zeer urgent wordt, urgenter dan 
+    bestaande bugs met prioriteit 980, dan wordt de prioriteit gewijzigd
+    naar 981.
+
+  - Een tijdslimiet of schatting kan als commentaar bij de prioriteit-
+    stelling worden gegeven.
+
+Een definitief systeem zal worden vastgesteld op basis van ervaringen met
+het huidige voorstel.
+
+
+6.1 Update on the priority system:
+---------------------------------
+
+There are now five priority classes:
+
+ 100      -   Critical bugs, that make it impossible to use vital programs
+ 200      -   Urgent requests or bugs
+ 300      -   Desirable things
+ 400/500  -   Pro memori
+
+The priority scheme does not show any timeslicing, but is complemented 
+in this respect by the Project Plan.
+
+The header tag Class has been added to distinguish between Bugs
+and Requests, the tag Category shows the program (e.g. NSCAN, NPLOT) 
+with which the Bug/Request is mainly concerned.
+
+
+7. Slotopmerkingen
+------------------
+
+Het moge duidelijk zijn dat een dergelijk systeem niet beperkt is tot 
+gebruik binnen Newstar. Met een aantal triviale wijzigingen in nbug
+is het mogelijk voor een willekeurig software project een dergelijke 
+rapportage op te zetten.
+
+Ook is deze strategie in principe bruikbaar voor alle processen waarbij 
+een "checklist" van status veranderingen moet worden bijgehouden. 
+Desgewenst kan de volgorde van veranderingen worden vastgelegd. 
+
+We kunnen nbug vergelijken met andere bug-reporting systemen (zoals bv het 
+GNATS systeem van GNU). Deze systemen hebben een grotere nadruk op 
+automatische interactie/responsies via electronische mail. De on-line 
+toegankelijkheid is kleiner dan bij nbug, evenals de centrale rapportage 
+mogelijkheden. Desgewenst kan meer eMail interactie worden ingebouwd in
+nbug. Dit lijkt me in de huidige situatie (waar verreweg de meeste 
+klachten verbaal worden ingediend) nauwelijks de moeite.
+
+
+ 
+  
+
+Appendix A: Casus
+-----------------
+
+> _nbug add_
+Creating bug-report project file with id-number 0036
+Enter name of file with associated eMail: _~devoscm/tmp_
+Enter origin [Pietje Puk]: __
+Enter email address [Unknown]: _puk@rux.timboektoe.edu_
+Enter subject [Unknown]: _Cannot make poststam images anymore_
+Any comments: _Seems the same old problem again_
+
+Please confirm the bug within two days and set a priority as soon 
+as possible. Indices for the bug-database will be updated.
+
+Edit the project file (y,n)? [n] _n_
+0036     0 Pietje Puk   None   Received   930909/000000
+     Cannot make poststamp images anymore
+Updating indices...
+
+After I called him back, I type...
+
+> _nbug confirm 36_
+0036     0 Pietje Puk   None   Received   930909/000000
+     Cannot make poststamp images anymore
+Any comments: _Called back, Mr. Puk seems quite upset about this_
+Associated file (may be -bugid or detail/...): __
+Edit the project file (y,n)? [n] __
+0036     0 Pietje Puk   None   Confirmed  930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+Then JEN decides this is quite important...
+
+> _nbug priority_
+Enter bug-id: _36_
+0036     0 Pietje Puk   None   Confirmed  930909/930909
+     Cannot make poststamp images anymore
+Enter (new) priority: _900_
+Assign job to: _HjV_
+Any comments: _Must be solved with a week_
+Associated file (may be -bugid or detail/...): __
+Edit the project file (y,n)? [n] __
+0036  1000 Pietje Puk   HjV    Assigned   930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+So it is analysed immediately...
+
+> _nbug analy 36_
+0036  1000 Pietje Puk   HjV    Assigned   930909/930909
+     Cannot make poststamp images anymore
+Any comments: _Missing check on array bounds in NPLSTM_
+Associated file (may be -bugid or detail/...): _test.log_
+
+Edit the project file (y,n)? [n] __
+0036  1000 Pietje Puk   HjV    Analysed   930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+And when Dr. Puk calls me occasionally...
+
+> _nbug feedback 36_
+0036  1000 Pietje Puk   HjV    Analysed   930909/930909
+     Cannot make poststamp images anymore
+Any comments: _Pietje called again, told him Henk found it_
+Associated file (may be -bugid or detail/...): __
+Edit the project file (y,n)? [n] __
+0036  1000 Pietje Puk   HjV    Analysed   930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+Etc.
+
+Appendix B: Format of project file and indices
+----------------------------------------------
+
+n0036.prj:
+------------------------------------------------------------
+ <TITLE>Newstar Bug Report # 0036</TITLE>
+
+ <H1>Newstar Bug Report # 0036 </H1>
+
+ <DT><STRONG>Origin:</STRONG>           Pietje Puk
+ <DT><STRONG>Address:</STRONG>          puk@rux.timboektoe.edu
+ <DT><STRONG>Subject:</STRONG>          Cannot make poststamp images anymore
+ <DT><STRONG>Status:</STRONG>           Analysed
+ <DT><STRONG>Priority:</STRONG>         1000
+ <DT><STRONG>Worker:</STRONG>           <A HREF=../html/people.html#HjV>HjV</A>
+ <DT><STRONG>Last action:</STRONG>      930909
+ <DT><STRONG>Last feedback:</STRONG>    930909
+
+ <P>
+ <H2>Detailed description</H2>
+
+ <P>
+ <H2>History</H2>
+
+ <DT>930909 18:05 - <STRONG>Received</STRONG> by Marco de Vos
+ <DD>Seems the same old problem again 
+ (<A HREF=detail/n0036.1>detail</A>)
+ <DT>930909 18:07 - <STRONG>Confirmed</STRONG> by Marco de Vos
+ <DD>Called back, Mr. Puk seems quite upset about this
+ <DT>930909 18:07 - <STRONG>Assigned (HjV, priority 1000)</STRONG> by Jan Noordam
+ <DD>Must be solved with a week
+ <DT>930909 18:08 - <STRONG>Analysed</STRONG> by Henk Vosmeijer
+ <DD>Missing check on array bounds in NPLSTM
+ (<A HREF=detail/n0036.2>detail</A>)
+ <DT>930909 18:09 - <STRONG>Feedback</STRONG> by Marco de Vos
+ <DD>Pietje called again, told him Henk found it
+------------------------------------------------------------
+
+
+nbug.idx:
+------------------------------------------------------------
+ <TITLE>Newstar Bug Index: all keys</TITLE>
+ <H1>Index of all bugs sorted on ID number</H1>
+
+ <P>
+ <LI> For an index sorted on priority, click <A HREF=npriority.idx>here</A>
+ <LI> For an index of active items only, click <A HREF=nactive.idx>here</A>
+ <P>
+
+ <TT><DT>BugID Pr.ty - Subject
+ <DD><STRONG>Status...</STRONG> - Action/Feedback 
+ (<EM>Origin</EM> - Worked on)</TT><P>
+
+ <TT><DT><A HREF=n0001.prj>0001</A>: +0000 </TT> - Lines in NPLOT to ...
+ <TT><DT><A HREF=n0002.prj>0002</A>: +0000 </TT> - Programs stay sile...
+
+------------------------------------------------------------
+
diff --git a/calculate.txt b/calculate.txt
new file mode 100644
index 0000000000000000000000000000000000000000..7c81e21d5d092d92591a10bd58d5acf5cc4017ab
--- /dev/null
+++ b/calculate.txt
@@ -0,0 +1,263 @@
+!CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC
+!
+!
+!	  ***********************************************************
+!	  *                                                         *
+!	  *        NETHERLANDS FOUNDATION FOR RADIO ASTRONOMY       *
+!	  *        P.O. BOX 2                                       *
+!	  *        7990 AA  DWINGELOO                               *
+!	  *        THE NETHERLANDS                                  *
+!	  *                                                         *
+!	  ***********************************************************
+!
+!
+! MODULE-NAME:		CALCULATE
+! ------------
+!
+! FILE-NAME:		CALCULATE.HLP
+! ----------
+!
+! BRIEF DESCRIPTION:
+! ------------------
+!	This file defines the help-text for the program CALCULATE.
+!	CALCULATE is derived from DWARF (Dwingeloo Westerbork
+!	Astronomical Reduction Facility).
+!
+!
+! HISTORY:
+! --------
+!	8-oct-86	Ger van Diepen
+!
+!
+!CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC
+!
+!
+!
+!
+!
+1 CALCULATE
+ The program CALCULATE is a handy desk-calculator, allowing the use of
+ expressions (with units), symbols and formulae.
+ It is derived from the Dutch image processing system DWARF.
+ (Dwingeloo Westerbork Astronomical Reduction Facility).
+ Note that DWARF is designed in such a way, that applications can
+ run outside the DWARF-environment.
+
+ The program is started by the command CALC(ULATE).
+ Qualifiers can be used to control the program. If they are given
+ at the CALC command-line, they serve as a global qualifier.
+ Global qualifiers can be overridden for each individual expression-line
+ by ending the line with the qualifiers, preceeded by at least one space
+ (to distinguish it from the division operator).
+
+ The input expressions are read from SYS$INPUT.
+ The results are listed on SYS$OUTPUT.
+ Optionally (part of) input and output can be logged.
+2 EXPRESSIONS
+ After having started the program, the program asks you for an expression.
+ By giving a null-answer the program will be stopped.
+ Typing a question mark starts a help session.
+ Typing UNIT=? will show you the available units on printer or terminal.
+
+ Expressions have the normal arithmetical format, using +,-,*,/,**
+ and parentheses. Blanks and unary signs are allowed.
+ However, note that / cannot be preceeded by a blank to distinguish
+ it from the qualifier-indicator.
+ The relational operators .NOT.,.EQ.,.NE.,.GT.,.GE.,.LE. and .LT.
+ are also allowed.
+ Also available are:
+   - some built-in functions (goniometric, etc.)
+   - unit specification and conversion
+   - special format for time or positions (using colons)
+   - symbol definition and substitution
+
+ As in DCL, integer numbers can be specified in octal or hexadecimal
+ format (use %O, %X, resp.).
+3 FUNCTIONS
+ The following functions (similar to Fortran) can be used in expressions:
+   MIN   MAX                   1-10 arguments
+   SIN   COS   TAN
+   ASIN  ACOS  ATAN  ATAN2
+   ABS
+   EXP   LOG   LOG10
+   SQRT
+   TRUNC ROUND
+   MOD
+   SIGN
+
+ Default unit for goniometric function is degrees, which can be
+ overridden via the /UNIT-qualifier or by giving the unit in the
+ expression.
+
+ The result of SIGN is:
+   -1  for negative values
+    0  for zero
+    1  for positive values
+
+ Note that conversion to integer format implies rounding.
+3 UNITS
+ CALCULATE is able of converting from one unit to another.
+ It converts the units given in the expression to the unit given by
+ the /UNIT-qualifier. The units must belong to the same group (so
+ conversion from SEC to KM is impossible).
+
+ A unit can be given at several places:
+   - after a number           e.g. 10DEG
+   - after a subexpression    e.g. (10+3)deg
+   - after a symbol           e.g. PI RAD
+
+ Note that in the last case the blank is significant, else it is
+ optional.
+3 TIME_POSITION
+ Times and positions can be given in HH:MM:SS (or DD:MM:SS) format
+ using colons as separators. A unit may follow the value.
+ Each part can be a floating number, which may exceed 60.
+
+ The output can also be listed in that format by giving
+ /UNIT=HMS or /UNIT=DMS.
+
+ This sexagesimal format allows for easy addition, subtraction and
+ conversion of times and positions.
+3 SYMBOLS
+ Symbols are very useful for storing results and for handling formulae.
+ Both symbol substitution and definition is possible in CALCULATE.
+ CALCULATE will always define global symbols.
+ It is also possible to use predefined local or global symbols,
+ either numeric or alphanumeric.
+
+ By defining a formula as a symbol, it is very easy to calculate
+ the result of the formula for several values of its parameters.
+ E.g.     $ VOLUME = "4/3*pi*r**3"
+          $ CALC
+          Expression: r=3
+          Expression: volume
+          Expression: r=10
+          Expression: volume
+4 DEFINITION
+ A symbol can be defined by using the construct:
+   symbol_name = expression
+ or
+   symbol_name = "expression"
+
+ In the first case the expression is evaluated and the result
+ will be assigned to the symbol.
+ In the second case the expression-text is assigned to the symbol,
+ which is useful for defining formulae.
+
+ Note that DCL uses the same procedure.
+4 SUBSTITUTION
+ Symbols can be substituted in an expression by
+   giving its name enclosed in apostrophes
+ or
+   giving its name without apostrophes.
+
+ In the first case its value is substituted literally.
+ In the second case its value is treated as a subexpression.
+
+ E.g.   if I=3+4  then     3*'i'   results in 3*3+4   = 13
+                   and     3*i     results in 3*(3+4) = 21
+
+ Note that nested substitution is possible.
+ Mutual substitution is detected by allowing a maximum of 25
+ substitutions.
+2 Examples
+ Convert miles to kilometers
+        $ calc
+         10mile /unit=km
+
+ If a whole serie must be done it would be better to do:
+        $ calc/unit=km
+         10mile
+         8 mile
+         (1.25+3.48)mile
+
+ Convert rigth ascension from HH:MM:SS to degrees.
+        $ calc/unit=deg
+         9:23:48.329 hms
+
+ Convert a time to seconds
+        $ calc/unit=sec
+         9:23:48.329 hr
+
+ Do some time calculation
+        $ calc/unit=hms
+         10:34:48 + 2::45 - :34:56.89
+
+ Calculate an expression and define the symbol ABC
+ The result must be an integer
+        $calc
+         ABC = (2.34 * pi)+8*-cos(135+pi*28) /unit=deg
+
+ Define a formula and calculate it for several parameters
+        $calc
+         VOLUME = "4/3*PI*R**3"
+         R=2
+         VOLUME
+         R=10
+         VOLUME
+
+ Convert from hexadecimal to decimal
+         %x1a2f
+
+ Convert from decimal to hexadecimal
+         2546 /rad=x
+2 /UNIT
+ This qualifier defines the default unit for the given values
+ and the unit in which the result will be expressed.
+ In this way it can be used for converting from one unit to another.
+ Note however that conversion between different groups of units
+ is not allowed (e.g. seconds to meters is illegal).
+
+ From DCL the available units can be shown via the command PRTUNIT.
+ From CALCULATE they can be shown via UNIT=?.
+
+ Default is no units.
+2 /RADIX
+ This qualifier defines in which radix the output will be listed.
+ Possible values are:
+    D   decimal
+    O   octal
+    X   hexadecimal
+
+ The default is D.
+ O and X force TYPE=J if type is non-integer.
+2 /TYPE
+ This qualifier defines in which format the output will be listed.
+ Note that all calculations are done in double precision and that
+ the program tests on integer overflow before conversion to an
+ integer format.
+ Possible values are:
+    B   signed byte
+    I   signed word       (integer*2)
+    J   signed longword   (integer*4)
+    L   logical
+    R   single precision  (real*4)
+    D   double precision  (real*8)
+
+ The default is D.
+2 /STREAM
+ This qualifier is special to DWARF.
+ It controls the stream of the application symbols.
+ The stream-name will be inserted in a symbol-name, if that symbol-name
+ has the format "image_keyword".
+
+ Default is no stream.
+2 /LIST
+ This qualifier controls if the results will be listed.
+ Normally you will always list the result, but in command-files
+ it can be useful to negate this qualifier (i.e. /NOLIST).
+ 
+ Default is list.
+2 /LOG
+ This qualifier controls if the expressions and results will be written
+ in the log-file CALCULATE.LOG (in the default directory).
+ This log-file is written in such a way that it can be executed as a
+ DCL command-file or can be used as input for the ARCHIVE-programs.
+ This means that most lines will be flagged with an exclamation mark
+ (indicating comments), but symbol definitions are valid commands,
+ which can be executed.
+ In this way users can calculate complex expressions and define the
+ results as symbols in a subprocess and execute the log-file in the
+ main process in order to obtain the results.
+
+ Default is no logging.
diff --git a/calibr_models.txt b/calibr_models.txt
new file mode 100644
index 0000000000000000000000000000000000000000..8084547dd901c38e875e126f9aa5d213e50be0db
--- /dev/null
+++ b/calibr_models.txt
@@ -0,0 +1,62 @@
+Beste mensen,
+
+Op /user4/92calib staan 5 modellen voor 325 MHz
+van 5 in Westerbork gebruikte calibrators (3C48, 147,
+286, 295 en 345)
+
+Ze bevatten ruim honderd componenten, voldoende voor een
+nauwkeurige zelfcalibratie.
+
+Bedenk echter het volgende:
+
+1) Ze gelden voor 325 MHz en als je ze in NCALIB
+wilt gebruiken op andere banden van het
+breedband 92cm systeem moet de BEAM optie aangezet
+worden. Dat corrigeert dan in eerste orde (met behulp
+van  een (cos**6(cfr) functie) voor de veranderende primaire
+bundel (met c=0.0629 dat nu geldt voor alle
+frequenties beneden 500 MHz). Echter op de laagste frequenties
+is de bundel waarschijnlijk breder dan een simpele
+frequentie schaling. Daar moet dan dus een nieuwe 
+coefficient voor worden bepaald alsmede een nieuw frequentie
+interval waarvoor die constante geldt voor worden gecreeerd.
+
+2) De calibratie bronnen zijn in werkelijkheid natuurlijk minder sterk
+op de hogere frequenties. Maar om redenen uitgelegd in een
+README help file in dezelfde directory wordt daar NIET voor
+gecorrigeerd !! Daar moeten de astronomen zelf voor corrigeren
+met behulp van de spectrale indices van die bronnen.
+
+
+3) De bron 3C345 mag niet als flux calibrator gebruikt worden omdat
+hij in fluxdichtheid varieert. Deze bron wordt slechts zo af en toe
+gemeten om dat hij gepolariseerd is waardoor met behulp van het Stokes
+U signaal het phase verschil van de XX en YY kanalen gecontroleerd
+kan worden onder de aanname dat V=0 (VZERO optie in NCALIB-polar)
+Deze bron heeft ook een RM van ongeveer 15-20 rad/m**2 waardoor de
+Stokes Q en U percentages afhangen van frequentie.
+Deze percentages staan dus ook niet in het model.
+Ze zijn trouwens afhankelijk van de ionosferische Faraday draaiiing
+die niet nauwkeurig bekend is.
+
+4) Voor de bron 3C303 (die ook i.v.m. met zijn hoge lineaire
+polarisatie wordt waargeneomen, net als 3C345) 
+wacht ik nog steeds op een aantal metingen 
+waaruit ik een goede kaart kan maken waaruit een model te halen is.
+Verder geldt voor deze bron hetzelfde als voor 3C345 behalve dat hij
+niet verandert in flux dichtheid.
+
+Henk: Kun jij deze modellen neerzetten op de plaats waar NEWSTAR
+zijn default modellen weghaalt.
+
+Als er vragen zijn dan hoor ik het wel.
+
+Ger
+-- 
+
+A.G. de Bruyn  (Ger)           | Internet:   ger@astron.nl
+NFRA                           | 
+Postbus 2                      | Phone: (31)-521-595257
+7990 AA Dwingeloo              | Fax:   (31)-521-597332 
+The Netherlands
+
diff --git a/cmv.gif b/cmv.gif
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new file mode 100644
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--- /dev/null
+++ b/common_descr/_7152_tex2html_wrap404.xbm
@@ -0,0 +1,5 @@
+#define noname_width 24
+#define noname_height 9
+static char noname_bits[] = {
+ 0x80,0x01,0x00,0xe0,0x00,0x00,0x38,0x80,0x7f,0x0e,0x80,0xcd,0x03,0x00,0xff,
+ 0x0f,0x80,0x0d,0x3c,0xc0,0x8c,0xf0,0x80,0x7f,0xc0,0x01,0x00};
diff --git a/common_descr/_7152_tex2html_wrap410.png b/common_descr/_7152_tex2html_wrap410.png
new file mode 100644
index 0000000000000000000000000000000000000000..f3042598a669b7af73d1a9025f49bc82b285318a
Binary files /dev/null and b/common_descr/_7152_tex2html_wrap410.png differ
diff --git a/common_descr/_7152_tex2html_wrap410.xbm b/common_descr/_7152_tex2html_wrap410.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ad5f4e3534e2bd6a43dc6ce557ddd03a3efbc04f
--- /dev/null
+++ b/common_descr/_7152_tex2html_wrap410.xbm
@@ -0,0 +1,5 @@
+#define noname_width 9
+#define noname_height 10
+static char noname_bits[] = {
+ 0x10,0x00,0x38,0x00,0x38,0x00,0x28,0x00,0x6c,0x00,0x44,0x00,0xc6,0x00,0x82,
+ 0x00,0x83,0x01,0x03,0x01};
diff --git a/common_descr/_7152_tex2html_wrap420.png b/common_descr/_7152_tex2html_wrap420.png
new file mode 100644
index 0000000000000000000000000000000000000000..2b5cb676792d18daf8d9863d4ed0eb99f5ab1183
Binary files /dev/null and b/common_descr/_7152_tex2html_wrap420.png differ
diff --git a/common_descr/_7152_tex2html_wrap420.xbm b/common_descr/_7152_tex2html_wrap420.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..201ffa9763aa9e7f4ab4aefe523c152224ea16eb
--- /dev/null
+++ b/common_descr/_7152_tex2html_wrap420.xbm
@@ -0,0 +1,4 @@
+#define noname_width 5
+#define noname_height 7
+static char noname_bits[] = {
+ 0x04,0x04,0x1f,0x0e,0x1f,0x15,0x04};
diff --git a/common_descr/common_descr.html b/common_descr/common_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..3a22dca9ac3b322af6eb3c599512de4ef58c7b57
--- /dev/null
+++ b/common_descr/common_descr.html
@@ -0,0 +1,300 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Common features of <i>NEWSTAR </i> programs</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=common_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=common_descr.html#SECTION0002000000000000000> <b>Running <i>NEWSTAR </i> programs under DWARF</b></A>
+<UL> 
+<LI> <A NAME=tex2html3 HREF=common_descr.html#SECTION0002100000000000000> <b>DWARF environment set-up</b></A>
+<LI> <A NAME=tex2html4 HREF=common_descr.html#SECTION0002200000000000000> <b>Running programs</b></A>
+<LI> <A NAME=tex2html5 HREF=common_descr.html#SECTION0002300000000000000> <b>Streams</b></A>
+<LI> <A NAME=tex2html6 HREF=common_descr.html#SECTION0002400000000000000> <b>Specifying program parameters (keywords)</b></A>
+<LI> <A NAME=tex2html7 HREF=common_descr.html#SECTION0002500000000000000> <b>Asking all</b></A>
+<LI> <A NAME=tex2html8 HREF=common_descr.html#SECTION0002600000000000000> <b>Maintenance of keyword values</b></A>
+</UL> 
+<LI> <A NAME=tex2html9 HREF=common_descr.html#SECTION0003000000000000000> <b>Some common <i>NEWSTAR </i> keywords</b></A>
+<UL> 
+<LI> <A NAME=tex2html10 HREF=common_descr.html#SECTION0003100000000000000> <b>NGEN: General keywords</b></A>
+<LI> <A NAME=tex2html11 HREF=common_descr.html#SECTION0003200000000000000> <b>Some frequently used <i>NEWSTAR </i> keywords</b></A>
+</UL>
+</UL>
+<A NAME=common.descr.dwarf><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Running <i>NEWSTAR </i> programs under DWARF</b></A></H1>
+<P>
+All <i>NEWSTAR </i> programs run under  the Dwingeloo Westerbork Astronomical Reduction Facility (DWARF).  This means that the programs communicate with the user via the DWARF interface, especially the DWARF parameter interface. DWARF also provides the user with various commands to modify the environment in which programs will be executed. This chapter tells you enough of DWARF to be able to run your first 
+<i>NEWSTAR </i> programs.
+<P>
+A full explanation of all the DWARF possibilities can be found in the  ``DWARF User's Guide'', written by Friso Olnon.
+<P>
+<H2><A NAME=SECTION0002100000000000000> <b>DWARF environment set-up</b></A></H2>
+<P>
+Before running the programs some symbols and logicals (aliases) should be known. Ask the System manager about the proper login commands. 
+The current values of the DWARF environment variables can be viewed: 
+ <BR> > <i>dwv dwarf</i> 
+		<i>dwview (see below)</i>
+<P>
+		<BR><tt>DWARF$0_STREAM(program) = 1</tt>
+<P>
+		<BR><tt>DWARF$0_CURNODE(program) = 0</tt>
+<P>
+		<BR><tt>DWARF$0_ASK(program) = NO</tt>
+<P>
+		<BR><tt>DWARF$0_SAVELAST(program) = NO</tt>
+<P>
+		<BR><tt>DWARF$0_USERLEVEL(program) = BEGINNER</tt>
+<P>
+		<BR><tt>DWARF$0_BELL(program) = ON</tt>
+<P>
+		<BR><tt>DWARF$0_MESSAGEDEVICE(program) = TERMINAL</tt>
+<P>
+		<BR><tt>DWARF$0_EXTENDSIZE(program) = 64</tt>
+<P>
+		<BR><tt>DWARF$0_IOBUFSIZE(program) = 32768</tt>
+<P>
+		<BR><tt>DWARF$0_TEST(program) = NO</tt>
+<P>
+		<BR><tt>DWARF$0_LOGLEVEL(program) = 4</tt>
+<P>
+		<BR><tt>DWARF$0_LOGFATAL(program) = NO</tt>
+<P>
+		<BR><tt>DWARF$0_IDENT(local) = 143</tt>
+<P>
+		<BR><tt>DWARF$0_IBMODE(local) = INTERACTIVE</tt>
+<P>
+The DWARF environment variables can also be changed by typing: 
+ <BR> > <i>dws dwarf</i>
+		<i>dwspecify (see below)</i>
+<P>
+<A NAME=common.descr.dwarf-run><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002200000000000000> <b>Running programs</b></A></H2>
+<P>
+Programs are normally run by typing:
+<P>
+ <BR> > <i>exe <IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap404.png">programname></i>
+		<i>(e.g. exe[cute] NSCAN)</i>
+<P>
+Note: <tt>exe</tt> stands for execute, and can, and this is preferred,  also be given as <tt>dwe</tt> or <tt>dwexe</tt>.
+<P>
+The program starts running, and asks questions (parameters, or `keywords')  that will specify the action of the program. All questions have some prompt information, and more help on the specific question can be obtained by typing a `?' as answer.
+<P>
+The type of answer (value, name, option, yes/no, ...) depends on the question. Some answer should be a single value, some should be a list separated by commas. In the case of a numeric list, the answer can also be of the form: start-value [by increment] [to end-value] There are three special answers that can always be given:
+<P>
+<UL><LI>   #or <IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap410.png">D (<IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap410.png">Z) means end-of-file.  
+                        The general action is to restart the 
+                          asking of questions at a <em>higher logical level</em>  
+                          in the 
+                          program. In the case of options it indicates in 
+                          general the QUIT option. 
+<LI>   &quot;&quot; means empty answer. In general this is taken to mean that no 
+                          answer is given. Depending on the keyword this can 
+                          mean to by-pass a certain action, or to go back to 
+                          another level of questions. If the answer is 
+                          essential, it will be repeated. 
+<LI>   * means `all'. If interpretable it is taken as meaning &quot;all 
+                          possible values&quot;, otherwise the question is repeated, 
+                          or a special default value is taken. 
+</UL>
+<P>
+In general (but with the exception of obvious interactive programs) all questions for the program are asked and checked for consistency, availability of files etc, before the program starts actually executing.
+<P>
+After the program is finished, a log of the program, including the questions and their answers and all data produced by the program, may be spooled to the lineprinter (controlled by the common <i>NEWSTAR </i> keyword <b>LOG</b>, see below). On this log you will see the answers to some questions that were never asked. The default answers to these hidden questions need normally sufficient,  and are, therefore, not asked. Ways to change them are given in below.
+<P>
+<A NAME=common.descr.DWARF-stream><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002300000000000000> <b>Streams</b></A></H2>
+<P>
+It is sometimes useful to run the same program in parallel, or to run a program regularly with a specified set of answers. To be able to differentiate between the programs, programs can be run in different streams. For all practical purposes the program (and its parameters) have different names. Streamnames can be any alpha-numeric string, although for practical reasons integers may be preferred by the user:
+<P>
+		<BR><tt>`program-name'$`stream'</tt>
+		<i>(e.g. dwe nscan$5)</i>
+<P>
+The zero stream has a special meaning in specifying values across streams.
+<P>
+<H2><A NAME=SECTION0002400000000000000> <b>Specifying program parameters (keywords)</b></A></H2>
+<P>
+In addition to answering questions asked, keyword values can be also be specified beforehand.  This is especially handy if you want to run programs in Batch mode, or you want to make sure that for a set of programs the  keyword values will be the same. 
+Keyword values can be specified before a program is run, by using the  <tt>dws(pecify)</tt> command. To answer all questions, type: 
+ <BR> > <i>dws `program-name'</i>
+		<i>(e.g. dws NSCAN)</i>  
+All keywords (and their current values) will now be displayed one after the other, and may be modified by the user. The process can be stopped at any time by giving <IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap410.png">D (<IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap410.png">Z) as answer. If you only want to specify a few keyword values only (and know the name of the keyword), type:  
+ <BR> > <i>dws `program-name'/nomenu</i>
+		<i>(e.g. dws nscan/nom)</i>
+<P>
+		<BR><tt>: keyword=`value'</tt>
+		<i>(e.g. ha-range=-10,10)</i>
+<P>
+		<BR><tt>:</tt>
+<P>
+The prog-name can be replaced  by <tt>`prog-name'$`stream'</tt> to specify keyword values for a separate stream (the default stream is in general $1). NB: The program name and/or stream can contain the wildcard <IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap420.png">.
+<P>
+Some questions are asked more than once in the program, for instance in an interactive loop.  To specify all answers beforehand, seperate them in <tt>dws</tt> with a  semi-colon (;). However, to make really sure that all answers are given, it is much safer to use the `Dry-run' or the `Saved-run' method (see below).
+<P>
+Keywords in DWARF have several levels of default values. The decision  process is as follows:
+<P>
+- is there a value for this keyword in the currect stream? If yes: use it. 
+<BR>- is there a value for this keyword in stream 0? If yes: use it. 
+<BR>- is there a value for this keyword in NGEN in this stream? If yes: use it. 
+<BR>- is there a value for this keyword in NGEN for stream 0? If yes: use it. 
+<BR>- should the program ask the keyword? If no: use program default. 
+<BR>- prompt the user for a value and use it.
+<P>
+Note: NGEN is a collection of special <i>NEWSTAR </i> keywords, described below.
+<P>
+<A NAME=common.descr.dwarf-ask><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002500000000000000> <b>Asking all</b></A></H2>
+<P>
+All questions (including the hidden ones) will be asked if you run the program as:
+<P>
+ <BR> > <i>dwe `name' /ask</i>
+		<i>(e.g. dwe nscan/ask)</i>
+<P>
+Asking can also be enabled for all runs of all programs by setting the global DWARF parameter ASK:
+<P>
+ <BR> > <i>dws dwarf/nomenu</i>
+<P>
+		<BR><tt>: ask=yes</tt>
+<P>
+		<BR><tt>:</tt>
+<P>
+<H2><A NAME=SECTION0002600000000000000> <b>Maintenance of keyword values</b></A></H2>
+<P>
+From the above it is clear that the variety of possibilities to specify keyword values also makes the possibility of errors quite large. It is therefore recommended to make sure that programs are run as intended. To aid in maintaining the specified answers, run the following regularly: 
+ <BR> > <i>dwv(iew) 'prog-name'[$`stream']/extern</i> 
+shows all current values for the specified program and stream. 
+ <BR> > <i>dwc(lear) `prog-name'[$`stream']</i> 
+clears all current values for the specified program and stream.
+<P>
+<A NAME=common.descr.newstar><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Some common <i>NEWSTAR </i> keywords</b></A></H1>
+<P>
+<A NAME=common.descr.newstar.ngen><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000> <b>NGEN: General keywords</b></A></H2>
+<P>
+The following keywords (parameters) are used for most <i>NEWSTAR </i> programs, but they are usually hidden from the user (default switch /NOASK). Their current values  can be inspected by:
+<P>
+ <BR> > <i>dwv ngen</i>
+<P>
+		<BR><tt>NGEN$1_LOG(program) = SPOOL /NOASK</tt>
+<P>
+		<BR><tt>NGEN$1_RUN(program) = YES /NOASK</tt>
+<P>
+		<BR><tt>NGEN$1_DATAB(program) = "" /NOASK</tt>
+<P>
+		<BR><tt>NGEN$1_INFIX(program) = "" /NOASK</tt>
+<P>
+		<BR><tt>NGEN$1_APPLY(program) = * /NOASK</tt>
+<P>
+		<BR><tt>NGEN$1_DE_APPLY(program) = NONE /NOASK</tt>
+<P>
+		<BR><tt>NGEN$1_LOOPS(program) = "" /ASK</tt>
+<P>
+		<BR><tt>NGEN$1_DELETE_NODE(program) = NO /ASK</tt>
+<P>
+More information about these keywords can be found in the Summary of Common keywords in the next section.
+<P>
+Usually, their default values are taken for the NGEN keywords,  but they may also be specified by the user in a number of ways, for instance with <tt>dwspecify</tt>:
+<P>
+ <BR> > <i>dws `prog-name'[$`stream']/nomenu</i>
+<P>
+		<i>will set the keyword for specified program and stream.</i>
+<P>
+ <BR> > <i>dws `prog-name'$0/nomenu</i>
+<P>
+		<i>will set the keyword for specified program and all streams.</i>
+<P>
+ <BR> > <i>dws ngen[$`stream']/nomenu</i>
+<P>
+		<i>will set the keyword for all programs in the stream.</i>
+<P>
+ <BR> > <i>dws ngen$0/nomenu</i>
+<P>
+		<i>will set the keyword for all programs and streams.</i>
+<P>
+It is also possible to give (any) keyword values as switches when running the program:
+<P>
+ <BR> > <i>dwe `prog-name'[$`stream']/keyw[=`value']</i>
+		<i>or</i>  
+ <BR> > <i>dwe `prog-name'[$`stream']/nokeyw</i>
+<P>
+will set the keyword for the specified program and stream
+<P>
+Some examples in the case of NGEN keywords:
+<P>
+<UL><LI> <tt>/LOG= spool/yes/no/append</tt><BR>specify if program log should be 
+        spooled (the name will be the first 
+        three letters of the program name 
+        (capital), followed by date, time, 
+        letter (capital), .LOG), made but not 
+        spooled (name will be PROG-NAME.LOG), 
+        not made, appended to PROG-NAME.LOG. 
+<LI> <tt>/LOG X /LOG=spool</tt> 
+<LI> <tt>/NOLOG X /LOG=no</tt> 
+<LI> <tt>/RUN</tt><BR>run the program 
+<LI> <tt>/NORUN</tt><BR>start the program, ask all questions, 
+        save all the keyword values (as if specified). 
+        This can be used to prepare a batch run for intance. 
+<LI> <tt>/INFIX= 'node shorthand'</tt><BR>specify a part of the node name that is always the same (see later) 
+<LI> <tt>/INFIX X /INFIX=&quot;&quot;</tt> 
+<LI> <tt>/NOINFIX X /INFIX=&quot;&quot;</tt> 
+<LI> <tt>/APPLY=list-of-options</tt><BR>specify the corrections to be applied to data (see later for full 
+        explanation). The list can contain one or more of: 
+        ALL, NONE, RED, ALG, OTH, EXT, POL, 
+        FAR, MOD, IFR, MIFR , NORED, ... NOMIFR 
+<LI> <tt>/APPLY X /APPLY=*</tt><BR><LI> <tt>/NOAPPLY X /APPLY=NONE</tt><BR><LI> <tt>/DE_APPLY='list-of-options'</tt><BR><LI> <tt>/DE_APPLYX /DE_APPLY=NONE</tt><BR><LI> <tt>/NODE_APPLYX /DE_APPLY=*</tt><BR>(i.e. NO DE_APPLY) 
+</UL>
+<P>
+<A NAME=common.descr.NEWSTAR-other><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000> <b>Some frequently used <i>NEWSTAR </i> keywords</b></A></H2>
+<P>
+Some other keywords are also used by many <i>NEWSTAR </i> programs, but not hidden to the user. They are usually concerned with the  selection of data: <b>SETS, POLARISATION, SELECT_IFRS, HA_RANGE, AREA</b>. There are also some others. They have been collected into this `common' section to emphasize their communality, and also to make it possible to treat some of them in some more detail. More information about these keywords can be found in the Summary of Common keywords in the next section.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/common_descr/images.pl b/common_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..67e74b7ff0071f6aed8b4e0b2436a326e8ddb783
--- /dev/null
+++ b/common_descr/images.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$<${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap404.xbm">'; 
+$key = q/{}$wedge${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap410.xbm">'; 
+$key = q/{}$ast${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7152_tex2html_wrap420.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/common_descr/labels.pl b/common_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..ae3768f1f6c6f91e9e864c716c5243dafa1d4394
--- /dev/null
+++ b/common_descr/labels.pl
@@ -0,0 +1,13 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"common.descr.newstar.ngen"} ="$URL/common_descr.html"; 
+$external_labels{"common.descr.newstar"} ="$URL/common_descr.html"; 
+$external_labels{"common.descr.dwarf"} ="$URL/common_descr.html"; 
+$external_labels{"common.descr.DWARF-stream"} ="$URL/common_descr.html"; 
+$external_labels{"common.descr.dwarf-ask"} ="$URL/common_descr.html"; 
+$external_labels{"common.descr.dwarf-run"} ="$URL/common_descr.html"; 
+$external_labels{"common.descr.NEWSTAR-other"} ="$URL/common_descr.html"; 
+$external_labels{".contents"} ="$URL/common_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/control_c.txt b/control_c.txt
new file mode 100644
index 0000000000000000000000000000000000000000..8f09648f448cff2d8b7f88fdf36c6a44826e8168
--- /dev/null
+++ b/control_c.txt
@@ -0,0 +1,38 @@
+Trapping control-C in Newstar programs -------------------------------------- 
+
+        (contributed by JPH 941005, gleaned from wndpar_x.fun, wngex.for) 
+
+
+
+
+        INCLUDE WXH_DEF ... 
+        XHCC(0)=1                       ! inhibit ... 
+        XHCC(0)=0                       ! clear 
+        IF (XHCC(1) .NE.0) THEN         ! was a control-C caught? 
+          XHCC(1)=0 
+          <action, typically CALL WNGEX> 
+        ENDIF 
+
+        This code has been used to create module WNGCC with entry points 
+
+                WNGCCD          disable control-C 
+                WNGCCE          enable control-C 
+                LOGICAL WNGCCC  check and reset 'control-c seen' status
+
+and several other entry points to check, count and reset the number of
+interrupts seen. 
+
+
+        The implementation is in entry point WNGEX0 in wngex.for. This routine
+is declared the handler for signal SIGINT by wngsxh.fsc. Its action is very
+simple: 
+
+        if xhcc(0) !=0 
+                xhcc(1)+=1 
+        else 
+                fall through to WNGEX 
+
+        endif 
+
+
+
diff --git a/copyright.txt b/copyright.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6d061df0b1319b0765c5ae880d738eaffea10792
--- /dev/null
+++ b/copyright.txt
@@ -0,0 +1,157 @@
+NEWSTAR - Copyright Notice
+--------------------------
+
+    COPYRIGHT (c) 1991, 1994
+      by the Netherlands Foundation for Research in Astronomy
+
+    NFRA/St. ASTRON
+    P.O. Box 2
+    7990 AA Dwingeloo 
+    The Netherlands 
+
+
+     The information in this document is subject to change without
+     notice and should not be construed as a commitment by the NFRA.
+
+     The NFRA assumes no responsibility  for the use or reliability 
+     of the Newstar package and software exported together with it.
+
+     Permission to use, copy, and distribute Newstar software and its
+     documentation for any purpose is hereby granted, provided that
+     this copyright notice appears in all copies.
+
+     Permission to modify the software is granted, but not the right
+     to distribute the modified code. Modifications are to be distributed
+     exclusively through the Newstar Master Installation at the NFRA.
+     Please send any modifications to the Newstar manager who may 
+     include them in the Master Installation for further distribution.
+
+     Requests for copies of the Master Installation, for assistance with
+     the installation and for support of an unmodified version of the
+     Master Installation can be directed to the Newstar manager, who
+     can be reached by electronic mail as  newstar@astron.nl  or through
+     the Newstar User Feedback System (refer to the documentation for
+     details). 
+
+
+     The Gipsy program gids and the giplib-library are distributed 
+     with Newstar. Gipsy is copyrighted by the Kapteyn Astronomical
+     Institute, University of Groningen. The original copyright notice 
+     for the Gipsy software is included at the end of this document.
+
+     A binary version of the Mosaic hypertext browser, developed at 
+     the NCSA (Illinois) is distributed with Newstar. The original
+     copyright notice for Mosaic is included at the end of this document.
+
+     Newstar includes a modified version of the X11-driver originally
+     developed for the PGPLOT package by Tim Pearson (Caltech). 
+
+
+
+COPYRIGHT Release 3.5
+
+                  Groningen Image Processing SYstem (GIPSY)
+
+                    COPYRIGHT (c) 1978, 1984, 1992, 1993, 1994
+
+                    Kapteyn Astronomical Institute,
+                    University of Groningen
+                    P.O. Box 800
+                    9700 AV Groningen
+                    The Netherlands
+
+
+     The information in this document is subject to change without
+     notice and should not be construed as a commitment by the Kapteyn
+     Astronomical Institute.
+
+     The Kapteyn Astronomical Institute assumes no responsibility  for
+     the use or reliability of its software.
+
+     Permission to use, copy, and distribute GIPSY software and its
+     documentation for any purpose is hereby granted, provided that
+     this copyright notice appears in all copies.
+
+     Permission to modify the software is granted, but not the right
+     to distribute the modified code. Modifications are to be distributed
+     via the GIPSY source server, which is currently kapteyn.astro.rug.nl.
+     You can send your modifications to the GIPSY manager, who will take
+     care of the distribution.
+
+     Permission to install modified or new code directly can be obtained
+     from the GIPSY Manager. The E-Mail address of the GIPSY Manager
+     is listed in $gip_sys/manager.mgr.
+
+     Reports of software failures will only be considered when you have
+     an automatic update of GIPSY sources installed at your site. See
+     $gip_sys/README.
+
+
+Everything not already copyrighted by CERN is copyrighted by NCSA
+(including the contents of the libhtmlw, libnet, libXmx, and src
+directories, but not including the contents of libdtm, which is
+entirely public domain).
+
+The official NCSA Mosaic copyright statement follows.
+
+/****************************************************************************
+ * NCSA Mosaic for the X Window System                                      *
+ * Software Development Group                                               *
+ * National Center for Supercomputing Applications                          *
+ * University of Illinois at Urbana-Champaign                               *
+ * 605 E. Springfield, Champaign IL 61820                                   *
+ * mosaic@ncsa.uiuc.edu                                                     *
+ *                                                                          *
+ * Copyright (C) 1993, Board of Trustees of the University of Illinois      *
+ *                                                                          *
+ * NCSA Mosaic software, both binary and source (hereafter, Software) is    *
+ * copyrighted by The Board of Trustees of the University of Illinois       *
+ * (UI), and ownership remains with the UI.                                 *
+ *                                                                          *
+ * The UI grants you (hereafter, Licensee) a license to use the Software    *
+ * for academic, research and internal business purposes only, without a    *
+ * fee.  Licensee may distribute the binary and source code (if released)   *
+ * to third parties provided that the copyright notice and this statement   *
+ * appears on all copies and that no charge is associated with such         *
+ * copies.                                                                  *
+ *                                                                          *
+ * Licensee may make derivative works.  However, if Licensee distributes    *
+ * any derivative work based on or derived from the Software, then          *
+ * Licensee will (1) notify NCSA regarding its distribution of the          *
+ * derivative work, and (2) clearly notify users that such derivative       *
+ * work is a modified version and not the original NCSA Mosaic              *
+ * distributed by the UI.                                                   *
+ *                                                                          *
+ * Any Licensee wishing to make commercial use of the Software should       *
+ * contact the UI, c/o NCSA, to negotiate an appropriate license for such   *
+ * commercial use.  Commercial use includes (1) integration of all or       *
+ * part of the source code into a product for sale or license by or on      *
+ * behalf of Licensee to third parties, or (2) distribution of the binary   *
+ * code or source code to third parties that need it to utilize a           *
+ * commercial product sold or licensed by or on behalf of Licensee.         *
+ *                                                                          *
+ * UI MAKES NO REPRESENTATIONS ABOUT THE SUITABILITY OF THIS SOFTWARE FOR   *
+ * ANY PURPOSE.  IT IS PROVIDED "AS IS" WITHOUT EXPRESS OR IMPLIED          *
+ * WARRANTY.  THE UI SHALL NOT BE LIABLE FOR ANY DAMAGES SUFFERED BY THE    *
+ * USERS OF THIS SOFTWARE.                                                  *
+ *                                                                          *
+ * By using or copying this Software, Licensee agrees to abide by the       *
+ * copyright law and all other applicable laws of the U.S. including, but   *
+ * not limited to, export control laws, and the terms of this license.      *
+ * UI shall have the right to terminate this license immediately by         *
+ * written notice upon Licensee's breach of, or non-compliance with, any    *
+ * of its terms.  Licensee may be held legally responsible for any          *
+ * copyright infringement that is caused or encouraged by Licensee's        *
+ * failure to abide by the terms of this license.                           *
+ *                                                                          *
+ * Comments and questions are welcome and can be sent to                    *
+ * mosaic-x@ncsa.uiuc.edu.                                                  *
+ ****************************************************************************/
+
+For more information on copyright and licensing issues, contact:
+
+Marc Andreessen 
+Software Development Group
+National Center for Supercomputing Applications
+605 E. Springfield, Champaign IL 61820
+marca@ncsa.uiuc.edu
diff --git a/debug_efficiently.txt b/debug_efficiently.txt
new file mode 100644
index 0000000000000000000000000000000000000000..9d6ad328325e8dbb362ede302dcae95ebf598ba2
--- /dev/null
+++ b/debug_efficiently.txt
@@ -0,0 +1,36 @@
+Efficient use of the dbx debugger on the SUNs
+---------------------------------------------
+
+(contributed by JPH 940919; based on research by CMV)
+
+
+	For the convenience of programmers who want to use dbx with Newstar
+programs, the objects in the Newstar libraries are routinely compiled with the
+-g option (Newstar nsh option 'build -d') which creates objects including the
+necessary symbolic information. When an executable is built with this same
+option, all this information is carried over, resulting in a .exe file in which
+all modules are accessible to dbx.
+
+	This is very convenient for a programmer who needs access not only to
+modules that he is modifying in his own shadow system but also to other
+unmodified modules in the master libraries; indeed, there is no need for him to
+copy master files to his shadow system for the mere purpose of recompiling them.
+	The disadvantage is that the .exe file carries a huge ballast of
+symbolic information (typically several hundred thousands of items) which take
+a long time (many minutes) to load at the expense of a more than unmodest
+consumption of machine resources.
+
+	CMV found the following simple procedure to load only those symbols
+that one actually needs:
+
+	> dbx
+	dbx> modules select <object_1>.o, <object_2>.o, ...
+	dbx> debug <$n_exe/<program>.exe
+	dbx> <set breakpoints or whatever>
+	dbx> run
+
+Should one discover in the subsequent debugging session that more modules are
+needed, then one may restart the above sequence without leaving dbx.
+Breakpoints and the like remain valid, but the modules selected before must
+again be spelled out, - this is not nice but usually one needs only a few ...
+
diff --git a/doc_guide.ps b/doc_guide.ps
new file mode 100644
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diff --git a/doc_guide/doc_guide.html b/doc_guide/doc_guide.html
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@@ -0,0 +1,696 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ &quot;,,&quot;  
+substitutes  
+''
+<P>
+<b>Guide for writing and maintaining <i>NEWSTAR </i> documents</b>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=doc_guide.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=doc_guide.html#SECTION0002000000000000000>  <b>Summary of <i>NEWSTAR </i> LaTeX commands </b></A>
+<LI> <A NAME=tex2html3 HREF=doc_guide.html#SECTION0003000000000000000>  <b>The <i>NEWSTAR </i> documentation system</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=doc_guide.html#SECTION0003100000000000000>  <b>General layout</b></A>
+</UL> 
+<LI> <A NAME=tex2html5 HREF=doc_guide.html#SECTION0004000000000000000>  <b>Cross-references</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=doc_guide.html#SECTION0004100000000000000>  <b>Cross-references to text in LaTeX documents </b></A>
+<LI> <A NAME=tex2html7 HREF=doc_guide.html#SECTION0004200000000000000>  <b>Cross-references to other types of documents</b></A>
+<LI> <A NAME=tex2html8 HREF=doc_guide.html#SECTION0004300000000000000>  <b>Equations and equation references</b></A>
+</UL> 
+<LI> <A NAME=tex2html9 HREF=doc_guide.html#SECTION0005000000000000000>  <b>Figures and figure references</b></A>
+<UL> 
+<LI> <A NAME=tex2html10 HREF=doc_guide.html#SECTION0005100000000000000>  <b>Caption files</b></A>
+<LI> <A NAME=tex2html11 HREF=doc_guide.html#SECTION0005200000000000000>  <b>Xfig figures</b></A>
+<LI> <A NAME=tex2html12 HREF=doc_guide.html#SECTION0005300000000000000>  <b>Postscript figures</b></A>
+<LI> <A NAME=tex2html13 HREF=doc_guide.html#SECTION0005400000000000000>  <b>Figure references</b></A>
+</UL> 
+<LI> <A NAME=tex2html14 HREF=doc_guide.html#SECTION0006000000000000000>  <b>Session transcripts</b></A>
+<UL> 
+<LI> <A NAME=tex2html15 HREF=doc_guide.html#SECTION0006100000000000000>  <b>Programmer's commands: Processing individual files </b></A>
+<LI> <A NAME=tex2html16 HREF=doc_guide.html#SECTION0006200000000000000>  <b><i>NEWSTAR </i> manager's commands: Maintaining the documentation system
+</b></A>
+</UL> 
+<LI> <A NAME=tex2html17 HREF=doc_guide.html#SECTION0007000000000000000>  <b>Debugging .tex files</b></A>
+<UL> 
+<LI> <A NAME=tex2html18 HREF=doc_guide.html#SECTION0007100000000000000>  <b>LaTeX bugs</b></A>
+<LI> <A NAME=tex2html19 HREF=doc_guide.html#SECTION0007200000000000000>  <b>Processing errors in ndoc</b></A>
+<LI> <A NAME=tex2html20 HREF=doc_guide.html#SECTION0007300000000000000> <b>Processing errors in ndoc Cook</b></A>
+</UL> 
+<LI> <A NAME=tex2html21 HREF=doc_guide.html#SECTION0008000000000000000> <b>latex2html </b></A>
+<UL> 
+<LI> <A NAME=tex2html22 HREF=doc_guide.html#SECTION0008100000000000000>  <b>Formulas and the like in latex2html </b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Summary of <i>NEWSTAR </i> LaTeX commands </b></A></H1>
+<P>
+        For quick reference use the following list of special LaTeX commands available in the <i>NEWSTAR </i> documentation system:  
+<BR><BR><A HREF="#.cross.ref.other">ascref</A> <BR><A HREF="#.cross.ref">Ascref</A> <BR><A HREF="#.caption">caption</A> <BR><A HREF="#.layout">chapter</A> <BR><A HREF="#.eqref">eqref</A> <BR><A HREF="#.eqref">Eqref</A> <BR><A HREF="#.caption">fig</A> <BR><A HREF="#.figref">figref</A> <BR><A HREF="#.figref">Figref</A> <BR><A HREF="#.cross.ref.latex">label</A> <BR><A HREF="#.ps">ps</A> <BR><A HREF="#.cross.ref.other">psref</A> <BR><A HREF="#.cross.ref">Psref</A> <BR><A HREF="#.cross.ref.latex">ref</A>: <em>Not to be used</em> <BR><A HREF="#.layout">tableofcontents</A> <BR><A HREF="#.cross.ref.latex">textref</A> <BR><A HREF="#.cross.ref">Textref</A> <BR><A HREF="#.cross.ref">whichref</A> <BR><H1><A NAME=SECTION0003000000000000000>  <b>The <i>NEWSTAR </i> documentation system</b></A></H1>
+<P>
+        The <i>NEWSTAR </i> documentation system provides documentation in two forms: An on-line hypertext system based on the public-domain program &quot;xmosaic&quot; and standard LATeX documents. Both forms are derived from a single set of LaTeX source files; for the hypertext form, the public-domain translator  latex2html  is used.  
+        Broadly speaking, authors are free to use the standard LaTeX constructs. In particular,  latex2html  handles tabular material, mathematical formulas and the inclusion of diagrams very well. Writers should be aware, however, that every bit of math-mode text is translated into a little bitmap that must be loaded separately for display. This considerably slows down both the processing by ndoc Cook and the display by xmosaic.  
+         Simple macros defined through  
+\newcommand can be used freely, but complicated nesting of macros should be avoided.  
+        To satisfy the specific needs of the <i>NEWSTAR </i> system and circumvent some deficiencies of  latex2html , the guidelines given below should be followed.
+<P>
+<A NAME=.layout><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0003100000000000000>  <b>General layout</b></A></H2>
+<P>
+ <UL><LI>   Preamble
+<P>
+        The document compiler  ndoc automatically inserts a preamble including the \begin{document} and also appends the \end{document}. The source of a document may add private preamble elements such as  
+\newcommand definitions. Apart from that, the first document line is the  
+\chapter line:
+<P>
+<LI> \chapter{&lt;text&gt;}
+<P>
+        The chapter is the basic documentation unit.  ndoc formats the argument  
+&lt;text&gt; as a hypertext or printed document title.
+<P>
+<LI> \tableofcontents
+<P>
+        This creates a standard table of the chapter's contents in the printed document and an equivalent unnumbered table with links to the (sub)(sub)sections in the hypertext display.
+<P>
+<LI>   ,,[sub]sub]]section{&lt;text&gt;}
+<P>
+        These commands produce standard section headings, numbered in the printed document, unnumbered in the hypertext display.  
+ </UL>
+<P>
+<A NAME=.cross.ref><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000>  <b>Cross-references</b></A></H1>
+<P>
+        In writing documents, the placeholder \whichref{text}{} can be used for references whose target is not yet known.
+<P>
+        For most referencing commands, a companion with the leading character capitalised is available; these work the same way except that the text argument is printed in boldface. This feature is intended for use in the documentation home-page document, hb_contents.tex.
+<P>
+<A NAME=.cross.ref.latex><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004100000000000000>  <b>Cross-references to text in LaTeX documents </b></A></H2>
+<P>
+        Cross-references must work in both the printed and hypertext versions of a document. For this reason, <i>the standard LaTeX \ref command is unsuitable</i> and the rules given below must be followed instead.
+<P>
+ <UL><LI>   \label{.&lt;label&gt;}
+<P>
+        A label name <em>must start in a dot</em> as shown. LaTeX <em>forbids the use of underscores in labels</em>, even if they are escaped by a backslash; it is recommended to use <em>dots</em> instead.
+<P>
+<LI>   \textref{&lt;text&gt;}{.&lt;label&gt;}
+<P>
+        This is translated for the printed document as &lt;text&gt; (sec. &lt;section number&gt;). In the hypertext display, &lt;text&gt; becomes a hypertext link to &lt;label&gt;. &lt;text&gt; may have a local format of its own, e.g.  
+{\em &lt;text&gt;} or {\bf &lt;text&gt;}.
+<P>
+<LI>   \textref{&lt;text&gt;}{&lt;file name&gt;.&lt;label&gt;}
+<P>
+        This is the form for a reference to a label in an external file. In the printed document it becomes &lt;text&gt; with a numbered footnote showing the directory and name of the target file's source and the target label.
+<P>
+        &lt;file name&gt; is the name of a .tex file (without the .tex extension!) in directory \$n\_doc/latex; the name may contain <em>neither dots nor uppercase characters</em>, but underscores are allowed (and need not to be quotes with a backslash).
+<P>
+<LI>   \whichref{&lt;text&gt;}{}
+<P>
+         can be used as a placeholder for a \textref whose target is as yet unknown.
+<P>
+ </UL>
+<P>
+<A NAME=.cross.ref.other><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004200000000000000>  <b>Cross-references to other types of documents</b></A></H2>
+<P>
+        The documentation system also contains ASCII documents and PostScript documents imported from elswehere. Such documents may be referred to through the following commands:
+<P>
+ <UL><LI>   \ascref{&lt;text&gt;}{&lt;file name&gt;}  
+<LI>   \psref{&lt;text&gt;}{&lt;file name&gt;}  
+ </UL>
+<P>
+        &lt;file name&gt; is the name (without extension!) of a .txt file in directory \$n\_doc/txt or of a .ps file in directory \$n\_hlp; the name may contain <em>neither dots nor uppercase characters</em>, but underscores are allowed (and need not to be quotes with a backslash).
+<P>
+ <UL><LI>   \srcref{&lt;text&gt;}{&lt;directory&gt;&lt;file name&gt;&lt;extension&gt;}  
+ </UL>
+<P>
+        This command is used to refer to program code or WNTINC table definitions (.dsc files). directory must be specified relative to  
+n_src and the file extension must be included.
+<P>
+<A NAME=.eqref><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004300000000000000>  <b>Equations and equation references</b></A></H2>
+<P>
+        The commands \Eqref{.&lt;label&gt;} and \eqref{.&lt;label&gt;} are entirely analogous to the <A HREF="#.figref">figure references</A>  
+\Figref and \figref.
+<P>
+<A NAME=.fig><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000>  <b>Figures and figure references</b></A></H1>
+<P>
+        Figures with their captions reside in the directory  
+\$n\_doc/fig. A figure consists of two components:  
+ <UL><LI>   a &lt;name&gt;.cap <em>caption file</em> containing a caption and a the directive to include the figure.
+<P>
+<LI>   the diagram proper in the form of either an xfig drawing  
+&lt;name&gt;.fig, or a binary (e.g. &lt;name&gt;.ps or &lt;name&gt;.gif) file.  
+ </UL>
+<P>
+        A figure with its caption is included in a document source file through the command
+<P>
+  \input{../fig/&lt;name&gt;.cap  
+<P>
+In the printed document, figure and caption are included in the standard way. In the hypertext display the word FIGURE is included, followed by the caption text, with a hypertext link from FIGURE to a postscript file.  ndoc generates that file automatically from the .fig file.
+<P>
+<A NAME=.caption><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005100000000000000>  <b>Caption files</b></A></H2>
+<P>
+        The purpose of the caption file (as opposed to spelling out the caption text in the document source) is to enable the figure with its caption to exist as an independent unit that can be included in more than one document and also exist outside the context of any document.
+<P>
+        The caption file must not only provide the caption, but also the title under which the figure may be listed in the Handbook Overview. It is therefore important to adhere strictly to the following format:
+<P>
+ <PRE> 
+        \begin{figure}[htbp] 
+          \fig{<name>} 
+          \caption[]{<optional LaTeX commands, e.g. \it> 
+        <title> 
+        <optional LaTeX commands, e.g. \> <optional remainder of caption> 
+        } 
+          \label{.<label>} 
+        \end{figure} 
+</PRE>
+<P>
+ Examples can be found in the 
+/\$n\_doc/fig directory.
+<P>
+        You are free to choose the label; the recommended choice, however, is
+the file name with underscores replaced by dots. (Remember that underscores are
+illegal in labels and that labels must start with a dot.)
+<P>
+        Comment lines (but no <em>empty</em> lines!) may be arbitrarily added,
+except that the &lt;title&gt; line must <em>immediately follow</em> the 
+\caption command.
+<P>
+<A NAME=.xfig><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000>  <b>Xfig figures</b></A></H2>
+<P>
+        .fig files may be created without any restrictions with the
+public-domain program xfig. It is not necessary to produce a postscript
+file with this program.  ndoc/ will take the .fig file and convert it
+automatically.
+<P>
+        Often, figures drawn on a convenient scale on a workstation screen will
+not fit on a standard A4 page.  ndoc/ may be instructed to automatically reduce
+its scale by including in the figure a text line
+<P>
+  &lt;file name&gt;.fig &lt;nn&gt; It is best to put this text in an inconspicuous corner and a small font (e.g.
+10pt as opposed to a standard 20pt).
+<P>
+<A NAME=.ps><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005300000000000000>  <b>Postscript figures</b></A></H2>
+<P>
+        It is also possible to include Postscript figures produced in other
+ways than through xfig: Use the command \ps{&lt;filename&gt;} instead of 
+\fig and place the postscript file &lt;filename&gt;.ps in the
+directory /\$n\_doc/bin with a soft link to it in \$n\_hlp. If it
+can not be easily recovered, it is advisable to protect it against accidental
+deletion!
+<P>
+<A NAME=.figref><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005400000000000000>  <b>Figure references</b></A></H2>
+<P>
+        For references to figures, use
+<P>
+  \figref{.&lt;label&gt;} and   \Figref{.&lt;label&gt;}
+<P>
+ These commands translate to hypertext links figure or Figure
+in the hypertext document, and to a standard reference figure &lt;n&gt; or 
+Figure &lt;n&gt; in the printed document.
+<P>
+<H1><A NAME=SECTION0006000000000000000>  <b>Session transcripts</b></A></H1>
+<P>
+        Verbatim transcripts of pieces of terminal dialogue controlling program
+execution are an important ingredient to documentation. Such transcripts are
+easily produced through the command 
+        ndoc S[cript] &lt;file name&gt; 
+This starts a cshell script session in which you execute the program of which
+you want a transcript. After exit from the script session, the collected script
+is automatically formatted into a LaTeX file &lt;file name&gt;.trs; what
+remains for you to do is to cut out the irrelevant parts and perhaps add some
+comments. A sample section of such a file is shown below
+<P>
+  <PRE> %
+\spbegin %
+\skeyword{USE\_SCN\_NODE} \sprompt{(input node name)} \sdefault{= *:}
+\suser{?} %
+\svbegin \begin{verbatim} 
+ Specify the node name from which the corrections should be calculated. 
+ * indicates the same as the output node name. 
+</PRE>  
+\end{verbatim}\svend 
+  <PRE> \spend
+%
+%
+\spbegin %
+\skeyword{USE\_SCN\_NODE} \sprompt{(input node name)} \sdefault{= *:}
+\suser{*} \sinline{Use the same SCN file} \spend
+%
+%
+\spbegin %
+\skeyword{USE\_SCN\_SETS} \sprompt{(Set(s) of input uv-data Sectors:
+g.o.f.c.s)} \sdefault{= "":} \suser{2.0.0.0.0} \sinline{Sets in job 2}
+\spend %
+%
+\spbegin %
+\skeyword{HA\_RANGE} \sprompt{(DEG) (HA range)} \sdefault{= *:}
+\suser{\scr} \sinline{Use all scans in these sets} %
+\svbegin \begin{verbatim} 
+   0123456789ABCD 
+ 0 -+++++++++++++ 
+ 1  -++++++++++++ 
+ 2   -+++++++++++ 
+ 3    -++++++++++ 
+ 4     -+++++++++ 
+ 5      -++++++++ 
+ 6       -+++++++ 
+ 7        -++++++ 
+ 8         -+++++ 
+ 9          -++++ 
+ A           -+++ 
+ B            -++ 
+ C             -+ 
+ D              - 
+</PRE>  
+\end{verbatim}\svend 
+  <PRE>
+\spend%
+</PRE>
+<P>
+        The file consists of sections delimited by \spbegin and 
+\spend, each consisting of a prompt with its reply and the ensuing
+output from the computer. LaTeX will treat these sections as blocks in which a
+page break can not occur. The following LaTeX commands are used:
+<P>
+ <UL><LI>   \skeyword, \sprompt and \sdefault are the
+components of a program prompt;
+<P>
+<LI>   \suser is the user's reply (in which \scr represents a
+null reply (carriage return only) and \seof an end-of-file
+(control-D)).;
+<P>
+<LI>   \sinline is an inline comment typed in during the session (an
+exclamation mark plus text following the answer to a prompt);
+<P>
+<LI>   \svbegin and \svend delimit the verbatim section in
+which computer output is rendered.
+<P>
+ </UL>
+<P>
+        It is necessary to check these scripts with some care. The system does
+occasionally get confused by the way the parameter interface splits long input
+and output lines. The errors are usually easily corrected.
+<P>
+ <UL><LI>   To replace parts of lengthy computer output, e.g. by ellipses; note
+that, since this occurs inside verbatim sections, LaTeX commands such as 
+\vdots can not be used. A line consisting of just three dots gives a
+satisfactory effect.
+<P>
+<LI>   To add \sinline comments. These must be placed either
+immediately following \suser commands or between an 
+\end{verbatim} and the adjacent \svend.
+<P>
+<LI>   To reduce the size of verbatim sections that are more than 80
+characters wide (e.g. sections from a log file).
+<P>
+ </UL>
+<P>
+<A NAME=.doc.sources.and.hyper><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  On-line Help files in the <i>NEWSTAR </i>
+<A HREF="../fig/doc_sources_and_hyper.ps"><STRONG>FIGURE</STRONG></A>  
+ .] <i>documentation system and their origins.  
+<BR>Files shown in boldface are the documentation and program sources, those
+shown in regular print are the derived Help files. 
+<BR>The full-drawn arrows indicate hypertext links for diagrams. The links to
+the other files types are not shown. The dotted arrow indicate links to in-line
+picture files that contain <A HREF="#.formulas"><b>formulas and tables</b></A>.    
+<BR>The dashed arrows indicate the relations between the files: Straight arrows
+represent a direct derivation, merging arrows a source-file inclusion. The
+capital letters on the arrows show in which procedure the derivation is
+implemented: 
+<BR>C= ndoc Cook; F= ndoc Fig; T= ndoc Test; P= ndoc Print. </i>
+<P>
+<A NAME=.doc.sources.and.print><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  Printable documents in the <i>NEWSTAR </i>
+<A HREF="../fig/doc_sources_and_print.ps"><STRONG>FIGURE</STRONG></A> 
+ .] <i>documentation system and their origins. 
+<BR>Files shown in boldface are the documentation and program sources, those
+shown in regular print are the derived printable files in the Help system.
+<BR>The dashed arrows indicate the relations between the files: Straight arrows
+represent a direct derivation, merging arrows a source-file inclusion. The
+capital letters on the arrows show in which procedure the derivation is
+implemented: F= ndoc Fig; T= ndoc Test; P= ndoc Print. </i>
+<P>
+        The documentation system encompasses three classes of files. The
+document source files reside in subdirectories of $n_doc; the code
+source files which may also be referenced reside in subdirectories of 
+$n_src. All hypertext files reside in a tree of subdirectories rooted in 
+\$n\_hlp. The interrelations of all these files are shown in 
+<A HREF=" #.doc.sources.and.hyper">figure</A>.
+<P>
+        The following types of source texts are used: 
+ <UL><LI>   Narrative LaTeX source texts: $n_doc/latex/&lt;name&gt;.tex
+<P>
+<LI>   Caption LaTeX source texts: $n_doc/fig/&lt;name&gt;.cap
+<P>
+<LI>   Standardised LaTeX files describing the private and public program
+parameter interfaces: $n_doc/intfc/&lt;name&gt;.tex. These files incorporate 
+.tef files derived from the program-parameter definition files
+(&lt;name&gt;.psc).
+<P>
+<LI>   ASCII texts: $n_doc/txt/&lt;name&gt;.txt
+<P>
+<LI>   Postscript files for which no source exists: $n_doc/ps/&lt;name&gt;.ps
+<P>
+<LI>   Code sources: $n_src/&lt;directory&gt;/&lt;name&gt;.&lt;extension&gt; 
+ </UL>
+<P>
+        In processing, temporary files are created in the current directory;
+their names either contain the string \_tmp. or end in .tmp. 
+ ndoc normally deletes them when exiting.
+<P>
+        latex2html, invoked by ndoc Cook, translates each file 
+&lt;name&gt;.tex into a file 
+\$n\_hlp/&lt;name&gt;/&lt;name&gt;.html. A large number of 
+.html files are therefore in subdirectories of 
+\$n\_hlp.
+<P>
+        ndoc Print creates .ps PostScript text files in \$n\_hlp. 
+        ndoc Fig creates .fps PostScript diagram files in 
+\$n\_hlp.
+<P>
+<H2><A NAME=SECTION0006100000000000000>  <b>Programmer's commands: Processing individual files </b></A></H2>
+<P>
+        The commands are of the form 
+        ndoc &lt;operation&gt; [-&lt;option&gt;] &lt;file&gt; 
+        &lt;file&gt; is the full file name including the extension, and it
+must be in the current directory. Wildcards may be used. 
+        The &lt;operation&gt; and -&lt;option&gt; arguments may be
+abbreviated and are case-insensitive. The following operations and options are
+available:
+<P>
+ <DL COMPACT><DT><DD>   P[rint] creates [a] PostScript file[s] from [a] .tex source
+file[s], with the following options: 
+   <UL><DT>
+<DD> -S[yntax] do nothing else; 
+  <DT>
+<DD> -V[iew] display the output using ghostview; 
+  <DT>
+<DD> -P[rint] print the PostScript output. 
+   </UL>
+<P>
+Print uses the LaTeX program. It attempts to suppress the verbose output
+of this program by filtering out everything except essential error messages. If
+you encounter a problem that you can not solve, submit your source file to the 
+<i>NEWSTAR </i> group for diagnosis.
+<P>
+<DT><DD>   C[ook] creates a Hypertext file from [a] .tex document[s]. This
+operation makes use of  latex2html . This program may crash over LaTeX syntax errors
+without properly analysing them. <em>It is therefore recommended to first do a 
+Print -Syntax check.</em>
+<P>
+<DT><DD>   K[ey] creates Hypertext files from [a] .pin, .psc or .pef
+file[s]
+<P>
+<DT><DD>   L[ink] creates the softlinks from the n_hlp directory to
+the $n_doc/txt and $n_src directories.
+<P>
+ </DL>
+<P>
+         ndoc checks the dates of its input and output files. If the output is
+newer than the date,  ndoc emits a message and proceeds with the next input
+file. This check is incomplete in that it does not check the status of 
+\input files such as figure captions.
+<P>
+        There are two ways of bypassing this check: 
+ <UL><LI>   Setting the environment variable n_force. 
+<LI>   touching the inpout file to set its modification time to the
+present time. 
+ </UL>
+<P>
+        When working in a shadow system,  ndoc makes no difference between hard
+copies and soft links to the master system: Both are unconditionally compiled.
+<P>
+<H2><A NAME=SECTION0006200000000000000>  <b><i>NEWSTAR </i> manager's commands: Maintaining the documentation system
+</b></A></H2>
+<P>
+        To recompile the entire documentation collection from its sources, one
+uses the command 
+          ndoc All 
+ndoc will ask which parts of the system to recompile, the default
+being 'yes' for all subsystems. In this mode of operation  ndoc bypasses the
+check for an up-to-date output file.
+<P>
+        One of the actions available in ndoc All is a systematic check
+of the correspondence between source and output files. This is a very useful
+action because it clears up leftovers of obsolete documents and pinpoints areas
+of trouble.
+<P>
+<H1><A NAME=SECTION0007000000000000000>  <b>Debugging .tex files</b></A></H1>
+<P>
+         ndoc goes a long way in filtering from the verbiage that LaTeX spews
+out the essential diagnostics. It shows the essential section of LaTeX output
+where the error is reported (including a line number) plus five lines of text
+in the middle of which the error was found. Very often this information
+suffices to pinpoint the error. If it does not, you may have to take a better
+look either at your source or at the &lt;file name&gt;_tmp.tex file that is
+the file LaTeX was actually processing. Note that the line number reported
+refers to this latter file!
+<P>
+        Specific errors that have been encountered and are not covered by this
+diagnosis mechanism are described below.
+<P>
+<H2><A NAME=SECTION0007100000000000000>  <b>LaTeX bugs</b></A></H2>
+<P>
+        Both ndoc Print and ndoc Cook make use of LaTeX and may
+therefore be affected by LaTeX bugs. For cases not covered here, refer to &quot;The
+LaTex Book&quot;, which is probably the best informed source about that program. 
+ <UL><LI>   Symptom: 
+        <em>The word dump appears in the place of a Figure or Table.</em>
+<P>
+        This is an obscure problem. One situation in which it has been observed
+is when a \figure environment is put at the very start of a document,
+i.e. without any preceding text. (This condition will not occur for regular
+documents but may occur in test situations.) It has also been seen in a case
+where a tabular environment was nested inside a table, in which
+case the solution was to remove the table environment.
+<P>
+<LI>   Symptom: 
+        <em>LaTeX complains about a 'runaway argument' in a \caption
+environment.</em>
+<P>
+        This may happen when the optional argument in square brackets is
+omitted. As of 940914, this argument is automatically provided for by 
+doc_preprocess.csh.
+<P>
+<LI>   Symptom: 
+        <em>ndoc Print runs without reporting any error, but produces a
+PostScript file in which figure references appear without numbers filled in.</em>
+<P>
+        This happens when the \label directive in a figure
+declaration is placed before the \caption command.!
+<P>
+<LI>   Symptom: 
+        <em>LaTeX reports: TeX capacity exceeded, sorry [parameter stack
+size=60].</em>
+<P>
+        This has been seen to happen when a \section title argument is
+too complicated, e.g. because it contains italicised text.
+<P>
+<LI>   Symptom: 
+        <em>LaTeX finds a $or _in a \textref file argument that is
+not escaped by a preceding backslash.</em>
+<P>
+        This may happen when the expansion of a command defined through 
+\newcommand contains a <A HREF="#.cross.ref">referencing command</A>. Fix
+the problem by including escape charaters in the \newcommand
+definition.
+<P>
+<LI>   Symptom: 
+        <em>LaTeX complains about &quot;Paragraph ended before \sbox was
+complete&quot; in a figure caption.</em>
+<P>
+        The \caption environment appears to be sensitive to formatting.
+In particular new paragraphs (i.e. blank lines) and \indent commands
+have been noted to produce this nasty error. In some cases it was found
+necessary to put the \label before the \caption. 
+ </UL>
+<P>
+<H2><A NAME=SECTION0007200000000000000>  <b>Processing errors in ndoc</b></A></H2>
+<P>
+        When LaTeX reports an error to  ndoc,  ndoc displays a five-line text
+section in the middle of which the error occurred. This is not from the
+original input text, but from the preprocessed text as it was eventually
+presented tp LaTeX. Most errors are easily recognised and traced back to the
+input  .tex  file.
+<P>
+ <UL><LI>   Symptom: 
+        An error occurs which is associated with lines from the .tex input that
+were concatenated by ndoc.
+<P>
+        This may very well be an error in the algorithm used by ndoc to merge
+paragraphs into single long lines. It is not necessarily clear why LaTeX does
+not accept the long line. An any rate, the recommended action is to check with
+the <i>NEWSTAR </i> manager.
+<P>
+<LI>   Symptom: 
+        ndoc cook stops with message 
+           nawk: record `[...]' has too many fields
+<P>
+        In preprocessing documents, ndoc formats paragraphs into single lines
+to make it easier to identify LaTeX command sequences. Find the offending
+paragraph in you documents and insert &lt;newline&gt;&lt;blank&gt; at some
+appropriate place. The leading paragraph will inhibit the merger of the two
+parts of the paragraph, yet LaTeX will format the two parts into one paragraph.
+<P>
+ </UL>
+<P>
+<H2><A NAME=SECTION0007300000000000000> <b>Processing errors in ndoc Cook</b></A></H2>
+<P>
+        The program  latex2html  on which ndoc Cook is based is rather lax on
+checking LaTeX syntax but may stumble over the consequences of an error missed.
+<i>It is therefore strongly recommended to first check the syntactical
+correctness of the .tex file through ndoc P</i>. 
+ <UL><LI>   Symptom: 
+        .DVI file can't be opened
+<P>
+         latex2html  runs LaTeX on a selection from the .tex file consisting of
+formulas, tabular material and diagrams. This run failed to produce a 
+.dvi file, but  latex2html  gobbled up all the error information. This error
+may be due to improper configuration of your system, <em>e.g.</em> a misplaced 
+.sty file. It is virtually impossible to diagnose except by using a 
+<A HREF="#.latex2html">modified version of  latex2html </A>.
+<P>
+<LI>   Symptom 
+ <PRE> The nplot_descr.aux file was not found, so sections will not
+be numbered and cross-references will be shown as icons. 
+</PRE>
+<P>
+        Your .tex file contains a \ref directive. Convert al 
+\refs to \textrefs.
+<P>
+<LI>   Symptom: 
+        Commands that are normally accepted are reported as unknown.
+<P>
+        This is likely to be the result of a syntax error. (For example, a
+missing \end{itemize} will cause \item to be reported as
+unknown.) Check your input file by running ndoc Print on it.
+<P>
+<LI>   Symptom: 
+        xmosaic can not find a file pointed at by a hypertext link.
+<P>
+        Note the file name appearing at the bottom of the xmosaic window
+when you point at the reference. This reference should be in either of the
+forms:
+<P>
+        &lt;file name&gt;/&lt;file name&gt;.html 
+\indent \verb../&lt;file name&gt;/&lt;file name&gt;.html
+<P>
+If it starts in a /, you have to replace your  latex2html  by the 
+<A HREF="#.latex2html">modified version</A>.
+<P>
+<LI>   Symptom: 
+        latex2html warns that the .aux file was not found but
+otherwise ndoc Cook seems to complete normally.
+<P>
+        The precise nature of this error is not understood, but it seems to
+indicate that something is wrong in a cross-reference. (e.g. a LaTeX 
+\ref command). It has been seen to occur when a \ref with a
+label name containing dots is used (cf. the section on <A HREF="#.cross.ref">cross references</A>). 
+ </UL>
+<P>
+<A NAME=.latex2html><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0008000000000000000> <b>latex2html </b></A></H1>
+<P>
+         latex2html  is a public-domain perl script created by Nikos Drakos at Leeds
+University, England (Email: nikos@cbl.leeds.ac.uk) and available through
+anonymous ftp. It has been found to be a reliable and highly capable program.
+Apart from configuring it to the local environment, two changes were found
+necessary:
+<P>
+ <UL><LI>   All lines containing the string s/\W//g must be commented out by
+prefixing them with a #. This makes  latex2html  capable of handling relative
+file references and removes an inconsistency it the processing of labels and
+references.
+<P>
+<LI>   After the line
+<P>
+system(&quot;$LATEX $$_images.tex&quot;);
+<P>
+insert the lines
+<P>
+ <PRE> 
+        if (!-e "20756_images.dvi") 
+          {system("cat 20756_images.log"); die "Failure to process formulas"; } 
+</PRE>
+ </UL>
+<P>
+<A NAME=.formulas><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0008100000000000000>  <b>Formulas and the like in latex2html </b></A></H2>
+<P>
+        LaTeX allows many constructs, such as formulas, tables etc., for which
+there is no HTML counterpart (yet).  latex2html  converts each single occurrence of
+these into a little picture file that is linked in-line into the .html
+document. The pictures are stored in .png files in the same directory as
+the .html file.
+<P>
+        Since building these pictures is a very time-consuming process,  latex2html 
+seeks to reuse them as much as possible whenever it recompiles a .tex
+file. To this end, it maintains an administration in the file images.pl
+in the .html file's directory. Therefore, to insure the integrity of the
+.html document, both the .png files and images.pl must be left in
+place. As of May 1996, doc_cook.csh contains a section of code that
+finds all in-line picture references in the renewed .html file, reports
+any referred-to files that are missing and deletes unreferenced .png
+files.
+<P>
+        In cases a .png file is reported missing, the way to get it
+rebuilt is to delete images.pl in order to force  latex2html  to rebuild all
+the picture files from scratch.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/doc_guide/images.pl b/doc_guide/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/doc_guide/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/doc_guide/labels.pl b/doc_guide/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..6c237b46a7b0fb668ad51072fc94a5a12cbc9b30
--- /dev/null
+++ b/doc_guide/labels.pl
@@ -0,0 +1,20 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".eqref"} ="$URL/doc_guide.html"; 
+$external_labels{".cross.ref.latex"} ="$URL/doc_guide.html"; 
+$external_labels{".fig"} ="$URL/doc_guide.html"; 
+$external_labels{".doc.sources.and.hyper"} ="$URL/doc_guide.html"; 
+$external_labels{".figref"} ="$URL/doc_guide.html"; 
+$external_labels{".cross.ref.other"} ="$URL/doc_guide.html"; 
+$external_labels{".caption"} ="$URL/doc_guide.html"; 
+$external_labels{".contents"} ="$URL/doc_guide.html"; 
+$external_labels{".latex2html"} ="$URL/doc_guide.html"; 
+$external_labels{".doc.sources.and.print"} ="$URL/doc_guide.html"; 
+$external_labels{".cross.ref"} ="$URL/doc_guide.html"; 
+$external_labels{".ps"} ="$URL/doc_guide.html"; 
+$external_labels{".formulas"} ="$URL/doc_guide.html"; 
+$external_labels{".layout"} ="$URL/doc_guide.html"; 
+$external_labels{".xfig"} ="$URL/doc_guide.html"; 
+
+1;
\ No newline at end of file
diff --git a/doc_organisation.txt b/doc_organisation.txt
new file mode 100644
index 0000000000000000000000000000000000000000..4f37612030a1c841c912ceebdf8e8aa56c342538
--- /dev/null
+++ b/doc_organisation.txt
@@ -0,0 +1,776 @@
+The Organisation of Newstar documentation
+-----------------------------------------
+
+
+@(#) newdoc.txt  v1.6 08/09/93 CMV
+     newdoc.txt  v1.5 03/09/93 CMV
+     newdoc.txt  v1.4 05/08/93 CMV
+
+
+1. Introduction
+---------------
+
+
+This document defines the format and organisation of the Newstar 
+documentation. The next sections describe the way documentation can be 
+accessed, the way in which the documentation as a whole is organised and
+the way in which documentation should be formatted. This corresponds to the
+the point of view of a user, a Newstar site manager and a documentation 
+editor respectively. Appendices give detailed instructions for naming 
+conventions and editing.
+
+End-users who are just interested in using the documentation only
+need to read section 2, site managers and contributors should read
+the remaining sections as well.
+
+
+2. Accessebility
+----------------
+
+The Newstar user documentation is accessible in three forms:
+
+  1e. As on-line help from program prompts, either as "dumb-terminal"
+      text or through NCSA's xmosaic browser decribed below.
+
+  2e. By browsing the documentation using xmosaic or any other 
+      hypertext reader (e.g. the "dumb-terminal" reader for the
+      World Wide Web, developed at CERN)
+
+  3e. By reading the printed form of the documentation (the Newstar
+      Cookbook) either on paper or using an appropriate Postscript or
+      dvi viewer.
+
+
+The documentation is organised as a hypertext network, which means that
+various smaller pieces of information are connected by "links". This
+not only gives flexible index and glossary functions, but also allows for 
+a menu-like presentation of the on-line documentation (options 1e and
+2e). The pieces of information can also be put together in a single 
+large document, the Newstar Cookbook, where "links" show up as the
+usual references like "see also section 1.3".
+
+To access the on-line documentation, the user enters one or more
+questionmarks (?) in response to a prompt. If a single ? is entered,
+the help text will be shown on the terminal screen. If more than 
+one ? is entered, a separate window will be opened in which xmosaic 
+presents the requested information. If no window could be started,
+the help text will be given on the terminal. When an xmosaic window
+is open, all help text will be presented there, regardless of the
+number of questionmarks typed. The window remains active when the
+program quits, so the same window can be used by several programs 
+(so far only if run on the same host).  Xmosaic has been developed at 
+the NCSA and has many interesting options which fall outside the 
+scope of this document. 
+
+If the information is shown through xmosaic, the user can access the 
+remainder of the documentation though that browser. Certain words in 
+the text will appear underlined. The user can move the mouse on one
+of these words and click the left mouse button. Xmosaic will now display
+the information that is associated with the underlined word. This can 
+be a brief explanation of that word (glossary function) or a related 
+piece of documentation.
+
+Any help text explaining a prompt will have at least the following links
+appended to it (words within underscores will appear underlined):
+
+    More information:
+         _List of keywords_ for NSCAN
+         _The Newstar Cookbook_
+         Description of _program NSCAN_
+         Description of _common keywords_
+         The _DWARF User Interface_
+
+The list of keywords for any program will have the following list appended
+to it:
+
+    More information:
+         _The Newstar Cookbook_
+         Description of _program NSCAN_
+         Description of _common keywords_
+         
+Prompts related to specific file types will also contain links to
+documents revealing the secrets of such files.
+
+The hypertext network can also be accessed from outside a Newstar program
+by typing "nhyper" at the command line. This will present you a page
+with general information containing links to the table of contents of 
+the Newstar Cookbook and to some general help files (in particular the
+Newstar News file).
+
+
+3. Organisation
+---------------
+
+There are four different sources of information for the Newstar 
+documentation:
+
+  - Cookbook sections, which are LaTeX documents (with some restrictions
+    on the commands to be used, see below). They may contain ordinary
+    text, terminal scripts (created with help of "nscript", see below)
+    and may include postscript figures. These LaTeX files are translated
+    into the HTML format for inclusion in the hypertext network.
+
+    The LaTeX source files are all found in directory $n_src/doc/cook
+    The HTML versions are found in directory $n_src/doc/html
+ 
+
+  - Descriptive text (help-text) for program keywords, stored in 
+    so called PIN files (extensions .pin, .psc or .pef). The PIN files
+    are translated into LaTeX (for inclusion in the printed version
+    of the cookbook) and into HTML for inclusion in the hypertext
+    network. 
+
+    The PIN files are located in $n_src/nscan etc.
+    The LaTeX versions are found in directory $n_src/doc/cook
+    The HTML  versions are found in directory $n_src/doc/html
+
+
+  - Miscellaneous documents called Memo's, which are generally plain
+    ASCII files. For details on Newstar Memo's, refer to document
+    newmemo.txt
+
+    The NEWSTAR Memo's are found in directory $n_src/doc/memo
+
+  - Program source files can contain specially marked documentation
+    which can be extracted. The extracted documentation can be included
+    in the hypertext network.
+
+    Documentation from file abc.def is stored in $n_src/doc/extractabc.def
+
+
+  - Bugreports, with their present status and history, are a separate 
+    issue and are described in document bug_reports.txt.
+
+    Bugreports are found in directory $n_src/doc/bug
+
+
+Apart from these files there are:
+ 
+  - Files with LaTeX commands used to generated printed versions of the
+    cookbook or parts thereof. These files are found in $n_src/doc/cook
+    and have names cb_*.tex
+
+  - Index files for the hypertext network, generated automatically in
+    directory $n_src/doc/html
+
+
+Files are maintained though utility $n_src/sys/document.csh which uses 
+the program docaid.c ($n_exe/docaid.exe).
+
+There is a groupfile $n_src/doc/doc.grp listing files in or below $n_src/doc
+that have been created "by hand". A groupfile $n_src/doc/auto.grp will be
+updated together with the hypertext indices.
+
+Note: the files in directories keys and html are derived from files in 
+the source tree ($n_src). These files are updated automatically when 
+other files (e.g. ppd-files) are being compiled.
+This validates the principle that the source tree contains only all
+files needed for installation. The alternative would be to create a 
+directory in either the library or the executable tree for
+documentation. However, I think it is important that a full set of 
+documentation is available before installation. In my opinion this 
+outweights the violation of the source tree policy. It also makes
+it possible that, at least for the time being, files in the keys 
+and html directory are explicitly updated at NFRA. 
+
+
+An update of the documentation proceeds as follows:
+
+ "ndoc keys all"  Convert all pin, psc and pef files to LaTeX and html files
+ "ndoc extr all"  Extract documentation from files in $n_src/sys
+ "ndoc html all"  Convert all cookbook sections to html files
+ "ndoc index"     Make indices for the files in the html directory
+
+A shorthand for these commands is:  "ndoc full"
+
+Updating the documentation takes a few minutes and needs to be done at
+a single host only for all machines that share a filesystem.
+
+Other options of ndoc are:
+
+ "ndoc script"    Start the script utility (see Appendix C)
+ "ndoc print"     Print part of the Newstar Cookbook 
+ "ndoc hyper"     Start the hypertext browser at the Newstar Home Page
+ "ndoc memo"      Insert an external file into the Newstar Memo system
+
+The print command will ask you for a cookbook file to print. 
+
+
+4. Formatting 
+-------------
+
+Since a large amount of documentation is available already in 
+LaTeX, we choose to use LaTeX as our principle documentation 
+format. Although it is probably easier to convert an html document 
+to a LaTeX source than vice versa, this approach allows us to make 
+a fast start. To facilate translation we put some constrains on the
+infinite flexibility of LaTeX. These are given in the "style guide"
+found as Appendix A.
+
+Appendix A lists the "allowed" LaTeX commands, these are the commands
+that will be recognised by the LaTeX to HTML converter. Any other
+command will, for the time being, show up as ordinary text in the 
+xmosaic browser.
+
+The most important rules for writing documentation are the following:
+
+    1e. The basic element of Cookbook documentation is the section.
+        Each section should appear in a separate file.
+        It is well possible (and in fact preferable) to break
+        up sections in smaller units. 
+
+    2e. Figures, tables and other blocks containing large amounts 
+        of LaTeX commands not listed in Appendix A should be put in the
+        Cookbook by means of an \input or \include command. The embedding
+        commands (like \begin{figure} and \end{figure}) should also be
+        in that separate file. 
+
+        Such figures and tables will be converted to dvi or postscript 
+        files in the html directory.
+
+    3e. Terminal sessions can be included within cookbook sections.
+        However, for extended examples it is better to put them in a
+        separate file which is included by an \input or \include command.
+        This makes the hypertext more readable and facilates regeneration
+        if the programs change.
+
+        For a list of the LaTeX commands that will appear in terminal 
+        sessions, refer to Appendix A.
+ 
+        Refer to Appendix C for instructions on how to make 
+        terminal sessions using the  nscript command
+
+    4e. Within a section, the target of a hypertext link is marked 
+        through the \label command. See the naming conventions in 
+        Appendix B (eg. \label{nscan.descr.general}) 
+
+    5e. Within a section, a hypertext link is made though the \ref, \refn, 
+        \input and \include commands. The \input and \include commands
+        will translate to a lines: "See also: _Name of the include file_" 
+        in the browser. The \ref command will translate as follows:
+
+         ... This is explained in \ref{nscan.descr} where we see ...    ->
+         ... This is explained in _here_ where we see ...
+
+         ... This is explained in \ref{nscan.descr}{Chapter 4} ...    ->
+         ... This is explained in _Chapter 4_ ...
+
+        The last for will give a somewhat confusing output in the 
+        printed version.
+ 
+    6e. Within PIN files, links can also be made through the \ref command. 
+        In the "dumb-terminal" on-line help, these \ref commands show up 
+        as text and may at best serve as an entry in the printed version 
+        of the Cookbook.
+
+    7e. Filenames and labels should obey a strict naming scheme to 
+        allow for the proper files to be constructed. This naming 
+        scheme is given in Appendix B.
+
+
+5. Contributing to the Newstar documentation
+--------------------------------------------
+
+Contributions to the Newstar documentation are very welcome, in particular
+new recipes are appreciated. To contribute a recipe, put your text in a 
+file either as plain ASCII (with some indication as to sections etc) or
+using the LaTeX commands from Appendix A. Preferably you should use the 
+naming conventions from Appendix B. Send the files to me and we will put
+them in their proper place.
+
+
+    
+Appendix A:  Style Guide for the Newstar Cookbook
+----------
+
+The following conventions should be obeyed when writing LaTeX documents
+that should be converted to html using the docaid program:
+
+ - Only commands in the recognised subset (see below) may be used.
+
+ - The \begin{...} and \end{...} commands should be on a line of 
+   their own.
+
+ - To change font temporarily, use something like {\bf ...}, without
+   any space between the brace and \bf. Curently recognised fonts 
+   are:     \rm \bf \it \tt \tiny
+
+ - For verbatim text use either 
+
+      \begin{verbatim}
+      ...
+      \end{verbatim}
+
+   or {\tt ...} (with special characters escaped).
+   The commands used by nscript (\sline etc) use the latter strategy.
+
+ - The tabbing environment can be used inside documents with the
+   following restrictions. There should be a single definition line 
+   (with \= commands), which should follow the \begin{tabbing} line
+   without intervening empty/comment lines. The definition line will
+   not be copied to the hypertext, so use the \kill command.
+
+   Since tabbing in HTML is extremely poor, do not expect to much of 
+   presentation in xmosaic.
+
+ 
+The following subset of LaTeX commands is currently recognised by docaid.
+
+/*
+
+   Translation table for LaTeX to html
+   
+   Format: 
+
+     Column 1: name of the command (minimal match) without leading \
+     Column 2: length of command (all zero's, set by program)
+     Column 3: action routine
+                 NULL  No special action (just print replacement string)
+                _PUSH  Print closing tag for the replacement string when
+                        closing } is found
+                _SKIP  Skip any arghuments to the command
+                other  Special action, refer to code for details
+     Column 4: replacement string (or NULL if none)
+     
+    
+   Any LaTeX commands that do not start with a \ are handled separately,
+   however they are included in this table inside comments.
+
+*/
+     
+/*
+     The following lines correspond to definitions in cb_symbols.tex
+     Please update this list when cb_symbols.tex is changed
+*/
+   "cbdir",     0, NULL, "$n_src/doc/cook",
+   "NEWSTAR",   0, NULL, "<EM>NEWSTAR</EM>",
+   "Nseries",   0, NULL, "<EM>NEWSTAR</EM>",
+
+   "cVis",      0, NULL, "<EM>V</EM>",   
+   "pvis",      0, NULL, "<EM>Phi</EM>",
+   "avis",      0, NULL, "<EM>|V|</EM>",
+   "lavis",     0, NULL, "<EM>rho</EM>",
+
+   "cGain",     0, NULL, "<EM>G</EM>",
+   "cNoise",    0, NULL, "<EM>N</EM>",
+   "cCadd",     0, NULL, "<EM>C</EM>",
+
+   "perr",      0, NULL, "<EM>p</EM>",
+   "gerr",      0, NULL, "<EM>g</EM>",
+   "lerr",      0, NULL, "<EM>q</EM>",
+   "dang",      0, NULL, "<EM>phi</EM>",
+   "derr",      0, NULL, "<EM>Delta</EM>",
+   "eerr",      0, NULL, "<EM>Theta</EM>",
+
+   "Apol",      0, NULL, "<EM>epsilon</EM>",
+   "Bpol",      0, NULL, "<EM>eta</EM>",
+
+   "wgt",       0, NULL, "<EM>W</EM>",
+   "pwgt",      0, NULL, "<EM>W**p</EM>",
+   "lwgt",      0, NULL, "<EM>W**g</EM>",
+
+   "pzd",       0, NULL, "<EM>psi</EM>",
+
+   "farang",    0, NULL, "<EM>chi</EM>",
+
+/*
+   Here are the commands defined in cb_preamble.tex
+   Please update this list when cb_preamble.tex is changed
+*/
+  
+   "cbfile{",    0, _PUSH, "<TT>",
+   
+   "skeyword{",  0, _PUSH, "<DD><STRONG>",
+   "sprompt{",   0, _PUSH, "<EM>",
+   "sdefault{",  0, _PUSH, NULL,
+   "suser{",     0, _PUSH, " <KBD>",
+   "sline{",     0, _PUSH, "<DD><SAMP>",
+   "slong{",     0, _PUSH, "<DD><SAMP>",
+   "sskip",      0, NULL,  "<P>",
+   "scmd{",      0, _PUSH, "<DD>&gt; <KBD>",
+
+   "sinline{",  0, _PUSH, " . . . <EM>",
+   "scomment{", 0, _PUSH, "<EM><P>",
+
+   "setc",      0, NULL,  "<P>:<P>:<P>",   
+   "scr",       0, NULL,  "&lt;CR&gt;",
+   "gloshead{", 0, _PUSH, "<H2>",
+
+
+/*
+   Now follow the supported built-in LaTeX special characters
+
+   A tilde (~, smallspace) is replaced by an normal space character
+
+   Please mind that all commands below are prefixed by a backslash!
+*/
+
+   " ",          0, NULL, " ",
+   "$",          0, NULL, "$",
+   "#",          0, NULL, "#",
+   "&",          0, NULL, "&amp;",
+   "{",          0, NULL, "{",
+   "}",          0, NULL, "}",
+   "%",          0, NULL, "%",
+   "_",          0, NULL, "_",
+   "-",          0, NULL, NULL,
+   "\"o",        0, NULL, "&ouml;",
+   "wedge",      0, NULL, "^",
+
+   "arctan",     0, NULL, "<STRONG>arctan</STRONG>",
+   "ast",        0, NULL, "*",
+   "bigotimes",  0, NULL, "<STRONG>*</STRONG>",
+   "cdots",      0, NULL, "...",
+   "circ",       0, NULL, "o",
+   "copyright",  0, NULL, "(c)",
+   "delta",      0, NULL, "<EM>delta</EM>",
+   "div",        0, NULL, "-/-",
+   "equiv",      0, NULL, "==",
+   "exp",        0, NULL, "<STRONG>exp</STRONG>",
+   "gg",         0, NULL, "&gt;&gt;",
+   "infty",      0, NULL, "<STRONG>inf</STRONG>",
+   "lambda",     0, NULL, "<EM>lambda</EM>",
+   "ldots",      0, NULL, "...",
+   "log",        0, NULL, "<STRONG>log</STRONG>",
+   "over",       0, NULL, "/",
+   "phi",        0, NULL, "<EM>phi</EM>",
+   "pm",         0, NULL, "+/-",
+   "rightarrow", 0, NULL, "--&gt;",
+   "sigma",      0, NULL, "<EM>sigma</EM>",
+   "sqrt",       0, NULL, "<STRONG>sqrt</STRONG>",
+   "sum",        0, NULL, "<STRONG>SUM</STRONG>",
+   "theta",      0, NULL, "<EM>theta</EM>",
+   "times",      0, NULL, ".",
+   "vdots",      0, NULL, ":",
+
+/*
+   Line separating commands
+   
+   An empty line will also translate to a <P> tag
+*/
+   
+  "\\",                    0, NULL,         "<DD>", /* Trick to get newline */
+  "par",                   0, NULL,         "<P>",
+  "newpage",               0, NULL,         "<P>",
+  "vspace",                0, _SKIP,        "<P>",
+
+/*
+   Math modes
+   
+   $>$ and $<$ translate to the &gt; and &lt; entities,
+   any other $ .... $ construct is identical to \( ... \)
+   
+   $$ ... $$ constructs are identical to \[ ... \]
+*/
+                                                       /* Inline math mode  */
+  "(",                     0, NULL,         "  <EM> ",
+  ")",                     0, NULL,         " </EM> ",
+  "begin{math}",           0, NULL,         "  <EM> ",
+  "end{math}",             0, NULL,         " </EM> ",
+                                                      /* Display math mode */
+  "[",                     0, NULL,         "<P><EM>",
+  "]",                     0, NULL,         "</EM><P>",  
+  "begin{displaymath}",    0, NULL,         "<P><EM>",  
+  "end{displaymath}",      0, NULL,         "</EM><P>",  
+  "begin{equation}",       0, NULL,         "<P><EM>",  
+  "end{equation}",         0, NULL,         "</EM><P>",  
+  "begin{eqnarray}",       0, NULL,         "<P><EM>",  
+  "end{eqnarray}",         0, NULL,         "</EM><P>",  
+
+/*
+  Headings and references
+*/
+  "title{",                0, _PUSH,        "<H1>",
+  "chapter{",              0, _PUSH,        "<H1>",
+  "section{",              0, _PUSH,        "<H1>",
+  "subsection{",           0, _PUSH,        "<H2>",
+  "subsubsection{",        0, _PUSH,        "<H3>",
+
+  "label{",                0, _LABEL,       NULL,
+  "ref{",                  0, _ANCHOR,      NULL,
+  "pageref{",              0, _ANCHOR,      NULL,
+  "input{",                0, _ANCINP,      NULL,
+  "include{",              0, _ANCINP,      NULL,
+
+  "eqno{",                 0, _PUSH,        "<EM>",
+ 
+/*
+  Many things are just ignored
+*/
+  "tableofcontents",       0, NULL,         NULL,
+  "listoffigures",         0, NULL,         NULL,
+  "listoftable",           0, NULL,         NULL,
+  "makeindex",             0, NULL,         NULL,
+  "documentstyle",         0, _SKIP,        NULL,
+  "hskip",                 0, _SKIP,        NULL,
+  "hspace",                0, _SKIP,        NULL,
+  "hline",                 0, NULL,         NULL,
+  "maketitle",             0, NULL,         NULL,
+  "nonumber",              0, NULL,         NULL,
+  "pagestyle",             0, _SKIP,        NULL,
+  "pagenumbering",         0, _SKIP,        NULL,
+  "parbox",                0, _SKIP,        NULL,
+
+/*
+  Special handling for some environments
+*/  
+  "begin{thebibliography}",0, NULL,         "<H1>Bibliography</H1>\n",
+  "end{thebibliography}",  0, NULL,         "<P>",
+  "bibitem",               0, _LABBIB,      NULL,
+  "cite",                  0, _ANCBIB,      NULL,
+
+  "begin{tabbing}",        0, _TABBING,     NULL,
+  "end{tabbing}",          0, _TABBING,     "<P>",
+  ">",                     0, NULL,         " ",
+
+  "begin{figure",          0, _FIGURE,      NULL,
+  "end{figure",            0, _FIGURE,      "<P>",
+  "begin{tab",             0, _TABLE,       NULL,
+  "end{tab",               0, _TABLE,       "<P>",
+  "caption{",              0, _PUSH,        "<EM>",
+  
+  "begin{enumerate}",      0, NULL,         "<OL>",
+  "end{enumerate}",        0, NULL,         "</OL>",
+
+  "begin{itemize}",        0, NULL,         "<UL>",
+  "end{itemize}",          0, NULL,         "</UL>",
+  "item{",                 0, _PUSH,        "<LI> <STRONG>",
+  "itemitem{",             0, _PUSH,        "<LI> <STRONG>",
+  "item",                  0, NULL,         "<LI>",
+  "itemitem",              0, NULL,         "<LI>",
+  
+  "begin{verbatim}",       0, _VERBON,      "<PRE>",
+  "begin{verbatim*}",      0, _VERBON,      "<PRE>",
+  "end{verbatim}",         0, _VERBOF,      "</PRE>",
+
+/*
+  All other environments are just skipped.
+  Note: the order in the table is important here!
+*/    
+  "begin{",                0, _SKIP,        "<P>",
+  "end{",                  0, _SKIP,        "<P>",
+  "author{",               0, _SKIP,        NULL,
+
+  "end",                   0, NULL,         NULL,
+
+/*
+  Font selections. These are special case things, since the required
+  syntax for a temporary font change is:
+  
+    {\bf ... }
+    
+  etc, so we test on the {\ rather than on the \
+
+  "rm",                    0, _PUSH,        "<STRONG>",
+  "bf",                    0, _PUSH,        "<STRONG>",
+  "em",                    0, _PUSH,        "<EM>",
+  "it",                    0, _PUSH,        "<EM>",
+  "tt",                    0, _PUSH,        "<TT>",
+
+  Any isolated occurence of a font change is just ignored.
+  So you should use   \chapter{{\it Something fresh}} 
+  and not             \chapter{\it Something fresh}
+  
+*/
+  "tiny",                  0, NULL,         NULL,
+  "bf",                    0, NULL,         NULL,
+  "it",                    0, NULL,         NULL,
+  "rm",                    0, NULL,         NULL,
+  "tt",                    0, NULL,         NULL,
+  
+/*
+  The end of the table should be marked by a NULL command!
+*/
+  NULL,                    0, NULL,         NULL
+
+
+
+Appendix B:  Naming convention for Newstar Documentation
+-----------  
+
+***** ALL LABELS AND FILENAMES SHOULD BE IN LOWER CASE *****
+
+
+1e. Labels
+
+The following conventions should be used for the naming of labels 
+and references (commands \ref{...}, \pageref{...} \label{...}):
+
+  - The name of the label should consist of two or more elements 
+    separated by dots. The first two elements uniquely identify the
+    file to which the reference is made. As a consequence all labels 
+    in a file start with the same two elements. The remaining
+    elements serve as a reference within the file.
+
+  - The label corresponding to a file  a_b    is  a.b
+    A label within this file might be  a.b.c  or  a.b.c.d 
+
+    The label corresponding to a file  a_b_x    is  a.b_x
+    A label within this file might be  a.b_x.c  or  a.b_x.c.d_y-z 
+
+  - References to keywords should be made as follows: 
+
+     \ref{<name of pin/psc/pef file>.<name of keyword>}
+
+ *   In general the name of the pin/psc/pef file will be the name of
+ *   the program. For common keywords (including things like SCN_SETS)
+ *   the name of the PEF file should be used!
+
+
+  - Figures, tables, formulea and other pieces of "difficult" LaTeX 
+    will be included as GIF images, and should therefore be in separate
+    files. These files should have names fig_*.tex, tab_*.tex and 
+    eqn_*.tex. Normal labeling conventions apply to such files.
+
+For bibliographic references (commands \bibitem and \cite) the normal
+LaTeX conventions apply.
+
+
+2e. Filenames
+
+The cookbook is built based on the following tree (all filenames have
+extension .tex):
+                                                    Label
+  cookbook  (tittle page, table of contents)        cookbook
+   |
+   |
+   +-- ch_biblio                                    ch.biblio
+   |
+   +-- ch_general                                   ch.general
+   |    |
+   |    +-- gen_intro                               gen.intro
+   |    :
+   |
+   +-- ch_recipes                                   ch.recipes
+   |    |
+   |    +-- rcp_line_21cm                           rcp.line_21cm
+   |    +-- rcp_linear_polarisation                 rcp.linear_polarisation
+   |    :
+   |
+   +-- ch_files                                     ch.files
+   |    |
+   |    +-- files_descr                             files.descr
+   |    +-- scn_descr                               scn.descr
+   |    +-- mdl_descr                               mdl.descr
+   |    :
+   |
+   +-- ch_programs                                  ch.programs
+   |    |
+   |    +-- common_descr                            common.descr
+   |    +-- common_keys                             common.keys
+   |    |    |
+   |    |    + ngen_comm                            ngen.comm
+   |    |    :
+   |    |
+   |    +-- nscan_descr                             nscan.descr
+   |    +-- nscan_keys                              nscan.keys
+   |    |    |
+   |    |    + ngen_short                           ngen.short
+   |    |    :
+   |    |
+   |    +-- ncalib_descr                            ncalib.descr
+   |    +-- ncalib_redun                            ncalib.redun
+   |    +-- ncalib_polar                            ncalib.polar
+   |    +-- ncalib_keys                             ncalib.keys
+   |    |
+   |    :
+   |
+   +-- ch_appendices                                ch.appendices
+        |
+        + apx_wsrtfactsheet                         apx.wsrtfactsheet
+        + apx_arquery                               apx.arquery
+        :
+
+
+Files with keyword descriptions are generated automatically from the
+pin/psc/pef files:
+
+  - Each pin, psc and pef file is translated into a single LaTeX file
+    <name>_keys.tex (for pin/psc) or <name>_comm.tex (for pef). These 
+    files contain the full description of each keyword define in the
+    pin/psc/pef file. For pef files, a keyword summary is generated 
+    in file <name>_short.tex. An INCLUDE=NAME_PEF keyword in a psc file 
+    will be translated in a \include{name_short} and a \ref{name.comm}
+  
+  - Each pin, psc and pef file is translated into a html file with
+    links to files with information on the individual keywords.
+    The index file has name <name>_keys.html (for pin/psc) or 
+    <name>_comm.html (for pef). The files with keyword information are
+    named <name>_<keyword>.html
+
+Files with names fig_*.tex, tab_*.tex and eqn_*.tex will be included
+as GIF figures.
+
+
+Appendix C:  Creating scripts of terminal sessions
+-----------
+
+To create a script of a terminal session, the command
+
+   $n_src/sys/document.csh script [file]    
+
+should be used, this is conveniently aliased to "nscript".
+If no filename is given, you will be prompted for one.
+
+This command will start the script command. The user has to initialise
+Newstar by typing "$go" (this is not necessary if initialisation is done
+in the user's .cshrc file). The initialisation procedure (in 
+$n_src/sys/newstar_init.csh) notices that the script utility is used 
+and will switch the DWARF bell "on". The prmpt will be set to "script> ".
+You can execute all commands you like and then enter either "exit" or ^D. 
+The terminal session will now be transformed to a LaTeX file, which you 
+can edit at wish.
+
+The nscript command will ask you wether the terminal script should be
+"Latex'ed" and printed or displayed (using xdvi, which should be in 
+your path). Often, you will want to edit the file first and then
+view it. This is possible by typing:
+
+    nscript -p [file]
+
+When answering to system prompts, you can add comments by prefixing 
+them with a semicolon followed by a hash mark, e.g.:
+
+ script> dwe nscan   ;# First we start reading data from tape
+ script> ls -l ;      # This gives a directory listing
+
+If the hash is the first non-blank character on the line, the comment 
+will be on a line of it's own.
+ 
+ script> # To start newstar, just type the following commands:
+
+
+When answering to DWARF prompts, you can add comments by prefixing
+them with an exclamation mark, e.g.:
+
+ LEVELS = -20 -10 : 20 ! For this test, we use a single level
+ OPTION (blabla) = QUIT : ! No further processing needed!
+
+In the latter example, the second exclamation mark will just show up
+as an exclamation mark (of course), the "empty" user respons will 
+translate to "<CR>" in the output.
+
+
+   NB: In order to facilate the script command, the DWARF "bell" is 
+       now rung at the start of the prompt (used to be at the end).
+       The exclamation-mark comments turned out to be an existing DWARF
+       feature that had somewhat faded in the mist of times.
+
+The following LaTeX commands are used in translated terminal sessions;
+they are defined for LaTeX in $n_src/doc/cook/cb_preamble.tex:
+
+   \skeyword{ name of keyword }
+   \sprompt{  text of prompt  }
+   \sdefault{ default value   }
+   \suser{    user response   }
+
+   \sline{    line with terminal output }
+   \slong{    long line with terminal output }
+
+   \scmd{      respons of user to operating system prompt }
+
+   \sinline{  inline comment }
+   \scomment{ comment that is on a line of it's own }
+   \setc      % Vertical dots replacing terminal output
+   \scr       % Carriage Return in fixed width font
+
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+h(WWW)e(serv)o(er.)27 b(F)m(or)16 b(this)0 851 y(purp)q(ose,)g(a)f
+(directory)h($n)p 429 851 V 15 w(hlp/src)f(m)o(ust)g(b)q(e)g(created)i
+(with)e(a)g(shado)o(w)g(directory)h(tree)g(con)o(taining)e(copies)i(of)
+f(only)0 901 y(those)g(\014les)f(that)g(are)g(referenced)j(\(see)e(ndo)
+q(c)f(options)g(b)q(elo)o(w\)..)118 975 y(A)f(new)f(pro)q(cedure,)j(do)
+q(c)p 514 975 V 15 w(cop)o(y)m(.csh,)d(has)h(b)q(een)g(created)h(for)e
+(this)h(purp)q(ose.)18 b(It)13 b(is)f(driv)o(en)g(b)o(y)h(an)f(in)o
+(ternal)g(table)0 1025 y(sho)o(wing)h(whic)o(h)h(\014les)g(m)o(ust)f(b)
+q(e)i(copied.)0 1187 y Fg(5)89 b(ndo)r(c)23 b(options)0
+1303 y Fd(ndo)q(c)14 b(o)o(v)o(erview)g(has)g(b)q(een)h(phased)g(out.)
+118 1378 y(ndo)q(c)20 b(test)h(will)e(carry)h(out)g(a)g(series)h(of)e
+(consistency)j(c)o(hec)o(ks)f(b)q(et)o(w)o(een)h(the)e(do)q(cumen)o(t)f
+(source)j(tree)f(and)0 1428 y(the)e($n)p 122 1428 V 14
+w(hlp)f(tree,)i(eliminating)15 b(\014les)j(in)g(the)h(latter)f(for)g
+(whic)o(h)g(no)f(corresp)q(onding)i(source)h(exists)e(and)g(rep)q
+(orting)0 1478 y(anomalies.)e(It)e(also)118 1552 y(ndo)q(c)h(all)f
+(compiles)g(all)f(program-in)o(terface)h(descriptions,)i(all)d(LaT)m
+(eX)i(do)q(cumen)o(ts)g(and)f(p)q(erforms)h(an)f(ndo)q(c)0
+1602 y(test.)935 2995 y(2)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/doc_release9511/doc_release9511.html b/doc_release9511/doc_release9511.html
new file mode 100644
index 0000000000000000000000000000000000000000..7efa2019eae6fbced1cd1052a081959346cdb048
--- /dev/null
+++ b/doc_release9511/doc_release9511.html
@@ -0,0 +1,58 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Changes to the <i>NEWSTAR </i> documentation system, November 1995</b> <i>by Johan Hamaker, 951012</i>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=doc_release9511.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/doc_release9511/images.pl b/doc_release9511/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/doc_release9511/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/doc_release9511/labels.pl b/doc_release9511/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..5f0326625d227e5a50b2a2a6dd2887c7830b03b7
--- /dev/null
+++ b/doc_release9511/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/doc_release9511.html"; 
+
+1;
\ No newline at end of file
diff --git a/dwarf/dwarf__ask.html b/dwarf/dwarf__ask.html
new file mode 100644
index 0000000000000000000000000000000000000000..ed3c9d29412114efba7ad4f4e0867a3ffd87ee17
--- /dev/null
+++ b/dwarf/dwarf__ask.html
@@ -0,0 +1,17 @@
+<TITLE>Description of ASK (DWARF)</TITLE>
+<H1>Program DWARF: private keyword ASK</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Character(4).<P>
+	ASK=YES directs DWARF programs to always prompt for parameters, even if <P>
+an external default has been defined (through SPECIFY or otherwise). 
+	This setting can be overridden by use of the /NOASK qualifier with the 
+EXECUTE command or with run-time parameter input. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__bell.html b/dwarf/dwarf__bell.html
new file mode 100644
index 0000000000000000000000000000000000000000..f20778621690e5ccb47cb1212de19b17e8d406c7
--- /dev/null
+++ b/dwarf/dwarf__bell.html
@@ -0,0 +1,15 @@
+<TITLE>Description of BELL (DWARF)</TITLE>
+<H1>Program DWARF: private keyword BELL</H1> 
+
+<DT><EM>Prompt:</EM> ON, OFF Terminal bell with prompts and error messages
+<DT><EM>Default:</EM> OFF.
+<DT><EM>Expected input:</EM> Character(4).<P>
+	Controls the sounding of the terminal bell with error messages and <P>
+with prompts for parameters <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__curnode.html b/dwarf/dwarf__curnode.html
new file mode 100644
index 0000000000000000000000000000000000000000..3ea9b24cb254c8647b1836b7edfb5b829fc65c1d
--- /dev/null
+++ b/dwarf/dwarf__curnode.html
@@ -0,0 +1,15 @@
+<TITLE>Description of CURNODE (DWARF)</TITLE>
+<H1>Program DWARF: private keyword CURNODE</H1> 
+
+<DT><EM>Prompt:</EM> Current node name
+<DT><EM>Default:</EM> 0.
+<DT><EM>Expected input:</EM> Character(80).<P>
+	This is the node name with respect to which relative node names, i.e. <P>
+node specifications starting with "." or "-", will be expanded <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__extendsize.html b/dwarf/dwarf__extendsize.html
new file mode 100644
index 0000000000000000000000000000000000000000..3cb45832daa6692e180e3071682d05800c6a4ba2
--- /dev/null
+++ b/dwarf/dwarf__extendsize.html
@@ -0,0 +1,16 @@
+<TITLE>Description of EXTENDSIZE (DWARF)</TITLE>
+<H1>Program DWARF: private keyword EXTENDSIZE</H1> 
+
+<DT><EM>Prompt:</EM> Default extension size in blocks for DWARF data files
+<DT><EM>Default:</EM> 64.
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000; max.value: 512.000000.<P>
+	Defines the minimum extension size to be applied by DWARF I/O routines. <P>
+An actual extension will be the maximum of this parameter and the extension 
+requested by the program. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__ibmode.html b/dwarf/dwarf__ibmode.html
new file mode 100644
index 0000000000000000000000000000000000000000..7fad9f92b5a4a5aba65d02cd7c6331f703569ec8
--- /dev/null
+++ b/dwarf/dwarf__ibmode.html
@@ -0,0 +1,15 @@
+<TITLE>Description of IBMODE (DWARF)</TITLE>
+<H1>Program DWARF: private keyword IBMODE</H1> 
+
+<DT><EM>Prompt:</EM> INTERACTIVE, BATCH, NETWORK
+<DT><EM>Default:</EM> INTERACTIVE.
+<DT><EM>Expected input:</EM> Character(11).<P>
+	This is the batch/interactive flag maintained by DWARF, It can not be <P>
+changed by the user. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__ident.html b/dwarf/dwarf__ident.html
new file mode 100644
index 0000000000000000000000000000000000000000..d777cf8b1584b1f419917c79e201d06e2ed4de3f
--- /dev/null
+++ b/dwarf/dwarf__ident.html
@@ -0,0 +1,15 @@
+<TITLE>Description of IDENT (DWARF)</TITLE>
+<H1>Program DWARF: private keyword IDENT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> XYZ.
+<DT><EM>Expected input:</EM> Character(3).<P>
+	This is the process identification used by DWARF. It can not be <P>
+changed by the user. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__iobufsize.html b/dwarf/dwarf__iobufsize.html
new file mode 100644
index 0000000000000000000000000000000000000000..da74436c55fa9aef2aec70a98fcd02842dbf284e
--- /dev/null
+++ b/dwarf/dwarf__iobufsize.html
@@ -0,0 +1,16 @@
+<TITLE>Description of IOBUFSIZE (DWARF)</TITLE>
+<H1>Program DWARF: private keyword IOBUFSIZE</H1> 
+
+<DT><EM>Prompt:</EM> Default I/O buffer size in bytes
+<DT><EM>Default:</EM> 32768.
+<DT><EM>Expected input:</EM> Integer number; min.value: 2048.000000; max.value: 32768.000000.<P>
+	This is the default size of I/O buffers to be allocated by the DWARF <P>
+bulk I/O routines. This parameter is intended primarily for adapting DWARF to 
+host systems with limited physical memory. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__logfatal.html b/dwarf/dwarf__logfatal.html
new file mode 100644
index 0000000000000000000000000000000000000000..b1b43bc6a57f27e563ae6a19ba8ea2faa7557153
--- /dev/null
+++ b/dwarf/dwarf__logfatal.html
@@ -0,0 +1,15 @@
+<TITLE>Description of LOGFATAL (DWARF)</TITLE>
+<H1>Program DWARF: private keyword LOGFATAL</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO Do you want unsuccessful program runs logged
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Character(4).<P>
+	This parameter controls the logging of program runs that terminate <P>
+with a failure status. If LOGFATAL=NO, only successfull runs will be logged. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__loglevel.html b/dwarf/dwarf__loglevel.html
new file mode 100644
index 0000000000000000000000000000000000000000..56a66d0bab8520963b85b4273bf653658a2dc09e
--- /dev/null
+++ b/dwarf/dwarf__loglevel.html
@@ -0,0 +1,18 @@
+<TITLE>Description of LOGLEVEL (DWARF)</TITLE>
+<H1>Program DWARF: private keyword LOGLEVEL</H1> 
+
+<DT><EM>Prompt:</EM> Severity threshold for logging messages
+<DT><EM>Default:</EM> 4.
+<DT><EM>Expected input:</EM> Integer number; min.value: 0.000000; max.value: 8.000000.<P>
+	This parameter defines the level below which messages will not be <P>
+logged. If LOGLEVEL=0, all messages are logged; if it is 8 you get no log at 
+all. 
+	LOGLEVEL=4 will give you all informational messages from DWARF programs 
+plus fatal error messages. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__messagedevice.html b/dwarf/dwarf__messagedevice.html
new file mode 100644
index 0000000000000000000000000000000000000000..a05613f2a4a617842562cbfb106717dc5529356e
--- /dev/null
+++ b/dwarf/dwarf__messagedevice.html
@@ -0,0 +1,15 @@
+<TITLE>Description of MESSAGEDEVICE (DWARF)</TITLE>
+<H1>Program DWARF: private keyword MESSAGEDEVICE</H1> 
+
+<DT><EM>Prompt:</EM> TERMINAL, PRINTER Device(s) for messages
+<DT><EM>Default:</EM> TERMINAL.
+<DT><EM>Expected input:</EM> Character(8), 2 values.<P>
+	Defines where messages will be shown: On the terminal and/or in a file <P>
+to be spooled automatically to the line printer <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__savelast.html b/dwarf/dwarf__savelast.html
new file mode 100644
index 0000000000000000000000000000000000000000..bc4c058c80d7ab04801d479979cd70c8a37560eb
--- /dev/null
+++ b/dwarf/dwarf__savelast.html
@@ -0,0 +1,17 @@
+<TITLE>Description of SAVELAST (DWARF)</TITLE>
+<H1>Program DWARF: private keyword SAVELAST</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Character(4).<P>
+	SAVELAST=YES directs DWARF programs to save the last value typed in <P>
+during program execution as an external default for later program runs. 
+	The setting of this paramater can be overriden by use of the 
+/[NO]SAVELAST qualifier with the EXECUTE command or with parameter input. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__stream.html b/dwarf/dwarf__stream.html
new file mode 100644
index 0000000000000000000000000000000000000000..46e3e2fb38eda2160e66425e657ccbd7c1940a57
--- /dev/null
+++ b/dwarf/dwarf__stream.html
@@ -0,0 +1,15 @@
+<TITLE>Description of STREAM (DWARF)</TITLE>
+<H1>Program DWARF: private keyword STREAM</H1> 
+
+<DT><EM>Prompt:</EM> Stream name
+<DT><EM>Default:</EM> 1.
+<DT><EM>Expected input:</EM> Character(11).<P>
+	Defines the "current stream name" to be used as default for the <P>
+stream component in program and DWARF symbol names <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__test.html b/dwarf/dwarf__test.html
new file mode 100644
index 0000000000000000000000000000000000000000..70810b00300fd5b6f9c976794c312dc84b4d29cf
--- /dev/null
+++ b/dwarf/dwarf__test.html
@@ -0,0 +1,20 @@
+<TITLE>Description of TEST (DWARF)</TITLE>
+<H1>Program DWARF: private keyword TEST</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO Set DWARF test mode
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Character(4).<P>
+	In testing mode: <P>
+		Parameters with the TEST attribute will be prompted for. 
+		The debugger will be automatically invoked at the instant an 
+error is reported. (Note that this may already happen during the execution 
+of the remainder of the SPECIFY DWARF command. In that case, just type "GO" in 
+reply to debugger prompts, and "EXIT" when the debugger reports program 
+completion.) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf/dwarf__userlevel.html b/dwarf/dwarf__userlevel.html
new file mode 100644
index 0000000000000000000000000000000000000000..b0434f1cd10c81db630aab22a513388c3db71252
--- /dev/null
+++ b/dwarf/dwarf__userlevel.html
@@ -0,0 +1,20 @@
+<TITLE>Description of USERLEVEL (DWARF)</TITLE>
+<H1>Program DWARF: private keyword USERLEVEL</H1> 
+
+<DT><EM>Prompt:</EM> BEGINNER, AVERAGE, EXPERT How do you rate yourself as a DWARF user
+<DT><EM>Default:</EM> BEGINNER.
+<DT><EM>Expected input:</EM> Character(8).<P>
+	Defines the amount of information to be given with parameter prompts: <P>
+<DT><STRONG>		EXPERT:</STRONG> Keyword name and default only 
+		AVERAGE: Same plus available options where applicable 
+		BEGINNER: Some descriptive information in addition 
+	While being prompted, you may temporarily descend to a "lower" level 
+by typing a question mark; by adding /KEEP to the "?" you may retain this lower 
+level until program exit. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../dwarf/dwarf_keys.html">List of keywords</A> for DWARF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/dwarf_keys/dwarf_keys.html b/dwarf_keys/dwarf_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..e93d200629b231ddd4cab848f02995cc57ae1a98
--- /dev/null
+++ b/dwarf_keys/dwarf_keys.html
@@ -0,0 +1,54 @@
+<TITLE>Index of private keywords for DWARF </TITLE>
+<H1>Description of keywords for program DWARF</H1>
+
+<UL>
+<LI> <A HREF="../dwarf/dwarf__stream.html">
+  STREAM</A>
+  Stream name
+<LI> <A HREF="../dwarf/dwarf__curnode.html">
+  CURNODE</A>
+  Current node name
+<LI> <A HREF="../dwarf/dwarf__ask.html">
+  ASK</A>
+  YES, NO
+<LI> <A HREF="../dwarf/dwarf__savelast.html">
+  SAVELAST</A>
+  YES, NO
+<LI> <A HREF="../dwarf/dwarf__userlevel.html">
+  USERLEVEL</A>
+  BEGINNER, AVERAGE, EXPERT How do you rate yourself as a DWARF user
+<LI> <A HREF="../dwarf/dwarf__bell.html">
+  BELL</A>
+  ON, OFF Terminal bell with prompts and error messages
+<LI> <A HREF="../dwarf/dwarf__messagedevice.html">
+  MESSAGEDEVICE</A>
+  TERMINAL, PRINTER Device(s) for messages
+<LI> <A HREF="../dwarf/dwarf__extendsize.html">
+  EXTENDSIZE</A>
+  Default extension size in blocks for DWARF data files
+<LI> <A HREF="../dwarf/dwarf__iobufsize.html">
+  IOBUFSIZE</A>
+  Default I/O buffer size in bytes
+<LI> <A HREF="../dwarf/dwarf__test.html">
+  TEST</A>
+  YES, NO Set DWARF test mode
+<LI> <A HREF="../dwarf/dwarf__loglevel.html">
+  LOGLEVEL</A>
+  Severity threshold for logging messages
+<LI> <A HREF="../dwarf/dwarf__logfatal.html">
+  LOGFATAL</A>
+  YES, NO Do you want unsuccessful program runs logged
+<LI> <A HREF="../dwarf/dwarf__ident.html">
+  IDENT</A>
+  
+<LI> <A HREF="../dwarf/dwarf__ibmode.html">
+  IBMODE</A>
+  INTERACTIVE, BATCH, NETWORK
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../dwarf_descr/dwarf_descr.html">program DWARF</A>
+</UL>
diff --git a/dwarf_private_intfc.ps b/dwarf_private_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..9ac4d1c2327e48812835311b9878aee65995486e
--- /dev/null
+++ b/dwarf_private_intfc.ps
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+A438301C80A3EA383C38184D00EA0F8611127C9116>I E
+%EndDVIPSBitmapFont
+end
+%%EndProlog
+%%BeginSetup
+%%Feature: *Resolution 300dpi
+TeXDict begin
+%%PaperSize: a4
+
+%%EndSetup
+%%Page: 1 1
+1 0 bop 118 -41 a Fe(Printout)15 b(of)g(NEWST)m(AR)g(do)n(cument)h
+(chapter)f(-)f(June)i(13,)f(1997)17 133 y Fd(The)i(generic)h(con)n
+(trol)g(parameters)f(of)f(the)i(NEWST)-6 b(AR)18 b(user)f(in)n(terface)
+0 295 y(Con)n(ten)n(ts)0 395 y Fc(1)54 b(Description)o(s)13
+b(of)i(the)g(individu)o(al)e(parameters)917 b(1)62 453
+y Fb(1.1)56 b(References)16 b(to)d(public)h(in)o(terfaces)31
+b(.)20 b(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)
+f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)71
+b(1)0 733 y Fd(1)89 b(Descriptions)23 b(of)f(the)g(indivi)q(dual)k
+(parameters)0 858 y Fa(1.1)74 b(References)17 b(to)i(public)f(in)n
+(terfaces)935 2995 y Fb(1)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/dwarf_private_intfc/dwarf_private_intfc.html b/dwarf_private_intfc/dwarf_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..9543f6a5da6d52d033da7bc257e8d4f57c68098f
--- /dev/null
+++ b/dwarf_private_intfc/dwarf_private_intfc.html
@@ -0,0 +1,68 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The generic control parameters of the NEWSTAR user interface</b>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=dwarf_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=dwarf_private_intfc.html#SECTION0002000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html3 HREF=dwarf_private_intfc.html#SECTION0002100000000000000>  <b>References to public interfaces</b></A>
+</UL>
+</UL>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/dwarf_private_intfc/images.pl b/dwarf_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/dwarf_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/dwarf_private_intfc/labels.pl b/dwarf_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..92068e573baec520285b162d8e9742543693fe5f
--- /dev/null
+++ b/dwarf_private_intfc/labels.pl
@@ -0,0 +1,8 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/dwarf_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/dwarf_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/dwarf_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/dwarfini.txt b/dwarfini.txt
new file mode 100644
index 0000000000000000000000000000000000000000..e4e1529cf57459f7cbac99b9f4458befc05653dd
--- /dev/null
+++ b/dwarfini.txt
@@ -0,0 +1,4 @@
+
+1 Type dwnews to get information about the recent changes in the DWARF system.
+
+**************************************************  16-Dec-92 WNB  ***********
diff --git a/dwarfnews.txt b/dwarfnews.txt
new file mode 100644
index 0000000000000000000000000000000000000000..ec34bde921b0c94db24c5e81d2420760cd5b9c68
--- /dev/null
+++ b/dwarfnews.txt
@@ -0,0 +1,94 @@
+1 DWARFnews
+
+
+ 911210	Some improvements have been made to DWARF.
+	The main improvement is that a program is starting faster because
+	the symbol handling software is much faster. The number of symbols
+	allowed is unlimited, but of course you should not let it grow too
+	much. The symbol files are now located in a separate subdirectory,
+	which is automatically created by .dwarflogin when it does not exist.
+	.dwarflogout saves your symbol files and deletes symbol files older
+	than 1 week.  You should therefore use
+		source $SYSDWARF/.dwarflogout    in your logout file.
+	Secondly the EXEC call is used as much as possible to start the
+	programs. This has the benefit that no shell is created to run the
+	program and that EXECUTE disappears after having started the program.
+	Thirdly some environment variables resembling the VAX logical names
+	have been defined. These are $SYSDWARF, $RUNDWARF and $LIBDWARF.
+	These variables should be used as much as possible instead of the
+	~dwarf construction, because they are more system independent.
+	At last a few minor bugs have been removed.
+
+ 910913	The following DWARF command aliases have been defined:
+	dwc	for dwclear (see 910814)
+	dwe	for dwexe (see below)
+	dwl	for dwlet (see 910814)
+	dwn	for dwnews (display this file)
+	dwr	for restore (see 910814)
+	dws	for specify
+	dwsa	for dwsave (see 910814)
+	dwv	for dwview (see 910817)
+
+	The DWARF command dwexe has been installed. It behaves roughly like
+	the EXE*CUTE command on the VAX, e.g.:
+	dwexe 'program$stream <qualifiers>'
+		runs the program in the given stream taking the qualifiers
+		into account.
+	The following qualifiers are recognized:
+	/[no]ask /[no]save /[no]test	(as on the VAX);
+	/input=<file>		lets the program read input from the file;
+	/nowait			runs the program in the background (it will
+				stop when it needs input from the terminal);
+	/batch			runs the program in the background, but lets
+				the program take its input from the null device
+				and writes the output to <prognam><stream>.log;
+	/debug			executes the program under dbx;
+	/norun			for N-type programs: runs the program in
+				specify mode: only asks for parameter input
+				and saves the answers in external defaults);
+				for other programs: only saves any ask, save
+				or test switch given (as on the VAX);
+	/nolog or /log=<value>
+	/nodatab
+	/noinfix
+	/noapply or /apply=<list>
+	/node_apply or /de_apply=<list>
+				are only recognized for N-type programs; first,
+				defaults for the corresponding program
+				parameters are specified according to the
+				qualifiers 	given.
+
+ 910817	Command dwview installed (similar to DWARF/VAX's VIEW):
+	Examples:
+	dwview
+		lists all external defaults (specified or restored)
+	dwview 'program$stream'
+		lists all program parameters and their current defaults
+		(external or PPD) in the given or current stream
+	dwview 'program /external'
+		only lists the program parameters with external defaults
+	dwview 'name_list /input=save_file'
+		lists all saved parameter defaults matching the namelist
+
+ 910814	Some more VAX/DWARF commands have been activated on the Alliant.
+	The command lines given below are meant to show all the possible
+	qualifiers; all their names can be abbreviated to a single letter.
+	The quotes suppress the interpretation of meta-characters by the shell.
+
+	dwclear 'list /exclude=list /confirm /log=long'
+		clears the listed parameter defaults (list required)
+	dwsave 'list /output=file /exclude=list /confirm /log=short'
+		saves the listed defaults in the file
+		(default: save all defaults in .dwarfsave.sav)
+	restore 'file /include=list /exclude=list /confirm /overwrite /nolog'
+		restores (all) defaults from the file
+	dwlet 'name=value /log=short'
+		defines a global symbol
+	prtunits
+		displays DWARF units and conversion factors
+
+ 910806	External defaults are no longer automatically carried over from your
+	previous session. However, you can activate this option by copying
+	~dwarf/protologout to ~/.logout. From then on, when you log out, all
+	the defaults are saved in the file ~/symbol.sav and, when you log in
+	again, DWARF's login procedure will restore them.
diff --git a/dwcalc.txt b/dwcalc.txt
new file mode 100644
index 0000000000000000000000000000000000000000..9dccc78319cb0089a052f3a7a0ea7d481154b43c
--- /dev/null
+++ b/dwcalc.txt
@@ -0,0 +1,276 @@
+The desk-calcutor program DWCALC
+--------------------------------
+
+HISTORY: 
+	 This file was originally written as a VAX/VMS HELP file. The program
+dwcalc was part of the DWARF infrastructure which has been merged into Newstar.
+This file has been taken over essentially as it was found.
+
+	8-oct-86        Ger van Diepen
+	JPH 940718      Update for Newstar
+	JPH 940918      Formatting for line-breaking algorithm
+
+
+DWCALC 
+======
+
+The program DWCALC is a handy desk-calculator, allowing the use of expressions
+(with units), symbols and formulae.  It is derived from the Dutch image
+processing system DWARF.  (Dwingeloo Westerbork Astronomical Reduction
+Facility). 
+
+ The program is started by the command 'dwcalc'.  Qualifiers can be used to
+control the program. If they are given  at the 'dwcalc' command-line, they
+serve as a global qualifier.  Global qualifiers can be overridden for each
+individual expression-line  by ending the line with the qualifiers, preceeded
+by at least one space  (to distinguish it from the division operator).
+
+ The input expressions are read from stdin.  The results are listed on stdout.
+Optionally (part of) input and output can be logged.  All input is converted to
+uppercase, therefore input is NOT case-sensitive.
+
+
+EXPRESSIONS 
+===========
+ After having started the program, the program asks you for an expression.  By
+giving a null-answer the program will be stopped.  Typing a question mark
+starts a help session.  Typing UNIT=? will show you the available units on
+printer or terminal.
+
+Expressions have the normal arithmetical format, using +,-,*,/,**  and
+parentheses. Blanks and unary signs are allowed.  However, note that / cannot
+be preceeded by a blank to distinguish  it from the qualifier-indicator.  The
+relational operators .NOT.,.EQ.,.NE.,.GT.,.GE.,.LE. and .LT.  are also allowed.
+ Also available are:    - some built-in functions (goniometric, etc.)    - unit
+specification and conversion    - special format for time or positions (using
+colons)    - symbol definition and substitution
+
+Integer numbers can be specified in octal or hexadecimal  format (use %O, %X,
+resp.). 
+
+
+FUNCTIONS 
+=========
+
+The following functions (similar to Fortran) can be used in expressions:
+
+	MIN     MAX     (1-10 arguments)
+	SIN     COS     TAN
+	ASIN    ACOS    ATAN     ATAN2
+	ABS     EXP     LOG     LOG10    SQRT
+	TRUNC   ROUND   MOD     SIGN
+
+Default unit for goniometric function is degrees, which can be overridden via
+the /UNIT-qualifier or by giving the unit in the  expression.
+
+The result of SIGN is:
+	-1  for negative values
+	 0  for zero
+	 1  for positive values
+
+Note that conversion to integer format implies rounding.
+
+
+UNITS 
+=====
+
+CALCULATE is able of converting from one unit to another.  It converts the
+units given in the expression to the unit given by  the /UNIT-qualifier. The
+units must belong to the same group (so  conversion from SEC to KM is
+impossible). 
+
+A unit can be given at several places:
+
+	- after a number           e.g. 10DEG
+	- after a subexpression    e.g. (10+3)deg
+	- after a symbol           e.g. PI RAD
+
+ Note that in the last case the blank is significant, else it is  optional.
+
+
+TIME_POSITION 
+-------------
+
+Times and positions can be given in HH:MM:SS (or DD:MM:SS) format using colons
+as separators. A unit may follow the value. Each part can be a floating number,
+which may exceed 60.
+
+The output can also be listed in that format by giving  /UNIT=HMS or /UNIT=DMS.
+
+This sexagesimal format allows for easy addition, subtraction and  conversion
+of times and positions.
+
+
+SYMBOLS 
+=======
+
+Symbols are very useful for storing results and for handling formulae. Both
+symbol substitution and definition is possible in DWCALC. DWCALC will always
+define global symbols. It is also possible to use predefined local or global
+symbols,  either numeric or alphanumeric.
+
+By defining a formula as a symbol, it is very easy to calculate the result of
+the formula for several values of its parameters. E.g.
+
+	$ VOLUME = "4/3*pi*r**3"
+	$ CALC
+	   Expression: r=3
+	   Expression: volume
+	   Expression: r=10
+	   Expression: volume
+
+
+DEFINITION 
+----------
+
+A symbol can be defined by using the constructS:
+
+	symbol_name = expression
+	symbol_name = "expression"
+
+In the first case the expression is evaluated and the result will be assigned
+to the symbol. In the second case the expression-text is assigned to the
+symbol, which is useful for defining formulae.
+
+Note that DCL uses the same procedure.
+
+SUBSTITUTION 
+------------
+
+Symbols can be substituted in an expression by giving its name enclosed in
+apostrophes or giving its name without  apostrophes.
+
+In the former case its value is substituted literally.  In the latter case its
+value is treated as a subexpression. E.g. if I=3+4 then
+
+	3*'i'   results in 3*3+4   = 13 and
+	3*i     results in 3*(3+4) = 21
+
+Note that nested substitution is possible. Circular substitution is detected by
+allowing a maximum of 25 substitutions.
+
+
+Examples 
+========
+
+Convert miles to kilometers
+
+	 $ dwcalc          10mile /unit=km
+
+If a whole series must be done it would be better to do:
+
+	 $ dwcalc/unit=km
+	    10mile
+	    8 mile
+	    (1.25+3.48)mile
+
+Convert right ascension from HH:MM:SS to degrees.
+
+	 $ dwcalc/unit=deg 9:23:48.329 hms
+
+Convert a time to seconds
+
+	 $ dwcalc/unit=sec 9:23:48.329 hr
+
+Do some time calculation
+
+	 $ dwcalc/unit=hms 10:34:48 + 2::45 - :34:56.89
+
+Calculate an expression and define the symbol ABC The result must be an integer
+
+	 $ dwcalc ABC = (2.34 * pi)+8*-cos(135+pi*28) /unit=deg
+
+Define a formula and calculate it for several parameters
+
+	 $ dwcalc
+	    VOLUME = "4/3*PI*R**3"
+	    R=2
+	    VOLUME
+	    R=10
+	    VOLUME
+
+Convert from hexadecimal to decimal
+
+	  %x1a2f
+
+Convert from decimal to hexadecimal
+
+	  2546 /rad=x
+
+/UNIT 
+=====
+
+This qualifier defines the default unit for the given values  and the unit in
+which the result will be expressed.  In this way it can be used for converting
+rom one unit to another.  Note however that conversion between different groups
+of units  is not allowed (e.g. seconds to meters is illegal).
+
+From DCL the available units can be shown via the command PRTUNIT.  From
+CALCULATE they can be shown via UNIT=?.
+
+Default is no units.
+
+
+/RADIX 
+======
+
+This qualifier defines in which radix the output will be listed. Possible
+values are:
+
+     D   decimal
+     O   octal
+     X   hexadecimal
+
+The default is D. O and X force TYPE=J if type is non-integer.
+
+
+/TYPE 
+=====
+
+This qualifier defines in which format the output will be listed. Note that all
+calculations are done in double precision and that  the program tests on
+integer overflow before conversion to an  integer format.  Possible values are:
+
+     B   signed byte
+     I   signed word       (integer*2)
+     J   signed longword   (integer*4)
+     L   logical
+     R   single precision  (real*4)
+     D   double precision  (real*8)
+
+The default is D.
+
+
+/STREAM 
+=======
+
+This qualifier is special to DWARF. It controls the stream of the application
+symbols. The stream-name will be inserted in a symbol-name, if that symbol-name
+ has the format "image_keyword".
+
+Default is no stream.
+
+
+/LIST 
+=====
+
+This qualifier controls if the results will be listed. Normally you will always
+list the result, but in command-files  it can be useful to negate this
+qualifier (i.e. /NOLIST).
+
+Default is list.
+
+
+/LOG 
+====
+
+This qualifier controls if the expressions and results will be written in the
+log-file CALCULATE.LOG (in the default directory). This log-file is written in
+such a way that it can be executed as a DCL command-file or can be used as
+input for the ARCHIVE-programs. This means that most lines will be flagged with
+an exclamation mark  (indicating comments), but symbol definitions are valid
+commands,  which can be executed. In this way users can calculate complex
+expressions and define the  results as symbols in a subprocess and execute the
+log-file in the  main process in order to obtain the results.
+
+Default is no logging.
diff --git a/elsewhere_inst_maint.html b/elsewhere_inst_maint.html
new file mode 100644
index 0000000000000000000000000000000000000000..f6766aaf37e8481a0d2db99fb9f2171b2f5b3473
--- /dev/null
+++ b/elsewhere_inst_maint.html
@@ -0,0 +1,423 @@
+<TITLE>Installation and maintenance of Newstar outside NFRA</TITLE>
+
+<STRONG>Subject:</STRONG> Installation and maintenance of Newstar outside NFRA
+<BR><STRONG>Author:</STRONG>  Marco de Vos (CMV), Henk Vosmeijer (HjV)
+<BR><STRONG>To:</STRONG>      Friends of Newstar
+<P><STRONG>Date:</STRONG>     24/11/94
+<P>
+<EM>Revision history</EM>
+<UL>
+<LI>18/06/96 - add Solaris as available machine, correct Building Newstar part
+<LI>24/11/94 - add questionnaire new Newstar sites, make html
+<LI>16/02/94 - first release
+<LI>04/03/94 - prerelease 
+</UL>
+
+<PRE></PRE>
+<H1>Installation and maintenance of Newstar outside NFRA</H1>
+<PRE></PRE>
+
+<H2>1. About Newstar and this document</H2>
+
+Newstar is the reduction package for WSRT data. 
+<BR>It makes optimal use of the specific properties of the WSRT. 
+
+<P>You can use it to:
+<UL>
+<LI>read, display, calibrate and analyse WSRT data.
+<LI>flag bad data interactively or in semi-automatic mode. 
+<LI>extract and improve parametrised models from the data.
+<LI>make and manipulate calibrated maps.
+<LI>save raw or calibrated data as UVFITS tapes or files.
+<LI>save maps as FITS tapes or files.
+</UL>
+
+General information on Newstar operations can be found in the Newstar
+Documentation. This documentation is available on-line. If you are 
+familiar with World Wide Web browsers like XMosaic, you can get at the
+documentation by opening <A HREF=http://www.astron.nl/newstar/hlp/homepage.html>http://www.astron.nl/newstar/hlp/homepage.html</A>
+<BR>Otherwise, please send an eMail to <EM>newstar@astron.nl</EM> for assistance.
+<P>
+This document is concerned with installation and maintenance of Newstar
+at institutes other than the NFRA. It descibes our export policy, the
+procedure for first time installation and the procedures for local 
+maintenance.
+<PRE></PRE>
+
+<H2>2. Export policy</H2>
+
+The master copy of the Newstar software is maintained at the NFRA in
+Dwingeloo. Newstar is available for end-users on the following machines:
+<UL>
+<LI>hp =  HP Workstations  (9000 series, others at request)   
+<LI>sw =  Sun Workstations (sun4)
+<LI>dw =  DEC Workstations (DEC3100)
+<LI>da =  DEC Alpha/OSF1
+<LI>so =  Sun Solaris
+</UL>
+    
+(the two-letter codes will be used in the remainder of this document)
+<P>
+This list may be extended with other Unix systems in future. Newstar 
+can also be run on Convex (cv) systems, but this is not officially 
+supported by the NFRA.
+<P>
+If you want to install Newstar on your institute, the Newstar group 
+will assist with the first time installation of the package. We expect 
+you to assign a local "Friend of Newstar" who will take care of local
+maintenance, using the procedures described in this document. In case 
+of problems, you can of course contact the Newstar group, who will do
+it's best to solve things on a short notice. 
+<P>
+The Newstar maintenance at the radio-observatory in Westerbork is 
+updated by the Newstar group at a weekly basis.
+<PRE></PRE>
+
+<H2>3. First time installation</H2>
+
+It should be noted that the Newstar group is available for assistance
+with the first time installation of Newstar. Also we can implement such
+things as changes in printers and tapeunits. However, this section 
+describes the installation process in full detail.
+<P>
+<H3>3A. Before installation</H3>
+
+Before you can install Newstar, you have to sort out the following 
+things:
+<UL> 
+<LI>Set up an account for Newstar, or at least a directory where 
+Newstar can be installed (this directory will be refered to as 
+the "Newstar root-directory" in the remainder of this document). 
+<P>
+At present, disk-space requirements are:
+<UL>
+<LI>Sources:      15 ... 27 MByte 
+<LI>Libraries:    20 ... 25 MByte (for each architecture)
+<LI>Executables:  60 ... 90 MByte (for each architecture)
+</UL>
+<BR>The amount of diskspace varies per architecture.
+<BR>Sources, libraries and executables may reside at separate filesystems.
+<P>
+<LI>Find out the commands to send ASCII and postscript files to 
+your local printer(s).
+<P>
+<LI>Find out the names of the tapeunits connected to your hosts
+</UL>
+You should fill out the form in <STRONG>Appendix A</STRONG> and eMail
+it to <EM>newstar@astron.nl</EM> (from this point on the Newstar group
+can take care of installation).
+
+
+<H3>3B. Installing the Newstar sources</H3>
+
+You should have tar-archives  nstar_src.tar.Z   and  nstar_src_aa.tar
+(where aa is the abbreviation of the architecture on which you want to 
+use Newstar, you may need several nstar_src_aa.tar files) from tape or 
+from anonymous ftp to  ftp.astron.nl (directory newstar). 
+<BR>To unpack this archive, use the following commands:
+<PRE>
+>>>    cd "Newstar root-directory"
+>>>    mkdir src
+>>>    cd src
+>>>    uncompress [directory_with_archive/]nstar_src.tar.Z
+>>>    tar xvf    [directory_with_archive/]nstar_src.tar
+>>>    tar xvf    [directory_with_archive/]nstar_src_aa.tar
+</PRE>
+
+<H3>3C. Adapting to your local situation</H3>
+
+Assign an abbreviated name for your institute (up to 5 characters). This 
+name will be refered to as "xxxx" in the remainder of this document.
+<P>
+Your local situation will be reflected in the following files, all in 
+directory  "Newstar root-directory"/src/sys
+<PRE>
+newstar_xxxx.csh   Directory structure, tape-units, some details
+wngfex_xxxx.csh    Commands for printing
+i_aaxxxx.csh       Fine-tuning for compilation on architecture "aa"
+</PRE>
+In general, the Newstar group will create these files based on information
+supplied by you. In case you want to create the files yourself, please use
+the versions for the nfra (newstar_nfra.csh etc.) as a template, since 
+they are extensively documented.
+<P>
+In newstar_xxxx.csh you should define at least the following:
+<OL>
+<LI>The Newstar rootdirectory
+<BR><TT>(setenv n_root "Newstar root-directory")</TT>
+<P>
+<LI>The Newstar site
+<BR><TT>(setenv n_site xxxx)</TT>
+<P>
+<LI>The architectures you want to install Newstar for (we distribute 
+some precompiled binaries and libraries for which you need only the 
+versions specified here, these are in fact in nstar_src_aa.tar)   
+<BR><TT>(setenv n_install hp/sw)</TT>
+<P>
+<LI>The hosts on which Newstar has to be compiled (just one host per 
+architecture please...)
+<BR><TT>(setenv n_hosts   host1,host2)</TT>
+<P>
+The order in n_install and n_hosts is arbitrary, but you best keep it
+the same in both variables for your own convenience.
+<P>
+<LI>Definition of tape-units
+<BR><TT>(setenv MAG4 /dev/rmt/0mn)</TT>
+<P>
+<LI>The location of the executable files and libraries if they 
+should not reside on the same filesystem as the sources. 
+You should create those directories yourself. If you do not 
+specify directories here, they will be created automatically.
+</OL>
+If you create any files yourself, we would like to receive a copy of them.
+The files will then be included in the Newstar master.
+
+
+<H3>3D. Building Newstar</H3>
+
+If you want to make an executable installation for architecture aa, login 
+on a host of that architecture and initialise the Newstar environment:
+<PRE>
+>>>    source "Newstar root-directory"/src/sys/newstar_xxxx.csh
+</PRE>
+You may have received archives nstar_exe_aa.tar or nstar_lib_aa.tar.
+If aa matches the name of your architecture, you may just untar these files
+in the appropriate directories to get a working system:
+<PRE>
+>>>    nup quit
+>>>    cd $n_lib
+>>>    uncompress [directory_with_archive/]nstar_lib_aa.tar.Z
+>>>    tar xvf    [directory with_archive]/nstar_lib_aa.tar
+>>>    uncompress [directory_with_archive/]nstar_lib_inc.tar.Z
+>>>    tar xvf    [directory with_archive]/nstar_lib_inc.tar
+>>>    cd $n_exe
+>>>    uncompress [directory_with_archive/]nstar_exe_aa.tar.Z
+>>>    tar xvf    [directory_with_archive/]nstar_exe_aa.tar
+</PRE>
+If you need to build Newstar from scratch, use the following commands:
+<PRE>
+>>>    nup build -u wntinc            (will give 9 errors for dsc-files which could not be 
+				       translated because wntinc does not yet exist.)
+>>>    nup build -u -t:exe wntinc
+>>>    nup build -u all
+</PRE>
+Logs of all transactions and errors are kept in $n_src/updyymmddaa[i].log
+where i is an index (e.g. upd930623sw.log, upd930623sw1.log).
+<P>
+If something goes wrong during the installation, the log-files will be sent
+to the Newstar group by eMail. This assumes you have the  elm  mailer 
+running at your institute. If you do not have it, you should supply an
+alias to e.g. mail or mailx in newstar_xxxx.csh 
+(add a line like alias elm 'mail -s "\!1" \!2 ')
+<PRE></PRE>
+
+<H2>4. Using Newstar, revisions and releases</H2>
+
+If someone wants to run Newstar programs, the Newstar environment should
+be initialised first:
+<PRE>
+>>>    source "Newstar root-directory"/src/sys/newstar_xxxx.csh
+</PRE>
+This can be safely done in a .cshrc or .login file.
+<P>
+You can now display the version of Newstar you are currently using:
+<PRE>
+>>>    nnews
+</PRE>
+This will display the version number first, followed by a list of 
+recent changes. The version number consists of a release number followed
+by a dot and a revision number. 
+<PRE>
+>>>    dwe nscan
+</PRE>
+Programs are started by typing dwe (or exe) followed by the name of the
+program. This will display a line like "NSCAN$1 (v4.21) started ...".
+The version number can be lower than the version displayed by nnews, since
+a revision may concern only some programs. A full revision history with 
+the revisions for every program can be found in the on-line documentation
+(select "Revision history" from the Newstar home page presented by nhyper). 
+<P>
+A revision of Newstar is a series of minor changes that do not affect 
+the overall operation of Newstar. Revisions are typically bug repairs,
+small additions to the functionality of a program etc. They do not affect
+keyword syntax and fileformats. 
+<P>
+A release of Newstar is issued when any of the following occured:
+<OL>
+<LI>A change of fileformats (so you will have to use the 
+NVS "New Version" option in some programs)
+<LI>A change in keyword syntax (so you will have to type different 
+things or change batch files in some cases)
+<LI>Addition of a new program, or a full rewrite of an existing one.
+</OL>
+<PRE></PRE>
+
+<H2>5. Keeping your installation up to date</H2>
+
+In the following we assume that the Newstar environment has been initialised.
+<P>
+If we modify the Newstar master at NFRA, all Friends of Newstar that we
+know of will receive an eMail describing the changes. This message will
+also contain instructions how to upgrade your installation. 
+<P>
+In most cases, upgrading is done through a single command:
+<PRE>
+>>>    nup update
+</PRE>
+This in fact causes the following commands to be executed, which you may
+also execute by hand:
+<PRE>
+  >>>    cd $n_import
+</PRE>
+The default directory is set to $n_import, which is the proper place to
+receive new files. This keeps your current sources intact.
+<PRE>
+  >>>    nup retrieve all
+</PRE>
+This will make a fresh version of the file $n_src/sys/database.idx, which
+gives a full description of your current installation.
+Than it will retrieve the version of database.idx from the NFRA for 
+comparison. Any files that need to be updated are retrieved in $n_import.
+The list of files retrieved is in file  retrieved.grp.
+<PRE>
+  >>>    nup build -Update -T:^exe retrieved.grp
+</PRE>
+This will build all files just retrieved, and any files dependent on them.
+No executables will be built, this will be done after the library check.
+<PRE>
+  >>>    nup clear -NConfirm
+</PRE>
+This will throw away any source files in the master system that are no 
+longer needed.
+<PRE>
+  >>>    nup check l
+</PRE>
+This will check your libraries. Experience shows that escpecially on HP
+workstations libraries tend to get cluttered. This will be found by the
+library check. If necessary, an additional build command will be scheduled
+to rebuilt modules. Objects for which no source is present are removed 
+from the libraries. Duplicate entries are both removed and replaced by 
+a fresh entry. Out-of-date entries are updated.
+<PRE>
+  >>>    nup check e -Update
+</PRE>
+This will check your executables. Executables that do not yet exist 
+or are out-of-date with respect to the NFRA are rebuilt. Note that usually
+not all versions need to be rebuilt for a new revision. Thus some programs
+may show a lower version than the version shown by nnews.
+<PRE>
+  >>>    rsh HOST '( source $n_src/sys/newstar_xxxx.csh; nup update rsh)
+</PRE>
+If $n_hosts (as defined in newstar_xxxx.csh) contains more hosts, the above
+command will be issued for each of them. This will carry out the build 
+and check commands listed above, but not the retrieve.
+<P>
+The proceedings of the update command will dump a lot of output on your
+screen, which is also stored in logfiles $n_src/updyymmdd[i].log (see 
+above). You may want to redirect the output to a file or /dev/null.
+If any errors occur, the log-file will be sent to the Newstar group by eMail.
+<P>
+<P>
+The nup command has many more uses than the ones described above. Most of
+them should not be relevant to you, since they are related to partial
+rebuilds, making backups etc. In case you are interested though, you can
+get more information through the command
+<PRE>
+>>>    nup help -help
+
+</PRE>
+<HR>
+<H2>Appendix 1: Questionnaire new Newstar sites</H2>
+
+Provide the following information, and send it to <EM>newstar@astron.nl</EM>
+<OL>
+
+<H3><LI>Site:</H3>
+<OL>
+<LI>Institute: 
+<P>
+<LI>Abbreviated institute name (up to 5 char):
+<P>
+<LI>Address:   
+<PRE>
+
+</PRE>
+<P>
+<LI>Friend of newstar: 
+<P>
+<LI>eMail address:  
+<P>
+<LI>ftp node(s):    
+<P>
+<LI>Phone:
+<PRE></PRE>
+</OL>
+
+<H3><LI>Platform:</H3>
+<OL>
+<LI>Platform(s) and their hostname(s) on which Newstar should run: 
+<OL>
+<LI>Convex (cv)
+<LI>DEC Alpha/OSF1 (da)
+<LI>DECstation (dw)
+<LI>HP workstation (hp)
+<LI>SUN (sw)
+</OL>
+If not in list contact to <EM>newstar@astron.nl</EM> for possible inclusion of
+your platform.
+<P>
+<LI>Do platforms have a common NFS on which to place sources? 
+<OL>
+<LI>Yes
+<LI>No
+</OL>
+(only if more than one platform requested at 2.1)
+<P>
+<LI>Root directory for Newstar: 
+<BR>(e.g. /usr/src/newstar )
+<PRE></PRE>
+<LI>If object-libraries should be placed on a different file system,
+specify here:
+<PRE></PRE>
+<LI>Idem executables: 
+<PRE></PRE>
+<LI>Could you provide an account on your platform(s) in which we can
+login to do some remote checks can be made? 
+<OL>
+<LI>Yes
+<LI>No
+</OL>
+If <STRONG>YES</STRONG>, please specify it: 
+<PRE></PRE>
+</OL>
+
+<H3><LI>Software:</H3>
+<OL>
+<LI>Are you using the standard f77, cc and ld provided with your system? 
+<OL>
+<LI>Yes
+<LI>No
+</OL>
+If not, provide details on how to call them, and the switches provided)
+<PRE></PRE>
+<LI>What is your standard command to print 132 wide ASCII files? 
+<PRE></PRE>
+<LI>What is your standard command to plot A4-format PostScript files? 
+<PRE></PRE>
+<LI>What is your standard command to plot A3-format PostScript files? 
+<PRE></PRE>
+<LI>Which other plotters would you like to use? 
+<BR>(contact <EM>newstar@astron.nl</EM> to see if support is possible)
+<PRE></PRE>
+</OL>
+
+<H3><LI>Input/Output medium:</H3>
+<OL>
+<LI>Specify the device-names of the available mediums for reading/writing data?
+<PRE></PRE>
+<LI>Specify on which medium you want to receive Newstar if you cannot 
+support ftp: 
+<BR>(9track/density, Exabyte, DAT, ...)
+<PRE></PRE>
+</OL>
+</OL>
diff --git a/elsewhere_inst_maint/elsewhere_inst_maint.html b/elsewhere_inst_maint/elsewhere_inst_maint.html
new file mode 100644
index 0000000000000000000000000000000000000000..4446d669b26f580f68c401b9625edd607b6aa253
--- /dev/null
+++ b/elsewhere_inst_maint/elsewhere_inst_maint.html
@@ -0,0 +1,423 @@
+<TITLE>Installation and maintenance of Newstar outside NFRA</TITLE>
+
+<STRONG>Subject:</STRONG> Installation and maintenance of Newstar outside NFRA
+<BR><STRONG>Author:</STRONG>  Marco de Vos (CMV), Henk Vosmeijer (HjV)
+<BR><STRONG>To:</STRONG>      Friends of Newstar
+<P><STRONG>Date:</STRONG>     24/11/94
+<P>
+<EM>Revision history</EM>
+<UL>
+<LI>18/06/96 - add Solaris as available machine, correct Building Newstar part
+<LI>24/11/94 - add questionnaire new Newstar sites, make html
+<LI>16/02/94 - first release
+<LI>04/03/94 - prerelease 
+</UL>
+
+<PRE></PRE>
+<H1>Installation and maintenance of Newstar outside NFRA</H1>
+<PRE></PRE>
+
+<H2>1. About Newstar and this document</H2>
+
+Newstar is the reduction package for WSRT data. 
+<BR>It makes optimal use of the specific properties of the WSRT. 
+
+<P>You can use it to:
+<UL>
+<LI>read, display, calibrate and analyse WSRT data.
+<LI>flag bad data interactively or in semi-automatic mode. 
+<LI>extract and improve parametrised models from the data.
+<LI>make and manipulate calibrated maps.
+<LI>save raw or calibrated data as UVFITS tapes or files.
+<LI>save maps as FITS tapes or files.
+</UL>
+
+General information on Newstar operations can be found in the Newstar
+Documentation. This documentation is available on-line. If you are 
+familiar with World Wide Web browsers like XMosaic, you can get at the
+documentation by opening <A HREF=http://www.nfra.nl/newstar/hlp/homepage.html>http://www.nfra.nl/newstar/hlp/homepage.html</A>
+<BR>Otherwise, please send an eMail to <EM>newstar@nfra.nl</EM> for assistance.
+<P>
+This document is concerned with installation and maintenance of Newstar
+at institutes other than the NFRA. It descibes our export policy, the
+procedure for first time installation and the procedures for local 
+maintenance.
+<PRE></PRE>
+
+<H2>2. Export policy</H2>
+
+The master copy of the Newstar software is maintained at the NFRA in
+Dwingeloo. Newstar is available for end-users on the following machines:
+<UL>
+<LI>hp =  HP Workstations  (9000 series, others at request)   
+<LI>sw =  Sun Workstations (sun4)
+<LI>dw =  DEC Workstations (DEC3100)
+<LI>da =  DEC Alpha/OSF1
+<LI>so =  Sun Solaris
+</UL>
+    
+(the two-letter codes will be used in the remainder of this document)
+<P>
+This list may be extended with other Unix systems in future. Newstar 
+can also be run on Convex (cv) systems, but this is not officially 
+supported by the NFRA.
+<P>
+If you want to install Newstar on your institute, the Newstar group 
+will assist with the first time installation of the package. We expect 
+you to assign a local "Friend of Newstar" who will take care of local
+maintenance, using the procedures described in this document. In case 
+of problems, you can of course contact the Newstar group, who will do
+it's best to solve things on a short notice. 
+<P>
+The Newstar maintenance at the radio-observatory in Westerbork is 
+updated by the Newstar group at a weekly basis.
+<PRE></PRE>
+
+<H2>3. First time installation</H2>
+
+It should be noted that the Newstar group is available for assistance
+with the first time installation of Newstar. Also we can implement such
+things as changes in printers and tapeunits. However, this section 
+describes the installation process in full detail.
+<P>
+<H3>3A. Before installation</H3>
+
+Before you can install Newstar, you have to sort out the following 
+things:
+<UL> 
+<LI>Set up an account for Newstar, or at least a directory where 
+Newstar can be installed (this directory will be refered to as 
+the "Newstar root-directory" in the remainder of this document). 
+<P>
+At present, disk-space requirements are:
+<UL>
+<LI>Sources:      15 ... 27 MByte 
+<LI>Libraries:    20 ... 25 MByte (for each architecture)
+<LI>Executables:  60 ... 90 MByte (for each architecture)
+</UL>
+<BR>The amount of diskspace varies per architecture.
+<BR>Sources, libraries and executables may reside at separate filesystems.
+<P>
+<LI>Find out the commands to send ASCII and postscript files to 
+your local printer(s).
+<P>
+<LI>Find out the names of the tapeunits connected to your hosts
+</UL>
+You should fill out the form in <STRONG>Appendix A</STRONG> and eMail
+it to <EM>newstar@nfra.nl</EM> (from this point on the Newstar group
+can take care of installation).
+
+
+<H3>3B. Installing the Newstar sources</H3>
+
+You should have tar-archives  nstar_src.tar.Z   and  nstar_src_aa.tar
+(where aa is the abbreviation of the architecture on which you want to 
+use Newstar, you may need several nstar_src_aa.tar files) from tape or 
+from anonymous ftp to  ftp.nfra.nl (directory newstar). 
+<BR>To unpack this archive, use the following commands:
+<PRE>
+>>>    cd "Newstar root-directory"
+>>>    mkdir src
+>>>    cd src
+>>>    uncompress [directory_with_archive/]nstar_src.tar.Z
+>>>    tar xvf    [directory_with_archive/]nstar_src.tar
+>>>    tar xvf    [directory_with_archive/]nstar_src_aa.tar
+</PRE>
+
+<H3>3C. Adapting to your local situation</H3>
+
+Assign an abbreviated name for your institute (up to 5 characters). This 
+name will be refered to as "xxxx" in the remainder of this document.
+<P>
+Your local situation will be reflected in the following files, all in 
+directory  "Newstar root-directory"/src/sys
+<PRE>
+newstar_xxxx.csh   Directory structure, tape-units, some details
+wngfex_xxxx.csh    Commands for printing
+i_aaxxxx.csh       Fine-tuning for compilation on architecture "aa"
+</PRE>
+In general, the Newstar group will create these files based on information
+supplied by you. In case you want to create the files yourself, please use
+the versions for the nfra (newstar_nfra.csh etc.) as a template, since 
+they are extensively documented.
+<P>
+In newstar_xxxx.csh you should define at least the following:
+<OL>
+<LI>The Newstar rootdirectory
+<BR><TT>(setenv n_root "Newstar root-directory")</TT>
+<P>
+<LI>The Newstar site
+<BR><TT>(setenv n_site xxxx)</TT>
+<P>
+<LI>The architectures you want to install Newstar for (we distribute 
+some precompiled binaries and libraries for which you need only the 
+versions specified here, these are in fact in nstar_src_aa.tar)   
+<BR><TT>(setenv n_install hp/sw)</TT>
+<P>
+<LI>The hosts on which Newstar has to be compiled (just one host per 
+architecture please...)
+<BR><TT>(setenv n_hosts   host1,host2)</TT>
+<P>
+The order in n_install and n_hosts is arbitrary, but you best keep it
+the same in both variables for your own convenience.
+<P>
+<LI>Definition of tape-units
+<BR><TT>(setenv MAG4 /dev/rmt/0mn)</TT>
+<P>
+<LI>The location of the executable files and libraries if they 
+should not reside on the same filesystem as the sources. 
+You should create those directories yourself. If you do not 
+specify directories here, they will be created automatically.
+</OL>
+If you create any files yourself, we would like to receive a copy of them.
+The files will then be included in the Newstar master.
+
+
+<H3>3D. Building Newstar</H3>
+
+If you want to make an executable installation for architecture aa, login 
+on a host of that architecture and initialise the Newstar environment:
+<PRE>
+>>>    source "Newstar root-directory"/src/sys/newstar_xxxx.csh
+</PRE>
+You may have received archives nstar_exe_aa.tar or nstar_lib_aa.tar.
+If aa matches the name of your architecture, you may just untar these files
+in the appropriate directories to get a working system:
+<PRE>
+>>>    nup quit
+>>>    cd $n_lib
+>>>    uncompress [directory_with_archive/]nstar_lib_aa.tar.Z
+>>>    tar xvf    [directory with_archive]/nstar_lib_aa.tar
+>>>    uncompress [directory_with_archive/]nstar_lib_inc.tar.Z
+>>>    tar xvf    [directory with_archive]/nstar_lib_inc.tar
+>>>    cd $n_exe
+>>>    uncompress [directory_with_archive/]nstar_exe_aa.tar.Z
+>>>    tar xvf    [directory_with_archive/]nstar_exe_aa.tar
+</PRE>
+If you need to build Newstar from scratch, use the following commands:
+<PRE>
+>>>    nup build -u wntinc            (will give 9 errors for dsc-files which could not be 
+				       translated because wntinc does not yet exist.)
+>>>    nup build -u -t:exe wntinc
+>>>    nup build -u all
+</PRE>
+Logs of all transactions and errors are kept in $n_src/updyymmddaa[i].log
+where i is an index (e.g. upd930623sw.log, upd930623sw1.log).
+<P>
+If something goes wrong during the installation, the log-files will be sent
+to the Newstar group by eMail. This assumes you have the  elm  mailer 
+running at your institute. If you do not have it, you should supply an
+alias to e.g. mail or mailx in newstar_xxxx.csh 
+(add a line like alias elm 'mail -s "\!1" \!2 ')
+<PRE></PRE>
+
+<H2>4. Using Newstar, revisions and releases</H2>
+
+If someone wants to run Newstar programs, the Newstar environment should
+be initialised first:
+<PRE>
+>>>    source "Newstar root-directory"/src/sys/newstar_xxxx.csh
+</PRE>
+This can be safely done in a .cshrc or .login file.
+<P>
+You can now display the version of Newstar you are currently using:
+<PRE>
+>>>    nnews
+</PRE>
+This will display the version number first, followed by a list of 
+recent changes. The version number consists of a release number followed
+by a dot and a revision number. 
+<PRE>
+>>>    dwe nscan
+</PRE>
+Programs are started by typing dwe (or exe) followed by the name of the
+program. This will display a line like "NSCAN$1 (v4.21) started ...".
+The version number can be lower than the version displayed by nnews, since
+a revision may concern only some programs. A full revision history with 
+the revisions for every program can be found in the on-line documentation
+(select "Revision history" from the Newstar home page presented by nhyper). 
+<P>
+A revision of Newstar is a series of minor changes that do not affect 
+the overall operation of Newstar. Revisions are typically bug repairs,
+small additions to the functionality of a program etc. They do not affect
+keyword syntax and fileformats. 
+<P>
+A release of Newstar is issued when any of the following occured:
+<OL>
+<LI>A change of fileformats (so you will have to use the 
+NVS "New Version" option in some programs)
+<LI>A change in keyword syntax (so you will have to type different 
+things or change batch files in some cases)
+<LI>Addition of a new program, or a full rewrite of an existing one.
+</OL>
+<PRE></PRE>
+
+<H2>5. Keeping your installation up to date</H2>
+
+In the following we assume that the Newstar environment has been initialised.
+<P>
+If we modify the Newstar master at NFRA, all Friends of Newstar that we
+know of will receive an eMail describing the changes. This message will
+also contain instructions how to upgrade your installation. 
+<P>
+In most cases, upgrading is done through a single command:
+<PRE>
+>>>    nup update
+</PRE>
+This in fact causes the following commands to be executed, which you may
+also execute by hand:
+<PRE>
+  >>>    cd $n_import
+</PRE>
+The default directory is set to $n_import, which is the proper place to
+receive new files. This keeps your current sources intact.
+<PRE>
+  >>>    nup retrieve all
+</PRE>
+This will make a fresh version of the file $n_src/sys/database.idx, which
+gives a full description of your current installation.
+Than it will retrieve the version of database.idx from the NFRA for 
+comparison. Any files that need to be updated are retrieved in $n_import.
+The list of files retrieved is in file  retrieved.grp.
+<PRE>
+  >>>    nup build -Update -T:^exe retrieved.grp
+</PRE>
+This will build all files just retrieved, and any files dependent on them.
+No executables will be built, this will be done after the library check.
+<PRE>
+  >>>    nup clear -NConfirm
+</PRE>
+This will throw away any source files in the master system that are no 
+longer needed.
+<PRE>
+  >>>    nup check l
+</PRE>
+This will check your libraries. Experience shows that escpecially on HP
+workstations libraries tend to get cluttered. This will be found by the
+library check. If necessary, an additional build command will be scheduled
+to rebuilt modules. Objects for which no source is present are removed 
+from the libraries. Duplicate entries are both removed and replaced by 
+a fresh entry. Out-of-date entries are updated.
+<PRE>
+  >>>    nup check e -Update
+</PRE>
+This will check your executables. Executables that do not yet exist 
+or are out-of-date with respect to the NFRA are rebuilt. Note that usually
+not all versions need to be rebuilt for a new revision. Thus some programs
+may show a lower version than the version shown by nnews.
+<PRE>
+  >>>    rsh HOST '( source $n_src/sys/newstar_xxxx.csh; nup update rsh)
+</PRE>
+If $n_hosts (as defined in newstar_xxxx.csh) contains more hosts, the above
+command will be issued for each of them. This will carry out the build 
+and check commands listed above, but not the retrieve.
+<P>
+The proceedings of the update command will dump a lot of output on your
+screen, which is also stored in logfiles $n_src/updyymmdd[i].log (see 
+above). You may want to redirect the output to a file or /dev/null.
+If any errors occur, the log-file will be sent to the Newstar group by eMail.
+<P>
+<P>
+The nup command has many more uses than the ones described above. Most of
+them should not be relevant to you, since they are related to partial
+rebuilds, making backups etc. In case you are interested though, you can
+get more information through the command
+<PRE>
+>>>    nup help -help
+
+</PRE>
+<HR>
+<H2>Appendix 1: Questionnaire new Newstar sites</H2>
+
+Provide the following information, and send it to <EM>newstar@nfra.nl</EM>
+<OL>
+
+<H3><LI>Site:</H3>
+<OL>
+<LI>Institute: 
+<P>
+<LI>Abbreviated institute name (up to 5 char):
+<P>
+<LI>Address:   
+<PRE>
+
+</PRE>
+<P>
+<LI>Friend of newstar: 
+<P>
+<LI>eMail address:  
+<P>
+<LI>ftp node(s):    
+<P>
+<LI>Phone:
+<PRE></PRE>
+</OL>
+
+<H3><LI>Platform:</H3>
+<OL>
+<LI>Platform(s) and their hostname(s) on which Newstar should run: 
+<OL>
+<LI>Convex (cv)
+<LI>DEC Alpha/OSF1 (da)
+<LI>DECstation (dw)
+<LI>HP workstation (hp)
+<LI>SUN (sw)
+</OL>
+If not in list contact to <EM>newstar@nfra.nl</EM> for possible inclusion of
+your platform.
+<P>
+<LI>Do platforms have a common NFS on which to place sources? 
+<OL>
+<LI>Yes
+<LI>No
+</OL>
+(only if more than one platform requested at 2.1)
+<P>
+<LI>Root directory for Newstar: 
+<BR>(e.g. /usr/src/newstar )
+<PRE></PRE>
+<LI>If object-libraries should be placed on a different file system,
+specify here:
+<PRE></PRE>
+<LI>Idem executables: 
+<PRE></PRE>
+<LI>Could you provide an account on your platform(s) in which we can
+login to do some remote checks can be made? 
+<OL>
+<LI>Yes
+<LI>No
+</OL>
+If <STRONG>YES</STRONG>, please specify it: 
+<PRE></PRE>
+</OL>
+
+<H3><LI>Software:</H3>
+<OL>
+<LI>Are you using the standard f77, cc and ld provided with your system? 
+<OL>
+<LI>Yes
+<LI>No
+</OL>
+If not, provide details on how to call them, and the switches provided)
+<PRE></PRE>
+<LI>What is your standard command to print 132 wide ASCII files? 
+<PRE></PRE>
+<LI>What is your standard command to plot A4-format PostScript files? 
+<PRE></PRE>
+<LI>What is your standard command to plot A3-format PostScript files? 
+<PRE></PRE>
+<LI>Which other plotters would you like to use? 
+<BR>(contact <EM>newstar@nfra.nl</EM> to see if support is possible)
+<PRE></PRE>
+</OL>
+
+<H3><LI>Input/Output medium:</H3>
+<OL>
+<LI>Specify the device-names of the available mediums for reading/writing data?
+<PRE></PRE>
+<LI>Specify on which medium you want to receive Newstar if you cannot 
+support ftp: 
+<BR>(9track/density, Exabyte, DAT, ...)
+<PRE></PRE>
+</OL>
+</OL>
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+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/file_indexing/file_indexing.html b/file_indexing/file_indexing.html
new file mode 100644
index 0000000000000000000000000000000000000000..56fd930093fecdc915f3ee4163d1e5278ea931ca
--- /dev/null
+++ b/file_indexing/file_indexing.html
@@ -0,0 +1,290 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The indexing and navigation of <i>NEWSTAR </i>'s compound data files </b>
+<P>
+<P><em>Contributed by Johan Hamaker, November 1994 <BR>960104: Add <A HREF="#.loops.vs.aggregates">loops vs. aggregates</A> 
+                and <A HREF="#.repetitive">repetitive processing</A> 
+ <P></em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=file_indexing.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=file_indexing.html#SECTION0002000000000000000>  <b>Indexed data-file types </b></A>
+<LI> <A NAME=tex2html3 HREF=file_indexing.html#SECTION0003000000000000000>  <b>The index structure </b></A>
+<LI> <A NAME=tex2html4 HREF=file_indexing.html#SECTION0004000000000000000>  <b>Addressing groups of data blocks </b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=file_indexing.html#SECTION0004100000000000000>  <b>Data-block aggregates </b></A>
+<LI> <A NAME=tex2html6 HREF=file_indexing.html#SECTION0004200000000000000>  <b>Looping</b></A>
+<UL> 
+<LI> <A NAME=tex2html7 HREF=file_indexing.html#SECTION0004210000000000000>  <b>Repetitive execution </b></A>
+</UL> 
+<LI> <A NAME=tex2html8 HREF=file_indexing.html#SECTION0004300000000000000>  <b>Nested loops, aggregate start sets </b></A>
+<LI> <A NAME=tex2html9 HREF=file_indexing.html#SECTION0004400000000000000>  <b>Loops versus data-block aggregates </b></A>
+</UL> 
+<LI> <A NAME=tex2html10 HREF=file_indexing.html#SECTION0005000000000000000>  <b>When one is not sure of the existing index ranges </b></A>
+<LI> <A NAME=tex2html11 HREF=file_indexing.html#SECTION0006000000000000000>  <b>Absolute indexing </b></A>
+</UL>
+<A NAME=.file.types><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Indexed data-file types </b></A></H1>
+<P>
+        The indexing structure described in this document is common to three types of <i>NEWSTAR </i> files. Each of these is a collection of 'elementary' <em>data blocks</em> under a <em>hierarchical index</em>:
+<P>
+ <UL><LI>   The <A HREF="../scn_file/scn_file.html">.SCN file</A>, collecting visibility <em>sectors</em>;
+<P>
+<LI>   The <A HREF="../wmp_descr/wmp_descr.html">.WMP file</A>, collecting <em>images</em>: maps and antenna patterns;
+<P>
+<LI>   The <A HREF="../ngcalc_descr/ngcalc_descr.html#.ngf.file">.NGF file</A>, collecting one-dimensional <em>cuts</em> through the visibility and correction 
+<A HREF="../scn_file/scn_file.html#.hypercube">hypercubes</A>. 
+ </UL>
+<P>
+        This document describes the generic properties of the index mechanism and the versatile mechanisms in the <i>NEWSTAR </i> program-parameter interface through which sets of data blocks can be defined for processing.
+<P>
+<A NAME=.index.structure><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>The index structure </b></A></H1>
+<P>
+        The data blocks are organised in a <em>hierarchical index</em>. This structure is isomorphous to the familiar directory structure for files, the data blocks taking the place of the individual files. Unlike directories, however, the indices are not names but <em>numbers</em>. As we shall see below, in some cases these numbers are related to some physical parameter, in other cases they are simply administrative sequence numbers.
+<P>
+        Just like a full file path is composed of concatenated directory names, a data block is adressed through its <em>compound index</em>, <em>i.e.</em> its concatenated indices: 
+<BR><BR>  &lt;index0&gt;.&lt;index1&gt;.&lt;index2&gt;.... 
+<BR><BR>At all levels, the first index value is 0. You may find this uncomfortable at first, but you will soon get used to it
+<P>
+        The successive indices convey specific information which is different between file types. The following information levels are used:
+<P>
+ <DL COMPACT><DT>
+<DD>   &lt;grp&gt;   group 
+<DT>
+<DD>   &lt;obs&gt;   observation 
+<DT>
+<DD>   &lt;fld&gt;   mosaic subfield 
+<DT>
+<DD>   &lt;chn&gt;   frequency channel 
+<DT>
+<DD>   &lt;pol&gt;   polarisation 
+<DT>
+<DD>   &lt;typ&gt;   type 
+<DT>
+<DD>   &lt;ifr&gt;   interferometer 
+<DT>
+<DD>   &lt;seq&gt;   sequence number
+<P>
+ </DL>  
+  The compound indices are:
+<P>
+ <DL COMPACT><DT>
+<DD>   &lt;grp&gt;.&lt;obs&gt;.&lt;fld&gt;.&lt;chn&gt;.&lt;seq&gt;             for the 
+<A HREF="../scn_file/scn_file.html">.SCN file</A>; 
+<DT>
+<DD>   &lt;grp&gt;.&lt;fld&gt;.&lt;chn&gt;.&lt;pol&gt;.&lt;typ&gt;.&lt;seq&gt;       for the <A HREF="../wmp_descr/wmp_descr.html">.WMP file</A>; 
+<DT>
+<DD>   &lt;grp&gt;.&lt;fld&gt;.&lt;chn&gt;.&lt;pol&gt;.&lt;ifr&gt;.&lt;seq&gt;       for the 
+<A HREF="../ngcalc_descr/ngcalc_descr.html#.ngf.file">.NGF file</A>.
+<P>
+ </DL>  
+  More details about the meaning and use of these levels is given in the documents on the individual file types.
+<P>
+<A NAME=.addressing.groups><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>Addressing groups of data blocks </b></A></H1>
+<P>
+        The true power of the indexing mechanism lies in its ability to address data blocks in aggregates of widely varying composition, through shorthand notations that one may type in response to a prompt asking for the data blocks to be processed.
+<P>
+<A NAME=.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000>  <b>Data-block aggregates </b></A></H2>
+<P>
+        Firstly, a compound index may refer to a <em>set</em> or <em>aggregate</em> of data blocks in several ways:
+<P>
+ <DL COMPACT><DT><DD>   Instead of a single index value, one may define an aggregate through a <em>range</em> with an <em>increment</em>: 
+<BR><BR>  &lt;start value&gt;-&lt;end value&gt;:&lt;step&gt; 
+<BR><BR>or abbreviations thereof (with obvious meaning):
+<P>
+  &lt;start value&gt;-&lt;end value&gt; 
+  &lt;start value&gt;-:&lt;step&gt; 
+  &lt;start value&gt;-
+<P>
+   <UL><DT>
+<DD> <em>WARNING: The range ('-') and step (':') notation is valid <em>only</em> for the index parameter &lt;xxx&gt;_SETS. In all other contexts they will be interpreted as expression operators.</em> 
+   </UL>  
+<DT><DD>   One may also use the <em>wildcard</em> character '*', meaning 'all values'. An index level may be omitted (by putting nothing between the dots that delimit it), and even the dots themselves for the trailing values; in all these cases <i>NEWSTAR </i> will substitute wildcards. Thus 
+<BR><BR>  3.*.1.*.*       3..1.*.*        3.*.1           3..1 
+<BR><BR>all mean the same thing.
+<P>
+<DT><DD>   Secondly, a number of sets in any of these forms may be concatenated with commas in between,  <em>e.g. </em>  
+<BR><BR>  3.1-5:2, 4, 5.1..3-:3
+<P>
+ </DL>
+<P>
+        For all practical purposes, the number of data blocks that can be addressed in these ways through a single specification is unlimited.
+<P>
+<A NAME=.looping><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000>  <b>Looping</b></A></H2>
+<P>
+        Suppose one wants to make 8 maps from 16 visibility sectors and specifies 
+ <DL COMPACT><DT>
+<DD>   3.5.0-15.1.0
+<P>
+ </DL>   for the input. NMAP will take this specification to mean that all 16 sectors must be used in the first map and will then stop because the input sectors are exhausted.
+<P>
+        What one needs is a mechanism to tell NMAP that it should use the sectors in pairs. One way to do this is to 'manually' execute it 8 times with sector specifications
+<P>
+ <DL COMPACT><DT>
+<DD>   SCN_SETS = 3.5.0-1.1.0 
+<DT>
+<DD>   SCN_SETS = 3.5.2-3.1.0 
+<DT>
+<DD> <em>etc.</em>
+<P>
+ </DL>
+<P>
+        <em>LOOPS</em> provide an efficient shorthand to do just that. With a LOOP specification, one directs the program to execute a program a number of times, incrementing the data-block specification after every cycle. The LOOP specification takes the form 
+ <DL COMPACT><DT>
+<DD>   &lt;number of cycles&gt;,&lt;compound-index increment per cycle&gt;
+<P>
+ </DL>
+<P>
+In combination with this, the initial set of data blocks is specified.
+<P>
+        Thus for the above example one would specify
+<P>
+ <DL COMPACT><DT>
+<DD>   SCN_LOOPS = 8,0.0.2  
+<DT>
+<DD>   SCN_SETS  = 3.1.0-1.1.0 
+<P>
+ </DL>  
+   Zeros may be omitted in the increment; thus in the above, the shorter notation 
+SCN_LOOPS = 8,..2 is just as good.
+<P>
+<A NAME=.repetitive><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H3><A NAME=SECTION0004210000000000000>  <b>Repetitive execution </b></A></H3>
+<P>
+        The LOOPS construct may also be used for executing the same operation more than once in a single run. viz. by specifying an increment of 0. E.g. 
+ <DL COMPACT><DT>
+<DD>   SCN_LOOPS = 8,...1, 3,0 
+<P>
+ </DL>  will select 8 sector aggregates, processing each 3 times in a row.
+<P>
+<A NAME=.nested.loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004300000000000000>  <b>Nested loops, aggregate start sets </b></A></H2>
+<P>
+        It is possible to specify more than one loop simultaneously,  <em>e.g. </em>
+<P>
+ <DL COMPACT><DT>
+<DD>   SCN_LOOPS = 64,..1, 8,...1 
+<DT>
+<DD>   SCN_SETS = 2.0.0.1.* 
+<P>
+ </DL>  
+  for a mosaic of 64 subfields and 8 frequency channels. This will result in 8 maps being made in succession for each of the 64 subfiels; <em>i.e.</em> a following loop is nested <em>inside</em> the ones specified before it.
+<P>
+        It more than one set is specified for the start cycle, incrementation is applied to each set. Thus,  <em>e.g. </em> , for a specification
+<P>
+ <DL COMPACT><DT>
+<DD>   SCN_LOOPS = 8,.1 
+<DT>
+<DD>   SCN_SETS = 1.0.3.1, 1.1-3:2.0.7
+<P>
+ </DL>
+<P>
+the data blocks used would be 
+ <DL COMPACT><DT>
+<DD>   1.0.3.1, 1.1.0.7, 1.3.0.7 for the first cycle; 
+<DT>
+<DD>   1.1.3.1, 1.2.0.7, 1.4.0.7 for the second cycle; 
+<DT>
+<DD>   1.1.3.1, 1.3.0.7, 1.5.0.7 for the third cycle;
+<P>
+ </DL>  
+  <em>etc.</em>. (This example merely serves to show how the loop mechanism works; one is not likely in reality to want successive cycles with partly overlapping input data blocks.)
+<P>
+<A NAME=.loops.vs.aggregates><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004400000000000000>  <b>Loops versus data-block aggregates </b></A></H2>
+<P>
+        In those operations where each data block is processaed individually, the blocks to be selected may be specified either as an aggregate or through a loop construct. For instance, Self-calibration operates on each data block ('sector') in a .SCN file in isolation; in this case, e.g. the specifications 
+ <DL COMPACT><DT>
+<DD>   SCN_SETS = 0.3-6.0.0-8
+<P>
+ </DL>  and 
+ <DL COMPACT><DT>
+<DD>   SCN_LOOPS = 4,.1, 9,...1  
+<DT>
+<DD>   SCN_SETS = 0.3.0.0 
+<P>
+ </DL>  are equivalent. The only reason why one might want to use a LOOPS specification in this case is to control the order in shich the dat blocks are selected.
+<P>
+        There are also applications in which data blocks are combined, for instance when a sky map is made using an aggregate of .SCN-file sectors as input. Here the LOOPS construct results in a separate map for each loop cycle, rather than a single map from all input sectors as an aggregate specification would. See <A HREF="#.nested.loops">above</A> for an example where a number of maps are made each using a sector aggregate as input.
+<P>
+<A NAME=.query><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000>  <b>When one is not sure of the existing index ranges </b></A></H1>
+<P>
+        Data files may become so large and complex that one does not remember precisely the ranges of the indices in all the various branches of the index hierarchy. If one doesn't particularly care, one may use wildcards or deliberately specify an index range that is too large: In most cases a <i>NEWSTAR </i> program, finding that a requested data block does not exist, will simply proceed to the next one. Thus, for example, if one specifies 8 loop cycles but there are only data for the first three, the 4th through 8th cycles will be traversed but nothing will be done in them.
+<P>
+        Another possibility one has is to reply with 'L' (for <em>Layout</em>) or 'O' (for <em>Overview</em>) to a _SETS or _LOOPS prompt. This will give you information about the composition of your data file.
+<P>
+<H1><A NAME=SECTION0006000000000000000>  <b>Absolute indexing </b></A></H1>
+<P>
+        In addition to the compound indices discussed so far, one may also use the <em>absolute</em> index to address a data block. The absolute index is a sequence number that is allocated sequentially to each new data block created; thus the newest data block invariably has the highest absolute index. Like the other indices, the absolute index starts at 0. 
+        To address a data block through its absolute index, prefix the number with a hash sign,  <em>e.g. </em>  
+ <DL COMPACT><DT>
+<DD>   WMP_SETS = #23-27
+<P>
+ </DL>
+<P>
+Absolute indices can be used throughout in place of compound indices. For example, the loop specification 
+ <DL COMPACT><DT>
+<DD>   NGF_LOOPS = 3,#1, 4,#3 
+<DT>
+<DD>   MGF_SETS = 3.7.5.1.*
+<P>
+ </DL>
+<P>
+is valid (but is may not be very easy to be sure that it does the right thing).
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/file_indexing/images.pl b/file_indexing/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/file_indexing/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/file_indexing/labels.pl b/file_indexing/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..b590a6ef0376165d0db714721dbd2677e5356f7a
--- /dev/null
+++ b/file_indexing/labels.pl
@@ -0,0 +1,15 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".query"} ="$URL/file_indexing.html"; 
+$external_labels{".repetitive"} ="$URL/file_indexing.html"; 
+$external_labels{".index.structure"} ="$URL/file_indexing.html"; 
+$external_labels{".loops.vs.aggregates"} ="$URL/file_indexing.html"; 
+$external_labels{".looping"} ="$URL/file_indexing.html"; 
+$external_labels{".file.types"} ="$URL/file_indexing.html"; 
+$external_labels{".sets"} ="$URL/file_indexing.html"; 
+$external_labels{".addressing.groups"} ="$URL/file_indexing.html"; 
+$external_labels{".contents"} ="$URL/file_indexing.html"; 
+$external_labels{".nested.loops"} ="$URL/file_indexing.html"; 
+
+1;
\ No newline at end of file
diff --git a/files_descr.ps b/files_descr.ps
new file mode 100644
index 0000000000000000000000000000000000000000..43c6e2708a94d72f53114c6206c1cc0c42947948
--- /dev/null
+++ b/files_descr.ps
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diff --git a/files_descr/_12872_tabular150.png b/files_descr/_12872_tabular150.png
new file mode 100644
index 0000000000000000000000000000000000000000..dc414323b1ab25b8906e2a8e0043a8b5c4dea509
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diff --git a/files_descr/_12872_tabular150.xbm b/files_descr/_12872_tabular150.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..28af250e351edc99d249f746a698f192b144e27c
--- /dev/null
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@@ -0,0 +1,437 @@
+#define noname_width 450
+#define noname_height 114
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x10,0x08,0x00,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x60,0x18,0x00,0x00,0x00,0x00,0x02,0x62,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x00,0x80,0x01,0x40,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,
+ 0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x0c,0x00,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x18,
+ 0x00,0x00,0x00,0x00,0x02,0x62,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x80,0x01,
+ 0x40,0x00,0x00,0x00,0x40,0x00,0x03,0x80,0xff,0x01,0x00,0x01,0x60,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x7e,0xff,0xcf,0x7d,0x3e,0x9f,
+ 0x3f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x70,0x3f,0xf0,0xf8,0x3c,0xf0,0x3f,
+ 0xe7,0xe3,0x63,0x9e,0x81,0xfb,0x3d,0xde,0xff,0xf9,0xde,0xf3,0x7c,0x80,0xe7,
+ 0x03,0x40,0x00,0x03,0x00,0x00,0x00,0x00,0x01,0x60,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x67,0xee,0x8c,0x19,0x8c,0xb3,0x39,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x60,0x26,0x60,0x98,0x66,0x60,0x66,0x36,0x32,0x62,
+ 0xb3,0x01,0x33,0x19,0xb3,0x37,0xf3,0xb3,0x99,0x47,0x80,0x6d,0x02,0xf0,0x01,
+ 0x03,0x00,0x00,0x00,0xc0,0x07,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xe3,0xe6,0x8c,0x19,0x8c,0xff,0x39,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x60,0x26,0x60,0x98,0x7e,0x60,0x66,0x36,0x32,0x62,0x3f,0x00,0x33,
+ 0x19,0xbf,0x31,0x32,0xbf,0xf9,0x47,0x00,0xef,0x01,0xe0,0x00,0x03,0x80,0xff,
+ 0x01,0x80,0x03,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xe3,0xe6,0x8c,0x59,0xac,0xc1,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x26,0x60,0x99,0x06,0x60,0x66,0x36,0x32,0x62,0x03,0x00,0x33,0x59,0x83,0x31,
+ 0x32,0x83,0x1d,0x46,0x80,0xed,0x03,0xf0,0x01,0x03,0x00,0x00,0x00,0xc0,0x07,
+ 0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x67,0xe6,0x8c,
+ 0x59,0xac,0xa3,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x26,0x60,0x99,
+ 0x46,0x60,0x66,0x36,0x32,0x62,0xa3,0x01,0x33,0x59,0xa3,0x31,0x33,0xa3,0x1d,
+ 0x47,0xc0,0x3c,0x02,0x53,0x01,0x63,0x06,0x00,0x80,0x41,0x05,0x63,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x7e,0xff,0xdf,0x7b,0x3c,0xbf,
+ 0x7f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x7f,0xe0,0xfd,0x3d,0xf0,0xff,
+ 0xef,0xe7,0xf7,0x9e,0x81,0xff,0x7b,0xde,0xf3,0x79,0x9e,0xf7,0xfc,0x80,0xff,
+ 0x03,0x43,0x00,0x63,0x86,0xff,0x81,0x01,0x01,0x63,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x02,0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x78,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,
+ 0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x3c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x38,0x00,0x00,0x00,0x80,0x01,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x00,0x00,0x00,0x00,0x80,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x03,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,
+ 0x11,0x08,0x00,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x80,0x30,
+ 0x00,0x00,0x00,0x00,0x01,0xc0,0x00,0x04,0x00,0x00,0x00,0x40,0x00,0x10,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x6c,0x00,0x00,0x00,0x00,0x00,0x80,0x0d,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x08,0x00,
+ 0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xc0,0x30,0x00,0x00,0x00,
+ 0x00,0x01,0x00,0x00,0x06,0x00,0x00,0x00,0x60,0x00,0x10,0x00,0x00,0x00,0x00,
+ 0x40,0x00,0x6e,0x00,0x00,0x00,0x00,0x00,0xc0,0x0d,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x0c,0x00,0x38,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xc0,0x30,0x00,0x00,0x00,0x00,0x01,0x00,
+ 0x00,0x06,0x00,0x00,0x00,0x60,0x00,0x10,0x00,0x00,0x00,0x10,0x60,0x00,0x4e,
+ 0xf0,0x3f,0x40,0x00,0x08,0xc0,0x09,0x80,0x00,0x00,0x01,0x40,0x30,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0xff,0xcf,0x7d,0x3e,0x9f,0x3f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0x79,0xe0,0xf1,0x79,0xc0,0xfb,0xf1,0x19,0xe0,0x7e,0xcf,0xfb,
+ 0x7e,0x9f,0xf7,0x3c,0x1f,0xe0,0xf9,0x00,0x10,0x60,0x00,0x60,0x00,0x00,0x40,
+ 0x00,0x08,0x00,0x0c,0x80,0x00,0x00,0x01,0x40,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x67,0xee,0x8c,0x19,0x8c,0xb3,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x33,0xc0,0x30,0xcd,0x60,0x36,0x19,0x19,0xc0,0x4c,0x66,0xf6,0xcc,0xde,0x6c,
+ 0xe6,0x11,0x60,0x9b,0x00,0x7c,0x60,0x00,0x60,0x00,0x00,0xf0,0x01,0x3e,0x00,
+ 0x0c,0xe0,0x03,0xc0,0x07,0xf0,0x31,0x00,0x00,0x00,0x00,0x00,0xe3,0xe6,0x8c,
+ 0x19,0x8c,0xff,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x33,0xc0,0x30,
+ 0xfd,0xe0,0x37,0x19,0x01,0xc0,0x4c,0xe6,0x37,0x8c,0xc6,0x6f,0xfe,0x11,0xc0,
+ 0x7b,0x00,0x38,0x60,0x00,0x30,0xf0,0x3f,0xe0,0x00,0x1c,0x00,0x06,0xc0,0x01,
+ 0x80,0x03,0xe0,0x30,0x00,0x00,0x00,0x00,0x00,0xe3,0xe6,0x8c,0x59,0xac,0xc1,
+ 0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xb3,0xc0,0x32,0x0d,0x60,0x30,
+ 0x19,0x01,0xc0,0x4c,0x76,0x30,0x8c,0xc6,0x60,0x87,0x11,0x60,0xfb,0x00,0x7c,
+ 0x60,0x00,0x58,0x00,0x00,0xf0,0x01,0x3e,0x00,0x0b,0xe0,0x03,0xc0,0x07,0xf0,
+ 0x31,0x00,0x00,0x00,0x00,0x00,0x67,0xe6,0x8c,0x59,0xac,0xa3,0x39,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0xb7,0xc0,0x32,0x8d,0x60,0x34,0x19,0x19,0xc0,
+ 0x4c,0x76,0x34,0xcc,0xc6,0x68,0xc7,0x11,0x30,0x8f,0xc0,0x54,0x60,0xcc,0x4c,
+ 0x00,0x00,0x50,0x19,0x2a,0x98,0xc9,0xa0,0x82,0x41,0x05,0x53,0x31,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0xff,0xdf,0x7b,0x3c,0xbf,0x7f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0xf7,0xc0,0xfb,0x7b,0xc0,0xfb,0xf3,0x1b,0xe0,0xff,0xde,0x7b,
+ 0x7c,0x8f,0xe7,0x3d,0x3f,0xe0,0xff,0xc0,0x10,0x60,0xcc,0x7e,0xf0,0x3f,0x40,
+ 0x18,0x08,0xd8,0xcf,0x80,0x80,0x01,0x01,0x43,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00};
diff --git a/files_descr/_7464_tabular149.png b/files_descr/_7464_tabular149.png
new file mode 100644
index 0000000000000000000000000000000000000000..dc414323b1ab25b8906e2a8e0043a8b5c4dea509
Binary files /dev/null and b/files_descr/_7464_tabular149.png differ
diff --git a/files_descr/_7464_tabular149.xbm b/files_descr/_7464_tabular149.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..28af250e351edc99d249f746a698f192b144e27c
--- /dev/null
+++ b/files_descr/_7464_tabular149.xbm
@@ -0,0 +1,437 @@
+#define noname_width 450
+#define noname_height 114
+static char noname_bits[] = {
+ 0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x70,0x00,0x30,0x00,0x0c,0x00,0x00,0x00,0xc0,0x01,0x00,0x00,0x00,
+ 0x00,0x1c,0x18,0x00,0x07,0x00,0x80,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x60,
+ 0x00,0x30,0x00,0x08,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x80,0x18,0x18,
+ 0x00,0x06,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,
+ 0x08,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x30,0xc0,0x18,0x00,0x00,0x06,0x00,
+ 0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x0c,0x00,0x38,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xc0,0x30,0x00,0x00,0x00,0x00,0x01,0x00,
+ 0x00,0x06,0x00,0x00,0x00,0x60,0x00,0x10,0x00,0x00,0x00,0x10,0x60,0x00,0x4e,
+ 0xf0,0x3f,0x40,0x00,0x08,0xc0,0x09,0x80,0x00,0x00,0x01,0x40,0x30,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0xff,0xcf,0x7d,0x3e,0x9f,0x3f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0x79,0xe0,0xf1,0x79,0xc0,0xfb,0xf1,0x19,0xe0,0x7e,0xcf,0xfb,
+ 0x7e,0x9f,0xf7,0x3c,0x1f,0xe0,0xf9,0x00,0x10,0x60,0x00,0x60,0x00,0x00,0x40,
+ 0x00,0x08,0x00,0x0c,0x80,0x00,0x00,0x01,0x40,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x67,0xee,0x8c,0x19,0x8c,0xb3,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x33,0xc0,0x30,0xcd,0x60,0x36,0x19,0x19,0xc0,0x4c,0x66,0xf6,0xcc,0xde,0x6c,
+ 0xe6,0x11,0x60,0x9b,0x00,0x7c,0x60,0x00,0x60,0x00,0x00,0xf0,0x01,0x3e,0x00,
+ 0x0c,0xe0,0x03,0xc0,0x07,0xf0,0x31,0x00,0x00,0x00,0x00,0x00,0xe3,0xe6,0x8c,
+ 0x19,0x8c,0xff,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x33,0xc0,0x30,
+ 0xfd,0xe0,0x37,0x19,0x01,0xc0,0x4c,0xe6,0x37,0x8c,0xc6,0x6f,0xfe,0x11,0xc0,
+ 0x7b,0x00,0x38,0x60,0x00,0x30,0xf0,0x3f,0xe0,0x00,0x1c,0x00,0x06,0xc0,0x01,
+ 0x80,0x03,0xe0,0x30,0x00,0x00,0x00,0x00,0x00,0xe3,0xe6,0x8c,0x59,0xac,0xc1,
+ 0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xb3,0xc0,0x32,0x0d,0x60,0x30,
+ 0x19,0x01,0xc0,0x4c,0x76,0x30,0x8c,0xc6,0x60,0x87,0x11,0x60,0xfb,0x00,0x7c,
+ 0x60,0x00,0x58,0x00,0x00,0xf0,0x01,0x3e,0x00,0x0b,0xe0,0x03,0xc0,0x07,0xf0,
+ 0x31,0x00,0x00,0x00,0x00,0x00,0x67,0xe6,0x8c,0x59,0xac,0xa3,0x39,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0xb7,0xc0,0x32,0x8d,0x60,0x34,0x19,0x19,0xc0,
+ 0x4c,0x76,0x34,0xcc,0xc6,0x68,0xc7,0x11,0x30,0x8f,0xc0,0x54,0x60,0xcc,0x4c,
+ 0x00,0x00,0x50,0x19,0x2a,0x98,0xc9,0xa0,0x82,0x41,0x05,0x53,0x31,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0xff,0xdf,0x7b,0x3c,0xbf,0x7f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0xf7,0xc0,0xfb,0x7b,0xc0,0xfb,0xf3,0x1b,0xe0,0xff,0xde,0x7b,
+ 0x7c,0x8f,0xe7,0x3d,0x3f,0xe0,0xff,0xc0,0x10,0x60,0xcc,0x7e,0xf0,0x3f,0x40,
+ 0x18,0x08,0xd8,0xcf,0x80,0x80,0x01,0x01,0x43,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00};
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+#define noname_width 5
+#define noname_height 7
+static char noname_bits[] = {
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new file mode 100644
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b><i>NEWSTAR </i> data-file organisation and the programs' associated user interfaces</b>
+<P>
+<i>Contributed by J.E. Noordam, August 1993</i>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=files_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=files_descr.html#SECTION0002000000000000000> <b><i>NEWSTAR </i> data and ancillary file types</b></A>
+<LI> <A NAME=tex2html3 HREF=files_descr.html#SECTION0003000000000000000> <b>Directories and nodes (files)</b></A>
+<LI> <A NAME=tex2html4 HREF=files_descr.html#SECTION0004000000000000000> <b>The <i>NEWSTAR </i> data files (SCN, MDL, WMP)</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=files_descr.html#SECTION0004100000000000000> <b>Data file logical organisation: Sets</b></A>
+<LI> <A NAME=tex2html6 HREF=files_descr.html#SECTION0004200000000000000> <b>Using loops</b></A>
+</UL> 
+<LI> <A NAME=tex2html7 HREF=files_descr.html#SECTION0005000000000000000> <b>Overview of interactions with the SCN file</b></A>
+<UL> 
+<LI> <A NAME=tex2html8 HREF=files_descr.html#SECTION0005100000000000000> <b>Creating SCN files</b></A>
+<LI> <A NAME=tex2html9 HREF=files_descr.html#SECTION0005200000000000000> <b>Inspecting the contents of a SCN file</b></A>
+<LI> <A NAME=tex2html10 HREF=files_descr.html#SECTION0005300000000000000> <b>Editing the header information of a SCN file</b></A>
+<LI> <A NAME=tex2html11 HREF=files_descr.html#SECTION0005400000000000000> <b>Applying corrections to uv-data</b></A>
+<LI> <A NAME=tex2html12 HREF=files_descr.html#SECTION0005500000000000000> <b>Modyfing the stored corrections</b></A>
+<LI> <A NAME=tex2html13 HREF=files_descr.html#SECTION0005600000000000000> <b>Modifying a uv-model in the SCN-file</b></A>
+<LI> <A NAME=tex2html14 HREF=files_descr.html#SECTION0005700000000000000> <b>Reorganisation of SCN files</b></A>
+<LI> <A NAME=tex2html15 HREF=files_descr.html#SECTION0005800000000000000> <b>Export of uv-data from SCN files</b></A>
+</UL> 
+<LI> <A NAME=tex2html16 HREF=files_descr.html#SECTION0006000000000000000> <b>Overview of interactions with an MDL file</b></A>
+<UL> 
+<LI> <A NAME=tex2html17 HREF=files_descr.html#SECTION0006100000000000000> <b>Adding source components to an MDL file</b></A>
+<LI> <A NAME=tex2html18 HREF=files_descr.html#SECTION0006200000000000000> <b>Modifying a model in an MDL file</b></A>
+<LI> <A NAME=tex2html19 HREF=files_descr.html#SECTION0006300000000000000> <b>Inspecting, displaying and sorting an MDL model</b></A>
+<LI> <A NAME=tex2html20 HREF=files_descr.html#SECTION0006400000000000000> <b>Relation with the uv-model in the .SCN file</b></A>
+<LI> <A NAME=tex2html21 HREF=files_descr.html#SECTION0006500000000000000> <b>The various uses of an MDL model</b></A>
+</UL> 
+<LI> <A NAME=tex2html22 HREF=files_descr.html#SECTION0007000000000000000> <b>Overview of interactions with a WMP file</b></A>
+<UL> 
+<LI> <A NAME=tex2html23 HREF=files_descr.html#SECTION0007100000000000000> <b>Creating maps in WMP files</b></A>
+<LI> <A NAME=tex2html24 HREF=files_descr.html#SECTION0007200000000000000> <b>Inspecting the contents of a WMP file</b></A>
+<LI> <A NAME=tex2html25 HREF=files_descr.html#SECTION0007300000000000000> <b>Editing the WMP header information</b></A>
+<LI> <A NAME=tex2html26 HREF=files_descr.html#SECTION0007400000000000000> <b>Operations on WMP images</b></A>
+<LI> <A NAME=tex2html27 HREF=files_descr.html#SECTION0007500000000000000> <b>.LOG files</b></A>
+<LI> <A NAME=tex2html28 HREF=files_descr.html#SECTION0007600000000000000> <b>.PLT files</b></A>
+<LI> <A NAME=tex2html29 HREF=files_descr.html#SECTION0007700000000000000> <b>.NGI files</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000> <b><i>NEWSTAR </i> data and ancillary file types</b></A></H1>
+<P>
+The <i>NEWSTAR </i> programs recognize three major types of data files, which are identified by their extension:  
+<BR><BR>.SCN files: uv-data and uv-model  
+<BR>.MDL files: SELFCAL source model  
+<BR>.WMP files: maps of various kinds
+<P>
+<i>NEWSTAR </i> programs also produce a number of ancillary files, with the following extensions (the list may no longer be complete):  
+<BR><BR>.PLT-files: to be plotted  
+<BR>.LOG-files: to be printed  
+<BR>.NGF-files: produced by NGALC  
+<BR>.MNG-files: used to make plots with the MONGO package
+<P>
+        The relations between these files and the <i>NEWSTAR </i> programs are shown in <A HREF=" #.newstar.overview">figure</A>.
+<P>
+<A NAME=.newstar.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  Overview of the Newstar programs and data files and their interrelations. For information on entities in this diagram see <BR><A HREF="../fig/newstar_overview.ps"><STRONG>FIGURE</STRONG></A> 
+ <i><BR>programs  
+  <A HREF="../ncalib_descr/ncalib_descr.html"><b>NCALIB</b></A>,  
+  <A HREF="../nmap_descr/nmap_descr.html"><b>NMAP</b></A>,  
+  <A HREF="../nscan_descr/nscan_descr.html"><b>NSCAN</b></A> <BR>files 
+  <A HREF="../scn_file/scn_file.html"><b>.SCN file</b></A>,  
+  <A HREF="../wmp_descr/wmp_descr.html"><b>.WMP file</b></A>, 
+  <A HREF="../mdl_descr/mdl_descr.html"><b>.MDL file</b></A> </i>
+<P>
+<A NAME=.nodes><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>Directories and nodes (files)</b></A></H1>
+<P>
+        For historical reasons, the <i>NEWSTAR </i> programs refer to data files as <b>nodes</b> in a <b>database</b>.  In fact, they are just files in a directory. Users are recommended to use a separate sub-directory for each data reduction project.
+<P>
+        However, although they refer to the same thing, there is a slight difference between <b>node names</b> used by the user and the actual <b>file names</b>: Node names are a series of alpha-numeric character strings separated by dots, e.g.:
+<P>
+ <PRE> 
+    mynode 
+    mynode.21cm.yesterday.s.x.c.d.file.dd 
+</PRE>
+<P>
+The maximum length of a node name is 80 characters (which means maximally 39
+dots). This is converted to a <em>file name</em> by: 
+<BR>- appending the extension (.SCN, .MDL or .WMP), <BR>- converting all dots (.) to underscores (_), <BR>- converting all lowercase to uppercase, 
+- replacing the underscore nearest but less than 47 to a dot. (?) <BR><BR>This file name is then prefixed with the current database (default nothing).
+<P>
+        Parts of a node name can be set aside for short-hand use.  This can be
+done by the INFIX keyword (see COMMON keywords), or in a node specification by
+enclosing a part in parenthesis ().  This enclosed part will from then on be
+available to all programs that are run in <b>the current stream</b>.  Reference
+to `the infix' is made by typing a #, e.g.:
+<P>
+ <PRE> 
+    mynode.21(cm.yesterday.s.x.c.d.file.d)d 
+</PRE>
+<P>
+Typing <tt>mynode.92#e</tt> will then produce <tt>mynode.92cm.yesterday.s.x.c.d.file.de</tt>
+<P>
+The database (directory) name can also be included in the node definition:
+<P>
+ <PRE> 
+    wnb/data/mynode 
+    ../other/mynode.21cm.yesterday.s.x.c.d.file.dd 
+</PRE>
+<P>
+        If a database is specified in this way, it will be saved in such a way
+that all subsequent program runs <b>in the same stream</b> that have no explicit
+database specified, will use it, including the currently running program at all
+its further node questions.
+<P>
+<H1><A NAME=SECTION0004000000000000000> <b>The <i>NEWSTAR </i> data files (SCN, MDL, WMP)</b></A></H1>
+<P>
+        These three <i>NEWSTAR </i> data files are each described in detail in their
+own `File Description' chapter in this Handbook.  In this Overview section, it
+is explained how the basic units (called Sets) in such a file can be selected
+individually or in groups.  For each of the three data files, an overview is
+given of the various ways in which the user may interact with these `objects',
+with references to the relevant program options.
+<P>
+<A NAME=data.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000> <b>Data file logical organisation: Sets</b></A></H2>
+<P>
+        The three main <i>NEWSTAR </i> data file (node) types are logically organised
+in the same way: they consist of a number of basic units called `Sets', which
+can be selected by the user in two ways:
+<P>
+<UL><LI> 
+        By <b>direct reference</b> to an absolute set index: <tt>#ir</tt> selects
+set nr <tt>ir</tt>, in which <tt>ir</tt> can be a range of contiguous sets (see
+below).  Direct reference is only useful if the user knows exactly how the
+various Sets are ordered in the file.
+<P>
+<LI> 
+        By <b>indexed reference</b> to a series of indices that represent
+parameters like map or channel nr.  A `selector' consists of a series on
+integer indices, separated by points.  The indices may also be specified as
+ranges of indices or wildcards (<IMG ALIGN=BOTTOM ALT="" SRC="_7464_tex2html_wrap362.png">).  For instance: <tt>ir1.ir2.*.ir4</tt>
+selects all Sets with index values in the indicated ranges.
+<P>
+</UL>
+<P>
+        <b>Index ranges</b> (<tt>ir</tt>) can take the following forms <b>(NB:
+Indices start at 0!)</b>:
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_12872_tabular150.png"><P>
+<P>
+<A NAME=loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000> <b>Using loops</b></A></H2>
+<P>
+        Sometimes a program must be run more than once for the same 
+SCN-file, but for different Sets.  In that case, the <b>LOOPS</b> keyword can
+used to specify subsequent ranges of Sets.  A loop is specified by means of a
+pair of values: The first value indicates how often the loop should execute,
+the second specifies an increment to be given to the Set specification at each
+run.
+<P>
+        For example: <tt>loops=3,..2</tt> indicates that the program has to run
+three times, each time incrementing the 3rd Set index by 2.  So, if the first
+Set (selected with the keyword SETS) was <tt>0.0-3.2.5.*</tt>, the program will be
+run three times, for the Sets
+<P>
+ <PRE> 
+   0.0-3.2.5.*.
+   0.0-3.4.5.*.
+   0.0-3.6.5.*.
+</PRE>
+<P>
+<b>Nested loops</b> can be specified by stringing loop definitions (pairs of
+values) together.  For instance: <tt>loops=3,..2,5,...3</tt> adds an inner loop of
+5 program runs in which the 4th Set index is incremented by 3 each time:
+<P>
+ <PRE> 
+   0.0-3.2.5.*.   0.0-3.2.8.*.   0.0-3.2.11.*.
+                  0.0-3.2.14.*.   0.0-3.2.17.*.
+   0.0-3.4.5.*.   0.0-3.4.8.*.   0.0-3.4.11.*.
+                  0.0-3.4.14.*.   0.0-3.4.17.*.
+   0.0-3.6.5.*.   0.0-3.6.8.*.   0.0-3.6.11.*.
+                  0.0-3.6.14.*.   0.0-3.6.17.*.
+</PRE>
+<P>
+<A NAME=scn><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>Overview of interactions with the SCN file</b></A></H1>
+<P>
+        The SCN-file contains uv-data, and possibly the uv-representation of a
+source model.  A single SCN-file may contain uv-data of different (but related)
+observations.
+<P>
+        For more information, see the dedicated SCN-file section in this
+chapter of the Handbook, and also the section on the program NSCAN.  It
+contains a description of the structure and the contents of the 
+SCN-file.
+<P>
+<A NAME=scn.create><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005100000000000000> <b>Creating SCN files</b></A></H2>
+<P>
+- From WSRT circle files: NSCAN option LOAD. <BR>- From ATCA (Australia Telescope Compact Array) files: NATNF.<BR>- From old (R-series) SCN-files: NSCAN option FROM_OLD.<BR>- Simulated uv-data: NSIMUL? (not implemented yet).<BR><A NAME=scn.inspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000> <b>Inspecting the contents of a SCN file</b></A></H2>
+<P>
+- File Layout: NSCAN option SHOW<BR>- File header: NSCAN option SHOW<BR>- Set headers: NSCAN option SHOW<BR> - Telescope (dipole) angle/ellipt corr: NCALIB option POLAR
+SHOW<BR>- Scan headers: NSCAN option SHOW<BR> - Telescope gain/phase corr: NCALIB option SHOW<BR>- uv-data (corrected, converted): NSCAN option SHOW<BR>- Display of (gridded) uv-data or uv-model: See WMP file below.<BR>- Plot telescope gain/phase corr (REDC+ALGC+OTHC): NPLOT option TELESCOPE<BR>- Plot Redundancy/Selfcal residuals: NPLOT option RESIDUAL<BR>- Plot uv-data or uv-model: NPLOT option DATA or MODEL<BR>- Print average telescope gain/phase corr (R+A+O): NCALIB option SHOW<BR>- Extract various astrophysical info: NGCALC<BR><A NAME=scnt><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005300000000000000> <b>Editing the header information of a SCN file</b></A></H2>
+<P>
+        Almost every value (observation parameters, corrections, etc) in the
+SCN-file headers may be edited manually by means of NSCAN option 
+SHOW EDIT.  This means that, even if there is no specific <i>NEWSTAR </i> routine to
+change something, it can always be done by hand.  This may be laborious in some
+cases, <em>but at least it is possible!</em>.  This feature is particularly useful
+in those (rare) cases where erroneous information has somehow been put in the
+header during the observations in Westerbork.
+<P>
+<A NAME=scn.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005400000000000000> <b>Applying corrections to uv-data</b></A></H2>
+<P>
+        In general, uv-data in a SCN-file is <em>never physically modified</em>.
+Corrections may be applied (or de-applied) to the uv-data whenever the data is
+read into memory to be processed.  The user may specify which corrections are
+applied (or de-applied) by specifying the value of the general <i>NEWSTAR </i>
+keywords APPLY and DE_APPLY, which are used by all <i>NEWSTAR </i> programs that
+handle uv-data.  Use <tt>dws NGEN</tt> 
+(see Common features of <i>NEWSTAR </i> programs).
+<P>
+<A NAME=scn.modify><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005500000000000000> <b>Modyfing the stored corrections</b></A></H2>
+<P>
+<b>Zeroeing</b> selected corrections: NCALIB option SET ZERO
+<P>
+<b>Set Header</b> (corrections that are `constant' in time):<BR>- Any value: NSCAN option SHOW EDIT<BR>- POLC (dipole angle error and ellipticity corr):<BR> - Estimation: NCALIB option POLAR CALC<BR> - Manual: NCALIB option POLAR SET, EDIT, ZERO<BR> - Copying from calibrator: NCALIB option POLAR COPY<BR><b>Scan Header</b> (corrections that vary per HA):<BR>- Any value: NSCAN option SHOW EDIT<BR>- Telescope (dipole) gain/phase corr:<BR> - Estimation: NCALIB option REDUN <BR> - Redundancy (no model): REDC<BR> - Align: ALGC<BR> - Selfcal ALGC<BR> - Manual: NCALIB option SET MANUAL, ZERO, RENORM <BR> - Copying from calibrator: NCALIB option SET COPY, CCOPY, LINE<BR>- Phase Zero Difference: OTHC<BR> - Estimation: NCALIB option POLAR VZERO CALC, APPLY, ASK, SCAN <BR> - Manual: NCALIB option POLAR VZERO MANUAL, ASK<BR> - Copying from calibrator: NCALIB option POLAR VZERO COPY<BR>- Extinction corr (manual): NCALIB option SET EXTINCT<BR>- Refraction corr (manual): NCALIB option SET REFRACT<BR>- Faraday corr (input of ionosonde data): NCALIB option SET FARADAY<BR><A NAME=scn.uvmodel><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005600000000000000> <b>Modifying a uv-model in the SCN-file</b></A></H2>
+<P>
+        See Overview of interactions with MDL file below.
+<P>
+<A NAME=scn.reorg><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005700000000000000> <b>Reorganisation of SCN files</b></A></H2>
+<P>
+- Create new `Job' from Sets in the same SCN-file: NSCAN option REGROUP<BR>- Create a `secondary' SCN-file (data selection, correction): NCOPY<BR>(not implemented yet)<BR>- Delete SCN-file: Use UNIX command <tt>rm &lt;xxx&gt;.SCN</tt> (be careful!)<BR><A NAME=scn.export><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005800000000000000> <b>Export of uv-data from SCN files</b></A></H2>
+<P>
+- To UVFITS format (AIPS): NSCAN option UVFITS, PFITS<BR>- To old (R-series) SCN-file format: NSCAN option TO_OLD<BR>- To WMP file (as gridded uv-data or maps): NMAP option MAKE<BR><A NAME=mdl.inter><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000> <b>Overview of interactions with an MDL file</b></A></H1>
+<P>
+        A MDL file contains a collection of source model components. 
+This may consist of a mixture of <b>multi-parameter components</b> and ordinary
+<b>CLEAN components</b>.  The MDL file may also contain <b>reference
+coordinates</b> (obtained from a SCN-file) for the position of the field centre
+and the observing frequency.
+<P>
+        For more information, see the dedicated MDL-file section in this
+chapter of the Cookbook, and also the section on the program NSCAN.  It
+contains a description of the structure and the contents of the 
+MDL-file.
+<P>
+        NOTE: Note that the model in the MDL file may be manipulated by means
+of NMODEL <b>options</b> (i.e.  options of the program NMODEL), or by MDL <b>handles</b>.  The latter operations (e.g.  READ, WRITE, EDIT, 
+SHOW) are available in all the programs that deal with source models: 
+NCALIB, NMAP, NCLEAN, NSCAN, NMODEL.
+<P>
+<A NAME=mdl.generate><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006100000000000000> <b>Adding source components to an MDL file</b></A></H2>
+<P>
+- Manual, by specifying source parameters: MDL handle ADD.<BR>- Automatic search of a map (in a WMP file): NMODEL action FIND<BR>- CLEANing a map (in a WMP file): NCLEAN option BEAM, UVCOVER, COMPON<BR>- Save model from SCN file in an MDL file: NMODEL option SAVE<BR>- Convert old (R-series) model to <i>NEWSTAR </i> MDL file format.<BR><A NAME=mdl.modify><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006200000000000000> <b>Modifying a model in an MDL file</b></A></H2>
+<P>
+Modifying <b>source components</b>:<BR>- Improve source parameters by fitting to the uv-data: 
+                NMODEL option UPDATE, XUPDATE<BR>- Manual editing: MDL handle EDIT, FEDIT<BR>- Delete:<BR> - All components: MDL handle CLEAR, ZERO<BR> - Selected components: 
+                MDL handle DELETE, DNCLOW, DCLOW, DAREA<BR> - Selected components: MDL handle EDIT, FEDIT<BR>- Calibrate (position, flux): MDL handle CALIB<BR>- Combine components at the same position: MDL handle MERGE<BR>- Correct for primary beam attenuation: NMODEL option BEAM, DEBEAM<BR>Modifying <b>reference coordinates</b>:<BR>- Change epoch or coordinate system: NMODEL option CONVERT<BR>NB: Reference position and frequency are obtained from SCN-file.<BR><A NAME=mdlspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006300000000000000> <b>Inspecting, displaying and sorting an MDL model</b></A></H2>
+<P>
+Inspecting:<BR>- Show list of components: MDL handle SHOW (screen) or PRINT (log-file)<BR>- Idem, in RA/DEC coordinates: MDL handle RSHOW, RLIST<BR>- Show source list statistics: MDL handle TOT <BR>Displaying:<BR>- As gridded uv-model from SCN file: See WMP file below<BR>- As a map of the uv-model in the SCN-file: See WMP file below<BR>- As position markers in a map: NPLOT option MAP<BR>- As `restored' components in a CLEAN residual map: NCLEAN option UREST <BR>Sorting:<BR>- According to decreasing flux: MDL handle SORT, WRITE(!)<BR>- According to the value of another source parameter: MDL handle FSORT<BR><A NAME=mdl.uvmodel><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006400000000000000> <b>Relation with the uv-model in the .SCN file</b></A></H2>
+<P>
+        The source components in an MDL file may be Fourier transformed to the
+uv-plane, to the uv-coordinates of the uv-data in a SCN-file. 
+This <b>uv-model</b> is then `saved' in the SCN-file, together with a copy of
+the MDL source components that produced it.
+<P>
+        Whenever a uv-model is needed (e.g.  for Selfcal in NCALIB, or source
+subtraction in NMAP) the user is always asked to specify a <b>input model</b>
+explicitly, even if there is already a <b>saved uv-model</b> in the SCN-file.
+This input model may be specified either by reading 
+(and editing) components from an MDL-file, or by editing source components
+manually.  In the following, the Fourier transform of the input model will be
+called the <b>input uv-model</b>.  The user may choose (keyword MODEL_ACTION)
+one of the following possibilities:
+<P>
+- <b>Merge:</b> Replace the saved uv-model with the input uv-model, 
+        and use it. <BR>- <b>Add:</b> Add the input uv-model to the saved uv-model in the SCN-file, 
+        and use it.<BR>- <b>New:</b> Replace the saved uv-model in the SCN file by the input uv-model, 
+        and use it.<BR>- <b>Temporary:</b> Use the input uv-model, 
+        but do not change the saved uv-model in the SCN-file.<BR>- <b>Increment:</b> Use the sum of the saved uv-model and the input uv-model, 
+        but do not change the saved uv-model in the SCN-file. <BR>NOTE: <i>NEWSTAR </i> regards the saved uv-model as <em>applied corrections</em>,
+i.e.  corrections that were applied (added) to the cosmic noise before the
+uv-data were put into the SCN file.  Hence, to subtract the saved uv-model from
+the data, one could specify `MOD' to the (NGEN) keyword DE_APPLY! Specifying
+`MOD' to the (NGEN) keyword APPLY will restore a model that was subtracted from
+the data before it was put in the SCN file (?).
+<P>
+<A NAME=mdl.uses><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006500000000000000> <b>The various uses of an MDL model</b></A></H2>
+<P>
+<b>Present uses</b> of an MDL model:<BR>- To solve for telescope gain/phase errors (Selfcal, Align): 
+        NCALIB option REDUN<BR>- To subtract sources from the uv-data: NMAP option MAKE<BR>- To combine multiple observations:<BR> - With different frequencies (broad-band mapping)<BR> - With different pointing centres (mosaicking)<BR> - With different observing times<BR>- To deal with instrumental polarisation<BR>- To undo large Faraday `rotation measures'<BR>- To detect variability <BR>- To simulate uv-data: clumsy at the moment<BR><b>Potential uses</b> of an MDL model:<BR>- To deal with non-isoplanaticity<BR>- To simulate uv-data: NSIMUL (not yet implemented)<BR><A NAME=wmpter><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0007000000000000000> <b>Overview of interactions with a WMP file</b></A></H1>
+<P>
+        A WMP file contains a collection of 2-dimensional arrays, that are
+related in some way (but that can have different dimensions).  These may be
+maps for various frequencies (line data) or pointing centres 
+(mosaicking), antenna patterns and CLEAN residual maps.  Even rectangular
+arrays of (gridded) uv-data may be put in a WMP file, for display purposes.
+<P>
+        For more information, see the dedicated WMP-file section in this
+chapter of the Cookbook, and also the section on the program NSCAN.  It
+contains a description of the structure and the contents of the 
+WMP-file.
+<P>
+<A NAME=wmp.create><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007100000000000000> <b>Creating maps in WMP files</b></A></H2>
+<P>
+- Making maps/ap's from uv-data (or uv-model) in SCN-file: NMAP option MAKE<BR> - Many types of maps:
+XX,YY,XY,YX,I,Q,U,V,cos,sin,ampl,phase,...<BR>- Residual maps: NCLEAN option BEAM, UVCOVER<BR>- Restored maps: NCLEAN option UREST<BR>- Gridded uv-data from SCN-file: NMAP option MAKE REAL, IMAG, AMPL, PHASE<BR> - In various forms: real or imaginary parts,ampl,phase,...<BR>- Gridded uv-coverage from SCN-file: NMAP option MAKE COVER<BR>- Copy maps: NMAP option FIDDLE COPY<BR>- Extract areas from maps: NMAP option FIDDLE EXTRACT<BR>- Convert from old (R-series) map files: NMAP option FROM_OLD<BR><b>Delete</b> WMP files: 
+Use operating system UNIX: <tt>rm &lt;....&gt;.WMP</tt> (be careful!)
+<P>
+<A NAME=wmpspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007200000000000000> <b>Inspecting the contents of a WMP file</b></A></H2>
+<P>
+- Show header information: NMAP option SHOW.<BR>- Display images on color screen (X): NGIDS<BR>- Make plots on X-screen or plotter: NPLOT option MAP 
+ - Various types: contour, greyscale, polar, ruled surface<BR><A NAME=wmp.edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007300000000000000> <b>Editing the WMP header information</b></A></H2>
+<P>
+- Edit header information: NMAP option SHOW.<BR><A NAME=wmp.oper><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007400000000000000> <b>Operations on WMP images</b></A></H2>
+<P>
+        Although <i>NEWSTAR </i> has primarily been designed for WSRT <em>uv-data</em>
+processing it offers some powerful image-plane features:
+<P>
+- Various map operations (very powerful): NMAP option FIDDLE<BR> - Add, subtract, average, extract, copy, mosaic, etc<BR>- Cleaning and restoring: NCLEAN option BEAM, UREST<BR>- Finding strong sources: NMODEL option FIND<BR>For many astrophysical projects, this will be sufficient. 
+However, for moreadvanced operations astrophysical image analysis, the user
+should transfer the images from the WMP file to other packages 
+(e.g.  GIPSY, AIPS) by means of the FITS format: NMAP option W16FITS, 
+W32FITS.
+<P>
+<A NAME=log><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007500000000000000> <b>.LOG files</b></A></H2>
+<P>
+        Each <i>NEWSTAR </i> program run produces a log-file, with the name <tt>&lt;progname&gt;.LOG</tt>.  It contains the `vital information' about the program run:
+keyword values (including the hidden ones) and essential results.  In some
+cases (e.g.  NCALIB REDUN), the user may specify how much information is
+printed in the log-file (keyword SHOW_LEVEL).
+<P>
+        The user may specify (NGEN keyword LOG) what happens with the log-file
+upon completion: it may be spooled automatically to the line printer, or thrown
+away, or kept for later inspection.  In the latter case, the log-file is
+automatically renamed with a unique name (e.g. <tt>NCA&lt;alphanumeric&gt;.LOG</tt>)
+when the program is run again.
+<P>
+<A NAME=plt><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007600000000000000> <b>.PLT files</b></A></H2>
+<P>
+        All plot files produced by the programs NPLOT and NGCALC have the
+extension .PLT.  The file names usually begin with the 3-4 letter code of the
+selected PLOTTER option (PSP, PAL, EMS etc), followed by a unique combination
+of alphanumeric characters derived from the date and time of creation.
+<P>
+<A NAME=ngi><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007700000000000000> <b>.NGI files</b></A></H2>
+<P>
+        NGI files are used to store the various information that the program
+NGCALC extracts from the SCN-file.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/files_descr/images.pl b/files_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..3b8b86e8c32e1d6df15e8fad0b722076b1f8703a
--- /dev/null
+++ b/files_descr/images.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{tabular}<<151>>ll<<151>><<152>>bfint<<152>>;html_special_mark_amp;singleindexvalueatthislevel<<153>>bf<<367>><<367>>$ast$<<368>><<368>><<153>>;html_special_mark_amp;wildcard:allpossibleindexvaluesatthislevel<<154>>bfint-<<154>>;html_special_mark_amp;allindexvaluesatthislevel,startingat`int'<<155>>bfint1-int2[:int3]<<155>>;html_special_mark_amp;indexvalues`int1'through`int2'bystep`int3'(dflt=1)<<156>>bfint1:int3<<156>>;html_special_mark_amp;interpretedasint1-<<369>><<369>>$ast$<<370>><<370>>:int3<<157>>bfomitted<<157>>;html_special_mark_amp;inthemiddle:interpretedas<<371>><<371>>$.ast$<<372>><<372>>(<<373>><<373>>$..equiv.ast.$<<374>><<374>>)<<158>>bfomitted<<158>>;html_special_mark_amp;atthe:interpretedas<<375>><<375>>$.ast$<<376>><<376>>(<<377>><<377>>$..2equivast.ast.2.ast.ast.ast$<<378>><<378>>){tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12872_tabular150.xbm">'; 
+$key = q/{tabular}<<150>>ll<<150>><<151>>bfint<<151>>;html_special_mark_amp;singleindexvalueatthislevel<<152>>bf<<364>><<364>>$ast$<<365>><<365>><<152>>;html_special_mark_amp;wildcard:allpossibleindexvaluesatthislevel<<153>>bfint-<<153>>;html_special_mark_amp;allindexvaluesatthislevel,startingat`int'<<154>>bfint1-int2[:int3]<<154>>;html_special_mark_amp;indexvalues`int1'through`int2'bystep`int3'(dflt=1)<<155>>bfint1:int3<<155>>;html_special_mark_amp;interpretedasint1-<<366>><<366>>$ast$<<367>><<367>>:int3<<156>>bfomitted<<156>>;html_special_mark_amp;inthemiddle:interpretedas<<368>><<368>>$.ast$<<369>><<369>>(<<370>><<370>>$..equiv.ast.$<<371>><<371>>)<<157>>bfomitted<<157>>;html_special_mark_amp;atthe:interpretedas<<372>><<372>>$.ast$<<373>><<373>>(<<374>><<374>>$..2equivast.ast.2.ast.ast.ast$<<375>><<375>>){tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7464_tabular149.xbm">'; 
+$key = q/{}$ast${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7464_tex2html_wrap362.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/files_descr/labels.pl b/files_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..58f1156180d2b439ac2b2a01de3fb9cb5f1162b3
--- /dev/null
+++ b/files_descr/labels.pl
@@ -0,0 +1,33 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"mdl.uvmodel"} ="$URL/files_descr.html"; 
+$external_labels{"scn.inspect"} ="$URL/files_descr.html"; 
+$external_labels{"ngi"} ="$URL/files_descr.html"; 
+$external_labels{"loops"} ="$URL/files_descr.html"; 
+$external_labels{"scn.uvmodel"} ="$URL/files_descr.html"; 
+$external_labels{".contents"} ="$URL/files_descr.html"; 
+$external_labels{"plt"} ="$URL/files_descr.html"; 
+$external_labels{"scn.apply"} ="$URL/files_descr.html"; 
+$external_labels{"mdlspect"} ="$URL/files_descr.html"; 
+$external_labels{"scn.export"} ="$URL/files_descr.html"; 
+$external_labels{"scn"} ="$URL/files_descr.html"; 
+$external_labels{"scn.reorg"} ="$URL/files_descr.html"; 
+$external_labels{"mdl.uses"} ="$URL/files_descr.html"; 
+$external_labels{"wmpter"} ="$URL/files_descr.html"; 
+$external_labels{"wmp.oper"} ="$URL/files_descr.html"; 
+$external_labels{"wmp.edit"} ="$URL/files_descr.html"; 
+$external_labels{".nodes"} ="$URL/files_descr.html"; 
+$external_labels{"mdl.modify"} ="$URL/files_descr.html"; 
+$external_labels{"scn.create"} ="$URL/files_descr.html"; 
+$external_labels{"scnt"} ="$URL/files_descr.html"; 
+$external_labels{"scn.modify"} ="$URL/files_descr.html"; 
+$external_labels{"log"} ="$URL/files_descr.html"; 
+$external_labels{"wmp.create"} ="$URL/files_descr.html"; 
+$external_labels{"data.sets"} ="$URL/files_descr.html"; 
+$external_labels{"wmpspect"} ="$URL/files_descr.html"; 
+$external_labels{"mdl.generate"} ="$URL/files_descr.html"; 
+$external_labels{"mdl.inter"} ="$URL/files_descr.html"; 
+$external_labels{".newstar.overview"} ="$URL/files_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/files_handle.ps b/files_handle.ps
new file mode 100644
index 0000000000000000000000000000000000000000..57946e197c8e5a1f0b7d0c36fbb5604f6c3ca3db
--- /dev/null
+++ b/files_handle.ps
@@ -0,0 +1,1718 @@
+%!PS-Adobe-2.0
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+%%Pages: 9
+%%PageOrder: Ascend
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+%%EndComments
+%DVIPSCommandLine: dvips -o /newstar/master/hlp/files_handle.ps
+%+ files_handle_tmp.dvi
+%DVIPSParameters: dpi=300, compressed
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+509 y(astroph)o(ysical)e(image)f(analysis,)g(the)i(user)h(should)e
+(transfer)i(the)f(images)e(from)f(the)j(WMP)g(\014le)f(to)h(other)g
+(pac)o(k)n(ages)0 559 y(\(e.g.)i(GIPSY,)13 b(AIPS\))i(b)o(y)e(means)g
+(of)h(the)g(FITS)g(format:)i(NMAP)f(option)e(W16FITS,)g(W32FITS.)0
+721 y Fi(7)67 b(Auxiliary)26 b Fj(NEWST)-5 b(AR)18 b
+Fi(\014les)0 845 y Fc(7.1)56 b(.LOG)18 b(\014les)0 946
+y Ff(Eac)o(h)c Fg(NEWST)m(AR)g Ff(program)e(run)i(pro)q(duces)i(a)d
+(log-\014le,)g(with)g(the)i(name)e Fd(<progname>.LOG)p
+Ff(.)d(It)k(con)o(tains)g(the)g(`vital)0 996 y(information')8
+b(ab)q(out)k(the)g(program)e(run:)18 b(k)o(eyw)o(ord)11
+b(v)n(alues)h(\(including)f(the)h(hidden)g(ones\))g(and)g(essen)o(tial)
+g(results.)19 b(In)0 1046 y(some)12 b(cases)i(\(e.g.)j(NCALIB)c
+(REDUN\),)f(the)h(user)h(ma)o(y)c(sp)q(ecify)j(ho)o(w)f(m)o(uc)o(h)g
+(information)d(is)k(prin)o(ted)g(in)f(the)h(log-\014le)0
+1096 y(\(k)o(eyw)o(ord)h(SHO)o(W)p 310 1096 13 2 v 15
+w(LEVEL\).)118 1171 y(The)h(user)g(ma)o(y)e(sp)q(ecify)h(\(NGEN)h(k)o
+(eyw)o(ord)f(LOG\))g(what)g(happ)q(ens)i(with)e(the)h(log-\014le)e(up)q
+(on)h(completion:)j(it)0 1220 y(ma)o(y)e(b)q(e)i(sp)q(o)q(oled)f
+(automatically)e(to)i(the)h(line)f(prin)o(ter,)h(or)g(thro)o(wn)f(a)o
+(w)o(a)o(y)m(,)f(or)i(k)o(ept)g(for)f(later)g(insp)q(ection.)27
+b(In)16 b(the)0 1270 y(latter)i(case,)h(the)f(log-\014le)f(is)h
+(automatically)c(renamed)k(with)f(a)g(unique)h(name)f(\(e.g.)29
+b Fd(NCA<alphanumeric>)o(.LOG)p Ff(\))0 1320 y(when)14
+b(the)h(program)d(is)i(run)g(again.)0 1461 y Fc(7.2)56
+b(.PL)-5 b(T)18 b(\014les)0 1563 y Ff(All)12 b(plot)h(\014les)h(pro)q
+(duced)g(b)o(y)f(the)h(programs)e(NPLOT)i(and)f(NGCALC)g(ha)o(v)o(e)g
+(the)h(extension)g(.PL)m(T.)e(The)h(\014le)h(names)0
+1612 y(usually)f(b)q(egin)h(with)g(the)h(3-4)e(letter)i(co)q(de)g(of)f
+(the)g(selected)i(PLOTTER)e(option)g(\(PSP)m(,)g(P)m(AL,)f(EMS)i
+(etc\),)f(follo)o(w)o(ed)0 1662 y(b)o(y)g(a)f(unique)h(com)o(bination)e
+(of)h(alphan)o(umeric)f(c)o(haracters)k(deriv)o(ed)e(from)e(the)j(date)
+f(and)g(time)e(of)i(creation.)0 1803 y Fc(7.3)56 b(.NGI)18
+b(\014les)0 1905 y Ff(NGI)10 b(\014les)h(are)g(used)g(to)g(store)g(the)
+g(v)n(arious)f(information)e(that)i(the)h(program)e(NGCALC)h(extracts)i
+(from)d(the)i(SCN-\014le.)935 2995 y(9)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/files_handle/_12969_tabular150.png b/files_handle/_12969_tabular150.png
new file mode 100644
index 0000000000000000000000000000000000000000..dc414323b1ab25b8906e2a8e0043a8b5c4dea509
Binary files /dev/null and b/files_handle/_12969_tabular150.png differ
diff --git a/files_handle/_12969_tabular150.xbm b/files_handle/_12969_tabular150.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..28af250e351edc99d249f746a698f192b144e27c
--- /dev/null
+++ b/files_handle/_12969_tabular150.xbm
@@ -0,0 +1,437 @@
+#define noname_width 450
+#define noname_height 114
+static char noname_bits[] = {
+ 0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x70,0x00,0x30,0x00,0x0c,0x00,0x00,0x00,0xc0,0x01,0x00,0x00,0x00,
+ 0x00,0x1c,0x18,0x00,0x07,0x00,0x80,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x60,
+ 0x00,0x30,0x00,0x08,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x80,0x18,0x18,
+ 0x00,0x06,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,
+ 0x08,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x30,0xc0,0x18,0x00,0x00,0x06,0x00,
+ 0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x64,0x00,0x00,0x00,0x08,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x00,0x30,0xc0,0x18,0x00,0x00,0x06,0x00,0x00,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xe7,0xcf,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xf0,0xdd,0xcf,0x6f,0x1e,0xb8,0x9f,0x8f,0x77,0x07,0x77,0x8f,0xdd,
+ 0x3c,0xe0,0x79,0xe0,0xf9,0xdc,0x07,0xe6,0xdd,0x3d,0x03,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xc6,0x9d,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,
+ 0x99,0x69,0x62,0x33,0x30,0xd3,0xc8,0xec,0x01,0x26,0x9b,0x99,0x66,0x60,0x33,
+ 0xc0,0x98,0xd8,0x04,0x36,0x9b,0x66,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x9c,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x98,0x69,0x62,
+ 0x3f,0x30,0xd3,0xc8,0xcf,0x01,0x36,0x9e,0x99,0x7e,0xc0,0x33,0xc0,0x98,0xd8,
+ 0x03,0xf6,0xdb,0x7e,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x9c,0x05,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x99,0xc9,0x63,0x03,0x30,0xd3,
+ 0xc8,0xc0,0x01,0x1c,0x9b,0x99,0x06,0x60,0xb3,0xc0,0x9a,0xd8,0x07,0x36,0x70,
+ 0x06,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x9c,0x05,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x99,0x49,0x60,0x23,0x30,0xd3,0xc8,0x68,0x03,
+ 0x9c,0xb9,0xd9,0x46,0x30,0xb7,0xc0,0x9a,0x58,0x04,0x36,0x72,0x46,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xef,0xbf,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xf0,0xfd,0xdf,0xf7,0x1e,0xf8,0xbf,0x9f,0x77,0x07,0x08,0xff,0xfb,
+ 0x3d,0xe0,0xf7,0xc0,0xff,0xfd,0x07,0xef,0x21,0xbc,0x07,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x60,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x0c,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x07,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x1d,0x0c,0x00,0x00,0x30,
+ 0x00,0x00,0xee,0x00,0x00,0x00,0x00,0x3b,0x1c,0x00,0x0c,0x00,0x06,0x00,0x00,
+ 0x00,0x70,0x00,0x00,0x00,0x00,0x00,0xc0,0xc1,0x00,0x38,0x00,0x00,0x1c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x19,0x08,0x00,0x00,0x20,0x00,0x00,0xcc,
+ 0x00,0x00,0x00,0x00,0x33,0x18,0x00,0x0c,0x00,0x04,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x02,0x84,0xc1,0x00,0x30,0x00,0x00,0x18,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x18,0x08,0x00,0x00,0x20,0x00,0x00,0xcc,0x00,0x00,0x00,
+ 0x00,0x30,0x18,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,
+ 0x03,0x86,0x01,0x00,0x30,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x08,0x00,0x00,0x20,0x00,0x00,0xcc,0x00,0x00,0x00,0x00,0x30,0x18,
+ 0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x03,0x86,0x01,
+ 0x00,0x30,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0xff,0x99,0x8f,
+ 0xef,0xf9,0x3e,0x06,0x78,0xcc,0xe0,0xc7,0xf7,0xbf,0xf3,0x99,0x07,0xee,0xc7,
+ 0xe7,0xdd,0xc1,0xdd,0x63,0x37,0xde,0x07,0x9e,0x07,0x8f,0xef,0x3e,0x30,0xef,
+ 0xee,0x19,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x3e,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x9b,0xd9,0xc8,0x6c,0xf3,0x23,
+ 0x06,0xd8,0xcc,0xc0,0x6c,0x34,0x27,0x33,0xdb,0x0c,0xcc,0x64,0x34,0x7b,0x80,
+ 0xc9,0x66,0x26,0xf3,0x04,0x36,0x03,0x86,0xc9,0x26,0xb0,0xd9,0x34,0x1b,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x60,0x8f,0xd9,0xc8,0xc0,0x33,0x23,0x00,0xf0,0xcc,
+ 0xc0,0x68,0xfc,0x1e,0x33,0xda,0x0f,0xcc,0x64,0xf4,0x73,0x80,0x8d,0x67,0x26,
+ 0xff,0x03,0x3c,0x03,0x86,0xc9,0x1e,0xb0,0xdf,0xf6,0x1b,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xc0,0x8f,0xd9,0xc8,0x60,0x33,0x23,0x00,0xd8,0xcc,0xc0,0x68,0xfc,
+ 0x3f,0x33,0xda,0x00,0xcc,0x64,0x34,0x70,0x00,0xc7,0x66,0x26,0xc3,0x07,0x36,
+ 0x0b,0x96,0xc9,0x3e,0xb0,0x81,0x33,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x2a,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,
+ 0x8e,0xd9,0xc8,0x38,0x37,0x23,0x06,0xcc,0xcd,0xc0,0x6c,0x14,0x23,0x33,0xdb,
+ 0x08,0xcc,0x64,0x34,0xda,0x00,0x67,0x6e,0x36,0x63,0x04,0x73,0x0b,0x96,0xc9,
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+ 0x7f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x7f,0xe0,0xfd,0x3d,0xf0,0xff,
+ 0xef,0xe7,0xf7,0x9e,0x81,0xff,0x7b,0xde,0xf3,0x79,0x9e,0xf7,0xfc,0x80,0xff,
+ 0x03,0x43,0x00,0x63,0x86,0xff,0x81,0x01,0x01,0x63,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x02,0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x78,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,
+ 0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x3c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x38,0x00,0x00,0x00,0x80,0x01,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x00,0x00,0x00,0x00,0x80,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x03,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,
+ 0x11,0x08,0x00,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x80,0x30,
+ 0x00,0x00,0x00,0x00,0x01,0xc0,0x00,0x04,0x00,0x00,0x00,0x40,0x00,0x10,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x6c,0x00,0x00,0x00,0x00,0x00,0x80,0x0d,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x08,0x00,
+ 0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xc0,0x30,0x00,0x00,0x00,
+ 0x00,0x01,0x00,0x00,0x06,0x00,0x00,0x00,0x60,0x00,0x10,0x00,0x00,0x00,0x00,
+ 0x40,0x00,0x6e,0x00,0x00,0x00,0x00,0x00,0xc0,0x0d,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x0c,0x00,0x38,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xc0,0x30,0x00,0x00,0x00,0x00,0x01,0x00,
+ 0x00,0x06,0x00,0x00,0x00,0x60,0x00,0x10,0x00,0x00,0x00,0x10,0x60,0x00,0x4e,
+ 0xf0,0x3f,0x40,0x00,0x08,0xc0,0x09,0x80,0x00,0x00,0x01,0x40,0x30,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0xff,0xcf,0x7d,0x3e,0x9f,0x3f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0x79,0xe0,0xf1,0x79,0xc0,0xfb,0xf1,0x19,0xe0,0x7e,0xcf,0xfb,
+ 0x7e,0x9f,0xf7,0x3c,0x1f,0xe0,0xf9,0x00,0x10,0x60,0x00,0x60,0x00,0x00,0x40,
+ 0x00,0x08,0x00,0x0c,0x80,0x00,0x00,0x01,0x40,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x67,0xee,0x8c,0x19,0x8c,0xb3,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x33,0xc0,0x30,0xcd,0x60,0x36,0x19,0x19,0xc0,0x4c,0x66,0xf6,0xcc,0xde,0x6c,
+ 0xe6,0x11,0x60,0x9b,0x00,0x7c,0x60,0x00,0x60,0x00,0x00,0xf0,0x01,0x3e,0x00,
+ 0x0c,0xe0,0x03,0xc0,0x07,0xf0,0x31,0x00,0x00,0x00,0x00,0x00,0xe3,0xe6,0x8c,
+ 0x19,0x8c,0xff,0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x33,0xc0,0x30,
+ 0xfd,0xe0,0x37,0x19,0x01,0xc0,0x4c,0xe6,0x37,0x8c,0xc6,0x6f,0xfe,0x11,0xc0,
+ 0x7b,0x00,0x38,0x60,0x00,0x30,0xf0,0x3f,0xe0,0x00,0x1c,0x00,0x06,0xc0,0x01,
+ 0x80,0x03,0xe0,0x30,0x00,0x00,0x00,0x00,0x00,0xe3,0xe6,0x8c,0x59,0xac,0xc1,
+ 0x39,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xb3,0xc0,0x32,0x0d,0x60,0x30,
+ 0x19,0x01,0xc0,0x4c,0x76,0x30,0x8c,0xc6,0x60,0x87,0x11,0x60,0xfb,0x00,0x7c,
+ 0x60,0x00,0x58,0x00,0x00,0xf0,0x01,0x3e,0x00,0x0b,0xe0,0x03,0xc0,0x07,0xf0,
+ 0x31,0x00,0x00,0x00,0x00,0x00,0x67,0xe6,0x8c,0x59,0xac,0xa3,0x39,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0xb7,0xc0,0x32,0x8d,0x60,0x34,0x19,0x19,0xc0,
+ 0x4c,0x76,0x34,0xcc,0xc6,0x68,0xc7,0x11,0x30,0x8f,0xc0,0x54,0x60,0xcc,0x4c,
+ 0x00,0x00,0x50,0x19,0x2a,0x98,0xc9,0xa0,0x82,0x41,0x05,0x53,0x31,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0xff,0xdf,0x7b,0x3c,0xbf,0x7f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0xf7,0xc0,0xfb,0x7b,0xc0,0xfb,0xf3,0x1b,0xe0,0xff,0xde,0x7b,
+ 0x7c,0x8f,0xe7,0x3d,0x3f,0xe0,0xff,0xc0,0x10,0x60,0xcc,0x7e,0xf0,0x3f,0x40,
+ 0x18,0x08,0xd8,0xcf,0x80,0x80,0x01,0x01,0x43,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00};
diff --git a/files_handle/_7567_tabular149.png b/files_handle/_7567_tabular149.png
new file mode 100644
index 0000000000000000000000000000000000000000..dc414323b1ab25b8906e2a8e0043a8b5c4dea509
Binary files /dev/null and b/files_handle/_7567_tabular149.png differ
diff --git a/files_handle/_7567_tabular149.xbm b/files_handle/_7567_tabular149.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..28af250e351edc99d249f746a698f192b144e27c
--- /dev/null
+++ b/files_handle/_7567_tabular149.xbm
@@ -0,0 +1,437 @@
+#define noname_width 450
+#define noname_height 114
+static char noname_bits[] = {
+ 0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x70,0x00,0x30,0x00,0x0c,0x00,0x00,0x00,0xc0,0x01,0x00,0x00,0x00,
+ 0x00,0x1c,0x18,0x00,0x07,0x00,0x80,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x60,
+ 0x00,0x30,0x00,0x08,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x80,0x18,0x18,
+ 0x00,0x06,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,
+ 0x08,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x30,0xc0,0x18,0x00,0x00,0x06,0x00,
+ 0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x64,0x00,0x00,0x00,0x08,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x00,0x30,0xc0,0x18,0x00,0x00,0x06,0x00,0x00,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xe7,0xcf,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xf0,0xdd,0xcf,0x6f,0x1e,0xb8,0x9f,0x8f,0x77,0x07,0x77,0x8f,0xdd,
+ 0x3c,0xe0,0x79,0xe0,0xf9,0xdc,0x07,0xe6,0xdd,0x3d,0x03,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xc6,0x9d,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,
+ 0x99,0x69,0x62,0x33,0x30,0xd3,0xc8,0xec,0x01,0x26,0x9b,0x99,0x66,0x60,0x33,
+ 0xc0,0x98,0xd8,0x04,0x36,0x9b,0x66,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x9c,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x98,0x69,0x62,
+ 0x3f,0x30,0xd3,0xc8,0xcf,0x01,0x36,0x9e,0x99,0x7e,0xc0,0x33,0xc0,0x98,0xd8,
+ 0x03,0xf6,0xdb,0x7e,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x9c,0x05,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x99,0xc9,0x63,0x03,0x30,0xd3,
+ 0xc8,0xc0,0x01,0x1c,0x9b,0x99,0x06,0x60,0xb3,0xc0,0x9a,0xd8,0x07,0x36,0x70,
+ 0x06,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x9c,0x05,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x99,0x49,0x60,0x23,0x30,0xd3,0xc8,0x68,0x03,
+ 0x9c,0xb9,0xd9,0x46,0x30,0xb7,0xc0,0x9a,0x58,0x04,0x36,0x72,0x46,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xef,0xbf,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xf0,0xfd,0xdf,0xf7,0x1e,0xf8,0xbf,0x9f,0x77,0x07,0x08,0xff,0xfb,
+ 0x3d,0xe0,0xf7,0xc0,0xff,0xfd,0x07,0xef,0x21,0xbc,0x07,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x18,0x08,0xd8,0xcf,0x80,0x80,0x01,0x01,0x43,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00};
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b><i>NEWSTAR </i> data-file organisation and the programs' associated user interfaces</b>
+<P>
+ <i>Contributed by J.E. Noordam, August 1993</i>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=files_handle.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=files_handle.html#SECTION0002000000000000000> <b><i>NEWSTAR </i> data and ancillary file types</b></A>
+<LI> <A NAME=tex2html3 HREF=files_handle.html#SECTION0003000000000000000> <b>Directories and nodes (files)</b></A>
+<LI> <A NAME=tex2html4 HREF=files_handle.html#SECTION0004000000000000000> <b>The <i>NEWSTAR </i> data files (SCN, MDL, WMP)</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=files_handle.html#SECTION0004100000000000000> <b>Data file logical organisation: Sets</b></A>
+<LI> <A NAME=tex2html6 HREF=files_handle.html#SECTION0004200000000000000> <b>Using loops</b></A>
+</UL> 
+<LI> <A NAME=tex2html7 HREF=files_handle.html#SECTION0005000000000000000> <b>Overview of interactions with the SCN file</b></A>
+<UL> 
+<LI> <A NAME=tex2html8 HREF=files_handle.html#SECTION0005100000000000000> <b>Creating SCN files</b></A>
+<LI> <A NAME=tex2html9 HREF=files_handle.html#SECTION0005200000000000000> <b>Inspecting the contents of a SCN file</b></A>
+<LI> <A NAME=tex2html10 HREF=files_handle.html#SECTION0005300000000000000> <b>Editing the header information of a SCN file</b></A>
+<LI> <A NAME=tex2html11 HREF=files_handle.html#SECTION0005400000000000000> <b>Applying corrections to uv-data</b></A>
+<LI> <A NAME=tex2html12 HREF=files_handle.html#SECTION0005500000000000000> <b>Modyfing the stored corrections</b></A>
+<LI> <A NAME=tex2html13 HREF=files_handle.html#SECTION0005600000000000000> <b>Modifying a uv-model in the SCN-file</b></A>
+<LI> <A NAME=tex2html14 HREF=files_handle.html#SECTION0005700000000000000> <b>Reorganisation of SCN files</b></A>
+<LI> <A NAME=tex2html15 HREF=files_handle.html#SECTION0005800000000000000> <b>Export of uv-data from SCN files</b></A>
+</UL> 
+<LI> <A NAME=tex2html16 HREF=files_handle.html#SECTION0006000000000000000> <b>Overview of interactions with an MDL file</b></A>
+<UL> 
+<LI> <A NAME=tex2html17 HREF=files_handle.html#SECTION0006100000000000000> <b>Adding source components to an MDL file</b></A>
+<LI> <A NAME=tex2html18 HREF=files_handle.html#SECTION0006200000000000000> <b>Modifying a model in an MDL file</b></A>
+<LI> <A NAME=tex2html19 HREF=files_handle.html#SECTION0006300000000000000> <b>Inspecting, displaying and sorting an MDL model</b></A>
+<LI> <A NAME=tex2html20 HREF=files_handle.html#SECTION0006400000000000000> <b>The various uses of an MDL model</b></A>
+</UL> 
+<LI> <A NAME=tex2html21 HREF=files_handle.html#SECTION0007000000000000000> <b>Overview
+of interactions with a WMP file</b></A>
+<UL> 
+<LI> <A NAME=tex2html22 HREF=files_handle.html#SECTION0007100000000000000> <b>Creating maps in WMP files</b></A>
+<LI> <A NAME=tex2html23 HREF=files_handle.html#SECTION0007200000000000000> <b>Inspecting the contents of a WMP file</b></A>
+<LI> <A NAME=tex2html24 HREF=files_handle.html#SECTION0007300000000000000> <b>Operations on WMP images</b></A>
+<LI> <A NAME=tex2html25 HREF=files_handle.html#SECTION0007400000000000000> <b>.LOG files</b></A>
+<LI> <A NAME=tex2html26 HREF=files_handle.html#SECTION0007500000000000000> <b>.PLT files</b></A>
+<LI> <A NAME=tex2html27 HREF=files_handle.html#SECTION0007600000000000000> <b>.NGI files</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000> <b><i>NEWSTAR </i> data and ancillary file types</b></A></H1>
+<P>
+The <i>NEWSTAR </i> programs recognize three major types of data files, which are identified by their extension:  
+<BR><BR>.SCN files: uv-data and uv-model  
+<BR>.MDL files: SELFCAL source model  
+<BR>.WMP files: maps of various kinds
+<P>
+<i>NEWSTAR </i> programs also produce a number of ancillary files, with the following extensions (the list may no longer be complete):  
+<BR><BR>.PLT-files: to be plotted  
+<BR>.LOG-files: to be printed  
+<BR>.NGF-files: produced by NGALC  
+<BR>.MNG-files: used to make plots with the MONGO package
+<P>
+        The relations between these files and the <i>NEWSTAR </i> programs are shown in <A HREF=" #.newstar.overview">figure</A>.
+<P>
+<A NAME=.newstar.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  Overview of the Newstar programs and data files and their interrelations. For information on entities in this diagram see <BR><A HREF="../fig/newstar_overview.ps"><STRONG>FIGURE</STRONG></A> 
+ <i><BR>programs  
+  <A HREF="../ncalib_descr/ncalib_descr.html"><b>NCALIB</b></A>,  
+  <A HREF="../nmap_descr/nmap_descr.html"><b>NMAP</b></A>,  
+  <A HREF="../nscan_descr/nscan_descr.html"><b>NSCAN</b></A> <BR>files 
+  <A HREF="../scn_file/scn_file.html"><b>.SCN file</b></A>,  
+  <A HREF="../wmp_descr/wmp_descr.html"><b>.WMP file</b></A>, 
+  <A HREF="../mdl_descr/mdl_descr.html"><b>.MDL file</b></A> </i>
+<P>
+<A NAME=.nodes><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>Directories and nodes (files)</b></A></H1>
+<P>
+        For historical reasons, the <i>NEWSTAR </i> programs refer to data files as <b>nodes</b> in a <b>database</b>.  In fact, they are just files in a directory.  Users are recommended to use a separate sub-directory for each data reduction project.
+<P>
+        However, although they refer to the same thing, there is a slight difference between <b>node names</b> used by the user and the actual <b>file names</b>: Node names are a series of alpha-numeric character strings separated by dots, e.g.:
+<P>
+ <PRE> 
+    mynode 
+    mynode.21cm.yesterday.s.x.c.d.file.dd 
+</PRE>
+<P>
+The maximum length of a node name is 80 characters (which means maximally 39
+dots). This is converted to a <em>file name</em> by: 
+<BR>- appending the extension (.SCN, .MDL or .WMP), <BR>- converting all dots (.) to underscores (_), <BR>- converting all lowercase to uppercase, 
+- replacing the underscore nearest but less than 47 to a dot. (?) <BR><BR>This file name is then prefixed with the current database (default nothing).
+<P>
+        Parts of a node name can be set aside for short-hand use.  This can be
+done by the INFIX keyword (see COMMON keywords), or in a node specification by
+enclosing a part in parenthesis ().  This enclosed part will from then on be
+available to all programs that are run in <b>the current stream</b>.  Reference
+to `the infix' is made by typing a #, e.g.:
+<P>
+ <PRE> 
+    mynode.21(cm.yesterday.s.x.c.d.file.d)d 
+</PRE>
+<P>
+Typing <tt>mynode.92#e</tt> will then produce <tt>mynode.92cm.yesterday.s.x.c.d.file.de</tt>
+<P>
+The database (directory) name can also be included in the node definition:
+<P>
+ <PRE> 
+    wnb/data/mynode 
+    ../other/mynode.21cm.yesterday.s.x.c.d.file.dd 
+</PRE>
+<P>
+        If a database is specified in this way, it will be saved in such a way
+that all subsequent program runs <b>in the same stream</b> that have no explicit
+database specified, will use it, including the currently running program at all
+its further node questions.
+<P>
+<H1><A NAME=SECTION0004000000000000000> <b>The <i>NEWSTAR </i> data files (SCN, MDL, WMP)</b></A></H1>
+<P>
+        These three <i>NEWSTAR </i> data files are each described in detail in their
+own `File Description' chapter in this Handbook.  In this Overview section, it
+is explained how the basic units (called Sets) in such a file can be selected
+individually or in groups.  For each of the three data files, an overview is
+given of the various ways in which the user may interact with these `objects',
+with references to the relevant program options.
+<P>
+<A NAME=data.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000> <b>Data file logical organisation: Sets</b></A></H2>
+<P>
+        The three main <i>NEWSTAR </i> data file (node) types are logically organised
+in the same way: they consist of a number of basic units called `Sets', which
+can be selected by the user in two ways:
+<P>
+<UL><LI> 
+        By <b>direct reference</b> to an absolute set index: <tt>#ir</tt> selects
+set nr <tt>ir</tt>, in which <tt>ir</tt> can be a range of contiguous sets (see
+below).  Direct reference is only useful if the user knows exactly how the
+various Sets are ordered in the file.
+<P>
+<LI> 
+        By <b>indexed reference</b> to a series of indices that represent
+parameters like map or channel nr.  A `selector' consists of a series on
+integer indices, separated by points.  The indices may also be specified as
+ranges of indices or wildcards (<IMG ALIGN=BOTTOM ALT="" SRC="_7567_tex2html_wrap362.png">).  For instance: <tt>ir1.ir2.*.ir4</tt>
+selects all Sets with index values in the indicated ranges. 
+</UL>
+<P>
+        <b>Index ranges</b> (<tt>ir</tt>) can take the following forms <b>(NB: 
+Indices start at 0!)</b>:
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_12969_tabular150.png"><P>
+<P>
+<A NAME=loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000> <b>Using loops</b></A></H2>
+<P>
+        Sometimes a program must be run more than once for the same 
+SCN-file, but for different Sets.  In that case, the <b>LOOPS</b> keyword can
+used to specify subsequent ranges of Sets.  A loop is specified by means of a
+pair of values: The first value indicates how often the loop should execute,
+the second specifies an increment to be given to the Set specification at each
+run.
+<P>
+        For example: <tt>loops=3,..2</tt> indicates that the program has to run
+three times, each time incrementing the 3rd Set index by 2.  So, if the first 
+Set (selected with the keyword SETS) was <tt>0.0-3.2.5.*</tt>, the program will be
+run three times, for the Sets
+<P>
+ <PRE> 
+   0.0-3.2.5.*.
+   0.0-3.4.5.*.
+   0.0-3.6.5.*.
+</PRE>
+<P>
+<b>Nested loops</b> can be specified by stringing loop definitions (pairs of
+values) together.  For instance: <tt>loops=3,..2,5,...3</tt> adds an inner loop of 
+5 program runs in which the 4th Set index is incremented by 3 each time:
+<P>
+ <PRE> 
+   0.0-3.2.5.*.   0.0-3.2.8.*.   0.0-3.2.11.*.
+                  0.0-3.2.14.*.   0.0-3.2.17.*.
+   0.0-3.4.5.*.   0.0-3.4.8.*.   0.0-3.4.11.*.
+                  0.0-3.4.14.*.   0.0-3.4.17.*.
+   0.0-3.6.5.*.   0.0-3.6.8.*.   0.0-3.6.11.*.
+                  0.0-3.6.14.*.   0.0-3.6.17.*.
+</PRE>
+<P>
+<A NAME=scn><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>Overview of interactions with the SCN file</b></A></H1>
+<P>
+        The SCN-file contains uv-data, and possibly the uv-representation of a
+source model.  A single SCN-file may contain uv-data of different (but related)
+observations.
+<P>
+        For more information, see the dedicated SCN-file section in this
+chapter of the Handbook, and also the section on the program NSCAN.  It
+contains a description of the structure and the contents of the 
+SCN-file.
+<P>
+<A NAME=scn.create><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005100000000000000> <b>Creating SCN files</b></A></H2>
+<P>
+- From WSRT circle files: NSCAN option LOAD. <BR>- From ATCA (Australia Telescope Compact Array) files: NATNF.<BR>- From old (R-series) SCN-files: NSCAN option FROM_OLD.<BR>- Simulated uv-data: NSIMUL? (not implemented yet).<BR><A NAME=scn.inspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000> <b>Inspecting the contents of a SCN file</b></A></H2>
+<P>
+- File Layout: NSCAN option SHOW<BR>- File header: NSCAN option SHOW<BR>- Set headers: NSCAN option SHOW<BR> - Telescope (dipole) angle/ellipt corr: NCALIB option POLAR 
+SHOW<BR>- Scan headers: NSCAN option SHOW<BR> - Telescope gain/phase corr: NCALIB option SHOW<BR>- uv-data (corrected, converted): NSCAN option SHOW<BR>- Display of (gridded) uv-data or uv-model: See WMP file below.<BR>- Plot telescope gain/phase corr (REDC+ALGC+OTHC): NPLOT option TELESCOPE<BR>- Plot Redundancy/Selfcal residuals: NPLOT option RESIDUAL<BR>- Plot uv-data or uv-model: NPLOT option DATA or MODEL<BR>- Print average telescope gain/phase corr (R+A+O): NCALIB option SHOW<BR>- Extract various astrophysical info: NGCALC<BR><A NAME=scnt><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005300000000000000> <b>Editing the header information of a SCN file</b></A></H2>
+<P>
+        Almost every value (observation parameters, corrections, etc) in the 
+SCN-file headers may be edited manually by means of NSCAN option 
+SHOW EDIT.  This means that, even if there is no specific <i>NEWSTAR </i> routine to
+change something, it can always be done by hand.  This may be laborious in some
+cases, <em>but at least it is possible!</em>.  This feature is particularly useful
+in those (rare) cases where erroneous information has somehow been put in the
+header during the observations in Westerbork.
+<P>
+<A NAME=scn.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005400000000000000> <b>Applying corrections to uv-data</b></A></H2>
+<P>
+        In general, uv-data in a SCN-file is <em>never physically modified</em>. 
+Corrections may be applied (or de-applied) to the uv-data whenever the data is
+read into memory to be processed.  The user may specify which corrections are
+applied (or de-applied) by specifying the value of the general <i>NEWSTAR </i>
+keywords APPLY and DE_APPLY, which are used by all <i>NEWSTAR </i> programs that
+handle uv-data.  Use <tt>dws NGEN</tt> 
+(see Common features of <i>NEWSTAR </i> programs).
+<P>
+<A NAME=scn.modify><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005500000000000000> <b>Modyfing the stored corrections</b></A></H2>
+<P>
+<b>Zeroeing</b> selected corrections: NCALIB option SET ZERO
+<P>
+<b>Set Header</b> (corrections that are `constant' in time):<BR>- Any value: NSCAN option SHOW EDIT<BR>- POLC (dipole angle error and ellipticity corr):<BR> - Estimation: NCALIB option POLAR CALC<BR> - Manual: NCALIB option POLAR SET, EDIT, ZERO<BR> - Copying from calibrator: NCALIB option POLAR COPY<BR><b>Scan Header</b> (corrections that vary per HA):<BR>- Any value: NSCAN option SHOW EDIT<BR>- Telescope (dipole) gain/phase corr:<BR> - Estimation: NCALIB option REDUN <BR> - Redundancy (no model): REDC<BR> - Align: ALGC<BR> - Selfcal ALGC<BR> - Manual: NCALIB option SET MANUAL, ZERO, RENORM <BR> - Copying from calibrator: NCALIB option SET COPY, CCOPY, LINE<BR>- Phase Zero Difference: OTHC<BR> - Estimation: NCALIB option POLAR VZERO CALC, APPLY, ASK, SCAN <BR> - Manual: NCALIB option POLAR VZERO MANUAL, ASK<BR> - Copying from calibrator: NCALIB option POLAR VZERO COPY<BR>- Extinction corr (manual): NCALIB option SET EXTINCT<BR>- Refraction corr (manual): NCALIB option SET REFRACT<BR>- Faraday corr (input of ionosonde data): NCALIB option SET FARADAY<BR><A NAME=scn.uvmodel><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005600000000000000> <b>Modifying a uv-model in the SCN-file</b></A></H2>
+<P>
+        See Overview of interactions with MDL file below.
+<P>
+<A NAME=scn.reorg><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005700000000000000> <b>Reorganisation of SCN files</b></A></H2>
+<P>
+- Create new `Job' from Sets in the same SCN-file: NSCAN option REGROUP<BR>- Create a `secondary' SCN-file (data selection, correction): NCOPY<BR>(not implemented yet)<BR>- Delete SCN-file: Use UNIX command <tt>rm &lt;xxx&gt;.SCN</tt> (be careful!)<BR><A NAME=scn.export><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005800000000000000> <b>Export of uv-data from SCN files</b></A></H2>
+<P>
+- To UVFITS format (AIPS): NSCAN option UVFITS, PFITS<BR>- To old (R-series) SCN-file format: NSCAN option TO_OLD<BR>- To WMP file (as gridded uv-data or maps): NMAP option MAKE<BR><A NAME=mdl.inter><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000> <b>Overview of interactions with an MDL file</b></A></H1>
+<P>
+        A MDL file contains a collection of source model components. 
+This may consist of a mixture of <b>multi-parameter components</b> and ordinary
+<b>CLEAN components</b>.  The MDL file may also contain <b>reference
+coordinates</b> (obtained from a SCN-file) for the position of the field centre
+and the observing frequency.
+<P>
+        For more information, see the dedicated MDL-file section in this
+chapter of the Cookbook, and also the section on the program NSCAN.  It
+contains a description of the structure and the contents of the 
+MDL-file.
+<P>
+        NOTE: Note that the model in the MDL file may be manipulated by means
+of NMODEL <b>options</b> (i.e.  options of the program NMODEL), or by MDL <b>handles</b>.  The latter operations (e.g.  READ, WRITE, EDIT, 
+SHOW) are available in all the programs that deal with source models: 
+NCALIB, NMAP, NCLEAN, NSCAN, NMODEL.
+<P>
+<A NAME=mdl.generate><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006100000000000000> <b>Adding source components to an MDL file</b></A></H2>
+<P>
+- Manual, by specifying source parameters: MDL handle ADD.<BR>- Automatic search of a map (in a WMP file): NMODEL action FIND<BR>- CLEANing a map (in a WMP file): NCLEAN option BEAM, UVCOVER, COMPON<BR>- Save model from SCN file in an MDL file: NMODEL option SAVE<BR>- Convert old (R-series) model to <i>NEWSTAR </i> MDL file format.<BR><A NAME=mdl.modify><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006200000000000000> <b>Modifying a model in an MDL file</b></A></H2>
+<P>
+Modifying <b>source components</b>:<BR>- Improve source parameters by fitting to the uv-data: 
+                NMODEL option UPDATE, XUPDATE<BR>- Manual editing: MDL handle EDIT, FEDIT<BR>- Delete:<BR> - All components: MDL handle CLEAR, ZERO<BR> - Selected components: 
+                MDL handle DELETE, DNCLOW, DCLOW, DAREA<BR> - Selected components: MDL handle EDIT, FEDIT<BR>- Calibrate (position, flux): MDL handle CALIB<BR>- Combine components at the same position: MDL handle MERGE<BR>- Correct for primary beam attenuation: NMODEL option BEAM, DEBEAM<BR>Modifying <b>reference coordinates</b>:<BR>- Change epoch or coordinate system: NMODEL option CONVERT<BR>NB: Reference position and frequency are obtained from SCN-file.<BR><A NAME=mdlspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006300000000000000> <b>Inspecting, displaying and sorting an MDL model</b></A></H2>
+<P>
+Inspecting:<BR>- Show list of components: MDL handle SHOW (screen) or PRINT (log-file)<BR>- Idem, in RA/DEC coordinates: MDL handle RSHOW, RLIST<BR>- Show source list statistics: MDL handle TOT <BR>Displaying:<BR>- As gridded uv-model from SCN file: See WMP file below<BR>- As a map of the uv-model in the SCN-file: See WMP file below<BR>- As position markers in a map: NPLOT option MAP<BR>- As `restored' components in a CLEAN residual map: NCLEAN option UREST <BR>Sorting:<BR>- According to decreasing flux: MDL handle SORT, WRITE(!)<BR>- According to the value of another source parameter: MDL handle FSORT<BR>subsectionRelation with the uv-model in the .SCN file 
+<A NAME=mdl.uvmodel><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P>
+        The source components in an MDL file may be Fourier transformed to the
+uv-plane, to the uv-coordinates of the uv-data in a SCN-file. 
+This <b>uv-model</b> is then `saved' in the SCN-file, together with a copy of
+the MDL source components that produced it.
+<P>
+        Whenever a uv-model is needed (e.g.  for Selfcal in NCALIB, or source
+subtraction in NMAP) the user is always asked to specify a <b>input model</b>
+explicitly, even if there is already a <b>saved uv-model</b> in the SCN-file. 
+This input model may be specified either by reading 
+(and editing) components from an MDL-file, or by editing source components
+manually.  In the following, the Fourier transform of the input model will be
+called the <b>input uv-model</b>.  The user may choose (keyword MODEL_ACTION)
+one of the following possibilities:
+<P>
+- <b>Merge:</b> Replace the saved uv-model with the input uv-model, 
+        and use it. <BR>- <b>Add:</b> Add the input uv-model to the saved uv-model in the SCN-file, 
+        and use it.<BR>- <b>New:</b> Replace the saved uv-model in the SCN file by the input uv-model, 
+        and use it.<BR>- <b>Temporary:</b> Use the input uv-model, 
+        but do not change the saved uv-model in the SCN-file.<BR>- <b>Increment:</b> Use the sum of the saved uv-model and the input uv-model, 
+        but do not change the saved uv-model in the SCN-file. <BR>NOTE: <i>NEWSTAR </i> regards the saved uv-model as <em>applied corrections</em>,
+i.e.  corrections that were applied (added) to the cosmic noise before the
+uv-data were put into the SCN file.  Hence, to subtract the saved uv-model from
+the data, one could specify `MOD' to the (NGEN) keyword DE_APPLY! Specifying
+`MOD' to the (NGEN) keyword APPLY will restore a model that was subtracted from
+the data before it was put in the SCN file (?).
+<P>
+<A NAME=mdl.uses><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006400000000000000> <b>The various uses of an MDL model</b></A></H2>
+<P>
+<b>Present uses</b> of an MDL model:<BR>- To solve for telescope gain/phase errors (Selfcal, Align): 
+        NCALIB option REDUN<BR>- To subtract sources from the uv-data: NMAP option MAKE<BR>- To combine multiple observations:<BR> - With different frequencies (broad-band mapping)<BR> - With different pointing centres (mosaicking)<BR> - With different observing times<BR>- To deal with instrumental polarisation<BR>- To undo large Faraday `rotation measures'<BR>- To detect variability <BR>- To simulate uv-data: clumsy at the moment<BR><b>Potential uses</b> of an MDL model:<BR>- To deal with non-isoplanaticity<BR>- To simulate uv-data: NSIMUL (not yet implemented)<BR><A NAME=wmpter><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0007000000000000000> <b>Overview
+of interactions with a WMP file</b></A></H1>
+<P>
+        A WMP file contains a collection of 2-dimensional arrays, that are
+related in some way (but that can have different dimensions).  These may be
+maps for various frequencies (line data) or pointing centres 
+(mosaicking), antenna patterns and CLEAN residual maps.  Even rectangular
+arrays of (gridded) uv-data may be put in a WMP file, for display purposes.
+<P>
+        For more information, see the dedicated WMP-file section in this
+chapter of the Cookbook, and also the section on the program NSCAN.  It
+contains a description of the structure and the contents of the 
+WMP-file.
+<P>
+<A NAME=wmp.create><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007100000000000000> <b>Creating maps in WMP files</b></A></H2>
+<P>
+- Making maps/ap's from uv-data (or uv-model) in SCN-file: NMAP option MAKE<BR> - Many types of maps: 
+XX,YY,XY,YX,I,Q,U,V,cos,sin,ampl,phase,...<BR>- Residual maps: NCLEAN option BEAM, UVCOVER<BR>- Restored maps: NCLEAN option UREST<BR>- Gridded uv-data from SCN-file: NMAP option MAKE REAL, IMAG, AMPL, PHASE<BR> - In various forms: real or imaginary parts,ampl,phase,...<BR>- Gridded uv-coverage from SCN-file: NMAP option MAKE COVER<BR>- Copy maps: NMAP option FIDDLE COPY<BR>- Extract areas from maps: NMAP option FIDDLE EXTRACT<BR>- Convert from old (R-series) map files: NMAP option FROM_OLD<BR><b>Delete</b> WMP files: 
+Use operating system UNIX: <tt>rm &lt;....&gt;.WMP</tt> (be careful!)
+<P>
+<A NAME=wmpspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007200000000000000> <b>Inspecting the contents of a WMP file</b></A></H2>
+<P>
+- Show header information: NMAP option SHOW.<BR>- Display images on color screen (X): NGIDS<BR>- Make plots on X-screen or plotter: NPLOT option MAP 
+ - Various types: contour, greyscale, polar, ruled surface<BR>subsectionEditing the WMP header information 
+<A NAME=wmp.edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P>
+- Edit header information: NMAP option SHOW.<BR><A NAME=wmp.oper><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007300000000000000> <b>Operations on WMP images</b></A></H2>
+<P>
+        Although <i>NEWSTAR </i> has primarily been designed for WSRT <em>uv-data</em>
+processing it offers some powerful image-plane features:
+<P>
+- Various map operations (very powerful): NMAP option FIDDLE<BR> - Add, subtract, average, extract, copy, mosaic, etc<BR>- Cleaning and restoring: NCLEAN option BEAM, UREST<BR>- Finding strong sources: NMODEL option FIND<BR>For many astrophysical projects, this will be sufficient. 
+However, for moreadvanced operations astrophysical image analysis, the user
+should transfer the images from the WMP file to other packages 
+(e.g.  GIPSY, AIPS) by means of the FITS format: NMAP option W16FITS, 
+W32FITS.
+<P>
+<A NAME=log><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007400000000000000> <b>.LOG files</b></A></H2>
+<P>
+        Each <i>NEWSTAR </i> program run produces a log-file, with the name <tt>&lt;progname&gt;.LOG</tt>.  It contains the `vital information' about the program run:
+keyword values (including the hidden ones) and essential results.  In some
+cases (e.g.  NCALIB REDUN), the user may specify how much information is
+printed in the log-file (keyword SHOW_LEVEL).
+<P>
+        The user may specify (NGEN keyword LOG) what happens with the log-file
+upon completion: it may be spooled automatically to the line printer, or thrown
+away, or kept for later inspection.  In the latter case, the log-file is
+automatically renamed with a unique name (e.g. <tt>NCA&lt;alphanumeric&gt;.LOG</tt>)
+when the program is run again.
+<P>
+<A NAME=plt><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007500000000000000> <b>.PLT files</b></A></H2>
+<P>
+        All plot files produced by the programs NPLOT and NGCALC have the
+extension .PLT.  The file names usually begin with the 3-4 letter code of the
+selected PLOTTER option (PSP, PAL, EMS etc), followed by a unique combination
+of alphanumeric characters derived from the date and time of creation.
+<P>
+<A NAME=ngi><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0007600000000000000> <b>.NGI files</b></A></H2>
+<P>
+        NGI files are used to store the various information that the program 
+NGCALC extracts from the SCN-file.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/files_handle/images.pl b/files_handle/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..992e44baff69731c95addce80c99621551516bd2
--- /dev/null
+++ b/files_handle/images.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{tabular}<<151>>ll<<151>><<152>>bfint<<152>>;html_special_mark_amp;singleindexvalueatthislevel<<153>>bf<<367>><<367>>$ast$<<368>><<368>><<153>>;html_special_mark_amp;wildcard:allpossibleindexvaluesatthislevel<<154>>bfint-<<154>>;html_special_mark_amp;allindexvaluesatthislevel,startingat`int'<<155>>bfint1-int2[:int3]<<155>>;html_special_mark_amp;indexvalues`int1'through`int2'bystep`int3'(dflt=1)<<156>>bfint1:int3<<156>>;html_special_mark_amp;interpretedasint1-<<369>><<369>>$ast$<<370>><<370>>:int3<<157>>bfomitted<<157>>;html_special_mark_amp;inthemiddle:interpretedas<<371>><<371>>$.ast$<<372>><<372>>(<<373>><<373>>$..equiv.ast.$<<374>><<374>>)<<158>>bfomitted<<158>>;html_special_mark_amp;atthe:interpretedas<<375>><<375>>$.ast$<<376>><<376>>(<<377>><<377>>$..2equivast.ast.2.ast.ast.ast$<<378>><<378>>){tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12969_tabular150.xbm">'; 
+$key = q/{tabular}<<150>>ll<<150>><<151>>bfint<<151>>;html_special_mark_amp;singleindexvalueatthislevel<<152>>bf<<364>><<364>>$ast$<<365>><<365>><<152>>;html_special_mark_amp;wildcard:allpossibleindexvaluesatthislevel<<153>>bfint-<<153>>;html_special_mark_amp;allindexvaluesatthislevel,startingat`int'<<154>>bfint1-int2[:int3]<<154>>;html_special_mark_amp;indexvalues`int1'through`int2'bystep`int3'(dflt=1)<<155>>bfint1:int3<<155>>;html_special_mark_amp;interpretedasint1-<<366>><<366>>$ast$<<367>><<367>>:int3<<156>>bfomitted<<156>>;html_special_mark_amp;inthemiddle:interpretedas<<368>><<368>>$.ast$<<369>><<369>>(<<370>><<370>>$..equiv.ast.$<<371>><<371>>)<<157>>bfomitted<<157>>;html_special_mark_amp;atthe:interpretedas<<372>><<372>>$.ast$<<373>><<373>>(<<374>><<374>>$..2equivast.ast.2.ast.ast.ast$<<375>><<375>>){tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7567_tabular149.xbm">'; 
+$key = q/{}$ast${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7567_tex2html_wrap362.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/files_handle/labels.pl b/files_handle/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..d6598eee9002a93c90038d9d4b273e0d2466590f
--- /dev/null
+++ b/files_handle/labels.pl
@@ -0,0 +1,33 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"mdl.uvmodel"} ="$URL/files_handle.html"; 
+$external_labels{"scn.inspect"} ="$URL/files_handle.html"; 
+$external_labels{"ngi"} ="$URL/files_handle.html"; 
+$external_labels{"loops"} ="$URL/files_handle.html"; 
+$external_labels{"scn.uvmodel"} ="$URL/files_handle.html"; 
+$external_labels{".contents"} ="$URL/files_handle.html"; 
+$external_labels{"plt"} ="$URL/files_handle.html"; 
+$external_labels{"scn.apply"} ="$URL/files_handle.html"; 
+$external_labels{"mdlspect"} ="$URL/files_handle.html"; 
+$external_labels{"scn.export"} ="$URL/files_handle.html"; 
+$external_labels{"scn"} ="$URL/files_handle.html"; 
+$external_labels{"scn.reorg"} ="$URL/files_handle.html"; 
+$external_labels{"mdl.uses"} ="$URL/files_handle.html"; 
+$external_labels{"wmpter"} ="$URL/files_handle.html"; 
+$external_labels{"wmp.oper"} ="$URL/files_handle.html"; 
+$external_labels{"wmp.edit"} ="$URL/files_handle.html"; 
+$external_labels{".nodes"} ="$URL/files_handle.html"; 
+$external_labels{"mdl.modify"} ="$URL/files_handle.html"; 
+$external_labels{"scn.create"} ="$URL/files_handle.html"; 
+$external_labels{"scnt"} ="$URL/files_handle.html"; 
+$external_labels{"scn.modify"} ="$URL/files_handle.html"; 
+$external_labels{"log"} ="$URL/files_handle.html"; 
+$external_labels{"wmp.create"} ="$URL/files_handle.html"; 
+$external_labels{"data.sets"} ="$URL/files_handle.html"; 
+$external_labels{"wmpspect"} ="$URL/files_handle.html"; 
+$external_labels{"mdl.generate"} ="$URL/files_handle.html"; 
+$external_labels{"mdl.inter"} ="$URL/files_handle.html"; 
+$external_labels{".newstar.overview"} ="$URL/files_handle.html"; 
+
+1;
\ No newline at end of file
diff --git a/flfnode/flfnode__flf_node.html b/flfnode/flfnode__flf_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..49d5a8217e7a20e444fb1f6f170b37428ea1b16b
--- /dev/null
+++ b/flfnode/flfnode__flf_node.html
@@ -0,0 +1,18 @@
+<TITLE>Description of FLF_NODE (FLFNODE)</TITLE>
+<H1>Description of general keyword FLF_NODE</H1>
+
+<DT><EM>Prompt:</EM> Input/output .FLF file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (no extension). <P>
+You may enter <P>
+	[&lt;directory&gt;/]** <P>
+to get a list of .SCN files in your current or another directory; then enter <P>
+	#&lt;n&gt; <P>
+to select the &lt;n&gt;'th file from that list. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../flfnode/flfnode_comm.html">List of general keywords</A> for FLFNODE
+<LI>Description of the <A HREF="../flf_descr/flf_descr.html">FLF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/flfnode/flfnode__input_flf_node.html b/flfnode/flfnode__input_flf_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..2b661d073f202a93b2538471f27362d9bf20b5f8
--- /dev/null
+++ b/flfnode/flfnode__input_flf_node.html
@@ -0,0 +1,18 @@
+<TITLE>Description of INPUT_FLF_NODE (FLFNODE)</TITLE>
+<H1>Description of general keyword INPUT_FLF_NODE</H1>
+
+<DT><EM>Prompt:</EM> Input .FLF file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (no extension). <P>
+You may enter <P>
+	[&lt;directory&gt;/]** <P>
+to get a list of .SCN files in your current or another directory; then enter <P>
+	#&lt;n&gt; <P>
+to select the &lt;n&gt;'th file from that list. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../flfnode/flfnode_comm.html">List of general keywords</A> for FLFNODE
+<LI>Description of the <A HREF="../flf_descr/flf_descr.html">FLF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/flfnode/flfnode__output_flf_node.html b/flfnode/flfnode__output_flf_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..08b62715cf31acd53e1e1eba5d43c7549f6e3579
--- /dev/null
+++ b/flfnode/flfnode__output_flf_node.html
@@ -0,0 +1,18 @@
+<TITLE>Description of OUTPUT_FLF_NODE (FLFNODE)</TITLE>
+<H1>Description of general keyword OUTPUT_FLF_NODE</H1>
+
+<DT><EM>Prompt:</EM> Output .FLF file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (no extension). <P>
+You may enter <P>
+	[&lt;directory&gt;/]** <P>
+to get a list of .SCN files in your current or another directory; then enter <P>
+	#&lt;n&gt; <P>
+to select the &lt;n&gt;'th file from that list. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../flfnode/flfnode_comm.html">List of general keywords</A> for FLFNODE
+<LI>Description of the <A HREF="../flf_descr/flf_descr.html">FLF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/flfnode_comm/flfnode_comm.html b/flfnode_comm/flfnode_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..42f6ff125a76e1c24ef7d47447353a9ff32748d7
--- /dev/null
+++ b/flfnode_comm/flfnode_comm.html
@@ -0,0 +1,20 @@
+<TITLE>Index of general keywords from FLFNODE</TITLE>
+<H1>Description of general keywords (FLFNODE)</H1>
+
+<UL>
+<LI> <A HREF="../flfnode/flfnode__flf_node.html">
+  FLF_NODE</A>
+  Input/output .FLF file name
+<LI> <A HREF="../flfnode/flfnode__input_flf_node.html">
+  INPUT_FLF_NODE</A>
+  Input .FLF file name
+<LI> <A HREF="../flfnode/flfnode__output_flf_node.html">
+  OUTPUT_FLF_NODE</A>
+  Output .FLF file name
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
diff --git a/flfnode_public_intfc.ps b/flfnode_public_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..2a21e422c98701c2eff0a59ae4f2c561fbdccba7
--- /dev/null
+++ b/flfnode_public_intfc.ps
@@ -0,0 +1,361 @@
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+(terfaces)935 2995 y Fc(1)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/flfnode_public_intfc/flfnode_public_intfc.html b/flfnode_public_intfc/flfnode_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..f83c4c68c9df4b0590302ba37c92f3a9ea42d60e
--- /dev/null
+++ b/flfnode_public_intfc/flfnode_public_intfc.html
@@ -0,0 +1,77 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group FLFNODE</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=flfnode_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=flfnode_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=flfnode_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=flfnode_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group FLFNODE, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/flfnode_public_intfc/images.pl b/flfnode_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/flfnode_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/flfnode_public_intfc/labels.pl b/flfnode_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..c3f248f0022f650d7e8073c0f06f0822e853c7a6
--- /dev/null
+++ b/flfnode_public_intfc/labels.pl
@@ -0,0 +1,8 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/flfnode_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/flfnode_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/flfnode_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/global/global__channel.html b/global/global__channel.html
new file mode 100644
index 0000000000000000000000000000000000000000..b5dcdd78c7c030367a43fac90c235720454b4645
--- /dev/null
+++ b/global/global__channel.html
@@ -0,0 +1,15 @@
+<TITLE>Description of CHANNEL (GLOBAL)</TITLE>
+<H1>Program GLOBAL: private keyword CHANNEL</H1> 
+
+<DT><EM>Prompt:</EM> &lt;DeAnza Imagechannel Nr&gt;
+<DT><EM>Expected input:</EM> I; min.value: 0.000000; max.value: 2.000000.<P>
+Defines the image-channel on the DeAnza image-processor <P>
+	Channel 0 is used as overlay-channel and should (unless necessary) 
+	not be used <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../global/global_keys.html">List of keywords</A> for GLOBAL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../global_descr/global_descr.html">program GLOBAL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/global/global__database.html b/global/global__database.html
new file mode 100644
index 0000000000000000000000000000000000000000..ff9a8108903fb5b1e8c1f6684decfa8b3ccac400
--- /dev/null
+++ b/global/global__database.html
@@ -0,0 +1,14 @@
+<TITLE>Description of DATABASE (GLOBAL)</TITLE>
+<H1>Program GLOBAL: private keyword DATABASE</H1> 
+
+<DT><EM>Prompt:</EM> &lt;DATA BASE NAME&gt;
+<DT><EM>Expected input:</EM> Character(80).<P>
+Defines the name of the delault database, which all programs will use unless <P>
+	prompting is forced through the /ASK qualifier <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../global/global_keys.html">List of keywords</A> for GLOBAL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../global_descr/global_descr.html">program GLOBAL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/global/global__ipunit.html b/global/global__ipunit.html
new file mode 100644
index 0000000000000000000000000000000000000000..3239dec03e8c85adbe1e0623c1e38291643a96cf
--- /dev/null
+++ b/global/global__ipunit.html
@@ -0,0 +1,15 @@
+<TITLE>Description of IPUNIT (GLOBAL)</TITLE>
+<H1>Program GLOBAL: private keyword IPUNIT</H1> 
+
+<DT><EM>Prompt:</EM> &lt;DeAnza-Unitnr&gt;
+<DT><EM>Default:</EM> 0 /NOASK.
+<DT><EM>Expected input:</EM> I; min.value: 0.000000; max.value: 0.000000.<P>
+Defines the unitnr of the DeAnza image-processor <P>
+	0 is the DeAnza in the image-room <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../global/global_keys.html">List of keywords</A> for GLOBAL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../global_descr/global_descr.html">program GLOBAL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/global/global__lutnr.html b/global/global__lutnr.html
new file mode 100644
index 0000000000000000000000000000000000000000..1122ebd79a6ada03386bab256968102e3736cfe2
--- /dev/null
+++ b/global/global__lutnr.html
@@ -0,0 +1,16 @@
+<TITLE>Description of LUTNR (GLOBAL)</TITLE>
+<H1>Program GLOBAL: private keyword LUTNR</H1> 
+
+<DT><EM>Prompt:</EM> &lt;Colour Lookup-Table Nr&gt;
+<DT><EM>Default:</EM> 0 /NOASK.
+<DT><EM>Expected input:</EM> I; min.value: 0.000000; max.value: 3.000000.<P>
+Defines the nr of the colour lookup-table, which drives the colours <P>
+on the screen. 
+	0 should normally be used <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../global/global_keys.html">List of keywords</A> for GLOBAL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../global_descr/global_descr.html">program GLOBAL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/global/global__tapeunit.html b/global/global__tapeunit.html
new file mode 100644
index 0000000000000000000000000000000000000000..75cc15455205be199ed6da3d40372511dba26845
--- /dev/null
+++ b/global/global__tapeunit.html
@@ -0,0 +1,15 @@
+<TITLE>Description of TAPEUNIT (GLOBAL)</TITLE>
+<H1>Program GLOBAL: private keyword TAPEUNIT</H1> 
+
+<DT><EM>Prompt:</EM> MTA0, MTB0
+<DT><EM>Expected input:</EM> Character(4).<P>
+Defines the tapeunit that have to be used <P>
+	MTA0 is the fast selfloading tapeunit 
+	MTB0 is the slower tapeunit (the left one) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../global/global_keys.html">List of keywords</A> for GLOBAL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../global_descr/global_descr.html">program GLOBAL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/global_keys/global_keys.html b/global_keys/global_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..6d60f1cff11d21daf22f961d0f7da9652f95b24f
--- /dev/null
+++ b/global_keys/global_keys.html
@@ -0,0 +1,27 @@
+<TITLE>Index of private keywords for GLOBAL </TITLE>
+<H1>Description of keywords for program GLOBAL</H1>
+
+<UL>
+<LI> <A HREF="../global/global__database.html">
+  DATABASE</A>
+  &lt;DATA BASE NAME&gt;
+<LI> <A HREF="../global/global__tapeunit.html">
+  TAPEUNIT</A>
+  MTA0, MTB0
+<LI> <A HREF="../global/global__ipunit.html">
+  IPUNIT</A>
+  &lt;DeAnza-Unitnr&gt;
+<LI> <A HREF="../global/global__channel.html">
+  CHANNEL</A>
+  &lt;DeAnza Imagechannel Nr&gt;
+<LI> <A HREF="../global/global__lutnr.html">
+  LUTNR</A>
+  &lt;Colour Lookup-Table Nr&gt;
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../global_descr/global_descr.html">program GLOBAL</A>
+</UL>
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diff --git a/global_private_intfc/global_private_intfc.html b/global_private_intfc/global_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..d3ac77e671b9b7c0903bf78b097a0f92e820ab1f
--- /dev/null
+++ b/global_private_intfc/global_private_intfc.html
@@ -0,0 +1,68 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The global control parameters of the NEWSTAR user interface</b>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=global_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=global_private_intfc.html#SECTION0002000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html3 HREF=global_private_intfc.html#SECTION0002100000000000000>  <b>References to public interfaces</b></A>
+</UL>
+</UL>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/global_private_intfc/images.pl b/global_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/global_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/global_private_intfc/labels.pl b/global_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..a2283117cfb7ba816f3db9ec3e474b904cf9baab
--- /dev/null
+++ b/global_private_intfc/labels.pl
@@ -0,0 +1,8 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/global_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/global_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/global_private_intfc.html"; 
+
+1;
\ No newline at end of file
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+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/hb_contents/hb_contents.html b/hb_contents/hb_contents.html
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>NEWSTAR documentation overview</b>
+<P>
+        <b>NOTE CAREFULLY: <em>Most of the documentation is not up-to-date in its details. Referencesthat <b>are</b> are shown in boldface. The others are left in place because theydo provide useful general information.</b></em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=hb_contents.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=hb_contents.html#SECTION0002000000000000000> <b>Introduction</b></A>
+<LI> <A NAME=tex2html3 HREF=hb_contents.html#SECTION0003000000000000000> <b>Data files</b></A>
+<LI> <A NAME=tex2html4 HREF=hb_contents.html#SECTION0004000000000000000> <b>Source models</b></A>
+<LI> <A NAME=tex2html5 HREF=hb_contents.html#SECTION0005000000000000000> <b>NEWSTAR Programs</b></A>
+<LI> <A NAME=tex2html6 HREF=hb_contents.html#SECTION0006000000000000000> <b>Bulk data: Batch processing</b></A>
+<LI> <A NAME=tex2html7 HREF=hb_contents.html#SECTION0007000000000000000> <b>Processing recipes</b></A>
+<LI> <A NAME=tex2html8 HREF=hb_contents.html#SECTION0008000000000000000> <b>Miscellaneous information</b></A>
+<LI> <A NAME=tex2html9 HREF=hb_contents.html#SECTION0009000000000000000> <b>Programmers' documentation</b></A>
+</UL>
+<H1><A NAME=SECTION0002000000000000000> <b>Introduction</b></A></H1>
+<P>
+<UL><LI>      <A HREF="../introduction/introduction.html"><b>Introduction</b></A> to Newstar for new and 
+        prospective users 
+<LI>      <A HREF="../make_model/make_model.html"><b>Source models</b></A> and their construction.  
+<LI>      <A HREF="../models_descr/models_descr.html">Models in Newstar</A>  
+<LI>      <A HREF="../introduction/introduction.html#.basic.functions"><b>Overview diagram</b></A> of programs 
+                and data files 
+</UL>
+<P>
+<H1><A NAME=SECTION0003000000000000000> <b>Data files</b></A></H1>
+<P>
+<UL><LI>      <A HREF="../file_indexing/file_indexing.html"><b>Indexing</b></A> and navigation 
+<LI>      Visibilities: The <A HREF="../scn_file/scn_file.html"><b>.SCN file</b></A> 
+  <UL><LI>    Data-structure definitions: 
+          <A HREF="../src/nscan/sth.dsc"><b>sector</b></A> header; 
+          <A HREF="../src/nscan/sch.dsc"><b>scan</b></A> header; 
+  </UL> 
+<LI>      Images: The <A HREF="../wmp_descr/wmp_descr.html">.WMP file</A> 
+  <UL><LI>    Data-structure definitions: 
+          <A HREF="../src/nmap/mph.dsc"><b>map</b></A> header 
+  </UL> 
+<LI>      Source model: The <A HREF="../mdl_descr/mdl_descr.html">.MDL file</A> 
+  <UL><LI>    Data-structure definitions: 
+  </UL> 
+<LI>      Low-level <A HREF="../show_edit/show_edit.html"><b>inspection/editing</b></A> of .SCN and .WMP 
+        files 
+<LI>      See also: The <A HREF="#.wsrt.tape"><b>WSRT tape</b></A> format. 
+</UL>
+<P>
+<H1><A NAME=SECTION0004000000000000000> <b>Source models</b></A></H1>
+<P>
+<UL><LI>      The <A HREF="../mdl_descr/mdl_descr.html">.MDL file</A> 
+<LI>      <A HREF="../make_model/make_model.html">Model-making</A>  
+<LI>     <A HREF="../models_descr/models_descr.html">Models in Newstar</A> 
+<LI>      <A HREF="../src/doc/txt/calibr_models.txt"><b>Calibrator models</b></A> <i>in Dutch</i> 
+</UL>
+<P>
+<H1><A NAME=SECTION0005000000000000000> <b>NEWSTAR Programs</b></A></H1>
+<P>
+<UL><LI>      <A HREF="../introduction/introduction.html#.programs"><b>Overview</b></A> of functionality 
+<LI>      The parameter interface: 
+  <UL><LI>    <A HREF="../introduction/introduction.html#.user.interface"><b>General</b></A> features common to all 
+        programs 
+  <LI>    <A HREF="../common_descr/common_descr.html">Advanced</A> common features 
+  </UL> 
+<LI>      NATNF: Descriptions of 
+        <A HREF="../natnf_private_intfc/natnf_private_intfc.html"><b>parameters</b></A>;  
+<LI>      NCALIB: Descriptions of <A HREF="../ncalib_descr/ncalib_descr.html">program</A> and 
+        <A HREF="../ncalib_private_intfc/ncalib_private_intfc.html"><b>parameters</b></A>;  
+  <UL><LI>    <A HREF="../ncalib_redun/ncalib_redun.html">Redundancy, Align and Selfcal</A>; 
+        <A HREF="../ncalib_polar/ncalib_polar.html">Polarisation</A>; 
+        <A HREF="../ncalib_descr/ncalib_descr.html">Utilities</A> 
+  </UL> 
+<LI>      NCLEAN: Descriptions of <A HREF="../nclean_descr/nclean_descr.html"><b>program</b></A> and 
+        <A HREF="../nclean_private_intfc/nclean_private_intfc.html"><b>parameters</b></A>; 
+        <A HREF="../nclean_descr/nclean_descr.html#.nclean.interface"><b>interface</b></A> diagram 
+<LI>      NCOPY: Descriptions of <A HREF="../ncopy_descr/ncopy_descr.html">program</A> and 
+        <A HREF="../ncopy_private_intfc/ncopy_private_intfc.html"><b>parameters</b></A>;  
+<LI>      NFLAG: Descriptions of <A HREF="../nflag_descr/nflag_descr.html">program</A> and 
+        <A HREF="../nflag_private_intfc/nflag_private_intfc.html"><b>parameters</b></A>;  
+<LI>      NGCALC: Descriptions of <A HREF="../ngcalc_descr/ngcalc_descr.html">program</A> and 
+        <A HREF="../ngcalc_private_intfc/ngcalc_private_intfc.html"><b>parameters</b></A>; 
+        <A HREF="../ngcalc_descr/ngcalc_descr.html#.ngcalc.interface"><b>interface</b></A> diagram 
+  <UL><LI>            <A HREF="../src/doc/txt/ngcalc_lightcurve.txt">Application example</A> 
+  </UL> 
+<LI>      NGIDS: Descriptions of <A HREF="../ngids_descr/ngids_descr.html">program</A> and 
+        <A HREF="../ngids_private_intfc/ngids_private_intfc.html"><b>parameters</b></A>;  
+<LI>      NMAP: Descriptions of <A HREF="../nmap_descr/nmap_descr.html">program</A> and 
+        <A HREF="../nmap_private_intfc/nmap_private_intfc.html"><b>parameters</b></A>; 
+        interface diagrams: 
+                <A HREF="../nmap_descr/nmap_descr.html#.nmap.make"><b>map-making</b></A>, with 
+                <A HREF="../nmap_descr/nmap_descr.html#.nmap.make.q"><b>hidden details</b></A> 
+  <UL><LI>    Use of <A HREF="../src/doc/txt/models_and_maps.txt">models in map-making</A>;  
+  </UL> 
+<LI>      NMODEL: Descriptions of  
+        <A HREF="../nmodel_private_intfc/nmodel_private_intfc.html"><b>parameters</b></A>; 
+        interface diagrams: 
+                        <A HREF="../nmodel_descr/nmodel_descr.html#.nmodel.interface"><b>general</b></A>, 
+                        <A HREF="../nmodel_descr/nmodel_descr.html#.nmodel.interface"><b>modelhandling</b></A>, 
+                        <A HREF="../nmodel_descr/nmodel_descr.html#.nmodel.convert"><b>modelconversions</b></A> 
+<LI>      NPLOT: Descriptions of <A HREF="../nplot_descr/nplot_descr.html">program</A> and 
+        <A HREF="../nplot_private_intfc/nplot_private_intfc.html"><b>parameters</b></A>;  
+<LI>      NSCAN: Descriptions of <A HREF="../nscan_descr/nscan_descr.html">program</A> and 
+        <A HREF="../nscan_private_intfc/nscan_private_intfc.html"><b>parameters</b></A>;  
+<LI>      Descriptions of<em>public</em> parameters, shared by more than oneprogram: 
+  <UL><LI>    .SCN-file access: 
+                <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html"><b>file</b></A>, 
+                <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html"><b>sector</b></A> and 
+                <A HREF="../select_public_intfc/select_public_intfc.html"><b>hour-angle, interferometer,                          polarisation</b></A> selection 
+    <UL><LI>  <A HREF="../unit_public_intfc/unit_public_intfc.html"><b>Magtape/disk</b></A> selection 
+    </UL> 
+  <LI>    .WMP-file access: <A HREF="../wmpnode_public_intfc/wmpnode_public_intfc.html"><b>file</b></A> and 
+        <A HREF="../wmpsets_public_intfc/wmpsets_public_intfc.html"><b>image</b></A> selection 
+  <LI>    .MDL-file access: <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html"><b>file</b></A> selection 
+  <LI>    Model <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">manipulation</A>; 
+        <A HREF="../nmodel_descr/nmodel_descr.html#.nmodel.handle"><b>diagram</b></A> 
+  <LI>    Mapping parameters: <A HREF="../nmap_public_intfc/nmap_public_intfc.html"><b>NMAP</b></A> group 
+  <LI>    <A HREF="../plotter_public_intfc/plotter_public_intfc.html"><b>Plot-device</b></A> selection 
+  <LI>    <A HREF="../flfnode_public_intfc/flfnode_public_intfc.html"><b>.FLF file</b></A> and 
+        <A HREF="../ngfsets_public_intfc/ngfsets_public_intfc.html"><b>.NGF sector</b></A> selection 
+  <LI>    Low-level <A HREF="../nshow_public_intfc/nshow_public_intfc.html"><b>inspection/editing</b></A> of 
+        .SCN and .WMP files 
+  <LI>    Advanced control of <A HREF="../ngen_public_intfc/ngen_public_intfc.html"><b>hidden parameters</b></A> 
+  </UL> 
+</UL>
+<P>
+<H1><A NAME=SECTION0006000000000000000> <b>Bulk data: Batch processing</b></A></H1>
+<P>
+<UL><LI>      <A HREF="../record_replay/record_replay.html"><b>Recording/replaying</b></A> program runs 
+<LI>      <A HREF="../src/doc/txt/batch.txt">Batch processing</A> in NEWSTAR 
+  <UL><LI>    <A HREF="../src/doc/txt/more_on_batch.txt">Hints</A> 
+  </UL> 
+</UL>
+<P>
+<H1><A NAME=SECTION0007000000000000000> <b>Processing recipes</b></A></H1>
+<P>
+<UL><LI>      <A HREF="../rcp_continuum_21cm/rcp_continuum_21cm.html">21cm-continuum</A> observation 
+<LI>      <A HREF="../rcp_mosaic_21cm/rcp_mosaic_21cm.html">21cm-mosaic</A> observation 
+<LI>      <A HREF="../rcp_line_21cm/rcp_line_21cm.html">21cm-line</A> observation 
+<LI>      <A HREF="../rcp_linear_polarisation/rcp_linear_polarisation.html">Linear-polarisation</A> obdervation 
+<LI>      <A HREF="../src/doc/txt/ngcalc_lightcurve.txt"><b>Lightcurves</b></A> using NGCALC 
+</UL>
+<P>
+<H1><A NAME=SECTION0008000000000000000> <b>Miscellaneous information</b></A></H1>
+<P>
+<UL><LI>      <A HREF="../wsrt_fact_sheet/wsrt_fact_sheet.html"><b>WSRT</b></A> fact sheet 
+<LI>      <A HREF="../src/doc/txt/spefu_type_categ.txt"><b>Category codes</b></A> in the WSRT 
+        Observation Header (OH) 
+</UL>
+<P>
+<H1><A NAME=SECTION0009000000000000000> <b>Programmers' documentation</b></A></H1>
+<P>
+<UL><LI>      Style guides: 
+  <UL><LI>    <A HREF="../doc_guide/doc_guide.html"><b>Document-writing</b></A>; 
+        <A HREF="../src/doc/txt/psc_guide.txt"><b>parameter definition</b></A> 
+  </UL> 
+<LI>      Programming techniques: 
+  <UL><LI>    Dynamic setting of parameter prompts: <A HREF="../src/doc/txt/wndpoh.txt"><b>WNDPOH</b></A> 
+  <LI>    <A HREF="../src/doc/txt/control_c.txt"><b>control-C handling</b></A> 
+  <LI>    <A HREF="../src/doc/txt/debug_efficiently.txt"><b>dbx debugging on SUN workstations</b></A> 
+  <LI>    <A HREF="../src/doc/txt/obscure_bugs.txt"><b>Obscure bugs</b></A> in Newstar programs 
+  <LI>    <A HREF="../show_edit/show_edit.html"><b>Inspection/editing of /.SCN/.WMP files</b></A> 
+  </UL> 
+<LI>      Program/subsystem documentation: 
+  <UL><LI>    <A HREF="../ncopy_progrmr/ncopy_progrmr.html"><b>NCOPY</b></A> 
+  <LI>    <A HREF="../src/doc/txt/ncalib_vzero.txt"><b>NCALIB VZERO</b></A> algorithm 
+  <LI>    <A HREF="../src/doc/txt/wntinc.txt"><b>Table-definition compiler</b></A> 
+  <LI>    <A HREF="../src/doc/txt/xmosaic_restart.txt"><b>Hypertext browser</b></A> restart protocol 
+  <LI>    Accessing <A HREF="../src/doc/txt/qube.txt"><b>.SCN data in various sort orders</b></A> 
+  <LI>    <A HREF="../src/doc/bin/lsq.ps"><b>Least-squares package</b></A> 
+  </UL> 
+<LI>      System maintenance: 
+  <UL><LI>    <A HREF="../src/doc/txt/bug_reports.txt">Bug reporting</A> (<em>in Dutch</em>) 
+  <LI>    <A HREF="../doc_guide/doc_guide.html"><b>Documentation</b></A> organisation; 
+        diagrams: 
+                <A HREF="../doc_guide/doc_guide.html#.doc.sources.and.hyper"><b>hypertext system</b></A>, 
+                <A HREF="../doc_guide/doc_guide.html#.doc.sources.and.print"><b>printable system</b></A>, 
+  <LI>    <A HREF="../src/doc/bin/alpha_portability.ps"><b>DEC Alpha portability</b></A>; 
+        <A HREF="../src/doc/bin/alpha_32_64.ps"><b>32/64 bit issues</b></A> 
+  <LI>    <A HREF="../src/doc/txt/ppd_buffer.txt"><b>PPD buffer size</b></A> adjustment <em>(in Dutch)</em> 
+  <LI>    NFRA <A HREF="../nfra_config_management/nfra_config_management.html">Configuration management</A> 
+  <LI>    Newstar <A HREF="../elsewhere_inst_maint/elsewhere_inst_maint.html">maintenance outside NFRA</A> 
+  </UL> 
+<A NAME=.wsrt.tape><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<LI>      The WSRT tape format: 
+  <UL><LI>      File descriptor (<A HREF="../src/nscan/fdw.dsc"><b>FD</b></A>); 
+          observation header (<A HREF="../src/nscan/ohw.dsc"><b>OH</b></A>); 
+          system calibration block (<A HREF="../src/nscan/scw.dsc"><b>SC</b></A>); 
+          set header (<A HREF="../src/nscan/shw.dsc"><b>SH</b></A>); 
+          interferometer header (<A HREF="../src/nscan/ihw.dsc"><b>IH</b></A>). 
+  <LI>      <A HREF="../src/doc/txt/spefu_type_categ.txt"><b>Category codes</b></A> in the 
+           Observation Header (OH) 
+  </UL> 
+</UL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/hb_contents/images.pl b/hb_contents/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/hb_contents/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/hb_contents/labels.pl b/hb_contents/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..eac25303400a31626f7d94c2a486d450cbfc9df4
--- /dev/null
+++ b/hb_contents/labels.pl
@@ -0,0 +1,7 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".wsrt.tape"} ="$URL/hb_contents.html"; 
+$external_labels{".contents"} ="$URL/hb_contents.html"; 
+
+1;
\ No newline at end of file
diff --git a/hjv.gif b/hjv.gif
new file mode 100644
index 0000000000000000000000000000000000000000..a598b9b2e2380ca9c07bb3cf75df5cf3fff6ff71
Binary files /dev/null and b/hjv.gif differ
diff --git a/icons.html b/icons.html
new file mode 100644
index 0000000000000000000000000000000000000000..3a45761ac46ac474c723bb6e964c4b9fc441f22b
--- /dev/null
+++ b/icons.html
@@ -0,0 +1,20 @@
+
+<FORM METHOD="POST" >
+<INPUT TYPE="submit" VALUE="Next">
+ <P>
+<INPUT TYPE="submit" VALUE="Previous">
+ <P>
+<INPUT TYPE="submit" VALUE="Up">
+ <P>
+<INPUT TYPE="submit" VALUE="Next Group">
+ <P>
+<INPUT TYPE="submit" VALUE="Previous Group">
+ <P>
+<INPUT TYPE="submit" VALUE="Contents">
+ <P>
+<INPUT TYPE="submit" VALUE="Index">
+ <P>
+
+
+
+</FORM>
diff --git a/icons/anchor.png b/icons/anchor.png
new file mode 100644
index 0000000000000000000000000000000000000000..103ad8322ac38d2cbee33ef10e67957622498e4c
Binary files /dev/null and b/icons/anchor.png differ
diff --git a/icons/anchor.xbm b/icons/anchor.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..e9e72aa1acab717f667e01739ad55bfcc731ad00
--- /dev/null
+++ b/icons/anchor.xbm
@@ -0,0 +1,6 @@
+#define anchor.xbm_width 16
+#define anchor.xbm_height 16
+static char anchor.xbm_bits[] = {
+   0x00, 0x00, 0xe0, 0x07, 0xe0, 0x07, 0x80, 0x05, 0x80, 0x05, 0x80, 0x05,
+   0x80, 0x03, 0x80, 0x01, 0x9e, 0x79, 0x8e, 0x71, 0x8e, 0x71, 0x8a, 0x51,
+   0x90, 0x09, 0xe0, 0x07, 0x80, 0x01, 0x00, 0x00};
diff --git a/icons/blank.png b/icons/blank.png
new file mode 100644
index 0000000000000000000000000000000000000000..300ca5812770f5a70db56fe2097ca42a910ab610
Binary files /dev/null and b/icons/blank.png differ
diff --git a/icons/blank.xbm b/icons/blank.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..3c724639131396f04cf2160158a14bb3ee553068
--- /dev/null
+++ b/icons/blank.xbm
@@ -0,0 +1,4 @@
+P4
+# CREATOR: XV Version 3.00  Rev: 3/30/93
+1 1
+
\ No newline at end of file
diff --git a/icons/contents.png b/icons/contents.png
new file mode 100644
index 0000000000000000000000000000000000000000..80edd89e4d0eb237e130f0ff5968b642deba3800
Binary files /dev/null and b/icons/contents.png differ
diff --git a/icons/contents.xbm b/icons/contents.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..a3aed9f8625c67129952f83a07497875fd2ab1f5
--- /dev/null
+++ b/icons/contents.xbm
@@ -0,0 +1,12 @@
+#define contents_width 63
+#define contents_height 16
+static char contents_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xc0,0x01,0x00,0x08,0x00,0x00,0x01,0x00,0x20,0x02,0x00,0x08,0x00,
+ 0x00,0x01,0x00,0x20,0xe2,0x74,0x7c,0x9c,0x8e,0x8f,0x03,0x20,0x10,0x99,0x08,
+ 0x22,0x13,0x41,0x04,0x20,0x10,0x89,0x08,0x3e,0x11,0x81,0x03,0x20,0x12,0x89,
+ 0x08,0x02,0x11,0x01,0x04,0x20,0x12,0x89,0x88,0x22,0x11,0x51,0x04,0xc0,0xe1,
+ 0x9c,0x71,0x9c,0x33,0x8e,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/icons/contents_motif.gif b/icons/contents_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..ddb24ce671d219174f0e1e0d3c366ff23371d5b8
Binary files /dev/null and b/icons/contents_motif.gif differ
diff --git a/icons/cross-ref.png b/icons/cross-ref.png
new file mode 100644
index 0000000000000000000000000000000000000000..370d7c1175f7046262181a809555d90b1056d2b2
Binary files /dev/null and b/icons/cross-ref.png differ
diff --git a/icons/cross-ref.xbm b/icons/cross-ref.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..c2ff90eaa3ea1478676a68139f884040f5d0cdb9
--- /dev/null
+++ b/icons/cross-ref.xbm
@@ -0,0 +1,6 @@
+#define cross-ref.xbm_width 16
+#define cross-ref.xbm_height 16
+static char cross-ref.xbm_bits[] = {
+   0x00, 0x01, 0x80, 0x01, 0xc0, 0x01, 0xe0, 0x01, 0xf0, 0x01, 0xf8, 0x61,
+   0xfc, 0x71, 0xfe, 0x79, 0xff, 0x7f, 0x00, 0x7f, 0x00, 0x7f, 0x80, 0x7f,
+   0xc0, 0x7f, 0xe0, 0x7f, 0xe0, 0x7f, 0x00, 0x00};
diff --git a/icons/cross_ref_motif.gif b/icons/cross_ref_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..1cb5a9b47a64d878d53385636238e12ae0139e65
Binary files /dev/null and b/icons/cross_ref_motif.gif differ
diff --git a/icons/foot.png b/icons/foot.png
new file mode 100644
index 0000000000000000000000000000000000000000..a40a52fadb98b6cca96084b9ed18340e9a2e5352
Binary files /dev/null and b/icons/foot.png differ
diff --git a/icons/foot.xbm b/icons/foot.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..19952073e20bd30f0d142048523cddfc135f51ea
--- /dev/null
+++ b/icons/foot.xbm
@@ -0,0 +1,6 @@
+#define foot.xbm_width 16
+#define foot.xbm_height 16
+static char foot.xbm_bits[] = {
+   0x00, 0x00, 0xc0, 0x01, 0xc0, 0x01, 0xc0, 0x01, 0x80, 0x00, 0x98, 0x0c,
+   0xf8, 0x0f, 0x98, 0x0c, 0x80, 0x00, 0x80, 0x00, 0x80, 0x00, 0x80, 0x00,
+   0x80, 0x00, 0x80, 0x00, 0x80, 0x00, 0x00, 0x00};
diff --git a/icons/foot_motif.gif b/icons/foot_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..b801393f38c66bcd32af988e8d44de0f605c3a99
Binary files /dev/null and b/icons/foot_motif.gif differ
diff --git a/icons/icons.html b/icons/icons.html
new file mode 100644
index 0000000000000000000000000000000000000000..3a45761ac46ac474c723bb6e964c4b9fc441f22b
--- /dev/null
+++ b/icons/icons.html
@@ -0,0 +1,20 @@
+
+<FORM METHOD="POST" >
+<INPUT TYPE="submit" VALUE="Next">
+ <P>
+<INPUT TYPE="submit" VALUE="Previous">
+ <P>
+<INPUT TYPE="submit" VALUE="Up">
+ <P>
+<INPUT TYPE="submit" VALUE="Next Group">
+ <P>
+<INPUT TYPE="submit" VALUE="Previous Group">
+ <P>
+<INPUT TYPE="submit" VALUE="Contents">
+ <P>
+<INPUT TYPE="submit" VALUE="Index">
+ <P>
+
+
+
+</FORM>
diff --git a/icons/index.png b/icons/index.png
new file mode 100644
index 0000000000000000000000000000000000000000..7db778b85a41374c2ce7866ac5f54592ecd61eb3
Binary files /dev/null and b/icons/index.png differ
diff --git a/icons/index.xbm b/icons/index.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..4c8c10616fb3242e52863a04453eeeaa67d43353
--- /dev/null
+++ b/icons/index.xbm
@@ -0,0 +1,10 @@
+#define index_width 41
+#define index_height 16
+static char index_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0xf0,0x01,0x40,0x00,0x00,0x00,
+ 0x40,0x00,0x40,0x00,0x00,0x00,0x40,0x74,0x78,0x9c,0x3b,0x00,0x40,0x98,0x44,
+ 0x22,0x0a,0x00,0x40,0x88,0x44,0x3e,0x04,0x00,0x40,0x88,0x44,0x02,0x0a,0x00,
+ 0x40,0x88,0x44,0x22,0x11,0x00,0xf0,0x9d,0xb9,0x9c,0x31,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/icons/index_motif.gif b/icons/index_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..cab027c0212a65601c3ea6bfa6690c823b661698
Binary files /dev/null and b/icons/index_motif.gif differ
diff --git a/icons/invis_anchor.png b/icons/invis_anchor.png
new file mode 100644
index 0000000000000000000000000000000000000000..45ecb7f2c29eb97f37a8d5a9b994b91605fc4d80
Binary files /dev/null and b/icons/invis_anchor.png differ
diff --git a/icons/invis_anchor.xbm b/icons/invis_anchor.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..cc208a31ff7090c51c647e04d889f7d0eb4490b5
--- /dev/null
+++ b/icons/invis_anchor.xbm
@@ -0,0 +1,4 @@
+#define dot_anchor_width 1
+#define dot_anchor_height 1
+static char dot_anchor_bits[] = {
+ 0xfe};
diff --git a/icons/latex2html.png b/icons/latex2html.png
new file mode 100644
index 0000000000000000000000000000000000000000..04e428f72c5d0637b9ac50e4df2c8c4b970c8ed4
Binary files /dev/null and b/icons/latex2html.png differ
diff --git a/icons/latex2html.xbm b/icons/latex2html.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..d9879963bcf75d353bfd0ef590891ced6ab7d885
--- /dev/null
+++ b/icons/latex2html.xbm
@@ -0,0 +1,16 @@
+#define noname_width 84
+#define noname_height 17
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x20,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xe0,0xc0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0xc0,0x01,0x00,
+ 0x00,0x00,0x00,0x1f,0xfc,0x07,0xfc,0xe7,0xc1,0x07,0x00,0x00,0x00,0x00,0x8c,
+ 0xcd,0x04,0x38,0xe3,0xc3,0x0f,0x00,0x00,0x00,0x00,0x8c,0xc5,0x0c,0x70,0xe1,
+ 0xc7,0x1f,0x00,0x00,0x00,0x00,0xcc,0xc5,0x08,0xe0,0xe1,0xff,0x3f,0x00,0x00,
+ 0x00,0x00,0x4c,0xc3,0xfc,0xe3,0xe0,0xff,0x3f,0x00,0x00,0x00,0x00,0xcc,0xc3,
+ 0x30,0xc3,0xe0,0xff,0xbf,0xbb,0xff,0xfd,0x01,0xac,0xc2,0x30,0xe6,0xe1,0xc7,
+ 0x9f,0xbf,0xff,0xfd,0x01,0xfc,0xcf,0xb0,0xa4,0xe3,0xc3,0x0f,0x9b,0xb5,0xcd,
+ 0x00,0xcc,0xc0,0xb0,0x10,0xe3,0xc1,0x07,0x1b,0x84,0xcf,0x00,0xff,0xf0,0xf3,
+ 0xbc,0xef,0xc0,0x01,0x1f,0x84,0xcf,0x00,0x00,0x00,0xb0,0x04,0xe0,0xc0,0x01,
+ 0x1b,0x84,0xcf,0x00,0x00,0x00,0x30,0x04,0x20,0xc0,0x00,0x1b,0x84,0xca,0x0c,
+ 0x00,0x00,0x30,0x06,0x00,0x00,0x00,0x1b,0x84,0xc8,0x0c,0x00,0x00,0xfc,0x03,
+ 0x00,0x00,0x80,0x3f,0xdf,0xfd,0x0f};
diff --git a/icons/next.png b/icons/next.png
new file mode 100644
index 0000000000000000000000000000000000000000..c93df072902f3a0165363ac153c5f306f87d7daa
Binary files /dev/null and b/icons/next.png differ
diff --git a/icons/next.xbm b/icons/next.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..3e99395169322792e3565a62f4ca53e6810dc666
--- /dev/null
+++ b/icons/next.xbm
@@ -0,0 +1,6 @@
+#define next.xbm_width 16
+#define next.xbm_height 16
+static char next.xbm_bits[] = {
+   0x00, 0x00, 0x00, 0x00, 0x02, 0x03, 0x06, 0x07, 0x0e, 0x0f, 0x1e, 0x1f,
+   0x3e, 0x3f, 0xfe, 0x7f, 0xfe, 0x7f, 0x3e, 0x3f, 0x1e, 0x1f, 0x0e, 0x0f,
+   0x06, 0x07, 0x02, 0x03, 0x00, 0x00, 0x00, 0x00};
diff --git a/icons/next_group_motif.gif b/icons/next_group_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..96d4e5ddfdfbe5cba5c008485fd7daa0189a1ef2
Binary files /dev/null and b/icons/next_group_motif.gif differ
diff --git a/icons/next_group_motif_gr.gif b/icons/next_group_motif_gr.gif
new file mode 100644
index 0000000000000000000000000000000000000000..fabf730466e8be49e7b9a1cc33d93856016de06b
Binary files /dev/null and b/icons/next_group_motif_gr.gif differ
diff --git a/icons/next_motif.gif b/icons/next_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..9c81e8c92fed7fe851ce02e7854dc26a58eae9b2
Binary files /dev/null and b/icons/next_motif.gif differ
diff --git a/icons/next_motif_gr.gif b/icons/next_motif_gr.gif
new file mode 100644
index 0000000000000000000000000000000000000000..985c857a3e0f66f3bfd06820ef908e76cbfe0ed0
Binary files /dev/null and b/icons/next_motif_gr.gif differ
diff --git a/icons/next_page.png b/icons/next_page.png
new file mode 100644
index 0000000000000000000000000000000000000000..479a85cb57ed0ffec5ad0dc0f079a2db1a494c23
Binary files /dev/null and b/icons/next_page.png differ
diff --git a/icons/next_page.xbm b/icons/next_page.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..a9b5f23afaf3540a3e7c700d585eade3d5bb95c5
--- /dev/null
+++ b/icons/next_page.xbm
@@ -0,0 +1,13 @@
+#define next_page_width 68
+#define next_page_height 16
+static char next_page_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x98,0x03,0x00,
+ 0x04,0xc0,0x07,0x00,0x00,0x00,0x30,0x01,0x00,0x04,0x80,0x0c,0x00,0x00,0x00,
+ 0x30,0x71,0xee,0x3e,0x80,0xc8,0xc3,0xe5,0x00,0x50,0x89,0x28,0x04,0x80,0x0c,
+ 0x24,0x12,0x01,0x50,0xf9,0x10,0x04,0x80,0x87,0x27,0xf2,0x01,0x90,0x09,0x28,
+ 0x04,0x80,0x40,0x24,0x12,0x00,0x90,0x89,0x44,0x44,0x80,0x40,0x24,0x12,0x01,
+ 0x38,0x71,0xc6,0x38,0xc0,0x83,0xcb,0xe3,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xc0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/icons/previous.png b/icons/previous.png
new file mode 100644
index 0000000000000000000000000000000000000000..e5fd98f1bde967c51dc2a8afa090cc6f629664dc
Binary files /dev/null and b/icons/previous.png differ
diff --git a/icons/previous.xbm b/icons/previous.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..2c209a2beabc301ef32b1377f076148f6d76493d
--- /dev/null
+++ b/icons/previous.xbm
@@ -0,0 +1,6 @@
+#define previous.xbm_width 16
+#define previous.xbm_height 16
+static char previous.xbm_bits[] = {
+   0x00, 0x00, 0x00, 0x00, 0xc0, 0x40, 0xe0, 0x60, 0xf0, 0x70, 0xf8, 0x78,
+   0xfc, 0x7c, 0xfe, 0x7f, 0xfe, 0x7f, 0xfc, 0x7c, 0xf8, 0x78, 0xf0, 0x70,
+   0xe0, 0x60, 0xc0, 0x40, 0x00, 0x00, 0x00, 0x00};
diff --git a/icons/previous_group_motif.gif b/icons/previous_group_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..ff93c5920e154e07872c5ca79af1efc137f4f3f3
Binary files /dev/null and b/icons/previous_group_motif.gif differ
diff --git a/icons/previous_group_motif_gr.gif b/icons/previous_group_motif_gr.gif
new file mode 100644
index 0000000000000000000000000000000000000000..9ea0ce3ca756f390fad324d9b7b837c4dea6f56e
Binary files /dev/null and b/icons/previous_group_motif_gr.gif differ
diff --git a/icons/previous_motif.gif b/icons/previous_motif.gif
new file mode 100644
index 0000000000000000000000000000000000000000..d43c0320e665dccf4f429d8b9d3448cceee82333
Binary files /dev/null and b/icons/previous_motif.gif differ
diff --git a/icons/previous_motif_gr.gif b/icons/previous_motif_gr.gif
new file mode 100644
index 0000000000000000000000000000000000000000..8d40fd5e0221c056806d5d8467e0e56262cf3bf6
Binary files /dev/null and b/icons/previous_motif_gr.gif differ
diff --git a/icons/previous_page.png b/icons/previous_page.png
new file mode 100644
index 0000000000000000000000000000000000000000..c4b9557eda66be0e117b243c6ee62ac63e20dcfa
Binary files /dev/null and b/icons/previous_page.png differ
diff --git a/icons/previous_page.xbm b/icons/previous_page.xbm
new file mode 100755
index 0000000000000000000000000000000000000000..f3ac286bfaab0624357a8f32144a3a0ddee75738
--- /dev/null
+++ b/icons/previous_page.xbm
@@ -0,0 +1,17 @@
+#define previous_page_width 98
+#define previous_page_height 16
+static char previous_page_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xf8,0x00,0x00,0x00,0x00,0x20,0x03,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x90,0x01,0x00,0x00,0x00,0x20,0xd2,0x71,0xee,0x0e,0xce,0x8c,0x03,0x10,0x79,
+ 0xb8,0x1c,0x00,0x20,0x23,0x88,0x44,0x08,0x91,0x48,0x04,0x90,0x81,0x44,0x22,
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+ 0x20,0x08,0x28,0x08,0x91,0x08,0x04,0x10,0x88,0x44,0x02,0x00,0x20,0x20,0x88,
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+<! History: >
+<!	JPH 960326	Correct NFRA reference >
+<!	JPH 960426	Correct .gif references; replace gen_intro with >
+<!			 introduction>
+<!      TJD 180221      Remove dead links>
+<! >
+<! >
+<HEAD>
+<TITLE>Newstar Home Page nfra (local version!)</TiTLE>
+</HEAD>
+<BODY>
+<IMG SRC="src/doc/bin/newstar.gif">
+
+<H1>Welcome to the upgraded Newstar Documentation Service</H1>
+ 
+<H2>Historical reference documentation for Newstar</H1>
+
+<H2>The Netherlands East West Synthesis Telescope Array Reduction</H2>
+<P>
+
+<A HREF=introduction/introduction.html>Newstar</A>
+is the software package to reduce data from the
+ <A HREF=src/doc/bin/wsrt.gif>WSRT</A>, 
+the <EM>Westerbork Synthese Radio Telescope</EM>.
+<P>
+The WSRT is operated by the Netherlands Foundation for Research in 
+Astronomy (the <A HREF=http://www.astron.nl>NFRA</A>).
+<P>
+
+<P>
+This documentation server gives access to:
+
+<UL>
+<LI><A HREF=nnews.txt>The latest news on Newstar</A> (<EM>here at nfra</EM>)
+<LI><A HREF=hb_contents/hb_contents.html>The Newstar Documentation Collection</A>
+<LI><A HREF=newstar-cookbook.pdf>The Newstar Cookbook</A> by Jan Noordam (editor)
+<LI><A HREF=newstar-verheijen.pdf>How to calibrate, flag and transform 21cm line data from the WSRT using NEWSTAR</A> by Marc Verheijen
+</UL>
+
+<HR>
+<!-- <ADDRESS><A HREF=people/people.html>The Newstar projectgroup</A></ADDRESS> -->
+</BODY>
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+Ff(\))j(user-parameter)g(in)o(terface)104 1532 y(from)12
+b(NFRA.)62 1615 y Fb(\017)21 b Ff(The)14 b(Groningen)f(Image)g(Displa)o
+(y)f(Sy)o(etem)i(\()p Fj(GIDS)p Ff(\))h(displa)o(y)e(pac)o(k)n(age)g
+(from)f(Groningen's)h(GIPSY)h(system.)62 1698 y Fb(\017)21
+b Ff(The)14 b Fj(PGPLOT)g Ff(public-domain)d(screen-graphics)16
+b(pac)o(k)n(age.)924 2995 y(10)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
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+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Introduction to <i>NEWSTAR </i> for new and prospective users </b> <em>Contributed by Johan Hamaker, november 1994  <P></em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=introduction.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=introduction.html#SECTION0002000000000000000>  <b>Preface </b></A>
+<UL> 
+<LI> <A NAME=tex2html3 HREF=introduction.html#SECTION0002100000000000000>  <b>Portability </b></A>
+<LI> <A NAME=tex2html4 HREF=introduction.html#SECTION0002200000000000000>  <b>Terminology</b></A>
+</UL> 
+<LI> <A NAME=tex2html5 HREF=introduction.html#SECTION0003000000000000000>  <b>NEWSTAR's basic processing paradigm </b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=introduction.html#SECTION0003100000000000000>  <b>Source and instrumental-error modeling </b></A>
+<LI> <A NAME=tex2html7 HREF=introduction.html#SECTION0003200000000000000>  <b>Outline of the reduction process in <i>NEWSTAR </i> </b></A>
+<LI> <A NAME=tex2html8 HREF=introduction.html#SECTION0003300000000000000>  <b>The scan (.SCN) file </b></A>
+<UL> 
+<LI> <A NAME=tex2html9 HREF=introduction.html#SECTION0003310000000000000>  <b>Error categories and the Selfcal paradigm </b></A>
+</UL> 
+<LI> <A NAME=tex2html10 HREF=introduction.html#SECTION0003400000000000000>  <b>The map (.WMP) file </b></A>
+<LI> <A NAME=tex2html11 HREF=introduction.html#SECTION0003500000000000000>  <b>The source-model (.MDL) file </b></A>
+<LI> <A NAME=tex2html12 HREF=introduction.html#SECTION0003600000000000000>  <b>Organisation of collections of data structures: Indices</b></A>
+</UL> 
+<LI> <A NAME=tex2html13 HREF=introduction.html#SECTION0004000000000000000>  <b>The <i>NEWSTAR </i> programs</b></A>
+<UL> 
+<LI> <A NAME=tex2html14 HREF=introduction.html#SECTION0004100000000000000>  <b>NSCAN</b></A>
+<LI> <A NAME=tex2html15 HREF=introduction.html#SECTION0004200000000000000>  <b>NCALIB</b></A>
+<LI> <A NAME=tex2html16 HREF=introduction.html#SECTION0004300000000000000>  <b>NMAP</b></A>
+<LI> <A NAME=tex2html17 HREF=introduction.html#SECTION0004400000000000000>  <b>NFLAG</b></A>
+<LI> <A NAME=tex2html18 HREF=introduction.html#SECTION0004500000000000000>  <b>NMODEL</b></A>
+<LI> <A NAME=tex2html19 HREF=introduction.html#SECTION0004600000000000000>  <b>NCLEAN</b></A>
+<LI> <A NAME=tex2html20 HREF=introduction.html#SECTION0004700000000000000>  <b>Other programs</b></A>
+</UL> 
+<LI> <A NAME=tex2html21 HREF=introduction.html#SECTION0005000000000000000>  <b>Salient features of the user interface </b></A>
+<UL> 
+<LI> <A NAME=tex2html22 HREF=introduction.html#SECTION0005100000000000000>  <b>Controlling program runs </b></A>
+<LI> <A NAME=tex2html23 HREF=introduction.html#SECTION0005200000000000000>  <b>On-line Help </b></A>
+<LI> <A NAME=tex2html24 HREF=introduction.html#SECTION0005300000000000000>  <b>Log files </b></A>
+</UL> 
+<LI> <A NAME=tex2html25 HREF=introduction.html#SECTION0006000000000000000>  <b>Interfacing with other astronomical reduction packages </b></A>
+<LI> <A NAME=tex2html26 HREF=introduction.html#SECTION0007000000000000000>  <b>Acknowledgements </b></A>
+</UL>
+<A NAME=.preface><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Preface </b></A></H1>
+<P>
+        <i>NEWSTAR </i> is an acronym for the '<b>N</b>etherlands <b>E</b>ast-<b>W</b>est <b>S</b>ynthesis <b>T</b>elescope <b>A</b>nalysis and <b>R</b>eduction'. It stands for a small collection of programs whose purpose is to process 'raw' visibility data from the WSRT into sky maps, source lists and the like that are ready for astronomical interpretation.
+<P>
+        Its functionality allows one to fully exploit the strong points of East-West systhesis arrays in general and the WSRT in particular: Wide-field mapping, and high dynamic range both in 'total-power' and polarisation observations. To achieve this, <i>NEWSTAR </i> contains a number of powerful and refined algorithms not known to exist in other systems. Their presence makes 
+<i>NEWSTAR </i> quite overwhelming for the uninitiated. This document is intended to provide a simple introduction of a tutorial type.
+<P>
+        The documentation generally refers to the WSRT as the source of observations. <i>NEWSTAR </i> also includes provisions for the processing of data from the Australian Telecope (ATNF) compact array (ATCA), but these are few and simple and we skip them here.
+<P>
+<A NAME=.portability><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002100000000000000>  <b>Portability </b></A></H2>
+<P>
+        <i>NEWSTAR </i>'s primary maintenance is carried out by NFRA on Sun and HP systems. It is actively supported elsewhere for a DECstation and a DEC Alpha; it has been supported in the past for a Convex and is therefore likely to be readily portable to there. VAX support has been discontinued.
+<P>
+        For general operations, such as moving or deleting files, manipulating text files, <em>etc.</em> you must rely on your host system. Inasmuch as <i>NEWSTAR </i> now only runs in Unix environments, a generic knowledge of that environment should be sufficient, but also necessary.
+<P>
+<A NAME=.terminology><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002200000000000000>  <b>Terminology</b></A></H2>
+<P>
+        A perceptive user may well notice that <i>NEWSTAR </i> programs are rather careless in their use of terminology. This is a heritage that we are to some extent stuck with: Automatic 'batch' procedures in several on-going large WSRT projects (<em>WENSS</em> and <em>WHISP</em>) rely on the present structure and parameter names of the user interface. We try to clarify ambiguities in the documentation and on-line Help, but the user must be wary that names do not always mean what they seem to suggest.
+<P>
+<A NAME=.basic><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>NEWSTAR's basic processing paradigm </b></A></H1>
+<P>
+<A NAME=.basic.functions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> The basic functionality and data files of <i>NEWSTAR </i> in a Selfcal application. 
+<A HREF="../fig/basic_functions.ps"><STRONG>FIGURE</STRONG></A> 
+ <i><BR><BR>Rectangles represent the data files, ovals the programs. The numbers refer to the description in the text. 
+<BR>See text for further explanation. </i>
+<P>
+<A NAME=.source.error.modeling><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>Source and instrumental-error modeling </b></A></H2>
+<P>
+        The most common aim of processing visibility data is to obtain a representation of the sources observed, with artefacts from the observing process adequately removed. Such artefacts arise both from the finite sampling of the data (primary and synthesised antenna beams) and from instrumental errors.
+<P>
+        If errors were absent, the problem would be 'simply' to deconvolve the known antenna pattern (synthesised beam) from the observed data. This is an ambiguous process: There is an infinite number of possible solutions. Acceptable ones are favoured by the <em>a priori</em> knowledge incorporated in radio-astronomy algorithms; in addition, human judgment is needed to control the reduction process.
+<P>
+        Instrumental errors complicate the problem. To first order they may be determined from <em>calibrator</em> sources observed before and/or after the source. This typically yields a <em>dynamic range</em> in the order of one in a few hundred.
+<P>
+        Much higher dynamic ranges can only be obtained through <em>self-calibration</em>. This is a generic name for processes in which a source model and a model of the instrumental errors are constructed simultaneously. Self-calibration relies on the fact that the signature of true sources in an observation is quite different from that imposed by instrumental errors. Algorithms have been invented that discriminate between the two quite well. The separation is not perfect, however, and even more than for source modeling alone, human judgment must keep the process on course.
+<P>
+<A NAME=.outline><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Outline of the reduction process in <i>NEWSTAR </i> </b></A></H2>
+<P>
+        <A HREF=" #.basic.functions">Figure</A> shows the fundamental functions and the primary data files with their most important contents. The connecting arrows show the data flow in the basic reduction process. We enumerate the steps here in order for a typical reduction process. In practice, the complexity of the observed field and/or the quality of the observation may give rise to a wide variety of situations; the same steps or only part of them may have to be combined in a different sequence. If you need really high dynamic range, take your time to become an expert...
+<P>
+        The basic reduction steps shown combined in <A HREF=" #.basic.functions">figure</A> are: 
+ <OL><LI>   Visibilities are read in from a data archive by NSCAN; calibrator observation(s) are included. 
+<LI>   The calibrator data are processed in NCALIB to find the instrumental errors. A source model is used as a reference; such models are available in 
+<i>NEWSTAR </i> for all calibrators routinely used by the WSRT. The errors found are stored as <em>corrections</em> in the calibrator observation. 
+<LI>   NCALIB is invoked to copy the corrections from the calibrator to the astronomical observation. This provides the 'first-order' error correction referred to <A HREF="#.source.error.modeling">above</A>. 
+<LI>   A map is made from the astronomical observation, using the corrections. At this point, reduction may be complete. If the quality of the map is inadequate, one must continue. 
+<LI>   NMODEL FIND and NCLEAN are used to construct a <em>source model</em> for the astronomical field; such a model is a list of components, each of which can be arbitrarily positioned and have a finite extent. (<em>I.e.</em>, they are much more general than conventional CLEAN components.) 
+<LI>   The positions and other parameters defining the source components may be improved through an NMODEL UPDATE. This procedure is unique to <i>NEWSTAR </i>. It refines the parameters estimated by NMODEL FIND for each source component by comparing its computed visibilities against the observed ones. 
+<LI>   A 'self-calibration' <em>selfcal</em> can now be done with NCALIB in the same way as was done for the calibrator in step 2 above. This will refine the correction parameters stored in the .SCN file. 
+<LI>   NFLAG may be used to flag as 'bad' those scans for which the Selfcal operation produced a poor result (either an error message or an excessive mean error in the solution). 
+<LI>   Form this point on, steps 3-8 can be repeated <em>ad libitum</em>. 
+ </OL>
+<P>
+        With a general picture of the reduction process in mind, we can take a look first at the data files and then at the programs involved.
+<P>
+<A NAME=.scn.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003300000000000000>  <b>The scan (.SCN) file </b></A></H2>
+<P>
+<A NAME=.SCNSUM><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P>
+        .SCN files hold all visibility data in <i>NEWSTAR </i>. The basic unit of data is the <em>scan</em>, an array of visibilities for one mosiac subfield, hour angle and frequency channel, with polarisation (XX, XY, ,YX, YY) and interferometer sequence number as its two dimensions. Series of scans that are contiguous in hour angle together form a <em>sector</em>. The organisation of the sectors in a .SCN file will be discussed <A HREF="#.SCNSUM.indices">below</A>.
+<P>
+        It is a fundamental tenet of <i>NEWSTAR </i> that visibility data are always stored as received from Westerbork. <em>Corrections</em> are stored separately as such, and only applied to the visibilities when the data are read in by a program. Thus, what changes during the history of a .SCN file is the correction tables, <em>not</em> the visibility data.
+<P>
+        An important mechanism for eliminating faulty data points is the use of <em>flags</em>. Since there are several different reasons for rejecting data, 8 different flag types are recognised. A <em>flag byte</em> is associated with each data point. Programs normally reject a data point if any one of these flags is set, but the user has the option ignore certain flag types.
+<P>
+        The <em>self-calibration</em> methods in <i>NEWSTAR </i> rely on comparing the observed visibility data with the visibilities of a <em>source model</em> to find the instrumental errors. To economise on the lengthy calculations necessary to generate the <em>model visibilities</em>, the latter may be saved in the .SCN file for reuse.
+<P>
+<A NAME=.selfcal><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H3><A NAME=SECTION0003310000000000000>  <b>Error categories and the Selfcal paradigm </b></A></H3>
+<P>
+<A NAME=.error.model><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/error_model.ps"><STRONG>FIGURE</STRONG></A> 
+ <i>NEWSTAR's Selfcal error model. 
+<BR>The sums of all phase and gain errors that occur in the path between the source and the correlator differ per telescope and polarisation, i.e. per IF channel. Each IF channel contributes one and the same error to all interferometers in which it is connected. The correlator is assumed in first instance to be error-free; this is almost perfectly true for the WSRT in most observing modes. 
+<BR>See text for further explanation. </i>
+<P>
+        Errors, - and consequently corrections for them -, can be broken down in four categories, as shown schematically in <A HREF=" #.error.model">figure</A>:
+<P>
+ <UL><LI>   <em>Global:</em> Errors represented by a single parameter for the instrument as a whole: e.g. a clock error or refraction.
+<P>
+<LI>   <em>Telescope(-based):</em> Errors that occur <em>per telescope</em> and therefore affect all interferometers including that telescope in the same way: 
+e.g. tropospheric cloud effects and telescope position errors.
+<P>
+<LI>   <em>IF-based:</em> Errors that occur <em>per dipole/polarisation channel</em> 
+ and therefore affect all interferometers including that IF channel in the same way: e.g. elctronic gain and phase errors.
+<P>
+<LI>   <em>Interferometer(-based):</em> Errors that occur in the correlator and can therefore not be attributed to a telescope/polarisation channel: e.g. correlator zero offsets. In a well-designed correlator these errors can be very small and for the WSRT one can almost always ignore them. 
+ </UL>
+<P>
+        In the somewhat inaccurate terminology of <i>NEWSTAR </i> no dictinction is made between telescope- and IF-based errors; the two are jointly known as <em>telescope errors</em> as opposed to <em>interferometer errors</em>. The distinction between the two types of error is fundamental to the <em>Selfcal</em> methods which are used to separate instrumental errors from the true source visibilities. A basic understanding of the Selfcal paradigm is assumed throughout <i>NEWSTAR </i>.
+<P>
+        In addition to the Selfcal constraint, WSRT data are subject to the <em>Redundancy</em> constraint: Baselines of the same length (and the same orientation as they always have for the WSRT) must produce the same visibilities.
+<P>
+<A NAME=.wmp.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003400000000000000>  <b>The map (.WMP) file </b></A></H2>
+<P>
+        .WMP files are the containers for two-dimensional <em>images</em>: sky maps and antenna patterns. Each immage is an array of data points with horizontal and vertical positions <em>l, m</em> as coordinates. It represents a projection of the celestial sphere on a plane tangent in the field centre; the direction of the projection is <em>parallel to the polar axis</em>.
+<P>
+        The organisation of the images in a .WMP file will be discussed 
+<A HREF="#.indices">shortly</A>.
+<P>
+<A NAME=.mdl.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003500000000000000>  <b>The source-model (.MDL) file </b></A></H2>
+<P>
+        Unlike the .SCN and .WMP files that may contain a collection of sectors or images, the .MDL file harbours only a single <em>source model</em>. The concept of such a model is familiar from <em>CLEAN</em> as a list of point sources with a position and flux for each.
+<P>
+        The <i>NEWSTAR </i> source mode is more refined: It may also contain for each source an (elliptical-Gaussian) extent, its 4 Stokes parameters, its spectral index and its intrinsic rotation measure. Traditional CLEAN components are a degenerate case of this more general concept.
+<P>
+<A NAME=.indices><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A NAME=.SCNSUM.indices><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003600000000000000>  <b>Organisation of collections of data structures: Indices</b></A></H2>
+<P>
+        We have seen that <i>NEWSTAR </i> data files are collections of data units: Let us first consider the .SCN file, where these units are the 
+<A HREF="#.scn.file">sectors</A>. Each such unit is self-describing, but we need additional information to understand its relation to other units, viz. what are its channel number and field number (for a mosaic observation). Moreover it is possible to store more than one observation in a scan file and we need a way of knowing which is which.
+<P>
+        The organisation in <i>NEWSTAR </i> data files is by means <em>hierarchical indexing</em>: Each unit is addressed through a <em>composite index</em>, consisting of a string of integers <em>'indices'</em> separated by dots, e.g.
+<P>
+  3.1.0.5
+<P>
+        For the .SCN file the indices are:
+<P>
+  &lt;group&gt;.&lt;observation&gt;.&lt;field&gt;.&lt;channel&gt;.&lt;sequence\ nr where
+<P>
+ <UL><LI>   &lt;group is a purely administrative index that allows one, e.g. to collect observations that are intrinsically unrelated in a single file, 
+e.g. a scientific observation with the calibrator observations to be used with it.
+<P>
+<LI>   &lt;observation&gt; is related to <em>labels</em> and <em>observations</em> in which WSRT data tapes are structured.
+<P>
+<LI>   &lt;field&gt; is a subfield number in a mosaic observation.
+<P>
+<LI>   &lt;channel&gt; is a frequency-channel number (also known as band number).
+<P>
+<LI>   &lt;sequence number&gt; is an extra index that allows for the existence of multiple data structures having all preceding indices the same, 
+ </UL>
+<P>
+        For the .WMP file the indices are:
+<P>
+  &lt;group&gt;.&lt;field&gt;.&lt;channel&gt;.&lt;polarisation&gt;.&lt;image type&gt;.&lt;sequence nr&gt; 
+where &lt;group&gt;, &lt;field&gt; and &lt;channel&gt; are the same as for the .SCN file; in addition we have
+<P>
+ <UL><LI>   &lt;polarisation&gt; represents either a WSRT dipole combination or a Stokes parameter.
+<P>
+<LI>   &lt;image type&gt; indicates either a map or an antenna pattern. 
+ </UL>  
+        A number of mechanisms exist in the user interface that allow you to select set(s) of data units, e.g. 'all sectors', 'all channels for fields 3 through 7', etc.
+<P>
+        In closing, we note that the indexing structure is purely administrative. The data units are entirely self-contained in terms of their data contents and associated headers. A sector, for example, can be copied from one .SCN file to another without any loss of the information necessary for its interpretation.
+<P>
+<A NAME=.programs><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>The <i>NEWSTAR </i> programs</b></A></H1>
+<P>
+        <A HREF=" #.basic.functions">Figure</A> includes only the most basic functions of the most important programs. Each of the programs includes a considerable number of other <em>functions</em>: <i>NEWSTAR </i> is a small collection of large multifunctional programs rather than a large collection of small programs (like AIPS or GIPSY).
+<P>
+        We will briefly mention the most interesting functions in each of the programs, but ignore the <em>utility functions</em> which are part of most programs. These will, e.g.:
+<P>
+ <UL><LI>   list the contents of files;
+<P>
+<LI>   show headers and data blocks in detail and optionally edit them;
+<P>
+<LI>   convert files between number formats for different host systems;
+<P>
+<LI>   track version changes;
+<P>
+<LI>   write and/or read FITS tapes/files.
+<P>
+ </UL>
+<P>
+<A NAME=.nscan><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000>  <b>NSCAN</b></A></H2>
+<P>
+        NSCAN is the program that handles .SCN files. Apart from utilities, its only operation is:
+<P>
+ <UL><LI>   LOADing data from an external medium (classical magtape, DAT or Exabyte tape, optical disk) into a .SCN file. 
+ </UL>
+<P>
+It is capable to read WSRT data in all existing formats including the old 'Leiden format'.
+<P>
+<A NAME=.ncalib><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000>  <b>NCALIB</b></A></H2>
+<P>
+        NCALIB is the program that determines corrections from the visibilities in a .SCN file, optionally using a <A HREF="#.mdl.file">source model</A> as a reference. Its primary functions include:
+<P>
+ <UL><A NAME=.redun><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<LI>   REDUN: This is the Selfcal function of NEWSTAR. It includes several methods of estimating telescope errors from observed visibilities and (optionally) a source model, using the <A HREF="#.selfcal">Selfcal and Redundancy</A> constraints.
+<P>
+<LI>   POLAR: Determining deviations from the nominal dipole responses to polarised radiation from calibrator observations.
+<P>
+<LI>   SET: Function for reading corection parameters from external sources, such as
+<P>
+   <UL><LI> estimates of Faraday rotations calculated from ionosonde or chirp-sounder data;
+<P>
+  <LI> clock corrections from the International Earth Rotation Service (IERS, formerly the Bureau Internationale de l'Heure). 
+   </UL>  
+ </UL>
+<P>
+<A NAME=.nmap><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004300000000000000>  <b>NMAP</b></A></H2>
+<P>
+        NMAP is the program that handles .WMP files. Its primary functions include:
+<P>
+ <UL><LI>   MAKE: Its first and foremost function, <em>viz.</em> to Fourier-transform visibilities into sky maps with their assosiated antenna patterns.
+<P>
+<LI>   FIDDLE: A family of functions to modify maps or combine them into new ones in several useful ways, e.g.:
+<P>
+   <UL><LI> BEAM, DEBEAM: Apply/de-apply the primary-beam correction.
+<P>
+  <LI> POL, ANGLE: Convert a pair of Stokes Q and U maps into a pair representing the polarisation direction and magnitude.
+<P>
+  <LI> MOSCOM: Merge adjacent overlapping maps (e.g. mosaic subfields or adjacent full mosaics) into a single large map.
+<P>
+ </UL>  </UL>
+<P>
+<A NAME=.nflag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004400000000000000>  <b>NFLAG</b></A></H2>
+<P>
+        NFLAG is the <em>only</em> program that changes flag settings. Its FLAG function is composed of a large number of subfunctions that set different flags on the basis of criteria that may be
+<P>
+ <UL><LI>   <em>deterministic,</em> i.e. comparing data's coordinate parameters against fixed limits (e.g. elevation, shadowing, short baselines);
+<P>
+<LI>   <em>data-derived,</em> i.e. comparing data values against a fixed limit (e.g. an upper limit for data considered to be free of interference);
+<P>
+<LI>   derived from <em>data statistics</em>, such as comparing the noise in a 
+<A HREF="#.redun">selfcal</A> solution against a fixed limit. 
+ </UL>
+<P>
+        NFLAG is still evolving. It is hoped that both NFRA and the <i>NEWSTAR </i> users will contribute new ideas and algorithms, to further the art of eliminating faulty data with a minimum of efforts as well as minimal accidental loss of healthy data.
+<P>
+<A NAME=.nmodel><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004500000000000000>  <b>NMODEL</b></A></H2>
+<P>
+        NMODEL is the program that handles source-model (.MDL) files. Its most vital function is FIND, <em>i.e.</em> finding source components of small extent and fitting elliptical Gaussians to them. This operation differs from CLEAN in two ways:
+<P>
+ <UL><LI>   Components are merely located; to subtract them, one must make a new map as in the major cycles of Cotton-Schwab CLEAN.
+<P>
+<LI>   Sources may be at fractional grid positions and extended, which allows for a much more accurate representation of sources of small size. 
+ </UL>
+<P>
+        NMODEL also harbours the <A HREF="#.outline">UPDATE function</A>, which fine-tunes the components of a model by comparing the model visibilities with the observed ones.
+<P>
+<A NAME=.nclean><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004600000000000000>  <b>NCLEAN</b></A></H2>
+<P>
+        NCLEAN is <i>NEWSTAR </i>'s CLEAN program. It's purpose is to create source models for thos source components that cannot be adequately represented by elliptical Gaussian's. It implements only the H&#246;gbom, Clark and Cotton-Schwab CLEAN algorithms.
+<P>
+<A NAME=.other.programs><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004700000000000000>  <b>Other programs</b></A></H2>
+<P>
+        <A HREF=" #.basic.functions">Figure</A> shows only the most vital programs. There are several others:
+<P>
+ <UL><LI>   NATNF loads data from the Australian Telescope (ATNF) into a .SCN file.
+<P>
+<LI>   NCOPY copies selected parts of a .SCN file into another .SCN file. (In this process one may change visibility values irreversibly through the application of selected corrections.)
+<P>
+<LI>   NPLOT can display or print a variety of plots as well as images in various representations.
+<P>
+<LI>   NGIDS is an adaptation of <em>GIPSY</em>'s display program GIDS. It primary function is to display images in various modes, but it can also be used to select faulty data in a display of visibilities (the <em>TVFLAG</em> function of AIPS).
+<P>
+<LI>   NGCALC is a program to analyse one-dimensional <em>cuts</em>, either through the visibility hypercube or through the associated hypercube of correction values. It can be used, e.g., to analyse the 'light curve' of a variable source or to fit a polynomial to a cut of visibilities against baseline. 
+ </UL>
+<P>
+<A NAME=.user.interface><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000>  <b>Salient features of the user interface </b></A></H1>
+<P>
+<H2><A NAME=SECTION0005100000000000000>  <b>Controlling program runs </b></A></H2>
+<P>
+        <i>NEWSTAR </i> programs communicate with the user through a uniform parameter interface. (Historically this subsystem is referred to as <em>DWARF</em>, but this name now serves only to cause confusion.) We briefly mention the features one normally uses in an interactive session. 
+ <DL COMPACT><DT><DD>   A program is started from the shell through the commands 
+   <UL><DT>
+<DD>       dwe &lt;program name&gt; or dwexe &lt;program name&gt; 
+   </UL>
+<P>
+<DT><DD>   Except for those parameters that are intrinsically of an interactive nature, a program collects all necessary parameter values before any real processing and/or writing to data files is done.
+<P>
+<DT><DD>   Programs can be aborted at any time through control-C. This is safe <em>except when modification of data files is in progress.</em> Where the latter is the case, one would risk corrupting those files.
+<P>
+<DT><DD>   Parameters to be specified by the user are known by their name (also known as the <em>keyword</em>.
+<P>
+<DT><DD>   When a program needs a parameter value, it will prompt on the terminal showing the keyword, a short text explaining what is being asked for, a list of options where applicable, and the default value if one is available.
+<P>
+<DT><DD>   The user's reply is immediately checked to the extent possible: For numeric values a range of validity may have been defined, options must match the list of valid names (unique abbreviations being allowed in most cases.
+<P>
+<DT><DD>   When you reply with an EOF character (control-D in Unix) or a hash sign (#), the program will backtrack over one or several prompts, allowing you to recover from mistakes without having to abort and restart the program.
+<P>
+ </DL>
+<P>
+<A NAME=.help><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000>  <b>On-line Help </b></A></H2>
+<P>
+        On-line help in a running program is available in two modes: 
+ <UL><LI>   The <em>dumb-terminal mode</em>: When you type a '?' in reply to a prompt, the help text for the parameter will be shown on your terminal (window).
+<P>
+<LI>   You switch to <em>hypertext mode</em> by typing '??' in reply to a prompt; this mode then remains in effect until the program terminates. Help texts are displayed in the xmosaic window; the advantage is that you now have access to associated documentation through hypertext links. 
+ </UL>
+<P>
+<A NAME=.log.files><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005300000000000000>  <b>Log files </b></A></H2>
+<P>
+        Each program run produces a .LOG file in your current directory. These files are named
+<P>
+        &lt;prog&gt;&lt;timestamp&gt;A.LOG,
+<P>
+where &lt;prog&gt; is the first three characters of the program name and 
+&lt;timestamp&gt; is a string of 12 digits (yymmddhhmmss). The newest log for a program is also known under the name
+<P>
+        &lt;program&gt;.LOG 
+<BR>The log file contains a record of all the parameter values that were used in the program run, a copy of all messages and other output that appeared on the terminal and in some cases a lot more information.
+<P>
+        In many cases the best way to digest a log file is not to print it. Instead, take a quick look at it on your terminal to decide what information is most relevant; then use the Unix utility <em>grep</em> to extract it.
+<P>
+<A NAME=.interfacing><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000>  <b>Interfacing with other astronomical reduction packages </b></A></H1>
+<P>
+        The possibilities to exchange data between <i>NEWSTAR </i> and 'the rest of the world' are limited to the following:
+<P>
+ <UL><LI>   The sectors from a .SCN file can be exported in the UVFITS format that AIPS can read. The inverse operation is <em>not</em> provided for.
+<P>
+<LI>   Images can be written and read in 16- and 32-bit integer as well as 32-bit floating-point FITS formats. Other packages are likely to interface to at least one of these.
+<P>
+<LI>   Visibility data from ATNF/Miriad can be read.
+<P>
+<LI>   Interfaces between <i>NEWSTAR </i> and AIPS++ will probably be developed as a by-product of NFRA's active involvement in the latter project. The eventual conversion policy will be determined on the basis of the user's needs. 
+ </UL>
+<P>
+<H1><A NAME=SECTION0007000000000000000>  <b>Acknowledgements </b></A></H1>
+<P>
+        <i>NEWSTAR </i>'s history dates back to the pioneering work on Redundancy by J.E. Noordam in the early 1980s. W.N. Brouw systematised and expanded his work in subsequent years, in a suite of programs known as the 'R-series'. In 1990-1991, this series served as the prototype for an entirely new collection of programs that eventually became <i>NEWSTAR </i>. During this entire development, A.G.de Bruyn played an indispensable role as an active and stimulating user. 
+        Several users contributed to the documentation; they are acknowledged in the individual Document chapters. 
+        Incorporated in <i>NEWSTAR </i> are: 
+ <UL><LI>   The Dwingeloo-Westerbork Astronomical Reduction Facility (<em>DWARF</em>) user-parameter interface from NFRA.
+<P>
+<LI>   The Groningen Image Display Syetem (<em>GIDS</em>) display package from Groningen's GIPSY system.
+<P>
+<LI>   The <em>PGPLOT</em> public-domain screen-graphics package. 
+ </UL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/introduction/labels.pl b/introduction/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..91597d9a42b19df11e5acac3be25f3952c6c93ec
--- /dev/null
+++ b/introduction/labels.pl
@@ -0,0 +1,34 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".nclean"} ="$URL/introduction.html"; 
+$external_labels{".ncalib"} ="$URL/introduction.html"; 
+$external_labels{".wmp.file"} ="$URL/introduction.html"; 
+$external_labels{".indices"} ="$URL/introduction.html"; 
+$external_labels{".contents"} ="$URL/introduction.html"; 
+$external_labels{".nscan"} ="$URL/introduction.html"; 
+$external_labels{".selfcal"} ="$URL/introduction.html"; 
+$external_labels{".source.error.modeling"} ="$URL/introduction.html"; 
+$external_labels{".nmodel"} ="$URL/introduction.html"; 
+$external_labels{".SCNSUM"} ="$URL/introduction.html"; 
+$external_labels{".redun"} ="$URL/introduction.html"; 
+$external_labels{".SCNSUM.indices"} ="$URL/introduction.html"; 
+$external_labels{".help"} ="$URL/introduction.html"; 
+$external_labels{".user.interface"} ="$URL/introduction.html"; 
+$external_labels{".other.programs"} ="$URL/introduction.html"; 
+$external_labels{".outline"} ="$URL/introduction.html"; 
+$external_labels{".basic"} ="$URL/introduction.html"; 
+$external_labels{".log.files"} ="$URL/introduction.html"; 
+$external_labels{".basic.functions"} ="$URL/introduction.html"; 
+$external_labels{".interfacing"} ="$URL/introduction.html"; 
+$external_labels{".nflag"} ="$URL/introduction.html"; 
+$external_labels{".terminology"} ="$URL/introduction.html"; 
+$external_labels{".portability"} ="$URL/introduction.html"; 
+$external_labels{".programs"} ="$URL/introduction.html"; 
+$external_labels{".nmap"} ="$URL/introduction.html"; 
+$external_labels{".preface"} ="$URL/introduction.html"; 
+$external_labels{".error.model"} ="$URL/introduction.html"; 
+$external_labels{".scn.file"} ="$URL/introduction.html"; 
+$external_labels{".mdl.file"} ="$URL/introduction.html"; 
+
+1;
\ No newline at end of file
diff --git a/ionost/ionost__change_f0f2_inp.html b/ionost/ionost__change_f0f2_inp.html
new file mode 100644
index 0000000000000000000000000000000000000000..8abb1689611264422450bb0d67f201def5bca311
--- /dev/null
+++ b/ionost/ionost__change_f0f2_inp.html
@@ -0,0 +1,18 @@
+<TITLE>Description of CHANGE_F0F2_INP (IONOST)</TITLE>
+<H1>Program IONOST: private keyword CHANGE_F0F2_INP</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO (Should foF2 input data be changed?)
+<DT><EM>Default:</EM> NO /NOASK.
+<DT><EM>Expected input:</EM> Character(3).<P>
+	change f0F2 input data by used input Faraday rotation data flag: 
+			= NO  no change by using ionospheric Faraday rotation 
+			      input 
+			= YES change by using ionospheric Faraday rotation 
+			      input <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__corrections.html b/ionost/ionost__corrections.html
new file mode 100644
index 0000000000000000000000000000000000000000..1d2fdbb6521efcadd330edf9a412b53967edd1d2
--- /dev/null
+++ b/ionost/ionost__corrections.html
@@ -0,0 +1,18 @@
+<TITLE>Description of CORRECTIONS (IONOST)</TITLE>
+<H1>Program IONOST: private keyword CORRECTIONS</H1> 
+
+<DT><EM>Prompt:</EM> VLBI, RIF, FAR, DELAY (Corrections to be calculated)
+<DT><EM>Default:</EM> RIF, FAR /NOASK.
+<DT><EM>Expected input:</EM> Character(5), 2 values.<P>
+	Corrections which should be calculated: 
+	VLBI: VLBI refraction corrections are calculated 
+	RIF:  corrections for ionospheic refraction are calculated 
+	FAR:  corrections for Faraday rotation are calculated 
+	DELAY: corrections for path length errors are calculated <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__day_number.html b/ionost/ionost__day_number.html
new file mode 100644
index 0000000000000000000000000000000000000000..af2e98c477f1578c42cf76f0e4cf0953e95a96dd
--- /dev/null
+++ b/ionost/ionost__day_number.html
@@ -0,0 +1,18 @@
+<TITLE>Description of DAY_NUMBER (IONOST)</TITLE>
+<H1>Program IONOST: private keyword DAY_NUMBER</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 0 /ASK.
+<DT><EM>Expected input:</EM> Integer number.<P>
+	day number for which the calculations have to be done. The format is 
+	as YYMMDD, where YY is the year - 1900, MM the month number in the 
+	year and DD the daynumber in the month. Several dates may be specified: 
+	Specify after the last day wanted a "0" (= zero) - then the program 
+	will exit after the last calculations needed. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__declination.html b/ionost/ionost__declination.html
new file mode 100644
index 0000000000000000000000000000000000000000..be16e37d0ab8eba7169be6d713c73053e980142b
--- /dev/null
+++ b/ionost/ionost__declination.html
@@ -0,0 +1,14 @@
+<TITLE>Description of DECLINATION (IONOST)</TITLE>
+<H1>Program IONOST: private keyword DECLINATION</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Declination of source for which ionosphere corrections have 
+	to calculated: the value should be given in degrees <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__f2_bottom_height.html b/ionost/ionost__f2_bottom_height.html
new file mode 100644
index 0000000000000000000000000000000000000000..fcba78c886597035c9d3d02c86b9cbec9e5fce80
--- /dev/null
+++ b/ionost/ionost__f2_bottom_height.html
@@ -0,0 +1,14 @@
+<TITLE>Description of F2_BOTTOM_HEIGHT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword F2_BOTTOM_HEIGHT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 6440.0 /ASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Altitude of the bottomside of the F2-layer (in km) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__f2_max_height.html b/ionost/ionost__f2_max_height.html
new file mode 100644
index 0000000000000000000000000000000000000000..55e69dfc21398a7d300bd80e4e25d45b9a22c8e5
--- /dev/null
+++ b/ionost/ionost__f2_max_height.html
@@ -0,0 +1,14 @@
+<TITLE>Description of F2_MAX_HEIGHT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword F2_MAX_HEIGHT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 6770.0 /ASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Altitude of the maximum electron density in the F2-layer (in km) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__f2_p1_height.html b/ionost/ionost__f2_p1_height.html
new file mode 100644
index 0000000000000000000000000000000000000000..cc41e9f25d4009357563b336e6898eee5f1e09c5
--- /dev/null
+++ b/ionost/ionost__f2_p1_height.html
@@ -0,0 +1,14 @@
+<TITLE>Description of F2_P1_HEIGHT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword F2_P1_HEIGHT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 6470.0 /ASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Altitude of the P1 height of the F2-layer (in km) [see ITR-162] <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__f2_p2_height.html b/ionost/ionost__f2_p2_height.html
new file mode 100644
index 0000000000000000000000000000000000000000..74567a59b02b17a8a77e6ee29ab656cdf22b4e80
--- /dev/null
+++ b/ionost/ionost__f2_p2_height.html
@@ -0,0 +1,14 @@
+<TITLE>Description of F2_P2_HEIGHT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword F2_P2_HEIGHT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 7035.0 /ASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Altitude of the P2 height of the F2-layer (in km) [see ITR-162] <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__f2_top_height.html b/ionost/ionost__f2_top_height.html
new file mode 100644
index 0000000000000000000000000000000000000000..e020da008e986f98285b124de49507a98b1c48a0
--- /dev/null
+++ b/ionost/ionost__f2_top_height.html
@@ -0,0 +1,14 @@
+<TITLE>Description of F2_TOP_HEIGHT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword F2_TOP_HEIGHT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 7570.0 /ASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Altitude of the topside of the F2-layer (in km) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__faraday_input.html b/ionost/ionost__faraday_input.html
new file mode 100644
index 0000000000000000000000000000000000000000..761f4af97a7e394e80e72ef3d3037f2cf7932d44
--- /dev/null
+++ b/ionost/ionost__faraday_input.html
@@ -0,0 +1,15 @@
+<TITLE>Description of FARADAY_INPUT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword FARADAY_INPUT</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO (Is Faraday rotation input required?)
+<DT><EM>Default:</EM> NO /NOASK.
+<DT><EM>Expected input:</EM> Character(3).<P>
+	Faraday input flag: = NO  no input data for Faraday rotation are used 
+		            = YES input data for Faraday rotation are used <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__frequency.html b/ionost/ionost__frequency.html
new file mode 100644
index 0000000000000000000000000000000000000000..41fb1b51d59945baa77fdc6a207fb8430ce2e8ef
--- /dev/null
+++ b/ionost/ionost__frequency.html
@@ -0,0 +1,13 @@
+<TITLE>Description of FREQUENCY (IONOST)</TITLE>
+<H1>Program IONOST: private keyword FREQUENCY</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Observing frequency in MHz <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__geometry.html b/ionost/ionost__geometry.html
new file mode 100644
index 0000000000000000000000000000000000000000..1764568c2f2172bc4c30274daabbd9cc6a1d5c2e
--- /dev/null
+++ b/ionost/ionost__geometry.html
@@ -0,0 +1,17 @@
+<TITLE>Description of GEOMETRY (IONOST)</TITLE>
+<H1>Program IONOST: private keyword GEOMETRY</H1> 
+
+<DT><EM>Prompt:</EM> FIXED, VARIABLE, DEFAULT (Geometry selection)
+<DT><EM>Default:</EM> FIXED, DEFAULT /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 2 values.<P>
+	The following options for geometry selection are valid: 
+	FIXED:    fixed ionosphere geometry is taken 
+	VARIABLE: variable ionosphere geometry is taken 
+	DEFAULT:  default ionosphere is taken <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__latitude_obs.html b/ionost/ionost__latitude_obs.html
new file mode 100644
index 0000000000000000000000000000000000000000..d8b40ce15c8a3c1e0dbd634a4cc16ef2abbe4299
--- /dev/null
+++ b/ionost/ionost__latitude_obs.html
@@ -0,0 +1,14 @@
+<TITLE>Description of LATITUDE_OBS (IONOST)</TITLE>
+<H1>Program IONOST: private keyword LATITUDE_OBS</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 52.9169152 /NOASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Geographic latitude observatory (in degrees) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__latitude_stat.html b/ionost/ionost__latitude_stat.html
new file mode 100644
index 0000000000000000000000000000000000000000..43192c74a5819aec8efa9232274daae9902a8977
--- /dev/null
+++ b/ionost/ionost__latitude_stat.html
@@ -0,0 +1,14 @@
+<TITLE>Description of LATITUDE_STAT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword LATITUDE_STAT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 52.10 /NOASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Geographic latitude ionosphere station (in degrees) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__longitude_obs.html b/ionost/ionost__longitude_obs.html
new file mode 100644
index 0000000000000000000000000000000000000000..cbf4645aed19d123c119e62cf4524985cd2e819d
--- /dev/null
+++ b/ionost/ionost__longitude_obs.html
@@ -0,0 +1,14 @@
+<TITLE>Description of LONGITUDE_OBS (IONOST)</TITLE>
+<H1>Program IONOST: private keyword LONGITUDE_OBS</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 6.6041694 /NOASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Geographic longitude observatory (in degrees) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__longitude_stat.html b/ionost/ionost__longitude_stat.html
new file mode 100644
index 0000000000000000000000000000000000000000..cd47857778d9ba0274fc15a25f03cd8bbf840d51
--- /dev/null
+++ b/ionost/ionost__longitude_stat.html
@@ -0,0 +1,14 @@
+<TITLE>Description of LONGITUDE_STAT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword LONGITUDE_STAT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> 5.18 /NOASK.
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Geographic longitude ionosphere station (in degrees) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__next_day.html b/ionost/ionost__next_day.html
new file mode 100644
index 0000000000000000000000000000000000000000..c4eee456030718c2d79603518c693a86f56234e5
--- /dev/null
+++ b/ionost/ionost__next_day.html
@@ -0,0 +1,15 @@
+<TITLE>Description of NEXT_DAY (IONOST)</TITLE>
+<H1>Program IONOST: private keyword NEXT_DAY</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO (Next day flag)
+<DT><EM>Default:</EM> NO /NOASK.
+<DT><EM>Expected input:</EM> Character(3).<P>
+	next day flag: = NO  data not for next day 
+ 		       = YES data for next day. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__nr_180_deg_steps.html b/ionost/ionost__nr_180_deg_steps.html
new file mode 100644
index 0000000000000000000000000000000000000000..cd1f094fc3f9e23c19c6cfae8263c95f355a52fb
--- /dev/null
+++ b/ionost/ionost__nr_180_deg_steps.html
@@ -0,0 +1,13 @@
+<TITLE>Description of NR_180_DEG_STEPS (IONOST)</TITLE>
+<H1>Program IONOST: private keyword NR_180_DEG_STEPS</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Expected input:</EM> I.<P>
+	Number of 180 degree steps in Faraday rotation data at UT_TIME <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__observed_far_rot.html b/ionost/ionost__observed_far_rot.html
new file mode 100644
index 0000000000000000000000000000000000000000..e5e618b50980dc806e809d234094e3fafc12aaf6
--- /dev/null
+++ b/ionost/ionost__observed_far_rot.html
@@ -0,0 +1,13 @@
+<TITLE>Description of OBSERVED_FAR_ROT (IONOST)</TITLE>
+<H1>Program IONOST: private keyword OBSERVED_FAR_ROT</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Observed Faraday rotation values at moments UT_TIME (in degrees) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__right_ascension.html b/ionost/ionost__right_ascension.html
new file mode 100644
index 0000000000000000000000000000000000000000..d0de5a66fa68b439cdc66a4b774082ec34986136
--- /dev/null
+++ b/ionost/ionost__right_ascension.html
@@ -0,0 +1,14 @@
+<TITLE>Description of RIGHT_ASCENSION (IONOST)</TITLE>
+<H1>Program IONOST: private keyword RIGHT_ASCENSION</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Expected input:</EM> Double precision number.<P>
+	Right Ascension of source for which ionosphere corrections have 
+	to calculated: the value should be given in degrees <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__source_name.html b/ionost/ionost__source_name.html
new file mode 100644
index 0000000000000000000000000000000000000000..2535c5f4764ff5a30ce00c18b84a7de078563d4e
--- /dev/null
+++ b/ionost/ionost__source_name.html
@@ -0,0 +1,14 @@
+<TITLE>Description of SOURCE_NAME (IONOST)</TITLE>
+<H1>Program IONOST: private keyword SOURCE_NAME</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Expected input:</EM> Character(12).<P>
+	Specify the source name for which the ionosphere corrections have 
+	to be calculated <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__srce_altaz_fixed.html b/ionost/ionost__srce_altaz_fixed.html
new file mode 100644
index 0000000000000000000000000000000000000000..6d2404daa3610a45530042d6fe551f0f9c8135a2
--- /dev/null
+++ b/ionost/ionost__srce_altaz_fixed.html
@@ -0,0 +1,15 @@
+<TITLE>Description of SRCE_ALTAZ_FIXED (IONOST)</TITLE>
+<H1>Program IONOST: private keyword SRCE_ALTAZ_FIXED</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO (Is source fixed in altazimuth coordinates?)
+<DT><EM>Default:</EM> NO /NOASK.
+<DT><EM>Expected input:</EM> Character(3).<P>
+	source position flag: = NO  source not fixed in altazimuth coordinates 
+			      = YES source fixed in altazimtuh coordinates <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost/ionost__ut_time.html b/ionost/ionost__ut_time.html
new file mode 100644
index 0000000000000000000000000000000000000000..0e59bab431777af51ddb553131ec4cfb25bd2e7c
--- /dev/null
+++ b/ionost/ionost__ut_time.html
@@ -0,0 +1,16 @@
+<TITLE>Description of UT_TIME (IONOST)</TITLE>
+<H1>Program IONOST: private keyword UT_TIME</H1> 
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> -32767 /ASK.
+<DT><EM>Expected input:</EM> I.<P>
+	Universal Time of observations Faraday rotation [in hours and 
+	fractions of hours - i.e. hh.hhh]. If no more values are given: 
+	specify &lt;CR&gt;. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ionost/ionost_keys.html">List of keywords</A> for IONOST
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ionost_keys/ionost_keys.html b/ionost_keys/ionost_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..02fbe296e94e1e8d477a54e514671ade0d4cf655
--- /dev/null
+++ b/ionost_keys/ionost_keys.html
@@ -0,0 +1,81 @@
+<TITLE>Index of private keywords for IONOST </TITLE>
+<H1>Description of keywords for program IONOST</H1>
+
+<UL>
+<LI> <A HREF="../ionost/ionost__source_name.html">
+  SOURCE_NAME</A>
+  
+<LI> <A HREF="../ionost/ionost__day_number.html">
+  DAY_NUMBER</A>
+  
+<LI> <A HREF="../ionost/ionost__longitude_obs.html">
+  LONGITUDE_OBS</A>
+  
+<LI> <A HREF="../ionost/ionost__latitude_obs.html">
+  LATITUDE_OBS</A>
+  
+<LI> <A HREF="../ionost/ionost__longitude_stat.html">
+  LONGITUDE_STAT</A>
+  
+<LI> <A HREF="../ionost/ionost__latitude_stat.html">
+  LATITUDE_STAT</A>
+  
+<LI> <A HREF="../ionost/ionost__frequency.html">
+  FREQUENCY</A>
+  
+<LI> <A HREF="../ionost/ionost__right_ascension.html">
+  RIGHT_ASCENSION</A>
+  
+<LI> <A HREF="../ionost/ionost__declination.html">
+  DECLINATION</A>
+  
+<LI> <A HREF="../ionost/ionost__corrections.html">
+  CORRECTIONS</A>
+  VLBI, RIF, FAR, DELAY (Corrections to be calculated)
+<LI> <A HREF="../ionost/ionost__faraday_input.html">
+  FARADAY_INPUT</A>
+  YES, NO (Is Faraday rotation input required?)
+<LI> <A HREF="../ionost/ionost__change_f0f2_inp.html">
+  CHANGE_F0F2_INP</A>
+  YES, NO (Should foF2 input data be changed?)
+<LI> <A HREF="../ionost/ionost__srce_altaz_fixed.html">
+  SRCE_ALTAZ_FIXED</A>
+  YES, NO (Is source fixed in altazimuth coordinates?)
+<LI> <A HREF="../ionost/ionost__geometry.html">
+  GEOMETRY</A>
+  FIXED, VARIABLE, DEFAULT (Geometry selection)
+<LI> <A HREF="../ionost/ionost__f2_bottom_height.html">
+  F2_BOTTOM_HEIGHT</A>
+  
+<LI> <A HREF="../ionost/ionost__f2_p1_height.html">
+  F2_P1_HEIGHT</A>
+  
+<LI> <A HREF="../ionost/ionost__f2_max_height.html">
+  F2_MAX_HEIGHT</A>
+  
+<LI> <A HREF="../ionost/ionost__f2_p2_height.html">
+  F2_P2_HEIGHT</A>
+  
+<LI> <A HREF="../ionost/ionost__f2_top_height.html">
+  F2_TOP_HEIGHT</A>
+  
+<LI> <A HREF="../ionost/ionost__ut_time.html">
+  UT_TIME</A>
+  
+<LI> <A HREF="../ionost/ionost__observed_far_rot.html">
+  OBSERVED_FAR_ROT</A>
+  
+<LI> <A HREF="../ionost/ionost__nr_180_deg_steps.html">
+  NR_180_DEG_STEPS</A>
+  
+<LI> <A HREF="../ionost/ionost__next_day.html">
+  NEXT_DAY</A>
+  YES, NO (Next day flag)
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../ionost_descr/ionost_descr.html">program IONOST</A>
+</UL>
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/make_model/images.pl b/make_model/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/make_model/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/make_model/labels.pl b/make_model/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..fdde19097f13919dde8c2480528993447205ad5a
--- /dev/null
+++ b/make_model/labels.pl
@@ -0,0 +1,15 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".model.refine"} ="$URL/make_model.html"; 
+$external_labels{".cotton"} ="$URL/make_model.html"; 
+$external_labels{".nmodel.find"} ="$URL/make_model.html"; 
+$external_labels{".contents"} ="$URL/make_model.html"; 
+$external_labels{".model.update"} ="$URL/make_model.html"; 
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+$external_labels{".source.use"} ="$URL/make_model.html"; 
+$external_labels{".clean.vs.find"} ="$URL/make_model.html"; 
+$external_labels{".methods"} ="$URL/make_model.html"; 
+$external_labels{".clean"} ="$URL/make_model.html"; 
+
+1;
\ No newline at end of file
diff --git a/make_model/make_model.html b/make_model/make_model.html
new file mode 100644
index 0000000000000000000000000000000000000000..d558fb59dc8cdddf2e7d26055de6b86f711f947c
--- /dev/null
+++ b/make_model/make_model.html
@@ -0,0 +1,175 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Source models and their construction </b> <P><em>Contributed by Johan Hamaker, December 1994  <P></em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=make_model.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=make_model.html#SECTION0002000000000000000>  <b>The use of source models </b></A>
+<LI> <A NAME=tex2html3 HREF=make_model.html#SECTION0003000000000000000>  <b>The <i>NEWSTAR </i> source model </b></A>
+<LI> <A NAME=tex2html4 HREF=make_model.html#SECTION0004000000000000000>  <b>Model-making in the map domain </b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=make_model.html#SECTION0004100000000000000>  <b>CLEAN </b></A>
+<LI> <A NAME=tex2html6 HREF=make_model.html#SECTION0004200000000000000>  <b>NMODEL FIND </b></A>
+</UL> 
+<LI> <A NAME=tex2html7 HREF=make_model.html#SECTION0005000000000000000>  <b>Model refinement in the visibility domain </b></A>
+<UL> 
+<LI> <A NAME=tex2html8 HREF=make_model.html#SECTION0005100000000000000>  <b>Cotton-Schwab CLEAN </b></A>
+<LI> <A NAME=tex2html9 HREF=make_model.html#SECTION0005200000000000000>  <b>NMODEL UPDATE </b></A>
+</UL>
+</UL>
+<A NAME=.source.use><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>The use of source models </b></A></H1>
+<P>
+        The maps that a synthesis instrument produces do not represent the <em>true sky</em>, but the true sky convolved with the instrumental response, the so-called <em>synthesised beam</em>.
+<P>
+        Whether or not this form is an adequate representation for the purposes of the observer depends both on the information he is trying to extract and on the 'completeness' of the observation. In many cases it will be desirable to obtain a purer representation of the true source distribution. What one needs, then, is a <em>model</em> of the source; the process of constructing such a model is known under various names, such as <em>model-making</em> and <em>deconvolution</em>.
+<P>
+        Even if the user could dispense with a model, a model is needed in <em>self-calibration</em>, the process which seeks to determine instrumental errors from the observation itself. In self-calibration, a source model and a model of the instrumental errors are built up side by side, using algorithms that take into account <em>a priori</em> knowledge about their signatures in an observation.
+<P>
+        Deconvolution amounts to extrapolating from the data actually observed into in the rest of the data domain: In aperture synthesis, one tries to estimate the visibilities between and outside the interferometer baselines and hour angles covered by the observation. The extrapolation is essentially no more than an 'intelligent guess' and one must always remain wary of the possibility that it may be wrong, - in particular when the observed field has complex structure, and/or when the observation has incomplete hour-angle or baseline coverage or parts are unusable due to interference. You are advised to start with relatively simple cases and only tackle more complicated jobs when you have developed a feeling for the possibilities and pitfalls of the methods.
+<P>
+<H1><A NAME=SECTION0003000000000000000>  <b>The <i>NEWSTAR </i> source model </b></A></H1>
+<P>
+        A <em>source model</em> is a list of <em>source components</em> that together approximate the true brightness distribution of a region on the celestial sphere. 
+        A simple and widely known type of model is the list of CLEAN components. A CLEAN model is restricted by the fact that its components lie on grid points of the map in which they were found and that they are point sources. In <i>NEWSTAR </i> a much more general model is used: 
+<UL><LI>   Components can be arbitrarily placed. 
+<LI>   Components can have an elliptic-Gaussian shape, characterised by its half-widths along the long and short axes and the position angle of its long axis.
+<P>
+<LI>   Components can have a spectral index.
+<P>
+<LI>   Components can be polarised, their polarisation state being described by the ratios of stokes parameters <em>Q/I, U/I, V/I</em> as well as an intrinsic rotation measure. 
+</UL>
+<P>
+        Obviously, to take full advantage of these modeling options one needs a lot of functionality. Not all of it is presently available in <i>NEWSTAR </i>, and you are encouraged to share with us ideas that you might have on extending what exists.
+<P>
+<A NAME=.clean.vs.find><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Comparison of <em>(a)</em> the iterative CLEAN and <em>(b)</em> NMODEL FIND/UPDATE procedures. <BR><A HREF="../fig/clean_vs_find.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>Drawn lines show the process loops, dashed lines the auxiliary data involved. <BR><BR>(a) In CLEAN, both the source finding and subtraction occur in the map and can therefore be combined in a single program, <em>NCLEAN</em>. <BR><BR>(b) In FIND, sources are modeled in the map but their subtraction must take place in the visibility domain when a new map is made. <BR>In UPDATE, parameters of an existing source model are refined by comparing the corresponding visibilities against the observed ones. <BR><BR>In both procedures, the final product is a source model plus a residual map containing, along with error artefacts, a fraction of the source that has not (yet) been modeled. </i>
+<P>
+<A NAME=.methods><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>Model-making in the map domain </b></A></H1>
+<P>
+<A NAME=.clean><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000>  <b>CLEAN </b></A></H2>
+<P>
+        The most well-known method of constructing a source model is through the <A HREF="../nclean_descr/nclean_descr.html">CLEAN algorithm</A>. In its simplest form, this iterative algorithm consists of a repetition of the following steps:
+<P>
+<UL><LI>   Find the highest point in the map.
+<P>
+<LI>   Subtract from the map the theoretical response corresponding to a point source at that position with some fraction of the peak intensity found. 
+</UL>
+<P>
+The user defines the map areas in which sources are looked for, and also has control over several other process parameters. Since CLEAN removes each model component found from the map, it is capable in principle of modeling an entire observed field in a single operation.
+<P>
+        The model obtained is a collection of point sources at map-grid positions. Consequently, a CLEAN model is not particularly suitable for representing point sources at arbitrary locations nor for sources of an extent in the order of a few syntesised-beam widths. It is, on the other hand, the only representation we have for extended sources of arbitrary shape.
+<P>
+        CLEAN depends on the subtraction of an antenna pattern shifted to the position of each new source component. Since an antenna pattern normally has the same size as the map to which it applies, shifting it leaves part of the map 'uncovered'. Moreover, both the map and the antenna pattern are contaminated near their edges by aliasing effects. The net result is that satisfactory CLEANING is limited to (somewhat less than) the central quarter of the map.
+<P>
+        For incomplete observations (e.g. Southern sources with limited hour-angle coverage) CLEAN is known to produce artefacts (i.e. incorrect visibility interpolations) which are difficult to control.
+<P>
+        Several variations on the basic theme of CLEAN have been proposed, both to speed it up and to suppress undesirable artefacts. <i>NEWSTAR </i>'s 
+<A HREF="../nclean_descr/nclean_descr.html">NCLEAN</A> includes only a few of these; of them, Cotton-Schwab CLEAN is the most inportant one because it addresses the fundamental limitations outlined above.
+<P>
+<A NAME=.nmodel.find><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000>  <b>NMODEL FIND </b></A></H2>
+<P>
+        The FIND algorithm in NMODEL determines source positions and shapes by fitting a two-dimensional quadratic function to selected source peaks. The selection is made by finding peaks in the map as for CLEAN; the user defines the map areas in which such peaks are looked for.
+<P>
+        Subtracting the source components found is not part of the FIND process. Therefore, FINDing can only proceed to the extent that sources being fitted are not too much disturbed by sidelobes from other sources. Before prpoceeding any further, one must first make a new map in which the source model constructed so far is subtracted.
+<P>
+        <A HREF=" #.clean.vs.find">Figure</A> shows the similarities and differences between FIND and CLEAN.
+<P>
+<A NAME=.model.refine><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000>  <b>Model refinement in the visibility domain </b></A></H1>
+<P>
+        The complicated details of making a map on a Cartesian grid out of the visibilities observed on a polar grid need not concern us here. It is important to realise, however, that it involves several parameters whose definition is in principle quite arbitrary:
+<P>
+<UL><LI>   The <em>convolution function</em> used in interpolating the visibilities from a polar grid to a Cartesian grid.
+<P>
+<LI>   The <em>taper function</em> used for weighing down the long baselines in order to suppress near-in sidelobes in the antenna pattern.
+<P>
+<LI>   The selection of baselines and hour angle ranges, which may be dictated by scheduling constraints, malfunctions and interference. 
+</UL>
+<P>
+        The choice of such parameters affects the source-modeling procedures in various ways, <em>e.g.</em>:
+<P>
+<UL><LI>   In general, the model cannot be expected to accurately represent structure on a scale significantly smaller than the syntesised beamwidth. Thus, the model to be constructed from a map is affected by the taper used in making the map.
+<P>
+<LI>   The peak-fitting process in FIND is affected by sidelobes from other sources: A sloping sidelobe will shift the peak. a non-zero local 'base level' in the map will result in an incotrrect flux estimate. 
+</UL>
+<P>
+        CLEAN, being an iterative procedure, automatically corrects inaccuraccies in its flux determinations, but it works only for the central part of the map as discussed above. FIND does not do this <em>per se</em>. In all methods, the ultimate method of source removal rely on a comparison or subtraction not in the map, but in the visibility domain.
+<P>
+<A NAME=.cotton><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005100000000000000>  <b>Cotton-Schwab CLEAN </b></A></H2>
+<P>
+        Cotton-Schwab CLEAN is a variant of CLEAN is which only a rough model is constructed in the map domain and then properly subtracted in the visibility domain. This variant of CLEAN is thus very similar to the FIND loop of 
+<A HREF=" #.clean.vs.find">figure</A><em>b</em>, the difference being that instead of FIND a quick-and-dirty H&#246;gbom CLEAN is used.
+<P>
+<A NAME=.nmodel.update><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000>  <b>NMODEL UPDATE </b></A></H2>
+<P>
+<A NAME=.model.update><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Schematic diagram of the model-update operation. 
+<A HREF="../fig/model_update.ps"><STRONG>FIGURE</STRONG></A> 
+ <i><BR><BR>The observation consists of the true source visibilities plus observing errors. The source model consists of the true source components minus some unknown defects. 
+<BR><BR>It is these latter defects that the update procedure tries to determine. To do this, it transforms the model into visibilities and compares it to the observed visibilities. It then uses a least-square model fit to determine which part of the difference is attributable to a model defect. 
+<BR><BR>The update model to be fitted is different for each model component; moreover it depends on constraints defined by the user in the form of an update mode (i.e. update position, update flux, update extents etc.) </i>
+<P>
+        As discussed above, both iterated FINDing and Cotton-Schwab CLEAN rely on successive refinement of the model by locating additional components in the map domain. NMODEL's UPDATE function refines the model through a compariuson in the <em>visibility</em> domain; in doing so it relies exclusively on observed data and avoids all the ambiguities introduced by the <A HREF="#.model.refine">map-making process</A>.
+<P>
+        The UPDATE procedure is shown schematically in <A HREF=" #.model.update">figure</A>. Starting from an initial model (typically generated by FIND), it calculates its contribution to the observed visibilities. It then tries to explain the difference between observed and model visibilities in terms of errors in the parameters of each of the model components and adjusts the components accordingly. The result is an improved model. i.e. one that more accurately represents the true observed source distribution.
+<P>
+        Note that UPDATE does not generate any new components. Thus, a complete source model can usually only be obtained by iterating through FIND and UPDATE, mixing in some form of CLEAN for modeling the more extended sources.
+<P>
+        A very neat property of UPDATE is that it suppresses 'mistaken' sources: for example, peaks in the map where grating rings of two sources cross and sources 'aliased in' from ouside the observed field. For such sources, no corresponding pattern exists in the visibility data and UPDATE consequently cancels them.
+<P>
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+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+	\newcommand{\Figref}[1]{\htmladdnormallink{Figure}{ \##1}}
+ 	\newcommand{\ascref}[2]{\htmladdnormallink{#1}{#2}}
+	\newcommand{\Ascref}[2]{\htmladdnormallink{{\bf #1}}{#2}}
+	\newcommand{\textref}[2]{\htmladdnormallink{#1}{#2}}
+	\newcommand{\Textref}[2]{\htmladdnormallink{{\bf #1}}{#2}}
+	\newcommand{\psref}[2]{\htmladdnormallink{#1}{#2}}
+	\newcommand{\Psref}[2]{\htmladdnormallink{{\bf #1}}{#2}}
+	\newcommand{\srcref}[2]{\htmladdnormallink{#1}{#2}}
+	\newcommand{\Srcref}[2]{\htmladdnormallink{{\bf #1}}{#2}}
+	\newcommand{\whichref}[2]{#1}
+%
+% macros that did not work with latex2html and were therefore implemented in 
+%  docScript.csh 
+%
+%	\newcommand{\textref}[3]{
+%		\htmladdnormallink{#1}{../#2/#2.html\##3} }
+%	\newcommand{\eqref}...
+%
+% \svbegin \svend are intended to define a smaller type font so that verbatim
+%  text will fit the standard window width, but latex2html ignores such commands
+%  as \small. Therefore, doc_cook translates the verbatim environment into a
+%  rawhtml environment with <PRE>.
+
+	    %
+%  @(#) cbSymbols.tex v1.1 13/07/93  JEN
+%
+%  Symbol definitions for the redundancy cookbook
+%  This file is included in all NEWSTAR Cookbook sections to ensure a 
+%  uniform naming convention. 
+%
+%  This file is also translated into a NEWSTAR "glossary" called
+%  FORMSYMBOLS.TEX by means of the program SYMBOLSLATEX.FOR.
+%
+%  This file should be included right after cb_preamble.tex
+%
+
+%\gloshead{General:}
+
+\def\cbdir{\$n_src/doc/cook}	% cookbook directory
+\def\NEWSTAR{{\sf NEWSTAR~}}	% name of software package
+\def\Nseries{\NEWSTAR}		% name of package (was N-series)
+
+%\gloshead{Visibility components:}
+
+\def\cVis{{\cal V}}		% (complex) visibility
+\def\pvis{{\Phi}} 		% visibility phase 
+\def\avis{{|{\cVis}|}}		% visibility amplitude
+\def\lavis{{\varrho}}		% visibility ln(ampl)
+
+\def\cGain{{G}}			% (complex) Gain (multiplicative)
+\def\cNoise{{N}}		% (complex) random noise (additive)
+\def\cCadd{{C}}			% (complex) offset (additive)
+
+%\gloshead{The four types of dipole errors and related quantities:}
+
+\def\perr{{p}}			% dipole phase error
+\def\gerr{{g}}			% dipole gain error 
+\def\lerr{{q}}			% dipole ln(gain) error 
+\def\dang{{\phi}}		% dipole position angle
+\def\derr{{\Delta}}		% dipole position angle error 
+\def\eerr{{\Theta}}		% dipole ellipticity
+
+%\gloshead{Miscellaneous:}
+
+\def\Apol{{\epsilon}}		% Polarisation A-factor
+\def\Bpol{{\eta}}		% Polarisation B-factor
+
+\def\wgt{{\cal W}}		% Weight factor
+\def\pwgt{{\wgt^p}}		% Weight for phase equation
+\def\lwgt{{\wgt^g}}		% Weight for ln(gain) equation
+
+\def\pzd{{\psi}}		% XY phase zero difference (PZD)
+
+\def\farang{{\chi}}		% Faraday rotation angle
+
+%*********************************** end of CBSYMBOLS.TEX ***************
+
+%
+%
+%
+%
+{\Large\bf The MDL-file (model components)} 
+\label{.contents}
+\tableofcontents  
+
+A \NEWSTAR MDL file contains a collection of source model components. This may be a mixture of multi-parameter components and ordinary CLEAN components. The former are much more versatile, and represent one of the main differences between \NEWSTAR and other uv-data reduction packages. 
+
+%
+%
+%
+
+%
+\label{mdl.descr.example} 
+\section{\bf Inspecting the list of model components} 
+
+
+******* Insert new script here ****** 
+
+
+The above model is in `local mode', which means that no reference position or reference frequency is known. This information may be taken from a SCN-file (use NMODEL option CONVERT), and stored with the model in the MDL file. The model then looks like this:  
+
+
+******* Insert new script here ****** 
+
+\newpage The coordinates may als be viewed in RA and DEC: 
+
+
+******* Insert new script here ****** 
+
+
+Note that not all source parameters (see below) are visible here. They may be inspected in the log-file whenever the model has been used. 
+
+%
+\label{mdl.descr.param} 
+\section{\bf Source component parameters} 
+
+The source components in a \NEWSTAR model have the following parameters: 
+
+\begin{itemize} 
+\item {\bf I:}           total flux in W.U. (even when extended or polarised) 
+\item {\bf l, m:}        offset from the reference point (map centre) in arcsec 
+\item {\bf ID:}          identification number (1,2,3,...) in the list. 
+\item {\bf Q, U, V:}     Stokes Q, U, V in percent (of I) 
+\item {\bf long, short, PA:}  long and short axes (full halfwidth in arcsec) of an elliptic gaussian extended source, and the position angle of the long axis (degrees North thru East). 
+\item {\bf si:}          spectral index ($flux \div frequ^{si}$). Only used if reference frequency is known. 
+\item {\bf rm:}          Faraday rotation measure ($rot~=~ rm \times (c/frequ^{2}) ~in~rad/m^{2}$). Only used if reference frequency is known. 
+\item {\bf flags:}  (e.g. a `proper' source (0) or a CLEAN component (1))  
+\end{itemize} 
+
+
+NB: CLEAN components: ~\\ - Are not corrected for beam smearing in SELFCAL. ~\\ - Are confined to map grid postions, which may result in poor subtraction. ~\\ - Their positions cannot be "updated" automatically after SELFCAL. ~\\ Therefore, use ``proper sources'' for strong point sources,  and CLEAN components for weak extended sources (but only if necessary). 
+
+
+
+
+%
+\newpage 
+\label{mdl.descr.handle} 
+\section{\bf Overview of model `handling' options.} 
+
+In various \NEWSTAR programs (NMODEL, NCALIB, NMAP etc) the user is able to  {\bf handle} the list of model components in various ways.  The keyword often used is {\bf MODEL\_OPTION}: 
+
+\begin{itemize} 
+\item {\bf READ/WRITE:}         Read/write from/to an external MDL file 
+\item {\bf CLEAR:}              Clear the source component list,  
+                                while resetting reference coordinates 
+\item {\bf ZERO:}               Empty the source component list,  
+                                but keep the coordinates of the field centre 
+                                and frequency. 
+\item {\bf SHOW/LIST:}          Show source list on terminal screen,  
+                                or both terminal and LOG-file. 
+                                See example above. 
+\item {\bf RSHOW/RLIST:}        Show source list in RA/DEC coordinates 
+                                See example above. 
+\item {\bf TOT:}                Show source list statistics (for a specified 
+                                range of sources). The result looks like: 
+\sline{Sources at epoch 1950 at 05:38:43.51, 49.49.42.8, 1417.248 MHz} 
+\sline{10 sources (0 deleted) with 4453.700 W.U. (Max= 1900.000, Min= 2.200)}\\ 
+\item {\bf ADD:}                Add sources to the list by hand. 
+\item {\bf CALIB:}              Convert the source list by scaling intensities 
+                                and/or moving l,m positions. 
+\item {\bf EDIT:}               Edit the sources in the list  
+                                (an amplitude of zero will delete the source) 
+\item {\bf FEDIT:}              Edit a `field' (parameter) for a range of sources 
+\item {\bf MERGE:}              Combine sources components that have  
+                                the same position 
+\item {\bf SORT:}               Sort the source list in decreasing amplitude  
+                                (sorting will always precede a write) 
+\item {\bf FSORT:}              Sort on a specified `field' (parameter) 
+                                in the source list 
+\item {\bf DEL:}                Delete sources 
+\item {\bf DNCLOW:}             Delete non-CLEAN components with low amplitudes 
+\item {\bf DCLOW:}              Delete CLEAN components with low amplitudes 
+\item {\bf DAREA:}              Delete sources in specified area 
+\end{itemize} 
+
+In many cases, the user may specify sources in the list upon which some `handling' options is to act. The specification may be in the form of a {\bf SOURCE\_LIST} of id-numbers, separated by comma's (e.g. 3,6,7,2,34). If the user answers with \scr, a {\bf SOURCE\_RANGE} is asked, i.e. the first and last id-number of a contiguous sublist: 
+
+\skeyword{SOURCE\_LIST} 
+\sprompt{(Source number list)} 
+\sdefault{ = $\ast$:} 
+\suser{?} 
+\skeyword{SOURCE\_RANGE} 
+\sprompt{(Source number range)} 
+\sdefault{ = "":} 
+\suser{*} 
+\sinline{$\ast$ means all sources} 
+
+%
+\newpage 
+\label{mdl.descr.handle-calib} 
+\subsection{\bf Calibration} 
+
+If the flux or position of one of the sources in the list is known, it may be used as a calibrator. In the example, all 10 fluxes of the example model used above are multiplied by a factor (2000/1900), to make the flux of the first one equal to 2000 W.U. At the same time, all positions are shifted. 
+
+
+******* Insert new script here ****** 
+
+
+%
+\newpage 
+\label{mdl.descr.handle-sort} 
+\subsection{\bf Sorting} 
+
+The source components may be sorted in many different ways. The option  SORT orders all components in order of decreasing flux. {\it This operation is performed before each WRITE, so that the components in an MDL file are always sorted this way!}. 
+
+\skeyword{MODEL\_OPTION} 
+\sprompt{(READ,WRITE,CLEAR,ZERO,SHOW, $\ldots$)} 
+\sdefault{= QUIT:}~ 
+\suser{sort} 
+
+FSORT allows the sorting on a range of criteria. In this example, the soorces are sorted in the order of decreasing m-coordinate: 
+
+
+****** Insert new script here ***** 
+
+
+Other possibilities are: ~\\- I:  amplitude ~\\- L,M:  l or m ~\\- LM,ML:  l and m, or m and l ~\\- ID:  identification ~\\- Q,U,V:  Q or U or V ~\\- SI,RM:  spectral index or rotation measure ~\\- LA,SA,PA: long or short axis, position angle ~\\- BITS:  bits (i.e. if source is extended or has polarisation) ~\\- TYP:  source type (0 is the standard) ~\\- CC:  clean component ~\\- TP2:  reserved ~\\- DIST:  distance to a specified centre ~\\- POL:  polarised intensity 
+
+
+%
+\newpage 
+\label{mdl.descr.handle-edit} 
+\subsection{\bf Editing} 
+
+Model components may be edited in various ways, using `handling' options CLEAR, ZERO, ADD, MERGE, DEL, DNCLOW, DCLOW (see the overview above). The handling options EDIT and FEDIT allow specific parameters (`fields') to be edited separately. EDIT acts on a specified source, and FEDIT acts on a range of sources. The possibilities are: 
+
+~\\- I:  amplitude ~\\- L,M:  l or m ~\\- ID:  identification ~\\- Q,U,V:  Q or U or V ~\\- SI,RM:  spectral index or rotation measure ~\\- LA,SA,PA: long or short axis, position angle ~\\- BITS:  bits (i.e. if source is extended or has polarisation) ~\\- TYP:  source type (0 is the standard) ~\\- CC:  clean component ~\\- TP2:  reserved 
+
+
+
+%
+\newpage 
+\label{mdl.descr.uvmodel} 
+\section{\bf Conversion to a uv-model for the .SCN file} 
+
+The calculation of uv-model data (for comparison with uv-data in NCALIB)i s time consuming. Therefore, a calculated uv-model is saved in the .SCN file for which it is calculated, together with the source list used. In all programs that use the model data it can be specified how the model calculation should be done, and if the calculation should be saved. The relevant question is MODEL\_ACTION, which expects a list of three answers. The first one can be one of: 
+
+\begin{itemize} 
+\item   {\bf merge:}     
+        replace the model saved in the SCN node with the one 
+                     specified by the user. However, first compare these two 
+                     lists, and only add the difference to the saved model data. 
+                     I.e. make the calculation as short as possible if the new 
+                     list differs only slightly from the saved one. 
+\item   {\bf add:}       
+                replace the saved model with the sum of the saved one and 
+                     the one specified by the user. The model calculated on the 
+                     basis of the user specified list is added to the saved 
+                     data. 
+\item   {\bf new:} 
+                replace the saved model by the model specified by the user, 
+                     and calculate a completely new set of model data 
+\item   {\bf temporary:} 
+                do not use any data in the SCN node, or write anything, but 
+                     use the data based on the list specified by the user 
+\item   {\bf increment:}         
+        use the saved model data, and add to it the model data 
+                    based on the user specified list, but do not save anything 
+\end{itemize} 
+
+The second answer can be BAND or NOBAND, and specifies if in the model calculation source data should be corrected for bandsmearing to match the actual data better.  The third answer can be TIME or NOTIME to indicate the use of integration time smearing.  
+
+
+
+
+
+
+
+
+
+
+\begin{rawhtml}
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML>\end{rawhtml} 
+\end{document}
diff --git a/mdl_descr/2775_styles b/mdl_descr/2775_styles
new file mode 100644
index 0000000000000000000000000000000000000000..47a723ad5b84e0af78deebb1b2163abc63de0251
--- /dev/null
+++ b/mdl_descr/2775_styles
@@ -0,0 +1,3 @@
+html
+hb_cook_preamble
+hb_symbols
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+++ b/mdl_descr/_7881_tex2html_wrap262.xbm
@@ -0,0 +1,15 @@
+#define noname_width 89
+#define noname_height 15
+static char noname_bits[] = {
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+#define noname_width 5
+#define noname_height 7
+static char noname_bits[] = {
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@@ -0,0 +1,5 @@
+#define noname_width 15
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x38,0x0e,0x0c,0x18,0x1e,0x3c,0x36,0x36,0x63,0x63,0xc3,0x61,0xc3,
+ 0x61,0x63,0x63,0x36,0x36,0x1e,0x3c,0x0c,0x18,0x38,0x0e,0xf0,0x07};
diff --git a/mdl_descr/_7881_tex2html_wrap278.png b/mdl_descr/_7881_tex2html_wrap278.png
new file mode 100644
index 0000000000000000000000000000000000000000..128acb75183abb80b30bff0b561db314a717bbc5
Binary files /dev/null and b/mdl_descr/_7881_tex2html_wrap278.png differ
diff --git a/mdl_descr/_7881_tex2html_wrap278.xbm b/mdl_descr/_7881_tex2html_wrap278.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8823da46d9608cdccce7f81d5866f44e68c86b66
--- /dev/null
+++ b/mdl_descr/_7881_tex2html_wrap278.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xc1,0x07,0x02,0xc1,0x07,0x02,0x01,0x0c,0x02,0x01,0x0e,0x02,0x01,0x07,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,
+ 0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/mdl_descr/_7881_tex2html_wrap280.png b/mdl_descr/_7881_tex2html_wrap280.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/mdl_descr/_7881_tex2html_wrap280.png differ
diff --git a/mdl_descr/_7881_tex2html_wrap280.xbm b/mdl_descr/_7881_tex2html_wrap280.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/mdl_descr/_7881_tex2html_wrap280.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/mdl_descr/_7881_tex2html_wrap284.png b/mdl_descr/_7881_tex2html_wrap284.png
new file mode 100644
index 0000000000000000000000000000000000000000..01a47a8a5b23f6f23ada8d47491965612c233eeb
Binary files /dev/null and b/mdl_descr/_7881_tex2html_wrap284.png differ
diff --git a/mdl_descr/_7881_tex2html_wrap284.xbm b/mdl_descr/_7881_tex2html_wrap284.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..04e515ef865688ba19c9b3a5e657a979370c88ea
--- /dev/null
+++ b/mdl_descr/_7881_tex2html_wrap284.xbm
@@ -0,0 +1,4 @@
+#define noname_width 15
+#define noname_height 2
+static char noname_bits[] = {
+ 0xc3,0x60,0xc3,0x60};
diff --git a/mdl_descr/_7881_tex2html_wrap286.png b/mdl_descr/_7881_tex2html_wrap286.png
new file mode 100644
index 0000000000000000000000000000000000000000..e37c7de516ad7f61c9f6ae2c29eabcd179e624dd
Binary files /dev/null and b/mdl_descr/_7881_tex2html_wrap286.png differ
diff --git a/mdl_descr/_7881_tex2html_wrap286.xbm b/mdl_descr/_7881_tex2html_wrap286.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a018b032a2ff44050d86b5d73009570921a368ac
--- /dev/null
+++ b/mdl_descr/_7881_tex2html_wrap286.xbm
@@ -0,0 +1,10 @@
+#define noname_width 35
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x0c,0x04,
+ 0x01,0x00,0x00,0x0c,0x04,0x81,0xe3,0xb0,0x3e,0x04,0xc1,0xf7,0xf3,0x3e,0x04,
+ 0x61,0x3e,0x73,0x0c,0x04,0xe1,0x1b,0x36,0x0c,0x04,0xc1,0x1f,0x36,0x0c,0x04,
+ 0x01,0x1e,0x37,0x0c,0x04,0x61,0xbe,0x33,0x2c,0x04,0xe1,0xf7,0x31,0x3c,0x04,
+ 0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x04,0xff,0xff,0xff,0xff,0x07};
diff --git a/mdl_descr/images.pl b/mdl_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..87b85409609e84a4bd0ef29e31f2e82685a14d63
--- /dev/null
+++ b/mdl_descr/images.pl
@@ -0,0 +1,21 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$ldots${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap284.xbm">'; 
+$key = q/{}fbox<<247>>largesf?<<247>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap278.xbm">'; 
+$key = q/{}fbox<<260>>largesfsort<<260>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap286.xbm">'; 
+$key = q/{}$fluxdivfrequ^<<120>>si<<120>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap262.xbm">'; 
+$key = q/{}$ast${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap272.xbm">'; 
+$key = q/{}fbox<<252>>largesf*<<252>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap280.xbm">'; 
+$key = q/{}$bigotimes${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap274.xbm">'; 
+$key = q/{}$rot~=~rmtimes(cfrequ^<<122>>2<<122>>)~in~radm^<<123>>2<<123>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap264.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/mdl_descr/labels.pl b/mdl_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9c0cfa56559b086c8bc7607770f7c501af8fb212
--- /dev/null
+++ b/mdl_descr/labels.pl
@@ -0,0 +1,13 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"mdl.descr.uvmodel"} ="$URL/mdl_descr.html"; 
+$external_labels{".contents"} ="$URL/mdl_descr.html"; 
+$external_labels{"mdl.descr.example"} ="$URL/mdl_descr.html"; 
+$external_labels{"mdl.descr.handle"} ="$URL/mdl_descr.html"; 
+$external_labels{"mdl.descr.param"} ="$URL/mdl_descr.html"; 
+$external_labels{"mdl.descr.handle-edit"} ="$URL/mdl_descr.html"; 
+$external_labels{"mdl.descr.handle-calib"} ="$URL/mdl_descr.html"; 
+$external_labels{"mdl.descr.handle-sort"} ="$URL/mdl_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/mdl_descr/mdl_descr.html b/mdl_descr/mdl_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..b207d7e860c335e79b1f26ca7196eea54facfa6c
--- /dev/null
+++ b/mdl_descr/mdl_descr.html
@@ -0,0 +1,211 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The MDL-file (model components)</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=mdl_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=mdl_descr.html#SECTION0002000000000000000> <b>Inspecting the list of model components</b></A>
+<LI> <A NAME=tex2html3 HREF=mdl_descr.html#SECTION0003000000000000000> <b>Source component parameters</b></A>
+<LI> <A NAME=tex2html4 HREF=mdl_descr.html#SECTION0004000000000000000> <b>Overview of model `handling' options.</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=mdl_descr.html#SECTION0004100000000000000> <b>Calibration</b></A>
+<LI> <A NAME=tex2html6 HREF=mdl_descr.html#SECTION0004200000000000000> <b>Sorting</b></A>
+<LI> <A NAME=tex2html7 HREF=mdl_descr.html#SECTION0004300000000000000> <b>Editing</b></A>
+</UL> 
+<LI> <A NAME=tex2html8 HREF=mdl_descr.html#SECTION0005000000000000000> <b>Conversion to a uv-model for the .SCN file</b></A>
+</UL>
+A <i>NEWSTAR </i> MDL file contains a collection of source model components. This may be a mixture of multi-parameter components and ordinary CLEAN components. The former are much more versatile, and represent one of the main differences between <i>NEWSTAR </i> and other uv-data reduction packages.
+<P>
+<A NAME=mdl.descr.example><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Inspecting the list of model components</b></A></H1>
+<P>
+******* Insert new script here ******
+<P>
+The above model is in `local mode', which means that no reference position or reference frequency is known. This information may be taken from a SCN-file (use NMODEL option CONVERT), and stored with the model in the MDL file. The model then looks like this:
+<P>
+******* Insert new script here ******
+<P>
+The coordinates may als be viewed in RA and DEC:
+<P>
+******* Insert new script here ******
+<P>
+Note that not all source parameters (see below) are visible here. They may be inspected in the log-file whenever the model has been used.
+<P>
+<A NAME=mdl.descr.param><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Source component parameters</b></A></H1>
+<P>
+The source components in a <i>NEWSTAR </i> model have the following parameters:
+<P>
+<UL><LI> <b>I:</b>           total flux in W.U. (even when extended or polarised) 
+<LI> <b>l, m:</b>        offset from the reference point (map centre) in arcsec 
+<LI> <b>ID:</b>          identification number (1,2,3,...) in the list. 
+<LI> <b>Q, U, V:</b>     Stokes Q, U, V in percent (of I) 
+<LI> <b>long, short, PA:</b>  long and short axes (full halfwidth in arcsec) of an elliptic gaussian extended source, and the position angle of the long axis (degrees North thru East). 
+<LI> <b>si:</b>          spectral index (<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap262.png">). Only used if reference frequency is known. 
+<LI> <b>rm:</b>          Faraday rotation measure (<IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap264.png">). Only used if reference frequency is known. 
+<LI> <b>flags:</b>  (e.g. a `proper' source (0) or a CLEAN component (1))  
+</UL>
+<P>
+NB: CLEAN components:  <BR>- Are not corrected for beam smearing in SELFCAL.  <BR>- Are confined to map grid postions, which may result in poor subtraction.  <BR>- Their positions cannot be &quot;updated&quot; automatically after SELFCAL.  <BR>Therefore, use ``proper sources'' for strong point sources,  and CLEAN components for weak extended sources (but only if necessary).
+<P>
+<A NAME=mdl.descr.handle><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Overview of model `handling' options.</b></A></H1>
+<P>
+In various <i>NEWSTAR </i> programs (NMODEL, NCALIB, NMAP etc) the user is able to  <b>handle</b> the list of model components in various ways.  The keyword often used is <b>MODEL_OPTION</b>:
+<P>
+<UL><LI> <b>READ/WRITE:</b>         Read/write from/to an external MDL file 
+<LI> <b>CLEAR:</b>              Clear the source component list,  
+                                while resetting reference coordinates 
+<LI> <b>ZERO:</b>               Empty the source component list,  
+                                but keep the coordinates of the field centre 
+                                and frequency. 
+<LI> <b>SHOW/LIST:</b>          Show source list on terminal screen,  
+                                or both terminal and LOG-file. 
+                                See example above. 
+<LI> <b>RSHOW/RLIST:</b>        Show source list in RA/DEC coordinates 
+                                See example above. 
+<LI> <b>TOT:</b>                Show source list statistics (for a specified 
+                                range of sources). The result looks like:
+<P>
+		<BR><tt>Sources at epoch 1950 at 05:38:43.51, 49.49.42.8, 1417.248 MHz</tt>
+<P>
+		<BR><tt>10 sources (0 deleted) with 4453.700 W.U. (Max= 1900.000, Min= 2.200)</tt><BR><LI> <b>ADD:</b>                Add sources to the list by hand. 
+<LI> <b>CALIB:</b>              Convert the source list by scaling intensities 
+                                and/or moving l,m positions. 
+<LI> <b>EDIT:</b>               Edit the sources in the list  
+                                (an amplitude of zero will delete the source) 
+<LI> <b>FEDIT:</b>              Edit a `field' (parameter) for a range of sources 
+<LI> <b>MERGE:</b>              Combine sources components that have  
+                                the same position 
+<LI> <b>SORT:</b>               Sort the source list in decreasing amplitude  
+                                (sorting will always precede a write) 
+<LI> <b>FSORT:</b>              Sort on a specified `field' (parameter) 
+                                in the source list 
+<LI> <b>DEL:</b>                Delete sources 
+<LI> <b>DNCLOW:</b>             Delete non-CLEAN components with low amplitudes 
+<LI> <b>DCLOW:</b>              Delete CLEAN components with low amplitudes 
+<LI> <b>DAREA:</b>              Delete sources in specified area 
+</UL>
+<P>
+In many cases, the user may specify sources in the list upon which some `handling' options is to act. The specification may be in the form of a <b>SOURCE_LIST</b> of id-numbers, separated by comma's (e.g. 3,6,7,2,34). If the user answers with  <i><CR></i>, a <b>SOURCE_RANGE</b> is asked, i.e. the first and last id-number of a contiguous sublist:
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap274.png"> <b>SOURCE_LIST</b> 
+ (Source number list) 
+ = <IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap272.png">: 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap278.png"> 
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap274.png"> <b>SOURCE_RANGE</b> 
+ (Source number range) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap280.png">
+<P>
+		<i><IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap272.png"> means all sources</i>
+<P>
+<A NAME=mdl.descr.handle-calib><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000> <b>Calibration</b></A></H2>
+<P>
+If the flux or position of one of the sources in the list is known, it may be used as a calibrator. In the example, all 10 fluxes of the example model used above are multiplied by a factor (2000/1900), to make the flux of the first one equal to 2000 W.U. At the same time, all positions are shifted.
+<P>
+******* Insert new script here ******
+<P>
+<A NAME=mdl.descr.handle-sort><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000> <b>Sorting</b></A></H2>
+<P>
+The source components may be sorted in many different ways. The option  SORT orders all components in order of decreasing flux. <i>This operation is performed before each WRITE, so that the components in an MDL file are always sorted this way!</i>.
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap274.png"> <b>MODEL_OPTION</b> 
+ (READ,WRITE,CLEAR,ZERO,SHOW, <IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap284.png">) 
+ = QUIT:  
+ <IMG ALIGN=BOTTOM ALT="" SRC="_7881_tex2html_wrap286.png">
+<P>
+FSORT allows the sorting on a range of criteria. In this example, the soorces are sorted in the order of decreasing m-coordinate:
+<P>
+****** Insert new script here *****
+<P>
+Other possibilities are:  <BR>- I:  amplitude  <BR>- L,M:  l or m  <BR>- LM,ML:  l and m, or m and l  <BR>- ID:  identification  <BR>- Q,U,V:  Q or U or V  <BR>- SI,RM:  spectral index or rotation measure  <BR>- LA,SA,PA: long or short axis, position angle  <BR>- BITS:  bits (i.e. if source is extended or has polarisation)  <BR>- TYP:  source type (0 is the standard)  <BR>- CC:  clean component  <BR>- TP2:  reserved  <BR>- DIST:  distance to a specified centre  <BR>- POL:  polarised intensity
+<P>
+<A NAME=mdl.descr.handle-edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004300000000000000> <b>Editing</b></A></H2>
+<P>
+Model components may be edited in various ways, using `handling' options CLEAR, ZERO, ADD, MERGE, DEL, DNCLOW, DCLOW (see the overview above). The handling options EDIT and FEDIT allow specific parameters (`fields') to be edited separately. EDIT acts on a specified source, and FEDIT acts on a range of sources. The possibilities are:
+<P>
+ <BR>- I:  amplitude  <BR>- L,M:  l or m  <BR>- ID:  identification  <BR>- Q,U,V:  Q or U or V  <BR>- SI,RM:  spectral index or rotation measure  <BR>- LA,SA,PA: long or short axis, position angle  <BR>- BITS:  bits (i.e. if source is extended or has polarisation)  <BR>- TYP:  source type (0 is the standard)  <BR>- CC:  clean component  <BR>- TP2:  reserved
+<P>
+<A NAME=mdl.descr.uvmodel><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>Conversion to a uv-model for the .SCN file</b></A></H1>
+<P>
+The calculation of uv-model data (for comparison with uv-data in NCALIB)i s time consuming. Therefore, a calculated uv-model is saved in the .SCN file for which it is calculated, together with the source list used. In all programs that use the model data it can be specified how the model calculation should be done, and if the calculation should be saved. The relevant question is MODEL_ACTION, which expects a list of three answers. The first one can be one of:
+<P>
+<UL><LI>   <b>merge:</b>     
+        replace the model saved in the SCN node with the one 
+                     specified by the user. However, first compare these two 
+                     lists, and only add the difference to the saved model data. 
+                     I.e. make the calculation as short as possible if the new 
+                     list differs only slightly from the saved one. 
+<LI>   <b>add:</b>       
+                replace the saved model with the sum of the saved one and 
+                     the one specified by the user. The model calculated on the 
+                     basis of the user specified list is added to the saved 
+                     data. 
+<LI>   <b>new:</b> 
+                replace the saved model by the model specified by the user, 
+                     and calculate a completely new set of model data 
+<LI>   <b>temporary:</b> 
+                do not use any data in the SCN node, or write anything, but 
+                     use the data based on the list specified by the user 
+<LI>   <b>increment:</b>         
+        use the saved model data, and add to it the model data 
+                    based on the user specified list, but do not save anything 
+</UL>
+<P>
+The second answer can be BAND or NOBAND, and specifies if in the model calculation source data should be corrected for bandsmearing to match the actual data better.  The third answer can be TIME or NOTIME to indicate the use of integration time smearing.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/mdlnode/mdlnode__input_mdl_node.html b/mdlnode/mdlnode__input_mdl_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..6127fbf894d956f4586596b3a0a66d4cbea16172
--- /dev/null
+++ b/mdlnode/mdlnode__input_mdl_node.html
@@ -0,0 +1,16 @@
+<TITLE>Description of INPUT_MDL_NODE (MDLNODE)</TITLE>
+<H1>Description of general keyword INPUT_MDL_NODE</H1>
+
+<DT><EM>Prompt:</EM> input .MDL file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the input .MDL filee name. <P>
+Enter ** (or e.g. /user0/mydata/**) to get a list of .MDL files in your current 
+(or the indicated) directory; then enter #&lt;n&gt; to select the &lt;n&gt;th file from 
+such a list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../mdlnode/mdlnode_comm.html">List of general keywords</A> for MDLNODE
+<LI>Description of the <A HREF="../mdl_descr/mdl_descr.html">MDL file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/mdlnode/mdlnode__mdl_node.html b/mdlnode/mdlnode__mdl_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..bba7d6c85f9c81fc9b4bf9fb7b3295d6e82b2f81
--- /dev/null
+++ b/mdlnode/mdlnode__mdl_node.html
@@ -0,0 +1,16 @@
+<TITLE>Description of MDL_NODE (MDLNODE)</TITLE>
+<H1>Description of general keyword MDL_NODE</H1>
+
+<DT><EM>Prompt:</EM> input/output .MDL file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the .MDL file name. <P>
+Enter ** (or e.g. /user0/mydata/**) to get a list of .MDL files in your current 
+(or the indicated) directory; then enter #&lt;n&gt; to select the &lt;n&gt;th file from 
+such a list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../mdlnode/mdlnode_comm.html">List of general keywords</A> for MDLNODE
+<LI>Description of the <A HREF="../mdl_descr/mdl_descr.html">MDL file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/mdlnode/mdlnode__output_mdl_node.html b/mdlnode/mdlnode__output_mdl_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..6e88d5a4f13b7a7fa4a6ccc9de5c2b75bd38c3e8
--- /dev/null
+++ b/mdlnode/mdlnode__output_mdl_node.html
@@ -0,0 +1,16 @@
+<TITLE>Description of OUTPUT_MDL_NODE (MDLNODE)</TITLE>
+<H1>Description of general keyword OUTPUT_MDL_NODE</H1>
+
+<DT><EM>Prompt:</EM> output .MDL file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the output .MDL file name. <P>
+Enter ** (or e.g. /user0/mydata/**) to get a list of .MDL files in your current 
+(or the indicated) directory; then enter #&lt;n&gt; to select the &lt;n&gt;th file from 
+such a list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../mdlnode/mdlnode_comm.html">List of general keywords</A> for MDLNODE
+<LI>Description of the <A HREF="../mdl_descr/mdl_descr.html">MDL file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/mdlnode_comm/mdlnode_comm.html b/mdlnode_comm/mdlnode_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..54996800af4194da4a2dfdc45928132de7961957
--- /dev/null
+++ b/mdlnode_comm/mdlnode_comm.html
@@ -0,0 +1,20 @@
+<TITLE>Index of general keywords from MDLNODE</TITLE>
+<H1>Description of general keywords (MDLNODE)</H1>
+
+<UL>
+<LI> <A HREF="../mdlnode/mdlnode__mdl_node.html">
+  MDL_NODE</A>
+  input/output .MDL file name
+<LI> <A HREF="../mdlnode/mdlnode__input_mdl_node.html">
+  INPUT_MDL_NODE</A>
+  input .MDL file name
+<LI> <A HREF="../mdlnode/mdlnode__output_mdl_node.html">
+  OUTPUT_MDL_NODE</A>
+  output .MDL file name
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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+y(such)g(a)h(list.)935 2995 y Fd(2)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/mdlnode_public_intfc/images.pl b/mdlnode_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/mdlnode_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/mdlnode_public_intfc/labels.pl b/mdlnode_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..7255b4e0629ca0bbee29238436a3e155028459d7
--- /dev/null
+++ b/mdlnode_public_intfc/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/mdlnode_public_intfc.html"; 
+$external_labels{".input.mdl.node"} ="$URL/mdlnode_public_intfc.html"; 
+$external_labels{".mdl.node"} ="$URL/mdlnode_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/mdlnode_public_intfc.html"; 
+$external_labels{".output.mdl.node"} ="$URL/mdlnode_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/mdlnode_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/mdlnode_public_intfc/mdlnode_public_intfc.html b/mdlnode_public_intfc/mdlnode_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..2f0fd02d7f14cd6f17b6e66d28e3682198fb95b4
--- /dev/null
+++ b/mdlnode_public_intfc/mdlnode_public_intfc.html
@@ -0,0 +1,125 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group MDLNODE</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=mdlnode_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=mdlnode_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=mdlnode_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=mdlnode_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=mdlnode_public_intfc.html#SECTION0003200000000000000>  <b>Parameter INPUT_MDL_NODE</b></A>
+<LI> <A NAME=tex2html6 HREF=mdlnode_public_intfc.html#SECTION0003300000000000000>  <b>Parameter MDL_NODE</b></A>
+<LI> <A NAME=tex2html7 HREF=mdlnode_public_intfc.html#SECTION0003400000000000000>  <b>Parameter OUTPUT_MDL_NODE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group MDLNODE, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.input.mdl.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter INPUT_MDL_NODE</b></A></H2>
+<P>
+  <em>Prompt:</em> input .MDL file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+    <PRE>
+        Specify the input .MDL filee name.
+</PRE>
+<P>
+  <PRE>
+Enter ** (or e.g. /user0/mydata/**) to get a list of .MDL files in your current
+(or the indicated) directory; then enter #<n> to select the <n>th file from
+such a list.
+</PRE>
+<P>
+<A NAME=.mdl.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter MDL_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> input/output .MDL file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the .MDL file name.
+</PRE>
+<P>
+  <PRE>
+Enter ** (or e.g. /user0/mydata/**) to get a list of .MDL files in your current
+(or the indicated) directory; then enter #<n> to select the <n>th file from
+such a list.
+</PRE>
+<P>
+<A NAME=.output.mdl.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter OUTPUT_MDL_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> output .MDL file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the output .MDL file name.
+</PRE>
+<P>
+  <PRE>
+Enter ** (or e.g. /user0/mydata/**) to get a list of .MDL files in your current
+(or the indicated) directory; then enter #<n> to select the <n>th file from
+such a list.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/memos.txt b/memos.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6fc76ebf4f0749ad7556c3bba1ad7c1bdc8c0983
--- /dev/null
+++ b/memos.txt
@@ -0,0 +1,145 @@
+The NEWSTAR memo system
+-----------------------
+
+This memo proposes a format for software memo series. 
+The vital element in this format is the Memo Header which gives
+all vital information. The various header elements are described 
+with their possible values,
+
+The only implementation currently available is for Newstar memo's. Some
+sample headers from this series are added.
+
+
+1. Function of memo's
+---------------------
+
+The function of a memo series is to document a design process and to 
+offer a convenient place where notes of various kinds can be dumped.
+
+In order to achieve this, it is essential that the header of each note
+clearly states what the purpose, subject and intended audience is.
+
+That way, it is sufficient to browse the headers of memo's in order
+to find information relevant to a certain person or problem
+
+
+2. Layout of memo headers
+-------------------------
+
+A memo header consists of the following fields, some of which are 
+required, others are optional:
+
+ * Name of memo series + index number                 [Required]
+
+   In fact the name of the memo series is a first order
+   selection of the intended audience. 
+   The serial number should be assigned on a central basis (preferably 
+   some automated procedure) and runs incrementally from 1.
+
+ * Subject                                            [Required]
+
+   The subject or description should be one line of highly descriptive
+   information. Since this line will show up in overview indices, 
+   it has to contain sufficient information to identify the scope
+   of the memo.
+
+ * Author                                             [Required]
+
+   This is just a textual identification. Preferably some database
+   with additional information on Memo authors should exist (including
+   up to date information on (eMail) addresses).
+
+ * Date                                               [Required]
+
+   This should be the date of issue of the original memo, for
+   updates see the next section
+
+ * Status                                             [Optional]
+
+   Possible values:  Info Proposal Design 
+
+   More than one value may be given, the list of possible values
+   may be extended
+
+   IF MISSING a status of Info should be assumed
+
+ * Action                                             [Optional]
+
+   Possible values:    Decision  Read  Feedback
+   Optional extension: "before <date>"
+
+   The action should be taken before the specified date, if no date
+   is given this is NOT equivalent to "as soon as possible" (in that
+   case a specific date should be given) but to "not necessary"
+
+   IF MISSING a status of Read should be assumed
+
+   
+ * To                                                 [Required]
+
+   The intended audience. This may be a specific name (e.g. Dr. P. Puk),
+   a generic name (WHISP Project Team) or The ... Memo Series
+
+ * Summary                                            [Required]
+
+   The full header including the summary should not exeed a single
+   page. Since Memo's are intended to be brief, no more than the
+   summary will be required in many cases.
+
+ * Replaces                                           [Optional]
+
+   Gives the numbers of the memo's that become obsolete by this one.
+
+ * Update on                                          [Optional]
+
+   Gives the numbers of the memo's are updated by this one.
+
+
+3. An example: the Newstar Memo Series
+--------------------------------------
+
+The Newstar memo series is part of the hypertext network of Newstar 
+documentation. The header layout in current practice does not follow
+the proposal in all details. 
+
+The body of the memo can be in any form (WP, ASCII text, Hypertext, LaTeX).
+In order enter the memo into the memo series, one enters the command
+
+    ndoc memo new [file]
+
+This will assign a unique number to the memo and create an empty memo
+header. You will be prompted for all header entries, and in addition 
+be asked for memo's, bug-reports and source files with which the memo 
+is concerned. These references appear as hypertext links in the on-line 
+version of the memo, and in normal text in the memo header.
+
+The specified file (which may be "none") will be moved into the directory
+with memo headers. The final header page will be presented for editing, 
+together with the associated file. This is the time to fill in the summary
+(which may be copied from the associated file).
+
+After completion, an index of all memo's will be automatically updated.
+
+
+4. Updates on existing memo's
+-----------------------------
+
+If a memo is updated, it is advised to enter the updates as a separate memo,
+indicating the differences only. If a modified text is stored, users are 
+forced to read through the entire memo and the preceding version to find 
+the differences. 
+
+Only if a memo has been changed substantially, so it is in fact better 
+to go through the whole text once more, a new memo can be created to 
+replace the original one.
+
+The header fields "Replaces" and "Update on" should be used to 
+indicate such cases.
+
+In the on-line implementation of the Newstar Memo Series, the headers
+of the updated/replaced memo's are modified to reflect this information
+as well. People keeping a paper copy can replace their header pages
+with the updates.
+
+
+
diff --git a/models_and_maps.txt b/models_and_maps.txt
new file mode 100644
index 0000000000000000000000000000000000000000..c4b4bd644dd816f2aa9185cd233dba4b269a8d14
--- /dev/null
+++ b/models_and_maps.txt
@@ -0,0 +1,89 @@
+How to apply models when making maps
+------------------------------------
+
+1e. Models and scanfiles
+------------------------
+
+Models can exist in two places:
+
+   1e. As a list of model parameters in a Model (MDL) file
+   2e. As a list of model parameters and complex uv-data points
+         in a Scan (SCN) file
+
+The model-list and the uv-model in a SCN file are always in accordance 
+with each other. 
+
+Models are update in the SCN files after a respons to the MODEL_ACTION 
+prompt. MODEL_ACTION is in fact: "What model is actually going to be used
+for processing and what model will finally end up in the SCN file?"
+
+The MODEL_ACTION question is asked in many cases:
+  1e. After the NMODEL option SAVE has been choosen
+  2e. After the NMAP option SUBTRACT has been choosen
+  3e. After the NCALIB option REDUNDANCY has been choosen
+  4e. After the NFLAG flagging operation ARESID has been choosen
+
+In all cases, the MODEL_ACTION is preceded by the MODEL_OPTION prompt.
+This allows you to create a temporary model list in memory by reading
+MDL files or by creating model components "by hand". The temporary model 
+list can be editied as well.
+
+The MODEL_ACTION determines what model is actually used in the 
+following processing AND what model is stored in the SCN file
+
+                         Used            Stored
+MERGE                  SCN ^ List       SCN ^ List
+ADD                    SCN + List       SCN + List
+NEW                      List             List
+TEMP                     List             SCN
+INCR                   SCN + List         SCN
+
+SCN:   Model currently present in the SCN file
+List:  Model currently in memory (constructed at MODEL_OPTION)
+ ^     Combination of two models, with common components occuring only
+         once in the final model
+ +     Addition of the two models, components occuring in both models
+         are added as well, so they get the double amplitude
+
+Obviously, options MERGE and NEW will be most commonly used.
+
+Apart from this choice, MODEL_ACTION lets you decide how the model should
+be calculated: should band smearing and time smearing be taken into account,
+should instrumental polarisation be taken into account.
+
+
+2. Subtracting models with NMAP
+-------------------------------
+
+There are two ways to subtract a model from uv-data before a map is made:
+
+  1e. In NMAP, answer SUBTRACT=YES
+
+      You will be asked for MODEL_OPTION to construct a temporary list,
+      and for MODEL_ACTION to determine what model is to be used.
+
+      This way you cannot use just the model that is present in the SCN file.
+
+      Also, you cannot use different models for different sets or different
+      SCN files (NMAP allows you to combine various SCN files, and to make 
+      several maps based on several groups etc)
+
+
+  2e. With NMAP, use DEAPPLY=MOD and SUBTRACT=NO
+
+      The uv-model in the SCN file(s) will be subtracted from the uv-data 
+      it corresponds to. The uv-model is considered a modification of the
+      visibilities corresponding to an empty sky. Deapplying this 
+      modification thus corresponds to subtraction of the uv-model.
+
+      This way, you can only use the model that is present in the SCN file.
+      This way, you can use different models for different groups in a SCN 
+      file, and different models for different SCN files.
+
+      However, you cannot add sources from another model, and you cannot
+      control the BAND/TIME/INPOL parameters (you should have done this when
+      you put the model in the SCN file).
+
+The same reasoning applies to NCALIB and NFLAG.
+
+
diff --git a/models_descr.ps b/models_descr.ps
new file mode 100644
index 0000000000000000000000000000000000000000..73f7890423d134c535e6bc5012522c639fdb383e
--- /dev/null
+++ b/models_descr.ps
@@ -0,0 +1,841 @@
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+627 y(the)h(data)g(as)f(wel)r(l)g(as)g(p)n(ossible)h(to)f(an)h
+(observation)g(in)f(a)h(.SCN)f(\014le.The)h(up)n(date)g(pr)n(o)n(c)n
+(ess)f(extr)n(acts)g(its)g(information)0 677 y(fr)n(om)g(r)n(esiduals)f
+(of)i(the)f(observe)n(d)g(visibilities)f(after)h(al)r(l)g(mo)n(del)g(c)
+n(omp)n(onents)h(of)f(typ)n(es)h(\(se)n(c.)k(3\))15 b(0)h(and)g(1)f
+(have)h(b)n(e)n(en)0 726 y(subtr)n(acte)n(d.)j(Up)n(dating)c(is)f(a)h
+(pr)n(o)n(c)n(ess)f(of)h(\014ne-tuning)h(the)f(p)n(ar)n(ameters)f(of)h
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+776 y(not)g(applic)n(able)g(to)g(cle)n(an)g(c)n(omp)n(onents.)118
+851 y(T)m(o)g(make)h(the)f(pr)n(o)n(c)n(ess)g(not)g(to)n(o)g(slow,)g(e)
+n(ach)31 b(sour)n(c)n(e)968 836 y Fe(29)1018 851 y Fj(c)n(omp)n(onent)
+16 b(is)f(\014tte)n(d)g(sep)n(ar)n(ately,)g(sp)n(e)n(cial)g(c)n(ar)n(e)
+g(b)n(eing)0 901 y(taken)d(that)g(c)n(omp)n(onents)g(close)g(to)n
+(gether)f(do)h(not)g(unduly)h(in\015uenc)n(e)g(e)n(ach)f(other's)f(up)n
+(dates.)18 b(F)m(or)12 b(the)f(pr)n(o)n(c)n(ess)h(to)f(work)0
+950 y(it)17 b(is)g(ne)n(c)n(essary)h(that)g(observation\(s\))f(sp)n(an)
+h(as)g(lar)n(ge)f(an)h(HA)f(r)n(ange)h(as)g(p)n(ossible;)g(otherwise)f
+(the)g(exact)h(distanc)n(e)0 1000 y(b)n(etwe)n(en)d(to)g(closely-sp)n
+(ac)n(e)n(d)f(c)n(omp)n(onents)i(is)f(di\016cult)f(to)h(determine.)118
+1075 y(The)e(\014tting)g(pr)n(o)n(c)n(ess)g(is)g(line)n(ar,)f(and)i
+(uses)f(b)n(oth)g(the)g(r)n(e)n(al)f(and)i(imaginary)f(p)n(arts)g(of)g
+(the)g(visibilities.)j(Sinc)n(e)e(the)0 1125 y(e)n(quations)g(use)n(d)g
+(ar)n(e)g(line)n(arize)n(d,)f(mor)n(e)g(than)h(one)h(iter)n(ation)e(is)
+g(in)h(gener)n(al)f(ne)n(e)n(de)n(d)i(for)e(the)h(pr)n(o)n(c)n(ess)f
+(to)h(c)n(onver)n(ge.)k(In)0 1175 y(the)c(e)n(quations)h(no)f(ac)n(c)n
+(ount)h(is)e(taken)i(of)f(se)n(c)n(ondary)g(e\013e)n(cts)h(\(e.g.)j(a)c
+(shift)g(in)g Fg(l,m)d Fj(wil)r(l)i(le)n(ad)h(to)g(di\013er)n(ent)g
+(amplitudes)0 1224 y(due)j(to)f(primary)f(b)n(e)n(am)h(and)h(fr)n(e)n
+(quency)f(dep)n(endencies\).)23 b(It)16 b(is)g(assume)n(d)g(that)g
+(these)h(e\013e)n(cts)f(wil)r(l)f(also)h(iter)n(ate)f(out.)0
+1274 y(In)i(those)g(c)n(ases)g(wher)n(e)f(this)g(do)n(es)i(not)f(happ)n
+(en,)h(it)e(pr)n(ob)n(ably)g(would)h(not)g(have)g(happ)n(ene)n(d)h(if)f
+(they)g(wer)n(e)e(taken)j(into)0 1324 y(ac)n(c)n(ount;)d(due)h(to)f
+(dep)n(endencies)h(b)n(etwe)n(en)f(e)n(quations.)p 0
+2792 756 2 v 31 2819 a Fd(28)64 2830 y Fc(nmo)q(del)p
+181 2830 11 2 v 10 w(descr)31 2858 y Fd(29)64 2870 y
+Fc(.source.com)o(p)q(o)o(nen)n(ts)935 2995 y Fg(4)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/models_descr/_8020_tex2html_wrap413.png b/models_descr/_8020_tex2html_wrap413.png
new file mode 100644
index 0000000000000000000000000000000000000000..273cf4f8f062a2787fbf4b7d3fba250dc4404acb
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diff --git a/models_descr/_8020_tex2html_wrap413.xbm b/models_descr/_8020_tex2html_wrap413.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b7d7180e479dc6553c07ddf123ffbacf1ac02ae9
--- /dev/null
+++ b/models_descr/_8020_tex2html_wrap413.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 10
+static char noname_bits[] = {
+ 0x78,0x30,0x18,0x18,0x18,0x18,0x0c,0x0c,0x0c,0x1f};
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new file mode 100644
index 0000000000000000000000000000000000000000..fbd2246d709467b44699ffe8b418bc9de5f85daf
Binary files /dev/null and b/models_descr/_8020_tex2html_wrap415.png differ
diff --git a/models_descr/_8020_tex2html_wrap415.xbm b/models_descr/_8020_tex2html_wrap415.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..c57055752361bb720e8467b274b0225e28cd33be
--- /dev/null
+++ b/models_descr/_8020_tex2html_wrap415.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 12
+static char noname_bits[] = {
+ 0x00,0x00,0x30,0x00,0x00,0x78,0x00,0x00,0x0c,0x00,0x00,0x7c,0x00,0x00,0x4c,
+ 0x00,0x00,0x4c,0xbe,0xef,0x7b,0xf3,0x68,0x02,0xc3,0xf8,0x01,0xc3,0xf8,0x03,
+ 0xe3,0x28,0x02,0x9e,0xef,0x03};
diff --git a/models_descr/_8020_tex2html_wrap417.png b/models_descr/_8020_tex2html_wrap417.png
new file mode 100644
index 0000000000000000000000000000000000000000..977f86cb45bf0de82d72541e3429ef8f2b8196d6
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diff --git a/models_descr/_8020_tex2html_wrap417.xbm b/models_descr/_8020_tex2html_wrap417.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..99d20be113cb1ac7393f6bf163aaa96928abb5ae
--- /dev/null
+++ b/models_descr/_8020_tex2html_wrap417.xbm
@@ -0,0 +1,11 @@
+#define noname_width 55
+#define noname_height 16
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x02,0x00,0xc0,0x0b,0x00,
+ 0x00,0x00,0x01,0x00,0x60,0x10,0x00,0x00,0x80,0x01,0x00,0xe0,0x33,0x00,0x00,
+ 0x80,0x00,0x00,0x60,0x22,0x00,0x00,0xc0,0x00,0x00,0x60,0x62,0xde,0xfd,0xc7,
+ 0xf8,0xbe,0xcf,0x63,0xb3,0xc7,0xcc,0xcc,0xa3,0x09,0x60,0x3f,0xc7,0xc8,0x0c,
+ 0xe3,0x07,0x60,0x03,0xc7,0xc8,0x0c,0xe3,0x0f,0x60,0xa3,0xcd,0xcc,0x8c,0xa3,
+ 0x08,0x60,0xde,0xdd,0xc7,0x78,0xbe,0x0f,0x60,0x00,0xc0,0x80,0x00,0x00,0x00,
+ 0x20,0x00,0xc0,0x80,0x01,0x00,0x00,0x30,0x00,0xe0,0x81,0x01,0x00,0x00,0x30,
+ 0x00,0x00,0x00,0x03,0x00,0x00,0x18};
diff --git a/models_descr/images.pl b/models_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..7041f91494f11bc86834366f79a0bf7211c69f60
--- /dev/null
+++ b/models_descr/images.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$I${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8020_tex2html_wrap413.xbm">'; 
+$key = q/{}$exp(cos^<<228>>6<<228>>)${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8020_tex2html_wrap417.xbm">'; 
+$key = q/{}$cos^<<227>>6<<227>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8020_tex2html_wrap415.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/models_descr/labels.pl b/models_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..68ef9c154f0e462520621d13868b90658ab890f0
--- /dev/null
+++ b/models_descr/labels.pl
@@ -0,0 +1,19 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".primary.beam"} ="$URL/models_descr.html"; 
+$external_labels{".model.to.vis"} ="$URL/models_descr.html"; 
+$external_labels{".source.components"} ="$URL/models_descr.html"; 
+$external_labels{".model.header"} ="$URL/models_descr.html"; 
+$external_labels{".type"} ="$URL/models_descr.html"; 
+$external_labels{".contents"} ="$URL/models_descr.html"; 
+$external_labels{".lm"} ="$URL/models_descr.html"; 
+$external_labels{".update"} ="$URL/models_descr.html"; 
+$external_labels{".general"} ="$URL/models_descr.html"; 
+$external_labels{".coord.conversions"} ="$URL/models_descr.html"; 
+$external_labels{".beamed"} ="$URL/models_descr.html"; 
+$external_labels{".merge.lists"} ="$URL/models_descr.html"; 
+$external_labels{".ref.coord"} ="$URL/models_descr.html"; 
+$external_labels{".instr.pol"} ="$URL/models_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/models_descr/models_descr.html b/models_descr/models_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..068eab55ba20e4423c6c047ebdc412d7d904c017
--- /dev/null
+++ b/models_descr/models_descr.html
@@ -0,0 +1,216 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Models in Newstar</b>
+<P>
+<i>(contributed by W.N. Brouw 931011, edited by J.P. Hamaker 940411) </i>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=models_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=models_descr.html#SECTION0002000000000000000> <b>General</b></A>
+<LI> <A NAME=tex2html3 HREF=models_descr.html#SECTION0003000000000000000> <b>Model header</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=models_descr.html#SECTION0003100000000000000>  <b>Conversions between coordinate types</b></A>
+</UL> 
+<LI> <A NAME=tex2html5 HREF=models_descr.html#SECTION0004000000000000000>  <b>Source components</b></A>
+<LI> <A NAME=tex2html6 HREF=models_descr.html#SECTION0005000000000000000>  <b>Merging model lists</b></A>
+<LI> <A NAME=tex2html7 HREF=models_descr.html#SECTION0006000000000000000>  <b>Conversion of a model to visibilities</b></A>
+<UL> 
+<LI> <A NAME=tex2html8 HREF=models_descr.html#SECTION0006100000000000000>  <b>Instrumental polarisation</b></A>
+</UL> 
+<LI> <A NAME=tex2html9 HREF=models_descr.html#SECTION0007000000000000000>  <b>Primary beam model</b></A>
+<LI> <A NAME=tex2html10 HREF=models_descr.html#SECTION0008000000000000000>  <b>Updating a model</b></A>
+</UL>
+<A NAME=.general><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>General</b></A></H1>
+<P>
+        Source models in Newstar are in principle meant to belong to a certain observation, although models can be converted from/to belonging to other observations.
+<P>
+<A NAME=.model.header><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>    
+<H1><A NAME=SECTION0003000000000000000> <b>Model header</b></A></H1>
+<P>
+        Each model has a header.  In this header the following information is stored:
+<P>
+<UL><LI>   <em>TYPE</em> 
+        of coordinates used. This can be: 
+        <UL><LI>    
+                <em>local:</em> 
+                no information is available about the observation to which the model pertains.  Whenever the model is used in connection with an observation, it will be assumed that the model header data are identical to the corresponding data in the observation.  
+                <LI> 
+                 <em>apparent</em> : 
+                it is assumed that all coordinates are apparent. 
+                <LI> 
+                 <em>epoch</em> : 
+                it is assumed that all coordinates belong to B1950 or J2000 
+        </UL>
+<P>
+<LI>   <em>EPOCH:</em> 1950 or 2000 (if <em>TYPE</em> =  <em>epoch</em> )
+<P>
+<LI>   <em>RA, DEC:</em>  <A NAME=.ref.coord><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+        the reference right-ascension and declination ( <em>apparent</em>  or 
+ <em>epoch</em> ) to which the <A HREF="#.lm"><em>l,m</em></A> coordinates of the <A HREF=".source.components">source</A>  components refer.  It is assumed that this is also the centre of the primary beam of the individual telescopes.
+<P>
+<LI>   <em>FREQ:</em> 
+        the frequency ...
+<P>
+<LI>   <em>INST:</em> 
+        the instrument used in the observation. 
+</UL>
+<P>
+<A NAME=.coord.conversions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>Conversions between coordinate types</b></A></H2>
+<P>
+        If the model list was made through the <b>ADD</b> and <b>EDIT</b> options of <A HREF="nmodel_descr">NMODEL</A> , the type will be  <em>local</em> .  If it is generated through 
+<A HREF="../nclean_descr/nclean_descr.html">NCLEAN</A> or the <b>FIND</b> option of <A HREF="nmodel_descr">NMODEL</A> , the type and other data are taken from the corresponding map.
+<P>
+        A  <em>local</em>  list can be converted to an  <em>apparent</em>  or  <em>epoch</em>  type though the <b>CONVERT</b> or <b>EDIT</b> options of <A HREF="nmodel_descr">NMODEL</A> .  In this case the reference data provided (either from a scan header or manually) will be copied into the model header.
+<P>
+        An  <em>apparent</em>  or  <em>epoch</em>  list can be converted to  <em>local</em>  in the same way.
+<P>
+        An  <em>apparent</em>  or  <em>epoch</em>  list can be converted to another 
+ <em>apparent</em>  or  <em>epoch</em>  list with the <A HREF="nmodel_descr">NMODEL</A>  <b>EDIT</b> or <b>CONVERT</b> options.  For <b>EDIT</b>, the new reference data from the user will replace the existing <A HREF=".model.header">header</A>  data, without changing the actual <A HREF=".source.components">source</A>  components.  <b>CONVERT</b> will also convert the existing <A HREF=".source.components">source</A>  and 
+<A HREF=".model.header">header</A>  data to the new coordinates, i.e.  the new source list will be for the new RA, DEC, FREQ, INST, using the model components' spectral index, rotation measure, primary beam and sky position.
+<P>
+        An  <em>apparent</em>  or  <em>epoch</em>  list can be converted to an  <em>epoch</em>  or 
+ <em>apparent</em>  list by <A HREF="nmodel_descr">NMODEL</A>  <b>EDIT</b> or <b>CONVERT</b>.  For <b>EDIT</b>, the new values will replace the old <A HREF=".model.header">header</A>  data, and only the change in direction to the North Pole ('phi') will be applied to the individual sources.  If <b>CONVERT</b>, only a reference scan can be used, and the 
+<A HREF=".source.components">source</A>  components will be shifted, rotated, beamed, spectrally indexed etc.  to the new coordinates.
+<P>
+<A NAME=.source.components><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>Source components</b></A></H1>
+<P>
+        Each source in the source model has the following information: 
+<UL><LI>   <em>INTENSITY:</em> 
+        intensity (STOKES <IMG ALIGN=BOTTOM ALT="" SRC="_8020_tex2html_wrap413.png">, in general in Westerbork Units) of the source.  This value is always posaitive.
+<P>
+<LI>   <em>L, M:</em>     <A NAME=.lm><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P>
+        the <em>l</em> and <em>m</em> coordinate on the sky for an E-W interferometer pointed at the  
+<A HREF="#.ref.coord">reference coordinates</A>  in the model header; <em>l</em> and <em>m</em> are thus given as offsets to the header position.
+<P>
+<LI>   <em>Q,U,V:</em> 
+        Stokes polarisation parameters as percentages of Stokes <em>I</em>
+<P>
+<LI>   <em>SI:</em> 
+        spectral index of the source
+<P>
+<LI>   <em>RM:</em> 
+        the rotation measure of the source
+<P>
+<LI>   <em>extension:</em> 
+        extension parameters of the source modeled as a two-dimensional Gaussian: length major axis, minor axis, position angle major axis.  For a point source, both axes have length 0.
+<P>
+<LI>   <em>source type:</em>      <A NAME=.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+        a number to be used to select particular sources only for certain operations.  In general only type 0 will be used in the programs (e.g.  self-calibration, updates, subtractions), but sometimes type = 1 are used (in a different way, e.g.  in 
+<A HREF="../nmodel_descr/nmodel_descr.html#.update">UPDATE</A> they will not be updated, but subtracted from the observations before updating starts).  Other types are not used at present.  The user can manually set them (NMODEL 
+<A HREF="../nmodel_descr/nmodel_descr.html#.edit">EDIT</A>) to e.g.  temporarily 'delete' them from his model.
+<P>
+<LI>   <em>ID:</em> 
+        a simple sequence number for easily keeping track of sources across sorting and updates etc.
+<P>
+<LI>   <em>MODE:</em> 
+        this is a bit mask with bits to indicate that the source is: 
+        <UL><LI>   <em>clean component:</em> 
+        the source has been found by <A HREF="../nclean_descr/nclean_descr.html">NCLEAN</A> and is constrained to lie on a map grid point and to be a point source.
+<P>
+        <LI>   <em>beamed:</em>   <A NAME=.beamed><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>   
+        the source intensity has been corrected for the primary beam of the instrument.  
+        </UL> 
+</UL>
+<P>
+        Whenever <A HREF="../nmodel_descr/nmodel_descr.html">NMODEL</A> <b>CONVERT</b> is used, the above data will be adjusted to reflect the new <A HREF=".model.header">header</A>  data.  Note that a <em>beamed</em> source will remain unchanged if the frequency and/or instrument is changed but no spectral index is available.
+<P>
+        All of the above information can be changed by the <A HREF="nmodel_descr">NMODEL</A>  HANDLE <b>EDIT</b> and <b>FEDIT</b> options.
+<P>
+        The <em>beam</em> mode can be changed (and the intensity changed) by the <A HREF="nmodel_descr">NMODEL</A>  <b>[DE]BEAM</b> options.  This operation will only be applied to sources for which it is appropriate.
+<P>
+<A NAME=.merge.lists><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000>  <b>Merging model lists</b></A></H1>
+<P>
+        Models can be combined with the <A HREF="nmodel_descr">NMODEL</A>  <b>xxx</b> option, provided either
+<P>
+<UL><LI> one of the types is  <em>local</em>  (in which case the other type will be assumed to be the correct one); or
+<P>
+<LI> both type are either  <em>apparent</em>  or  <em>epoch</em> .  </UL>
+<P>
+        The two models will be automatically converted and merged into a single model with one of the <A HREF=".model.header">header</A> s being used.
+<P>
+<A NAME=.model.to.vis><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000>  <b>Conversion of a model to visibilities</b></A></H1>
+<P>
+        Conversion of a model to visibilities always occurs in the context of a particular scan in a <A HREF="../scn_descr/scn_descr.html">SCN file</A>.  In this process, the model is automatically converted from the model-<A HREF=".model.header">header</A>  coordinates to those in the <A HREF="../scn_descr/scn_descr.html">scan header</A>.
+<P>
+        In this process, <A HREF="#.beamed"><em>beamed</em></A> <A HREF=".source.components">source</A>  components will be de-beamed before being used; <em>de-beamed</em> components will first be <em>beamed</em> for the header coordinates, then <em>de-beamed</em> for the scan coordinates).  In addition non-clean components will be <em>smeared</em> for the appropriate bandwidth and integration time.
+<P>
+        The user can suppress the smearing and the beaming operations (<A HREF="nmodel_descr">NMODEL</A>  <b>MODEL_ACTION</b> keyword).  He has no control over the other conversions (spectral index, different position etc.).
+<P>
+<A NAME=.instr.pol><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006100000000000000>  <b>Instrumental polarisation</b></A></H2>
+<P>
+        In addition to the corrections discussed so far, <em>position-dependent</em> instrumental polarisation (somewhat unfortunately often referred to as <em>cross polarisation</em>) should be corrected for in the calculation of model visibilities.  It is understood in principle how this must be done, but the implementation has been suspended until proper measured parameyters become available.
+<P>
+<A NAME=.primary.beam><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0007000000000000000>  <b>Primary beam model</b></A></H1>
+<P>
+        The primary beam for the <em>WSRT</em> is currently modeled as a circularly symmetric <IMG ALIGN=BOTTOM ALT="" SRC="_8020_tex2html_wrap415.png"> function.  Pointing measurements show that this is a good approximation out to the first null.  If positions further out were to be included, it would probably be better to model the beam as a J0 (Bessel) function or as an <IMG ALIGN=BOTTOM ALT="" SRC="_8020_tex2html_wrap417.png">.
+<P>
+        For the ATCA the beam is given as an inverse polynomial, which is correct to the first side-lobe (except for non-symmetry around the legs).
+<P>
+<A NAME=.update><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0008000000000000000>  <b>Updating a model</b></A></H1>
+<P>
+        The <A HREF="nmodel_descr">NMODEL</A>  <b>UPDATE</b>, <b>XUPDATE</b> and <b>SUPDATE</b> options try to match a givel source model the data as well as possible to an observation in a .SCN file.The update process extracts its information from residuals of the observed visibilities after all model components of <A HREF="#.type">types</A> 0 and 1 have been subtracted.  Updating is a process of fine-tuning the parameters of the model components and is therefore not applicable to clean components.
+<P>
+        To make the process not too slow, each <A HREF=".source.components">source</A>  component is fitted separately, special care being taken that components close together do not unduly influence each other's updates.  For the process to work it is necessary that observation(s) span as large an HA range as possible; otherwise the exact distance between to closely-spaced components is difficult to determine.
+<P>
+        The fitting process is linear, and uses both the real and imaginary parts of the visibilities.  Since the equations used are linearized, more than one iteration is in general needed for the process to converge.  In the equations no account is taken of secondary effects (e.g.  a shift in <em>l,m</em> will lead to different amplitudes due to primary beam and frequency dependencies).  It is assumed that these effects will also iterate out.  In those cases where this does not happen, it probably would not have happened if they were taken into account; due to dependencies between equations.
+<P>
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+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0xe0,0x00,0x00,0x60,0x00,0x1c,
+ 0xe0,0x00,0x38,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x0e,0xc0,0x01,0xc0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x62,0x00,0xc0,0x00,0x00,0x60,0x00,0x18,0xc0,
+ 0x00,0x30,0x00,0x08,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x0f,0xc0,0x01,0xe0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x03,0x00,0xc0,0x00,0x00,0x00,0x00,0x18,0xc0,0x00,
+ 0x30,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x08,0x80,0x01,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x03,0x00,0xc0,0x00,0x00,0x00,0x00,0x18,0xc0,0x00,0x30,
+ 0x00,0x0c,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x7f,0x08,
+ 0x8f,0x8f,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x70,0xf7,0xbe,0x77,0xbe,0xc7,0x80,0xe7,0x7e,0x1f,0x98,0xc7,0xc7,0x33,0xf8,
+ 0xde,0xbf,0x1f,0x3f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x08,0x9b,
+ 0x9d,0x1d,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x9a,0x3d,0x63,0xb3,0xcd,0x80,0xcd,0x63,0x13,0x98,0xcd,0x6c,0x36,0x98,0x8c,
+ 0x37,0x93,0x09,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x08,0x9f,0xd9,
+ 0x1f,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xfb,
+ 0x0d,0x63,0x03,0xcf,0x00,0x8f,0x63,0x0f,0x18,0xcf,0xe8,0x37,0x78,0x8c,0x31,
+ 0x93,0x09,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x88,0x9b,0xd9,0x1f,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x19,0x0c,
+ 0x6b,0x83,0xcd,0x80,0x8d,0x63,0x1f,0x98,0xcd,0x68,0x30,0xf8,0xac,0x31,0x13,
+ 0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x88,0x9b,0x9d,0x19,0x01,
+ 0xe0,0xe0,0x70,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x19,0x0d,0x6b,
+ 0xe3,0xdc,0xc0,0xdc,0x66,0x11,0xd8,0xdc,0x6c,0x34,0x88,0xac,0x31,0x13,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x7f,0xbf,0x8f,0xef,0x0f,0xe0,
+ 0xe0,0x70,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xf0,0x1e,0xff,0x9e,
+ 0xff,0x81,0xff,0xfe,0x1f,0xbc,0xdf,0xc7,0x7b,0xf8,0xfc,0xfb,0x3f,0x1f,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x31,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x31,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1f,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,
+ 0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x3e,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x37,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x33,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x33,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x37,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x7e,0x7e,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/mongo_graphics/images.pl b/mongo_graphics/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..5f254a8021b0e5c5ae3561de0328edcdb1273de0
--- /dev/null
+++ b/mongo_graphics/images.pl
@@ -0,0 +1,7 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{tabbing}+++=+++++++++++++=kill><verb_mark>2datagain64a.dat;html_special_mark_amp;>MONGOdatafile><verb_mark>3limits-570-1010;html_special_mark_amp;>><verb_mark>4xcol1;html_special_mark_amp;>x-valuesin1stcolumnofdatafile><verb_mark>5ycol2;html_special_mark_amp;>y-valuesin2ndcolumnofdatafile><verb_mark>6box;html_special_mark_amp;>drawaboxaroundtheplot><verb_mark>7ptype43;html_special_mark_amp;>><verb_mark>8connect;html_special_mark_amp;>><verb_mark>9xlabelchannel#;html_special_mark_amp;>horizontalaxislabelstring><verb_mark>10ylabel....;html_special_mark_amp;>verticalaxislabelstring><verb_mark>11id;html_special_mark_amp;>{tabbing}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8122_tabbing110.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/mongo_graphics/labels.pl b/mongo_graphics/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..46f9d16c7503d857ac9eeb0fef84f99d0deb5b11
--- /dev/null
+++ b/mongo_graphics/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".simple.plot"} ="$URL/mongo_graphics.html"; 
+
+1;
\ No newline at end of file
diff --git a/mongo_graphics/mongo_graphics.html b/mongo_graphics/mongo_graphics.html
new file mode 100644
index 0000000000000000000000000000000000000000..daa0b771413ca1c6b586ee18c3c9b852c10ad301
--- /dev/null
+++ b/mongo_graphics/mongo_graphics.html
@@ -0,0 +1,73 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>MONGO graphics</b>
+<P>
+In many cases, the user will need the results of <i>NEWSTAR </i> processing in graphical form. In order to make this easier, the output of programs like NGCALC can be specified to be in `MONGO' format. These are ASCII files, organised in columns, which can be processed by the MONGO graphics program. Because it is ASCII, the knowledgeable user can easily edit the file with a standard editor, to fine-tune the  resulting representation.
+<P>
+MONGO &#169;is an interactive graphics program, written by John L. Tonry. 
+For a detailed description, see the MONGO manual. In this section, a few simple examples are given to give the user the general idea, and to get him/her over the initial barrier.
+<P>
+In Dwingeloo, MONGO is only available on the VAX. Create the MONGO command by typing 
+<BR>tex2html_html_special_mark_ampMONGO :== @user5:[mongo]mongo.com&amp;
+<P>
+MONGO can be used interactively, or by means of a command ``macro'' (.MAC). The data usually reside in an ASCII data file, which may be edited by the user.
+<P>
+<A NAME=.simple.plot><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0000100000000000000> <b>A simple MONGO plot</b></A></H2>
+<P>
+Create a MONGO data file (extension .DAT). This is an ASCII, in which the data is lined up in columns. In this case, replace the string &quot;.....&quot; in the first column with 0,1,2,3 etc to indicate channel nr.
+<P>
+Then make a MONGO command macro (ext .MAC): 
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_8122_tabbing110.png"><P>
+<P>
+Alternative: use MONGO interactively.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/more_on_batch.txt b/more_on_batch.txt
new file mode 100644
index 0000000000000000000000000000000000000000..306b40f416cb11255f2113d065c7b1bf84fe5801
--- /dev/null
+++ b/more_on_batch.txt
@@ -0,0 +1,230 @@
+Fm: Marco de Vos (Newstar Project Team)
+To: Ulrich Schwarz & Paul Stoppelenburg
+
+Subject: 
+Hints for batchprocessing with Newstar
+--------------------------------------
+
+
+A. Layout for a batch-script
+----------------------------
+
+Batch-scripts always have the follwing layout:
+
+>>>>>>>>>>>>>>>>>>> Example follows below this line >>>>>>>>>>>
+#!/bin/csh -f
+#
+# Startup Newstar
+#
+source ~newstar/src/sys/newstar_rug.csh
+
+#
+# Maybe some identification
+#
+echo "Name of the script: $0"     # Prints the name of the file
+echo "Purpose: ....."             # Print the purpose of the file
+
+#
+# Clear all symbols
+#
+dwc '*$ch0'
+
+#
+# Define the symbols for this job
+#
+dws nmap\$ch0 /nomenu <<_EOD_
+OPTION=MAKE;QUIT ! The QUIT is for final exit
+LOOPS="";#       ! The # is in case we want to stop at the SCN_NODE prompt
+SCN_NODE=obs2; ""/ask    ! Just set the two defaults (/ASK)
+SCN_SETS=0.0.0.0.0
+HA_RANGE= -90,90
+SELECT_IFRS= -mm,-ff;""  ! The second answer should be ""
+... etc ...
+#
+_EOD_
+
+#
+#  Start the program
+#
+dwe nmap\$ch0
+
+#
+#  End
+#
+<<<<<<<<<<<<<<<< End of example <<<<<<<<<<<<<<<<<<<<<<<<<<<<<<
+
+
+There may be many different dws and dwe commands in a single file.
+
+In stead of typing  nmap\$0  you can also use  'nmap$0'  .
+
+
+
+
+B. Starting a batch-script
+--------------------------
+
+To start such a batch script, just type it's name, eg:
+
+  > nmap0.scr
+
+This may give a message like:     nmap0.scr: Permission denied.
+
+In that case you sould first type:
+
+  > chmod a+x nmap0.scr
+
+to change the mode ("protection") of the file such that All users 
+can eXecute it. You probably created the script from scratch with 
+an editor, so Unix treated it as an ordinary text file.
+
+
+
+C. Starting batch jobs in the background
+----------------------------------------
+
+To start a batch job in the background, leaving your terminal free
+for other work, just type the following:
+
+   > nmap0.scr >& output_file &
+
+All output that normally was shown on your screen will now end up in 
+the file named output_file (you can use any name you like).
+
+To check wether the job is finished you can try:
+
+   > more output_file           shows all of the "screen output"
+   > tail output_file           shows the last 20 lines or so
+   > ps lws | grep nmap0.scr    shows the status of the process (with
+                                 elapsed time etc.), no output means
+                                 the batch is finished
+
+There is a Newstar command which will execute a job in the background
+and send the output to you by mail when it finishes. Just type:
+
+   > nspawn nmap0.scr 
+
+The "screen output" will end up in  nmap0.scr.output. 
+The mail will be sent using elm with the command as subject.
+
+NOTA BENE: If you start a job in the background, all parameters should
+           be known in advance. So you should not use /ASK when specifying
+           parameters.
+
+
+
+D. How to set the keywords for a program
+----------------------------------------
+
+In a batch-script, you can set keywords in two different ways:
+
+1e. Use the dwspecify (dws) command:
+
+dws nmap\$ch0 /nomenu <<_EOD_
+OPTION=first_answer;second_answer;third_answer
+SCN_NODE=TEST;""
+#
+_EOD_
+
+The sequence of the keywords is not relevant.
+Each keyword should be set like: KEYWORD= value (not: nmap$ch0_keyword=value).
+You can only specify the keywords for one program (and one stream).
+
+You can enter the KEYWORD=value lines by hand, or edit the output
+from dwsave (remove the PROGRAM$Stream_ prefixes!)
+
+Alternatively you can extract keywords from a logfile:
+
+   >  grep '^>' NMAP.LOG | sed -e 's/^>//'  > output_file
+
+If this seems an interesting option, I will create a Newstar command
+for it (to save innocent Unix users all the '^>' things).
+
+
+2e. Use the dwrestore command:
+
+
+Typically, you will now do the following:
+
+ > dwe ncalib\$ch0 /norun/save
+ > dwe nmap\$ch0 /norun/save
+ > dwsave nmap\$ch0 /output=nmap0.keys
+
+Now you may want to edit nmap0.keys, which contains lines like:
+
+ NMAP$1_LOOPS=""";#"
+ NMAP$1_OPTION="MAKE;#"
+ NMAP$1_RUN="YES"
+ NMAP$1_SCN_NODE=""""
+
+In the batch script, you say:
+
+dwrestore nmap0.keys
+
+
+3e. Combine the use of dws and dwrestore
+
+
+Suppose we want to do a job repeatedly with the parameters saved above,
+but with only SCN_SETS differing from command to command. We may then
+combine dws and dwrestore as follows:
+
+
+#!bin/csh
+#!/bin/csh -f
+#
+# Startup Newstar
+#
+source ~newstar/src/sys/newstar_rug.csh
+
+#
+# Maybe some identification
+#
+echo "Name of the script: $0"     # Prints the name of the file
+echo "Purpose: ....."             # Print the purpose of the file
+
+#
+# Clear all symbols
+#
+dwc '*'
+
+#
+# Set up all "global" symbols for this job
+#
+dwrestore nmap0.keys
+
+#
+# Start a loop over the sets
+#
+foreach set ( 0 1 3 4 )
+
+#
+# Define SCN_SETS for ncalib
+#
+dws ncalib\$ch0 /nomenu <<_EOD_
+SCN_SETS=0.0.$set
+#
+_EOD_
+
+#
+# Run ncalib for this set
+#
+dwe ncalib\$ch0
+
+#
+# Define SCN_SETS for nmap
+#
+dws nmap\$ch0 /nomenu <<_EOD_
+SCN_SETS=0.0.$set
+#
+_EOD_
+
+#
+# Run ncalib for this set
+#
+dwe nmap\$ch0
+
+#
+# Next set
+#
+end 
diff --git a/natnf/natnf__continuum.html b/natnf/natnf__continuum.html
new file mode 100644
index 0000000000000000000000000000000000000000..633dc1a828fa318c823efc7d9ecebfdff0671a32
--- /dev/null
+++ b/natnf/natnf__continuum.html
@@ -0,0 +1,18 @@
+<TITLE>Description of CONTINUUM (NATNF)</TITLE>
+<H1>Program NATNF: private keyword CONTINUUM</H1> 
+
+<DT><EM>Prompt:</EM> define channels for continuum
+<DT><EM>Expected input:</EM> Integer number, 16 values.<P>
+A continuum channel can be made by specifying up to 8 pairs of channel numbers. 
+The channel values will be averaged to produce a single continuum value. Each 
+pair specifies a low and high channel number to be included. <P>
+Special values: 
+  ""      No continuum wanted 
+  *       Central 75% of channels used <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__input_bands.html b/natnf/natnf__input_bands.html
new file mode 100644
index 0000000000000000000000000000000000000000..884c3221416269cacef8ac3ddb0bba4388db0e3b
--- /dev/null
+++ b/natnf/natnf__input_bands.html
@@ -0,0 +1,14 @@
+<TITLE>Description of INPUT_BANDS (NATNF)</TITLE>
+<H1>Program NATNF: private keyword INPUT_BANDS</H1> 
+
+<DT><EM>Prompt:</EM> input bands in cm
+<DT><EM>Expected input:</EM> Real number, 16 values.<P>
+Specify the bands to be read (20 etc in octave steps. * specifies all bands on 
+the tape <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__input_channels.html b/natnf/natnf__input_channels.html
new file mode 100644
index 0000000000000000000000000000000000000000..ffeb3ed06f821fa870b62064b8f8ea66a0e2a38f
--- /dev/null
+++ b/natnf/natnf__input_channels.html
@@ -0,0 +1,13 @@
+<TITLE>Description of INPUT_CHANNELS (NATNF)</TITLE>
+<H1>Program NATNF: private keyword INPUT_CHANNELS</H1> 
+
+<DT><EM>Prompt:</EM> input channels
+<DT><EM>Expected input:</EM> Integer number, 256 values; min.value: 1.000000.<P>
+Specify the channels (1, ..) to be read. * specifies all channels on the tape  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__input_file.html b/natnf/natnf__input_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..d08c08532b91249caa16f4d5eff6440c1583d785
--- /dev/null
+++ b/natnf/natnf__input_file.html
@@ -0,0 +1,14 @@
+<TITLE>Description of INPUT_FILE (NATNF)</TITLE>
+<H1>Program NATNF: private keyword INPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> input filename
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the input filename (without an extension for the LOAD from disk 
+option).  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__input_labels.html b/natnf/natnf__input_labels.html
new file mode 100644
index 0000000000000000000000000000000000000000..a4f83fc6fa3b498afc8c82b4987cd757ae5dc8f1
--- /dev/null
+++ b/natnf/natnf__input_labels.html
@@ -0,0 +1,13 @@
+<TITLE>Description of INPUT_LABELS (NATNF)</TITLE>
+<H1>Program NATNF: private keyword INPUT_LABELS</H1> 
+
+<DT><EM>Prompt:</EM> input labels
+<DT><EM>Expected input:</EM> Integer number, 256 values.<P>
+Specify the tape labels to be read. * specifies all labels on the tape  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__input_sources.html b/natnf/natnf__input_sources.html
new file mode 100644
index 0000000000000000000000000000000000000000..8c695e40e5f14573434abb4e727ad0fd3313c006
--- /dev/null
+++ b/natnf/natnf__input_sources.html
@@ -0,0 +1,13 @@
+<TITLE>Description of INPUT_SOURCES (NATNF)</TITLE>
+<H1>Program NATNF: private keyword INPUT_SOURCES</H1> 
+
+<DT><EM>Prompt:</EM> sources to get
+<DT><EM>Expected input:</EM> Character(16), 256 values.<P>
+Specify the sources to be read. * specifies all sources on the tape <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__integration_time.html b/natnf/natnf__integration_time.html
new file mode 100644
index 0000000000000000000000000000000000000000..724c83df5d7adbd037e01b171cb718625ebf0c7f
--- /dev/null
+++ b/natnf/natnf__integration_time.html
@@ -0,0 +1,13 @@
+<TITLE>Description of INTEGRATION_TIME (NATNF)</TITLE>
+<H1>Program NATNF: private keyword INTEGRATION_TIME</H1> 
+
+<DT><EM>Prompt:</EM> integration time (sec)
+<DT><EM>Expected input:</EM> Real number; min.value: 10.000000; max.value: 3600.000000.<P>
+Specify the integration time per scan.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__option.html b/natnf/natnf__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..76084239adba669192d281d7e96fbfa0c7a9ca61
--- /dev/null
+++ b/natnf/natnf__option.html
@@ -0,0 +1,15 @@
+<TITLE>Description of OPTION (NATNF)</TITLE>
+<H1>Program NATNF: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> LOAD, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify action to perform: <P>
+  LOAD    load RPFITS data into scan file 
+  QUIT    finish <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf/natnf__start_offset.html b/natnf/natnf__start_offset.html
new file mode 100644
index 0000000000000000000000000000000000000000..4d5e377baee14d762c23eac90c1c08e759273776
--- /dev/null
+++ b/natnf/natnf__start_offset.html
@@ -0,0 +1,16 @@
+<TITLE>Description of START_OFFSET (NATNF)</TITLE>
+<H1>Program NATNF: private keyword START_OFFSET</H1> 
+
+<DT><EM>Prompt:</EM> scan start offset (sec)
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000; max.value: 180.000000.<P>
+Often the first 10 sec of a scan are bad. By specifying an offset here, the 
+first n seconds of a scan will be discarded. E.g. specifying an integration of 
+70 sec and an offset of 10 sec will produce 4 points for a 5 min observation,  
+discarding the first and last 10 sec.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../natnf/natnf_keys.html">List of keywords</A> for NATNF
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/natnf_keys/natnf_keys.html b/natnf_keys/natnf_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..2683ea10c2fa498447fdca002bbb4438fcdae410
--- /dev/null
+++ b/natnf_keys/natnf_keys.html
@@ -0,0 +1,55 @@
+<TITLE>Index of private keywords for NATNF </TITLE>
+<H1>Description of keywords for program NATNF</H1>
+
+<UL>
+<LI> <A HREF="../natnf/natnf__option.html">
+  OPTION</A>
+  LOAD, QUIT
+<LI> <A HREF="../natnf/natnf__input_file.html">
+  INPUT_FILE</A>
+  input filename
+<LI> <A HREF="../natnf/natnf__input_labels.html">
+  INPUT_LABELS</A>
+  input labels
+<LI> <A HREF="../natnf/natnf__input_sources.html">
+  INPUT_SOURCES</A>
+  sources to get
+<LI> <A HREF="../natnf/natnf__input_bands.html">
+  INPUT_BANDS</A>
+  input bands in cm
+<LI> <A HREF="../natnf/natnf__input_channels.html">
+  INPUT_CHANNELS</A>
+  input channels
+<LI> <A HREF="../natnf/natnf__integration_time.html">
+  INTEGRATION_TIME</A>
+  integration time (sec)
+<LI> <A HREF="../natnf/natnf__start_offset.html">
+  START_OFFSET</A>
+  scan start offset (sec)
+<LI> <A HREF="../natnf/natnf__continuum.html">
+  CONTINUUM</A>
+  define channels for continuum
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../unit_comm/unit_comm.html">UNIT</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../natnf_descr/natnf_descr.html">program NATNF</A>
+</UL>
diff --git a/natnf_private_intfc.ps b/natnf_private_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..bdff1589cec2ced0b673070f59052222b0da1609
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NATNF</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=natnf_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=natnf_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=natnf_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=natnf_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=natnf_private_intfc.html#SECTION0003200000000000000>  <b>Parameter CONTINUUM</b></A>
+<LI> <A NAME=tex2html6 HREF=natnf_private_intfc.html#SECTION0003300000000000000>  <b>Parameter INPUT_BANDS</b></A>
+<LI> <A NAME=tex2html7 HREF=natnf_private_intfc.html#SECTION0003400000000000000>  <b>Parameter INPUT_CHANNELS</b></A>
+<LI> <A NAME=tex2html8 HREF=natnf_private_intfc.html#SECTION0003500000000000000>  <b>Parameter INPUT_FILE</b></A>
+<LI> <A NAME=tex2html9 HREF=natnf_private_intfc.html#SECTION0003600000000000000>  <b>Parameter INPUT_LABELS</b></A>
+<LI> <A NAME=tex2html10 HREF=natnf_private_intfc.html#SECTION0003700000000000000>  <b>Parameter INPUT_SOURCES</b></A>
+<LI> <A NAME=tex2html11 HREF=natnf_private_intfc.html#SECTION0003800000000000000>  <b>Parameter INTEGRATION_TIME</b></A>
+<LI> <A NAME=tex2html12 HREF=natnf_private_intfc.html#SECTION0003900000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html13 HREF=natnf_private_intfc.html#SECTION00031000000000000000>  <b>Parameter START_OFFSET</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NATNF. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>.
+<P>
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../unit_public_intfc/unit_public_intfc.html">UNIT</A> public keywords 
+</UL>
+<P>
+<A NAME=.continuum><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter CONTINUUM</b></A></H2>
+<P>
+  <em>Prompt:</em> define channels for continuum<BR><em>Expected input:</em> Integer:  1 to 16 values
+<P>
+    <PRE>
+A continuum channel can be made by specifying up to 8 pairs of channel numbers.
+The channel values will be averaged to produce a single continuum value. Each
+pair specifies a low and high channel number to be included.
+</PRE>
+<P>
+  <PRE>
+Special values:
+  ""      No continuum wanted
+  *       Central 75%
+</PRE>
+<P>
+<A NAME=.input.bands><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter INPUT_BANDS</b></A></H2>
+<P>
+<em>Prompt:</em> input bands in cm<BR><em>Expected input:</em> Real:  1 to 16 values
+<P>
+  <PRE>
+Specify the bands to be read (20 etc in octave steps. * specifies all bands on
+the tape
+</PRE>
+<P>
+<A NAME=.input.channels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter INPUT_CHANNELS</b></A></H2>
+<P>
+<em>Prompt:</em> input channels<BR><em>Expected input:</em> Integer:  1 to 256 values
+<P>
+  <PRE>
+Specify the channels (1,..) to be read. * specifies all channels on the tape
+</PRE>
+<P>
+<A NAME=.input.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter INPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> input filename<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the input filename (without an extension for the LOAD from disk
+option).
+</PRE>
+<P>
+<A NAME=.input.labels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter INPUT_LABELS</b></A></H2>
+<P>
+<em>Prompt:</em> input labels<BR><em>Expected input:</em> Integer:  1 to 256 values
+<P>
+  <PRE>
+Specify the tape labels to be read. * specifies all labels on the tape
+</PRE>
+<P>
+<A NAME=.input.sources><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter INPUT_SOURCES</b></A></H2>
+<P>
+<em>Prompt:</em> sources to get<BR><em>Expected input:</em> Character *16:  1 to 256 values
+<P>
+  <PRE>
+Specify the sources to be read. * specifies all sources on the tape
+</PRE>
+<P>
+<A NAME=.integration.time><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter INTEGRATION_TIME</b></A></H2>
+<P>
+<em>Prompt:</em> integration time (sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the integration time per scan.
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+  LOAD    load RPFITS data into scan file
+  QUIT    finish
+</PRE>
+<P>
+<A NAME=.start.offset><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter START_OFFSET</b></A></H2>
+<P>
+<em>Prompt:</em> scan start offset (sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Often the first 10 sec of a scan are bad. By specifying an offset here, the
+first n seconds of a scan will be discarded. E.g. specifying an integration of
+70 sec and an offset of 10 sec will produce 4 points for a 5 min observation,
+discarding the first and last 10 sec.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ncalib/ncalib__align_option.html b/ncalib/ncalib__align_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..358a925117b6007cfdb8f8263185fa8d11be8ebf
--- /dev/null
+++ b/ncalib/ncalib__align_option.html
@@ -0,0 +1,28 @@
+<TITLE>Description of ALIGN_OPTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword ALIGN_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Type of Selfcal desired SELFCAL, ALIGN
+<DT><EM>Expected input:</EM> Character(8).<P>
+Selfcal is the generic name for all methods that use a source model in 
+combination with your visibilities to estimate the telecope gain/phase 
+corrections. Since you have selected a model, NCALIB assumes that you want to 
+use it, by doing a Selfcal. (If you had not, it would propose a REDUNdancy-only 
+solution.) <P>
+The alternative you have here is to use the source model to recover the unknown 
+position shift that scans suffer when they are processed with the  redundancy 
+constraints only (REDUN solution). In this operation the source model is only 
+used as a position reference. The telescope phases are shifted by an amount 
+that is a linear function of position along the array; the telescope gains do 
+not change at all. <P>
+To summarise, the choices you have are: <P>
+   SELFCAL       use the model to constrain in position a redundancy solution 
+                  that will be made now 
+   ALIGN         use the model to constrain a redundancy solution that was made 
+                  earlier  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__basel_check.html b/ncalib/ncalib__basel_check.html
new file mode 100644
index 0000000000000000000000000000000000000000..a0637ce42d9f964cf7932f4b1af45e7bad2691a1
--- /dev/null
+++ b/ncalib/ncalib__basel_check.html
@@ -0,0 +1,15 @@
+<TITLE>Description of BASEL_CHECK (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword BASEL_CHECK</H1> 
+
+<DT><EM>Prompt:</EM> Redundant-baseline difference allowed (metres)
+<DT><EM>Default:</EM> .5.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.001000; max.value: 10.000000.<P>
+Specify the maximum difference between baselines for them still to be 
+considered identical in Redundancy calculations.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__basel_dx.html b/ncalib/ncalib__basel_dx.html
new file mode 100644
index 0000000000000000000000000000000000000000..524b35891f8d46ecfcb8014bb1922c874be184f4
--- /dev/null
+++ b/ncalib/ncalib__basel_dx.html
@@ -0,0 +1,19 @@
+<TITLE>Description of BASEL_DX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword BASEL_DX</H1> 
+
+<DT><EM>Prompt:</EM> Increments to telescope X positions (mm) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the X telescope corrections in mm, one value per telescope. <P>
+The correction will be added as an HA-dependent phase to the OTH telescope 
+corrections. It can only be undone by either zeroing the entire OTH corrections 
+by means of the SET ZERO option (which will destroy whatever other corrections 
+have been stored there), or by inserting the same BASEL_DX value with opposite 
+sign. <P>
+The default value 0, 0, ...0, 0 leaves the corrections unchanged. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__basel_dy.html b/ncalib/ncalib__basel_dy.html
new file mode 100644
index 0000000000000000000000000000000000000000..d77a917a7138df17e73a50d61428983b1f6b9d60
--- /dev/null
+++ b/ncalib/ncalib__basel_dy.html
@@ -0,0 +1,19 @@
+<TITLE>Description of BASEL_DY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword BASEL_DY</H1> 
+
+<DT><EM>Prompt:</EM> Increments to telescope Y positions (mm) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify 14 Y telescope corrections in mm, one value per telescope. <P>
+The correction will be added as an HA-dependent phase to the OTH telescope 
+corrections. It can only be undone by either zeroing the entire OTH corrections 
+by means of the SET ZERO option (which will destroy whatever other corrections 
+have been stored there), or by inserting the same BASEL_DY value with opposite 
+sign. <P>
+The default value 0, 0, ...0, 0 leaves the corrections unchanged. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__basel_dz.html b/ncalib/ncalib__basel_dz.html
new file mode 100644
index 0000000000000000000000000000000000000000..91b4b0e5d78f599a219b4504e591209bf8120bea
--- /dev/null
+++ b/ncalib/ncalib__basel_dz.html
@@ -0,0 +1,19 @@
+<TITLE>Description of BASEL_DZ (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword BASEL_DZ</H1> 
+
+<DT><EM>Prompt:</EM> increments to telescope Z positions (mm) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the Z telescope corrections in mm, one value per telescope. <P>
+The correction will be added as an HA-dependent phase to the OTH telescope 
+corrections. It can only be undone by either zeroing the entire OTH corrections 
+by means of the SET ZERO option (which will destroy whatever other corrections 
+have been stored there), or by inserting the same BASEL_DZ value with opposite 
+sign. <P>
+The default value 0, 0, ...0, 0 leaves the corrections unchanged. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__basel_pole.html b/ncalib/ncalib__basel_pole.html
new file mode 100644
index 0000000000000000000000000000000000000000..472f58a7cceaae5480ba21469cdc9b4533612e90
--- /dev/null
+++ b/ncalib/ncalib__basel_pole.html
@@ -0,0 +1,19 @@
+<TITLE>Description of BASEL_POLE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword BASEL_POLE</H1> 
+
+<DT><EM>Prompt:</EM> "Increment to baseline-pole declination correction (deg) |"
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the baseline-pole declination correction in degrees. <P>
+The correction will be added as an HA-dependent phase to the OTH telescope 
+corrections. It can only be undone by either zeroing the entire OTH corrections 
+by means of the SET ZERO option (which will destroy whatever other corrections 
+have been stored there), or by inserting the same BASEL_POLE value with 
+opposite sign.. <P>
+The default value 0 leaves the corrections unchanged. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__cal_equal.html b/ncalib/ncalib__cal_equal.html
new file mode 100644
index 0000000000000000000000000000000000000000..37acc2d472e3c925d96e104fcd5005b48b5d23a1
--- /dev/null
+++ b/ncalib/ncalib__cal_equal.html
@@ -0,0 +1,18 @@
+<TITLE>Description of CAL_EQUAL (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword CAL_EQUAL</H1> 
+
+<DT><EM>Prompt:</EM> Copy with equal length?
+<DT><EM>Default:</EM> NO /NOASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+If YES, all calibrators specified with USE_SCN_SETS will be made of equal 
+length, that is: the number of HA scans used for each calibrator will be the 
+same (and equal to the smallest number available). <P>
+This is necessary when calibrators have frequencies that have been offset (plus 
+and minus respectively) to the observing frequency of the target source.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__checks.html b/ncalib/ncalib__checks.html
new file mode 100644
index 0000000000000000000000000000000000000000..c72243984fa512b40d3a2cd1404cd7753c4d4c9f
--- /dev/null
+++ b/ncalib/ncalib__checks.html
@@ -0,0 +1,21 @@
+<TITLE>Description of CHECKS (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword CHECKS</H1> 
+
+<DT><EM>Prompt:</EM> Iterations, gain deviation, relative mean error: 3 values|
+<DT><EM>Default:</EM> 20, 1E-3, 3.
+<DT><EM>Expected input:</EM> Real number, 3 values; min.value: 5.000000; max.value: 50.000000.<P>
+Specify: <P>
+
+<DT>   - the maximum number of iterations in the complex solution; <P>
+
+<DT>   - the relative allowable gain deviation for successive complex solutions; <P>
+
+<DT>   - the mean error allowed per scan, relative to the average mean error 
+        for all scans already solved. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__clock_corr.html b/ncalib/ncalib__clock_corr.html
new file mode 100644
index 0000000000000000000000000000000000000000..5853c0bd0916ea55f1a9264cd2d228faeb2c578d
--- /dev/null
+++ b/ncalib/ncalib__clock_corr.html
@@ -0,0 +1,14 @@
+<TITLE>Description of CLOCK_CORR (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword CLOCK_CORR</H1> 
+
+<DT><EM>Prompt:</EM> Clock correction (sec)
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the clock correction in seconds to be applied to data. The new value 
+will be ADDED to the existing one. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__complex.html b/ncalib/ncalib__complex.html
new file mode 100644
index 0000000000000000000000000000000000000000..8d326f37ed0a04b8b1584c92e10d1910636703d5
--- /dev/null
+++ b/ncalib/ncalib__complex.html
@@ -0,0 +1,14 @@
+<TITLE>Description of COMPLEX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword COMPLEX</H1> 
+
+<DT><EM>Prompt:</EM> Complex solution (YES/NO)?
+<DT><EM>Default:</EM> YES.
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want a complex solution of gains-plus-phases. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__complex_only.html b/ncalib/ncalib__complex_only.html
new file mode 100644
index 0000000000000000000000000000000000000000..723a7c5995dde465b904e5b6afbdf9b7a25195a2
--- /dev/null
+++ b/ncalib/ncalib__complex_only.html
@@ -0,0 +1,16 @@
+<TITLE>Description of COMPLEX_ONLY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword COMPLEX_ONLY</H1> 
+
+<DT><EM>Prompt:</EM> Complex solution only (YES/NO)?
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want ONLY a complex solution. <P>
+Note: will only work if an initial guess for the gains (e.g. from a calibrator) 
+has been specified  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__continuity.html b/ncalib/ncalib__continuity.html
new file mode 100644
index 0000000000000000000000000000000000000000..4da1b06e4794fe4ac8c0bc659a3676670718fc3d
--- /dev/null
+++ b/ncalib/ncalib__continuity.html
@@ -0,0 +1,16 @@
+<TITLE>Description of CONTINUITY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword CONTINUITY</H1> 
+
+<DT><EM>Prompt:</EM> Continuity in solution (YES/NO)?
+<DT><EM>Default:</EM> YES.
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want continuity in gain solution. If not, the initial guess for 
+the solution will be 0 (gain) and the forced phases (phase), else the solution 
+found in a previous scan.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__dshift.html b/ncalib/ncalib__dshift.html
new file mode 100644
index 0000000000000000000000000000000000000000..7b303a1b5920cab25c4fc67ea774a36d1592d842
--- /dev/null
+++ b/ncalib/ncalib__dshift.html
@@ -0,0 +1,20 @@
+<TITLE>Description of DSHIFT (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword DSHIFT</H1> 
+
+<DT><EM>Prompt:</EM> Shift rate (dl/dt, dm/dt, arcsec/day)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the SHIFT rate in arcsec per sidereal day to be applied to the data 
+whenever the DE_APPLY SHIFT correction is requested. <P>
+This parameter is used for a first-order approximation to the proper motion of 
+a solar-system object through the formula: <P>
+        Total shift =  SHIFT + DSHIFT * (HA-HAB) <P>
+where hour angles are measured as fractions of a full circle and HAB is the 
+starting HA of the sector. 
+!               \whichref{}{}. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__extinction.html b/ncalib/ncalib__extinction.html
new file mode 100644
index 0000000000000000000000000000000000000000..4d2ccc37d6a25717b62f1a07b28ab2430d0366a6
--- /dev/null
+++ b/ncalib/ncalib__extinction.html
@@ -0,0 +1,16 @@
+<TITLE>Description of EXTINCTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword EXTINCTION</H1> 
+
+<DT><EM>Prompt:</EM> Extinction-1: quadratic's coefficients|
+<DT><EM>Default:</EM> .00557, .00461, -.000544.
+<DT><EM>Expected input:</EM> Real number, 3 values.<P>
+Specify the coefficients A, B and C in the quadratic representation of the 
+zenith extinction oefficient as a function of frequency F in GHz: <P>
+        EXT= (1+A) + B*F +C*F*F <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__faraday_file.html b/ncalib/ncalib__faraday_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..7a386d11c4c297e98f3263ce56dee14fab8309b7
--- /dev/null
+++ b/ncalib/ncalib__faraday_file.html
@@ -0,0 +1,18 @@
+<TITLE>Description of FARADAY_FILE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword FARADAY_FILE</H1> 
+
+<DT><EM>Prompt:</EM> Faraday-rotation data file
+<DT><EM>Expected input:</EM> Character(160).<P>
+Specify the name of a file with Faraday rotation data. The file must be an 
+ASCII file with lines <P>
+        &lt;hour angle in degrees&gt;, &lt;faraday rotation in degrees at 1GHz&gt; <P>
+The file will be used to calculate Faraday rotation values for each scan by 
+interpolation between the values in this file and scaling to the observing 
+frequency. The calculated values will be stored in the scans as corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__flw_factor.html b/ncalib/ncalib__flw_factor.html
new file mode 100644
index 0000000000000000000000000000000000000000..eb8cdb311b3c588879ae8b8ead9d8783ea4fd2be
--- /dev/null
+++ b/ncalib/ncalib__flw_factor.html
@@ -0,0 +1,21 @@
+<TITLE>Description of FLW_FACTOR (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword FLW_FACTOR</H1> 
+
+<DT><EM>Prompt:</EM> Weight for points flagged with WGT flag
+<DT><EM>Default:</EM> 1.
+<DT><EM>Expected input:</EM> Real number.<P>
+The WGT flag directs NCALIB to multiply the data weight with an additional 
+weighing factor. <P>
+You may use this feature to reduce the weight of data affected by interference 
+without rejecting it completely. The effect of this in a Selfcal solution is 
+that it prevents the interference from bad interferometers to infect the 
+healthy ones. <P>
+A value of 1 will give all interferometers the weight they have in the .SCN 
+file.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__force_freedom.html b/ncalib/ncalib__force_freedom.html
new file mode 100644
index 0000000000000000000000000000000000000000..fcc9239389421ff0b62c334e4b10f912bfae0049
--- /dev/null
+++ b/ncalib/ncalib__force_freedom.html
@@ -0,0 +1,17 @@
+<TITLE>Description of FORCE_FREEDOM (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword FORCE_FREEDOM</H1> 
+
+<DT><EM>Prompt:</EM>   Manual constraints for gain (1st value)|-
+and phase (2nd value)? YES/NO
+<DT><EM>Expected input:</EM> Logical, 2 values.<P>
+Specify if you want to force the constraint equations for the align solution. 
+If you reply NO, the program will determine them by itself from the 
+interferometers selected. <P>
+Your first reply refers to Gain, the second one to Phase. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__force_phase.html b/ncalib/ncalib__force_phase.html
new file mode 100644
index 0000000000000000000000000000000000000000..982f8f27788643d06a48d6003c075e711fc22fe5
--- /dev/null
+++ b/ncalib/ncalib__force_phase.html
@@ -0,0 +1,16 @@
+<TITLE>Description of FORCE_PHASE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword FORCE_PHASE</H1> 
+
+<DT><EM>Prompt:</EM> Define phase-zeroes
+<DT><EM>Default:</EM> 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0.
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Define initial phase zeros per telescope. <P>
+This is useful for pathological cases where NCALIB on its own cannot correctly 
+resolve the 360-deg phase ambiguities.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__freq_corr.html b/ncalib/ncalib__freq_corr.html
new file mode 100644
index 0000000000000000000000000000000000000000..776dfae261e959c2e2b61f6a49b32520d947e401
--- /dev/null
+++ b/ncalib/ncalib__freq_corr.html
@@ -0,0 +1,23 @@
+<TITLE>Description of FREQ_CORR (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword FREQ_CORR</H1> 
+
+<DT><EM>Prompt:</EM> Increment to frequency correction (MHz)
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the 'frequency correction' in MHz. <P>
+This is an idiosyncratic way of representing a correction to the metric scale 
+of the interferometer array: A scale correction with a factor (1+x) is 
+represented by correcting the nominal observing frequency F with an additive 
+term -x.F. <P>
+Clearly this does not represent a real frequency shift since the observing 
+frequency is precisely defined by the settings of local-oscillator frequencies 
+and fringe-stopping parameters during the observation. <P>
+The correction will be ADDED as an hour-angle-dependent phase to the OTH 
+telescope corrections, and can only be undone by either zeroing these 
+corrections, or inserting the same BASEL_POLE value with opposite sign.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_freedom.html b/ncalib/ncalib__gain_freedom.html
new file mode 100644
index 0000000000000000000000000000000000000000..95a5da74633a771b87f1ff1cfbd76c6784f1cc75
--- /dev/null
+++ b/ncalib/ncalib__gain_freedom.html
@@ -0,0 +1,17 @@
+<TITLE>Description of GAIN_FREEDOM (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_FREEDOM</H1> 
+
+<DT><EM>Prompt:</EM> Gain grouping
+<DT><EM>Expected input:</EM> Integer number, 14 values.<P>
+Define the telescope groups for which the gains will be solved independently. <P>
+To solve e.g. separate gains for the 10 fixed telescopes (0 through 9) and the 
+ 4 movable ones (A through D), specify: <P>
+        1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 2, 2, 2, 2 <P>
+* means one group containing all telescopes (i.e. 1, 1, ..., 1, 1).  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_norm.html b/ncalib/ncalib__gain_norm.html
new file mode 100644
index 0000000000000000000000000000000000000000..61b7fef35045b4c769766f5ed75b6d6bfae7a214
--- /dev/null
+++ b/ncalib/ncalib__gain_norm.html
@@ -0,0 +1,31 @@
+<TITLE>Description of GAIN_NORM (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_NORM</H1> 
+
+<DT><EM>Prompt:</EM> Gain reference telescopes
+<DT><EM>Expected input:</EM> Integer number, 14 values.<P>
+Define the telescopes to be used as reference for renormalising the telescope 
+gains. <P>
+Your reply should be an array of values (separated by commas) for telescopes 0 
+through D; 1 means that you select the telescope, 0 that you don't. Trailing 0s 
+may be omitted. <P>
+A wildcard ('*') means 'all', i.e. 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1 <P>
+Example: 
+        0, 1, 0, 1, 0 means 'use telescopes 1 and 3 as reference' <P>
+NOTES: <P>
+Renormalisation adjusts the gains so that the average for the fixed telescopes 
+selected equals that for the moving telescopes. If either group is absent from 
+yous selection, the average gain of the other group is made 0. <P>
+Consequently, proper gain renormalisation is possible only for the 'standard' 
+WSRT configuration: If there are any fixed-fixed or movable-movable 
+interferometers, a message will be given and the operation aborted. <P>
+You may, however, insist by putting a -1 instead of any of the 1s in your 
+reply. The renormalisation will then be performed as if the fixed-movable 
+interferometers were absent, and a warning given that the gain corrections for 
+those interferometers are jeopardized. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_x.html b/ncalib/ncalib__gain_x.html
new file mode 100644
index 0000000000000000000000000000000000000000..e9db62b55d02d35c0d4261f4ecad27e226ae50c0
--- /dev/null
+++ b/ncalib/ncalib__gain_x.html
@@ -0,0 +1,16 @@
+<TITLE>Description of GAIN_X (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_X</H1> 
+
+<DT><EM>Prompt:</EM> Gain corrections X (factors) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the X gain corrections per telescope as factors (1= no change). <P>
+The values you give will be multiplied with the existing gain factors if you 
+choose SET option MULT, they will replace the existing factors if you choose 
+SET option MANUAL. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_xx.html b/ncalib/ncalib__gain_xx.html
new file mode 100644
index 0000000000000000000000000000000000000000..94dbe754e18d1dcfc1bea54b31be85172e2e2bb7
--- /dev/null
+++ b/ncalib/ncalib__gain_xx.html
@@ -0,0 +1,15 @@
+<TITLE>Description of GAIN_XX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_XX</H1> 
+
+<DT><EM>Prompt:</EM> Interferometer gain corrections XX (factors) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the gain corrections for XX as factors (1= no change). You will be 
+prompted for values, which will OVERWRITE the existing interferometer gain 
+corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_xy.html b/ncalib/ncalib__gain_xy.html
new file mode 100644
index 0000000000000000000000000000000000000000..55dce03fb9d480fa989d02a0107f08292c97a936
--- /dev/null
+++ b/ncalib/ncalib__gain_xy.html
@@ -0,0 +1,15 @@
+<TITLE>Description of GAIN_XY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_XY</H1> 
+
+<DT><EM>Prompt:</EM> interferometer gain corrections XY (factors) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the gain corrections for XY as factors (1= no change). You will be 
+prompted for values, which will OVERWRITE the existing interferometer gain 
+corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_y.html b/ncalib/ncalib__gain_y.html
new file mode 100644
index 0000000000000000000000000000000000000000..da9a2d6ee4ce5247a09eb5cb609c7d76e38e2e2c
--- /dev/null
+++ b/ncalib/ncalib__gain_y.html
@@ -0,0 +1,16 @@
+<TITLE>Description of GAIN_Y (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_Y</H1> 
+
+<DT><EM>Prompt:</EM> Gain corrections Y (factors) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the Y gain corrections per telescope as factors (1= no change). <P>
+The values you give will be multiplied with the existing gain factors if you 
+choose SET option MULT, they will replace the existing factors if you choose 
+SET option MANUAL. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_yx.html b/ncalib/ncalib__gain_yx.html
new file mode 100644
index 0000000000000000000000000000000000000000..5ebf2100a5903446c985ec6bb88f6752d2000ee1
--- /dev/null
+++ b/ncalib/ncalib__gain_yx.html
@@ -0,0 +1,15 @@
+<TITLE>Description of GAIN_YX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_YX</H1> 
+
+<DT><EM>Prompt:</EM> interferometer gain corrections YX (factors) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the gain corrections for YX as factors (1= no change). You will be 
+prompted for values, which will OVERWRITE the existing interferometer 
+corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__gain_yy.html b/ncalib/ncalib__gain_yy.html
new file mode 100644
index 0000000000000000000000000000000000000000..38e40341c995d7c4b32ac0207ccdc5c7b111f647
--- /dev/null
+++ b/ncalib/ncalib__gain_yy.html
@@ -0,0 +1,15 @@
+<TITLE>Description of GAIN_YY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword GAIN_YY</H1> 
+
+<DT><EM>Prompt:</EM> interferometer gain corrections YY (factors) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the gain corrections for YY as factors (1= no change). You will be 
+prompted for values, which will OVERWRITE the existing interferometer 
+corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__ha_integration.html b/ncalib/ncalib__ha_integration.html
new file mode 100644
index 0000000000000000000000000000000000000000..f1ea559eb6f4a7cdcaae1c8158eb0caaefb0c1e1
--- /dev/null
+++ b/ncalib/ncalib__ha_integration.html
@@ -0,0 +1,17 @@
+<TITLE>Description of HA_INTEGRATION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword HA_INTEGRATION</H1> 
+
+<DT><EM>Prompt:</EM> Integration time (sec)
+<DT><EM>Expected input:</EM> Real number; max.value: 3600.000000.<P>
+Specify the time interval over which you want to integrate (if possible) before 
+calibrating. The value you specify will be rounded down to a multiple of the 
+hour-angle interval between successive scans. <P>
+'*' and '0' mean do not integrate, i.e. calibrate per scan. <P>
+The largest value allowed is 3600 (= 1 hour).  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__ifr_xx.html b/ncalib/ncalib__ifr_xx.html
new file mode 100644
index 0000000000000000000000000000000000000000..3d201687d817c0c333ed7515e03a9fb0183ec559
--- /dev/null
+++ b/ncalib/ncalib__ifr_xx.html
@@ -0,0 +1,14 @@
+<TITLE>Description of IFR_XX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword IFR_XX</H1> 
+
+<DT><EM>Prompt:</EM> additive interferometer corrections cos, sin XX (W.U.) |
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the additive interferometer corrections for XX in Westerbork Units 
+(W.U.). The values you specify will OVERWRITE any existing values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__ifr_xy.html b/ncalib/ncalib__ifr_xy.html
new file mode 100644
index 0000000000000000000000000000000000000000..a9a97efc71932bd32330e6d5d3e224e31c4869c3
--- /dev/null
+++ b/ncalib/ncalib__ifr_xy.html
@@ -0,0 +1,14 @@
+<TITLE>Description of IFR_XY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword IFR_XY</H1> 
+
+<DT><EM>Prompt:</EM> additive interferometer corrections cos, sin XY (W.U.) |
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the additive interferometer corrections for XY in Westerbork Units 
+(W.U.). The values you specify will OVERWRITE any existing values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__ifr_yx.html b/ncalib/ncalib__ifr_yx.html
new file mode 100644
index 0000000000000000000000000000000000000000..94008c56c64d23b5b33c6c367e95066116c3d805
--- /dev/null
+++ b/ncalib/ncalib__ifr_yx.html
@@ -0,0 +1,14 @@
+<TITLE>Description of IFR_YX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword IFR_YX</H1> 
+
+<DT><EM>Prompt:</EM> additive interferometer corrections cos, sin YX (W.U.) |
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the additive interferometer corrections for YX in Westerbork Units 
+(W.U.). The values you specify will OVERWRITE any existing values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__ifr_yy.html b/ncalib/ncalib__ifr_yy.html
new file mode 100644
index 0000000000000000000000000000000000000000..acff2b1fd2ff48e99623d05a528f55f7d983ae17
--- /dev/null
+++ b/ncalib/ncalib__ifr_yy.html
@@ -0,0 +1,14 @@
+<TITLE>Description of IFR_YY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword IFR_YY</H1> 
+
+<DT><EM>Prompt:</EM> additive interferometer corrections cos, sin YY (W.U.) |
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the additive interferometer corrections for YY in  Westerbork Units 
+(W.U.). The values you specify will OVERWRITE any existing values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__irefract_file.html b/ncalib/ncalib__irefract_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..5d76e410899db7927b229b30c23b039e4ead7c6d
--- /dev/null
+++ b/ncalib/ncalib__irefract_file.html
@@ -0,0 +1,18 @@
+<TITLE>Description of IREFRACT_FILE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword IREFRACT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> Ionospheric refraction data file
+<DT><EM>Expected input:</EM> Character(160).<P>
+Specify the name of a file with ionospheric refraction data. The file must be 
+an ASCII file with lines <P>
+        &lt;hour angle in degrees&gt;, &lt;refraction in degrees/km at 1GHz&gt; <P>
+The file will be used to calculate ionospheric refraction for each scan by 
+interpolation between the values in this file and scaling to the observing 
+frequency. The calculated values will be stored in the scans as corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__mweight_data.html b/ncalib/ncalib__mweight_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..2b4a1a1a9a0d7fed660e183b49bf433964136a38
--- /dev/null
+++ b/ncalib/ncalib__mweight_data.html
@@ -0,0 +1,16 @@
+<TITLE>Description of MWEIGHT_DATA (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword MWEIGHT_DATA</H1> 
+
+<DT><EM>Prompt:</EM> Centre, halfwidth (metres)
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.000000.<P>
+Specify the centre and the halfpower-halfwidth in metres of the model weight 
+function to be applied. <P>
+Only positive values are accepted. Note that the function you define may extend 
+over negative baselines but actual baselines are positive by definition. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__mweight_type.html b/ncalib/ncalib__mweight_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..3b95dc2b0a692b4c65cdd632fc6cc2ca7296dce0
--- /dev/null
+++ b/ncalib/ncalib__mweight_type.html
@@ -0,0 +1,22 @@
+<TITLE>Description of MWEIGHT_TYPE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword MWEIGHT_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> Type of weight function| STEP, ISTEP; GAUSSIAN, IGAUSSIAN; TRIANGLE, ITRIANGLE
+<DT><EM>Expected input:</EM> Character(10).<P>
+MWEIGHT_TYPE and MWEIGHT_DATA allow you to weigh baselines according to their 
+lengths, in order to take advantage of source characteristics that are a priori 
+known. The defaults for these parameters give all baselines the same weight. <P>
+This parameter selects the form of the weighting function; its position and 
+half-width will be defined by MWEIGHT_DATA. The following shapes can be chosen: <P>
+   STEP          a step function: 1 out to some radius, 0 beyond 
+   GAUSSIAN      a Gaussian 
+   TRIANGLE      a triangular function: linearly decreasing from 1 to 0 <P>
+   Each of these can be prefixed with an 'I' to invert it, i.e. ISTEP means 
+    '1 minus STEP'  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__ons.html b/ncalib/ncalib__ons.html
new file mode 100644
index 0000000000000000000000000000000000000000..5ea4f4c27d7421dac57e936fb1335094e2d68a7b
--- /dev/null
+++ b/ncalib/ncalib__ons.html
@@ -0,0 +1,22 @@
+<TITLE>Description of ons (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword ons</H1> 
+
+<DT><EM>Prompt:</EM> MULT, POLE, DX, DY, DZ, FREQ, QUIT SET action (others)|
+<DT><EM>Expected input:</EM> Character(6).<P>
+Specify action to perform to ADD corrections into the OTHer telescope 
+corrections: <P>
+ 
+        MULT    set an extra gain factor (multiply existing values) 
+        DX      add telescope X correction in selected scans 
+        DY      add telescope Y correction in selected scans 
+        DZ      add telescope Z correction in selected scans 
+        POLE    add baseline pole correction in selected scans 
+        FREQ    add frequency offset correction in selected scans <P>
+        QUIT    exit SET  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__option.html b/ncalib/ncalib__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..bb5da5b1bbc2b069cc9d3c32b4ae9a193ce02074
--- /dev/null
+++ b/ncalib/ncalib__option.html
@@ -0,0 +1,19 @@
+<TITLE>Description of OPTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Type of action  REDUNDANCY, POLAR, SET; SHOW; QUIT
+<DT><EM>Expected input:</EM> Character(12).<P>
+Specify type of action to perform: <P>
+   REDUNDANCY    create telescope corrections by solving the 
+                  redundancy/align/selfcal equations 
+   POLAR         operations on polarisation corrections 
+   SET           operations on all other corrections <P>
+   SHOW          show (in logfile) average corrections in specified sector(s) 
+   QUIT          finish <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__oth_option.html b/ncalib/ncalib__oth_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..d3fbcb8729523c865923f7d5229a0edfaa3d4a26
--- /dev/null
+++ b/ncalib/ncalib__oth_option.html
@@ -0,0 +1,21 @@
+<TITLE>Description of OTH_OPTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword OTH_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> MULT, POLE, DX, DY, DZ, FREQ, QUIT SET action (others)|
+<DT><EM>Expected input:</EM> Character(6).<P>
+Specify action to perform to ADD corrections into the OTHer telescope 
+corrections: <P>
+        MULT    set an extra gain factor (multiply existing values) 
+        DX      add telescope X correction in selected scans 
+        DY      add telescope Y correction in selected scans 
+        DZ      add telescope Z correction in selected scans 
+        POLE    add baseline pole correction in selected scans 
+        FREQ    add frequency offset correction in selected scans <P>
+        QUIT    exit SET  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_freedom.html b/ncalib/ncalib__phase_freedom.html
new file mode 100644
index 0000000000000000000000000000000000000000..8e182f39160fad253f1faff2e81302e8c108d604
--- /dev/null
+++ b/ncalib/ncalib__phase_freedom.html
@@ -0,0 +1,18 @@
+<TITLE>Description of PHASE_FREEDOM (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_FREEDOM</H1> 
+
+<DT><EM>Prompt:</EM> Phase grouping
+<DT><EM>Expected input:</EM> Integer number, 14 values.<P>
+Define the telescope groups for which the phases will be solved independently. <P>
+To solve e.g. separate gains for the 10 fixed telescopes (0 through 9) and the 
+ 4 movable ones (A through D), specify: <P>
+        1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 2, 2, 2, 2 <P>
+* means one group containing all telescopes (i.e. 1, 1, ..., 1, 1). Up to 14 groups 
+may be defined.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_norm.html b/ncalib/ncalib__phase_norm.html
new file mode 100644
index 0000000000000000000000000000000000000000..0faa8be635e4d40cad137e2a6ae2532f356064d7
--- /dev/null
+++ b/ncalib/ncalib__phase_norm.html
@@ -0,0 +1,20 @@
+<TITLE>Description of PHASE_NORM (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_NORM</H1> 
+
+<DT><EM>Prompt:</EM> Phase reference telescopes
+<DT><EM>Expected input:</EM> Integer number, 14 values.<P>
+Define the telescopes to use as reference for renormalising the telescope 
+phases. <P>
+Your reply should be an array of values (separated by commas) for telescopes 0 
+through D; 1 means that you select the telescope, 0 that you don't. Trailing 0s 
+may be omitted. <P>
+A wildcard ('*') means 'all', i.e. 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1, 1 <P>
+Example: 
+        0, 1, 0, 1, 0 means 'use telescopes 1 and 3 as reference <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_x.html b/ncalib/ncalib__phase_x.html
new file mode 100644
index 0000000000000000000000000000000000000000..6025e7f71406a1525ee076e8f5b9578df7e272ee
--- /dev/null
+++ b/ncalib/ncalib__phase_x.html
@@ -0,0 +1,16 @@
+<TITLE>Description of PHASE_X (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_X</H1> 
+
+<DT><EM>Prompt:</EM> Phase corrections X (deg) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the X phase corrections to be added per telescope (0 = no change). <P>
+The values you give will be added to the existing OTHer phases if you choose 
+SET option MULT, they will replace the existing phases if you choose SET option 
+MANUAL. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_xx.html b/ncalib/ncalib__phase_xx.html
new file mode 100644
index 0000000000000000000000000000000000000000..ae038c2c1779435bcc0fb250f74c0bb3e428737c
--- /dev/null
+++ b/ncalib/ncalib__phase_xx.html
@@ -0,0 +1,14 @@
+<TITLE>Description of PHASE_XX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_XX</H1> 
+
+<DT><EM>Prompt:</EM> interferometer phase corrections XX (deg) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the phase corrections for XX. You will be prompted for values, which 
+will OVERWRITE the existing interferometer corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_xy.html b/ncalib/ncalib__phase_xy.html
new file mode 100644
index 0000000000000000000000000000000000000000..9802b2d7dfa220a97062f2b636c44650b4b4aee6
--- /dev/null
+++ b/ncalib/ncalib__phase_xy.html
@@ -0,0 +1,14 @@
+<TITLE>Description of PHASE_XY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_XY</H1> 
+
+<DT><EM>Prompt:</EM> interferometer phase corrections XY (deg) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the phase corrections for XY. You will be prompted for values, which 
+will OVERWRITE the existing interferometer corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_y.html b/ncalib/ncalib__phase_y.html
new file mode 100644
index 0000000000000000000000000000000000000000..a7e8bb93fb3c02b45836d67ed6f7a1af5bee6028
--- /dev/null
+++ b/ncalib/ncalib__phase_y.html
@@ -0,0 +1,16 @@
+<TITLE>Description of PHASE_Y (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_Y</H1> 
+
+<DT><EM>Prompt:</EM> Phase corrections Y (deg) |
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the Y phase corrections to be added per telescope (0 = no change). <P>
+The values you give will be added to the existing OTHer phases if you choose 
+SET option MULT, they will replace the existing phases if you choose SET option 
+MANUAL. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_yx.html b/ncalib/ncalib__phase_yx.html
new file mode 100644
index 0000000000000000000000000000000000000000..1a0ce6d68238226f9291e1a5461200e791b5156f
--- /dev/null
+++ b/ncalib/ncalib__phase_yx.html
@@ -0,0 +1,14 @@
+<TITLE>Description of PHASE_YX (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_YX</H1> 
+
+<DT><EM>Prompt:</EM> interferometer phase corrections YX (deg) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the phase corrections for YX. You will be prompted for values, which 
+will OVERWRITE the existing interferometer corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__phase_yy.html b/ncalib/ncalib__phase_yy.html
new file mode 100644
index 0000000000000000000000000000000000000000..a628d98946cdfa23b299466b953452c20eebfcc1
--- /dev/null
+++ b/ncalib/ncalib__phase_yy.html
@@ -0,0 +1,14 @@
+<TITLE>Description of PHASE_YY (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword PHASE_YY</H1> 
+
+<DT><EM>Prompt:</EM> interferometer phase corrections YY (deg) |
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+Specify the phase corrections for YY. You will be prompted for values, which 
+will OVERWRITE the existing interferometer corrections.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__pol_orthog.html b/ncalib/ncalib__pol_orthog.html
new file mode 100644
index 0000000000000000000000000000000000000000..1514e1fdb50ac72a92c8d267dbedaba5bb869861
--- /dev/null
+++ b/ncalib/ncalib__pol_orthog.html
@@ -0,0 +1,14 @@
+<TITLE>Description of POL_ORTHOG (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword POL_ORTHOG</H1> 
+
+<DT><EM>Prompt:</EM> Dipole orthogonalities (deg)|
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the deviations from orthogonality in the dual-dipole assemblies per 
+telescope in degrees. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__pol_rotan.html b/ncalib/ncalib__pol_rotan.html
new file mode 100644
index 0000000000000000000000000000000000000000..9378f407e83d8f8bcaa7cce006e5b383a287e229
--- /dev/null
+++ b/ncalib/ncalib__pol_rotan.html
@@ -0,0 +1,14 @@
+<TITLE>Description of POL_ROTAN (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword POL_ROTAN</H1> 
+
+<DT><EM>Prompt:</EM> Dipole positions (deg)|
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the position angles of the dual-dipole assemblies per telescope in 
+degrees. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__pol_x_ellips.html b/ncalib/ncalib__pol_x_ellips.html
new file mode 100644
index 0000000000000000000000000000000000000000..b1592b62d136d912f97ab28051214402eabdb557
--- /dev/null
+++ b/ncalib/ncalib__pol_x_ellips.html
@@ -0,0 +1,13 @@
+<TITLE>Description of POL_X_ELLIPS (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword POL_X_ELLIPS</H1> 
+
+<DT><EM>Prompt:</EM> X-dipole ellipticities (%)|
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the X-dipole ellipticities per telescope in %. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__pol_y_ellips.html b/ncalib/ncalib__pol_y_ellips.html
new file mode 100644
index 0000000000000000000000000000000000000000..507bef8028f2d7930a159f840d712762d22647ec
--- /dev/null
+++ b/ncalib/ncalib__pol_y_ellips.html
@@ -0,0 +1,13 @@
+<TITLE>Description of POL_Y_ELLIPS (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword POL_Y_ELLIPS</H1> 
+
+<DT><EM>Prompt:</EM> Y-dipole ellipticities (%)|
+<DT><EM>Expected input:</EM> Real number, 14 values.<P>
+Specify the Y-dipole ellipticities per telescope in %. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__polar_option.html b/ncalib/ncalib__polar_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..cc1eaf0728e492d746a21113b02d392ce4561efb
--- /dev/null
+++ b/ncalib/ncalib__polar_option.html
@@ -0,0 +1,30 @@
+<TITLE>Description of POLAR_OPTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword POLAR_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> action on polarisation corrections| CALC, VZERO; COPY, SET, ZERO, INVERT; SHOW, EDIT; QUIT
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform on polarisation corrections: <P>
+   Calculate corrections from calibrator visibilities. The new correction values 
+   are ADDED to existing ones: <P>
+        CALC     calculate dipole corrections <P>
+        VZERO    select the set of operations dealing with the phase-zero 
+                 difference ('PZD') between the X and Y channel groups <P>
+   Copy/set corrections. The new corrections values generally OVERWRITE the 
+   existing ones: <P>
+        COPY     create dipole corrections in target sectors by copying them 
+                  from one source sector <P>
+        SET      set dipole corrections manually <P>
+        ZERO     zero dipole corrections <P>
+<DT><STRONG>	INVERT</STRONG>  invert dipole corrections <P>
+   Inspection: <P>
+        SHOW     show dipole corrections <P>
+        EDIT     edit dipole corrections <P>
+   Other: <P>
+        QUIT     exit from POLAR <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__qdetails.html b/ncalib/ncalib__qdetails.html
new file mode 100644
index 0000000000000000000000000000000000000000..eaea0c2f0499b11099eb5c2ac62396f7c5ad72cb
--- /dev/null
+++ b/ncalib/ncalib__qdetails.html
@@ -0,0 +1,14 @@
+<TITLE>Description of QDETAILS (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword QDETAILS</H1> 
+
+<DT><EM>Prompt:</EM> More details? (YES/NO)
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want to specify details of the solution procedure yourself 
+rather than relying on NCALIB's expert defaults. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__refraction.html b/ncalib/ncalib__refraction.html
new file mode 100644
index 0000000000000000000000000000000000000000..cf639093b3c3087e0698e3c5830386daff4ad71d
--- /dev/null
+++ b/ncalib/ncalib__refraction.html
@@ -0,0 +1,16 @@
+<TITLE>Description of REFRACTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword REFRACTION</H1> 
+
+<DT><EM>Prompt:</EM> Refraction-1: quadratic's coefficients|
+<DT><EM>Default:</EM> .00031, 0., 0..
+<DT><EM>Expected input:</EM> Real number, 3 values.<P>
+Specify the coefficients A, B and C in the quadratic representation of the 
+refraction coefficient as a function of frequency F in GHz: <P>
+        EXT= (1+A) + B*F +C*F*F <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__save_residuals.html b/ncalib/ncalib__save_residuals.html
new file mode 100644
index 0000000000000000000000000000000000000000..f24db075899d51a628e28301f5a62602b9e549da
--- /dev/null
+++ b/ncalib/ncalib__save_residuals.html
@@ -0,0 +1,15 @@
+<TITLE>Description of SAVE_RESIDUALS (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword SAVE_RESIDUALS</H1> 
+
+<DT><EM>Prompt:</EM> Save the interferometer residuals as interferometer errors?
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Logical.<P>
+If YES, the interferometer residuals after Selfcal, Align or Redun will be 
+saved for later use as Multiplicative Interferometer errors.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__set_option.html b/ncalib/ncalib__set_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..9369f1059c043618a399b1154a944fed22cc5fb7
--- /dev/null
+++ b/ncalib/ncalib__set_option.html
@@ -0,0 +1,50 @@
+<TITLE>Description of SET_OPTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword SET_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> SET action| QUIT; COPY, CCOPY, ICOPY, LINE; ZERO, MANUAL, INIT, RENORM;| -EXT, REF, IREF, FAR, IFR, MIFR; SHIFT, CLK, OTHER
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform to alter correction values. <P>
+   Note: POLARISATION corrections are NOT included here. They must be handled 
+    sparately through the POLAR main option. <P>
+These option write correction values in (a) set(s) of target sectors (selected 
+by the SCN_&lt;xxx&gt; parameters). These corrections are copied/calulated from 
+corrections /data in the same file or another one (USE_SCN_&lt;xxx&gt; parameters). 
+The calculations will use all source sectors you specify to obtain a single set 
+of corrections. Unless stated otherwise below, the new values will be ADDED to 
+the existing ones in each of the target sectors. <P>
+   Transfer of corrections from a reference source: <P>
+        COPY    copy all corrections from somewhere else 
+                 (all corrections in the input set(s) are averaged) 
+        CCOPY   copy corrections from surrounding (in time) observations 
+                 in the input sets with the same frequency channel 
+                 (corrections for the two input sets are averaged). 
+        ICOPY   copy all MIFR corrections from somewhere else 
+                 (all corrections in the input set(s) are averaged) 
+        LINE    copy all corrections from corresponding continuum channel <P>
+   Initialisation: <P>
+        ZERO    zero corrections 
+        MANUAL  copy input values into the OTH telescope corrections for 
+                 selected scans 
+        INIT    make an initial estimate of telescope corrections and shift the 
+                 present values accordingly 
+        RENORM  renormalise telescope corrections <P>
+   Manual-input actions. Each option represents a correction type for which 
+   your values will be requested. <P>
+
+<DT>   - For the following actions, your values will OVERWRITE the existing ones: <P>
+        EXT     set extinction in selected scans 
+        REF     set refraction in selected scans 
+        IREF    set ionospheric refraction in selected scans 
+        FAR     set Faraday rotation in selected scans 
+        IFR     set additive interferometer corrections in selected scans 
+        MIFR    set multiplicative interferometer corrections in selected scans 
+        CLK     set clock correction in selected scans 
+        SHIFT   set (de-apply!) coordinate shift in selected sectors <P>
+        QUIT    exit SET  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__shift.html b/ncalib/ncalib__shift.html
new file mode 100644
index 0000000000000000000000000000000000000000..fcb026d4e5e9a1c82cd2205298bf0ed87be7ae41
--- /dev/null
+++ b/ncalib/ncalib__shift.html
@@ -0,0 +1,21 @@
+<TITLE>Description of SHIFT (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword SHIFT</H1> 
+
+<DT><EM>Prompt:</EM> Shift to de-apply to data (arcsec)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the l, m shift in arcsec to be applied to data whenever the DE_APPLY 
+SHIFT correction is requested. (Ignore the 'de-apply) in the prompt.) <P>
+In the case where the shift is time-dependent (e.g. for a planet) it is 
+approximated by a linear function <P>
+        Total shift =  SHIFT + DSHIFT * (HA-HAB) <P>
+In this case the SHIFT you specify here is the value at the meridian, DSHIFT is 
+a second parameter for which you will be prompted. 
+!               \whichref{}{} 
+!!              HA-HAB or just HA? 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__show_level.html b/ncalib/ncalib__show_level.html
new file mode 100644
index 0000000000000000000000000000000000000000..75af2884a6aa2264f71a4c5b88cb9064c55ab62b
--- /dev/null
+++ b/ncalib/ncalib__show_level.html
@@ -0,0 +1,20 @@
+<TITLE>Description of SHOW_LEVEL (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword SHOW_LEVEL</H1> 
+
+<DT><EM>Prompt:</EM> Levels of terminal (1st value)| and log (2nd value) output
+<DT><EM>Default:</EM> 1, 1 /ASK.
+<DT><EM>Expected input:</EM> Integer number, 2 values; min.value: 0.000000; max.value: 4.000000.<P>
+Specify the level of the type and print output you want: <P>
+   0     none 
+   1     sector numbers, errors and summary of results only (the summary in the 
+          log file includes phase constraints and solution details which are not 
+          shown on the terminal) 
+   2     detailed report (several pages!) per integration interval (parameter 
+          HA_INTEGRATION) - intended primarily for debugging purposes  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__solve.html b/ncalib/ncalib__solve.html
new file mode 100644
index 0000000000000000000000000000000000000000..be27cb52db0c3ca67bdeb0efee448fb4b163bda3
--- /dev/null
+++ b/ncalib/ncalib__solve.html
@@ -0,0 +1,14 @@
+<TITLE>Description of SOLVE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword SOLVE</H1> 
+
+<DT><EM>Prompt:</EM> Solve for gain, phase (YES/NO, 2 values)?
+<DT><EM>Default:</EM> YES, YES.
+<DT><EM>Expected input:</EM> Logical, 2 values.<P>
+Specify if you want solutions for gain and for phase. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__use_scn_node.html b/ncalib/ncalib__use_scn_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..eb8cf5b5fd1b581664e622c07ad150f1a5976b3d
--- /dev/null
+++ b/ncalib/ncalib__use_scn_node.html
@@ -0,0 +1,15 @@
+<TITLE>Description of USE_SCN_NODE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword USE_SCN_NODE</H1> 
+
+<DT><EM>Prompt:</EM> Input .SCN-file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the input .SCN file from which the corrections should be calculated or 
+copied. A wildcard value ('*') indicates the same as the output .SCN file. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__use_scn_sets.html b/ncalib/ncalib__use_scn_sets.html
new file mode 100644
index 0000000000000000000000000000000000000000..0ff2b66498863463a935b2316e58f202e7097be3
--- /dev/null
+++ b/ncalib/ncalib__use_scn_sets.html
@@ -0,0 +1,14 @@
+<TITLE>Description of USE_SCN_SETS (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword USE_SCN_SETS</H1> 
+
+<DT><EM>Prompt:</EM> Sets of input .SCN-file sectors: grp.obs.fld.chn.seq|
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+Specify the .SCN-file sectors to be used as input in the calculations.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__value derived from.html b/ncalib/ncalib__value derived from.html
new file mode 100644
index 0000000000000000000000000000000000000000..c5deeae54b7359d3e3667918a5a8a3c003552fac
--- /dev/null
+++ b/ncalib/ncalib__value derived from.html	
@@ -0,0 +1,50 @@
+<TITLE>Description of value derived from (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword value derived from</H1> 
+
+<DT><EM>Prompt:</EM> SET action| QUIT; COPY, CCOPY, ICOPY, LINE; ZERO, MANUAL, INIT, RENORM;| -EXT, REF, IREF, FAR, IFR, MIFR; SHIFT, CLK, OTHER
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform to alter correction values. <P>
+   Note: POLARISATION corrections are NOT included here. They must be handled 
+    sparately through the POLAR main option. <P>
+These option write correction values in (a) set(s) of target sectors (selected 
+by the SCN_&lt;xxx&gt; parameters). These corrections are copied/calulated from 
+corrections /data in the same file or another one (USE_SCN_&lt;xxx&gt; parameters). 
+The calculations will use all source sectors you specify to obtain a single set 
+of corrections. Unless stated otherwise below, the new values will be ADDED to 
+the existing ones in each of the target sectors. <P>
+   Transfer of corrections from a reference source: <P>
+        COPY    copy all corrections from somewhere else 
+                 (all corrections in the input set(s) are averaged) 
+        CCOPY   copy corrections from surrounding (in time) observations 
+                 in the input sets with the same frequency channel 
+                 (corrections for the two input sets are averaged). 
+        ICOPY   copy all MIFR corrections from somewhere else 
+                 (all corrections in the input set(s) are averaged) 
+        LINE    copy all corrections from corresponding continuum channel <P>
+   Initialisation: <P>
+        ZERO    zero corrections 
+        MANUAL  copy input values into the OTH telescope corrections for 
+                 selected scans 
+        INIT    make an initial estimate of telescope corrections and shift the 
+                 present values accordingly 
+        RENORM  renormalise telescope corrections <P>
+   Manual-input actions. Each option represents a correction type for which 
+   your values will be requested. <P>
+
+<DT>   - For the following actions, your values will OVERWRITE the existing ones: <P>
+        EXT     set extinction in selected scans 
+        REF     set refraction in selected scans 
+        IREF    set ionospheric refraction in selected scans 
+        FAR     set Faraday rotation in selected scans 
+        IFR     set additive interferometer corrections in selected scans 
+        MIFR    set multiplicative interferometer corrections in selected scans 
+        CLK     set clock correction in selected scans 
+        SHIFT   set (de-apply!) coordinate shift in selected sectors <P>
+        QUIT    exit SET  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__vzero_option.html b/ncalib/ncalib__vzero_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..e14bc5a92193b15c721e460f5a27487a0fe755e6
--- /dev/null
+++ b/ncalib/ncalib__vzero_option.html
@@ -0,0 +1,51 @@
+<TITLE>Description of VZERO_OPTION (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword VZERO_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> VZERO action CALC, COPY, MANUAL; SCAN, APPLY, ASK; QUIT
+<DT><EM>Expected input:</EM> Character(8).<P>
+This branch of NCALIB implements methods to define the unknown X-Y phase-zero 
+difference ('PZD') in the parallel-dipole configuration. <P>
+Correction values may be saved in an arbitrary selection of target sectors,  
+selected by the SCN_&lt;xxx&gt; parameters. The new corrections are OTH telescope 
+phases which will be ADDED to any existing ones in each of the sectors you 
+specify for output. <P>
+In determining the corrections, the program uses a collection of input sectors,  
+which may coincide with the target sectors or be selected by the USE_SCN_ 
+parameters (for the COPY option). It is assumed that the source for these is a 
+calibrator with significant Stokes U and 'negligibly' small Stokes V. If this 
+condition is not fulfilled, the result will be meaningless. <P>
+The PZD is a phase value that is ADDED to the existing OTH phase correction of 
+the X channels. For this reason, you must be cautious to <P>
+
+<DT>        - avoid more than one COPY to the same target data and 
+
+<DT>        - avoid ruining a calibrator observation by doing an APPLY on it. (If 
+           you should do this by accident, use MANUAL to restore the observation 
+           to its previous state.) <P>
+Specify action to perform: <P>
+   Actions recommended for routine use: <P>
+        CALC    calculate PZD from the selected node and sectors (SCN_ 
+                 parameters) and display it with its mean error. Use this option 
+                 to check if a calibrator observation is suitable for 
+                 determining the PZD. <P>
+        COPY    as APPLY, but use X-Y phase-difference value derived from 
+                 a calibrator observation (USE_SCN_&lt;xxx&gt; parameters). Use this 
+                 option to set the correction for your observations <P>
+        MANUAL  manually input phase-difference value <P>
+   Other actions: <P>
+        SCAN    as CALC, but per individual scan <P>
+        APPLY   as CALC, then apply the correction to the sectors selected 
+                 (SCN_&lt;xxx&gt; parameters). 
+                NOTE that once you have performed this operation, a CALC or COPY 
+                 operation on the same input data will yield PZD=0, so these 
+                 data can no longer be used to calibrate another observation. <P>
+        ASK     as APPLY, but display and ask for confirmation before modifying 
+                 the existing values <P>
+        QUIT    exit from VZERO  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__vzero_phase.html b/ncalib/ncalib__vzero_phase.html
new file mode 100644
index 0000000000000000000000000000000000000000..b9c48fd0ba5b8d79ca73437f0df0518990a026c3
--- /dev/null
+++ b/ncalib/ncalib__vzero_phase.html
@@ -0,0 +1,20 @@
+<TITLE>Description of VZERO_PHASE (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword VZERO_PHASE</H1> 
+
+<DT><EM>Prompt:</EM> X-Y phase-zero difference 'PZD' (deg)
+<DT><EM>Expected input:</EM> Real number.<P>
+Specify the 'phase-zero difference' (PZD) in degrees. <P>
+In the parallel-dipole configuration, performing a Redundancy or Selfcal fit of 
+telescope errors to the visibilities introduces an unknown phase offset for the 
+set of telescope X channels and another unknown phase offset for the Y dipoles. 
+For correctly determining Stokes U and V, the (equally unknown) difference 
+between these must be corrected for. <P>
+This is a tricky problem and you should remain suspicious of the results that 
+you get.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__weight_min.html b/ncalib/ncalib__weight_min.html
new file mode 100644
index 0000000000000000000000000000000000000000..6241c9d8c83d28996b2ef8137858287840ef5f4e
--- /dev/null
+++ b/ncalib/ncalib__weight_min.html
@@ -0,0 +1,17 @@
+<TITLE>Description of WEIGHT_MIN (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword WEIGHT_MIN</H1> 
+
+<DT><EM>Prompt:</EM> Relative minimum weight accepted
+<DT><EM>Default:</EM> 0.01.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000; max.value: 1.000000.<P>
+Specify the minimum relative weight of a data point that is still acceptable. <P>
+The weight is relative to the maximum weight in the same scan, and in most 
+cases can be seen as the minimum data amplitude accepted as fraction of the 
+maximum in the scan. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib/ncalib__zero.html b/ncalib/ncalib__zero.html
new file mode 100644
index 0000000000000000000000000000000000000000..54af71f5ddeb33279d82c66ec6b95f9181996ebe
--- /dev/null
+++ b/ncalib/ncalib__zero.html
@@ -0,0 +1,35 @@
+<TITLE>Description of ZERO (NCALIB)</TITLE>
+<H1>Program NCALIB: private keyword ZERO</H1> 
+
+<DT><EM>Prompt:</EM> Corrections (plural) to be zeroed | ALL, NONE; RED, ALG, OTH; IFR, MIFR; EXT, REF, IREF, FAR, CLK, SHIFT;| -NOGAIN, NOPHASE|
+<DT><EM>Default:</EM> NONE.
+<DT><EM>Expected input:</EM> Character(8), 12 values.<P>
+Specify any number of corrections you want to zero: <P>
+   Generic: 
+        ALL or * All corrections 
+        NONE     None of the corrections: Return to previous prompt <P>
+   Telescope gains and phases: 
+        RED      Redundancy telescope corrections 
+        ALG      Align telescope corrections 
+        OTH      'Other' telescope gain/phase corrections <P>
+   Interferometer gains and phases: 
+        IFR      Additive interferometer corrections 
+        MIFR     Multiplicative interferometer corrections <P>
+   Corrections for the instrument as a whole: 
+        EXT      Extinction correction 
+        REF      Refraction correction 
+        IREF     Ionospheric refraction correction 
+        FAR      Faraday rotation 
+        CLK      Clock correction 
+        SHIFT    Coordinate shifts (de-apply!) <P>
+You may restrict the above to phase-only or gain-only by appending AT THE END 
+of your reply either of: <P>
+        NOGAIN   Zero only phases 
+        NOPHASE  Zero only gain <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncalib/ncalib_keys.html">List of keywords</A> for NCALIB
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncalib_descr.ps b/ncalib_descr.ps
new file mode 100644
index 0000000000000000000000000000000000000000..6df8c3eea79efe0b987769a9d90ebf26ce31ed0b
--- /dev/null
+++ b/ncalib_descr.ps
@@ -0,0 +1,987 @@
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diff --git a/ncalib_descr/_8208_tex2html_wrap397.xbm b/ncalib_descr/_8208_tex2html_wrap397.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3de7c867b7a086f206b16b15540bcba45cd07500
--- /dev/null
+++ b/ncalib_descr/_8208_tex2html_wrap397.xbm
@@ -0,0 +1,9 @@
+#define noname_width 25
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x01,0x01,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x01,0x01,0x00,0x00,0x01,0x01,0xc0,0x06,0x01,0x01,0xc0,0x06,0x01,0x01,0xc0,
+ 0x06,0x01,0x01,0xc0,0x06,0x01,0x81,0xc3,0x06,0x01,0xc1,0xc7,0x06,0x01,0x41,
+ 0xce,0x06,0x01,0x01,0xcf,0x06,0x01,0xc1,0xcf,0x06,0x01,0xe1,0xcc,0x06,0x01,
+ 0xe1,0xce,0x06,0x01,0xc1,0xcf,0x06,0x01,0x01,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x01,0x01,0x00,0x00,0x01,0x01,0x00,0x00,0x01,0xff,0xff,0xff,0x01};
diff --git a/ncalib_descr/_8208_tex2html_wrap399.png b/ncalib_descr/_8208_tex2html_wrap399.png
new file mode 100644
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diff --git a/ncalib_descr/_8208_tex2html_wrap399.xbm b/ncalib_descr/_8208_tex2html_wrap399.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..40816a023cba3c8b42bbb39d4293b3b4c608f3c8
--- /dev/null
+++ b/ncalib_descr/_8208_tex2html_wrap399.xbm
@@ -0,0 +1,5 @@
+#define noname_width 10
+#define noname_height 9
+static char noname_bits[] = {
+ 0x3c,0x00,0x36,0x02,0x36,0x02,0x32,0x01,0x92,0x03,0x9e,0x01,0x18,0x03,0x9b,
+ 0x03,0x0f,0x00};
diff --git a/ncalib_descr/_8208_tex2html_wrap401.png b/ncalib_descr/_8208_tex2html_wrap401.png
new file mode 100644
index 0000000000000000000000000000000000000000..3f974f8bfc23a845467b89df13e5bfc11961ecba
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diff --git a/ncalib_descr/_8208_tex2html_wrap401.xbm b/ncalib_descr/_8208_tex2html_wrap401.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7d497ddeed5dbc4f1e87496b1dd62b8f9715321a
--- /dev/null
+++ b/ncalib_descr/_8208_tex2html_wrap401.xbm
@@ -0,0 +1,5 @@
+#define noname_width 11
+#define noname_height 9
+static char noname_bits[] = {
+ 0xfc,0x00,0xde,0x04,0xcc,0x04,0xcc,0x02,0x6c,0x07,0x3c,0x03,0x06,0x06,0x06,
+ 0x07,0x0f,0x00};
diff --git a/ncalib_descr/images.pl b/ncalib_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..2248290fad249dbad1403f388218f4d57f7f5c55
--- /dev/null
+++ b/ncalib_descr/images.pl
@@ -0,0 +1,19 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$perr_<<200>>i<<200>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap401.xbm">'; 
+$key = q/{}fbox<<369>>largesf...<<369>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap389.xbm">'; 
+$key = q/{}$gerr_<<199>>i<<199>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap399.xbm">'; 
+$key = q/{}fbox<<379>>largesfall<<379>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap397.xbm">'; 
+$key = q/{}$bigotimes${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap383.xbm">'; 
+$key = q/{}fbox<<374>>largesfzero<<374>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap395.xbm">'; 
+$key = q/{}fbox<<364>>largesfset<<364>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap387.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/ncalib_descr/labels.pl b/ncalib_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..df8d99043bc795018f1ae05b5d6ab737d3afa246
--- /dev/null
+++ b/ncalib_descr/labels.pl
@@ -0,0 +1,18 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".set.manual"} ="$URL/ncalib_descr.html"; 
+$external_labels{".overview"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.extinct"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.copy"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.faraday"} ="$URL/ncalib_descr.html"; 
+$external_labels{".contents"} ="$URL/ncalib_descr.html"; 
+$external_labels{".option.set"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.ccopy"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.renorm"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.refract"} ="$URL/ncalib_descr.html"; 
+$external_labels{".option.show"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.zero"} ="$URL/ncalib_descr.html"; 
+$external_labels{".set.line"} ="$URL/ncalib_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/ncalib_descr/ncalib_descr.html b/ncalib_descr/ncalib_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..b2a0ec293437a4d0d7ab0ed0100e76cbdac485cb
--- /dev/null
+++ b/ncalib_descr/ncalib_descr.html
@@ -0,0 +1,218 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NCALIB</b>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncalib_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncalib_descr.html#SECTION0002000000000000000> <b>Overview of NCALIB options</b></A>
+<LI> <A NAME=tex2html3 HREF=ncalib_descr.html#SECTION0003000000000000000> <b>Option SET: Set various corrections in the SCN-file</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ncalib_descr.html#SECTION0003100000000000000> <b>SET ZERO: Set selected corrections to zero</b></A>
+<LI> <A NAME=tex2html5 HREF=ncalib_descr.html#SECTION0003200000000000000> <b>SET MANUAL: Manual input of telescope corrections</b></A>
+<LI> <A NAME=tex2html6 HREF=ncalib_descr.html#SECTION0003300000000000000> <b>SET RENORM: Renormalise telescope corrections</b></A>
+<LI> <A NAME=tex2html7 HREF=ncalib_descr.html#SECTION0003400000000000000> <b>SET LINE: Copy telescope corrections from continuum channel</b></A>
+<LI> <A NAME=tex2html8 HREF=ncalib_descr.html#SECTION0003500000000000000> <b>SET COPY: Copy telescope corrections from somewhere else</b></A>
+<LI> <A NAME=tex2html9 HREF=ncalib_descr.html#SECTION0003600000000000000> <b>SET CCOPY: Like COPY, but more intelligent</b></A>
+<LI> <A NAME=tex2html10 HREF=ncalib_descr.html#SECTION0003700000000000000> <b>SET EXTINCT: Set extinction correction</b></A>
+<LI> <A NAME=tex2html11 HREF=ncalib_descr.html#SECTION0003800000000000000> <b>SET REFRACT: Set refraction correction</b></A>
+<LI> <A NAME=tex2html12 HREF=ncalib_descr.html#SECTION0003900000000000000> <b>SET FARADAY: Set Faraday rotation</b></A>
+</UL> 
+<LI> <A NAME=tex2html13 HREF=ncalib_descr.html#SECTION0004000000000000000> <b>Option SHOW: Print average corrections (on line printer)</b></A>
+</UL>
+<b>Related chapters:</b> 
+<UL><LI> <A HREF="../ncalib_redun/ncalib_redun.html">NCALIB REDUN: Redundancy, Align and Selfcal</A> 
+<LI> <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR: Polarisation corrections</A> 
+</UL>
+<P>
+<A NAME=.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Overview of NCALIB options</b></A></H1>
+<P>
+        The program NCALIB is the heart of the NEWSTAR package.  It offers a wide range of options for the determination of all kinds of instrumental corrections (calibration) and their application to the data (correction). Corrections are stored in the Set headers and Scan headers of the <A HREF="../scn_descr/scn_descr.html">SCN file</A>.  They may be applied to the uv-data whenever they are read into memory, subject to the specifications given by means the 
+<A HREF="../common_descr/common_descr.html">APPLY</A> keyword. Corrections in the SCN-file may also be manipulated, or `imported' from other sources.
+<P>
+<UL><LI> <A HREF="../ncalib_redun/ncalib_redun.html"><b>REDUNDANCY</b></A>: Calculate Redundancy, Align or 
+Selfcal corrections. <LI> 
+<A HREF="../ncalib_polar/ncalib_polar.html"><b>POLAR</b></A>: 
+  Determine/manipulate polarisation corrections:   <UL><LI> <A HREF="../ncalib_polar/ncalib_polar.html#.calc"><b>CALC</b></A>:  Calculate polarisation corrections 
+  <LI> <A HREF="../ncalib_polar/ncalib_polar.html#.show"><b>SHOW</b></A>:  Show polarisation corrections 
+  <LI> <A HREF="../ncalib_polar/ncalib_polar.html#.set"><b>SET</b></A>:    Set corrections manually 
+  <LI> <A HREF="../ncalib_polar/ncalib_polar.html#.copy"><b>COPY</b></A>:  copy polarisation corrections from one set to others 
+  <LI> <A HREF="../ncalib_polar/ncalib_polar.html#.ccopy"><b>EDIT</b></A>: Edit polarisation corrections 
+  <LI> <A HREF="../ncalib_polar/ncalib_polar.html#.zero"><b>ZERO</b></A>:  Zero polarisation corrections 
+  <LI> <A HREF="../ncalib_polar/ncalib_polar.html#.vzero"><b>VZERO</b></A>:        Calculate X-Y phase zero difference, assuming V=0 
+  </UL> <LI>   <A HREF="#.option.set"><b>SET</b></A>: Set some correction data   <UL><LI> <A HREF="#.set.zero"><b>ZERO</b></A>:          Zero selected corrections 
+  <LI> <A HREF="#.set.manual"><b>MANUAL</b></A>:      Copy corrections from manual input 
+  <LI> <A HREF="#.set.copy"><b>COPY</b></A>:          Copy corrections from somewhere else 
+  <LI> <A HREF="#.set.line"><b>LINE</b></A>:          Copy all corrections from corresponding continuum channel 
+  <LI> <A HREF="#.set.extinct"><b>EXTINCT</b></A>:    Set extinction 
+  <LI> <A HREF="#.set.refract"><b>REFRACT</b></A>:    Set refraction 
+  <LI> <A HREF="#.set.faraday"><b>FARADAY</b></A>:    Set Faraday rotation 
+  <LI> <A HREF="#.set.renorm"><b>RENORM</b></A>:      Renormalise telescope corrections 
+  </UL> <LI>   <A HREF="#.option.show"><b>SHOW</b></A>:       Show (on printer) the average 
+telescope corrections (over all HA-Scans) in specified set(s). <LI>   <b>QUIT</b>:     Quit program NCALIB 
+</UL>
+<P>
+<A NAME=.option.set><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Option SET: Set various corrections in the SCN-file</b></A></H1>
+<P>
+        The NCALIB option SET is accessed in the following manner:
+<P>
+ <BR> > <i>dwe ncalib</i>
+<P>
+		<BR><tt>     NCALIB$1is started at 17-DEC-92 15:58:01</tt>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap383.png"> <b>OPTION</b> 
+ (REDUNDANCY,POLAR,SET,SHOW,QUIT) 
+ = QUIT: 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap387.png">
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap383.png"> <b>SET_OPTION</b> 
+ (ZERO,MANUAL,COPY,LINE,EXTINCT,...) 
+ = QUIT: 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap389.png">
+<P>
+In the following, the various sub-options of the NCALIB option SET will be treated in some detail.
+<P>
+<A NAME=.set.zero><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000> <b>SET ZERO: Set selected corrections to zero</b></A></H2>
+<P>
+The uv-data stored in a SCN file are never physically modified. Corrections are stored separately in the Scan and Set header(s), and applied to the data whenever they are read into memory for processing. Thus, by setting some (or all) corrections to zero, a reduction process that has gone wrong can always be returned to a known initial state. The keyword ZERO allows the user to specify which of the various kinds of corrections are to be set to zero.
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap383.png"> <b>SET_OPTION</b> 
+ (ZERO,MANUAL,COPY,LINE,EXTINCT,...) 
+ = QUIT: 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap395.png">
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap383.png"> <b>ZERO</b> 
+ (ALL,NONE,RED,ALG,OTH,...) 
+ = NONE: 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap397.png">
+<P>
+***** Insert new script here *****
+<P>
+NB: Going trough a large SCN file (e.g. one with many line channels) will take some time.
+<P>
+<A NAME=.set.manual><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000> <b>SET MANUAL: Manual input of telescope corrections</b></A></H2>
+<P>
+The telescope gain and phase corrections may be specified manually by the user. The given values will be stored as `other corrections' (OTHC) in the Scan headers of the specified range (Sets and HA-range).
+<P>
+<i>Note of the editor: It is not yet clear to me what happens to the other telescope corrections (REDC and ALGC) in the Scan header. It seems reasonable that they are set to zero.</i>
+<P>
+***** Insert new script here *****
+<P>
+<A NAME=.set.renorm><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003300000000000000> <b>SET RENORM: Renormalise telescope corrections</b></A></H2>
+<P>
+In the Redundancy calibration process, the <em>average</em> telescope gain and phase corrections over all telescopes are arbitrarily set to zero. This is a `reasonable' assumption, unless the correction for one or more telescopes happens to be  anomalously large. In that case, the gain and/or phase corrections of all the other telescopes will be shifted by an `unreasonable' amount (since the average must be zero). Therefore, it is sometimes desirable to RENORMalise by shifting the telescope corrections by a common amount, until the average is zero for a selection of `good' telescopes.
+<P>
+***** Insert new script here *****
+<P>
+Note that the program terminates upon completion, i.e. it does not return to the level of the SET option.
+<P>
+<A NAME=.set.line><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003400000000000000> <b>SET LINE: Copy telescope corrections from continuum channel</b></A></H2>
+<P>
+Since Selfcal/Redundancy calibration requires a S/N of more than 2-5, it is often possible for the continuum channel (0), but not for the individual line channels. In those cases, the telescope gain and phase corrections that have been found for channel 0 may be transferred to the line channels. This is a `reasonable' thing to do, since the total telescope errors will vary much more than the reletive errors between channels (i.e. the bandpass shape).
+<P>
+***** Insert new script here *****
+<P>
+<A NAME=.set.copy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003500000000000000> <b>SET COPY: Copy telescope corrections from somewhere else</b></A></H2>
+<P>
+In the Standard Calibration process, the telescope gain and phase errors <IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap399.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8208_tex2html_wrap401.png"> are calculated with the help of a strong calibrator source, which has been observed directly before (or after) the actual observation. In order to use these calibrator corrections to correct the latter, they must be transferred (copied) from the Scan header(s) of the calibrator to the Scan header(s) of the observed object.
+<P>
+There are two possibilities: The calibrator observation (and thus the desired corrections) may be stored in a separate SCN-file (node), or they may be stored as another `job' of the same SCN-file as the observed object. In the following example, the observed object is stored as job nr 0, while the calibrator observation is stored in the same SCN-file, as job nr 1:
+<P>
+***** Insert new script here *****
+<P>
+NB: Note that the program exits upon completion, and does not return to SET_OPTION.
+<P>
+<A NAME=.set.ccopy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003600000000000000> <b>SET CCOPY: Like COPY, but more intelligent</b></A></H2>
+<P>
+<A NAME=.set.extinct><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003700000000000000> <b>SET EXTINCT: Set extinction correction</b></A></H2>
+<P>
+The actual atmospheric extinction factor (as a function of telescope elevetion) may differ from the default value, which is based on a standard model of the atmosphere.
+<P>
+***** Insert new script here *****
+<P>
+<A NAME=.set.refract><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003800000000000000> <b>SET REFRACT: Set refraction correction</b></A></H2>
+<P>
+***** Insert new script here *****
+<P>
+<A NAME=.set.faraday><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003900000000000000> <b>SET FARADAY: Set Faraday rotation</b></A></H2>
+<P>
+Information about the ionospheric Faraday rotation during the observation may be obtained externally, e.g. from ionosonde measurements. NFRA receives these values routinely from meteorological stations not too far from the WSRT. The information may be entered into the SCN-file as a function of HA. They are stored as corrections (FARAD) in the Scan header, and will be applied routinely to the data if specified by the keyword APPLY.
+<P>
+***** Insert new script here *****
+<P>
+<A NAME=.option.show><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Option SHOW: Print average corrections (on line printer)</b></A></H1>
+<P>
+The average telescope gain and phase corrections that are stored in the SCN file can be printed, for a specified range of sets. The numbers printed are a <em>combination</em> of the several kinds of telescope corrections stored in the SCN file (see the SCN-file description section). The desired combination may be specified with the keywords APPLY and D_APPLY.
+<P>
+The output takes the form of 14 columns of 8 numbers: 
+<BR>- X gain: as gain factor and as percentage (%) 
+<BR>- X phase: in radians and in degrees 
+<BR>- Y gain: as gain factor and as percentage (%) 
+<BR>- Y phase: in radians and in degrees
+<P>
+***** Insert new script here *****
+<P>
+The output will now be printed on the line printer. Note that the program terminates upon completion, i.e. it does not return to the level of the SHOW option.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ncalib_keys/ncalib_keys.html b/ncalib_keys/ncalib_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..91c3c9929a8241aba1c498fcfc08200353e177a5
--- /dev/null
+++ b/ncalib_keys/ncalib_keys.html
@@ -0,0 +1,224 @@
+<TITLE>Index of private keywords for NCALIB </TITLE>
+<H1>Description of keywords for program NCALIB</H1>
+
+<UL>
+<LI> <A HREF="../ncalib/ncalib__option.html">
+  OPTION</A>
+  Type of action  REDUNDANCY, POLAR, SET; SHOW; QUIT
+<LI> <A HREF="../ncalib/ncalib__polar_option.html">
+  POLAR_OPTION</A>
+  action on polarisation corrections| CALC, VZERO; COPY, SET, ZERO, INVERT; SHOW, EDIT; QUIT
+<LI> <A HREF="../ncalib/ncalib__vzero_option.html">
+  VZERO_OPTION</A>
+  VZERO action CALC, COPY, MANUAL; SCAN, APPLY, ASK; QUIT
+<LI> <A HREF="../ncalib/ncalib__set_option.html">
+  SET_OPTION</A>
+  SET action| QUIT; COPY, CCOPY, ICOPY, LINE; ZERO, MANUAL, INIT, RENORM, INVERT;| -EXT, REF, IREF, FAR, IFR, MIFR; SHIFT, CLK, OTHER
+<LI> <A HREF="../ncalib/ncalib__oth_option.html">
+  OTH_OPTION</A>
+  MULT, POLE, DX, DY, DZ, FREQ, QUIT SET action (others)|
+<LI> <A HREF="../ncalib/ncalib__use_scn_sets.html">
+  USE_SCN_SETS</A>
+  Sets of input .SCN-file sectors: grp.obs.fld.chn.seq|
+<LI> <A HREF="../ncalib/ncalib__cal_equal.html">
+  CAL_EQUAL</A>
+  Copy with equal length?
+<LI> <A HREF="../ncalib/ncalib__use_scn_node.html">
+  USE_SCN_NODE</A>
+  Input .SCN-file name
+<LI> <A HREF="../ncalib/ncalib__mweight_type.html">
+  MWEIGHT_TYPE</A>
+  Type of weight function| STEP, ISTEP; GAUSSIAN, IGAUSSIAN; TRIANGLE, ITRIANGLE
+<LI> <A HREF="../ncalib/ncalib__mweight_data.html">
+  MWEIGHT_DATA</A>
+  Centre, halfwidth (metres)
+<LI> <A HREF="../ncalib/ncalib__align_option.html">
+  ALIGN_OPTION</A>
+  Type of Selfcal desired SELFCAL, ALIGN
+<LI> <A HREF="../ncalib/ncalib__force_freedom.html">
+  FORCE_FREEDOM</A>
+    Manual constraints for gain (1st value)|-
+and phase (2nd value)? YES/NO
+<LI> <A HREF="../ncalib/ncalib__gain_freedom.html">
+  GAIN_FREEDOM</A>
+  Gain grouping
+<LI> <A HREF="../ncalib/ncalib__phase_freedom.html">
+  PHASE_FREEDOM</A>
+  Phase grouping
+<LI> <A HREF="../ncalib/ncalib__gain_norm.html">
+  GAIN_NORM</A>
+  Gain reference telescopes
+<LI> <A HREF="../ncalib/ncalib__phase_norm.html">
+  PHASE_NORM</A>
+  Phase reference telescopes
+<LI> <A HREF="../ncalib/ncalib__ha_integration.html">
+  HA_INTEGRATION</A>
+  Integration time (sec)
+<LI> <A HREF="../ncalib/ncalib__save_residuals.html">
+  SAVE_RESIDUALS</A>
+  Save the interferometer residuals as interferometer errors?
+<LI> <A HREF="../ncalib/ncalib__show_level.html">
+  SHOW_LEVEL</A>
+  Levels of terminal (1st value)| and log (2nd value) output
+<LI> <A HREF="../ncalib/ncalib__zero.html">
+  ZERO</A>
+  Corrections (plural) to be zeroed or inverted | ALL, NONE; RED, ALG, OTH; IFR, MIFR; EXT, REF, IREF, FAR, CLK, SHIFT;| -NOGAIN, NOPHASE|
+<LI> <A HREF="../ncalib/ncalib__gain_x.html">
+  GAIN_X</A>
+  Gain corrections X (factors) |
+<LI> <A HREF="../ncalib/ncalib__gain_y.html">
+  GAIN_Y</A>
+  Gain corrections Y (factors) |
+<LI> <A HREF="../ncalib/ncalib__phase_x.html">
+  PHASE_X</A>
+  Phase corrections X (deg) |
+<LI> <A HREF="../ncalib/ncalib__phase_y.html">
+  PHASE_Y</A>
+  Phase corrections Y (deg) |
+<LI> <A HREF="../ncalib/ncalib__gain_xx.html">
+  GAIN_XX</A>
+  Interferometer gain corrections XX (factors) |
+<LI> <A HREF="../ncalib/ncalib__gain_xy.html">
+  GAIN_XY</A>
+  interferometer gain corrections XY (factors) |
+<LI> <A HREF="../ncalib/ncalib__gain_yx.html">
+  GAIN_YX</A>
+  interferometer gain corrections YX (factors) |
+<LI> <A HREF="../ncalib/ncalib__gain_yy.html">
+  GAIN_YY</A>
+  interferometer gain corrections YY (factors) |
+<LI> <A HREF="../ncalib/ncalib__phase_xx.html">
+  PHASE_XX</A>
+  interferometer phase corrections XX (deg) |
+<LI> <A HREF="../ncalib/ncalib__phase_xy.html">
+  PHASE_XY</A>
+  interferometer phase corrections XY (deg) |
+<LI> <A HREF="../ncalib/ncalib__phase_yx.html">
+  PHASE_YX</A>
+  interferometer phase corrections YX (deg) |
+<LI> <A HREF="../ncalib/ncalib__phase_yy.html">
+  PHASE_YY</A>
+  interferometer phase corrections YY (deg) |
+<LI> <A HREF="../ncalib/ncalib__ifr_xx.html">
+  IFR_XX</A>
+  additive interferometer corrections cos, sin XX (W.U.) |
+<LI> <A HREF="../ncalib/ncalib__ifr_xy.html">
+  IFR_XY</A>
+  additive interferometer corrections cos, sin XY (W.U.) |
+<LI> <A HREF="../ncalib/ncalib__ifr_yx.html">
+  IFR_YX</A>
+  additive interferometer corrections cos, sin YX (W.U.) |
+<LI> <A HREF="../ncalib/ncalib__ifr_yy.html">
+  IFR_YY</A>
+  additive interferometer corrections cos, sin YY (W.U.) |
+<LI> <A HREF="../ncalib/ncalib__extinction.html">
+  EXTINCTION</A>
+  Extinction-1: quadratic's coefficients|
+<LI> <A HREF="../ncalib/ncalib__refraction.html">
+  REFRACTION</A>
+  Refraction-1: quadratic's coefficients|
+<LI> <A HREF="../ncalib/ncalib__clock_corr.html">
+  CLOCK_CORR</A>
+  Clock correction (sec)
+<LI> <A HREF="../ncalib/ncalib__basel_pole.html">
+  BASEL_POLE</A>
+  "Increment to baseline-pole declination correction (deg) |"
+<LI> <A HREF="../ncalib/ncalib__freq_corr.html">
+  FREQ_CORR</A>
+  Increment to frequency correction (MHz)
+<LI> <A HREF="../ncalib/ncalib__basel_dx.html">
+  BASEL_DX</A>
+  Increments to telescope X positions (mm) |
+<LI> <A HREF="../ncalib/ncalib__basel_dy.html">
+  BASEL_DY</A>
+  Increments to telescope Y positions (mm) |
+<LI> <A HREF="../ncalib/ncalib__basel_dz.html">
+  BASEL_DZ</A>
+  increments to telescope Z positions (mm) |
+<LI> <A HREF="../ncalib/ncalib__shift.html">
+  SHIFT</A>
+  Shift to de-apply to data (arcsec)
+<LI> <A HREF="../ncalib/ncalib__dshift.html">
+  DSHIFT</A>
+  Shift rate (dl/dt, dm/dt, arcsec/day)
+<LI> <A HREF="../ncalib/ncalib__faraday_file.html">
+  FARADAY_FILE</A>
+  Faraday-rotation data file
+<LI> <A HREF="../ncalib/ncalib__irefract_file.html">
+  IREFRACT_FILE</A>
+  Ionospheric refraction data file
+<LI> <A HREF="../ncalib/ncalib__pol_rotan.html">
+  POL_ROTAN</A>
+  Dipole positions (deg)|
+<LI> <A HREF="../ncalib/ncalib__pol_orthog.html">
+  POL_ORTHOG</A>
+  Dipole orthogonalities (deg)|
+<LI> <A HREF="../ncalib/ncalib__pol_x_ellips.html">
+  POL_X_ELLIPS</A>
+  X-dipole ellipticities (%)|
+<LI> <A HREF="../ncalib/ncalib__pol_y_ellips.html">
+  POL_Y_ELLIPS</A>
+  Y-dipole ellipticities (%)|
+<LI> <A HREF="../ncalib/ncalib__vzero_phase.html">
+  VZERO_PHASE</A>
+  X-Y phase-zero difference 'PZD' (deg)
+<LI> <A HREF="../ncalib/ncalib__qdetails.html">
+  QDETAILS</A>
+  More details? (YES/NO)
+<LI> <A HREF="../ncalib/ncalib__basel_check.html">
+  BASEL_CHECK</A>
+  Redundant-baseline difference allowed (metres)
+<LI> <A HREF="../ncalib/ncalib__weight_min.html">
+  WEIGHT_MIN</A>
+  Relative minimum weight accepted
+<LI> <A HREF="../ncalib/ncalib__force_phase.html">
+  FORCE_PHASE</A>
+  Define phase-zeroes
+<LI> <A HREF="../ncalib/ncalib__continuity.html">
+  CONTINUITY</A>
+  Continuity in solution (YES/NO)?
+<LI> <A HREF="../ncalib/ncalib__flw_factor.html">
+  FLW_FACTOR</A>
+  Weight for points flagged with WGT flag
+<LI> <A HREF="../ncalib/ncalib__solve.html">
+  SOLVE</A>
+  Solve for gain, phase (YES/NO, 2 values)?
+<LI> <A HREF="../ncalib/ncalib__complex.html">
+  COMPLEX</A>
+  Complex solution (YES/NO)?
+<LI> <A HREF="../ncalib/ncalib__complex_only.html">
+  COMPLEX_ONLY</A>
+  Complex solution only (YES/NO)?
+<LI> <A HREF="../ncalib/ncalib__checks.html">
+  CHECKS</A>
+  Iterations, gain deviation, relative mean error: 3 values|
+<LI> <A HREF="../ncalib/ncalib__calchan.html">
+  CALCHAN</A>
+  Channel to take calibration from (Channel Zero)
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../ncalib_descr/ncalib_descr.html">program NCALIB</A>
+</UL>
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+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x92,0x07,0x3c,0xd7,0x0f,0x1c,0x53,0x01,
+ 0x04,0x5a,0x05,0x00,0xde,0x07,0x00,0x0b,0x00,0x00,0x0f,0x00};
diff --git a/ncalib_polar/_13658_tex2html_wrap1345.png b/ncalib_polar/_13658_tex2html_wrap1345.png
new file mode 100644
index 0000000000000000000000000000000000000000..d9779e5222b928dfefd8301a7c061a0ca849e747
Binary files /dev/null and b/ncalib_polar/_13658_tex2html_wrap1345.png differ
diff --git a/ncalib_polar/_13658_tex2html_wrap1345.xbm b/ncalib_polar/_13658_tex2html_wrap1345.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e23b70bedacc3a983ecf4d5959ff5c275129887a
--- /dev/null
+++ b/ncalib_polar/_13658_tex2html_wrap1345.xbm
@@ -0,0 +1,5 @@
+#define noname_width 19
+#define noname_height 9
+static char noname_bits[] = {
+ 0xfc,0x00,0x00,0xde,0x00,0x03,0xcc,0x80,0x06,0xcc,0xde,0x04,0x6c,0xff,0x04,
+ 0x3c,0xc5,0x04,0x06,0xd5,0x06,0x06,0x9f,0x07,0x0f,0x00,0x00};
diff --git a/ncalib_polar/_13658_tex2html_wrap1347.png b/ncalib_polar/_13658_tex2html_wrap1347.png
new file mode 100644
index 0000000000000000000000000000000000000000..6bab6f7f70a6eed45cf1d10469677575997fdeeb
Binary files /dev/null and b/ncalib_polar/_13658_tex2html_wrap1347.png differ
diff --git a/ncalib_polar/_13658_tex2html_wrap1347.xbm b/ncalib_polar/_13658_tex2html_wrap1347.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7a671fe3f1d26944dffb3aa4b2ff998f02ac3ff0
--- /dev/null
+++ b/ncalib_polar/_13658_tex2html_wrap1347.xbm
@@ -0,0 +1,5 @@
+#define noname_width 19
+#define noname_height 10
+static char noname_bits[] = {
+ 0xfc,0x00,0x00,0xde,0x00,0x03,0xcc,0x80,0x06,0xcc,0xd2,0x04,0x6c,0xd7,0x04,
+ 0x3c,0xd3,0x04,0x06,0xda,0x06,0x06,0x9e,0x07,0x0f,0x0b,0x00,0x00,0x0f,0x00};
diff --git a/ncalib_polar/_13658_tex2html_wrap1349.png b/ncalib_polar/_13658_tex2html_wrap1349.png
new file mode 100644
index 0000000000000000000000000000000000000000..b5bfdf5e9c6d532d84fd3b6066ce6f859809241b
Binary files /dev/null and b/ncalib_polar/_13658_tex2html_wrap1349.png differ
diff --git a/ncalib_polar/_13658_tex2html_wrap1349.xbm b/ncalib_polar/_13658_tex2html_wrap1349.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..eeaeffd3a4e6a28c8ef9aa1d283f9b56989836af
--- /dev/null
+++ b/ncalib_polar/_13658_tex2html_wrap1349.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 12
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x3c,0x86,0xf9,0x7f,0xee,0x29,0x0a,
+ 0x38,0xa8,0x2a,0x00,0xf8,0x3e};
diff --git a/ncalib_polar/_13658_tex2html_wrap1351.png b/ncalib_polar/_13658_tex2html_wrap1351.png
new file mode 100644
index 0000000000000000000000000000000000000000..aa2d50b2182e7418021f0af05eea8a4ad868ade8
Binary files /dev/null and b/ncalib_polar/_13658_tex2html_wrap1351.png differ
diff --git a/ncalib_polar/_13658_tex2html_wrap1351.xbm b/ncalib_polar/_13658_tex2html_wrap1351.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..344e9d81f2e35050db9bcc61f5565be08d60f9de
--- /dev/null
+++ b/ncalib_polar/_13658_tex2html_wrap1351.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x24,0x86,0xb9,0x2e,0xee,0x99,0x26,
+ 0x38,0xd0,0x34,0x00,0xf0,0x3c,0x00,0x58,0x16,0x00,0x78,0x1e};
diff --git a/ncalib_polar/_13658_tex2html_wrap1353.png b/ncalib_polar/_13658_tex2html_wrap1353.png
new file mode 100644
index 0000000000000000000000000000000000000000..e29443a545b82a10f015ca1dcce9cbd521160eae
Binary files /dev/null and b/ncalib_polar/_13658_tex2html_wrap1353.png differ
diff --git a/ncalib_polar/_13658_tex2html_wrap1353.xbm b/ncalib_polar/_13658_tex2html_wrap1353.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d068a8cc09189b1aa9d9a699f0c5a793d32cc8bf
--- /dev/null
+++ b/ncalib_polar/_13658_tex2html_wrap1353.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x24,0x86,0xf9,0x2f,0xee,0x29,0x26,
+ 0x38,0xa8,0x34,0x00,0xf8,0x3c,0x00,0x00,0x16,0x00,0x00,0x1e};
diff --git a/ncalib_polar/_13658_tex2html_wrap1355.png b/ncalib_polar/_13658_tex2html_wrap1355.png
new file mode 100644
index 0000000000000000000000000000000000000000..125f9be4f7803518976a45cfe859e0fc0f27add9
Binary files /dev/null and b/ncalib_polar/_13658_tex2html_wrap1355.png differ
diff --git a/ncalib_polar/_13658_tex2html_wrap1355.xbm b/ncalib_polar/_13658_tex2html_wrap1355.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6fb709724851e9baaf7a06a843d291728b3b8cc8
--- /dev/null
+++ b/ncalib_polar/_13658_tex2html_wrap1355.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x3c,0x86,0xb9,0x7e,0xee,0x99,0x0a,
+ 0x38,0xd0,0x2a,0x00,0xf0,0x3e,0x00,0x58,0x00,0x00,0x78,0x00};
diff --git a/ncalib_polar/_23919_eqnarray140.png b/ncalib_polar/_23919_eqnarray140.png
new file mode 100644
index 0000000000000000000000000000000000000000..17a2a06bf2950b3ac7f2905ca3afeb010df35bbe
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray140.png differ
diff --git a/ncalib_polar/_23919_eqnarray140.xbm b/ncalib_polar/_23919_eqnarray140.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7c98cfc023b8f7dcb9a1cd0cb44206f0fc8a8f4b
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray140.xbm
@@ -0,0 +1,296 @@
+#define noname_width 450
+#define noname_height 77
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x1c,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,0xc2,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x43,0x00,0x00,0x00,0x00,0x00,0xf0,0x07,0x00,0x00,
+ 0x80,0xe0,0x1d,0x00,0x00,0x04,0x04,0x00,0x00,0x00,0x02,0x08,0x00,0x00,0x00,
+ 0x00,0x00,0x18,0x00,0x01,0x01,0x00,0x00,0x80,0x00,0xc4,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x80,0xc3,0x00,0x00,0x00,0x00,0x00,0x18,0x07,0x00,0x00,0xc0,0xc0,0x04,
+ 0x00,0x00,0x06,0x04,0x00,0x00,0x00,0x02,0x18,0x00,0x00,0x00,0x00,0x00,0x18,
+ 0x80,0x01,0x01,0x00,0x00,0x80,0x00,0x8c,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,
+ 0x00,0x00,0x00,0x00,0x00,0x0c,0x02,0x00,0x00,0x40,0x60,0x04,0x00,0x00,0x02,
+ 0x04,0x00,0x00,0x00,0x02,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x01,
+ 0x00,0x00,0x80,0x00,0x88,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x86,0x00,0x00,0x00,
+ 0x00,0x00,0x06,0x02,0x00,0x00,0x60,0x60,0x04,0x00,0x00,0x03,0x06,0x00,0x00,
+ 0x00,0x03,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x80,0x01,0x00,0x00,0xc0,
+ 0x00,0x98,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x46,0x00,0x80,0xff,0x01,0x00,0x06,
+ 0x00,0x00,0x00,0x60,0x60,0xc4,0xf7,0x7d,0x83,0x0f,0x00,0x00,0xc0,0x07,0x30,
+ 0x00,0x00,0x38,0x00,0xf0,0xdd,0xcf,0xe0,0x03,0x00,0x00,0xf0,0x01,0x98,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x66,0xc4,0x81,0xff,0x01,0x00,0x07,0x20,0x1c,0x00,
+ 0x60,0x60,0x64,0x1e,0x4d,0xc3,0x9a,0x00,0x00,0x60,0xed,0x30,0x00,0x00,0x0c,
+ 0xe1,0x30,0x99,0xc9,0xb0,0x26,0x00,0x00,0x58,0x3b,0x98,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x36,0x66,0x03,0x00,0x00,0x00,0xc3,0x33,0x36,0x00,0x60,0x30,0x64,
+ 0x18,0x3f,0x63,0xda,0x80,0xff,0x30,0xbd,0x31,0xf0,0x1f,0x9e,0xb1,0xf1,0x98,
+ 0xc9,0x98,0x36,0xe0,0x3f,0x4c,0x6f,0x98,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x3e,
+ 0x64,0x03,0x00,0x00,0x00,0x83,0x21,0x36,0x00,0x60,0x30,0x64,0x18,0x7f,0x63,
+ 0x9b,0x00,0x00,0xb0,0xbd,0x31,0x00,0x00,0x06,0xb1,0xf1,0x99,0xc9,0xd8,0x26,
+ 0x00,0x00,0x6c,0x6f,0x98,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x04,0x83,0xff,
+ 0x01,0x00,0x86,0x21,0x30,0x00,0x60,0x30,0x64,0x1c,0x45,0x63,0x8d,0x00,0x00,
+ 0xb0,0x86,0x31,0x00,0x00,0x06,0x81,0x11,0x99,0xc9,0x58,0x23,0x00,0x00,0xac,
+ 0x61,0x98,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0e,0x84,0x01,0x00,0x00,0x00,0xee,
+ 0x21,0x18,0x00,0x60,0x7c,0xc4,0xf3,0x7d,0xc3,0x87,0x00,0x00,0xe0,0xc3,0x30,
+ 0x00,0x00,0x3c,0xc1,0xf0,0xfd,0xdf,0xf0,0x21,0x00,0x00,0xf8,0x30,0x98,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0xc4,0x02,0x00,0x00,0x00,0x38,0x20,0x2c,0x00,
+ 0x40,0x00,0x04,0x00,0x00,0x02,0x81,0x00,0x00,0x80,0x60,0x11,0x00,0x00,0x00,
+ 0x61,0x01,0x00,0x80,0x40,0x20,0x00,0x00,0x20,0x58,0x88,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xfe,0x03,0x00,0x00,0x00,0x00,0xf0,0x3e,0x00,0xc0,0x00,0x04,
+ 0x00,0x00,0x86,0xc1,0x03,0x00,0xc0,0xf0,0x19,0x00,0x00,0x80,0xf7,0x01,0x00,
+ 0x80,0x61,0xf0,0x00,0x00,0x30,0x7c,0x8c,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x1c,0x00,0x00,0x86,
+ 0x00,0x00,0x00,0x40,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x21,0x00,
+ 0x00,0x00,0x10,0x00,0xcc,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x1c,0x00,0x00,0x0c,0x00,0x00,0x00,
+ 0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,
+ 0x00,0xc6,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0xdf,0xff,0x8d,0x0f,0x02,0x00,0x80,0x0f,0xc3,0x00,0x04,0xf0,0x04,0x83,0xe7,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x20,0x00,0x00,0x08,
+ 0x02,0x02,0x00,0x00,0x82,0x45,0x00,0x04,0x00,0x84,0x05,0x00,0x00,0x08,0x02,
+ 0x01,0x00,0x00,0x81,0x45,0x8c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x18,0x03,0x0f,0x00,
+ 0x00,0xc3,0x67,0x00,0x04,0x00,0xde,0x07,0x00,0x00,0x18,0x83,0x07,0x00,0x80,
+ 0xc1,0x67,0xcc,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0xe0,0x00,0x00,0x18,0x01,0x00,0x00,0x00,0x01,0x60,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x01,0x00,0x00,0x80,0x00,0x60,0xce,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x30,0x6e,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray149.png b/ncalib_polar/_23919_eqnarray149.png
new file mode 100644
index 0000000000000000000000000000000000000000..b660ee27947999a1b7c8a1b9fec365ba6db4579d
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray149.png differ
diff --git a/ncalib_polar/_23919_eqnarray149.xbm b/ncalib_polar/_23919_eqnarray149.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b96f751090df5fe988f082dea88133c006c59df8
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray149.xbm
@@ -0,0 +1,140 @@
+#define noname_width 450
+#define noname_height 36
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,
+ 0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x08,0x04,0x00,0x00,0x00,0x20,0x00,0x08,0x00,0x00,0x08,0xe1,
+ 0x01,0x00,0x00,0x80,0x07,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x0c,0x0e,0x00,0x00,0x00,0x70,0x00,0x18,0x00,0x00,0x8c,0x31,0x07,0x00,0x00,
+ 0xc0,0x1c,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x0e,0x00,
+ 0x00,0x00,0x70,0x00,0x10,0x00,0x00,0x80,0x18,0x06,0x00,0x08,0x60,0x18,0x80,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x1f,0x00,0x00,0x00,0xf8,
+ 0x00,0x30,0x00,0x00,0xc0,0x18,0x0c,0x00,0x08,0x60,0x30,0x80,0x01,0x00,0x00,
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+ 0x00,0x00,0x00,0xff,0x03,0x00,0x06,0x19,0x00,0x00,0x00,0xc8,0x00,0x30,0x00,
+ 0x00,0xce,0xec,0x0f,0x00,0x08,0xb0,0x3f,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
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+ 0xff,0x03,0x00,0x86,0x39,0x08,0x00,0x00,0xcc,0xe1,0x30,0x00,0x00,0xcf,0xec,
+ 0x8f,0x00,0x08,0xb0,0x3f,0x87,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x8f,0xb1,0x01,0x00,0x00,0x00,0x00,
+ 0x86,0x30,0x0c,0xf8,0x0f,0x84,0xb1,0x31,0xf8,0x0f,0xc6,0x0c,0xcc,0xc0,0xff,
+ 0x30,0xb0,0x8d,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x03,0xb1,0x01,0x00,0x00,0x00,0x00,0xc6,0x70,0x08,
+ 0x00,0x00,0x86,0xb3,0x31,0x00,0x00,0xc6,0x18,0x8c,0x00,0x08,0x60,0xb0,0x8d,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x61,0x01,0x00,0x00,0x00,0x00,
+ 0x04,0x00,0x08,0x80,0x00,0x00,0x60,0x11,0x00,0x00,0x80,0xc0,0x81,0x00,0x00,
+ 0x00,0x07,0x8b,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x10,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x80,0x00,0x00,0xf0,0x19,0x00,0x00,0x80,0x01,0xc0,0x03,0x00,0x00,0x80,0xcf,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x30,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,
+ 0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray154.png b/ncalib_polar/_23919_eqnarray154.png
new file mode 100644
index 0000000000000000000000000000000000000000..de23cc154282f2cc3dc35f9134bad85fe4dcb1f0
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray154.png differ
diff --git a/ncalib_polar/_23919_eqnarray154.xbm b/ncalib_polar/_23919_eqnarray154.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e90490336fbc570b2eff8d71569eec23a1bd2dcc
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray154.xbm
@@ -0,0 +1,60 @@
+#define noname_width 450
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x40,0x08,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x20,
+ 0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x40,0x00,0x00,0x00,0x00,
+ 0x00,0xfc,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x80,0x10,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x40,0x10,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x8e,0x00,0x00,0x00,0x00,0x00,0xc6,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x8c,0x01,0x00,0x00,
+ 0x00,0x00,0x80,0x31,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x8c,0x01,0x00,0x00,0x00,0x00,0xc0,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0x9b,0x01,0x00,0x00,0x00,0x00,0x83,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x21,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x80,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x1b,0x01,0x00,0x00,0x00,0x80,0x81,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x06,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x80,0x01,0x00,0x00,0xff,0x03,0x1e,0xc0,0x03,0xf0,0xee,0x3f,
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diff --git a/ncalib_polar/_23919_eqnarray159.png b/ncalib_polar/_23919_eqnarray159.png
new file mode 100644
index 0000000000000000000000000000000000000000..4f25bccaa23dfae482e77dee097b27eb7790f4c8
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray159.png differ
diff --git a/ncalib_polar/_23919_eqnarray159.xbm b/ncalib_polar/_23919_eqnarray159.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e1a68989fb48e2dab4c30a78c8c6d5bcca2883d1
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray159.xbm
@@ -0,0 +1,140 @@
+#define noname_width 450
+#define noname_height 36
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray166.png b/ncalib_polar/_23919_eqnarray166.png
new file mode 100644
index 0000000000000000000000000000000000000000..facaa345ed3c6e33b3bc8523beb75eb5571f5950
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray166.png differ
diff --git a/ncalib_polar/_23919_eqnarray166.xbm b/ncalib_polar/_23919_eqnarray166.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1a323dc01cc58e54ab0937d0cc139b5a9bc97d95
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray166.xbm
@@ -0,0 +1,140 @@
+#define noname_width 450
+#define noname_height 36
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x58,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xe0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x00,0x30,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x78,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray178.png b/ncalib_polar/_23919_eqnarray178.png
new file mode 100644
index 0000000000000000000000000000000000000000..27e519425dde98d1b2773520c197c1ce15bbb1eb
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray178.png differ
diff --git a/ncalib_polar/_23919_eqnarray178.xbm b/ncalib_polar/_23919_eqnarray178.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3b77801891a87ca9e831afc188963c684fddbc54
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray178.xbm
@@ -0,0 +1,296 @@
+#define noname_width 450
+#define noname_height 77
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x10,0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0xc0,0x03,0x00,0x00,0x00,0x00,0x00,0x40,0x86,0x00,0x00,0x00,0x00,0x43,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x80,0x07,0x00,0x00,0x80,0x07,
+ 0x30,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray200.png b/ncalib_polar/_23919_eqnarray200.png
new file mode 100644
index 0000000000000000000000000000000000000000..09fbfc16fe447dd1823ebccd322e1b5dd3f4bbb7
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray200.png differ
diff --git a/ncalib_polar/_23919_eqnarray200.xbm b/ncalib_polar/_23919_eqnarray200.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..adfc57b8ec92274588c3b9a4cde31713206fde94
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray200.xbm
@@ -0,0 +1,296 @@
+#define noname_width 450
+#define noname_height 77
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,
+ 0x01,0x00,0x00,0x00,0x00,0x80,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xfc,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x88,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x21,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0xcc,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x63,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x04,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x42,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x1c,0x68,0x15,0x00,0x00,0x00,0x00,0x00,0xa3,0x61,0x1c,
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+ 0x84,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x0e,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x06,0x00,0x60,0x06,0x1e,0x00,0x00,0x83,0x0f,0x00,0x00,0x02,0xc6,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x2c,
+ 0x00,0x00,0x00,0x00,0x00,0xe0,0xb1,0x3c,0x00,0x00,0x80,0x07,0x06,0x00,0x60,
+ 0x0f,0x0b,0x00,0x80,0x07,0x00,0x00,0x00,0x02,0xc6,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x3c,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xf0,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0xc0,0x00,0x0f,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x63,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray213.png b/ncalib_polar/_23919_eqnarray213.png
new file mode 100644
index 0000000000000000000000000000000000000000..2cf24897dc924413156a5feb51ed1b72234f788d
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray213.png differ
diff --git a/ncalib_polar/_23919_eqnarray213.xbm b/ncalib_polar/_23919_eqnarray213.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4ed36efa8e8cd512023b861e1066a646b5457682
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray213.xbm
@@ -0,0 +1,296 @@
+#define noname_width 450
+#define noname_height 77
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x08,
+ 0x00,0x00,0x00,0x00,0x80,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,
+ 0x02,0x00,0x00,0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x00,
+ 0x40,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0xc0,0x10,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x1f,0x00,0x20,0x78,0x84,0x00,0x00,0x00,
+ 0x00,0x00,0x01,0x00,0x00,0x3e,0x08,0x01,0x00,0x00,0x00,0x00,0x04,0x00,0x00,
+ 0x9e,0x43,0x08,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x20,0xcf,0x23,0x08,0x00,
+ 0x00,0x00,0x00,0x08,0x02,0x00,0x00,0x00,0x00,0xe0,0x30,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x63,0xcc,0x01,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x0c,0x61,0x0e,
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+ 0x37,0x3c,0x00,0x30,0x18,0x06,0x01,0xff,0xe1,0x01,0x00,0x0c,0xff,0xc3,0xc0,
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+ 0x00,0x00,0xff,0xc1,0xb0,0xc0,0x20,0xf0,0x3f,0x3c,0x00,0x80,0x31,0x00,0x00,
+ 0x00,0x00,0x00,0x80,0xcf,0x23,0x01,0x00,0x00,0x00,0x00,0x00,0x30,0x18,0x4f,
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+ 0x20,0x00,0x02,0x0c,0xff,0x85,0x31,0x00,0x00,0x00,0x00,0x00,0x80,0xa3,0x30,
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+ 0x36,0x30,0x7c,0x00,0x01,0xb6,0xc2,0x04,0x00,0xc0,0x21,0xc0,0xf8,0x00,0x02,
+ 0x78,0xc5,0x84,0x31,0x00,0x00,0x00,0x00,0x00,0x80,0xa0,0xa2,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x80,0x83,0x4a,0x23,0x00,0x04,0x00,0x00,0x00,0xa8,0x34,0x04,
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+ 0x00,0x01,0xb0,0x8a,0x06,0x00,0x00,0x20,0x80,0x00,0x00,0x02,0x00,0x95,0x86,
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+ 0x61,0x00,0x0c,0x00,0x00,0x00,0x00,0x16,0x06,0x00,0x00,0x38,0x18,0x00,0x00,
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+ 0x00,0x00,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0xc1,0x00,0x18,
+ 0x00,0x00,0x00,0x00,0x1e,0x03,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0xf0,
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+ 0x01,0x00,0xff,0x03,0x00,0x00,0x18,0xe6,0xfa,0x19,0x86,0x81,0x00,0x00,0x30,
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+ 0xe0,0x40,0xab,0x10,0x00,0x01,0x00,0x00,0x00,0xb4,0x0a,0x01,0x00,0x00,0x27,
+ 0x04,0x00,0x00,0x00,0xa6,0x55,0x04,0x00,0x00,0x0e,0x10,0x00,0x40,0x00,0x98,
+ 0x56,0x21,0x00,0x00,0x00,0x02,0x08,0x00,0x20,0x00,0xa0,0x55,0x08,0x01,0x00,
+ 0x10,0x06,0x01,0x00,0xc0,0xfb,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0xfb,
+ 0x30,0x00,0x03,0x00,0x00,0x00,0xbc,0x8f,0x01,0x00,0x00,0x3c,0x0c,0x00,0x00,
+ 0x00,0xe6,0x7d,0x06,0x00,0x00,0x00,0x30,0x00,0x40,0x00,0x98,0xf7,0x31,0x00,
+ 0x00,0x00,0x00,0x18,0x00,0x20,0x00,0xe0,0x7d,0x8c,0x01,0x00,0x30,0x80,0x01,
+ 0x00,0x60,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x01,0x30,0x00,0x03,
+ 0x00,0x00,0x00,0x16,0x80,0x01,0x00,0x00,0x1c,0x0c,0x00,0x00,0x00,0xb2,0x00,
+ 0x06,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0xc8,0x02,0x30,0x00,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x00,0xb0,0x00,0x8c,0x01,0x00,0x30,0x80,0x01,0x00,0xe0,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x01,0x60,0x00,0x06,0x00,0x00,0x00,
+ 0x1e,0xc0,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0xf0,0x00,0x03,0x00,0x00,
+ 0x00,0x60,0x00,0x00,0x00,0xc0,0x03,0x18,0x00,0x00,0x00,0x00,0x30,0x00,0x00,
+ 0x00,0xf0,0x00,0xc6,0x00,0x00,0x60,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray247.png b/ncalib_polar/_23919_eqnarray247.png
new file mode 100644
index 0000000000000000000000000000000000000000..36d895d11a13eb54a906e243d56533c0027f4e6a
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray247.png differ
diff --git a/ncalib_polar/_23919_eqnarray247.xbm b/ncalib_polar/_23919_eqnarray247.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3a4e8e13d1dac1e0f1eb3df3e385fbeeb5d67fb6
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray247.xbm
@@ -0,0 +1,140 @@
+#define noname_width 450
+#define noname_height 36
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x02,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x04,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x0f,0x00,0x00,0x00,
+ 0x00,0x00,0x1f,0x00,0x00,0x00,0x00,0x80,0x30,0x00,0x04,0x00,0x00,0x9e,0x03,
+ 0x00,0x00,0x0c,0x00,0x31,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x18,0x00,0x00,0x00,0x00,0x80,0x31,
+ 0x00,0x00,0x00,0x00,0xc0,0xd8,0x00,0x0c,0x00,0x00,0x0c,0x01,0x00,0x00,0x0c,
+ 0x80,0xd9,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x80,
+ 0x30,0x06,0x00,0x00,0x38,0x00,0x00,0x00,0x00,0x80,0x01,0xc2,0x18,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0xc0,0x00};
diff --git a/ncalib_polar/_23919_eqnarray483.png b/ncalib_polar/_23919_eqnarray483.png
new file mode 100644
index 0000000000000000000000000000000000000000..2e9e7adf8535d799faa97b69544df88580479a9d
Binary files /dev/null and b/ncalib_polar/_23919_eqnarray483.png differ
diff --git a/ncalib_polar/_23919_eqnarray483.xbm b/ncalib_polar/_23919_eqnarray483.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7d56872fe38cc9f27392ad4e0921cb0c9781e618
--- /dev/null
+++ b/ncalib_polar/_23919_eqnarray483.xbm
@@ -0,0 +1,140 @@
+#define noname_width 450
+#define noname_height 36
+static char noname_bits[] = {
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+ 0x00,0x08,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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diff --git a/ncalib_polar/_23919_equation278.png b/ncalib_polar/_23919_equation278.png
new file mode 100644
index 0000000000000000000000000000000000000000..0f096b01c629997b50ddd68e4ece1e0814e4e76e
Binary files /dev/null and b/ncalib_polar/_23919_equation278.png differ
diff --git a/ncalib_polar/_23919_equation278.xbm b/ncalib_polar/_23919_equation278.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..44f7e0cf5ff2e26f3769595dd6af46b667c72158
--- /dev/null
+++ b/ncalib_polar/_23919_equation278.xbm
@@ -0,0 +1,60 @@
+#define noname_width 450
+#define noname_height 15
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x66,0xc4,0x81,0xc0,0xc0,0xff,
+ 0x60,0x10,0x07,0xfe,0x07,0x86,0x39,0x08,0x00,0x00,0xcc,0xe1,0x30,0x00,0x00,
+ 0xcf,0xec,0x8f,0x00,0x08,0xb0,0x3f,0x87,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0x08,0x04,0x03,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x66,0x83,0x60,0x00,0x00,0xf0,0x98,0x0d,
+ 0x00,0x00,0x86,0x30,0x0c,0xf8,0x0f,0x84,0xb1,0x31,0xf8,0x0f,0xc6,0x0c,0xcc,
+ 0xc0,0xff,0x30,0xb0,0x8d,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x30,0x08,0x04,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x3e,0x64,0xc3,0x60,0x00,0x00,0x30,0x90,0x0d,0x00,0x00,0xc6,
+ 0x70,0x08,0x00,0x00,0x86,0xb3,0x31,0x00,0x00,0xc6,0x18,0x8c,0x00,0x08,0x60,
+ 0xb0,0x8d,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,
+ 0x08,0x04,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x1e,0x04,0x43,0x60,0xc0,0xff,0x30,0x10,0x0c,0xfe,0x07,0x46,0xe0,0x08,0x00,
+ 0x00,0x02,0x87,0x31,0x00,0x00,0xce,0x18,0x86,0x00,0x08,0x60,0x18,0x8c,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x08,0x04,0x03,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0e,0x84,0x61,
+ 0xf8,0x00,0x00,0xe0,0x11,0x06,0x00,0x00,0xe6,0xff,0x08,0x00,0x00,0xff,0xc7,
+ 0x30,0x00,0x00,0xce,0x70,0x83,0x00,0x08,0xc0,0x0d,0x86,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x3e,0x1f,0x03,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0xc4,0x62,0x00,0x00,0x00,
+ 0x00,0x10,0x0b,0x00,0x00,0x04,0x00,0x08,0x00,0x00,0x00,0x60,0x11,0x00,0x00,
+ 0x80,0xc0,0x81,0x00,0x08,0x00,0x07,0x8b,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xfe,0x23,0x00,0x00,0x00,0x00,0xf8,0x0f,
+ 0x00,0x00,0x0c,0x00,0x3c,0x00,0x00,0x00,0xf0,0x19,0x00,0x00,0x80,0x01,0xc0,
+ 0x03,0x08,0x00,0x80,0xcf,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x60,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0xc0,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1277.png b/ncalib_polar/_8345_tex2html_wrap1277.png
new file mode 100644
index 0000000000000000000000000000000000000000..cffeae67d07e6a8dac8bc31fc13b0397e9dfc7ad
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1277.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1277.xbm b/ncalib_polar/_8345_tex2html_wrap1277.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..9aff6898e39aa608f34f36ab540e105d4ab5bd9b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1277.xbm
@@ -0,0 +1,13 @@
+#define noname_width 44
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,
+ 0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x80,0x01,0x00,0x08,0x01,0x00,0x80,0x01,0x00,0x08,0x01,0x00,0x80,
+ 0x01,0x00,0x08,0x01,0x00,0x80,0x01,0x00,0x08,0xc1,0x07,0x87,0x39,0x2c,0x08,
+ 0xc1,0x8f,0x9f,0x7d,0x3c,0x08,0xc1,0xcc,0x99,0xe5,0x1c,0x08,0xc1,0xdc,0xb0,
+ 0xf1,0x0c,0x08,0xc1,0xd8,0xb0,0xfd,0x0c,0x08,0xc1,0xdc,0xb8,0xcf,0x0c,0x08,
+ 0xc1,0xcf,0x9d,0xef,0x0c,0x08,0xc1,0x8f,0x8f,0xfd,0x0c,0x08,0xc1,0x00,0x00,
+ 0x00,0x00,0x08,0xc1,0x00,0x00,0x00,0x00,0x08,0xc1,0x00,0x00,0x00,0x00,0x08,
+ 0xc1,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,
+ 0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1279.png b/ncalib_polar/_8345_tex2html_wrap1279.png
new file mode 100644
index 0000000000000000000000000000000000000000..cfa2b4ade8c887157bab8dde3197be9a826970c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1279.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1279.xbm b/ncalib_polar/_8345_tex2html_wrap1279.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..362af5f87d18c3b58cf8eac72236af0f7b04f158
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1279.xbm
@@ -0,0 +1,12 @@
+#define noname_width 43
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x30,0x00,0x00,0x00,0x04,0x01,0x30,0x00,0x00,0x00,0x04,0x01,0x30,0x00,
+ 0x00,0x00,0x04,0x01,0x30,0x00,0x00,0x00,0x04,0x81,0xf3,0xc1,0x99,0x31,0x04,
+ 0xc1,0xf7,0xe3,0x9f,0x3b,0x04,0x61,0x36,0x73,0x9e,0x1b,0x04,0xe1,0x33,0x33,
+ 0xfc,0x1b,0x04,0xc1,0x37,0x33,0xfc,0x1b,0x04,0x01,0x36,0x33,0xfe,0x1e,0x04,
+ 0x61,0x36,0x73,0x77,0x0e,0x04,0xe1,0x37,0xe3,0x63,0x0e,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x00,0x04,0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1281.png b/ncalib_polar/_8345_tex2html_wrap1281.png
new file mode 100644
index 0000000000000000000000000000000000000000..c5639bcf27ab7b17ef39e3e38a5dc4a62ed34db2
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1281.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1281.xbm b/ncalib_polar/_8345_tex2html_wrap1281.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8954ec6574552f6816fcb31b3058307e301af882
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1281.xbm
@@ -0,0 +1,6 @@
+#define noname_width 19
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x20,0x04,0xc3,0x23,0x04,0x83,0x11,0x02,0x86,0x39,0x07,0xee,0x19,0x07,
+ 0x38,0x30,0x02,0x00,0x38,0x02,0x00,0x80,0x03,0x00,0xc0,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1283.png b/ncalib_polar/_8345_tex2html_wrap1283.png
new file mode 100644
index 0000000000000000000000000000000000000000..5b83bcc13a51951e2ffbdc7d9a0c0225168d2593
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1283.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1283.xbm b/ncalib_polar/_8345_tex2html_wrap1283.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..22e96e96636ea5af9b4c44109cdbce2ea1c9ca9c
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1283.xbm
@@ -0,0 +1,12 @@
+#define noname_width 68
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x01,0x00,0x00,0x00,0xe0,0x00,0x00,
+ 0x04,0x00,0x02,0x00,0x00,0x00,0xc0,0x00,0x00,0x06,0x00,0x06,0x00,0x00,0x00,
+ 0xc0,0x00,0x00,0x02,0x00,0x04,0x00,0x00,0x00,0xc0,0x00,0x20,0x03,0x00,0x0c,
+ 0x3c,0x00,0xff,0xc1,0x7c,0x7e,0xc3,0x03,0x0c,0x36,0x81,0xff,0xc1,0x46,0x13,
+ 0x63,0x23,0x0c,0x33,0x01,0x00,0xc0,0xc6,0x13,0x63,0x23,0x0c,0x93,0x00,0x00,
+ 0xc0,0xc6,0x1e,0x23,0x13,0x0c,0xdb,0x81,0xff,0xc1,0x46,0x02,0x23,0x39,0x0c,
+ 0xde,0x00,0x00,0xe0,0x7d,0x3e,0xe3,0x19,0x0c,0x98,0x01,0x00,0x00,0x00,0x63,
+ 0x82,0x31,0x04,0xc8,0x01,0x00,0x00,0x00,0x63,0xb6,0x39,0x06,0x1e,0x00,0x00,
+ 0x00,0x00,0x3e,0xf6,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1285.png b/ncalib_polar/_8345_tex2html_wrap1285.png
new file mode 100644
index 0000000000000000000000000000000000000000..3f974f8bfc23a845467b89df13e5bfc11961ecba
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1285.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1285.xbm b/ncalib_polar/_8345_tex2html_wrap1285.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7d497ddeed5dbc4f1e87496b1dd62b8f9715321a
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1285.xbm
@@ -0,0 +1,5 @@
+#define noname_width 11
+#define noname_height 9
+static char noname_bits[] = {
+ 0xfc,0x00,0xde,0x04,0xcc,0x04,0xcc,0x02,0x6c,0x07,0x3c,0x03,0x06,0x06,0x06,
+ 0x07,0x0f,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1287.png b/ncalib_polar/_8345_tex2html_wrap1287.png
new file mode 100644
index 0000000000000000000000000000000000000000..e29443a545b82a10f015ca1dcce9cbd521160eae
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1287.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1287.xbm b/ncalib_polar/_8345_tex2html_wrap1287.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d068a8cc09189b1aa9d9a699f0c5a793d32cc8bf
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1287.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x24,0x86,0xf9,0x2f,0xee,0x29,0x26,
+ 0x38,0xa8,0x34,0x00,0xf8,0x3c,0x00,0x00,0x16,0x00,0x00,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1289.png b/ncalib_polar/_8345_tex2html_wrap1289.png
new file mode 100644
index 0000000000000000000000000000000000000000..125f9be4f7803518976a45cfe859e0fc0f27add9
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1289.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1289.xbm b/ncalib_polar/_8345_tex2html_wrap1289.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6fb709724851e9baaf7a06a843d291728b3b8cc8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1289.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x3c,0x86,0xb9,0x7e,0xee,0x99,0x0a,
+ 0x38,0xd0,0x2a,0x00,0xf0,0x3e,0x00,0x58,0x00,0x00,0x78,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1295.png b/ncalib_polar/_8345_tex2html_wrap1295.png
new file mode 100644
index 0000000000000000000000000000000000000000..cf20fcf1474f289c098cc89a5710309880350fde
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1295.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1295.xbm b/ncalib_polar/_8345_tex2html_wrap1295.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0cf15deb4ee8034a4f3e5e46cec9f4e28dbacfcb
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1295.xbm
@@ -0,0 +1,5 @@
+#define noname_width 17
+#define noname_height 10
+static char noname_bits[] = {
+ 0x1c,0x00,0x00,0x06,0x00,0x00,0x0f,0x00,0x00,0x83,0x27,0x01,0xc3,0x7f,0x01,
+ 0x5e,0x31,0x01,0x40,0xa5,0x01,0xc0,0xe7,0x01,0x00,0xb0,0x00,0x00,0xf0,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1297.png b/ncalib_polar/_8345_tex2html_wrap1297.png
new file mode 100644
index 0000000000000000000000000000000000000000..841eb262fb6fe725f84603cd616695a36d1fb7df
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1297.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1297.xbm b/ncalib_polar/_8345_tex2html_wrap1297.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5d270d923a54f88c56ccfe1435781e61ef2a5630
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1297.xbm
@@ -0,0 +1,5 @@
+#define noname_width 18
+#define noname_height 10
+static char noname_bits[] = {
+ 0x1c,0x00,0x00,0x06,0x00,0x00,0x0f,0x00,0x00,0x83,0xe4,0x01,0xc3,0xf5,0x03,
+ 0xde,0x54,0x00,0x80,0x56,0x01,0x80,0xf7,0x01,0xc0,0x02,0x00,0xc0,0x03,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1301.png b/ncalib_polar/_8345_tex2html_wrap1301.png
new file mode 100644
index 0000000000000000000000000000000000000000..f2d04ff2f59a3e0a74c9254f2b393151de333fb9
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1301.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1301.xbm b/ncalib_polar/_8345_tex2html_wrap1301.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..14d4598482de470fd94ec2173e27bafa7bc8ed18
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1301.xbm
@@ -0,0 +1,4 @@
+#define noname_width 8
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x20,0x20,0x30,0x7c,0xd6,0xd3,0xdb,0x6b,0x3e,0x08,0x0c,0x04};
diff --git a/ncalib_polar/_8345_tex2html_wrap1303.png b/ncalib_polar/_8345_tex2html_wrap1303.png
new file mode 100644
index 0000000000000000000000000000000000000000..b42c6366846f18da49f8b60e44c48a1d44a26391
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1303.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1303.xbm b/ncalib_polar/_8345_tex2html_wrap1303.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b54e2162d6c6fb621a8a3f4fb1ae3cb71e29e1ae
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1303.xbm
@@ -0,0 +1,8 @@
+#define noname_width 39
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x60,0x38,0x20,0x00,0x00,0xb0,0x29,0x20,0x00,0x00,0x90,0x6d,
+ 0x30,0x00,0x00,0x18,0x6d,0x7c,0xe0,0x3f,0x18,0x39,0xd6,0xf0,0x3f,0x18,0x01,
+ 0xd3,0x00,0x00,0x18,0x01,0xdb,0x00,0x00,0x18,0x01,0x6b,0xf0,0x3f,0x90,0x01,
+ 0x3e,0x00,0x00,0xb0,0x01,0x08,0x00,0x00,0xe0,0x00,0x0c,0x00,0x00,0x00,0x00,
+ 0x04,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1305.png b/ncalib_polar/_8345_tex2html_wrap1305.png
new file mode 100644
index 0000000000000000000000000000000000000000..3ce8ef0c303b0b8bd30b3e27e8706ddc89c0b516
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1305.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1305.xbm b/ncalib_polar/_8345_tex2html_wrap1305.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e208634859c664df40496be97f22f263d05029ed
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1305.xbm
@@ -0,0 +1,9 @@
+#define noname_width 46
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x60,0x30,0x1c,0x20,0x00,0x00,0xb0,0xd9,0x14,0x20,0x00,0x00,
+ 0x98,0xc9,0x36,0x30,0x00,0x00,0x18,0x8d,0x36,0x7c,0xe0,0x3f,0x18,0x8d,0x1c,
+ 0xd6,0xf0,0x3f,0x90,0x8d,0x00,0xd3,0x00,0x00,0xf0,0x8d,0x00,0xdb,0x00,0x00,
+ 0x80,0x8d,0x00,0x6b,0xf0,0x3f,0xb0,0xc9,0x00,0x3e,0x00,0x00,0xd0,0xd8,0x00,
+ 0x08,0x00,0x00,0x60,0x70,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,
+ 0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1307.png b/ncalib_polar/_8345_tex2html_wrap1307.png
new file mode 100644
index 0000000000000000000000000000000000000000..56ae9ca9c97db90b9a43c7334136843daab8651e
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1307.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1307.xbm b/ncalib_polar/_8345_tex2html_wrap1307.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d84c3442a3fe9208a7b158815657354225e3d47e
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1307.xbm
@@ -0,0 +1,6 @@
+#define noname_width 19
+#define noname_height 12
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x84,0x03,0x6c,0xc6,0x06,0x7c,0xc4,0x06,0x3c,0x04,0x06,0x1c,0x04,0x03,
+ 0x04,0x84,0x05,0x00,0xde,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1309.png b/ncalib_polar/_8345_tex2html_wrap1309.png
new file mode 100644
index 0000000000000000000000000000000000000000..8bd3c7c53a8673d51ec2318e9bc97edb52f61919
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1309.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1309.xbm b/ncalib_polar/_8345_tex2html_wrap1309.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4950aa65a0e5ab3a8767f0189bfd733f588a05aa
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1309.xbm
@@ -0,0 +1,5 @@
+#define noname_width 13
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x00,0x20,0x00,0x20,0x00,0x30,0x00,0x7c,0x00,0xd6,0x04,0xd3,0x06,0xdb,
+ 0x04,0x6b,0x04,0x3e,0x04,0x08,0x04,0x0c,0x1e,0x04,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1311.png b/ncalib_polar/_8345_tex2html_wrap1311.png
new file mode 100644
index 0000000000000000000000000000000000000000..15ae46d62460aac1b0743591a0f7021267fc778f
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1311.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1311.xbm b/ncalib_polar/_8345_tex2html_wrap1311.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4e5a837a43dca189dc4d1735f2ef250f0e8658e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1311.xbm
@@ -0,0 +1,5 @@
+#define noname_width 13
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x00,0x20,0x00,0x20,0x00,0x30,0x00,0x7c,0x00,0xd6,0x0e,0xd3,0x1b,0xdb,
+ 0x1b,0x6b,0x18,0x3e,0x0c,0x08,0x16,0x0c,0x1f,0x04,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1313.png b/ncalib_polar/_8345_tex2html_wrap1313.png
new file mode 100644
index 0000000000000000000000000000000000000000..21d79339b23289d5162be83053a11c1cc7fcef1d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1313.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1313.xbm b/ncalib_polar/_8345_tex2html_wrap1313.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2ab0faf1f1e17243fac1d906aa85d1fa3b86bb01
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1313.xbm
@@ -0,0 +1,5 @@
+#define noname_width 11
+#define noname_height 11
+static char noname_bits[] = {
+ 0xf0,0x07,0x18,0x07,0x0c,0x02,0x06,0x02,0x06,0x00,0x07,0x00,0xc3,0x03,0x83,
+ 0x01,0x86,0x01,0xee,0x01,0x38,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1315.png b/ncalib_polar/_8345_tex2html_wrap1315.png
new file mode 100644
index 0000000000000000000000000000000000000000..5eb0c4a1ad56c5d3e1b9e1309a8d55e2ebadcdda
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1315.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1315.xbm b/ncalib_polar/_8345_tex2html_wrap1315.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0e7a1b57009d393549ed8f62980ac7ee395bf62b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1315.xbm
@@ -0,0 +1,4 @@
+#define noname_width 5
+#define noname_height 6
+static char noname_bits[] = {
+ 0x1c,0x06,0x0f,0x03,0x03,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1317.png b/ncalib_polar/_8345_tex2html_wrap1317.png
new file mode 100644
index 0000000000000000000000000000000000000000..eaae568685ed8c4cdeed69a0c0a69ae1d4bff5fb
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1317.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1317.xbm b/ncalib_polar/_8345_tex2html_wrap1317.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..c059f315d01cbc2e5803a264c9a5d7807e8249ea
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1317.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 9
+static char noname_bits[] = {
+ 0x7e,0x6f,0x66,0x66,0x26,0x36,0x30,0x30,0x10};
diff --git a/ncalib_polar/_8345_tex2html_wrap1319.png b/ncalib_polar/_8345_tex2html_wrap1319.png
new file mode 100644
index 0000000000000000000000000000000000000000..c37526ccdbb32df334aba481f5864d0b9ab3978b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1319.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1319.xbm b/ncalib_polar/_8345_tex2html_wrap1319.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1c011fa062dcb32a8341115e85166f367ea9b42f
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1319.xbm
@@ -0,0 +1,4 @@
+#define noname_width 8
+#define noname_height 9
+static char noname_bits[] = {
+ 0xfc,0xde,0xcc,0xcc,0x6c,0x3c,0x06,0x06,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1321.png b/ncalib_polar/_8345_tex2html_wrap1321.png
new file mode 100644
index 0000000000000000000000000000000000000000..ffcc2dc2579670bf1bdee71a1860ec2db56047fc
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1321.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1321.xbm b/ncalib_polar/_8345_tex2html_wrap1321.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..bfbb5cda2951ae19a8170d56910949d62f337730
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1321.xbm
@@ -0,0 +1,11 @@
+#define noname_width 59
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x80,0x00,0x00,0x00,0x00,0x0e,0x00,0x40,0x00,
+ 0x01,0x00,0x00,0x00,0x0c,0x00,0x60,0x00,0x03,0x00,0x00,0x00,0x0c,0x00,0x20,
+ 0x00,0x02,0x00,0x00,0x00,0x0c,0x00,0x32,0x00,0x06,0x3c,0xf8,0x0f,0xcc,0xe7,
+ 0x37,0x3c,0x06,0x36,0xfc,0x0f,0x6c,0x34,0x31,0x36,0x06,0x33,0x00,0x00,0x6c,
+ 0x3c,0x31,0x36,0x06,0x13,0x00,0x00,0x6c,0xec,0x31,0x32,0x06,0x1b,0xfc,0x0f,
+ 0x6c,0x24,0x30,0x12,0x06,0x1e,0x00,0x00,0xde,0xe7,0x33,0x1e,0x06,0x18,0x00,
+ 0x00,0x00,0x30,0x26,0x18,0x02,0x08,0x00,0x00,0x00,0x30,0x66,0x1b,0x03,0x1e,
+ 0x00,0x00,0x00,0xe0,0x63,0x0f,0x03,0x00,0x00,0x00,0x00,0x00,0xc0,0x80,0x01};
diff --git a/ncalib_polar/_8345_tex2html_wrap1325.png b/ncalib_polar/_8345_tex2html_wrap1325.png
new file mode 100644
index 0000000000000000000000000000000000000000..251b03a179035e2a890affebe583851f3751c6bf
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1325.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1325.xbm b/ncalib_polar/_8345_tex2html_wrap1325.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..844b8ef7e9caca80b88b819315aecfc5fe348472
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1325.xbm
@@ -0,0 +1,5 @@
+#define noname_width 10
+#define noname_height 11
+static char noname_bits[] = {
+ 0x78,0x00,0xcc,0x01,0x86,0x01,0x06,0x03,0xfb,0x03,0xfb,0x03,0x03,0x03,0x06,
+ 0x03,0x86,0x01,0xdc,0x00,0x70,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1327.png b/ncalib_polar/_8345_tex2html_wrap1327.png
new file mode 100644
index 0000000000000000000000000000000000000000..9c9a4846ada98beb48e96c42c44ce8728add4bee
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1327.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1327.xbm b/ncalib_polar/_8345_tex2html_wrap1327.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..55a81e2fdfba04bfeaa61e3fce6107d9fd372c82
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1327.xbm
@@ -0,0 +1,5 @@
+#define noname_width 11
+#define noname_height 10
+static char noname_bits[] = {
+ 0x20,0x00,0x70,0x00,0x70,0x00,0xf8,0x00,0xc8,0x00,0xcc,0x01,0x84,0x01,0x86,
+ 0x03,0x02,0x07,0xff,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1331.png b/ncalib_polar/_8345_tex2html_wrap1331.png
new file mode 100644
index 0000000000000000000000000000000000000000..b5ccc00f88ba014b1fdcf2f44e8920340773defb
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1331.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1331.xbm b/ncalib_polar/_8345_tex2html_wrap1331.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..759163f519883c30cb7f19ed7923117e96c0ba83
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1331.xbm
@@ -0,0 +1,10 @@
+#define noname_width 53
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x00,0x30,0x18,0x0e,0x20,0x00,0x00,0x00,0xd8,0x6c,0x0a,0x20,
+ 0x00,0x00,0x00,0xcc,0x64,0x1b,0x30,0x00,0x00,0x00,0x8c,0x46,0x1b,0x7c,0x00,
+ 0xf0,0x1f,0x8c,0x46,0x0e,0xd6,0x00,0xf8,0x1f,0xc8,0x46,0x00,0xd3,0x00,0x00,
+ 0x00,0xf8,0x46,0x00,0xdb,0x1e,0x00,0x00,0xc0,0x46,0x00,0x6b,0x3f,0xf8,0x1f,
+ 0xd8,0x64,0x00,0x3e,0x05,0x00,0x00,0x68,0x6c,0x00,0x08,0x15,0x00,0x00,0x30,
+ 0x38,0x00,0x0c,0x1f,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,
+ 0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1333.png b/ncalib_polar/_8345_tex2html_wrap1333.png
new file mode 100644
index 0000000000000000000000000000000000000000..7f345d49da8d4d02b7194411cddce92e2529b1d2
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1333.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1333.xbm b/ncalib_polar/_8345_tex2html_wrap1333.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1cb9226772d56921ddfd0f42e5821fea9ac2cc8b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1333.xbm
@@ -0,0 +1,11 @@
+#define noname_width 59
+#define noname_height 14
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x00,0x10,0x1c,0x86,0x03,0x20,0x00,0x00,0x00,0x1c,0x36,0x9b,
+ 0x02,0x20,0x00,0x00,0x00,0x10,0x22,0xd9,0x06,0x30,0x00,0x00,0x00,0x10,0xb6,
+ 0xd1,0x06,0x7c,0x00,0xf0,0x1f,0x10,0x9e,0x91,0x03,0xd6,0x00,0xf8,0x1f,0x10,
+ 0xbe,0x11,0x00,0xd3,0x00,0x00,0x00,0x10,0xba,0x11,0x00,0xdb,0x12,0x00,0x00,
+ 0x10,0xa3,0x11,0x00,0x6b,0x17,0xf8,0x1f,0x10,0x23,0x19,0x00,0x3e,0x13,0x00,
+ 0x00,0x7c,0x36,0x1b,0x00,0x08,0x1a,0x00,0x00,0x00,0x1c,0x0e,0x00,0x0c,0x1e,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x0b,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x0f,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1335.png b/ncalib_polar/_8345_tex2html_wrap1335.png
new file mode 100644
index 0000000000000000000000000000000000000000..35a53172bba51efa047ed6ee57456e1de56c3be0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1335.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1335.xbm b/ncalib_polar/_8345_tex2html_wrap1335.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..92ff9f4e5676ddee9d9d2ff365afa9bee7043770
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1335.xbm
@@ -0,0 +1,6 @@
+#define noname_width 21
+#define noname_height 12
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x1e,0x0f,0x3c,0xbf,0x1f,0x1c,0x85,0x02,
+ 0x04,0x95,0x0a,0x00,0x9f,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1337.png b/ncalib_polar/_8345_tex2html_wrap1337.png
new file mode 100644
index 0000000000000000000000000000000000000000..42f40267f7fd1dac434029d68cd0402ade0dc405
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1337.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1337.xbm b/ncalib_polar/_8345_tex2html_wrap1337.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f8edd121044ec2c7d99d933fdb550b17242446fb
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1337.xbm
@@ -0,0 +1,7 @@
+#define noname_width 35
+#define noname_height 11
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x00,0x01,0x18,0x07,0x00,0xc0,0x01,0x0c,0x02,0x00,0x00,0x01,
+ 0x06,0x02,0x00,0x00,0x01,0x06,0x00,0xff,0x01,0x01,0x07,0x80,0xff,0x01,0x01,
+ 0xc3,0x03,0x00,0x00,0x01,0x83,0x01,0x00,0x00,0x01,0x86,0x81,0xff,0x01,0x01,
+ 0xee,0x01,0x00,0xc0,0x07,0x38,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1339.png b/ncalib_polar/_8345_tex2html_wrap1339.png
new file mode 100644
index 0000000000000000000000000000000000000000..c9e2a2463e038fe8dcf50e2cd872e284f8c816e4
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1339.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1339.xbm b/ncalib_polar/_8345_tex2html_wrap1339.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b70769c6faffcfd686f563bb3eabf8cf96f256d8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1339.xbm
@@ -0,0 +1,6 @@
+#define noname_width 30
+#define noname_height 11
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x36,0x00,0x00,0x00,0x32,0x00,0x00,0x00,
+ 0x23,0x1c,0xfc,0x07,0x23,0x06,0xfe,0x07,0x23,0x0f,0x00,0x00,0x23,0x03,0x00,
+ 0x00,0x23,0x03,0xfe,0x07,0x32,0x1e,0x00,0x00,0x36,0x00,0x00,0x00,0x1c};
diff --git a/ncalib_polar/_8345_tex2html_wrap1341.png b/ncalib_polar/_8345_tex2html_wrap1341.png
new file mode 100644
index 0000000000000000000000000000000000000000..5bdddca70a6b355eb774331cc0688c5b7605e594
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1341.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1341.xbm b/ncalib_polar/_8345_tex2html_wrap1341.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..91c8bc81d4b770eceb1cd6e590c91e5583d9f528
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1341.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x1e,0x09,0x3c,0xbf,0x0b,0x1c,0x85,0x09,
+ 0x04,0x15,0x0d,0x00,0x1f,0x0f,0x00,0x80,0x05,0x00,0x80,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1343.png b/ncalib_polar/_8345_tex2html_wrap1343.png
new file mode 100644
index 0000000000000000000000000000000000000000..d4bf525533831a06d74a109b5790661218f83af8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1343.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1343.xbm b/ncalib_polar/_8345_tex2html_wrap1343.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..173463801eed149e1bdea3f2c39c26160c6a48d1
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1343.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x92,0x07,0x3c,0xd7,0x0f,0x1c,0x53,0x01,
+ 0x04,0x5a,0x05,0x00,0xde,0x07,0x00,0x0b,0x00,0x00,0x0f,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1345.png b/ncalib_polar/_8345_tex2html_wrap1345.png
new file mode 100644
index 0000000000000000000000000000000000000000..d9779e5222b928dfefd8301a7c061a0ca849e747
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1345.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1345.xbm b/ncalib_polar/_8345_tex2html_wrap1345.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e23b70bedacc3a983ecf4d5959ff5c275129887a
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1345.xbm
@@ -0,0 +1,5 @@
+#define noname_width 19
+#define noname_height 9
+static char noname_bits[] = {
+ 0xfc,0x00,0x00,0xde,0x00,0x03,0xcc,0x80,0x06,0xcc,0xde,0x04,0x6c,0xff,0x04,
+ 0x3c,0xc5,0x04,0x06,0xd5,0x06,0x06,0x9f,0x07,0x0f,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1347.png b/ncalib_polar/_8345_tex2html_wrap1347.png
new file mode 100644
index 0000000000000000000000000000000000000000..6bab6f7f70a6eed45cf1d10469677575997fdeeb
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1347.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1347.xbm b/ncalib_polar/_8345_tex2html_wrap1347.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7a671fe3f1d26944dffb3aa4b2ff998f02ac3ff0
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1347.xbm
@@ -0,0 +1,5 @@
+#define noname_width 19
+#define noname_height 10
+static char noname_bits[] = {
+ 0xfc,0x00,0x00,0xde,0x00,0x03,0xcc,0x80,0x06,0xcc,0xd2,0x04,0x6c,0xd7,0x04,
+ 0x3c,0xd3,0x04,0x06,0xda,0x06,0x06,0x9e,0x07,0x0f,0x0b,0x00,0x00,0x0f,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1349.png b/ncalib_polar/_8345_tex2html_wrap1349.png
new file mode 100644
index 0000000000000000000000000000000000000000..b5bfdf5e9c6d532d84fd3b6066ce6f859809241b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1349.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1349.xbm b/ncalib_polar/_8345_tex2html_wrap1349.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..eeaeffd3a4e6a28c8ef9aa1d283f9b56989836af
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1349.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 12
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x3c,0x86,0xf9,0x7f,0xee,0x29,0x0a,
+ 0x38,0xa8,0x2a,0x00,0xf8,0x3e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1351.png b/ncalib_polar/_8345_tex2html_wrap1351.png
new file mode 100644
index 0000000000000000000000000000000000000000..aa2d50b2182e7418021f0af05eea8a4ad868ade8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1351.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1351.xbm b/ncalib_polar/_8345_tex2html_wrap1351.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..344e9d81f2e35050db9bcc61f5565be08d60f9de
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1351.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x24,0x86,0xb9,0x2e,0xee,0x99,0x26,
+ 0x38,0xd0,0x34,0x00,0xf0,0x3c,0x00,0x58,0x16,0x00,0x78,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1353.png b/ncalib_polar/_8345_tex2html_wrap1353.png
new file mode 100644
index 0000000000000000000000000000000000000000..e29443a545b82a10f015ca1dcce9cbd521160eae
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1353.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1353.xbm b/ncalib_polar/_8345_tex2html_wrap1353.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d068a8cc09189b1aa9d9a699f0c5a793d32cc8bf
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1353.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x24,0x86,0xf9,0x2f,0xee,0x29,0x26,
+ 0x38,0xa8,0x34,0x00,0xf8,0x3c,0x00,0x00,0x16,0x00,0x00,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1355.png b/ncalib_polar/_8345_tex2html_wrap1355.png
new file mode 100644
index 0000000000000000000000000000000000000000..125f9be4f7803518976a45cfe859e0fc0f27add9
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1355.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1355.xbm b/ncalib_polar/_8345_tex2html_wrap1355.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6fb709724851e9baaf7a06a843d291728b3b8cc8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1355.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x3c,0x86,0xb9,0x7e,0xee,0x99,0x0a,
+ 0x38,0xd0,0x2a,0x00,0xf0,0x3e,0x00,0x58,0x00,0x00,0x78,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1359.png b/ncalib_polar/_8345_tex2html_wrap1359.png
new file mode 100644
index 0000000000000000000000000000000000000000..5f7150aea86ab73f34575e5b9863df96211c709e
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1359.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1359.xbm b/ncalib_polar/_8345_tex2html_wrap1359.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8829f33405cb49c2c42dd33f42c31c641fcb31d4
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1359.xbm
@@ -0,0 +1,19 @@
+#define noname_width 129
+#define noname_height 14
+static char noname_bits[] = {
+ 0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x1f,0xff,
+ 0x3f,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x33,0x73,0xe6,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x63,0x39,0xc6,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x63,0x19,0x86,0x01,0xae,0xc1,0x7f,0xe0,0x07,0x00,0x00,
+ 0x00,0x7e,0x00,0x00,0xff,0x01,0x33,0x1c,0x86,0x01,0xaf,0xe1,0x7f,0xf0,0x06,
+ 0x18,0x00,0x00,0x6f,0x80,0x81,0xff,0x01,0x1f,0x0c,0x86,0x01,0x96,0x01,0x00,
+ 0x60,0x06,0x34,0xf8,0x0f,0x66,0x40,0x03,0x00,0x00,0x03,0x4e,0x86,0x01,0x96,
+ 0x00,0x00,0x60,0xf6,0x26,0x00,0x00,0x66,0x69,0x02,0x00,0x00,0x03,0x67,0x86,
+ 0x01,0xd6,0xe0,0x7f,0x60,0xfb,0x27,0x00,0x00,0xb6,0x6b,0x82,0xff,0x01,0x03,
+ 0x23,0xc6,0x00,0x7c,0x00,0x00,0xe0,0x29,0x26,0x00,0x00,0x9e,0x69,0x02,0x00,
+ 0xc0,0x87,0xbf,0x7f,0x00,0x08,0x00,0x00,0x30,0xa8,0x36,0x00,0x00,0x03,0x6d,
+ 0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x30,0xf8,0x3c,0x00,0x00,
+ 0x03,0xcf,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x78,0x00,0x00,
+ 0x00,0x80,0x87,0x05,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1361.png b/ncalib_polar/_8345_tex2html_wrap1361.png
new file mode 100644
index 0000000000000000000000000000000000000000..e29443a545b82a10f015ca1dcce9cbd521160eae
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1361.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1361.xbm b/ncalib_polar/_8345_tex2html_wrap1361.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d068a8cc09189b1aa9d9a699f0c5a793d32cc8bf
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1361.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x24,0x86,0xf9,0x2f,0xee,0x29,0x26,
+ 0x38,0xa8,0x34,0x00,0xf8,0x3c,0x00,0x00,0x16,0x00,0x00,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1363.png b/ncalib_polar/_8345_tex2html_wrap1363.png
new file mode 100644
index 0000000000000000000000000000000000000000..59cf8f91539e8e45aa78fcd411f091a6729370ec
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1363.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1363.xbm b/ncalib_polar/_8345_tex2html_wrap1363.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ba83f3378b4c944632361e2cf035ccde76199aae
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1363.xbm
@@ -0,0 +1,4 @@
+#define noname_width 4
+#define noname_height 10
+static char noname_bits[] = {
+ 0x08,0x0c,0x00,0x00,0x0e,0x0f,0x06,0x06,0x0e,0x0e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1365.png b/ncalib_polar/_8345_tex2html_wrap1365.png
new file mode 100644
index 0000000000000000000000000000000000000000..b979821c5ea4a3de48fc68d90fc7c0d9c60815cb
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1365.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1365.xbm b/ncalib_polar/_8345_tex2html_wrap1365.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6369b31bedee08040adecda85259ef0c6bbe2208
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1365.xbm
@@ -0,0 +1,4 @@
+#define noname_width 6
+#define noname_height 13
+static char noname_bits[] = {
+ 0x30,0x30,0x00,0x00,0x1c,0x1e,0x18,0x18,0x08,0x0c,0x0c,0x0f,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1367.png b/ncalib_polar/_8345_tex2html_wrap1367.png
new file mode 100644
index 0000000000000000000000000000000000000000..84ceb7c104eef9f3d2a620483b0e611023b28cb0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1367.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1367.xbm b/ncalib_polar/_8345_tex2html_wrap1367.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3566e6376ccc9c31769576c0830ee27a1699dae0
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1367.xbm
@@ -0,0 +1,5 @@
+#define noname_width 20
+#define noname_height 10
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x20,0x20,0x0c,0x20,0x60,0x06,0x20,0xc0,0x03,0xff,0x83,0x01,
+ 0x20,0xc0,0x03,0x20,0x60,0x06,0x20,0x20,0x0c,0x20,0x00,0x00,0x20,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1369.png b/ncalib_polar/_8345_tex2html_wrap1369.png
new file mode 100644
index 0000000000000000000000000000000000000000..0b9c0ac1dfb90d230d198444907a7e08a619f8ce
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1369.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1369.xbm b/ncalib_polar/_8345_tex2html_wrap1369.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ea657c4f23fcbd844dc719014a2a7f8ba8fff6ff
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1369.xbm
@@ -0,0 +1,6 @@
+#define noname_width 19
+#define noname_height 11
+static char noname_bits[] = {
+ 0x10,0x99,0x03,0x18,0x8f,0x02,0x18,0xc1,0x06,0x1c,0xc1,0x06,0x16,0x8f,0x03,
+ 0x12,0x19,0x00,0x13,0x18,0x00,0xff,0x19,0x00,0x90,0x19,0x00,0x7c,0x1f,0x00,
+ 0x00,0x06,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1371.png b/ncalib_polar/_8345_tex2html_wrap1371.png
new file mode 100644
index 0000000000000000000000000000000000000000..7824e292260eea7d3b760c36eef8c1ed2a69b8f3
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1371.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1371.xbm b/ncalib_polar/_8345_tex2html_wrap1371.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a31d7ecb8f2d05aebec6a4e03500fc208fd9b0e0
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1371.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 7
+static char noname_bits[] = {
+ 0x61,0x33,0x1e,0x0c,0x1e,0x33,0x61};
diff --git a/ncalib_polar/_8345_tex2html_wrap1373.png b/ncalib_polar/_8345_tex2html_wrap1373.png
new file mode 100644
index 0000000000000000000000000000000000000000..ceb386be27ce86167cdd830f0fc3280b99997fac
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1373.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1373.xbm b/ncalib_polar/_8345_tex2html_wrap1373.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4b2817c7f61c942037b0b0f42af06c1330f2b6eb
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1373.xbm
@@ -0,0 +1,10 @@
+#define noname_width 53
+#define noname_height 13
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x00,0x40,0x64,0x0e,0x20,0x00,0x00,0x00,0x60,0x3c,0x0a,0x20,
+ 0x00,0x00,0x00,0x60,0x04,0x1b,0x30,0x00,0x00,0x00,0x70,0x04,0x1b,0x7c,0x00,
+ 0xf0,0x1f,0x58,0x3c,0x0e,0xd6,0x00,0xf8,0x1f,0x48,0x64,0x00,0xd3,0x00,0x00,
+ 0x00,0x4c,0x60,0x00,0xdb,0x1e,0x00,0x00,0xfc,0x67,0x00,0x6b,0x3f,0xf8,0x1f,
+ 0x40,0x66,0x00,0x3e,0x05,0x00,0x00,0xf0,0x7d,0x00,0x08,0x15,0x00,0x00,0x00,
+ 0x18,0x00,0x0c,0x1f,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,
+ 0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1375.png b/ncalib_polar/_8345_tex2html_wrap1375.png
new file mode 100644
index 0000000000000000000000000000000000000000..0cff45ce3c38f2ea74d692c02841dcdbfd1b8183
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1375.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1375.xbm b/ncalib_polar/_8345_tex2html_wrap1375.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..162f720efbba12395661549069df97ced27e79fa
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1375.xbm
@@ -0,0 +1,11 @@
+#define noname_width 59
+#define noname_height 14
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x00,0x10,0x1c,0x99,0x03,0x20,0x00,0x00,0x00,0x1c,0x36,0x8f,
+ 0x02,0x20,0x00,0x00,0x00,0x10,0x36,0xc1,0x06,0x30,0x00,0x00,0x00,0x10,0x36,
+ 0xc1,0x06,0x7c,0x00,0xf0,0x1f,0x10,0x18,0x8f,0x03,0xd6,0x00,0xf8,0x1f,0x10,
+ 0x3c,0x19,0x00,0xd3,0x00,0x00,0x00,0x10,0x30,0x18,0x00,0xdb,0x12,0x00,0x00,
+ 0x10,0xb7,0x19,0x00,0x6b,0x17,0xf8,0x1f,0x10,0xb7,0x19,0x00,0x3e,0x13,0x00,
+ 0x00,0x7c,0x36,0x1f,0x00,0x08,0x1a,0x00,0x00,0x00,0x0c,0x06,0x00,0x0c,0x1e,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x0b,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x0f,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1383.png b/ncalib_polar/_8345_tex2html_wrap1383.png
new file mode 100644
index 0000000000000000000000000000000000000000..2ae9a9dee8f3e50c8519750cf3da0072781b80d1
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1383.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1383.xbm b/ncalib_polar/_8345_tex2html_wrap1383.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7abbaedd4e377d672769178feac96e341446ba54
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1383.xbm
@@ -0,0 +1,7 @@
+#define noname_width 35
+#define noname_height 11
+static char noname_bits[] = {
+ 0xcf,0x03,0x00,0x80,0x01,0x82,0x01,0x00,0xc0,0x06,0xc2,0x00,0x00,0x40,0x06,
+ 0x46,0x00,0x00,0x60,0x04,0x66,0x80,0xff,0x60,0x04,0x26,0xc0,0xff,0x60,0x04,
+ 0x16,0x00,0x00,0x60,0x04,0x1e,0x00,0x00,0x60,0x04,0x0e,0xc0,0xff,0x40,0x06,
+ 0x04,0x00,0x00,0xc0,0x06,0x04,0x00,0x00,0x80,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1387.png b/ncalib_polar/_8345_tex2html_wrap1387.png
new file mode 100644
index 0000000000000000000000000000000000000000..273cf4f8f062a2787fbf4b7d3fba250dc4404acb
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1387.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1387.xbm b/ncalib_polar/_8345_tex2html_wrap1387.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b7d7180e479dc6553c07ddf123ffbacf1ac02ae9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1387.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 10
+static char noname_bits[] = {
+ 0x78,0x30,0x18,0x18,0x18,0x18,0x0c,0x0c,0x0c,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1389.png b/ncalib_polar/_8345_tex2html_wrap1389.png
new file mode 100644
index 0000000000000000000000000000000000000000..03aed7004396bcd4d4031e79e8f88a20b9f9be6b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1389.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1389.xbm b/ncalib_polar/_8345_tex2html_wrap1389.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..79b47dcc5782585edf493cc4f8d538e2b0ee9d06
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1389.xbm
@@ -0,0 +1,5 @@
+#define noname_width 10
+#define noname_height 11
+static char noname_bits[] = {
+ 0xcf,0x03,0x82,0x01,0xc2,0x00,0x46,0x00,0x66,0x00,0x26,0x00,0x16,0x00,0x1e,
+ 0x00,0x0e,0x00,0x04,0x00,0x04,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1391.png b/ncalib_polar/_8345_tex2html_wrap1391.png
new file mode 100644
index 0000000000000000000000000000000000000000..601a46c332eb440049a7cdae91f9a3f626b041f6
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1391.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1391.xbm b/ncalib_polar/_8345_tex2html_wrap1391.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8c82d87e097d54669199544b0b327b40d049c0be
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1391.xbm
@@ -0,0 +1,17 @@
+#define noname_width 95
+#define noname_height 17
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0xfc,0xff,0xff,0xff,0xff,0xff,0x7f,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,
+ 0x80,0x03,0x00,0x00,0x00,0x0e,0xf8,0x01,0x00,0x00,0x00,0x82,0xcf,0x06,0x00,
+ 0xc0,0x73,0x1b,0x30,0x03,0x00,0x00,0x00,0xc3,0xd8,0x06,0x00,0x80,0x21,0x1b,
+ 0x18,0x03,0x00,0x00,0x00,0x61,0x18,0x06,0x10,0x80,0x31,0x18,0x18,0x03,0x00,
+ 0x00,0x80,0x31,0x18,0x03,0x10,0x80,0x10,0x0c,0x98,0x03,0xff,0x01,0x80,0x30,
+ 0x98,0x05,0x10,0xc0,0x10,0x16,0xf8,0x81,0xff,0x81,0xc0,0x38,0xd8,0x07,0x10,
+ 0xc0,0x10,0x1f,0x0c,0x00,0x00,0xc0,0x41,0x18,0x18,0x80,0xff,0xc1,0x18,0x00,
+ 0x0c,0x00,0x00,0x80,0x61,0x18,0x0c,0x00,0x10,0x40,0x08,0x00,0x0c,0x80,0xff,
+ 0x01,0x23,0xf0,0x0f,0x00,0x10,0x40,0x0c,0x00,0x1f,0x00,0x00,0x00,0x33,0x70,
+ 0x0f,0x00,0x10,0xc0,0x06,0x00,0x00,0x00,0x00,0x00,0x16,0xc0,0x09,0x00,0x10,
+ 0x80,0x03,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x0f,0x00,0x10,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x0c,0x00,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1393.png b/ncalib_polar/_8345_tex2html_wrap1393.png
new file mode 100644
index 0000000000000000000000000000000000000000..413a9d920a137d1a7c871e2b160a22aca8783d33
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1393.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1393.xbm b/ncalib_polar/_8345_tex2html_wrap1393.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0a04011b945fc4ae692cc585be1488138b8dafe3
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1393.xbm
@@ -0,0 +1,4 @@
+#define noname_width 8
+#define noname_height 9
+static char noname_bits[] = {
+ 0x8e,0x4c,0x38,0x38,0x18,0x1c,0x36,0xb2,0x61};
diff --git a/ncalib_polar/_8345_tex2html_wrap1395.png b/ncalib_polar/_8345_tex2html_wrap1395.png
new file mode 100644
index 0000000000000000000000000000000000000000..59ff1d49abbc9e25c371d9d6791b3bb868e45599
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1395.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1395.xbm b/ncalib_polar/_8345_tex2html_wrap1395.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4d22c400c9c2a943e179cfb92bce9df38641cf7b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1395.xbm
@@ -0,0 +1,10 @@
+#define noname_width 49
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0xe0,0x00,0x00,0x00,0x00,0x00,0x00,0xb0,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0xb0,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x00,0xf0,0xc3,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x01,0x8e,0xe0,0x39,
+ 0x30,0x02,0xf0,0x01,0x4c,0x20,0x0f,0x30,0x03,0x00,0x00,0x38,0x10,0x06,0x30,
+ 0x03,0x00,0x00,0x38,0x10,0x0e,0xb0,0x01,0x00,0x00,0x18,0x20,0x0f,0xd0,0x00,
+ 0x00,0x00,0x1c,0xe0,0x39,0x78,0x00,0x00,0x00,0x36,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xb2,0x00,0x00,0x00,0x00,0x00,0x00,0x61,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1403.png b/ncalib_polar/_8345_tex2html_wrap1403.png
new file mode 100644
index 0000000000000000000000000000000000000000..cfa2b4ade8c887157bab8dde3197be9a826970c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1403.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1403.xbm b/ncalib_polar/_8345_tex2html_wrap1403.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..362af5f87d18c3b58cf8eac72236af0f7b04f158
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1403.xbm
@@ -0,0 +1,12 @@
+#define noname_width 43
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x30,0x00,0x00,0x00,0x04,0x01,0x30,0x00,0x00,0x00,0x04,0x01,0x30,0x00,
+ 0x00,0x00,0x04,0x01,0x30,0x00,0x00,0x00,0x04,0x81,0xf3,0xc1,0x99,0x31,0x04,
+ 0xc1,0xf7,0xe3,0x9f,0x3b,0x04,0x61,0x36,0x73,0x9e,0x1b,0x04,0xe1,0x33,0x33,
+ 0xfc,0x1b,0x04,0xc1,0x37,0x33,0xfc,0x1b,0x04,0x01,0x36,0x33,0xfe,0x1e,0x04,
+ 0x61,0x36,0x73,0x77,0x0e,0x04,0xe1,0x37,0xe3,0x63,0x0e,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x00,0x04,0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1405.png b/ncalib_polar/_8345_tex2html_wrap1405.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1405.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1405.xbm b/ncalib_polar/_8345_tex2html_wrap1405.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1405.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1407.png b/ncalib_polar/_8345_tex2html_wrap1407.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1407.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1407.xbm b/ncalib_polar/_8345_tex2html_wrap1407.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1407.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1409.png b/ncalib_polar/_8345_tex2html_wrap1409.png
new file mode 100644
index 0000000000000000000000000000000000000000..2985f58845d85ed7ee6ea437bb8f0fdc66f163ef
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1409.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1409.xbm b/ncalib_polar/_8345_tex2html_wrap1409.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..44345abc6ed0ad5c9c58458097309359ef7f2802
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1409.xbm
@@ -0,0 +1,5 @@
+#define noname_width 15
+#define noname_height 12
+static char noname_bits[] = {
+ 0x20,0x00,0x70,0x00,0x70,0x00,0xf8,0x00,0xc8,0x00,0xcc,0x41,0x84,0x41,0x86,
+ 0x23,0x02,0x77,0xff,0x37,0x00,0x60,0x00,0x70};
diff --git a/ncalib_polar/_8345_tex2html_wrap1413.png b/ncalib_polar/_8345_tex2html_wrap1413.png
new file mode 100644
index 0000000000000000000000000000000000000000..72e6f75b38d485be8ace122468ccd0eb1211186e
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1413.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1413.xbm b/ncalib_polar/_8345_tex2html_wrap1413.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3220a2664507c654f35c0a273f2e4959e3b3024e
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1413.xbm
@@ -0,0 +1,7 @@
+#define noname_width 34
+#define noname_height 11
+static char noname_bits[] = {
+ 0xcf,0x01,0x00,0xc0,0x00,0x86,0x00,0x00,0x60,0x03,0xc6,0x00,0x00,0x20,0x03,
+ 0x42,0x00,0x00,0x30,0x02,0x43,0x80,0xff,0x30,0x02,0x43,0xc0,0xff,0x30,0x02,
+ 0x63,0x00,0x00,0x30,0x02,0x21,0x00,0x00,0x30,0x02,0x31,0xc0,0xff,0x20,0x03,
+ 0x1b,0x00,0x00,0x60,0x03,0x0e,0x00,0x00,0xc0,0x01};
diff --git a/ncalib_polar/_8345_tex2html_wrap1417.png b/ncalib_polar/_8345_tex2html_wrap1417.png
new file mode 100644
index 0000000000000000000000000000000000000000..d3b8b722062139256f070bfc508d0425054a7226
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1417.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1417.xbm b/ncalib_polar/_8345_tex2html_wrap1417.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..9af6afd02047b20290aea35d75b46aa149d01358
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1417.xbm
@@ -0,0 +1,15 @@
+#define noname_width 90
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x00,0x00,0xc0,0x1f,0x00,0x00,0x00,0x80,0x00,0x18,0x07,0x00,
+ 0x00,0x00,0x60,0x1c,0x00,0x00,0x00,0xe0,0x00,0x0c,0x02,0x00,0x00,0x00,0x30,
+ 0x08,0x00,0x00,0x00,0x80,0x00,0x06,0x02,0x00,0x00,0x00,0x18,0x08,0x00,0x00,
+ 0x00,0x80,0x00,0x06,0x00,0x00,0xe0,0x3f,0x18,0x00,0x00,0x80,0xff,0x80,0x00,
+ 0x07,0x00,0x00,0xf0,0x3f,0x1c,0x00,0x00,0xc0,0xff,0x80,0x00,0xc3,0x03,0x00,
+ 0x00,0x00,0x0c,0x0f,0x00,0x00,0x00,0x80,0x00,0x83,0xf1,0x24,0x00,0x00,0x0c,
+ 0x46,0xf2,0x00,0x00,0x80,0x00,0x86,0xf9,0x2f,0xf0,0x3f,0x18,0xe6,0xfa,0xc1,
+ 0xff,0x80,0x00,0xee,0x29,0x26,0x00,0x00,0xb8,0x67,0x2a,0x00,0x00,0xe0,0x03,
+ 0x38,0xa8,0x34,0x00,0x00,0xe0,0x40,0xab,0x00,0x00,0x00,0x00,0x00,0xf8,0x3c,
+ 0x00,0x00,0x00,0xc0,0xfb,0x00,0x00,0x00,0x00,0x00,0x00,0x16,0x00,0x00,0x00,
+ 0x60,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0xe0,0x01,0x00,
+ 0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1419.png b/ncalib_polar/_8345_tex2html_wrap1419.png
new file mode 100644
index 0000000000000000000000000000000000000000..5a5ec0454e9efb79b1f0e3f4763d2b2ce69b772d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1419.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1419.xbm b/ncalib_polar/_8345_tex2html_wrap1419.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..44604b5e8b7086d3d2ed0514f744bfd53b9e861b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1419.xbm
@@ -0,0 +1,17 @@
+#define noname_width 107
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x08,0x00,0x78,
+ 0x00,0x00,0x20,0x43,0x00,0x00,0x00,0x60,0x08,0x00,0x02,0x88,0x01,0x30,0x00,
+ 0x00,0xb0,0xc3,0x00,0x00,0x00,0x70,0x18,0x00,0x06,0xcc,0x06,0x18,0x00,0x00,
+ 0x10,0xc6,0x00,0x00,0x08,0xc0,0x18,0x00,0x04,0xec,0x06,0x18,0x00,0x00,0x18,
+ 0x86,0x00,0x00,0x08,0xc0,0x10,0x00,0x0c,0xe4,0x04,0x18,0xf0,0x1f,0x18,0x46,
+ 0x00,0x00,0x08,0xc0,0x08,0x00,0x0c,0x06,0x06,0x18,0xf8,0x1f,0x18,0x66,0x82,
+ 0x00,0x08,0xc0,0xec,0x38,0x0c,0x02,0x06,0x0c,0x00,0x00,0x18,0x36,0xc3,0xc0,
+ 0xff,0xc0,0xb6,0x6d,0x0c,0x02,0x03,0x0c,0x00,0x00,0x18,0x3e,0x82,0x00,0x08,
+ 0xc0,0xb7,0x6d,0x0c,0x83,0x05,0x0c,0xf8,0x1f,0x18,0x1e,0x82,0x00,0x08,0xc0,
+ 0x83,0x61,0x0c,0xc1,0x04,0x1f,0x00,0x00,0x18,0x0e,0x82,0x00,0x08,0xc0,0xc1,
+ 0x30,0x8c,0xe1,0x07,0x00,0x00,0x00,0x10,0x02,0x82,0x00,0x08,0x40,0x60,0x59,
+ 0x84,0x01,0x00,0x00,0x00,0x00,0x30,0x00,0xcf,0x03,0x08,0x00,0xf0,0x7d,0x86,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc6,0x00,
+ 0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc3,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1421.png b/ncalib_polar/_8345_tex2html_wrap1421.png
new file mode 100644
index 0000000000000000000000000000000000000000..5bdddca70a6b355eb774331cc0688c5b7605e594
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1421.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1421.xbm b/ncalib_polar/_8345_tex2html_wrap1421.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..91c8bc81d4b770eceb1cd6e590c91e5583d9f528
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1421.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x1e,0x09,0x3c,0xbf,0x0b,0x1c,0x85,0x09,
+ 0x04,0x15,0x0d,0x00,0x1f,0x0f,0x00,0x80,0x05,0x00,0x80,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1423.png b/ncalib_polar/_8345_tex2html_wrap1423.png
new file mode 100644
index 0000000000000000000000000000000000000000..d4bf525533831a06d74a109b5790661218f83af8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1423.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1423.xbm b/ncalib_polar/_8345_tex2html_wrap1423.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..173463801eed149e1bdea3f2c39c26160c6a48d1
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1423.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x92,0x07,0x3c,0xd7,0x0f,0x1c,0x53,0x01,
+ 0x04,0x5a,0x05,0x00,0xde,0x07,0x00,0x0b,0x00,0x00,0x0f,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1429.png b/ncalib_polar/_8345_tex2html_wrap1429.png
new file mode 100644
index 0000000000000000000000000000000000000000..5bdddca70a6b355eb774331cc0688c5b7605e594
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1429.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1429.xbm b/ncalib_polar/_8345_tex2html_wrap1429.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..91c8bc81d4b770eceb1cd6e590c91e5583d9f528
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1429.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x1e,0x09,0x3c,0xbf,0x0b,0x1c,0x85,0x09,
+ 0x04,0x15,0x0d,0x00,0x1f,0x0f,0x00,0x80,0x05,0x00,0x80,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1431.png b/ncalib_polar/_8345_tex2html_wrap1431.png
new file mode 100644
index 0000000000000000000000000000000000000000..d4bf525533831a06d74a109b5790661218f83af8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1431.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1431.xbm b/ncalib_polar/_8345_tex2html_wrap1431.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..173463801eed149e1bdea3f2c39c26160c6a48d1
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1431.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x92,0x07,0x3c,0xd7,0x0f,0x1c,0x53,0x01,
+ 0x04,0x5a,0x05,0x00,0xde,0x07,0x00,0x0b,0x00,0x00,0x0f,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1469.png b/ncalib_polar/_8345_tex2html_wrap1469.png
new file mode 100644
index 0000000000000000000000000000000000000000..d8fd5c534f1f2abdc564aab2905b34c6e279a0f2
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1469.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1469.xbm b/ncalib_polar/_8345_tex2html_wrap1469.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4e4e8d7e46ba45b05a47094344ec1bf5a87a25bc
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1469.xbm
@@ -0,0 +1,11 @@
+#define noname_width 36
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x60,0x00,0x08,
+ 0x01,0x00,0x60,0x00,0x08,0x01,0x00,0x60,0x00,0x08,0x01,0x00,0x60,0x00,0x08,
+ 0x01,0xc7,0x61,0x38,0x08,0xc1,0xef,0x63,0x7e,0x08,0xc1,0x2c,0x67,0x66,0x08,
+ 0x61,0x80,0x67,0x03,0x08,0x61,0xe0,0x67,0x03,0x08,0xe1,0x70,0x66,0x07,0x08,
+ 0xc1,0x7d,0x67,0x6e,0x08,0x81,0xef,0x67,0x7c,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1471.png b/ncalib_polar/_8345_tex2html_wrap1471.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1471.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1471.xbm b/ncalib_polar/_8345_tex2html_wrap1471.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1471.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1473.png b/ncalib_polar/_8345_tex2html_wrap1473.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1473.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1473.xbm b/ncalib_polar/_8345_tex2html_wrap1473.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1473.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1475.png b/ncalib_polar/_8345_tex2html_wrap1475.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1475.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1475.xbm b/ncalib_polar/_8345_tex2html_wrap1475.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1475.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1477.png b/ncalib_polar/_8345_tex2html_wrap1477.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1477.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1477.xbm b/ncalib_polar/_8345_tex2html_wrap1477.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1477.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1479.png b/ncalib_polar/_8345_tex2html_wrap1479.png
new file mode 100644
index 0000000000000000000000000000000000000000..c2aca3de81513a8a697084c6aa264f03650b4222
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1479.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1479.xbm b/ncalib_polar/_8345_tex2html_wrap1479.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d03498aed57b5f8164109f7386d2c620c89ab341
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1479.xbm
@@ -0,0 +1,7 @@
+#define noname_width 18
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0xc1,0x07,0x02,
+ 0xc1,0x0f,0x02,0xc1,0x0c,0x02,0xc1,0x1c,0x02,0xc1,0x18,0x02,0xc1,0x1c,0x02,
+ 0xc1,0x0f,0x02,0xc1,0x0f,0x02,0xc1,0x00,0x02,0xc1,0x00,0x02,0xc1,0x00,0x02,
+ 0xc1,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1481.png b/ncalib_polar/_8345_tex2html_wrap1481.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1481.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1481.xbm b/ncalib_polar/_8345_tex2html_wrap1481.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1481.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1483.png b/ncalib_polar/_8345_tex2html_wrap1483.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1483.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1483.xbm b/ncalib_polar/_8345_tex2html_wrap1483.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1483.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1519.png b/ncalib_polar/_8345_tex2html_wrap1519.png
new file mode 100644
index 0000000000000000000000000000000000000000..322b5296b184fcd471f9d8a47266c33b9bf58e00
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1519.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1519.xbm b/ncalib_polar/_8345_tex2html_wrap1519.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..38db43f18f755445096eb6810bb38b1193a80422
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1519.xbm
@@ -0,0 +1,9 @@
+#define noname_width 29
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x10,0x01,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x10,0x01,0x00,0x00,0x10,0x01,0x00,0x30,0x10,0x01,0x00,0x30,0x10,0x81,0xe3,
+ 0xf8,0x10,0xc1,0xf7,0xf9,0x10,0x61,0x3e,0x33,0x10,0xe1,0xfb,0x33,0x10,0xc1,
+ 0xff,0x33,0x10,0x01,0x1e,0x30,0x10,0x61,0x3e,0xb3,0x10,0xe1,0xf7,0xf3,0x10,
+ 0x01,0x00,0x00,0x10,0x01,0x00,0x00,0x10,0x01,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x10,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1521.png b/ncalib_polar/_8345_tex2html_wrap1521.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1521.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1521.xbm b/ncalib_polar/_8345_tex2html_wrap1521.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1521.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1523.png b/ncalib_polar/_8345_tex2html_wrap1523.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1523.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1523.xbm b/ncalib_polar/_8345_tex2html_wrap1523.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1523.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1525.png b/ncalib_polar/_8345_tex2html_wrap1525.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1525.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1525.xbm b/ncalib_polar/_8345_tex2html_wrap1525.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1525.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1527.png b/ncalib_polar/_8345_tex2html_wrap1527.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1527.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1527.xbm b/ncalib_polar/_8345_tex2html_wrap1527.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1527.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1529.png b/ncalib_polar/_8345_tex2html_wrap1529.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1529.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1529.xbm b/ncalib_polar/_8345_tex2html_wrap1529.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1529.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1531.png b/ncalib_polar/_8345_tex2html_wrap1531.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1531.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1531.xbm b/ncalib_polar/_8345_tex2html_wrap1531.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1531.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1563.png b/ncalib_polar/_8345_tex2html_wrap1563.png
new file mode 100644
index 0000000000000000000000000000000000000000..7e45e24587b9951bf6c0e93cae5994a27b6ef32a
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1563.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1563.xbm b/ncalib_polar/_8345_tex2html_wrap1563.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7719bf6fc2d1953aeb9196b158ca210e7269015b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1563.xbm
@@ -0,0 +1,11 @@
+#define noname_width 35
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,0x01,0x00,0xc6,0x00,0x04,
+ 0x01,0x00,0xc6,0x00,0x04,0x01,0x00,0x06,0x06,0x04,0x01,0x00,0x06,0x06,0x04,
+ 0x81,0xc3,0xc7,0x1f,0x04,0xc1,0xe7,0xc7,0x1f,0x04,0xe1,0x6c,0xc6,0x06,0x04,
+ 0xe1,0x3f,0xc6,0x06,0x04,0xe1,0x3f,0xc6,0x06,0x04,0x61,0x70,0xc6,0x06,0x04,
+ 0xe1,0x6c,0xc7,0x16,0x04,0xc1,0xef,0xc7,0x1e,0x04,0x01,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x04,
+ 0xff,0xff,0xff,0xff,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1565.png b/ncalib_polar/_8345_tex2html_wrap1565.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1565.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1565.xbm b/ncalib_polar/_8345_tex2html_wrap1565.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1565.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1567.png b/ncalib_polar/_8345_tex2html_wrap1567.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1567.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1567.xbm b/ncalib_polar/_8345_tex2html_wrap1567.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1567.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1569.png b/ncalib_polar/_8345_tex2html_wrap1569.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1569.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1569.xbm b/ncalib_polar/_8345_tex2html_wrap1569.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1569.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1571.png b/ncalib_polar/_8345_tex2html_wrap1571.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1571.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1571.xbm b/ncalib_polar/_8345_tex2html_wrap1571.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1571.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1573.png b/ncalib_polar/_8345_tex2html_wrap1573.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1573.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1573.xbm b/ncalib_polar/_8345_tex2html_wrap1573.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1573.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1575.png b/ncalib_polar/_8345_tex2html_wrap1575.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1575.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1575.xbm b/ncalib_polar/_8345_tex2html_wrap1575.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1575.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1589.png b/ncalib_polar/_8345_tex2html_wrap1589.png
new file mode 100644
index 0000000000000000000000000000000000000000..1860280faa7cfa7fa5d81efcb0c92c8b6199a4af
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1589.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1589.xbm b/ncalib_polar/_8345_tex2html_wrap1589.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..596792ae21fce2faa747db8223eb22a970faba84
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1589.xbm
@@ -0,0 +1,9 @@
+#define noname_width 38
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x3f,0x01,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0x00,0x20,0xe1,0xcf,0xb1,0x38,0x20,0xe1,0xef,0xf3,0xfc,0x20,
+ 0x01,0x77,0x76,0xce,0x20,0x01,0xf3,0x37,0x86,0x21,0x81,0xf3,0x37,0x86,0x21,
+ 0xc1,0x31,0x30,0xc6,0x21,0xe1,0x70,0x36,0xee,0x20,0xe1,0xef,0x37,0x7c,0x20,
+ 0x01,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0x00,0x20,0xff,0xff,0xff,0xff,0x3f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1591.png b/ncalib_polar/_8345_tex2html_wrap1591.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1591.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1591.xbm b/ncalib_polar/_8345_tex2html_wrap1591.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1591.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1593.png b/ncalib_polar/_8345_tex2html_wrap1593.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1593.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1593.xbm b/ncalib_polar/_8345_tex2html_wrap1593.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1593.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1595.png b/ncalib_polar/_8345_tex2html_wrap1595.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1595.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1595.xbm b/ncalib_polar/_8345_tex2html_wrap1595.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1595.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1599.png b/ncalib_polar/_8345_tex2html_wrap1599.png
new file mode 100644
index 0000000000000000000000000000000000000000..13af9d951332a4a83a7131be2c4fddbcdd619896
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1599.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1599.xbm b/ncalib_polar/_8345_tex2html_wrap1599.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6cdf15731d0f84a7dfd307d9d39e87bb3e5ea14b
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1599.xbm
@@ -0,0 +1,5 @@
+#define noname_width 14
+#define noname_height 12
+static char noname_bits[] = {
+ 0x78,0x00,0xcc,0x01,0x86,0x01,0x06,0x03,0xfb,0x03,0xfb,0x23,0x03,0x23,0x06,
+ 0x13,0x86,0x39,0xdc,0x18,0x70,0x30,0x00,0x38};
diff --git a/ncalib_polar/_8345_tex2html_wrap1639.png b/ncalib_polar/_8345_tex2html_wrap1639.png
new file mode 100644
index 0000000000000000000000000000000000000000..d8051fb2f6bad7fa177d044d106d99b7db0bcc5d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1639.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1639.xbm b/ncalib_polar/_8345_tex2html_wrap1639.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ebc3de761874686cf722ea7ca10cb75bf8ffc046
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1639.xbm
@@ -0,0 +1,11 @@
+#define noname_width 41
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0xc7,0xe1,0x33,0x06,0x01,
+ 0xc1,0xef,0xe7,0x37,0x06,0x01,0xc1,0x7c,0x66,0x76,0x07,0x01,0x61,0x30,0x6c,
+ 0x6e,0x03,0x01,0x61,0x30,0x6c,0x6c,0x03,0x01,0xe1,0x30,0x6e,0xce,0x03,0x01,
+ 0xc1,0x7d,0xe7,0xc7,0x01,0x01,0x81,0xef,0xe3,0xc7,0x01,0x01,0x01,0x00,0x60,
+ 0xc0,0x00,0x01,0x01,0x00,0x60,0xc0,0x00,0x01,0x01,0x00,0x60,0xf0,0x00,0x01,
+ 0x01,0x00,0x60,0x70,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0x01};
diff --git a/ncalib_polar/_8345_tex2html_wrap1641.png b/ncalib_polar/_8345_tex2html_wrap1641.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1641.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1641.xbm b/ncalib_polar/_8345_tex2html_wrap1641.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1641.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1643.png b/ncalib_polar/_8345_tex2html_wrap1643.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1643.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1643.xbm b/ncalib_polar/_8345_tex2html_wrap1643.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1643.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1645.png b/ncalib_polar/_8345_tex2html_wrap1645.png
new file mode 100644
index 0000000000000000000000000000000000000000..299f444c449b70982e0f4043c5c6e54de1cfd072
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1645.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1645.xbm b/ncalib_polar/_8345_tex2html_wrap1645.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..21d6c0d20dec68127a2803f418d73ca4a72b0761
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1645.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x03,0x02,
+ 0xc1,0x07,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,
+ 0x61,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,
+ 0xc1,0x07,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1647.png b/ncalib_polar/_8345_tex2html_wrap1647.png
new file mode 100644
index 0000000000000000000000000000000000000000..128acb75183abb80b30bff0b561db314a717bbc5
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1647.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1647.xbm b/ncalib_polar/_8345_tex2html_wrap1647.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8823da46d9608cdccce7f81d5866f44e68c86b66
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1647.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xc1,0x07,0x02,0xc1,0x07,0x02,0x01,0x0c,0x02,0x01,0x0e,0x02,0x01,0x07,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,
+ 0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1649.png b/ncalib_polar/_8345_tex2html_wrap1649.png
new file mode 100644
index 0000000000000000000000000000000000000000..b4446b1cab1666d7a9cb7207adb2ab60e57b0257
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1649.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1649.xbm b/ncalib_polar/_8345_tex2html_wrap1649.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..215061ca242c847a430f689335b21a688d17d4f3
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1649.xbm
@@ -0,0 +1,12 @@
+#define noname_width 42
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x03,0x01,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x02,0x81,0x03,0x00,0x80,0x01,0x02,
+ 0xc1,0x07,0x80,0xe3,0x03,0x02,0xc1,0x0c,0x80,0x63,0x06,0x02,0x41,0x0c,0xc0,
+ 0x63,0x06,0x02,0x01,0x0c,0xc7,0x63,0x06,0x02,0x81,0xc7,0x6f,0xe3,0x03,0x02,
+ 0x81,0xc7,0x6c,0xe3,0x03,0x02,0x01,0x6c,0x30,0x63,0x06,0x02,0x01,0x6c,0xf0,
+ 0x3f,0x06,0x02,0x21,0xec,0x00,0x33,0x06,0x02,0x61,0xcc,0x0d,0x63,0x06,0x02,
+ 0xc1,0x8f,0x0f,0xe3,0x07,0x02,0x81,0x03,0x00,0x80,0x01,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x02,
+ 0xff,0xff,0xff,0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1651.png b/ncalib_polar/_8345_tex2html_wrap1651.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1651.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1651.xbm b/ncalib_polar/_8345_tex2html_wrap1651.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1651.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1653.png b/ncalib_polar/_8345_tex2html_wrap1653.png
new file mode 100644
index 0000000000000000000000000000000000000000..d8051fb2f6bad7fa177d044d106d99b7db0bcc5d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1653.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1653.xbm b/ncalib_polar/_8345_tex2html_wrap1653.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ebc3de761874686cf722ea7ca10cb75bf8ffc046
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1653.xbm
@@ -0,0 +1,11 @@
+#define noname_width 41
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0xc7,0xe1,0x33,0x06,0x01,
+ 0xc1,0xef,0xe7,0x37,0x06,0x01,0xc1,0x7c,0x66,0x76,0x07,0x01,0x61,0x30,0x6c,
+ 0x6e,0x03,0x01,0x61,0x30,0x6c,0x6c,0x03,0x01,0xe1,0x30,0x6e,0xce,0x03,0x01,
+ 0xc1,0x7d,0xe7,0xc7,0x01,0x01,0x81,0xef,0xe3,0xc7,0x01,0x01,0x01,0x00,0x60,
+ 0xc0,0x00,0x01,0x01,0x00,0x60,0xc0,0x00,0x01,0x01,0x00,0x60,0xf0,0x00,0x01,
+ 0x01,0x00,0x60,0x70,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0x01};
diff --git a/ncalib_polar/_8345_tex2html_wrap1655.png b/ncalib_polar/_8345_tex2html_wrap1655.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1655.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1655.xbm b/ncalib_polar/_8345_tex2html_wrap1655.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1655.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1657.png b/ncalib_polar/_8345_tex2html_wrap1657.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1657.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1657.xbm b/ncalib_polar/_8345_tex2html_wrap1657.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1657.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1659.png b/ncalib_polar/_8345_tex2html_wrap1659.png
new file mode 100644
index 0000000000000000000000000000000000000000..299f444c449b70982e0f4043c5c6e54de1cfd072
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1659.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1659.xbm b/ncalib_polar/_8345_tex2html_wrap1659.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..21d6c0d20dec68127a2803f418d73ca4a72b0761
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1659.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x03,0x02,
+ 0xc1,0x07,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,
+ 0x61,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,
+ 0xc1,0x07,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1661.png b/ncalib_polar/_8345_tex2html_wrap1661.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1661.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1661.xbm b/ncalib_polar/_8345_tex2html_wrap1661.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1661.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1663.png b/ncalib_polar/_8345_tex2html_wrap1663.png
new file mode 100644
index 0000000000000000000000000000000000000000..e08ee4ef74e39c7766328bc2cbf815070aef5884
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1663.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1663.xbm b/ncalib_polar/_8345_tex2html_wrap1663.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..dbd3ef8d30fd73112782116c3a9e67f37808eadb
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1663.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x02,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x03,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0xc1,0x03,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x01,0x03,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x01,0x03,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x03,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0x01,0xc3,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xc1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1667.png b/ncalib_polar/_8345_tex2html_wrap1667.png
new file mode 100644
index 0000000000000000000000000000000000000000..a8e52af2cecf82af29a8cec91327912bb8414aba
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1667.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1667.xbm b/ncalib_polar/_8345_tex2html_wrap1667.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5254652e47f2915df9367788eca7e6b2e34c08b0
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1667.xbm
@@ -0,0 +1,10 @@
+#define noname_width 45
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,0x61,0xfc,0xe7,0xb0,0x1c,0x10,
+ 0x61,0xfc,0xf7,0xf1,0x7e,0x10,0xe1,0x8e,0x3b,0x73,0x67,0x10,0xc1,0x86,0xf9,
+ 0x33,0xc3,0x10,0xc1,0xc6,0xf9,0x33,0xc3,0x10,0xc1,0xe7,0x18,0x30,0xe3,0x10,
+ 0x81,0x73,0x38,0x33,0x77,0x10,0x81,0xf3,0xf7,0x33,0x3e,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x00,0x10,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1669.png b/ncalib_polar/_8345_tex2html_wrap1669.png
new file mode 100644
index 0000000000000000000000000000000000000000..e29443a545b82a10f015ca1dcce9cbd521160eae
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1669.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1669.xbm b/ncalib_polar/_8345_tex2html_wrap1669.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d068a8cc09189b1aa9d9a699f0c5a793d32cc8bf
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1669.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x24,0x86,0xf9,0x2f,0xee,0x29,0x26,
+ 0x38,0xa8,0x34,0x00,0xf8,0x3c,0x00,0x00,0x16,0x00,0x00,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1671.png b/ncalib_polar/_8345_tex2html_wrap1671.png
new file mode 100644
index 0000000000000000000000000000000000000000..125f9be4f7803518976a45cfe859e0fc0f27add9
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1671.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1671.xbm b/ncalib_polar/_8345_tex2html_wrap1671.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6fb709724851e9baaf7a06a843d291728b3b8cc8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1671.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x3c,0x86,0xb9,0x7e,0xee,0x99,0x0a,
+ 0x38,0xd0,0x2a,0x00,0xf0,0x3e,0x00,0x58,0x00,0x00,0x78,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1673.png b/ncalib_polar/_8345_tex2html_wrap1673.png
new file mode 100644
index 0000000000000000000000000000000000000000..b5bfdf5e9c6d532d84fd3b6066ce6f859809241b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1673.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1673.xbm b/ncalib_polar/_8345_tex2html_wrap1673.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..eeaeffd3a4e6a28c8ef9aa1d283f9b56989836af
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1673.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 12
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0xf1,0x3c,0x86,0xf9,0x7f,0xee,0x29,0x0a,
+ 0x38,0xa8,0x2a,0x00,0xf8,0x3e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1675.png b/ncalib_polar/_8345_tex2html_wrap1675.png
new file mode 100644
index 0000000000000000000000000000000000000000..aa2d50b2182e7418021f0af05eea8a4ad868ade8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1675.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1675.xbm b/ncalib_polar/_8345_tex2html_wrap1675.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..344e9d81f2e35050db9bcc61f5565be08d60f9de
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1675.xbm
@@ -0,0 +1,6 @@
+#define noname_width 22
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x00,0x18,0x07,0x00,0x0c,0x02,0x00,0x06,0x02,0x00,0x06,0x00,0x00,
+ 0x07,0x00,0x00,0xc3,0x03,0x00,0x83,0x91,0x24,0x86,0xb9,0x2e,0xee,0x99,0x26,
+ 0x38,0xd0,0x34,0x00,0xf0,0x3c,0x00,0x58,0x16,0x00,0x78,0x1e};
diff --git a/ncalib_polar/_8345_tex2html_wrap1679.png b/ncalib_polar/_8345_tex2html_wrap1679.png
new file mode 100644
index 0000000000000000000000000000000000000000..bb6f18d8ce6e98220ae67999e6f1b79830f7369f
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1679.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1679.xbm b/ncalib_polar/_8345_tex2html_wrap1679.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..18fd0e442bde3abb92c8f9f09b56d8901b24b4e1
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1679.xbm
@@ -0,0 +1,13 @@
+#define noname_width 80
+#define noname_height 14
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0xd8,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc8,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x8c,0x1c,0x00,0x80,0xff,0x80,
+ 0x03,0x00,0xf0,0x1f,0x8c,0x06,0x00,0xc0,0xff,0xc0,0x00,0x00,0xf8,0x1f,0x8c,
+ 0x0f,0x00,0x00,0x00,0xe0,0x01,0x00,0x00,0x00,0x8c,0x83,0x27,0x01,0x00,0x60,
+ 0x90,0x3c,0x00,0x00,0x8c,0xc3,0x7f,0xc1,0xff,0x60,0xb8,0x7e,0xf8,0x1f,0xc8,
+ 0x5e,0x31,0x01,0x00,0xc0,0x9b,0x0a,0x00,0x00,0xd8,0x40,0xa5,0x01,0x00,0x00,
+ 0xd0,0x2a,0x00,0x00,0x70,0xc0,0xe7,0x01,0x00,0x00,0xf0,0x3e,0x00,0x00,0x00,
+ 0x00,0xb0,0x00,0x00,0x00,0x58,0x00,0x00,0x00,0x00,0x00,0xf0,0x00,0x00,0x00,
+ 0x78,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1681.png b/ncalib_polar/_8345_tex2html_wrap1681.png
new file mode 100644
index 0000000000000000000000000000000000000000..34deed29717d569ecccda43b52377b1e2fd691cd
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1681.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1681.xbm b/ncalib_polar/_8345_tex2html_wrap1681.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7fec97c69be6a0759421d6d0f16607f0f1093092
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1681.xbm
@@ -0,0 +1,11 @@
+#define noname_width 65
+#define noname_height 13
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xb0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x90,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x18,0x01,0x3c,0x00,0xff,0xc1,0x0f,0xc0,0x7f,0x18,0x01,
+ 0x36,0x81,0xff,0xe1,0x4d,0xe0,0x7f,0x18,0x01,0x33,0x01,0x00,0xc0,0x4c,0x00,
+ 0x00,0x18,0x01,0x93,0x00,0x00,0xc0,0x2c,0x00,0x00,0x18,0x01,0xdb,0x81,0xff,
+ 0xc1,0x76,0xe0,0x7f,0x90,0x01,0xde,0x00,0x00,0xc0,0x33,0x00,0x00,0xb0,0x01,
+ 0x98,0x01,0x00,0x60,0x60,0x00,0x00,0xe0,0x00,0xc8,0x01,0x00,0x60,0x70,0x00,
+ 0x00,0x00,0x00,0x1e,0x00,0x00,0xf0,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1683.png b/ncalib_polar/_8345_tex2html_wrap1683.png
new file mode 100644
index 0000000000000000000000000000000000000000..0ab29066dda29d16d9e92ccf2ed582aad97c416d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1683.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1683.xbm b/ncalib_polar/_8345_tex2html_wrap1683.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e97c677ae9ed918bcc39afecebd2aae1cd7a63bc
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1683.xbm
@@ -0,0 +1,5 @@
+#define noname_width 9
+#define noname_height 13
+static char noname_bits[] = {
+ 0x40,0x00,0x40,0x00,0x20,0x00,0x20,0x00,0xae,0x01,0xaf,0x01,0x96,0x01,0x96,
+ 0x00,0xd6,0x00,0x7c,0x00,0x08,0x00,0x08,0x00,0x08,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1685.png b/ncalib_polar/_8345_tex2html_wrap1685.png
new file mode 100644
index 0000000000000000000000000000000000000000..5bdddca70a6b355eb774331cc0688c5b7605e594
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1685.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1685.xbm b/ncalib_polar/_8345_tex2html_wrap1685.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..91c8bc81d4b770eceb1cd6e590c91e5583d9f528
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1685.xbm
@@ -0,0 +1,6 @@
+#define noname_width 20
+#define noname_height 14
+static char noname_bits[] = {
+ 0x86,0x00,0x00,0x87,0x01,0x00,0x8c,0x01,0x00,0x0c,0x01,0x00,0x8c,0x00,0x00,
+ 0xcc,0x00,0x00,0x6c,0x00,0x00,0x7c,0x1e,0x09,0x3c,0xbf,0x0b,0x1c,0x85,0x09,
+ 0x04,0x15,0x0d,0x00,0x1f,0x0f,0x00,0x80,0x05,0x00,0x80,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1715.png b/ncalib_polar/_8345_tex2html_wrap1715.png
new file mode 100644
index 0000000000000000000000000000000000000000..d8fd5c534f1f2abdc564aab2905b34c6e279a0f2
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1715.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1715.xbm b/ncalib_polar/_8345_tex2html_wrap1715.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4e4e8d7e46ba45b05a47094344ec1bf5a87a25bc
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1715.xbm
@@ -0,0 +1,11 @@
+#define noname_width 36
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x60,0x00,0x08,
+ 0x01,0x00,0x60,0x00,0x08,0x01,0x00,0x60,0x00,0x08,0x01,0x00,0x60,0x00,0x08,
+ 0x01,0xc7,0x61,0x38,0x08,0xc1,0xef,0x63,0x7e,0x08,0xc1,0x2c,0x67,0x66,0x08,
+ 0x61,0x80,0x67,0x03,0x08,0x61,0xe0,0x67,0x03,0x08,0xe1,0x70,0x66,0x07,0x08,
+ 0xc1,0x7d,0x67,0x6e,0x08,0x81,0xef,0x67,0x7c,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1717.png b/ncalib_polar/_8345_tex2html_wrap1717.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1717.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1717.xbm b/ncalib_polar/_8345_tex2html_wrap1717.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1717.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1719.png b/ncalib_polar/_8345_tex2html_wrap1719.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1719.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1719.xbm b/ncalib_polar/_8345_tex2html_wrap1719.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1719.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1721.png b/ncalib_polar/_8345_tex2html_wrap1721.png
new file mode 100644
index 0000000000000000000000000000000000000000..299f444c449b70982e0f4043c5c6e54de1cfd072
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1721.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1721.xbm b/ncalib_polar/_8345_tex2html_wrap1721.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..21d6c0d20dec68127a2803f418d73ca4a72b0761
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1721.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x03,0x02,
+ 0xc1,0x07,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,
+ 0x61,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,
+ 0xc1,0x07,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1723.png b/ncalib_polar/_8345_tex2html_wrap1723.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1723.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1723.xbm b/ncalib_polar/_8345_tex2html_wrap1723.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1723.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1725.png b/ncalib_polar/_8345_tex2html_wrap1725.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1725.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1725.xbm b/ncalib_polar/_8345_tex2html_wrap1725.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1725.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1751.png b/ncalib_polar/_8345_tex2html_wrap1751.png
new file mode 100644
index 0000000000000000000000000000000000000000..8a80cc710097568659d1df3c897c6152fca00f5a
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1751.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1751.xbm b/ncalib_polar/_8345_tex2html_wrap1751.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a203e0280908ee1bfa03a796aecda7afa36b70d1
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1751.xbm
@@ -0,0 +1,13 @@
+#define noname_width 46
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x3f,0x01,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,
+ 0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0xc0,0x00,0x20,0x01,0x00,0x00,0xc0,0x00,0x20,0x01,0x00,0x00,
+ 0xc0,0x00,0x20,0x01,0x00,0x00,0xc0,0x00,0x20,0x81,0xc3,0xc7,0xc7,0xc6,0x20,
+ 0xc1,0xc7,0xcf,0xcf,0xc6,0x20,0x41,0xce,0xcc,0xcc,0xee,0x20,0x01,0xcf,0xdc,
+ 0xdc,0x6c,0x20,0xc1,0xcf,0xd8,0xd8,0x6c,0x20,0xe1,0xcc,0xdc,0xdc,0x78,0x20,
+ 0xe1,0xce,0xcf,0xcf,0x38,0x20,0xc1,0xcf,0xcf,0xcf,0x38,0x20,0x01,0xc0,0xc0,
+ 0x00,0x18,0x20,0x01,0xc0,0xc0,0x00,0x18,0x20,0x01,0xc0,0xc0,0x00,0x1e,0x20,
+ 0x01,0xc0,0xc0,0x00,0x0e,0x20,0x01,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,
+ 0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x20,0xff,0xff,0xff,0xff,0xff,0x3f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1753.png b/ncalib_polar/_8345_tex2html_wrap1753.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1753.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1753.xbm b/ncalib_polar/_8345_tex2html_wrap1753.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1753.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1755.png b/ncalib_polar/_8345_tex2html_wrap1755.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1755.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1755.xbm b/ncalib_polar/_8345_tex2html_wrap1755.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1755.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1757.png b/ncalib_polar/_8345_tex2html_wrap1757.png
new file mode 100644
index 0000000000000000000000000000000000000000..299f444c449b70982e0f4043c5c6e54de1cfd072
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1757.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1757.xbm b/ncalib_polar/_8345_tex2html_wrap1757.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..21d6c0d20dec68127a2803f418d73ca4a72b0761
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1757.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x03,0x02,
+ 0xc1,0x07,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,
+ 0x61,0x0c,0x02,0x61,0x0c,0x02,0x61,0x0c,0x02,0xc1,0x0c,0x02,0xc1,0x0c,0x02,
+ 0xc1,0x07,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1759.png b/ncalib_polar/_8345_tex2html_wrap1759.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1759.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1759.xbm b/ncalib_polar/_8345_tex2html_wrap1759.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1759.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1761.png b/ncalib_polar/_8345_tex2html_wrap1761.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1761.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1761.xbm b/ncalib_polar/_8345_tex2html_wrap1761.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1761.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1801.png b/ncalib_polar/_8345_tex2html_wrap1801.png
new file mode 100644
index 0000000000000000000000000000000000000000..0f917e133cc34a127ab3b7f5ac1fb855b39780fa
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1801.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1801.xbm b/ncalib_polar/_8345_tex2html_wrap1801.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2fbfb2e6307a2d24778351a036d3b5f3df1000a3
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1801.xbm
@@ -0,0 +1,9 @@
+#define noname_width 32
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x80,0x01,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x80,0x01,0x00,0x30,0x80,0x01,0x00,0x30,0x80,0x01,0x00,
+ 0x30,0x80,0x01,0x00,0x30,0x80,0x81,0x83,0x33,0x83,0xc1,0xc7,0xb7,0x83,0x41,
+ 0x6e,0xf6,0x81,0x01,0xef,0xf3,0x80,0xc1,0xcf,0xf7,0x81,0xe1,0x0c,0xb6,0x81,
+ 0xe1,0x6e,0xb6,0x83,0xc1,0xef,0x37,0x87,0x01,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x80,0x01,0x00,0x00,0x80,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1803.png b/ncalib_polar/_8345_tex2html_wrap1803.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1803.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1803.xbm b/ncalib_polar/_8345_tex2html_wrap1803.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1803.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1805.png b/ncalib_polar/_8345_tex2html_wrap1805.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1805.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1805.xbm b/ncalib_polar/_8345_tex2html_wrap1805.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1805.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1807.png b/ncalib_polar/_8345_tex2html_wrap1807.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1807.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1807.xbm b/ncalib_polar/_8345_tex2html_wrap1807.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1807.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1809.png b/ncalib_polar/_8345_tex2html_wrap1809.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1809.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1809.xbm b/ncalib_polar/_8345_tex2html_wrap1809.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1809.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1811.png b/ncalib_polar/_8345_tex2html_wrap1811.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1811.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1811.xbm b/ncalib_polar/_8345_tex2html_wrap1811.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1811.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1813.png b/ncalib_polar/_8345_tex2html_wrap1813.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1813.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1813.xbm b/ncalib_polar/_8345_tex2html_wrap1813.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1813.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1815.png b/ncalib_polar/_8345_tex2html_wrap1815.png
new file mode 100644
index 0000000000000000000000000000000000000000..c6c5bf19c72bd237438646ac6e063e3638841bea
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1815.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1815.xbm b/ncalib_polar/_8345_tex2html_wrap1815.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..be858206e9d9c9da8c37e4eeef2b497bb8cc4ff6
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1815.xbm
@@ -0,0 +1,9 @@
+#define noname_width 63
+#define noname_height 11
+static char noname_bits[] = {
+ 0xf8,0xc1,0x1f,0x3f,0x00,0x00,0x60,0x38,0x30,0xc3,0x1c,0xe6,0x00,0x00,0xb0,
+ 0x29,0x18,0x63,0x0c,0xc3,0x00,0x00,0x90,0x6d,0x18,0x23,0x06,0xc3,0x00,0x00,
+ 0x18,0x6d,0x98,0x03,0x03,0xc3,0xc0,0x7f,0x18,0x39,0xf8,0x81,0x01,0xc3,0xe0,
+ 0x7f,0x18,0x01,0x0c,0xc0,0x8c,0xc1,0x00,0x00,0x18,0x01,0x0c,0x60,0x84,0x61,
+ 0x00,0x00,0x18,0x01,0x0c,0x70,0x86,0x71,0xe0,0x7f,0x90,0x01,0x1f,0xf8,0xe7,
+ 0x1f,0x00,0x00,0xb0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x00};
diff --git a/ncalib_polar/_8345_tex2html_wrap1845.png b/ncalib_polar/_8345_tex2html_wrap1845.png
new file mode 100644
index 0000000000000000000000000000000000000000..6e39f8f9bdbe1816b6ce5b1fb5393788816b0b1d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1845.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1845.xbm b/ncalib_polar/_8345_tex2html_wrap1845.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5767ecfc0c394087ddf54e27a00c91d45a382a49
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1845.xbm
@@ -0,0 +1,15 @@
+#define noname_width 59
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x18,0x04,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x18,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x18,0x04,0xc1,0x66,0x70,
+ 0xf8,0x98,0x71,0x18,0x04,0xc1,0xff,0xf8,0xf8,0x99,0xf9,0x18,0x04,0xc1,0xdd,
+ 0xc9,0x99,0x99,0xc9,0x19,0x04,0xc1,0x8c,0xe1,0x99,0x99,0xe1,0x19,0x04,0xc1,
+ 0x8c,0xf9,0x99,0x99,0xf9,0x19,0x04,0xc1,0x8c,0x9d,0x99,0x99,0x9d,0x19,0x04,
+ 0xc1,0x8c,0xdd,0x99,0xd9,0xdd,0x19,0x04,0xc1,0x8c,0xf9,0x99,0xf9,0xf9,0x19,
+ 0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1847.png b/ncalib_polar/_8345_tex2html_wrap1847.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1847.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1847.xbm b/ncalib_polar/_8345_tex2html_wrap1847.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1847.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1849.png b/ncalib_polar/_8345_tex2html_wrap1849.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1849.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1849.xbm b/ncalib_polar/_8345_tex2html_wrap1849.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1849.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1851.png b/ncalib_polar/_8345_tex2html_wrap1851.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1851.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1851.xbm b/ncalib_polar/_8345_tex2html_wrap1851.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1851.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1853.png b/ncalib_polar/_8345_tex2html_wrap1853.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1853.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1853.xbm b/ncalib_polar/_8345_tex2html_wrap1853.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1853.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1855.png b/ncalib_polar/_8345_tex2html_wrap1855.png
new file mode 100644
index 0000000000000000000000000000000000000000..2aef0ed91998c760ba2270dbb812a79c198109e3
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1855.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1855.xbm b/ncalib_polar/_8345_tex2html_wrap1855.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5d42a2f1c043127957eab65a92ea196a3d3ad7da
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1855.xbm
@@ -0,0 +1,8 @@
+#define noname_width 24
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x40,0x80,
+ 0x01,0x78,0x80,0x01,0x78,0x80,0x01,0x60,0x80,0x01,0x60,0x80,0x01,0x60,0x80,
+ 0x01,0x60,0x80,0xe1,0x63,0x80,0xe1,0x63,0x80,0x01,0x60,0x80,0x01,0x60,0x80,
+ 0x01,0xf8,0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0xff,0xff,0x7f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1857.png b/ncalib_polar/_8345_tex2html_wrap1857.png
new file mode 100644
index 0000000000000000000000000000000000000000..5355db230b7fe62ec4ae61e248b907d939e9ac15
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1857.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1857.xbm b/ncalib_polar/_8345_tex2html_wrap1857.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f64a3d2075f60ae2c5fa5c1b3e4f6a70db3788ce
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1857.xbm
@@ -0,0 +1,5 @@
+#define noname_width 15
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x38,0x0e,0x0c,0x18,0x1e,0x3c,0x36,0x36,0x63,0x63,0xc3,0x61,0xc3,
+ 0x61,0x63,0x63,0x36,0x36,0x1e,0x3c,0x0c,0x18,0x38,0x0e,0xf0,0x07};
diff --git a/ncalib_polar/_8345_tex2html_wrap1889.png b/ncalib_polar/_8345_tex2html_wrap1889.png
new file mode 100644
index 0000000000000000000000000000000000000000..745f6ef434dc9e8c8118dbeff560b14ddf05eb44
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1889.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1889.xbm b/ncalib_polar/_8345_tex2html_wrap1889.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..234d77a9411bb979329d54df57fdaef4f9b4255c
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1889.xbm
@@ -0,0 +1,9 @@
+#define noname_width 40
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x81,0xc3,0xe1,0xf8,0x80,0xc1,0xf7,0xf3,0xf9,0x81,
+ 0x61,0x36,0x93,0x9b,0x81,0xe1,0x1b,0xc0,0x9b,0x81,0xc1,0x1f,0xf0,0x9b,0x81,
+ 0x01,0x3e,0x38,0x9b,0x81,0x61,0x76,0xbb,0x9b,0x81,0xe1,0xe7,0xf3,0x9b,0x81,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1891.png b/ncalib_polar/_8345_tex2html_wrap1891.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1891.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1891.xbm b/ncalib_polar/_8345_tex2html_wrap1891.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1891.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1893.png b/ncalib_polar/_8345_tex2html_wrap1893.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1893.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1893.xbm b/ncalib_polar/_8345_tex2html_wrap1893.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1893.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1895.png b/ncalib_polar/_8345_tex2html_wrap1895.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1895.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1895.xbm b/ncalib_polar/_8345_tex2html_wrap1895.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1895.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1897.png b/ncalib_polar/_8345_tex2html_wrap1897.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1897.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1897.xbm b/ncalib_polar/_8345_tex2html_wrap1897.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1897.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1899.png b/ncalib_polar/_8345_tex2html_wrap1899.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1899.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1899.xbm b/ncalib_polar/_8345_tex2html_wrap1899.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1899.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1931.png b/ncalib_polar/_8345_tex2html_wrap1931.png
new file mode 100644
index 0000000000000000000000000000000000000000..d8051fb2f6bad7fa177d044d106d99b7db0bcc5d
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1931.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1931.xbm b/ncalib_polar/_8345_tex2html_wrap1931.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ebc3de761874686cf722ea7ca10cb75bf8ffc046
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1931.xbm
@@ -0,0 +1,11 @@
+#define noname_width 41
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0xc7,0xe1,0x33,0x06,0x01,
+ 0xc1,0xef,0xe7,0x37,0x06,0x01,0xc1,0x7c,0x66,0x76,0x07,0x01,0x61,0x30,0x6c,
+ 0x6e,0x03,0x01,0x61,0x30,0x6c,0x6c,0x03,0x01,0xe1,0x30,0x6e,0xce,0x03,0x01,
+ 0xc1,0x7d,0xe7,0xc7,0x01,0x01,0x81,0xef,0xe3,0xc7,0x01,0x01,0x01,0x00,0x60,
+ 0xc0,0x00,0x01,0x01,0x00,0x60,0xc0,0x00,0x01,0x01,0x00,0x60,0xf0,0x00,0x01,
+ 0x01,0x00,0x60,0x70,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0x01};
diff --git a/ncalib_polar/_8345_tex2html_wrap1933.png b/ncalib_polar/_8345_tex2html_wrap1933.png
new file mode 100644
index 0000000000000000000000000000000000000000..e68a0b4cdb1f4a96f801f99cb21c1243ad89d86b
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1933.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1933.xbm b/ncalib_polar/_8345_tex2html_wrap1933.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d92025bf97233f5e23b16486f33fca88287e17e9
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1933.xbm
@@ -0,0 +1,25 @@
+#define noname_width 104
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x20,0x30,0x38,0x00,0x80,0x01,0x00,
+ 0x60,0x70,0x80,0x01,0x00,0x00,0x3c,0x7c,0x7c,0xfe,0x80,0x01,0x00,0xf8,0xf8,
+ 0x80,0x01,0x00,0x00,0x3c,0xcc,0xcc,0xc0,0x00,0x00,0x00,0x98,0x99,0x81,0x01,
+ 0x00,0x00,0x30,0xce,0xc4,0xe0,0x00,0x00,0x00,0x9c,0x89,0x81,0xc1,0x87,0x63,
+ 0x31,0xc6,0xc0,0x60,0x80,0x71,0xf8,0x8c,0x81,0x81,0xc1,0xcf,0xe7,0x31,0xc6,
+ 0x78,0x30,0x80,0xf9,0xf8,0x8d,0xf1,0x80,0xc1,0x6c,0xe6,0x30,0xcc,0x78,0x30,
+ 0x80,0xc9,0x99,0x99,0xf1,0x80,0xc1,0xfc,0x63,0x30,0xfc,0xc0,0x30,0x80,0xe1,
+ 0x99,0xf9,0x81,0x81,0xc1,0xd8,0x67,0x30,0xf8,0xc0,0x18,0x80,0xf9,0x99,0xf1,
+ 0x81,0x81,0xc1,0x1c,0x66,0x30,0xc0,0xc2,0x18,0x80,0x9d,0x99,0x81,0x85,0x81,
+ 0xc1,0x6f,0x66,0x30,0x64,0xc6,0x18,0x8c,0xdd,0x99,0xc9,0x8c,0x81,0xc1,0xef,
+ 0x67,0xfc,0x7c,0xfc,0x18,0x8c,0xf9,0x99,0xf9,0xf8,0x81,0xc1,0x00,0x00,0x00,
+ 0x18,0x38,0x00,0x80,0x01,0x00,0x30,0x70,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xa0,0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,
+ 0x01,0x00,0x00,0x00,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/ncalib_polar/_8345_tex2html_wrap1935.png b/ncalib_polar/_8345_tex2html_wrap1935.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1935.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1935.xbm b/ncalib_polar/_8345_tex2html_wrap1935.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1935.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1937.png b/ncalib_polar/_8345_tex2html_wrap1937.png
new file mode 100644
index 0000000000000000000000000000000000000000..3e58544ff83fcb7ce6aafa9cb871f843ea5a66ae
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1937.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1937.xbm b/ncalib_polar/_8345_tex2html_wrap1937.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..c8756068dc0d2eb4d19aa7d98f3e74af027b8a82
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1937.xbm
@@ -0,0 +1,17 @@
+#define noname_width 69
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,0x01,0x03,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0xc1,0x07,0xf8,0x81,0x1f,0xf0,0x03,0x7e,0x10,0xc1,0x0c,0xf8,
+ 0x81,0x1f,0xf0,0x03,0x7e,0x10,0xc1,0x0c,0xf0,0x00,0x0f,0xe0,0x01,0x3c,0x10,
+ 0x61,0x0c,0xf8,0x81,0x1f,0xf0,0x03,0x7e,0x10,0x61,0x0c,0xe8,0x81,0x1e,0xd0,
+ 0x03,0x7a,0x10,0x61,0x0c,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,0x61,0x0c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x61,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xc1,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0xc1,0xcc,0x00,0x18,0x80,0x01,
+ 0x30,0x00,0x10,0xc1,0xc7,0x00,0x18,0x80,0x01,0x30,0x00,0x10,0x01,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1939.png b/ncalib_polar/_8345_tex2html_wrap1939.png
new file mode 100644
index 0000000000000000000000000000000000000000..128acb75183abb80b30bff0b561db314a717bbc5
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1939.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1939.xbm b/ncalib_polar/_8345_tex2html_wrap1939.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8823da46d9608cdccce7f81d5866f44e68c86b66
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1939.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xc1,0x07,0x02,0xc1,0x07,0x02,0x01,0x0c,0x02,0x01,0x0e,0x02,0x01,0x07,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,
+ 0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1941.png b/ncalib_polar/_8345_tex2html_wrap1941.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1941.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1941.xbm b/ncalib_polar/_8345_tex2html_wrap1941.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1941.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/ncalib_polar/_8345_tex2html_wrap1943.png b/ncalib_polar/_8345_tex2html_wrap1943.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d80fad1676a415cf87516278b4b9a2914d1e2c8
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1943.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1943.xbm b/ncalib_polar/_8345_tex2html_wrap1943.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6b45f10000f3214cc4649981fc402798c4c6cf48
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1943.xbm
@@ -0,0 +1,16 @@
+#define noname_width 69
+#define noname_height 21
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x81,0x03,0x60,0x00,0x06,0xc0,0x00,0x18,0x10,
+ 0xc1,0x07,0xf8,0x80,0x0f,0xf0,0x01,0x3e,0x10,0x41,0x0c,0x98,0x81,0x19,0x30,
+ 0x03,0x66,0x10,0x61,0x0c,0x98,0x81,0x19,0x30,0x03,0x66,0x10,0x41,0x0c,0x8c,
+ 0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x0c,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,
+ 0x01,0x0e,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x01,0x07,0x8c,0xc1,0x18,0x18,
+ 0x03,0x63,0x10,0x01,0x03,0x8c,0xc1,0x18,0x18,0x03,0x63,0x10,0x81,0x01,0x98,
+ 0x81,0x19,0x30,0x03,0x66,0x10,0xc1,0xc0,0x98,0x99,0x99,0x31,0x33,0x66,0x10,
+ 0xe1,0xcf,0xf8,0x98,0x8f,0xf1,0x31,0x3e,0x10,0x01,0x00,0x60,0x00,0x06,0xc0,
+ 0x00,0x18,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1945.png b/ncalib_polar/_8345_tex2html_wrap1945.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1945.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1945.xbm b/ncalib_polar/_8345_tex2html_wrap1945.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1945.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/_8345_tex2html_wrap1947.png b/ncalib_polar/_8345_tex2html_wrap1947.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_polar/_8345_tex2html_wrap1947.png differ
diff --git a/ncalib_polar/_8345_tex2html_wrap1947.xbm b/ncalib_polar/_8345_tex2html_wrap1947.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_polar/_8345_tex2html_wrap1947.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_polar/images.pl b/ncalib_polar/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..ff62bb5138e48568c8e1ec398b59cb466dcee354
--- /dev/null
+++ b/ncalib_polar/images.pl
@@ -0,0 +1,325 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$cGain_<<198>>yx<<198>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1355.xbm">'; 
+$key = q/{}fbox<<1092>>largesfask<<1092>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1801.xbm">'; 
+$key = q/{}$cVis_<<175>>xx<<175>>${}/;
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diff --git a/ncalib_polar/labels.pl b/ncalib_polar/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..62c1f1b37c6cb27f5a0112f9a93e30ece61cba1a
--- /dev/null
+++ b/ncalib_polar/labels.pl
@@ -0,0 +1,30 @@
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+
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diff --git a/ncalib_polar/ncalib_polar.html b/ncalib_polar/ncalib_polar.html
new file mode 100644
index 0000000000000000000000000000000000000000..9a4d111e2d3a1a71d8a7be6043e0a8861205fc30
--- /dev/null
+++ b/ncalib_polar/ncalib_polar.html
@@ -0,0 +1,978 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>NCALIB POLAR: Polarisation corrections</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncalib_polar.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncalib_polar.html#SECTION0002000000000000000>  <b>Preface </b></A>
+<LI> <A NAME=tex2html3 HREF=ncalib_polar.html#SECTION0003000000000000000> <b>WSRT polarisation calibration strategy</b></A>
+<LI> <A NAME=tex2html4 HREF=ncalib_polar.html#SECTION0004000000000000000> <b>Polarisation equations</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=ncalib_polar.html#SECTION0004100000000000000> <b>Parallel dipoles (++)</b></A>
+<LI> <A NAME=tex2html6 HREF=ncalib_polar.html#SECTION0004200000000000000> <b>X-Y Phase Zero Difference (PZD)</b></A>
+<LI> <A NAME=tex2html7 HREF=ncalib_polar.html#SECTION0004300000000000000> <b>Crossed dipoles (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1367.png">)</b></A>
+<LI> <A NAME=tex2html8 HREF=ncalib_polar.html#SECTION0004400000000000000> <b>Faraday rotation</b></A>
+</UL> 
+<LI> <A NAME=tex2html9 HREF=ncalib_polar.html#SECTION0005000000000000000> <b>POLAR SHOW: Show corrections</b></A>
+<LI> <A NAME=tex2html10 HREF=ncalib_polar.html#SECTION0006000000000000000> <b>POLAR CALC: Calculate corrections</b></A>
+<LI> <A NAME=tex2html11 HREF=ncalib_polar.html#SECTION0007000000000000000> <b>POLAR SET: Set corrections manually</b></A>
+<LI> <A NAME=tex2html12 HREF=ncalib_polar.html#SECTION0008000000000000000> <b>POLAR EDIT: Edit corrections</b></A>
+<LI> <A NAME=tex2html13 HREF=ncalib_polar.html#SECTION0009000000000000000> <b>POLAR ZERO: Zero corrections</b></A>
+<LI> <A NAME=tex2html14 HREF=ncalib_polar.html#SECTION00010000000000000000> <b>POLAR COPY: Copy corrections from somewhere else</b></A>
+<LI> <A NAME=tex2html15 HREF=ncalib_polar.html#SECTION00011000000000000000> <b>POLAR VZERO: X-Y Phase Zero Difference, assuming V=0</b></A>
+<UL> 
+<LI> <A NAME=tex2html16 HREF=ncalib_polar.html#SECTION00011100000000000000> <b>POLAR VZERO CALC: Calculate and show</b></A>
+<LI> <A NAME=tex2html17 HREF=ncalib_polar.html#SECTION00011200000000000000> <b>POLAR VZERO APPLY: Calculate, show and apply</b></A>
+<LI> <A NAME=tex2html18 HREF=ncalib_polar.html#SECTION00011300000000000000> <b>POLAR VZERO ASK: Calculate, check with user, and apply</b></A>
+<LI> <A NAME=tex2html19 HREF=ncalib_polar.html#SECTION00011400000000000000> <b>POLAR VZERO MANUAL: Ask for and apply</b></A>
+<LI> <A NAME=tex2html20 HREF=ncalib_polar.html#SECTION00011500000000000000> <b>POLAR VZERO SCAN: Calculate and apply on a per-scan basis</b></A>
+<LI> <A NAME=tex2html21 HREF=ncalib_polar.html#SECTION00011600000000000000> <b>POLAR VZERO COPY: Calculate from input and apply to output</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Preface </b></A></H1>
+<P>
+        This document describes the handling of polarisation calibration and correction by the NCALIB POLAR option.  This option is activated as follows: 
+   <BR> > <i>exe ncalib</i>   <PRE>
+      NCALIB$1 (v4.62) is started at 30-May-94 13:52:04
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>OPTION</b>
+ (REDUNDANCY, POLAR, SET, SHOW, QUIT)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1277.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1279.png">
+<P>
+		<i>Select option</i>
+<P>
+<A NAME=.strategy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0003000000000000000> <b>WSRT polarisation calibration strategy</b></A></H1>
+<P>
+        In the following, it will be assumed that the dipoles of the WSRT
+telescopes are <em>parallel</em> (++).  The usual calibration strategy consists of
+the following steps:
+<P>
+<UL><LI>
+        In addition to observing calibrators along with normal observations,
+the WSRT at regular intervals observes calibrators to determine various
+instrumental parameters which are reasonably constant. These corrections are
+automatically applied to your data at the telescope.
+<P>
+<LI>
+        The complex gain factors <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1281.png"> (i.e. dipole gain errors,
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1283.png">, and phase errors, <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1285.png"> are determined by
+observing a strong calibrator, for which an accurate model exists. The
+determination is done separately for the X-dipoles and the Y-dipoles, using
+<A HREF=" #.equ.pol.008">equation</A>.  <em>Note that any inaccuracy in the assumed value for Q
+will be interpreted as a gain error.  Also note that <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1287.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1289.png"> will be inaccurate by the value of the ``phase-zero difference
+(PZD)'' between the X and Y dipoles.</em>
+<P>
+<LI>
+        The dipole angle errors <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1409.png"> and ellipticities <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1599.png"> are
+determined by observing a strong <em>unpolarised</em> calibrator. This is done by
+means of NCALIB option POLAR CALC in this section, using <A HREF=" #.equ.pol.010">equation</A>.
+The measured corrections are stored (as POLC) in the <em>sector header</em> of the
+SCN-file. (I.e. they are assumed to be constant for the duration of an entire
+sector rather than to change from scan to scan.).
+<P>
+<LI>
+        The missing 'phase-zero difference (PZD)' between the X- and Y-dipoles
+is determined with the help of a calibrator with strong U. Again,
+<A HREF=" #.equ.pol.010">equation</A> is used.  It is assumed that <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1295.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1297.png">, which determine the `leakage' of the large I-term into the
+result, are negligible in this stage, and that <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1383.png">.  If this assumption is
+incorrect, this will translate into a spurious V in later observations.
+<P>
+<LI>
+        Ionospheric Faraday rotation may vary on much shorter timescales than
+the length of the observation.  This can be calibrated to a large extent by
+introducing external information, obtained by
+<A HREF="../ncalib_descr/ncalib_descr.html#.set.faraday">ionosonde measurements</A>.
+<P>
+<LI>
+        The WSRT instrumental polarisation is small, due to the placement of
+the feed on the axis of the antenna paraboloid.  The effect can be eliminated
+with the help of the multi-parameter <i>NEWSTAR </i> source model (see NMODEL).
+<P>
+</UL>
+<P>
+        For the best results, it may be necessary to iterate two or three
+times, because one pair of dipole errors (position angle/ellipticity) may
+affect the determination of the other pair (gain/phase).  However, the process
+will iterate to the correct result, because, <em>in the case of parallel
+dipoles</em>, all four types of dipole errors have distinct signatures.  This means
+that one type of dipole error cannot be interpreted as another type, and still
+give a consistent result.  Therefore, all four types can be determined
+independently.
+<P>
+<H1><A NAME=SECTION0004000000000000000> <b>Polarisation equations</b></A></H1>
+<P>
+        Each of the 14 WSRT telescopes have two perpendicular linear dipoles, X
+and Y.  In the existing front-ends, the XY-dipole unit can be rotated over an
+arbitrary angle.  The dipole position angle (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1301.png">) is defined from North
+(<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1303.png">) through East (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1305.png">).  The complex visibility
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1307.png"> that is measured with an interferometer (consisting of two dipoles
+with position angles <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1309.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1311.png"> can be written as (see Weiler,
+1973):
+<P>
+<P><A NAME=.equ.pol.002><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray140.png"><P>
+<P>
+in which I, Q, U and V are the Fourier transforms of the corresponding Stokes
+parameters of the observed source, and the <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1313.png">, <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1315.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1317.png">
+factors contain the four types of dipole errors: phase (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1319.png">), gain
+(<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1321.png">), dipole angle error (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1327.png">) and ellipticity (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1325.png">).
+In the ideal case, they are all zero. For small values of <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1327.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1325.png">,
+second-order terms can be ignored, and we can write:
+<P><A NAME=.equ.pol.004><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray149.png"><P>
+<P><A NAME=.equ.pol.006><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray154.png"><P>
+<P>
+<H2><A NAME=SECTION0004100000000000000> <b>Parallel dipoles (++)</b></A></H2>
+<P>
+In the `normal' position (+) of the dipole unit, <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1331.png"> (east), and
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1333.png"> (south). Usually the dipole units in all WSRT telescopes
+are set `parallel' (++) to each other. In this case, the equations reduce to a
+particularly simple form. Again ignoring second-order terms, we get <P><A NAME=.equ.pol.008><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray159.png"><P>
+<P><A NAME=.equ.pol.010><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray166.png"><P>
+in which <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1335.png"> is the visibility measured between the X-dipoles of
+telescopes <em>i</em> and <em>j</em>, etc. After calibration, <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1337.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1339.png">, and the complex Stokes values can be calculated from the observed
+visibilities:
+<P><A NAME=.equ.pol.014><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray178.png"><P>
+<P>
+In the parallel mode (++), the two sets of dipole errors (phase/gain and
+angle/ellipticity) are separable, and so can be determined. Nowadays (after
+December 1983), the dipoles are almost always parallel, and in the new
+frontends (after 1997), the dipoles will not be rotatable.
+<P>
+<H2><A NAME=SECTION0004200000000000000> <b>X-Y Phase Zero Difference (PZD)</b></A></H2>
+<P>
+In the case of parallel dipoles (++), the complex gain errors of the X-dipoles
+and those of the Y-dipoles are calibrated separately; <IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1341.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1343.png"> will usually not have enough signal for calibration, because these
+dipoles are nominally perpendicular and the fraction of linear polarisation is
+usually small in calibrators. Since we only calibrate phase <em>differences</em>,
+an arbitrary phase zero (<IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1345.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1347.png">) is assigned to the X-
+and Y-dipoles. These phase zeros will cancel out for <IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1349.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1351.png">, but not for <IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1353.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_13658_tex2html_wrap1355.png">. Thus, the latter
+will be multiplied by an unknown phase factor <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1683.png">, the so-called <em>XY
+Phase Zero Difference (PZD)</em>.
+<P>
+<P><A NAME=.equ.pol.018><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><A NAME=.equ.pol.016><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray200.png"><P>
+<P>
+in which <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1359.png">. Of course,
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1361.png"> is the complex gain of the interferometer made up of the X-dipole
+of telescope <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1363.png"> and Y-dipole of telescope <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1365.png">, etc.
+<P>
+<H2><A NAME=SECTION0004300000000000000> <b>Crossed dipoles (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1367.png">)</b></A></H2>
+<P>
+        Before 1983, polarisation measurements with the WSRT were usually
+carried out with dipoles in the fixed telescopes (0-9) in the `normal'
+position, and the dipoles in the movable telescopes (A-D) rotated by <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1369.png">
+(<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1371.png">), with <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1373.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1375.png">.  The 40 standard
+(fixed-movable) interferometers were said to have `crossed' (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1367.png">)
+dipoles.  In this case, the visibility equations take the following form:
+<P><A NAME=.equ.pol.022><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray213.png"><P>
+        With crossed dipoles, the signal-to-noise ratio of the xy/yx terms are
+similar to that of the xx/yy terms.  This makes it possible to make a
+redundancy calibration solution for all 28 dipoles simultaneously, <em>but
+only if we may assume that <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1383.png"></em>.  In principle, this would open the way to
+continuous polarisation calibration on the object itself, provided it has
+enough flux.
+<P>
+        However, crossed dipoles introduce a number of new problems that make
+them less attractive:
+<UL><LI> The two sets of dipole errors (phase/gain and angle/ellipticity) are no
+longer completely separable.  This means that the phase solution will influence
+the angle error solution, and the gain solution will influence the ellipticity
+solution.
+<P>
+<LI> For part of the telescopes, the four-petal clover-leaf pattern of
+instrumental polarisation will be rotated by <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1369.png"> with respect to the sky
+and with respect to the four legs that support the focus box. This complicates
+any calibration schemes for instrumental polarisation.
+<P>
+</UL>
+<P>
+        These problems, combined with the fact that the phase-zero problem is
+not really avoided (since redundancy solution is only possible if it has to be
+assumed that <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1383.png">) have led to the practice to use only parallel dipoles.
+<P>
+        <i>(Annotation by JPH 940624: The reader is cautioned that the
+arguments advanced here against the use of crossed dipoles are a matter of
+continuing controversy.  It can easily be shown from first principles that the
+separability of phase/gain and dipole errors is irrelevant. Furthermore, the
+parallel-dipole configuration is inherently asymmetric with respect to Stokes
+<em>Q</em> and <em>U</em> and crossed dipoles are clearly superior in this respect;
+how important this is is not clear.)</i>
+<P>
+<A NAME=.equ.pol.024><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004400000000000000> <b>Faraday rotation</b></A></H2>
+<P>
+When radiation passes through a charged medium (like the ionosphere), the place
+of linear polarisation will be rotated by the angle <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1393.png">:
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray247.png"><P>
+Note that <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1387.png">, <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1389.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1391.png"> are independent of <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1393.png">. The
+Faraday effect is strongly frequency-dependent: <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1395.png">.
+<P>
+<A NAME=.show><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0005000000000000000> <b>POLAR SHOW: Show corrections</b></A></H1>
+<P>
+The 56 correction factors (2 for each of the 28 dipoles) for angle errors and
+ellipticities that are stored in the <em>set header</em> (as POLC, see SCN-file
+description) can be viewed in a digestible form:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1403.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1405.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1407.png">
+<P>
+		<i>For example</i>    <PRE>
+ Sector: 2.0.0.0.0
+
+        Position          Ellipticity    Rotation Orthog.
+       X(%
+
+ 0    -1.13    -0.06    -0.37     0.54    -0.34     0.61
+ 1    -0.16     0.13     0.07     0.04    -0.01     0.17
+ 2     1.25     0.82     1.77    -2.56     0.59    -0.24
+ 3     0.49    -0.02     0.11     1.19     0.13    -0.29
+ 4    -0.72    -0.14    -0.03    -0.46    -0.25     0.33
+ 5    -0.09    -0.41     0.47     0.15    -0.14    -0.19
+ 6    -0.04    -0.21    -0.93     0.52    -0.07    -0.10
+ 7    -1.30    -1.42     0.45    -0.21    -0.78    -0.07
+ 8     2.51     1.77     0.86     0.99     1.23    -0.42
+ 9     0.80    -0.23    -0.69    -0.39     0.16    -0.59
+ A    -0.03    -0.73     1.61    -0.08    -0.22    -0.40
+ B    -0.13    -0.57    -0.57     0.30    -0.20    -0.26
+ C     0.00     0.00     0.00     0.00     0.00     0.00
+ D    -0.05    -0.31    -1.23     1.50    -0.10    -0.15
+</PRE>
+<P>
+The first two columns (position) give the dipole angle error, expressed as the
+percentage of I that will corrupt Q, U and V. This is equivalent to expressing
+the dipole misalignment errors as percentages of one radian. In the last two
+columns, these same numbers are re-interpreted as a position error (rotation)
+of the entire XY-dipole assembly in degrees, and a deviation from the nominal
+orthogonality between the X and Y dipole. This is useful, since the entire
+XY-dipole assembly can be rotated as a whole for each WSRT telescope.
+<P>
+The ellipticities are also given as percentages of the corrupting I, or as
+percentages of one radian.
+<P>
+<A NAME=.calc><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0006000000000000000> <b>POLAR CALC: Calculate corrections</b></A></H1>
+<P>
+The dipole angle <em>errors</em> <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1409.png"> and ellipticities <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1599.png"> are
+calculated using <A HREF=" #.equ.pol.010">equation</A>. A strong calibrator is observed, which
+is known to be unpolarised  (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1413.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1383.png">). It is assumed that gain and
+phase have already been calibrated by other means (e.g. Selfcal): <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1417.png">. Thus,
+<A HREF=" #.equ.pol.010">equation</A> reduces to:
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_23919_equation278.png"><P>
+with <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1419.png">.
+<P>
+The system of linear equations (one for each <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1421.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1423.png">) can
+be solved in a manner that is entirely analogous to the
+<A HREF="../ncalib/ncalib.html#.redun">redundancy solution</A> for gain and phase errors. The
+separate solutions for the real and imaginary parts now give the <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1409.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1599.png"> respectively.
+<P>
+Since the S/N of the <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1429.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1431.png"> will be small, the
+least-squares solution will be more accurate if more data (Sets and HA-range)
+are used. However, it must of course be assumed that the <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1409.png"> and
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1599.png"> values are the same for all these data.  This is a fairly safe
+assumption, since the causes for these dipole errors are `mechanical', and vary
+only slowly in time. If the estimated values are to be useful for correction
+subsequent observations, they must at least be constant for the duration of the
+calibrator observation.
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1469.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1471.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1473.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1475.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1477.png">   <PRE>
+ All cross interferometers pre-selected
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1479.png">   <PRE>
+   0123456789ABCD
+ 0 -+++++++++++++
+ 1  -++++++++++++
+ 2   -+++++++++++
+ 3    -++++++++++
+ 4     -+++++++++
+ 5      -++++++++
+ 6       -+++++++
+ 7        -++++++
+ 8         -+++++
+ 9          -++++
+ A           -+++
+ B            -++
+ C             -+
+ D              -
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1481.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>BASEL_CHECK</b>
+ (M) (Baseline deviation allowed)
+ = 0.5 M:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1483.png">
+<P>
+The only difference with a `normal' (gain/phase) Redundancy solution is that
+these solutions are for all 28 dipoles simultaneously. Therefore, the necessary
+constraint equations have 28 coefficients. The words `gain' and `phase' refer
+to the separate Real and Imaginary solutions. The succession of dipoles is
+0X,0Y,1X,1Y,...etc.
+<P>
+The constraint equations arbitrarily set the <em>average ellipticity</em> and the
+<em>average dipole angle errors</em> over the array to zero. Without further
+information, this may be the most reasonable value. But if it is wrong it could
+affect the observations that are calibrated with the results.
+<P>
+The result of CALC looks very much like the output of SHOW (see above), except
+that the estimated accuracy (mean error) of the numbers is give in brackets.
+<P>
+    <PRE>
+ Sector: 2.0.0.0
+
+         Position                     Ellipticity           Rotation Orthog.
+         X(%
+
+ 0    -1.13(0.06)    -0.06(0.06)    -0.37(0.06)     0.54(0.06)    -0.34     0.61
+ 1    -0.16(0.06)     0.13(0.06)     0.07(0.06)     0.04(0.06)    -0.01     0.17
+ 2     1.25(0.06)     0.82(0.06)     1.77(0.06)    -2.56(0.06)     0.59    -0.24
+ 3     0.49(0.06)    -0.02(0.06)     0.11(0.06)     1.19(0.06)     0.13    -0.29
+ 4    -0.72(0.06)    -0.14(0.06)    -0.03(0.06)    -0.46(0.06)    -0.25     0.33
+ 5    -0.09(0.06)    -0.41(0.06)     0.47(0.06)     0.15(0.06)    -0.14    -0.19
+ 6    -0.04(0.06)    -0.21(0.06)    -0.93(0.06)     0.52(0.06)    -0.07    -0.10
+ 7    -1.30(0.06)    -1.42(0.06)     0.45(0.06)    -0.21(0.06)    -0.78    -0.07
+ 8     2.51(0.06)     1.77(0.06)     0.86(0.06)     0.99(0.06)     1.23    -0.42
+ 9     0.80(0.07)    -0.23(0.07)    -0.69(0.07)    -0.39(0.07)     0.16    -0.59
+ A    -0.03(0.04)    -0.73(0.04)     1.61(0.04)    -0.08(0.04)    -0.22    -0.40
+ B    -0.13(0.05)    -0.57(0.05)    -0.57(0.05)     0.30(0.05)    -0.20    -0.26
+ C     0.00(0.72)     0.00(0.72)     0.00(0.72)     0.00(0.72)     0.00     0.00
+ D    -0.05( 0.2)    -0.31( 0.2)    -1.23( 0.2)     1.50( 0.2)    -0.10    -0.15
+</PRE>
+<P>
+The dipole corrections estimated by CALC will be <em>added</em> to the corrections
+that were applied to the data when they were read in.
+<P>
+<A NAME=.set><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0007000000000000000> <b>POLAR SET: Set corrections manually</b></A></H1>
+<P>
+The user may specify values for the dipole angle errors <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1409.png"> and
+ellipticity <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1599.png"> manually. The numbers given by the user are converted to
+internal format, and stored (as POLC) in the headers of the given range of
+Sets. The default values are zero.
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1519.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1521.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1523.png">
+<P>
+		<i>For example</i> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_ROTAN</b>
+ (dipole position)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1525.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_ORTHOG</b>
+ (dipole orthogonality)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1527.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_X_ELLIPS</b>
+ (X ellipticity)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1529.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_Y_ELLIPS</b>
+ (Y ellipticity)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1531.png">   <PRE>
+ Sector: 2.0.0.0.0
+</PRE>
+<P>
+<A NAME=.edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0008000000000000000> <b>POLAR EDIT: Edit corrections</b></A></H1>
+<P>
+This is similar to POLAR SET above, except that the default values are the
+corrections (POLC) that are already stored in the Set headers. Thus, the
+existing POLC corrections in each Set header of the given range can be edited
+separately:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1563.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1565.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1567.png">
+<P>
+		<i>For example</i>    <PRE>
+ Sector: 2.0.0.0.0
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_ROTAN</b>
+ (dipole position)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1569.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_ORTHOG</b>
+ (dipole orthogonality)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1571.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_X_ELLIPS</b>
+ (X ellipticity)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1573.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POL_Y_ELLIPS</b>
+ (Y ellipticity)
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1575.png">
+<P>
+<A NAME=.zero><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0009000000000000000> <b>POLAR ZERO: Zero corrections</b></A></H1>
+<P>
+For the specified range of sets, the POLC corrections in the set header are set
+to zero:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1589.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1591.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1593.png">   <PRE>
+ Sector: 2.0.0.0.0
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1595.png">
+<P>
+<A NAME=.copy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION00010000000000000000> <b>POLAR COPY: Copy corrections from somewhere else</b></A></H1>
+<P>
+The polarisation corrections <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1409.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1599.png">  are calculated with the
+help of a strong, unpolarised calibrator source, using the option POLAR CALC
+(see above). In order to use these corrections to correct a real observation,
+they must be transferred (copied) from the Set header of the calibrator to the
+Set header(s) of the observed object.
+<P>
+There are two possibilities: The calibrator observation (and thus the desired
+corrections) may be stored in a separate SCN-file (node), or they may be stored
+in another `group' in the same SCN-file as the observed object. Below, an
+example is given for both situations:
+<P>
+If the calibrator observation is stored in a separate SCN-file:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1639.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1641.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1643.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1645.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_NODE</b>
+ (input node name)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1647.png">   <PRE>
+ Specify the node name from which the corrections should be calculated.
+ * indicates the same as the output node name.
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_NODE</b>
+ (input node name)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1649.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_SETS</b>
+ (Set(s) of input uv-data Sectors:  g.o.f.c.s)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1651.png">   <PRE>
+ Sector: 0.0.0.0.0
+ Sector: 0.0.0.4.0
+</PRE>
+<P>
+If the calibrator observation is stored in the same SCN-file (e.g. as group 1,
+while the observed object is stored as group 0), the process runs as follows:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1653.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1655.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1657.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1659.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_NODE</b>
+ (input node name)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1661.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_SETS</b>
+ (Set(s) of input uv-data Sectors:  g.o.f.c.s)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1663.png">   <PRE>
+ Sector: 0.0.0.0.0
+ Sector: 0.0.0.4.0
+</PRE>
+<P>
+<A NAME=.vzero><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION00011000000000000000> <b>POLAR VZERO: X-Y Phase Zero Difference, assuming V=0</b></A></H1>
+<P>
+The VZERO option deals with the determination and manipulation of the <em>Phase Zero Difference (PZD)</em> between the X and Y dipoles. It is invoked in the
+following way:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>POLAR_OPTION</b>
+ (CALC, SHOW, SET, COPY, EDIT...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1667.png">
+<P>
+<A NAME=.vzero.calc><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00011100000000000000> <b>POLAR VZERO CALC: Calculate and show</b></A></H2>
+<P>
+An Phase Zero Difference (PZD) between the X-dipoles an the Y-dipoles affects
+the phase of the complex gain factors <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1669.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1671.png"> (but not
+<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1673.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1675.png">). The PZD is determined with the help of a
+strong calibrator source, which must have a relatively large U-component of
+linear polarisation, and an accurately known amount of circular polarisation
+(Stokes V). The latter is important, since a wrong value for V will be
+incorrectly interpreted as a PZD. Since the V is difficult to measure
+accurately, it is safer to use a calibrator that `should not' have any circular
+polarisation: <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1383.png">.
+<P>
+The algorithm uses <A HREF=" #.equ.pol.010">equation</A> and <A HREF=" #.equ.pol.018">equation</A>. It is assumed
+that the `leakage' of the strong I-term is eliminated by means
+<A HREF="#.calc">POLAR CALC</A>: <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1679.png">.  It is also assumed
+that the gain and phase errors have also been well-calibrated: <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1681.png">. Thus, <A HREF=" #.equ.pol.010">equation</A> reduce to:
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_23919_eqnarray483.png"><P>
+<P>
+The calculation of the PZD angle (<IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1683.png">) is now quite straightforward. Because
+of the low S/N of the `cross-terms' <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1685.png">, as many data (Sets, HA-range)
+should be used in the estimation as possible. However, the PZD may change with
+time.
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_OPTION</b>
+ (CALC, APPLY, ASK, MANUAL, SCAN...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1715.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "PSR1937.JAN93":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1717.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1719.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1721.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1723.png">   <PRE>
+ All cross interferometers pre-selected
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1725.png">   <PRE>
+ Sector: 0.0.0.0
+ Sector: 0.0.0.4
+</PRE>
+<P>
+The resulting PZD angle is given as follows:
+<P>
+    <PRE>
+ A complex angle of 0.54+0.12I(0.01+0.01I) or 12.44 degrees
+</PRE>
+<P>
+This message is somewhat confusing as the interesting information in the
+``complex angle'' has been truncated in the printing (the relative sizes of the
+real and imaginary parts). The angle given in degrees is somewhat more
+informative.
+<P>
+<A NAME=.vzero.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00011200000000000000> <b>POLAR VZERO APPLY: Calculate, show and apply</b></A></H2>
+<P>
+The PZD angle is `applied' by adjusting the phase in the `other corrections'
+(OTHC) in the Scan headers. This is done for the entire specified range (Sets
+and HA-range).
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_OPTION</b>
+ (CALC, APPLY, ASK, MANUAL, SCAN...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1751.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1753.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1755.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1757.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1759.png">   <PRE>
+ All cross interferometers pre-selected
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1761.png">   <PRE>
+ Sector: 0.0.0.0
+ Sector: 0.0.0.4
+ A complex angle of 0.55+0.01I(0.01+0.01I) or 1.00 degrees
+</PRE>
+<P>
+<A NAME=.vzero.ask><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00011300000000000000> <b>POLAR VZERO ASK: Calculate, check with user, and apply</b></A></H2>
+<P>
+The user may influence the result by giving another PZD, which will be
+`applied' for the entire specified range (Sets and HA-range). The default is
+the calculated value.
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_OPTION</b>
+ (CALC, APPLY, ASK, MANUAL, SCAN...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1801.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "PSR1937.JAN93":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1803.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1805.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1807.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1809.png">   <PRE>
+   0123456789ABCD
+ 0 -+++++++++++++
+ 1  -++++++++++++
+ 2   -+++++++++++
+ 3    -++++++++++
+ 4     -+++++++++
+ 5      -++++++++
+ 6       -+++++++
+ 7        -++++++
+ 8         -+++++
+ 9          -++++
+ A           -+++
+ B            -++
+ C             -+
+ D              -
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1811.png">   <PRE>
+ Sector: 0.0.0.0
+ Sector: 0.0.0.4
+ A complex angle of 0.55-0.00I(0.01+0.01I) or -0.19 degrees
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_PHASE</b>
+ (X-Y difference)
+ = -0.1857903:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1813.png">
+<P>
+		<i>Use the calculated value</i>
+<P>
+<A NAME=.vzero.manual><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00011400000000000000> <b>POLAR VZERO MANUAL: Ask for and apply</b></A></H2>
+<P>
+The PZD angle given by the user is `applied' to the entire specified range
+(Sets and HA-range). The default value is <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1815.png">.
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_OPTION</b>
+ (CALC, APPLY, ASK, MANUAL, SCAN...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1845.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "PSR1937.JAN93":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1847.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1849.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1851.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1853.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_PHASE</b>
+ (X-Y difference)
+ = 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1855.png">
+<P>
+		<i>User specifies a PZD = -1 degrees</i>
+<P>
+<A NAME=.vzero.scan><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00011500000000000000> <b>POLAR VZERO SCAN: Calculate and apply on a per-scan basis</b></A></H2>
+<P>
+The change of the PZD angle as a function of time can be studied by estimating
+it for each Scan (HA) separately. The S/N of the estimation will necessarily be
+low.
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_OPTION</b>
+ (CALC, APPLY, ASK, MANUAL, SCAN...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1889.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = "PSR1937.JAN93":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1891.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1893.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1895.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1897.png">   <PRE>
+   0123456789ABCD
+ 0 -+++++++++++++
+ 1  -++++++++++++
+ 2   -+++++++++++
+ 3    -++++++++++
+ 4     -+++++++++
+ 5      -++++++++
+ 6       -+++++++
+ 7        -++++++
+ 8         -+++++
+ 9          -++++
+ A           -+++
+ B            -++
+ C             -+
+ D              -
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1899.png">
+<P>
+<A NAME=.vzero.copy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00011600000000000000> <b>POLAR VZERO COPY: Calculate from input and apply to output</b></A></H2>
+<P>
+The PZD angle is calculated with the help of a strong, unpolarised calibrator
+source. In order to use it to correct a real observation, it must be
+transferred (copied) from the Scan header(s) of the calibrator to the Scan
+header(s) of the observed object.
+<P>
+There are two possibilities: The calibrator observation (and thus the desired
+corrections) may be stored in a separate SCN-file (node), or it may be stored
+in another group in the same SCN-file as the observed object. NB: In the latter
+case, it could even be the same observation!  In both cases, the PZD is
+calculated from a range of data (Sets and HA-range) in the INPUT_NODE, and
+`applied' (i.e. stored as `other corrections' (OTHC)) to the Scan Headers in
+the SCAN_NODE. In the following example, the calibrator is stored in the same
+SCN-file as group 1, while the observed object is stored as group 0):
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>VZERO_OPTION</b>
+ (CALC, APPLY, ASK, MANUAL, SCAN...)
+ = QUIT:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1931.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_NODE</b>
+ (input/output 'node' name)
+ = ""
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1933.png">
+<P>
+		<i>SCN-file</i> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_LOOPS</b>
+ (niter, Setincr(g.o.f.c.s) ....)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1935.png">
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SCN_SETS</b>
+ (Set(s) to do:  g.o.f.c.s )
+ = 0:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1937.png">
+<P>
+		<i>Apply the PZD to all sets of job 0</i> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_NODE</b>
+ (input node name)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1939.png">   <PRE>
+ Specify the node name from which the corrections should be calculated.
+ * indicates the same as the output node name.
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_NODE</b>
+ (input node name)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1941.png">
+<P>
+		<i>Use the same SCN file</i> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>USE_SCN_SETS</b>
+ (Set(s) of input uv-data Sectors:  g.o.f.c.s)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1943.png">
+<P>
+		<i>Sets in job 2</i> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>HA_RANGE</b>
+ (DEG) (HA range)
+ = *:
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1945.png">
+<P>
+		<i>Use all scans in these sets</i>    <PRE>
+   0123456789ABCD
+ 0 -+++++++++++++
+ 1  -++++++++++++
+ 2   -+++++++++++
+ 3    -++++++++++
+ 4     -+++++++++
+ 5      -++++++++
+ 6       -+++++++
+ 7        -++++++
+ 8         -+++++
+ 9          -++++
+ A           -+++
+ B            -++
+ C             -+
+ D              -
+</PRE> 
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1857.png"> <b>SELECT_IFRS</b>
+ (Select/de-select ifrs)
+ = "":
+ <IMG ALIGN=BOTTOM ALT="" SRC="_8345_tex2html_wrap1947.png">
+<P>
+		<i>Use all interferometers</i>    <PRE>
+ Sector: 0.0.0.0
+ Sector: 0.0.0.4
+ A complex angle of 0.55-0.00I(0.01+0.01I) or -0.89 degrees
+</PRE>
+<P>
+Warning: Remember that the PZD may partly be an <em>artifact</em> of the separate
+phase/gain calibration of the X-dipoles and the Y-dipoles. This may lead to a
+different PZD angle for the calibrator and the subsequent observation. The
+difference may be several degrees, which is much greater than the accuracy that
+is required for the measurement of very small percentages of circular
+polarisation. However, the measured V may be more accurate if the observed
+object is extended, which will often be the case. But the truth of the matter
+is that, even though the WSRT may offer the best conditions for very accurate
+polarisation measurements, the PZD problem is essentially unsolved.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ncalib_private_intfc.ps b/ncalib_private_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..0f60984800492a8eee130cab0f91a8900aaa7a2b
--- /dev/null
+++ b/ncalib_private_intfc.ps
@@ -0,0 +1,1601 @@
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+b(Zero)19 b(only)f(phases)157 2667 y(NOPHASE)36 b(Zero)19
+b(only)f(gain)924 2995 y Fh(16)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/ncalib_private_intfc/images.pl b/ncalib_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ncalib_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ncalib_private_intfc/labels.pl b/ncalib_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..19b23f8e39342540c1ef9fea1493058d221c1393
--- /dev/null
+++ b/ncalib_private_intfc/labels.pl
@@ -0,0 +1,71 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
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diff --git a/ncalib_private_intfc/ncalib_private_intfc.html b/ncalib_private_intfc/ncalib_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..974f3dee9233cc6f4ee8c471c3688b040ea60831
--- /dev/null
+++ b/ncalib_private_intfc/ncalib_private_intfc.html
@@ -0,0 +1,1362 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NCALIB</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncalib_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncalib_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ncalib_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ncalib_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=ncalib_private_intfc.html#SECTION0003200000000000000>  <b>Parameter ALIGN_OPTION</b></A>
+<LI> <A NAME=tex2html6 HREF=ncalib_private_intfc.html#SECTION0003300000000000000>  <b>Parameter BASEL_CHECK</b></A>
+<LI> <A NAME=tex2html7 HREF=ncalib_private_intfc.html#SECTION0003400000000000000>  <b>Parameter BASEL_DX</b></A>
+<LI> <A NAME=tex2html8 HREF=ncalib_private_intfc.html#SECTION0003500000000000000>  <b>Parameter BASEL_DY</b></A>
+<LI> <A NAME=tex2html9 HREF=ncalib_private_intfc.html#SECTION0003600000000000000>  <b>Parameter BASEL_DZ</b></A>
+<LI> <A NAME=tex2html10 HREF=ncalib_private_intfc.html#SECTION0003700000000000000>  <b>Parameter BASEL_POLE</b></A>
+<LI> <A NAME=tex2html11 HREF=ncalib_private_intfc.html#SECTION0003800000000000000>  <b>Parameter CAL_EQUAL</b></A>
+<LI> <A NAME=tex2html12 HREF=ncalib_private_intfc.html#SECTION0003900000000000000>  <b>Parameter CHECKS</b></A>
+<LI> <A NAME=tex2html13 HREF=ncalib_private_intfc.html#SECTION00031000000000000000>  <b>Parameter CLOCK_CORR</b></A>
+<LI> <A NAME=tex2html14 HREF=ncalib_private_intfc.html#SECTION00031100000000000000>  <b>Parameter COMPLEX</b></A>
+<LI> <A NAME=tex2html15 HREF=ncalib_private_intfc.html#SECTION00031200000000000000>  <b>Parameter COMPLEX_ONLY</b></A>
+<LI> <A NAME=tex2html16 HREF=ncalib_private_intfc.html#SECTION00031300000000000000>  <b>Parameter CONTINUITY</b></A>
+<LI> <A NAME=tex2html17 HREF=ncalib_private_intfc.html#SECTION00031400000000000000>  <b>Parameter DSHIFT</b></A>
+<LI> <A NAME=tex2html18 HREF=ncalib_private_intfc.html#SECTION00031500000000000000>  <b>Parameter EXTINCTION</b></A>
+<LI> <A NAME=tex2html19 HREF=ncalib_private_intfc.html#SECTION00031600000000000000>  <b>Parameter FARADAY_FILE</b></A>
+<LI> <A NAME=tex2html20 HREF=ncalib_private_intfc.html#SECTION00031700000000000000>  <b>Parameter FLW_FACTOR</b></A>
+<LI> <A NAME=tex2html21 HREF=ncalib_private_intfc.html#SECTION00031800000000000000>  <b>Parameter FORCE_FREEDOM</b></A>
+<LI> <A NAME=tex2html22 HREF=ncalib_private_intfc.html#SECTION00031900000000000000>  <b>Parameter FORCE_PHASE</b></A>
+<LI> <A NAME=tex2html23 HREF=ncalib_private_intfc.html#SECTION00032000000000000000>  <b>Parameter FREQ_CORR</b></A>
+<LI> <A NAME=tex2html24 HREF=ncalib_private_intfc.html#SECTION00032100000000000000>  <b>Parameter GAIN_FREEDOM</b></A>
+<LI> <A NAME=tex2html25 HREF=ncalib_private_intfc.html#SECTION00032200000000000000>  <b>Parameter GAIN_NORM</b></A>
+<LI> <A NAME=tex2html26 HREF=ncalib_private_intfc.html#SECTION00032300000000000000>  <b>Parameter GAIN_X</b></A>
+<LI> <A NAME=tex2html27 HREF=ncalib_private_intfc.html#SECTION00032400000000000000>  <b>Parameter GAIN_XX</b></A>
+<LI> <A NAME=tex2html28 HREF=ncalib_private_intfc.html#SECTION00032500000000000000>  <b>Parameter GAIN_XY</b></A>
+<LI> <A NAME=tex2html29 HREF=ncalib_private_intfc.html#SECTION00032600000000000000>  <b>Parameter GAIN_Y</b></A>
+<LI> <A NAME=tex2html30 HREF=ncalib_private_intfc.html#SECTION00032700000000000000>  <b>Parameter GAIN_YX</b></A>
+<LI> <A NAME=tex2html31 HREF=ncalib_private_intfc.html#SECTION00032800000000000000>  <b>Parameter GAIN_YY</b></A>
+<LI> <A NAME=tex2html32 HREF=ncalib_private_intfc.html#SECTION00032900000000000000>  <b>Parameter HA_INTEGRATION</b></A>
+<LI> <A NAME=tex2html33 HREF=ncalib_private_intfc.html#SECTION00033000000000000000>  <b>Parameter IFR_XX</b></A>
+<LI> <A NAME=tex2html34 HREF=ncalib_private_intfc.html#SECTION00033100000000000000>  <b>Parameter IFR_XY</b></A>
+<LI> <A NAME=tex2html35 HREF=ncalib_private_intfc.html#SECTION00033200000000000000>  <b>Parameter IFR_YX</b></A>
+<LI> <A NAME=tex2html36 HREF=ncalib_private_intfc.html#SECTION00033300000000000000>  <b>Parameter IFR_YY</b></A>
+<LI> <A NAME=tex2html37 HREF=ncalib_private_intfc.html#SECTION00033400000000000000>  <b>Parameter IREFRACT_FILE</b></A>
+<LI> <A NAME=tex2html38 HREF=ncalib_private_intfc.html#SECTION00033500000000000000>  <b>Parameter MWEIGHT_DATA</b></A>
+<LI> <A NAME=tex2html39 HREF=ncalib_private_intfc.html#SECTION00033600000000000000>  <b>Parameter MWEIGHT_TYPE</b></A>
+<LI> <A NAME=tex2html40 HREF=ncalib_private_intfc.html#SECTION00033700000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html41 HREF=ncalib_private_intfc.html#SECTION00033800000000000000>  <b>Parameter OTH_OPTION</b></A>
+<LI> <A NAME=tex2html42 HREF=ncalib_private_intfc.html#SECTION00033900000000000000>  <b>Parameter PHASE_FREEDOM</b></A>
+<LI> <A NAME=tex2html43 HREF=ncalib_private_intfc.html#SECTION00034000000000000000>  <b>Parameter PHASE_NORM</b></A>
+<LI> <A NAME=tex2html44 HREF=ncalib_private_intfc.html#SECTION00034100000000000000>  <b>Parameter PHASE_X</b></A>
+<LI> <A NAME=tex2html45 HREF=ncalib_private_intfc.html#SECTION00034200000000000000>  <b>Parameter PHASE_XX</b></A>
+<LI> <A NAME=tex2html46 HREF=ncalib_private_intfc.html#SECTION00034300000000000000>  <b>Parameter PHASE_XY</b></A>
+<LI> <A NAME=tex2html47 HREF=ncalib_private_intfc.html#SECTION00034400000000000000>  <b>Parameter PHASE_Y</b></A>
+<LI> <A NAME=tex2html48 HREF=ncalib_private_intfc.html#SECTION00034500000000000000>  <b>Parameter PHASE_YX</b></A>
+<LI> <A NAME=tex2html49 HREF=ncalib_private_intfc.html#SECTION00034600000000000000>  <b>Parameter PHASE_YY</b></A>
+<LI> <A NAME=tex2html50 HREF=ncalib_private_intfc.html#SECTION00034700000000000000>  <b>Parameter POLAR_OPTION</b></A>
+<LI> <A NAME=tex2html51 HREF=ncalib_private_intfc.html#SECTION00034800000000000000>  <b>Parameter POL_ORTHOG</b></A>
+<LI> <A NAME=tex2html52 HREF=ncalib_private_intfc.html#SECTION00034900000000000000>  <b>Parameter POL_ROTAN</b></A>
+<LI> <A NAME=tex2html53 HREF=ncalib_private_intfc.html#SECTION00035000000000000000>  <b>Parameter POL_X_ELLIPS</b></A>
+<LI> <A NAME=tex2html54 HREF=ncalib_private_intfc.html#SECTION00035100000000000000>  <b>Parameter POL_Y_ELLIPS</b></A>
+<LI> <A NAME=tex2html55 HREF=ncalib_private_intfc.html#SECTION00035200000000000000>  <b>Parameter QDETAILS</b></A>
+<LI> <A NAME=tex2html56 HREF=ncalib_private_intfc.html#SECTION00035300000000000000>  <b>Parameter REFRACTION</b></A>
+<LI> <A NAME=tex2html57 HREF=ncalib_private_intfc.html#SECTION00035400000000000000>  <b>Parameter SAVE_RESIDUALS</b></A>
+<LI> <A NAME=tex2html58 HREF=ncalib_private_intfc.html#SECTION00035500000000000000>  <b>Parameter SET_OPTION</b></A>
+<LI> <A NAME=tex2html59 HREF=ncalib_private_intfc.html#SECTION00035600000000000000>  <b>Parameter SHIFT</b></A>
+<LI> <A NAME=tex2html60 HREF=ncalib_private_intfc.html#SECTION00035700000000000000>  <b>Parameter SHOW_LEVEL</b></A>
+<LI> <A NAME=tex2html61 HREF=ncalib_private_intfc.html#SECTION00035800000000000000>  <b>Parameter SOLVE</b></A>
+<LI> <A NAME=tex2html62 HREF=ncalib_private_intfc.html#SECTION00035900000000000000>  <b>Parameter USE_SCN_NODE</b></A>
+<LI> <A NAME=tex2html63 HREF=ncalib_private_intfc.html#SECTION00036000000000000000>  <b>Parameter USE_SCN_SETS</b></A>
+<LI> <A NAME=tex2html64 HREF=ncalib_private_intfc.html#SECTION00036100000000000000>  <b>Parameter VZERO_OPTION</b></A>
+<LI> <A NAME=tex2html65 HREF=ncalib_private_intfc.html#SECTION00036200000000000000>  <b>Parameter VZERO_PHASE</b></A>
+<LI> <A NAME=tex2html66 HREF=ncalib_private_intfc.html#SECTION00036300000000000000>  <b>Parameter WEIGHT_MIN</b></A>
+<LI> <A NAME=tex2html67 HREF=ncalib_private_intfc.html#SECTION00036400000000000000>  <b>Parameter ZERO</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NCALIB. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show parameters that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+</UL>
+<P>
+<A NAME=.align.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter ALIGN_OPTION</b></A></H2>
+<P>
+  <em>Prompt:</em> Type of Selfcal desired<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+    <PRE>
+Selfcal is the generic name for all methods that use a source model in
+combination with your visibilities to estimate the telecope gain/phase
+corrections. Since you have selected a model, NCALIB assumes that you want to
+use it, by doing a Selfcal. (If you had not, it would propose a REDUNdancy-only
+solution.)
+</PRE>
+<P>
+  <PRE>
+The alternative you have here is to use the source model to recover the unknown
+position shift that scans suffer when they are processed with the  redundancy
+constraints only (REDUN solution). In this operation the source model is only
+used as a position reference. The telescope phases are shifted by an amount
+that is a linear function of position along the array; the telescope gains do
+not change at all.
+</PRE>
+<P>
+  <PRE>
+To summarise, the choices you have are:
+</PRE>
+<P>
+  <PRE>
+   SELFCAL       use the model to constrain in position a redundancy solution
+                  that will be made now
+   ALIGN         use the model to constrain a redundancy solution that was made
+                  earlier
+</PRE>
+<P>
+<A NAME=.basel.check><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter BASEL_CHECK</b></A></H2>
+<P>
+<em>Prompt:</em> Redundant-baseline difference allowed (metres)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the maximum difference between baselines for them still to be
+considered identical in Redundancy calculations.
+</PRE>
+<P>
+<A NAME=.basel.dx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter BASEL_DX</b></A></H2>
+<P>
+<em>Prompt:</em> Increments to telescope X positions (mm) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the X telescope corrections in mm, one value per telescope.
+</PRE>
+<P>
+  <PRE>
+The correction will be added as an HA-dependent phase to the OTH telescope
+corrections. It can only be undone by either zeroing the entire OTH corrections
+by means of the SET ZERO option (which will destroy whatever other corrections
+have been stored there), or by inserting the same BASEL_DX value with opposite
+sign.
+</PRE>
+<P>
+  <PRE>
+The default value 0,0,...0,0 leaves the corrections unchanged.
+</PRE>
+<P>
+<A NAME=.basel.dy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter BASEL_DY</b></A></H2>
+<P>
+<em>Prompt:</em> Increments to telescope Y positions (mm) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify 14 Y telescope corrections in mm, one value per telescope.
+</PRE>
+<P>
+  <PRE>
+The correction will be added as an HA-dependent phase to the OTH telescope
+corrections. It can only be undone by either zeroing the entire OTH corrections
+by means of the SET ZERO option (which will destroy whatever other corrections
+have been stored there), or by inserting the same BASEL_DY value with opposite
+sign.
+</PRE>
+<P>
+  <PRE>
+The default value 0,0,...0,0 leaves the corrections unchanged.
+</PRE>
+<P>
+<A NAME=.basel.dz><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter BASEL_DZ</b></A></H2>
+<P>
+<em>Prompt:</em> increments to telescope Z positions (mm) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the Z telescope corrections in mm, one value per telescope.
+</PRE>
+<P>
+  <PRE>
+The correction will be added as an HA-dependent phase to the OTH telescope
+corrections. It can only be undone by either zeroing the entire OTH corrections
+by means of the SET ZERO option (which will destroy whatever other corrections
+have been stored there), or by inserting the same BASEL_DZ value with opposite
+sign.
+</PRE>
+<P>
+  <PRE>
+The default value 0,0,...0,0 leaves the corrections unchanged.
+</PRE>
+<P>
+<A NAME=.basel.pole><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter BASEL_POLE</b></A></H2>
+<P>
+<em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the baseline-pole declination correction in degrees.
+</PRE>
+<P>
+  <PRE>
+The correction will be added as an HA-dependent phase to the OTH telescope
+corrections. It can only be undone by either zeroing the entire OTH corrections
+by means of the SET ZERO option (which will destroy whatever other corrections
+have been stored there), or by inserting the same BASEL_POLE value with
+opposite sign..
+</PRE>
+<P>
+  <PRE>
+The default value 0 leaves the corrections unchanged.
+</PRE>
+<P>
+<A NAME=.cal.equal><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter CAL_EQUAL</b></A></H2>
+<P>
+<em>Prompt:</em> Copy with equal length?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+If YES, all calibrators specified with USE_SCN_SETS will be made of equal
+length, that is: the number of HA scans used for each calibrator will be the
+same (and equal to the smallest number available).
+</PRE>
+<P>
+  <PRE>
+This is necessary when calibrators have frequencies that have been offset (plus
+and minus respectively) to the observing frequency of the target source.
+</PRE>
+<P>
+<A NAME=.checks><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter CHECKS</b></A></H2>
+<P>
+<em>Prompt:</em> Iterations, gain deviation, relative mean error: 3 values|<BR><em>Expected input:</em> Real:  1 to 3 values
+<P>
+  <PRE>
+Specify:
+</PRE>
+<P>
+  <PRE>
+   - the maximum number of iterations in the complex solution;
+</PRE>
+<P>
+  <PRE>
+   - the relative allowable gain deviation for successive complex solutions;
+</PRE>
+<P>
+  <PRE>
+   - the mean error allowed per scan, relative to the average mean error
+        for all scans already solved.
+</PRE>
+<P>
+<A NAME=.clock.corr><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter CLOCK_CORR</b></A></H2>
+<P>
+<em>Prompt:</em> Clock correction (sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the clock correction in seconds to be applied to data. The new value
+will be ADDED to the existing one.
+</PRE>
+<P>
+<A NAME=.complex><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter COMPLEX</b></A></H2>
+<P>
+<em>Prompt:</em> Complex solution (YES/NO)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want a complex solution of gains-plus-phases.
+</PRE>
+<P>
+<A NAME=.complex.only><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter COMPLEX_ONLY</b></A></H2>
+<P>
+<em>Prompt:</em> Complex solution only (YES/NO)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want ONLY a complex solution.
+</PRE>
+<P>
+  <PRE>
+Note: will only work if an initial guess for the gains (e.g. from a calibrator)
+has been specified
+</PRE>
+<P>
+<A NAME=.continuity><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter CONTINUITY</b></A></H2>
+<P>
+<em>Prompt:</em> Continuity in solution (YES/NO)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want continuity in gain solution. If not, the initial guess for
+the solution will be 0 (gain) and the forced phases (phase), else the solution
+found in a previous scan.
+</PRE>
+<P>
+<A NAME=.dshift><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter DSHIFT</b></A></H2>
+<P>
+<em>Prompt:</em> Shift rate (dl/dt, dm/dt, arcsec/day)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the SHIFT rate in arcsec per sidereal day to be applied to the data
+whenever the DE_APPLY SHIFT correction is requested.
+</PRE>
+<P>
+  <PRE>
+This parameter is used for a first-order approximation to the proper motion of
+a solar-system object through the formula:
+</PRE>
+<P>
+  <PRE>
+        Total shift =  SHIFT + DSHIFT * (HA-HAB)
+</PRE>
+<P>
+  <PRE>
+where hour angles are measured as fractions of a full circle and HAB is the
+starting HA of the sector.
+</PRE> 
+               .
+<P>
+<A NAME=.extinction><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter EXTINCTION</b></A></H2>
+<P>
+<em>Prompt:</em> Extinction-1: quadratic's coefficients|<BR><em>Expected input:</em> Real:  1 to 3 values
+<P>
+  <PRE>
+Specify the coefficients A, B and C in the quadratic representation of the
+zenith extinction oefficient as a function of frequency F in GHz:
+</PRE>
+<P>
+  <PRE>
+        EXT= (1+A) + B*F +C*F*F
+</PRE>
+<P>
+<A NAME=.faraday.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter FARADAY_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> Faraday-rotation data file<BR><em>Expected input:</em> Character:  1 value
+<P>
+  <PRE>
+Specify the name of a file with Faraday rotation data. The file must be an
+ASCII file with lines
+</PRE>
+<P>
+  <PRE>
+        <hour angle in degrees>, <faraday rotation in degrees at 1GHz>
+</PRE>
+<P>
+  <PRE>
+The file will be used to calculate Faraday rotation values for each scan by
+interpolation between the values in this file and scaling to the observing
+frequency. The calculated values will be stored in the scans as corrections.
+</PRE>
+<P>
+<A NAME=.flw.factor><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter FLW_FACTOR</b></A></H2>
+<P>
+<em>Prompt:</em> Weight for points flagged with WGT flag<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+The WGT flag directs NCALIB to multiply the data weight with an additional
+weighing factor.
+</PRE>
+<P>
+  <PRE>
+You may use this feature to reduce the weight of data affected by interference
+without rejecting it completely. The effect of this in a Selfcal solution is
+that it prevents the interference from bad interferometers to infect the
+healthy ones.
+</PRE>
+<P>
+  <PRE>
+A value of 1 will give all interferometers the weight they have in the .SCN
+file.
+</PRE>
+<P>
+<A NAME=.force.freedom><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter FORCE_FREEDOM</b></A></H2>
+<P>
+<em>Prompt:</em>   Manual constraints for gain (1st value)|-<BR><em>Expected input:</em> Yes/No:  1 to 2 values
+<P>
+  <PRE>
+Specify if you want to force the constraint equations for the align solution.
+If you reply NO, the program will determine them by itself from the
+interferometers selected.
+</PRE>
+<P>
+  <PRE>
+Your first reply refers to Gain, the second one to Phase.
+</PRE>
+<P>
+<A NAME=.force.phase><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031900000000000000>  <b>Parameter FORCE_PHASE</b></A></H2>
+<P>
+<em>Prompt:</em> Define phase-zeroes<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Define initial phase zeros per telescope.
+</PRE>
+<P>
+  <PRE>
+This is useful for pathological cases where NCALIB on its own cannot correctly
+resolve the 360-deg phase ambiguities.
+</PRE>
+<P>
+<A NAME=.freq.corr><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032000000000000000>  <b>Parameter FREQ_CORR</b></A></H2>
+<P>
+<em>Prompt:</em> Increment to frequency correction (MHz)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the 'frequency correction' in MHz.
+</PRE>
+<P>
+  <PRE>
+This is an idiosyncratic way of representing a correction to the metric scale
+of the interferometer array: A scale correction with a factor (1+x) is
+represented by correcting the nominal observing frequency F with an additive
+term -x.F.
+</PRE>
+<P>
+  <PRE>
+Clearly this does not represent a real frequency shift since the observing
+frequency is precisely defined by the settings of local-oscillator frequencies
+and fringe-stopping parameters during the observation.
+</PRE>
+<P>
+  <PRE>
+The correction will be ADDED as an hour-angle-dependent phase to the OTH
+telescope corrections, and can only be undone by either zeroing these
+corrections, or inserting the same BASEL_POLE value with opposite sign.
+</PRE>
+<P>
+<A NAME=.gain.freedom><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032100000000000000>  <b>Parameter GAIN_FREEDOM</b></A></H2>
+<P>
+<em>Prompt:</em> Gain grouping<BR><em>Expected input:</em> Integer:  1 to 14 values
+<P>
+  <PRE>
+Define the telescope groups for which the gains will be solved independently.
+</PRE>
+<P>
+  <PRE>
+To solve e.g. separate gains for the 10 fixed telescopes (0 through 9) and the
+ 4 movable ones (A through D), specify:
+</PRE>
+<P>
+  <PRE>
+        1,1,1,1,1,1,1,1,1,1, 2,2,2,2
+</PRE>
+<P>
+  <PRE>
+* means one group containing all telescopes (i.e. 1,1,...,1,1).
+</PRE>
+<P>
+<A NAME=.gain.norm><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032200000000000000>  <b>Parameter GAIN_NORM</b></A></H2>
+<P>
+<em>Prompt:</em> Gain reference telescopes<BR><em>Expected input:</em> Integer:  1 to 14 values
+<P>
+  <PRE>
+Define the telescopes to be used as reference for renormalising the telescope
+gains.
+</PRE>
+<P>
+  <PRE>
+Your reply should be an array of values (separated by commas) for telescopes 0
+through D; 1 means that you select the telescope, 0 that you don't. Trailing 0s
+may be omitted.
+</PRE>
+<P>
+  <PRE>
+A wildcard ('*') means 'all', i.e. 1,1,1,1,1,1,1,1,1,1,1,1,1,1
+</PRE>
+<P>
+  <PRE>
+Example:
+        0,1,0,1,0 means 'use telescopes 1 and 3 as reference'
+</PRE>
+<P>
+  <PRE>
+NOTES:
+</PRE>
+<P>
+  <PRE>
+Renormalisation adjusts the gains so that the average for the fixed telescopes
+selected equals that for the moving telescopes. If either group is absent from
+yous selection, the average gain of the other group is made 0.
+</PRE>
+<P>
+  <PRE>
+Consequently, proper gain renormalisation is possible only for the 'standard'
+WSRT configuration: If there are any fixed-fixed or movable-movable
+interferometers, a message will be given and the operation aborted.
+</PRE>
+<P>
+  <PRE>
+You may, however, insist by putting a -1 instead of any of the 1s in your
+reply. The renormalisation will then be performed as if the fixed-movable
+interferometers were absent, and a warning given that the gain corrections for
+those interferometers are jeopardized.
+</PRE>
+<P>
+<A NAME=.gain.x><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032300000000000000>  <b>Parameter GAIN_X</b></A></H2>
+<P>
+<em>Prompt:</em> Gain corrections X (factors) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the X gain corrections per telescope as factors (1= no change).
+</PRE>
+<P>
+  <PRE>
+The values you give will be multiplied with the existing gain factors if you
+choose SET option MULT, they will replace the existing factors if you choose
+SET option MANUAL.
+</PRE>
+<P>
+<A NAME=.gain.xx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032400000000000000>  <b>Parameter GAIN_XX</b></A></H2>
+<P>
+<em>Prompt:</em> Interferometer gain corrections XX (factors) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the gain corrections for XX as factors (1= no change). You will be
+prompted for values, which will OVERWRITE the existing interferometer gain
+corrections.
+</PRE>
+<P>
+<A NAME=.gain.xy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032500000000000000>  <b>Parameter GAIN_XY</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer gain corrections XY (factors) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the gain corrections for XY as factors (1= no change). You will be
+prompted for values, which will OVERWRITE the existing interferometer gain
+corrections.
+</PRE>
+<P>
+<A NAME=.gain.y><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032600000000000000>  <b>Parameter GAIN_Y</b></A></H2>
+<P>
+<em>Prompt:</em> Gain corrections Y (factors) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the Y gain corrections per telescope as factors (1= no change).
+</PRE>
+<P>
+  <PRE>
+The values you give will be multiplied with the existing gain factors if you
+choose SET option MULT, they will replace the existing factors if you choose
+SET option MANUAL.
+</PRE>
+<P>
+<A NAME=.gain.yx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032700000000000000>  <b>Parameter GAIN_YX</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer gain corrections YX (factors) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the gain corrections for YX as factors (1= no change). You will be
+prompted for values, which will OVERWRITE the existing interferometer
+corrections.
+</PRE>
+<P>
+<A NAME=.gain.yy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032800000000000000>  <b>Parameter GAIN_YY</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer gain corrections YY (factors) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the gain corrections for YY as factors (1= no change). You will be
+prompted for values, which will OVERWRITE the existing interferometer
+corrections.
+</PRE>
+<P>
+<A NAME=.ha.integration><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032900000000000000>  <b>Parameter HA_INTEGRATION</b></A></H2>
+<P>
+<em>Prompt:</em> Integration time (sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the time interval over which you want to integrate (if possible) before
+calibrating. The value you specify will be rounded down to a multiple of the
+hour-angle interval between successive scans.
+</PRE>
+<P>
+  <PRE>
+'*' and '0' mean do not integrate, i.e. calibrate per scan.
+</PRE>
+<P>
+  <PRE>
+The largest value allowed is 3600 (= 1 hour).
+</PRE>
+<P>
+<A NAME=.ifr.xx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033000000000000000>  <b>Parameter IFR_XX</b></A></H2>
+<P>
+<em>Prompt:</em> additive interferometer corrections cos,sin XX (W.U.) |<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the additive interferometer corrections for XX in Westerbork Units
+(W.U.). The values you specify will OVERWRITE any existing values.
+</PRE>
+<P>
+<A NAME=.ifr.xy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033100000000000000>  <b>Parameter IFR_XY</b></A></H2>
+<P>
+<em>Prompt:</em> additive interferometer corrections cos,sin XY (W.U.) |<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the additive interferometer corrections for XY in Westerbork Units
+(W.U.). The values you specify will OVERWRITE any existing values.
+</PRE>
+<P>
+<A NAME=.ifr.yx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033200000000000000>  <b>Parameter IFR_YX</b></A></H2>
+<P>
+<em>Prompt:</em> additive interferometer corrections cos,sin YX (W.U.) |<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the additive interferometer corrections for YX in Westerbork Units
+(W.U.). The values you specify will OVERWRITE any existing values.
+</PRE>
+<P>
+<A NAME=.ifr.yy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033300000000000000>  <b>Parameter IFR_YY</b></A></H2>
+<P>
+<em>Prompt:</em> additive interferometer corrections cos,sin YY (W.U.) |<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the additive interferometer corrections for YY in  Westerbork Units
+(W.U.). The values you specify will OVERWRITE any existing values.
+</PRE>
+<P>
+<A NAME=.irefract.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033400000000000000>  <b>Parameter IREFRACT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> Ionospheric refraction data file<BR><em>Expected input:</em> Character:  1 value
+<P>
+  <PRE>
+Specify the name of a file with ionospheric refraction data. The file must be
+an ASCII file with lines
+</PRE>
+<P>
+  <PRE>
+        <hour angle in degrees>, <refraction in degrees/km at 1GHz>
+</PRE>
+<P>
+  <PRE>
+The file will be used to calculate ionospheric refraction for each scan by
+interpolation between the values in this file and scaling to the observing
+frequency. The calculated values will be stored in the scans as corrections.
+</PRE>
+<P>
+<A NAME=.mweight.data><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033500000000000000>  <b>Parameter MWEIGHT_DATA</b></A></H2>
+<P>
+<em>Prompt:</em> Centre, halfwidth (metres)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the centre and the halfpower-halfwidth in metres of the model weight
+function to be applied.
+</PRE>
+<P>
+  <PRE>
+Only positive values are accepted. Note that the function you define may extend
+over negative baselines but actual baselines are positive by definition.
+</PRE>
+<P>
+<A NAME=.mweight.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033600000000000000>  <b>Parameter MWEIGHT_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Type of weight function|<BR><em>Expected input:</em> Character *10:  1 value
+<P>
+  <PRE>
+MWEIGHT_TYPE and MWEIGHT_DATA allow you to weigh baselines according to their
+lengths, in order to take advantage of source characteristics that are a priori
+known. The defaults for these parameters give all baselines the same weight.
+</PRE>
+<P>
+  <PRE>
+This parameter selects the form of the weighting function; its position and
+half-width will be defined by MWEIGHT_DATA. The following shapes can be chosen:
+</PRE>
+<P>
+  <PRE>
+   STEP          a step function: 1 out to some radius, 0 beyond
+   GAUSSIAN      a Gaussian
+   TRIANGLE      a triangular function: linearly decreasing from 1 to 0
+</PRE>
+<P>
+  <PRE>
+   Each of these can be prefixed with an 'I' to invert it, i.e. ISTEP means
+    '1 minus STEP'
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033700000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Type of action<BR><em>Expected input:</em> Character *12:  1 value
+<P>
+  <PRE>
+Specify type of action to perform:
+</PRE>
+<P>
+  <PRE>
+   REDUNDANCY    create telescope corrections by solving the
+                  redundancy/align/selfcal equations
+   POLAR         operations on polarisation corrections
+   SET           operations on all other corrections
+</PRE>
+<P>
+  <PRE>
+   SHOW          show (in logfile) average corrections in specified sector(s)
+   QUIT          finish
+</PRE>
+<P>
+<A NAME=.oth.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033800000000000000>  <b>Parameter OTH_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> SET action (others)|<BR><em>Expected input:</em> Character *6:  1 value
+<P>
+  <PRE>
+Specify action to perform to ADD corrections into the OTHer telescope
+corrections:
+        MULT    set an extra gain factor (multiply existing values)
+        DX      add telescope X correction in selected scans
+        DY      add telescope Y correction in selected scans
+        DZ      add telescope Z correction in selected scans
+        POLE    add baseline pole correction in selected scans
+        FREQ    add frequency offset correction in selected scans
+</PRE>
+<P>
+  <PRE>
+        QUIT    exit SET
+</PRE>
+<P>
+<A NAME=.phase.freedom><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033900000000000000>  <b>Parameter PHASE_FREEDOM</b></A></H2>
+<P>
+<em>Prompt:</em> Phase grouping<BR><em>Expected input:</em> Integer:  1 to 14 values
+<P>
+  <PRE>
+Define the telescope groups for which the phases will be solved independently.
+</PRE>
+<P>
+  <PRE>
+To solve e.g. separate gains for the 10 fixed telescopes (0 through 9) and the
+ 4 movable ones (A through D), specify:
+</PRE>
+<P>
+  <PRE>
+        1,1,1,1,1,1,1,1,1,1, 2,2,2,2
+</PRE>
+<P>
+  <PRE>
+* means one group containing all telescopes (i.e. 1,1,...,1,1). Up to 14 groups
+may be defined.
+</PRE>
+<P>
+<A NAME=.phase.norm><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034000000000000000>  <b>Parameter PHASE_NORM</b></A></H2>
+<P>
+<em>Prompt:</em> Phase reference telescopes<BR><em>Expected input:</em> Integer:  1 to 14 values
+<P>
+  <PRE>
+Define the telescopes to use as reference for renormalising the telescope
+phases.
+</PRE>
+<P>
+  <PRE>
+Your reply should be an array of values (separated by commas) for telescopes 0
+through D; 1 means that you select the telescope, 0 that you don't. Trailing 0s
+may be omitted.
+</PRE>
+<P>
+  <PRE>
+A wildcard ('*') means 'all', i.e. 1,1,1,1,1,1,1,1,1,1,1,1,1,1
+</PRE>
+<P>
+  <PRE>
+Example:
+        0,1,0,1,0 means 'use telescopes 1 and 3 as reference
+</PRE>
+<P>
+<A NAME=.phase.x><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034100000000000000>  <b>Parameter PHASE_X</b></A></H2>
+<P>
+<em>Prompt:</em> Phase corrections X (deg) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the X phase corrections to be added per telescope (0 = no change).
+</PRE>
+<P>
+  <PRE>
+The values you give will be added to the existing OTHer phases if you choose
+SET option MULT, they will replace the existing phases if you choose SET option
+MANUAL.
+</PRE>
+<P>
+<A NAME=.phase.xx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034200000000000000>  <b>Parameter PHASE_XX</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer phase corrections XX (deg) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the phase corrections for XX. You will be prompted for values, which
+will OVERWRITE the existing interferometer corrections.
+</PRE>
+<P>
+<A NAME=.phase.xy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034300000000000000>  <b>Parameter PHASE_XY</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer phase corrections XY (deg) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the phase corrections for XY. You will be prompted for values, which
+will OVERWRITE the existing interferometer corrections.
+</PRE>
+<P>
+<A NAME=.phase.y><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034400000000000000>  <b>Parameter PHASE_Y</b></A></H2>
+<P>
+<em>Prompt:</em> Phase corrections Y (deg) |<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the Y phase corrections to be added per telescope (0 = no change).
+</PRE>
+<P>
+  <PRE>
+The values you give will be added to the existing OTHer phases if you choose
+SET option MULT, they will replace the existing phases if you choose SET option
+MANUAL.
+</PRE>
+<P>
+<A NAME=.phase.yx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034500000000000000>  <b>Parameter PHASE_YX</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer phase corrections YX (deg) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the phase corrections for YX. You will be prompted for values, which
+will OVERWRITE the existing interferometer corrections.
+</PRE>
+<P>
+<A NAME=.phase.yy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034600000000000000>  <b>Parameter PHASE_YY</b></A></H2>
+<P>
+<em>Prompt:</em> interferometer phase corrections YY (deg) |<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the phase corrections for YY. You will be prompted for values, which
+will OVERWRITE the existing interferometer corrections.
+</PRE>
+<P>
+<A NAME=.polar.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034700000000000000>  <b>Parameter POLAR_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> action on polarisation corrections|<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify action to perform on polarisation corrections:
+</PRE>
+<P>
+  <PRE>
+   Calculate corrections from calibrator visibilities. The new correction values
+   are ADDED to existing ones:
+</PRE>
+<P>
+  <PRE>
+        CALC     calculate dipole corrections
+</PRE>
+<P>
+  <PRE>
+        VZERO    select the set of operations dealing with the phase-zero
+                 difference ('PZD') between the X and Y channel groups
+</PRE>
+<P>
+  <PRE>
+   Copy/set corrections. The new corrections values generally OVERWRITE the
+   existing ones:
+</PRE>
+<P>
+  <PRE>
+        COPY     create dipole corrections in target sectors by copying them
+                  from one source sector
+</PRE>
+<P>
+  <PRE>
+        SET      set dipole corrections manually
+</PRE>
+<P>
+  <PRE>
+        ZERO     zero dipole corrections
+</PRE>
+<P>
+  <PRE>
+   Inspection:
+</PRE>
+<P>
+  <PRE>
+        SHOW     show dipole corrections
+</PRE>
+<P>
+  <PRE>
+        EDIT     edit dipole corrections
+</PRE>
+<P>
+  <PRE>
+   Other:
+</PRE>
+<P>
+  <PRE>
+        QUIT     exit from POLAR
+</PRE>
+<P>
+<A NAME=.pol.orthog><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034800000000000000>  <b>Parameter POL_ORTHOG</b></A></H2>
+<P>
+<em>Prompt:</em> Dipole orthogonalities (deg)|<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the deviations from orthogonality in the dual-dipole assemblies per
+telescope in degrees.
+</PRE>
+<P>
+<A NAME=.pol.rotan><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00034900000000000000>  <b>Parameter POL_ROTAN</b></A></H2>
+<P>
+<em>Prompt:</em> Dipole positions (deg)|<BR><em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the position angles of the dual-dipole assemblies per telescope in
+degrees.
+</PRE>
+<P>
+<A NAME=.pol.x.ellips><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035000000000000000>  <b>Parameter POL_X_ELLIPS</b></A></H2>
+<P>
+<em>Prompt:</em> X-dipole ellipticities (<em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the X-dipole ellipticities per telescope in %
+</PRE>
+<P>
+<A NAME=.pol.y.ellips><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035100000000000000>  <b>Parameter POL_Y_ELLIPS</b></A></H2>
+<P>
+<em>Prompt:</em> Y-dipole ellipticities (<em>Expected input:</em> Real:  1 to 14 values
+<P>
+  <PRE>
+Specify the Y-dipole ellipticities per telescope in %
+</PRE>
+<P>
+<A NAME=.qdetails><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035200000000000000>  <b>Parameter QDETAILS</b></A></H2>
+<P>
+<em>Prompt:</em> More details? (YES/NO)<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want to specify details of the solution procedure yourself
+rather than relying on NCALIB's expert defaults.
+</PRE>
+<P>
+<A NAME=.refraction><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035300000000000000>  <b>Parameter REFRACTION</b></A></H2>
+<P>
+<em>Prompt:</em> Refraction-1: quadratic's coefficients|<BR><em>Expected input:</em> Real:  1 to 3 values
+<P>
+  <PRE>
+Specify the coefficients A, B and C in the quadratic representation of the
+refraction coefficient as a function of frequency F in GHz:
+</PRE>
+<P>
+  <PRE>
+        EXT= (1+A) + B*F +C*F*F
+</PRE>
+<P>
+<A NAME=.save.residuals><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035400000000000000>  <b>Parameter SAVE_RESIDUALS</b></A></H2>
+<P>
+<em>Prompt:</em> Save the interferometer residuals as interferometer errors?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+If YES, the interferometer residuals after Selfcal, Align or Redun will be
+saved for later use as Multiplicative Interferometer errors.
+</PRE>
+<P>
+<A NAME=.set.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035500000000000000>  <b>Parameter SET_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> SET action|<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify action to perform to alter correction values.
+</PRE>
+<P>
+  <PRE>
+   Note: POLARISATION corrections are NOT included here. They must be handled
+    sparately through the POLAR main option.
+</PRE>
+<P>
+  <PRE>
+These option write correction values in (a) set(s) of target sectors (selected
+by the SCN_<xxx> parameters). These corrections are copied/calulated from
+corrections /data in the same file or another one (USE_SCN_<xxx> parameters).
+The calculations will use all source sectors you specify to obtain a single set
+of corrections. Unless stated otherwise below, the new values will be ADDED to
+the existing ones in each of the target sectors.
+</PRE>
+<P>
+  <PRE>
+   Transfer of corrections from a reference source:
+</PRE>
+<P>
+  <PRE>
+        COPY    copy all corrections from somewhere else
+                 (all corrections in the input set(s) are averaged)
+        CCOPY   copy corrections from surrounding (in time) observations
+                 in the input sets with the same frequency channel
+                 (corrections for the two input sets are averaged).
+        ICOPY   copy all MIFR corrections from somewhere else
+                 (all corrections in the input set(s) are averaged)
+        LINE    copy all corrections from corresponding continuum channel
+</PRE>
+<P>
+  <PRE>
+   Initialisation:
+</PRE>
+<P>
+  <PRE>
+        ZERO    zero corrections
+        MANUAL  copy input values into the OTH telescope corrections for
+                 selected scans
+        INIT    make an initial estimate of telescope corrections and shift the
+                 present values accordingly
+        RENORM  renormalise telescope corrections
+</PRE>
+<P>
+  <PRE>
+   Manual-input actions. Each option represents a correction type for which
+   your values will be requested.
+   - For the following actions, your values will OVERWRITE the existing ones:
+        EXT     set extinction in selected scans
+        REF     set refraction in selected scans
+        IREF    set ionospheric refraction in selected scans
+        FAR     set Faraday rotation in selected scans
+        IFR     set additive interferometer corrections in selected scans
+        MIFR    set multiplicative interferometer corrections in selected scans
+        CLK     set clock correction in selected scans
+        SHIFT   set (de-apply) coordinate shift in selected sectors
+</PRE>
+<P>
+  <PRE>
+        QUIT    exit SET
+</PRE>
+<P>
+<A NAME=.shift><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035600000000000000>  <b>Parameter SHIFT</b></A></H2>
+<P>
+<em>Prompt:</em> Shift to de-apply to data (arcsec)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the l,m shift in arcsec to be applied to data whenever the DE_APPLY
+SHIFT correction is requested. (Ignore the 'de-apply) in the prompt.)
+</PRE>
+<P>
+  <PRE>
+In the case where the shift is time-dependent (e.g. for a planet) it is
+approximated by a linear function
+</PRE>
+<P>
+  <PRE>
+        Total shift =  SHIFT + DSHIFT * (HA-HAB)
+</PRE>
+<P>
+  <PRE>
+In this case the SHIFT you specify here is the value at the meridian, DSHIFT is
+a second parameter for which you will be prompted.
+</PRE>
+<P>
+<A NAME=.show.level><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035700000000000000>  <b>Parameter SHOW_LEVEL</b></A></H2>
+<P>
+<em>Prompt:</em> Levels of terminal (1st value)| and log (2nd value) output<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+Specify the level of the type and print output you want:
+</PRE>
+<P>
+  <PRE>
+   0     none
+   1     sector numbers, errors and summary of results only (the summary in the
+          log file includes phase constraints and solution details which are not
+          shown on the terminal)
+   2     detailed report (several pages) per integration interval (parameter
+          HA_INTEGRATION) - intended primarily for debugging purposes
+</PRE>
+<P>
+<A NAME=.solve><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035800000000000000>  <b>Parameter SOLVE</b></A></H2>
+<P>
+<em>Prompt:</em> Solve for gain, phase (YES/NO, 2 values)?<BR><em>Expected input:</em> Yes/No:  1 to 2 values
+<P>
+  <PRE>
+Specify if you want solutions for gain and for phase.
+</PRE>
+<P>
+<A NAME=.use.scn.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00035900000000000000>  <b>Parameter USE_SCN_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> Input .SCN-file name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the input .SCN file from which the corrections should be calculated or
+copied. A wildcard value ('*') indicates the same as the output .SCN file.
+</PRE>
+<P>
+<A NAME=.use.scn.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00036000000000000000>  <b>Parameter USE_SCN_SETS</b></A></H2>
+<P>
+<em>Prompt:</em> Sets of input .SCN-file sectors: grp.obs.fld.chn.seq|<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+Specify the .SCN-file sectors to be used as input in the calculations.
+</PRE>
+<P>
+<A NAME=.vzero.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00036100000000000000>  <b>Parameter VZERO_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> VZERO action<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+This branch of NCALIB implements methods to define the unknown X-Y phase-zero
+difference ('PZD') in the parallel-dipole configuration.
+</PRE>
+<P>
+  <PRE>
+Correction values may be saved in an arbitrary selection of target sectors,
+selected by the SCN_<xxx> parameters. The new corrections are OTH telescope
+phases which will be ADDED to any existing ones in each of the sectors you
+specify for output.
+</PRE>
+<P>
+  <PRE>
+In determining the corrections, the program uses a collection of input sectors,
+which may coincide with the target sectors or be selected by the USE_SCN_
+parameters (for the COPY option). It is assumed that the source for these is a
+calibrator with significant Stokes U and 'negligibly' small Stokes V. If this
+condition is not fulfilled, the result will be meaningless.
+</PRE>
+<P>
+  <PRE>
+The PZD is a phase value that is ADDED to the existing OTH phase correction of
+the X channels. For this reason, you must be cautious to
+</PRE>
+<P>
+  <PRE>
+        - avoid more than one COPY to the same target data and
+        - avoid ruining a calibrator observation by doing an APPLY on it. (If
+           you should do this by accident, use MANUAL to restore the observation
+           to its previous state.)
+</PRE>
+<P>
+  <PRE>
+Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+   Actions recommended for routine use:
+</PRE>
+<P>
+  <PRE>
+        CALC    calculate PZD from the selected node and sectors (SCN_
+                 parameters) and display it with its mean error. Use this option
+                 to check if a calibrator observation is suitable for
+                 determining the PZD.
+</PRE>
+<P>
+  <PRE>
+        COPY    as APPLY, but use X-Y phase-difference value derived from
+                 a calibrator observation (USE_SCN_<xxx> parameters). Use this
+                 option to set the correction for your observations
+</PRE>
+<P>
+  <PRE>
+        MANUAL  manually input phase-difference value
+</PRE>
+<P>
+  <PRE>
+   Other actions:
+</PRE>
+<P>
+  <PRE>
+        SCAN    as CALC, but per individual scan
+</PRE>
+<P>
+  <PRE>
+        APPLY   as CALC, then apply the correction to the sectors selected
+                 (SCN_<xxx> parameters).
+                NOTE that once you have performed this operation, a CALC or COPY
+                 operation on the same input data will yield PZD=0, so these
+                 data can no longer be used to calibrate another observation.
+</PRE>
+<P>
+  <PRE>
+        ASK     as APPLY, but display and ask for confirmation before modifying
+                 the existing values
+</PRE>
+<P>
+  <PRE>
+        QUIT    exit from VZERO
+</PRE>
+<P>
+<A NAME=.vzero.phase><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00036200000000000000>  <b>Parameter VZERO_PHASE</b></A></H2>
+<P>
+<em>Prompt:</em> X-Y phase-zero difference 'PZD' (deg)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the 'phase-zero difference' (PZD) in degrees.
+</PRE>
+<P>
+  <PRE>
+In the parallel-dipole configuration, performing a Redundancy or Selfcal fit of
+telescope errors to the visibilities introduces an unknown phase offset for the
+set of telescope X channels and another unknown phase offset for the Y dipoles.
+For correctly determining Stokes U and V, the (equally unknown) difference
+between these must be corrected for.
+</PRE>
+<P>
+  <PRE>
+This is a tricky problem and you should remain suspicious of the results that
+you get.
+</PRE>
+<P>
+<A NAME=.weight.min><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00036300000000000000>  <b>Parameter WEIGHT_MIN</b></A></H2>
+<P>
+<em>Prompt:</em> Relative minimum weight accepted<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the minimum relative weight of a data point that is still acceptable.
+</PRE>
+<P>
+  <PRE>
+The weight is relative to the maximum weight in the same scan, and in most
+cases can be seen as the minimum data amplitude accepted as fraction of the
+maximum in the scan.
+</PRE>
+<P>
+<A NAME=.zero><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00036400000000000000>  <b>Parameter ZERO</b></A></H2>
+<P>
+<em>Prompt:</em> Corrections (plural) to be zeroed |<BR><em>Expected input:</em> Character *8:  1 to 12 values
+<P>
+  <PRE>
+Specify any number of corrections you want to zero:
+</PRE>
+<P>
+  <PRE>
+   Generic:
+        ALL or * All corrections
+        NONE     None of the corrections: Return to previous prompt
+</PRE>
+<P>
+  <PRE>
+   Telescope gains and phases:
+        RED      Redundancy telescope corrections
+        ALG      Align telescope corrections
+        OTH      'Other' telescope gain/phase corrections
+</PRE>
+<P>
+  <PRE>
+   Interferometer gains and phases:
+        IFR      Additive interferometer corrections
+        MIFR     Multiplicative interferometer corrections
+</PRE>
+<P>
+  <PRE>
+   Corrections for the instrument as a whole:
+        EXT      Extinction correction
+        REF      Refraction correction
+        IREF     Ionospheric refraction correction
+        FAR      Faraday rotation
+        CLK      Clock correction
+        SHIFT    Coordinate shifts (de-apply)
+</PRE>
+<P>
+  <PRE>
+You may restrict the above to phase-only or gain-only by appending AT THE END
+of your reply either of:
+</PRE>
+<P>
+  <PRE>
+        NOGAIN   Zero only phases
+        NOPHASE  Zero only gain
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
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index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_19828_tex2html_wrap451.png differ
diff --git a/ncalib_redun/_19828_tex2html_wrap451.xbm b/ncalib_redun/_19828_tex2html_wrap451.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_19828_tex2html_wrap451.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_24705_tex2html_wrap385.png b/ncalib_redun/_24705_tex2html_wrap385.png
new file mode 100644
index 0000000000000000000000000000000000000000..ab472c77e25093d023deeb0b807b9f4c81dbddd9
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap385.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap385.xbm b/ncalib_redun/_24705_tex2html_wrap385.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..07b852e678b32798e640050bdc49c690b966853b
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap385.xbm
@@ -0,0 +1,4 @@
+#define noname_width 5
+#define noname_height 10
+static char noname_bits[] = {
+ 0x04,0x07,0x04,0x04,0x04,0x04,0x04,0x04,0x04,0x1f};
diff --git a/ncalib_redun/_24705_tex2html_wrap387.png b/ncalib_redun/_24705_tex2html_wrap387.png
new file mode 100644
index 0000000000000000000000000000000000000000..bed3a04d5749de45fbb0a81b963b1d86a89c785f
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap387.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap387.xbm b/ncalib_redun/_24705_tex2html_wrap387.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..286cbcc1eeea43689b259552a27514cb96a90d7a
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap387.xbm
@@ -0,0 +1,44 @@
+#define noname_width 251
+#define noname_height 19
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x1f,0x00,0x00,0x00,0x40,0x00,
+ 0x00,0xfe,0x00,0x00,0x00,0x00,0x00,0x00,0x07,0x0e,0x00,0x00,0x00,0x00,0x00,
+ 0x03,0x00,0x80,0x03,0x00,0x70,0x00,0x00,0x40,0x00,0x40,0x16,0x00,0x40,0xf0,
+ 0x43,0x00,0x00,0xb2,0x00,0x00,0x70,0x00,0x00,0x07,0x07,0x0e,0x00,0x00,0xde,
+ 0x7b,0x00,0x02,0x00,0x80,0x03,0x00,0x7c,0x00,0x00,0x20,0xef,0x7d,0x16,0xef,
+ 0xbd,0x00,0x40,0x78,0xef,0xb3,0x00,0x00,0x70,0x00,0xc0,0x07,0x01,0x0c,0x00,
+ 0x00,0x86,0x31,0x00,0x02,0x00,0x80,0x00,0x00,0x6c,0x00,0x00,0x30,0xc3,0x18,
+ 0x03,0xc3,0x98,0x01,0xe0,0x19,0xc6,0x18,0x00,0x00,0x10,0x00,0xc0,0x06,0x01,
+ 0x0c,0x00,0x00,0xc4,0x11,0x3f,0x02,0x00,0x80,0x00,0x00,0x6c,0x00,0x00,0x10,
+ 0xe2,0x08,0x03,0xe2,0x08,0x01,0x00,0x10,0x47,0x18,0x00,0x00,0x10,0x00,0xc0,
+ 0x06,0x01,0x0c,0x00,0x00,0xc4,0x09,0x00,0x02,0x84,0x81,0x00,0x00,0x6c,0x00,
+ 0x00,0x18,0xe2,0x04,0x03,0xe2,0x04,0x03,0x00,0x10,0x27,0x18,0x80,0x30,0x10,
+ 0x00,0xc0,0x06,0xe1,0x0c,0xfc,0x07,0xe4,0x09,0x00,0x0f,0xcc,0x80,0xb8,0x8d,
+ 0x67,0xf0,0x1f,0x18,0xf2,0xc4,0x07,0xf2,0x04,0x03,0x00,0x90,0x27,0x3e,0x80,
+ 0x19,0x10,0xb7,0x79,0x06,0xb1,0x0d,0xfe,0x07,0xa4,0x05,0x00,0x00,0x78,0x80,
+ 0xbc,0xcd,0x66,0xf8,0x1f,0x18,0xd2,0x02,0x00,0xd2,0x02,0x03,0x00,0x90,0x16,
+ 0x00,0x00,0x0f,0x90,0xb7,0x6d,0x06,0xf9,0x0c,0x00,0x00,0x9c,0x07,0x00,0x00,
+ 0x30,0x80,0x98,0x6d,0x66,0x00,0x00,0x18,0xce,0x03,0x00,0xce,0x03,0x03,0x00,
+ 0x70,0x1e,0x00,0x00,0x06,0x10,0xb3,0x67,0x06,0x19,0x0c,0x00,0x00,0x9c,0x03,
+ 0x00,0x00,0x78,0x80,0x98,0x64,0x66,0x00,0x00,0x18,0xce,0x01,0x00,0xce,0x01,
+ 0x03,0x00,0x70,0x0e,0x00,0x00,0x0f,0x10,0x93,0x66,0x06,0x99,0x0d,0xfe,0x07,
+ 0x8c,0x03,0x00,0x00,0xcc,0x80,0xd8,0x64,0x6a,0xf8,0x1f,0x18,0xc6,0x01,0x00,
+ 0xc6,0x01,0x03,0x00,0x30,0x0e,0x00,0x80,0x19,0x10,0x9b,0xa6,0x06,0xf1,0x0c,
+ 0x00,0x00,0x8c,0x01,0x00,0x00,0x84,0x81,0xf8,0xc3,0x6f,0x00,0x00,0x18,0xc6,
+ 0x00,0x00,0xc6,0x00,0x03,0x00,0x30,0x06,0x00,0x80,0x30,0x10,0x7f,0xfc,0x06,
+ 0x01,0x0c,0x00,0x00,0x84,0x01,0x00,0x00,0x00,0x80,0x00,0x00,0x60,0x00,0x00,
+ 0x10,0xc2,0x00,0x00,0xc2,0x00,0x01,0x00,0x10,0x06,0x00,0x00,0x00,0x10,0x00,
+ 0x00,0x06,0x01,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x00,0x60,
+ 0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0x06,0x07,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x03,
+ 0x00,0x70,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x70,0x00,0x00,0x07,0x07,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x03,0x00,0x70,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x70,0x00,0x00,0x07};
diff --git a/ncalib_redun/_24705_tex2html_wrap389.png b/ncalib_redun/_24705_tex2html_wrap389.png
new file mode 100644
index 0000000000000000000000000000000000000000..f19d994ee5a7776cbbf192f67580fc6a66886d7e
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap389.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap389.xbm b/ncalib_redun/_24705_tex2html_wrap389.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..63c83f944fa199c7565be59c194b504e38afe7c2
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap389.xbm
@@ -0,0 +1,14 @@
+#define noname_width 62
+#define noname_height 19
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0xf8,0x03,0x00,0x00,
+ 0x00,0x08,0x08,0x00,0xc8,0x02,0x00,0x08,0x7e,0x08,0xe4,0xbd,0xcf,0xe2,0xbd,
+ 0x17,0x00,0x08,0x66,0x18,0x63,0x60,0x18,0x33,0x00,0x3c,0x42,0x1c,0x61,0x40,
+ 0x1c,0x21,0x00,0x00,0x43,0x9c,0x60,0x40,0x9c,0x60,0x00,0x00,0x43,0x9e,0xf8,
+ 0x40,0x9e,0x60,0x00,0x00,0x43,0x5a,0x00,0x40,0x5a,0x60,0x00,0x00,0xc3,0x79,
+ 0x00,0xc0,0x79,0x60,0x00,0x00,0xc3,0x39,0x00,0xc0,0x39,0x60,0x00,0x00,0xc3,
+ 0x38,0x00,0xc0,0x38,0x60,0x00,0x00,0xc3,0x18,0x00,0xc0,0x18,0x60,0x00,0x00,
+ 0x42,0x18,0x00,0x40,0x18,0x20,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x30,0x00,
+ 0x00,0x06,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x18,
+ 0x00,0x00};
diff --git a/ncalib_redun/_24705_tex2html_wrap443.png b/ncalib_redun/_24705_tex2html_wrap443.png
new file mode 100644
index 0000000000000000000000000000000000000000..0f2e44f1b07f876cd616ad5d56ca46bf7188fd32
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap443.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap443.xbm b/ncalib_redun/_24705_tex2html_wrap443.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f41e3c79d14817105842e9626d4118671e79f4d5
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap443.xbm
@@ -0,0 +1,10 @@
+#define noname_width 47
+#define noname_height 16
+static char noname_bits[] = {
+ 0x00,0xc0,0x1f,0x00,0x00,0x00,0x00,0x40,0x16,0x07,0x00,0x70,0xef,0x7d,0x16,
+ 0x07,0x00,0x7c,0xc3,0x18,0x03,0x01,0x00,0x6c,0xe2,0x08,0x03,0x01,0x00,0x6c,
+ 0xe2,0x04,0x03,0x01,0x00,0x6c,0xf2,0xc4,0x07,0x71,0x9b,0x67,0xd2,0x02,0x00,
+ 0x79,0xdb,0x66,0xce,0x03,0x00,0x31,0x7b,0x66,0xce,0x01,0x00,0x31,0x69,0x66,
+ 0xc6,0x01,0x00,0xb1,0x69,0x6a,0xc6,0x00,0x00,0xf1,0xc7,0x6f,0xc2,0x00,0x00,
+ 0x01,0x00,0x60,0x00,0x00,0x00,0x01,0x00,0x60,0x00,0x00,0x00,0x07,0x00,0x70,
+ 0x00,0x00,0x00,0x07,0x00,0x70};
diff --git a/ncalib_redun/_24705_tex2html_wrap445.png b/ncalib_redun/_24705_tex2html_wrap445.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap445.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap445.xbm b/ncalib_redun/_24705_tex2html_wrap445.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap445.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_24705_tex2html_wrap447.png b/ncalib_redun/_24705_tex2html_wrap447.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap447.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap447.xbm b/ncalib_redun/_24705_tex2html_wrap447.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap447.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_24705_tex2html_wrap449.png b/ncalib_redun/_24705_tex2html_wrap449.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap449.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap449.xbm b/ncalib_redun/_24705_tex2html_wrap449.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap449.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_24705_tex2html_wrap451.png b/ncalib_redun/_24705_tex2html_wrap451.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap451.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap451.xbm b/ncalib_redun/_24705_tex2html_wrap451.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap451.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_24705_tex2html_wrap453.png b/ncalib_redun/_24705_tex2html_wrap453.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap453.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap453.xbm b/ncalib_redun/_24705_tex2html_wrap453.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap453.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_24705_tex2html_wrap455.png b/ncalib_redun/_24705_tex2html_wrap455.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_24705_tex2html_wrap455.png differ
diff --git a/ncalib_redun/_24705_tex2html_wrap455.xbm b/ncalib_redun/_24705_tex2html_wrap455.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_24705_tex2html_wrap455.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tabbing169.png b/ncalib_redun/_9871_tabbing169.png
new file mode 100644
index 0000000000000000000000000000000000000000..17d2fc6834070d38b1235367765967397c2e09b8
Binary files /dev/null and b/ncalib_redun/_9871_tabbing169.png differ
diff --git a/ncalib_redun/_9871_tabbing169.xbm b/ncalib_redun/_9871_tabbing169.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..dac8f19200a027d15a56142c0147a59c29a5f82e
--- /dev/null
+++ b/ncalib_redun/_9871_tabbing169.xbm
@@ -0,0 +1,667 @@
+#define noname_width 436
+#define noname_height 181
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0x00,0x00,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xff,0xc3,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x00,0x00,0x00,0xe0,0x70,0x80,0x83,0xf9,0x4e,0x00,0x00,0x00,
+ 0xfe,0x07,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x10,0x0c,0x00,0x00,0x02,0x00,
+ 0x00,0x60,0x00,0x00,0x70,0x00,0x60,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x86,0xc1,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,
+ 0x00,0xb0,0xd9,0xc0,0xc6,0x73,0xc6,0x00,0x00,0x00,0x0c,0x03,0x00,0x00,0x00,
+ 0x00,0x00,0x18,0x00,0x18,0x08,0x00,0x00,0x06,0x00,0x00,0x40,0x00,0x00,0x60,
+ 0x00,0x60,0x00,0x80,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x86,0xc1,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,0x10,0xd9,0x40,0x64,
+ 0xe3,0x82,0x00,0x00,0x00,0x0c,0x03,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x08,
+ 0x08,0x00,0x00,0x04,0x00,0x00,0x40,0x00,0x00,0x60,0x00,0x00,0x00,0xc0,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x86,0xe1,0x01,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x04,0x00,0xb0,0xd9,0xc0,0x26,0xc0,0x83,0x01,0x00,0x00,
+ 0x0c,0x03,0x00,0x00,0x00,0x00,0x00,0x19,0x00,0x0c,0x08,0x00,0x02,0x0c,0x00,
+ 0x00,0x40,0x00,0x00,0x60,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x86,0xa1,0x01,0x00,0x00,0x00,0x80,0xf1,0xc0,0x0f,
+ 0x00,0xf0,0x60,0xc0,0xf3,0xc1,0x81,0x01,0x00,0x00,0x0c,0xe3,0xbb,0x7d,0xe0,
+ 0xf9,0xf1,0x9b,0x07,0x8c,0x8f,0xe7,0xff,0x0c,0x78,0x7e,0x7c,0xe0,0xc7,0x67,
+ 0x9e,0x7f,0x9f,0xe7,0x9d,0xef,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xfe,0xa1,0x01,0x00,0x00,0x00,0x80,0x99,0x61,0x02,0x00,0xf0,0xf1,0xc0,0x37,
+ 0x83,0x81,0x01,0x00,0x00,0xfc,0x33,0x32,0x79,0x60,0x33,0x99,0xd8,0x0c,0xcc,
+ 0xc8,0x3c,0xf1,0x0c,0xd8,0x4c,0x46,0xc0,0x6c,0x64,0x36,0x6f,0x93,0xcd,0xd8,
+ 0xc8,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x86,0xf1,0x03,0x00,0x00,
+ 0x00,0x80,0xf9,0x61,0x02,0xc0,0xd3,0xc1,0x40,0x37,0xc2,0x83,0x01,0x00,0x00,
+ 0x0c,0x33,0x36,0x19,0xcf,0x33,0x99,0xd8,0x0f,0xcc,0xc8,0x3f,0x31,0x0c,0xf0,
+ 0x4c,0x46,0xc0,0x68,0x6c,0x3c,0x63,0x0f,0xcf,0xd8,0xd8,0x04,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x86,0x11,0x03,0x00,0x00,0x00,0x80,0x19,0xc0,0x03,
+ 0xc0,0x1b,0xdd,0x60,0x34,0x42,0x87,0x01,0x00,0x00,0x0c,0x33,0x36,0x19,0x6f,
+ 0x33,0xf1,0xd8,0x00,0xcc,0xc8,0xe0,0x31,0x0c,0xd8,0x4c,0x46,0xc0,0x68,0x6c,
+ 0x36,0x63,0x9f,0xcd,0xda,0xd8,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x86,0x19,0x07,0x00,0x00,0x00,0x80,0x19,0x4d,0x60,0x00,0x18,0xdd,0x6c,0x24,
+ 0x23,0x86,0x01,0x00,0x00,0x0c,0x33,0xb2,0x19,0x30,0x37,0x11,0xd8,0x08,0xcc,
+ 0xc8,0x28,0x30,0x0c,0xcc,0x4d,0x46,0xc0,0x6c,0x64,0x73,0x63,0xd1,0xdc,0xda,
+ 0xc8,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xff,0x9f,0x0f,0x00,0x00,
+ 0x00,0x80,0xf1,0xcc,0x67,0x00,0xb0,0xd9,0xcc,0x66,0x7b,0x9e,0x01,0x00,0x00,
+ 0xfe,0xe7,0xf3,0x3f,0xe0,0xff,0xf3,0xbd,0x07,0x8c,0x9f,0xe7,0x7b,0x0c,0xf8,
+ 0xff,0xfc,0xc0,0xc7,0xf7,0xfe,0xf7,0x9f,0xdf,0xbf,0xef,0x0f,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x60,0x0c,
+ 0x00,0xe0,0x30,0x80,0xc3,0x01,0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x03,0x00,0x08,0x00,0x30,0x06,0x04,0x00,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x60,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x03,0x00,0x18,
+ 0x00,0x30,0x06,0x06,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x03,0xc0,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x01,0x00,0x18,0x00,0xe0,0x03,0x06,0x00,
+ 0x00,0x00,0xe0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,
+ 0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x3f,0x1c,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x82,0x21,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x7e,0x00,0x00,0x1c,0x00,0x80,0x03,0x38,0x00,0x00,
+ 0x00,0x60,0x00,0x00,0x00,0xc0,0x00,0xc0,0x01,0x00,0x00,0x00,0x00,0x0e,0x00,
+ 0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0xec,0x18,0x00,0x00,0x00,
+ 0x00,0x00,0x03,0x00,0x00,0x80,0xc3,0x66,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xd8,0x01,0x00,0x18,0x00,0xc0,0x03,0x31,0x00,0x00,0x00,0x60,0x00,0x00,0x00,
+ 0x80,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x0c,0x80,0x18,0x00,0x00,0x00,0x00,
+ 0x40,0x00,0x03,0x00,0x00,0x8c,0x19,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,
+ 0x00,0xe2,0x46,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x03,0x00,0x18,0x00,
+ 0xc0,0x80,0x31,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x0c,0xc0,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,
+ 0x8c,0x19,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x04,0x00,0xe2,0xc4,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x18,0x03,0x00,0x18,0x00,0xc0,0x80,0x31,0x00,0x00,
+ 0x08,0x00,0x00,0x00,0x00,0x80,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x0c,0xc0,
+ 0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0xec,0xd8,0x01,0x00,0x00,
+ 0x00,0x80,0xf1,0xc0,0x0f,0x00,0x02,0xc6,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xd8,0xe1,0xf9,0xd9,0x81,0xef,0xc1,0xf3,0xf1,0x80,0xdf,0x73,0x3f,0xe0,0xf9,
+ 0xf9,0x80,0x9f,0x8f,0xe7,0x7b,0xe0,0xfb,0xec,0xe6,0x9d,0xef,0x07,0xfe,0xc7,
+ 0xf3,0xfc,0xf3,0xbd,0x0f,0xfc,0x78,0x00,0x00,0x00,0x00,0x80,0x99,0x61,0x02,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x01,0x60,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x01,0x00,0x00,
+ 0x00,0x00,0x8c,0x01,0x00,0xc0,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x60,0x0c,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x8c,0x01,0x00,
+ 0xc0,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0xc0,0x07,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0x00,0xf8,0x00,0x00,0x80,0x0f,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x30,0x7f,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,
+ 0x00,0x06,0x38,0x80,0xd7,0x1f,0x04,0x00,0x00,0x00,0x0e,0x00,0x00,0x00,0x00,
+ 0x00,0xc0,0x01,0x00,0x00,0x00,0x00,0xc0,0x60,0x00,0x00,0x07,0xc8,0x7b,0xfe,
+ 0xbd,0x00,0x60,0x1c,0x00,0x80,0xd7,0x1f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x20,0xcc,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x0f,0x6c,0xc0,0x18,
+ 0x73,0x0c,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x40,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x00,0xc0,0x40,0x00,0x00,0x06,0x8c,0x31,0x66,0x98,0x01,0x60,0x1e,0x00,
+ 0xc0,0x18,0x73,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x8c,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x00,0x00,0x80,0x0d,0x6c,0x60,0x10,0x63,0x08,0x00,0x00,0x00,
+ 0x0c,0x00,0x00,0x00,0x60,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x40,0x00,
+ 0x00,0x06,0x84,0x73,0x66,0x10,0x01,0x00,0x06,0x00,0x60,0x10,0x63,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x20,0x8c,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x04,
+ 0x80,0x00,0x6c,0x60,0x10,0xc3,0x18,0x00,0x00,0x00,0x0c,0x00,0x80,0x00,0x60,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x06,0x06,0x73,0x62,
+ 0x10,0x03,0x00,0x06,0x00,0x60,0x10,0xc3,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x3e,0xcc,0xfe,0xc7,0x73,0x07,0x80,0xf1,0xc0,0x0f,0xc0,0x07,0x30,0x30,0x00,
+ 0xc3,0x18,0x00,0x00,0x00,0xcc,0xf3,0xf9,0xbd,0xff,0xc0,0x8f,0xcf,0xf3,0x79,
+ 0xe0,0x7b,0xff,0x7c,0x6e,0x3c,0x06,0x06,0x73,0x62,0x10,0x03,0x70,0xff,0xf9,
+ 0x3f,0x00,0xc3,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x23,0x7c,0xcc,0xcc,0xe6,
+ 0x01,0x80,0x99,0x61,0x02,0xc0,0x0c,0x78,0x30,0x00,0xc3,0x18,0x00,0x00,0x00,
+ 0xcc,0xe6,0x4d,0xe6,0x69,0x80,0x99,0xc9,0x36,0xcd,0xc0,0xcf,0xd3,0x46,0x4c,
+ 0x6c,0x06,0x06,0xff,0x63,0x10,0x03,0x60,0xe6,0xfd,0x3f,0x00,0xc3,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x23,0x0c,0xcc,0x8c,0xc7,0x01,0x80,0xf9,0x61,0x02,
+ 0xc0,0x08,0x60,0x30,0x10,0xc3,0x18,0x00,0x00,0x00,0x8c,0x67,0x4c,0xfe,0x67,
+ 0x80,0x91,0x89,0xf7,0xfc,0xc0,0xfc,0xcf,0x46,0x4c,0x78,0x06,0x06,0xce,0x61,
+ 0x10,0x03,0x60,0x66,0x00,0x30,0x10,0xc3,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x23,0x0c,0xcc,0xcc,0xc6,0x01,0x80,0x19,0xc0,0x03,0xc0,0x08,0x6e,0x60,0x10,
+ 0xc3,0x18,0x00,0x00,0x00,0xcc,0x66,0x78,0x86,0x6f,0x81,0x91,0xc9,0xf6,0x0d,
+ 0xc0,0x0c,0xdf,0x46,0x4c,0x6c,0x06,0x06,0xce,0x61,0x10,0x03,0x60,0x66,0x00,
+ 0x60,0x10,0xc3,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x23,0x0c,0xcc,0x6c,0x6e,
+ 0x03,0x80,0x19,0x4d,0x60,0x80,0xcc,0x6e,0x60,0x10,0x63,0x18,0x00,0x00,0x00,
+ 0x6c,0x6e,0x08,0xc6,0x68,0x81,0x99,0x69,0x1e,0x8d,0xc0,0x8c,0xd1,0x46,0x6c,
+ 0xe6,0x06,0x06,0xce,0xc1,0x08,0x63,0x60,0x66,0xfc,0x6f,0x10,0x63,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x7e,0x1f,0xfe,0xdf,0x7f,0x07,0x80,0xf1,0xcc,0x67,
+ 0x80,0xcd,0x6c,0xc0,0xcd,0x3f,0x18,0x00,0x00,0x00,0xde,0xff,0xf8,0xbc,0xef,
+ 0x81,0xcf,0xdf,0xff,0x79,0xe0,0x79,0xff,0xfd,0xfc,0xfc,0x0f,0x06,0x84,0xc0,
+ 0x0d,0x63,0xf0,0xff,0x00,0xc0,0xcd,0x3f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x60,0x0c,0x00,0x07,0x18,0x00,0x07,
+ 0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x8c,0x01,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x84,0x00,0x03,0x41,0x00,0x00,0x00,
+ 0x00,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x03,0x60,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,
+ 0x00,0x00,0x8c,0x01,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x0c,0x00,0x00,0x80,0x41,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0xc0,0x07,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0xf8,0x00,0x00,
+ 0xc0,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,
+ 0x80,0x21,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap348.png b/ncalib_redun/_9871_tex2html_wrap348.png
new file mode 100644
index 0000000000000000000000000000000000000000..1e8d6ab2c0e0cc5cd2acaf2a1629c8cab0ee7c43
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap348.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap348.xbm b/ncalib_redun/_9871_tex2html_wrap348.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..af08146f2c9193d2615d94af1df94eaec01cc43e
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap348.xbm
@@ -0,0 +1,13 @@
+#define noname_width 73
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x02,0x00,0x00,0x00,0x40,0x00,0x02,0x00,0x38,0x0f,0xe1,0x3c,0x00,
+ 0x00,0x84,0x00,0x62,0x00,0x30,0x86,0xc1,0x18,0x00,0x00,0x87,0x01,0xb3,0x01,
+ 0x38,0x82,0xe0,0x08,0x00,0x00,0x04,0x01,0xbb,0x01,0x68,0xc2,0xa0,0x09,0x00,
+ 0x00,0x04,0x03,0x39,0x01,0x68,0xc2,0xa0,0x09,0x00,0x00,0x04,0x83,0x81,0x01,
+ 0xc8,0xc3,0x20,0x0f,0x00,0x00,0x04,0x83,0x80,0x01,0xcc,0xc1,0x30,0x07,0xf8,
+ 0x0f,0x04,0x83,0xc0,0x00,0xc4,0xc1,0x10,0x07,0x00,0x00,0x04,0xc3,0x60,0x01,
+ 0x84,0xc1,0x10,0x06,0x00,0x00,0x04,0x43,0x30,0x01,0x8f,0xc1,0x3c,0x06,0x00,
+ 0x00,0x1f,0x63,0xf8,0x01,0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x61,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x21,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x80,0x31,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0xc0,0x30,0x00,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap350.png b/ncalib_redun/_9871_tex2html_wrap350.png
new file mode 100644
index 0000000000000000000000000000000000000000..1623db814ad204f0b25118ebe6184086e415df23
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap350.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap350.xbm b/ncalib_redun/_9871_tex2html_wrap350.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0a75d6a84ade76264cfa5b66d7a9d7f355535c6b
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap350.xbm
@@ -0,0 +1,7 @@
+#define noname_width 35
+#define noname_height 10
+static char noname_bits[] = {
+ 0x38,0x0f,0x00,0x00,0x01,0x30,0x06,0x00,0xc0,0x01,0x38,0x02,0x00,0x00,0x01,
+ 0x68,0x02,0x00,0x00,0x01,0x68,0x02,0x00,0x00,0x01,0xc8,0x03,0x00,0x00,0x01,
+ 0xcc,0x01,0xfe,0x03,0x01,0xc4,0x01,0x00,0x00,0x01,0x84,0x01,0x00,0x00,0x01,
+ 0x8f,0x01,0x00,0xc0,0x07};
diff --git a/ncalib_redun/_9871_tex2html_wrap352.png b/ncalib_redun/_9871_tex2html_wrap352.png
new file mode 100644
index 0000000000000000000000000000000000000000..b9595289c5c2a9bf084a8543d7a8440fb4cd0876
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap352.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap352.xbm b/ncalib_redun/_9871_tex2html_wrap352.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..357f3a9a8f20ce616316aee6afe509b7e67f2961
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap352.xbm
@@ -0,0 +1,5 @@
+#define noname_width 24
+#define noname_height 9
+static char noname_bits[] = {
+ 0x80,0x01,0x00,0xe0,0x00,0x00,0x38,0x80,0x7f,0x0e,0x80,0xcd,0x03,0x00,0xff,
+ 0x0f,0x80,0x0d,0x3c,0xc0,0x8c,0xf0,0x80,0x7f,0xc0,0x01,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap354.png b/ncalib_redun/_9871_tex2html_wrap354.png
new file mode 100644
index 0000000000000000000000000000000000000000..c32a23a18dc3a87c18e2655b8397546a343d9601
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap354.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap354.xbm b/ncalib_redun/_9871_tex2html_wrap354.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8d698b15fc4a953a3f65c20892069335b5516f18
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap354.xbm
@@ -0,0 +1,5 @@
+#define noname_width 19
+#define noname_height 10
+static char noname_bits[] = {
+ 0x0c,0x9c,0x07,0x36,0x18,0x03,0x37,0x1c,0x01,0x27,0x34,0x01,0x30,0x34,0x01,
+ 0x30,0xe4,0x01,0x18,0xe6,0x00,0x2c,0xe2,0x00,0x26,0xc2,0x00,0xbf,0xc7,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap356.png b/ncalib_redun/_9871_tex2html_wrap356.png
new file mode 100644
index 0000000000000000000000000000000000000000..e378fbc28034ad991ed0db9483438b87e09d6cc0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap356.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap356.xbm b/ncalib_redun/_9871_tex2html_wrap356.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..094bd0a2851f723347c74bebf30c01293f8ea97b
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap356.xbm
@@ -0,0 +1,14 @@
+#define noname_width 88
+#define noname_height 15
+static char noname_bits[] = {
+ 0x07,0x00,0xe0,0x00,0x00,0x00,0x00,0x00,0x00,0x38,0xe0,0x07,0x00,0xec,0x00,
+ 0x00,0xf0,0xde,0x03,0x00,0x38,0xe0,0x01,0x00,0xcc,0x00,0x00,0x30,0x8c,0x01,
+ 0x00,0x08,0xc0,0x01,0x00,0xcc,0x00,0x00,0x20,0x8e,0x00,0x00,0x08,0xc0,0x01,
+ 0x00,0xcc,0x00,0x00,0x20,0x4e,0x80,0x30,0x08,0xc0,0x71,0x9b,0xc7,0xe0,0x3f,
+ 0x20,0x4f,0x80,0x19,0x08,0xc7,0x79,0xdb,0xc6,0xf0,0x3f,0x20,0x2d,0x00,0x0f,
+ 0x88,0xcd,0x31,0x7b,0xc6,0x00,0x00,0xe0,0x3c,0x00,0x06,0xc8,0xc7,0x31,0x69,
+ 0xc6,0x00,0x00,0xe0,0x1c,0x00,0x0f,0xc8,0xc0,0xb1,0x69,0xca,0xf0,0x3f,0x60,
+ 0x1c,0x80,0x19,0xc8,0xcc,0xf1,0xc7,0xcf,0x00,0x00,0x60,0x0c,0x80,0x30,0x88,
+ 0xc7,0x01,0x00,0xc0,0x00,0x00,0x20,0x0c,0x00,0x00,0x08,0xc0,0x01,0x00,0xc0,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x08,0xc0,0x07,0x00,0xe0,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x38,0xe0,0x07,0x00,0xe0,0x00,0x00,0x00,0x00,0x00,0x00,0x38,0xe0};
diff --git a/ncalib_redun/_9871_tex2html_wrap358.png b/ncalib_redun/_9871_tex2html_wrap358.png
new file mode 100644
index 0000000000000000000000000000000000000000..8b1e6b2075835df301cb7d190c901b053b43501e
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap358.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap358.xbm b/ncalib_redun/_9871_tex2html_wrap358.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..46012c3415d0ae0eee7819e3a07d7ed32d4ea4a4
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap358.xbm
@@ -0,0 +1,6 @@
+#define noname_width 24
+#define noname_height 15
+static char noname_bits[] = {
+ 0x07,0x00,0xe0,0x07,0x00,0xec,0x01,0x00,0xcc,0x01,0x00,0xcc,0x01,0x00,0xcc,
+ 0x71,0x9b,0xc7,0x79,0xdb,0xc6,0x31,0x7b,0xc6,0x31,0x69,0xc6,0xb1,0x69,0xca,
+ 0xf1,0xc7,0xcf,0x01,0x00,0xc0,0x01,0x00,0xc0,0x07,0x00,0xe0,0x07,0x00,0xe0};
diff --git a/ncalib_redun/_9871_tex2html_wrap360.png b/ncalib_redun/_9871_tex2html_wrap360.png
new file mode 100644
index 0000000000000000000000000000000000000000..d960db72898947b0eeb8ad0eb8b6a9ec1220e25f
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap360.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap360.xbm b/ncalib_redun/_9871_tex2html_wrap360.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..375a7a0d1bde8e3ad57a2a12a1e0f02994489f37
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap360.xbm
@@ -0,0 +1,5 @@
+#define noname_width 12
+#define noname_height 15
+static char noname_bits[] = {
+ 0x07,0x0e,0x07,0x0e,0x01,0x0c,0x01,0x0c,0x01,0x0c,0xe1,0x0c,0xb1,0x0d,0xf9,
+ 0x0c,0x19,0x0c,0x99,0x0d,0xf1,0x0c,0x01,0x0c,0x01,0x0c,0x07,0x0e,0x07,0x0e};
diff --git a/ncalib_redun/_9871_tex2html_wrap364.png b/ncalib_redun/_9871_tex2html_wrap364.png
new file mode 100644
index 0000000000000000000000000000000000000000..cd29600d6905c80cad7bffa9163c3b4965a6df31
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap364.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap364.xbm b/ncalib_redun/_9871_tex2html_wrap364.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d3e9f1a22fc7e683e4a30d7892a0e37e1c93f75a
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap364.xbm
@@ -0,0 +1,5 @@
+#define noname_width 14
+#define noname_height 11
+static char noname_bits[] = {
+ 0xef,0x3d,0xc3,0x18,0xe2,0x08,0xe2,0x04,0xf2,0x04,0xd2,0x02,0xce,0x03,0xce,
+ 0x01,0xc6,0x01,0xc6,0x00,0xc2,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap366.png b/ncalib_redun/_9871_tex2html_wrap366.png
new file mode 100644
index 0000000000000000000000000000000000000000..bed3a04d5749de45fbb0a81b963b1d86a89c785f
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap366.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap366.xbm b/ncalib_redun/_9871_tex2html_wrap366.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..286cbcc1eeea43689b259552a27514cb96a90d7a
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap366.xbm
@@ -0,0 +1,44 @@
+#define noname_width 251
+#define noname_height 19
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x1f,0x00,0x00,0x00,0x40,0x00,
+ 0x00,0xfe,0x00,0x00,0x00,0x00,0x00,0x00,0x07,0x0e,0x00,0x00,0x00,0x00,0x00,
+ 0x03,0x00,0x80,0x03,0x00,0x70,0x00,0x00,0x40,0x00,0x40,0x16,0x00,0x40,0xf0,
+ 0x43,0x00,0x00,0xb2,0x00,0x00,0x70,0x00,0x00,0x07,0x07,0x0e,0x00,0x00,0xde,
+ 0x7b,0x00,0x02,0x00,0x80,0x03,0x00,0x7c,0x00,0x00,0x20,0xef,0x7d,0x16,0xef,
+ 0xbd,0x00,0x40,0x78,0xef,0xb3,0x00,0x00,0x70,0x00,0xc0,0x07,0x01,0x0c,0x00,
+ 0x00,0x86,0x31,0x00,0x02,0x00,0x80,0x00,0x00,0x6c,0x00,0x00,0x30,0xc3,0x18,
+ 0x03,0xc3,0x98,0x01,0xe0,0x19,0xc6,0x18,0x00,0x00,0x10,0x00,0xc0,0x06,0x01,
+ 0x0c,0x00,0x00,0xc4,0x11,0x3f,0x02,0x00,0x80,0x00,0x00,0x6c,0x00,0x00,0x10,
+ 0xe2,0x08,0x03,0xe2,0x08,0x01,0x00,0x10,0x47,0x18,0x00,0x00,0x10,0x00,0xc0,
+ 0x06,0x01,0x0c,0x00,0x00,0xc4,0x09,0x00,0x02,0x84,0x81,0x00,0x00,0x6c,0x00,
+ 0x00,0x18,0xe2,0x04,0x03,0xe2,0x04,0x03,0x00,0x10,0x27,0x18,0x80,0x30,0x10,
+ 0x00,0xc0,0x06,0xe1,0x0c,0xfc,0x07,0xe4,0x09,0x00,0x0f,0xcc,0x80,0xb8,0x8d,
+ 0x67,0xf0,0x1f,0x18,0xf2,0xc4,0x07,0xf2,0x04,0x03,0x00,0x90,0x27,0x3e,0x80,
+ 0x19,0x10,0xb7,0x79,0x06,0xb1,0x0d,0xfe,0x07,0xa4,0x05,0x00,0x00,0x78,0x80,
+ 0xbc,0xcd,0x66,0xf8,0x1f,0x18,0xd2,0x02,0x00,0xd2,0x02,0x03,0x00,0x90,0x16,
+ 0x00,0x00,0x0f,0x90,0xb7,0x6d,0x06,0xf9,0x0c,0x00,0x00,0x9c,0x07,0x00,0x00,
+ 0x30,0x80,0x98,0x6d,0x66,0x00,0x00,0x18,0xce,0x03,0x00,0xce,0x03,0x03,0x00,
+ 0x70,0x1e,0x00,0x00,0x06,0x10,0xb3,0x67,0x06,0x19,0x0c,0x00,0x00,0x9c,0x03,
+ 0x00,0x00,0x78,0x80,0x98,0x64,0x66,0x00,0x00,0x18,0xce,0x01,0x00,0xce,0x01,
+ 0x03,0x00,0x70,0x0e,0x00,0x00,0x0f,0x10,0x93,0x66,0x06,0x99,0x0d,0xfe,0x07,
+ 0x8c,0x03,0x00,0x00,0xcc,0x80,0xd8,0x64,0x6a,0xf8,0x1f,0x18,0xc6,0x01,0x00,
+ 0xc6,0x01,0x03,0x00,0x30,0x0e,0x00,0x80,0x19,0x10,0x9b,0xa6,0x06,0xf1,0x0c,
+ 0x00,0x00,0x8c,0x01,0x00,0x00,0x84,0x81,0xf8,0xc3,0x6f,0x00,0x00,0x18,0xc6,
+ 0x00,0x00,0xc6,0x00,0x03,0x00,0x30,0x06,0x00,0x80,0x30,0x10,0x7f,0xfc,0x06,
+ 0x01,0x0c,0x00,0x00,0x84,0x01,0x00,0x00,0x00,0x80,0x00,0x00,0x60,0x00,0x00,
+ 0x10,0xc2,0x00,0x00,0xc2,0x00,0x01,0x00,0x10,0x06,0x00,0x00,0x00,0x10,0x00,
+ 0x00,0x06,0x01,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x00,0x60,
+ 0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0x06,0x07,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x03,
+ 0x00,0x70,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x70,0x00,0x00,0x07,0x07,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x03,0x00,0x70,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x70,0x00,0x00,0x07};
diff --git a/ncalib_redun/_9871_tex2html_wrap368.png b/ncalib_redun/_9871_tex2html_wrap368.png
new file mode 100644
index 0000000000000000000000000000000000000000..f19d994ee5a7776cbbf192f67580fc6a66886d7e
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap368.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap368.xbm b/ncalib_redun/_9871_tex2html_wrap368.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..63c83f944fa199c7565be59c194b504e38afe7c2
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap368.xbm
@@ -0,0 +1,14 @@
+#define noname_width 62
+#define noname_height 19
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0xf8,0x03,0x00,0x00,
+ 0x00,0x08,0x08,0x00,0xc8,0x02,0x00,0x08,0x7e,0x08,0xe4,0xbd,0xcf,0xe2,0xbd,
+ 0x17,0x00,0x08,0x66,0x18,0x63,0x60,0x18,0x33,0x00,0x3c,0x42,0x1c,0x61,0x40,
+ 0x1c,0x21,0x00,0x00,0x43,0x9c,0x60,0x40,0x9c,0x60,0x00,0x00,0x43,0x9e,0xf8,
+ 0x40,0x9e,0x60,0x00,0x00,0x43,0x5a,0x00,0x40,0x5a,0x60,0x00,0x00,0xc3,0x79,
+ 0x00,0xc0,0x79,0x60,0x00,0x00,0xc3,0x39,0x00,0xc0,0x39,0x60,0x00,0x00,0xc3,
+ 0x38,0x00,0xc0,0x38,0x60,0x00,0x00,0xc3,0x18,0x00,0xc0,0x18,0x60,0x00,0x00,
+ 0x42,0x18,0x00,0x40,0x18,0x20,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x30,0x00,
+ 0x00,0x06,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x18,
+ 0x00,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap370.png b/ncalib_redun/_9871_tex2html_wrap370.png
new file mode 100644
index 0000000000000000000000000000000000000000..0f2e44f1b07f876cd616ad5d56ca46bf7188fd32
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap370.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap370.xbm b/ncalib_redun/_9871_tex2html_wrap370.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f41e3c79d14817105842e9626d4118671e79f4d5
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap370.xbm
@@ -0,0 +1,10 @@
+#define noname_width 47
+#define noname_height 16
+static char noname_bits[] = {
+ 0x00,0xc0,0x1f,0x00,0x00,0x00,0x00,0x40,0x16,0x07,0x00,0x70,0xef,0x7d,0x16,
+ 0x07,0x00,0x7c,0xc3,0x18,0x03,0x01,0x00,0x6c,0xe2,0x08,0x03,0x01,0x00,0x6c,
+ 0xe2,0x04,0x03,0x01,0x00,0x6c,0xf2,0xc4,0x07,0x71,0x9b,0x67,0xd2,0x02,0x00,
+ 0x79,0xdb,0x66,0xce,0x03,0x00,0x31,0x7b,0x66,0xce,0x01,0x00,0x31,0x69,0x66,
+ 0xc6,0x01,0x00,0xb1,0x69,0x6a,0xc6,0x00,0x00,0xf1,0xc7,0x6f,0xc2,0x00,0x00,
+ 0x01,0x00,0x60,0x00,0x00,0x00,0x01,0x00,0x60,0x00,0x00,0x00,0x07,0x00,0x70,
+ 0x00,0x00,0x00,0x07,0x00,0x70};
diff --git a/ncalib_redun/_9871_tex2html_wrap372.png b/ncalib_redun/_9871_tex2html_wrap372.png
new file mode 100644
index 0000000000000000000000000000000000000000..4fb7174e1c37b0a0cf46209e6e9f77a5d2725124
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap372.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap372.xbm b/ncalib_redun/_9871_tex2html_wrap372.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..930dd009ab984dfe3f327a3ae28d0fdd77a2e6bd
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap372.xbm
@@ -0,0 +1,4 @@
+#define noname_width 2
+#define noname_height 13
+static char noname_bits[] = {
+ 0x03,0x03,0x00,0x00,0x00,0x00,0x03,0x03,0x00,0x00,0x00,0x03,0x03};
diff --git a/ncalib_redun/_9871_tex2html_wrap404.png b/ncalib_redun/_9871_tex2html_wrap404.png
new file mode 100644
index 0000000000000000000000000000000000000000..340a961e0dbfdd85d74d9189cae2945e93283250
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap404.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap404.xbm b/ncalib_redun/_9871_tex2html_wrap404.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..db427a0ace063ae73fdf2d51f8d8aa221156f9da
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap404.xbm
@@ -0,0 +1,10 @@
+#define noname_width 63
+#define noname_height 13
+static char noname_bits[] = {
+ 0x00,0x40,0x70,0x18,0x00,0x06,0x00,0x00,0x20,0x70,0xd8,0x6c,0x00,0x06,0x00,
+ 0x00,0x20,0x40,0x88,0x64,0x00,0x06,0x00,0x00,0x20,0x40,0xd8,0x46,0x00,0x06,
+ 0x00,0x00,0x20,0x40,0x78,0x46,0xc0,0xe3,0xf0,0x7c,0xff,0x43,0xf8,0x46,0x60,
+ 0xb3,0xd9,0x7e,0x20,0x40,0xe8,0x46,0x30,0xfb,0xd8,0x0c,0x20,0x40,0x8c,0x46,
+ 0x30,0x1b,0xc8,0x0c,0x20,0x40,0x8c,0x64,0x30,0x9d,0x49,0x0c,0xff,0xf3,0xd9,
+ 0x6c,0xe0,0xf7,0x78,0x0c,0xff,0x03,0x70,0x38,0x00,0x00,0x60,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x6c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x3c,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap406.png b/ncalib_redun/_9871_tex2html_wrap406.png
new file mode 100644
index 0000000000000000000000000000000000000000..cbe33869f7698a962fbadd11285754977fdfd5e5
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap406.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap406.xbm b/ncalib_redun/_9871_tex2html_wrap406.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..80b9cdf03e0fd204abe5e26a7fd36dd5532bc424
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap406.xbm
@@ -0,0 +1,5 @@
+#define noname_width 24
+#define noname_height 10
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x20,0x00,0x00,0x20,0x00,0x00,0x20,0xf0,0x79,0xff,0x93,0x8f,
+ 0x20,0x08,0x87,0x20,0x08,0x86,0x20,0x10,0x8f,0xff,0xf3,0x79,0xff,0x03,0x00};
diff --git a/ncalib_redun/_9871_tex2html_wrap410.png b/ncalib_redun/_9871_tex2html_wrap410.png
new file mode 100644
index 0000000000000000000000000000000000000000..5355db230b7fe62ec4ae61e248b907d939e9ac15
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap410.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap410.xbm b/ncalib_redun/_9871_tex2html_wrap410.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f64a3d2075f60ae2c5fa5c1b3e4f6a70db3788ce
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap410.xbm
@@ -0,0 +1,5 @@
+#define noname_width 15
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x38,0x0e,0x0c,0x18,0x1e,0x3c,0x36,0x36,0x63,0x63,0xc3,0x61,0xc3,
+ 0x61,0x63,0x63,0x36,0x36,0x1e,0x3c,0x0c,0x18,0x38,0x0e,0xf0,0x07};
diff --git a/ncalib_redun/_9871_tex2html_wrap424.png b/ncalib_redun/_9871_tex2html_wrap424.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap424.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap424.xbm b/ncalib_redun/_9871_tex2html_wrap424.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap424.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tex2html_wrap426.png b/ncalib_redun/_9871_tex2html_wrap426.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap426.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap426.xbm b/ncalib_redun/_9871_tex2html_wrap426.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap426.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tex2html_wrap428.png b/ncalib_redun/_9871_tex2html_wrap428.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap428.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap428.xbm b/ncalib_redun/_9871_tex2html_wrap428.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap428.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tex2html_wrap430.png b/ncalib_redun/_9871_tex2html_wrap430.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap430.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap430.xbm b/ncalib_redun/_9871_tex2html_wrap430.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap430.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tex2html_wrap432.png b/ncalib_redun/_9871_tex2html_wrap432.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap432.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap432.xbm b/ncalib_redun/_9871_tex2html_wrap432.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap432.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tex2html_wrap434.png b/ncalib_redun/_9871_tex2html_wrap434.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap434.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap434.xbm b/ncalib_redun/_9871_tex2html_wrap434.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap434.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/_9871_tex2html_wrap436.png b/ncalib_redun/_9871_tex2html_wrap436.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/ncalib_redun/_9871_tex2html_wrap436.png differ
diff --git a/ncalib_redun/_9871_tex2html_wrap436.xbm b/ncalib_redun/_9871_tex2html_wrap436.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/ncalib_redun/_9871_tex2html_wrap436.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/ncalib_redun/images.pl b/ncalib_redun/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..a5cdbc2550601507d37648d715ab2ebc7dfd2b1c
--- /dev/null
+++ b/ncalib_redun/images.pl
@@ -0,0 +1,85 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$[e]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap360.xbm">'; 
+$key = q/{}$W${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap364.xbm">'; 
+$key = q/{}$pm180~degr${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap404.xbm">'; 
+$key = q/{}fbox<<330>>largesf~<<331>>smallsf<<403>><<403>>$<$<<404>><<404>>CR<<405>><<405>>$>$<<406>><<406>><<331>><<330>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap443.xbm">'; 
+$key = q/{}fbox<<336>>largesf~<<337>>smallsf<<412>><<412>>$<$<<413>><<413>>CR<<414>><<414>>$>$<<415>><<415>><<337>><<336>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap434.xbm">'; 
+$key = q/{}$[e]=W^<<141>>-1<<141>>times[wd]=<<282>>(W^<<142>>T<<142>>W)<<282>>^<<143>>-1<<143>>W^<<144>>T<<144>>times[wd]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap385.xbm">'; 
+$key = q/{}$N(N-1)2${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap348.xbm">'; 
+$key = q/{}fbox<<323>>largesf~<<324>>smallsf<<397>><<397>>$<$<<398>><<398>>CR<<399>><<399>>$>$<<400>><<400>><<324>><<323>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap441.xbm">'; 
+$key = q/{}fbox<<315>>largesf~<<316>>smallsf<<388>><<388>>$<$<<389>><<389>>CR<<390>><<390>>$>$<<391>><<391>><<316>><<315>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap428.xbm">'; 
+$key = q/{tabbing}+++++=+++++=+++++=+++++=+++++=+++++=+++++=+++++=+++++=kill>HA>(e.g.-83.86X)>>Hour-angle(degr)andpolarisation>Rk>(e.g.12)>>Rankofthegainandphasesolutionmatrices>A(%)>(e.g.3.3)>>RMSgainresidual(%)>P(deg)>(e.g.2.2)>>RMSphaseresidual(degr)>A(WU)>(e.g.1.6)>>RMSgainresidual(WU=WesterborkUnit)>P(WU)>(e.g.1.8)>>RMSphaseresidual(WU)>Amax>(e.g.63)>>Maximumampl(WU)>Aavg>(e.g.50.1)>>Averageampl(WU)>Arms>(e.g.5.1)>>RMSampl(WU)>dAmax>(e.g.-12.423)>>largestgain>dPmax>(e.g.6.3CD)>>largestphaseresidual(WU),ifr=CD{tabbing}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tabbing169.xbm">'; 
+$key = q/{}$W^<<141>>T<<141>>[wd]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap370.xbm">'; 
+$key = q/{}fbox<<323>>largesf~<<324>>smallsf<<401>><<401>>$<$<<402>><<402>>CR<<403>><<403>>$>$<<404>><<404>><<324>><<323>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap445.xbm">'; 
+$key = q/{}$<<270>>(W^<<139>>T<<139>>W)<<270>>^<<140>>-1<<140>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap368.xbm">'; 
+$key = q/{}fbox<<301>>largesf~<<302>>smallsf<<376>><<376>>$<$<<377>><<377>>CR<<378>><<378>>$>$<<379>><<379>><<302>><<301>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap424.xbm">'; 
+$key = q/{}$[wd]=Wtimes[e]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap356.xbm">'; 
+$key = q/{}$[wd]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap358.xbm">'; 
+$key = q/{}fbox<<359>>largesf~<<360>>smallsf<<435>><<435>>$<$<<436>><<436>>CR<<437>><<437>>$>$<<438>><<438>><<360>><<359>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap451.xbm">'; 
+$key = q/{}fbox<<337>>largesf~<<338>>smallsf<<409>><<409>>$<$<<410>><<410>>CR<<411>><<411>>$>$<<412>><<412>><<338>><<337>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap445.xbm">'; 
+$key = q/{}fbox<<316>>largesf~<<317>>smallsf<<391>><<391>>$<$<<392>><<392>>CR<<393>><<393>>$>$<<394>><<394>><<317>><<316>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap439.xbm">'; 
+$key = q/{}fbox<<308>>largesf~<<309>>smallsf<<382>><<382>>$<$<<383>><<383>>CR<<384>><<384>>$>$<<385>><<385>><<309>><<308>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap426.xbm">'; 
+$key = q/{}$vdots${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap372.xbm">'; 
+$key = q/{}fbox<<351>>largesf~<<352>>smallsf<<431>><<431>>$<$<<432>><<432>>CR<<433>><<433>>$>$<<434>><<434>><<352>><<351>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap453.xbm">'; 
+$key = q/{}$<<283>>(W^<<145>>T<<145>>W)<<283>>^<<146>>-1<<146>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap387.xbm">'; 
+$key = q/{}fbox<<344>>largesf~<<345>>smallsf<<415>><<415>>$<$<<416>><<416>>CR<<417>><<417>>$>$<<418>><<418>><<345>><<344>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap447.xbm">'; 
+$key = q/{}fbox<<329>>largesf~<<330>>smallsf<<400>><<400>>$<$<<401>><<401>>CR<<402>><<402>>$>$<<403>><<403>><<330>><<329>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap432.xbm">'; 
+$key = q/{}$[e]=W^<<135>>-1<<135>>times[wd]=<<269>>(W^<<136>>T<<136>>W)<<269>>^<<137>>-1<<137>>W^<<138>>T<<138>>times[wd]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap366.xbm">'; 
+$key = q/{}$N-1${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap350.xbm">'; 
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+$key = q/{}$W^<<147>>T<<147>>[wd]${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap389.xbm">'; 
+$key = q/{}$bigotimes${}/;
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diff --git a/ncalib_redun/labels.pl b/ncalib_redun/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..fa2b9c26c1afc7497be77f984fe328a19b51727a
--- /dev/null
+++ b/ncalib_redun/labels.pl
@@ -0,0 +1,15 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".redundancy"} ="$URL/ncalib_redun.html"; 
+$external_labels{".ncalib.3c48"} ="$URL/ncalib_redun.html"; 
+$external_labels{".ncalib.matrix"} ="$URL/ncalib_redun.html"; 
+$external_labels{".qdetails"} ="$URL/ncalib_redun.html"; 
+$external_labels{".ncalib.vispace"} ="$URL/ncalib_redun.html"; 
+$external_labels{".contents"} ="$URL/ncalib_redun.html"; 
+$external_labels{".selfcal"} ="$URL/ncalib_redun.html"; 
+$external_labels{".log.output"} ="$URL/ncalib_redun.html"; 
+$external_labels{".ncalib.scan"} ="$URL/ncalib_redun.html"; 
+$external_labels{".align"} ="$URL/ncalib_redun.html"; 
+
+1;
\ No newline at end of file
diff --git a/ncalib_redun/ncalib_redun.html b/ncalib_redun/ncalib_redun.html
new file mode 100644
index 0000000000000000000000000000000000000000..ccb1876405b788179bd3a0fefe12ef3caf8cafcd
--- /dev/null
+++ b/ncalib_redun/ncalib_redun.html
@@ -0,0 +1,237 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>NCALIB REDUN: Redundancy, Align and Selfcal</b> <A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncalib_redun.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncalib_redun.html#SECTION0002000000000000000> <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ncalib_redun.html#SECTION0003000000000000000> <b>Redundancy</b></A>
+<LI> <A NAME=tex2html4 HREF=ncalib_redun.html#SECTION0004000000000000000> <b>Align</b></A>
+<LI> <A NAME=tex2html5 HREF=ncalib_redun.html#SECTION0005000000000000000> <b>Selfcal</b></A>
+<LI> <A NAME=tex2html6 HREF=ncalib_redun.html#SECTION0006000000000000000> <b>Discussion of the screen/log output</b></A>
+<LI> <A NAME=tex2html7 HREF=ncalib_redun.html#SECTION0007000000000000000> <b>QDETAILS: Hidden parameters</b></A>
+</UL>
+<H1><A NAME=SECTION0002000000000000000> <b>Overview</b></A></H1>
+<P>
+        The NCALIB option <b>REDUN</b> actually covers three related methods of estimating telescope gain and phase errors from the uv-data itself: Redundancy, Selfcal and Align. All three methods require the socalled `Selfcal assumption', which states that all phase and gain errors are <em>telescope-based</em>.    
+ This means that the errors can be fully decomposed into contributions from individual telescopes, and that interferometer-based errors can be ignored. This assumption implies a drastic reduction in the number of <em>independent</em> errors in the data taken with an N-telescope array: from <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap348.png"> to <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap350.png"> per integration interval.  This relatively small number of independent errors can be determined with a <em>least-squares fitting</em> technique.   
+        Any <em>interferometer-based</em> errors (e.g.  thermal noise or correlator errors) violate the basic Selfcal assumption, and cause propagating errors in the solution.  Fortunately, the WSRT correlators only contribute very 
+small interferometer errors (typically <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap352.png">0.01%),   
+but the S/N per uv-sample should be at least 2-5 for a good solution.
+<P>
+        Independent solutions can be obtained for telescope gain and phase errors, because they are mathematically `orthogonal'.
+<P>
+<UL><LI> <b>Selfcal:</b>   
+        The telescope gain and phase errors are estimated by comparing the uv-data with a model of the observed source.  In WSRT Selfcal, the information from redundant spacings can be added as <em>extra constraints</em> on the Selfcal solution.  Since this extra information is model-independent, the Selfcal process is less likely to converge to the wrong result.
+<P>
+<LI> <b>Redundancy:</b>   
+        Telescope gain and phase errors are estimated by comparing the uv-data of `redundant' interferometers, i.e.  interferometers that have the same baseline length and orientation.  Since this is a comparative method, the absolute gain (flux) and the absolute phase gradient (position) cannot be determined.  The result is a set of `internally perfect' HA-scans, that still have to be `aligned' (see below) to each other in flux and position.
+<P>
+<LI> <b>Align:</b>   
+        The absolute gain and the absolute phase gradient for misaligned HA-scans can be determined with the help of a source model.  This is similar to Selfcal, except that one only solves for one parameter per HA-scan, rather than for N telescope errors.  This has the advantage that the source model may be less perfect, and the SNR of the uv-data may be lower.  Therefore, this method may also be used to remove ionosferic phase gradients from data that have too little SNR to warrant Redundancy or Selfcal.
+<P>
+</UL>
+<P>
+        The figures of this section may help to illustrate the effects of these three methods.  There is also a description of the relevant mathematical formalism.  Finally, this section contains processing examples and an explanation of the output that is produced on the screen and in the log file.
+<P>
+<A NAME=.ncalib.3c48><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/ncalib_3c48.ps"><STRONG>FIGURE</STRONG></A>
+<P>
+ .]<i>Principal features of the Selfcal, Redundancy and Align methods. 
+<BR><BR>These four maps of 3C48 may serve to demonstrate the main features of the three methods: 
+<BR><BR>The <em>radial stripes</em> in (a) are caused by large-scale effects at specific Hour Angles. These limit the dynamic range of the 'Standard Reduction' to about 1:100 (20 dB). They are still present after a Redundancy solution, but can be be removed with an Align. 
+<BR><BR>The <em>prominent rings</em> in (b) are caused by a slowly varying gain or phase errors between telescopes A and B. They could be removed by Redundancy, but only if there is a full solution for all 14 telescopes. Otherwise they can be removed with Align or Selfcal. 
+<BR><BR>The <em>almost perfect map</em> in (c) is the result of Selfcal, without Redundancy. The minor remaining problems are caused by the incompleteness of the source model, particularly the small source near 3C48. 
+<BR><BR>The <em>finished product</em> in (d) is essentially perfect, and has a dynamic range in excess of 1:10000 (40 dB), limited by the noise only. The remaining rings are the grating rings of sources which have not been completely subtracted. The result has been produced by a full Redundancy solution, followed by an Align with a model that contained about 10 point sources. 
+(and Reduction very low </i>
+<P>
+<A NAME=.ncalib.scan><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/ncalib_scan.ps"><STRONG>FIGURE</STRONG></A>
+<P>
+ .]<i>The effects of Redundancy, Selfcal and Align on the visibilities in a single HA-scan.  
+<BR><BR>In all four pictures, the broken line represents the `true' visibility amplitudes and phases, as a function of baseline length (u).  The actual uv-data are given by crosses.  Note the multiple uv-data for redundant baselines.  The source model in this example (full line) is an off-axis point source.  
+<BR><BR><b>Redundancy</b>: In (a), he actually measured uv-samples are scattered, because of instrumental errors.  After Redundancy calibration (b), the amplitudes and phases of redundant baselines are the same (except for a little residual scatter caused by noise).  The result is an `internally perfect HA-scan', i.e.  its shape is as it should be, but two parameters are still missing: the absolute flux and the absolute position in the sky.  A map made in this stage would show radial stripes around strong sources.  
+<BR><BR><b>Align</b>: In (c), the perfect HA-scans that are produced by Redundancy are `Aligned' with the help of a model of the observed source.  The `rigid' Scans are moved as a whole to fit the model in a <em>weighted least-squares</em> sense.  Arrows indicate the two parameters that are determined by Align: one to shift all amplitudes vertically, and one to rotate all phases around the origin.  Note that the outcome can be influenced by giving more weight to certain baselines.  
+<BR><BR><b>Selfcal</b>: In `normal' Selfcal (d), the source model is used to determine <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap354.png"> telescope gain and phase errors.  Since this number of independent parameters is larger than the two that were needed for Align, the Scan is less `rigid'.  This means that the data have greater freedom to adapt themselves to the <em>wrong</em> source model.  
+<BR><BR>To counter this effect, Redundancy constraints can be added to the Selfcal solution In the <i>NEWSTAR </i> implementation.  If the Redundancy constraints would be given infinite weight, the outcome would be identical to that of Redundancy followed by Align.  However, this has the disadvantage that a Redundancy solution may have `frozen-in' errors caused by noise in certain critical baselines.  Such errors may be `thawed out' by giving more weight to Selfcal (model) constraints.  In the present implementation, Selfcal and Redundancy constraints have equal weights, which may be close to optimum.  </i>
+<P>
+<A NAME=.ncalib.matrix><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/ncalib_matrix.ps"><STRONG>FIGURE</STRONG></A>
+<P>
+ .]<i>Least-squares fit of telescope errors through matrix inversion. 
+<BR><BR>The <b>problem</b> is formulated by the matrix equation 
+        <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap356.png"> in which <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap358.png"> is a vector of known values, and <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap360.png"> is a vector of unkown telescope errors. Each row (equation) in the matrix is multiplied by a weight factor, which determines its relative influence on the solution. The same matrix can contain a mixture of Selfcal equations and Redundancy equations, both of which have the same general form. If there are only Redundancy equations, extra constraint equations are needed to supply the missing information about the absolute gain (flux) and/or the absolute phase gradient over the array (position in the sky). 
+<BR><BR>The matrix <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap364.png"> is rectangular because there are more equations than unknowns. A least-squares <b>solution</b> is obtained by the pseudo-inversion of <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap364.png">: 
+<BR><BR><IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap385.png"> 
+<BR><BR>To save space and time, the <i>NEWSTAR </i> implementation uses the much smaller matrix <IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap387.png"> and the vector <IMG ALIGN=BOTTOM ALT="" SRC="_24705_tex2html_wrap389.png">, which is of course mathematically equivalent. </i>
+<P>
+<A NAME=.ncalib.vispace><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/ncalib_vispace.ps"><STRONG>FIGURE</STRONG></A>
+<P>
+ .] A qualitative interpretation of Selfcal, with or without Redundancy constraints. 
+<BR><BR>A perfect instrument would give visibility values that are represented by a point (the <em>true</em> visibilities) in a 2N-dimensional <em>visibility space</em>. N is the number of measured uv-samples. The actual visibility values, which will be corrupted by instrumental errors, are represented by some other point in this space. 
+<BR><BR>In a calibration process, a priori knowledge is used to constrain the volume of visibility space in which this other point can lie.  In Selfcal, the data are compared with a model of the source (model constraints), under the assumption that the only instrumental errors are telescope-based gain and phase errors (instrumental constraints).  The points in visibility space that represent Selfcal Solutions must lie in the shaded volume that is bounded by the <em>model</em> and <em>Selfcal</em> constraints. The technique works because the two constraint volumes are largely 'orthogonal' to each other, so that the intersection volume is relatively small.  Every extra constraint (more telescopes, redundant spacings) will make this intersection volume smaller. 
+<P>
+<A NAME=.redundancy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>   
+<H1><A NAME=SECTION0003000000000000000> <b>Redundancy</b></A></H1>
+<P>
+        Redundancy-only is selected by <b>not</b> specifying a source model. The resulting telescope gain and phase errors are stored in the Scan file headers, as REDC.
+<P>
+**** Put new script here ****
+<P>
+<A NAME=.align><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>   
+<H1><A NAME=SECTION0004000000000000000> <b>Align</b></A></H1>
+<P>
+        Align is selected by specifying a source model, and explicitly specifying the <b>ALIGN_OPTION</b>.  It is then assumed by default that the Scan is `perfect', i.e.  that all 14 telescopes are grouped together.  In that case, only two parameters have to be determined: the absolute gain, and the absolute phase gradient over the array. Experienced users can specify multi-parameter solutions for more than one independent groups of telescopes by manipulating the <b>FORCE_FREEDOM</b> keyword.  The <b>MWEIGHT</b> keywords are used to give greater weight to those baselines (by length), for which the model is `known' to be most accurate.
+<P>
+        The resulting telescope gain and phase corrections are stored in the Scan headers, as ALGC.
+<P>
+*** Put new script here ****
+<P>
+<A NAME=.selfcal><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>   
+<H1><A NAME=SECTION0005000000000000000> <b>Selfcal</b></A></H1>
+<P>
+        Selfcal is selected by specifying a source model, and explicitly specifying `Selfcal' to the <b>ALIGN_OPTION</b>.  Redundancy constraints (equations) are included automatically if redundant spacings have been selected with <b>SELECT_IFRS</b>.  The <b>MWEIGHT</b> keywords are used to give greater weight to those baselines (by length), for which the model is `known' to be most accurate.
+<P>
+        The resulting telescope gain and phase corrections are stored in the Scan headers, as ALGC.
+<P>
+*** Put new script here ****
+<P>
+<A NAME=.log.output><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>   
+<H1><A NAME=SECTION0006000000000000000> <b>Discussion of the screen/log output</b></A></H1>
+<P>
+The following information per HA-scan may be printed in the LOG-file and/or displayed on the terminal screen (keyword <b>SHOW_LEVEL</b>).
+<P>
+		<BR><tt>HA    Rk  A(%) P(deg) A(WU)  P(WU) Amax    Aavg   Arms    dAmax   
+dPmax  I</tt>
+<P>
+		<BR><tt>Set: 0.0.0.0</tt>
+<P>
+		<BR><tt>11.53X New phase constraints:</tt>
+<P>
+		<BR><tt>1   1   1   1   1   1   1   1   1   1   1   1   1   1</tt>
+<P>
+		<BR><tt>11.53X 01   0.6   0.2   12.9    7.1  2012  2000.0   5.2    1.9 67 0.5 58 3</tt>
+<P>
+		 <BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap372.png">
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tabbing169.png"><P>
+<P>
+		<BR><tt>X average amplitude= 2000.005 (0.892)</tt>
+<P>
+		<BR><tt>X overall noise (gain, phase in W.U.):     14.2     11.1</tt>
+<P>
+<UL><LI>   <b>Average amplitude:</b>
+<P>
+<LI>   <b>Average gain and phase errors per telescope:</b>   
+        Over the whole observation (or rather, the part that has just been processed). These numbers can also be calculated separately by means of NCALIB option SHOW.
+<P>
+<LI>   <b>Overall noise:</b>   
+        Useful for automatic deletion of `bad' scans (see NSCAN). Redundancy-only is model-independent, so the overall noise should be equal to the thermal noise. If not, it is an indication of problems. A difference between SELFCAL noise and Redundancy-only noise is an  indication of the completeness of the SELFCAL model (caution: there are different interferometers involved).
+<P>
+<LI>   <b>Graphs:</b>   
+        There are three kinds of line-printer graphs produced in the log-file. They give various overall gain and phase quantities per interferometer. The baseline length increases to the right. The gain axis (A) is on the left, and the phase axis (P) on the right.   
+  <UL><LI> <b>Graph: Average residual error X (W.U.):</b>   
+  <LI> <b>Graph: Average residual error X (%, deg):</b>   
+  <LI> <b>Graph: RMS X (W.U.):</b>   
+  </UL> </UL>
+<P>
+        The SELFCAL and Redundancy residuals contain a wealth of information about the quality of the data and the completeness of the SELFCAL model. The user is urged to make residual plots by means of the program NPLOT.
+<P>
+<A NAME=.qdetails><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>   
+<H1><A NAME=SECTION0007000000000000000> <b>QDETAILS: Hidden parameters</b></A></H1>
+<P>
+        For all REDUN options, the user is prompted for `more details?' by the NCALIB keyword QDETAILS.  Hidden behind this are a number of keywords that may be manipulated by experienced users in special cases. Their default values are optimised for normal use, and wil be printed in the NCALIB LOG-file.
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>BASEL_CHECK</b>   
+ (M)   
+ = 0.5 M:   
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap439.png">   
+<BR><i>Criterion for two baselines to be considered redundant, i.e. of identical length.</i>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>WEIGHT_MIN</b>   
+ (Minimum weight accepted)   
+ = 0.01:   
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap441.png">   
+<BR><i>The weight of Selfcal and Redundancy equations is proportional to the amplitude of their uv-data. If the amplitude is very small, the information will be very noisy, and may do more harm than good to the solution. Therefore, it may be excluded by raising the value of WEIGHT_MIN, as a fraction of the maximum weight.</i>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>SOLVE</b>   
+ (Solve for gain, phase (Y/N)   
+ = YES,YES:   
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap443.png">   
+<BR><i>Normally, both a gain and a phase solution will be required. But it is possible to ask for only one at a time.</i>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>COMPLEX</b>   
+ (Complex solution (Y/N)   
+ = NO:   
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap445.png">   
+<BR><i>The non-linear conversion to gain and phase skews the gaussian distribution of the noise on the measured cos/sine values. Therefore, gain and phase solutions will produce a `noise bias', which is more serious for low S/N data. This can be avoided by specifying a `complex solution' (see also section   
+...)</i>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>FORCE_PHASE</b>   
+ ()   
+ = 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0    
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap447.png">   
+<BR><i>If the visibility phases are close to <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap404.png">, the conversion from cos/sine to phase may cause phase ambiguities (jumps) of 360 degr. This will cause problems in the phase solution, where the phases are assumed to be on a linear scale between <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap406.png">. In order to avoid this, the user may specify initial phase corrections for all telescopes, which will be used to move the data away from <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap404.png"> before processing. This is of course taken into account for the total correction afterwards.</i>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>CONTINUITY</b>   
+ (Continuity in solution (Y/N)   
+ = YES:   
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap449.png">   
+<BR><i>Normally, the HA-scans are processed in HA-order. The gain and phase errors determined for the last Scan may be used to correct the data of the next Scan <em>before</em> processing. (This is of course taken into account for the total correction afterwards).  This approach is useful to keep phases away from <IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap404.png">, where they may cause unwanted phase-ambiguity problems.</i>
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_9871_tex2html_wrap410.png"> <b>CHECKS</b>   
+ (Maximum deviations)   
+ = 5,5,3:   
+ <IMG ALIGN=BOTTOM ALT="" SRC="_19828_tex2html_wrap451.png">   
+<BR><i>The user may set some threshold values for an automatic check on the quality of the solution of each HA-scan. A warning will be issued in the log whenever the tresholds are exceeded. However, no further action is taken by the program!</i>
+<P>
+
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+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ncalib_vzero.txt b/ncalib_vzero.txt
new file mode 100644
index 0000000000000000000000000000000000000000..d2b9347543be8855aea80f016bedc91690398e36
--- /dev/null
+++ b/ncalib_vzero.txt
@@ -0,0 +1,82 @@
+The VZERO algorithm	- JPH 960212
+
+Summary
+-------
+	Following a query by Jayaram Chengalur, this note provides an exegesis of W.N. Brouw's algorithm for determining the phase-zero-difference ('PZD') between the XX and YY interferometer subsets as implemeneted in the Newstar program NCALIB. The 180-degree ambiguity suggested by Chengalur appears indeed to exist; I suggest that a check could be implemented to insure selection of the  proper value for the PZD.
+				-------------
+
+
+Brouw's algorithm
+-----------------
+	I reproduce here the relevant lines of code from the program module NCAPVZ where the PZD is calculated:
+
+
+ 1	    DO I1=0,STHJ(STH_NIFR_J)-1			!ALL IFRS
+ 2	      IF (WGT(I1,1).GT.0 .AND. WGT(I1,2).GT.0 .AND. !XY/YX PRESENT
+ 3	1		ABS(DATC(I1,2)).NE.0) THEN	!SOME POWER
+ 4		CF=1					!COEFFICIENT
+ 5		CW=-DATC(I1,2)*DATC(I1,1)		!-YX.XY
+ 6		R0=ABS(CW)				!WEIGHT
+ 7		IF (R0.NE.0)
+ 8	1		CALL WNMLMN(MAR,LSQ_C_COMPLEX,CF,R0,
+ 9	1			(DATC(I1,2)-CONJG(DATC(I1,1)))/SQRT(CW))
+			.
+			solve 
+			.
+	IF (ABS(CSOL).NE.0) THEN
+10	  XYDIF=ATAN2(AIMAG(CSOL),REAL(CSOL))		!GET ANGLE
+	ELSE
+	  XYDIF=0
+	END IF
+11	CALL WNCTXT(F_TP,'A complex angle of !EC9.2\(!EC9.2) '//
+	1		'or !EAR9.2 degrees',
+	1		CSOL,CME,XYDIF)
+C
+
+	1: Process all interferometers, I1 = interferometer index
+	2: DATC = cpomplex visibility, WGT = weight; the first index is the 
+	   interferometer number, second index is 1 for XY, 2 for YX. Check 
+	   validity of data: if weight WGT equals 0, point has been deleted.	
+	3: This check seems to be redundant: If either XY or YX is 0, so will 
+	   be R0 in line 6 and consequently lines 8 and 9 will be skipped.
+	5: CW = -XY.YX
+	6: R0 = weight of this interferometer in the solution.
+	7: If the weight is 0, bypass lines 8 and 9 including the division by
+	   sqrt(CW).
+	8: Accumulate sum of (XY-YX*)/sqrt(-XY.YX) with weights |XY.YX|.
+	10: The result is a complex number, the weighted average of the 
+	   quantities of line 9 over all interferometers; its argument is the 
+	   phase difference we were after.
+	11: The test displaying this result is a bit sloppy!
+ 
+So the quantity that is averaged (line 8) is
+
+		P = sqrt(XY/YX) - sqrt(YX*/YX).sqrt(YX/XY)
+
+
+Interpretation
+--------------
+
+	I suggest the following interpretation:
+
+We seek to minimise |V| by multiplying X with a factor a.e^(i.phi), so
+
+		YX' = YX.a^2.e^(2i.phi)
+
+making
+
+		P' = sqrt(XY/YX) - a.e^(i.phi).sqrt(YX/XY)
+
+Setting P' = 0 gives us 
+
+		a.e^(i.phi) = sum[sqrt(XY/YX)] / sum[sqrt(YX/XY)]
+
+The amplitude factor a should be 1 after XX and YY Selfcal, and could be used for a consistency check. NCALIB implicity displays its value by printing out a.e^(i.phi) as a 'complex angle', but otherwise ignores it. 
+
+
+The PZD ambiguity
+-----------------
+ 
+	The 180-degree ambiguity in the VZERO determination noted by Chengalur is represented in the algorithm above by the sign ambiguity of the sqrt() function. 
+
+	It seems to me that whatever algorithm one uses, there is probably no way to avoid the appearance in one form or another of a factor 2 on the unknown phase phi. This means that one must check afterwards in some way that the algorithm selected the right value; for a calibrator there should be enough flux in a single scan to do this straightaway.  
diff --git a/nclean/nclean__ the.html b/nclean/nclean__ the.html
new file mode 100644
index 0000000000000000000000000000000000000000..792b092f72def55833a9a6535b2f62a85d26207d
--- /dev/null
+++ b/nclean/nclean__ the.html	
@@ -0,0 +1,13 @@
+<TITLE>Description of  the (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword  the</H1> 
+
+<DT><EM>Prompt:</EM> ONE input map: grp.fld.chn.pol.0.seq
+<DT><EM>Expected input:</EM> Character(32), 1 values.<P>
+Specify ONE input map (group.field.channel.polar.type(=0).sequence_number) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__ap_wmp_set.html b/nclean/nclean__ap_wmp_set.html
new file mode 100644
index 0000000000000000000000000000000000000000..aa6925bcc9d78b6d66ff5f4a65b3580213b96464
--- /dev/null
+++ b/nclean/nclean__ap_wmp_set.html
@@ -0,0 +1,15 @@
+<TITLE>Description of AP_WMP_SET (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword AP_WMP_SET</H1> 
+
+<DT><EM>Prompt:</EM> ONE antenna pattern (grp.fld.chn.pol.1.seq)
+<DT><EM>Expected input:</EM> Character(32), 1 values.<P>
+Specify ONE antenna pattern 
+                (group.field.channel.polarisation.type(=1).sequence_number) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI>Description of the <A HREF="../wmp_descr/wmp_descr.html">WMP file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__area.html b/nclean/nclean__area.html
new file mode 100644
index 0000000000000000000000000000000000000000..6c3a82ac358cd288081ebba13ecda8eff16cb403
--- /dev/null
+++ b/nclean/nclean__area.html
@@ -0,0 +1,21 @@
+<TITLE>Description of AREA (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword AREA</H1> 
+
+<DT><EM>Prompt:</EM> Window area l, m, dl, dm
+<DT><EM>Expected input:</EM> Integer number, 4 values.<P>
+The CLEAN window is defined as the union of up to 32 rectangular areas (which 
+may arbitrarily overlap). For BEAM clean this is also the window within which 
+source responses will be subtracted. <P>
+You are being prompted for these areas one by one until you give a null reply 
+(&lt;CR&gt; only). An area is specified by four numbers: l, m, dl, dm, where <P>
+   l, m     l and m in grid points for the area centre; (l, m)=(0, 0) at the map 
+            centre, increasing toward the upper right (i.e. with decreasing RA 
+            and increasing DEC) 
+   dl, dm   width and height of the area in grid points  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__clean_limit.html b/nclean/nclean__clean_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..0bed437b95335b6b1315fe587866822b246572d6
--- /dev/null
+++ b/nclean/nclean__clean_limit.html
@@ -0,0 +1,14 @@
+<TITLE>Description of CLEAN_LIMIT (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword CLEAN_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Limit in fraction of map maximum
+<DT><EM>Default:</EM> .1 /ASK.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000010; max.value: 1.000000.<P>
+Specify the level to which to clean in fraction of the initial map maximum. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__clip_area.html b/nclean/nclean__clip_area.html
new file mode 100644
index 0000000000000000000000000000000000000000..20b3db7f3471dc1c7ce99390da1d1ba47ec0f76c
--- /dev/null
+++ b/nclean/nclean__clip_area.html
@@ -0,0 +1,15 @@
+<TITLE>Description of CLIP_AREA (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword CLIP_AREA</H1> 
+
+<DT><EM>Prompt:</EM> UV-radius range for clipping (m)
+<DT><EM>Default:</EM> 0., 100000..
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.000000.<P>
+Specify the (circular) UV-plane radii (in metres) between which you want to 
+clip the data. The default is to clip everywhere. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__clip_levels.html b/nclean/nclean__clip_levels.html
new file mode 100644
index 0000000000000000000000000000000000000000..afc0581567eda2c62387e8b5dee5260a1014e879
--- /dev/null
+++ b/nclean/nclean__clip_levels.html
@@ -0,0 +1,23 @@
+<TITLE>Description of CLIP_LEVELS (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword CLIP_LEVELS</H1> 
+
+<DT><EM>Prompt:</EM> Amplitude range to be discarded
+<DT><EM>Default:</EM> 100000., 100000..
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify amplitude range (in Westerbork Units) of visibility magnitudes that you 
+want to discard. <P>
+In the annulus defined by CLIP_AREA, values between the limits you specify will 
+be discarded. 
+! {\em parameter \textref{CLIP_AREA}{.clip.area} } <P>
+NOTE: It would be more natural to define a range within which visibilities are 
+considered valid. As it is, only the lower limit is actually useful, allowing 
+you to define a rejection threshold for interference. To do so, specify your 
+threshold for the lower and 'infinity' for the upper limit, e.g. <P>
+                &lt;threshold&gt;, 100000  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__cmemory_use.html b/nclean/nclean__cmemory_use.html
new file mode 100644
index 0000000000000000000000000000000000000000..6e2edc04fa9fad87a5bc20f69cc745a71bf9e3d5
--- /dev/null
+++ b/nclean/nclean__cmemory_use.html
@@ -0,0 +1,19 @@
+<TITLE>Description of CMEMORY_USE (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword CMEMORY_USE</H1> 
+
+<DT><EM>Prompt:</EM> UV-clean memory size
+<DT><EM>Default:</EM> 150000 /NOASK.
+<DT><EM>Expected input:</EM> Integer number; min.value: 32000.000000; max.value: 128000000.000000.<P>
+Specify the work memory size in bytes for the UV Clean option, to be allowed in 
+defining the beam patch and to be used in executing the Fourier transforms. <P>
+The default shown is normally adequate; a larger value may speed up the 
+execution of major cycles in UV Clean. 
+!. 
+!NCLEAN will not accept a value in excess of 32000000 (32 MB). 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__compon_limit.html b/nclean/nclean__compon_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..7ec9d02c64f8d6d8c762fe7ec61f1c674320301f
--- /dev/null
+++ b/nclean/nclean__compon_limit.html
@@ -0,0 +1,14 @@
+<TITLE>Description of COMPON_LIMIT (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword COMPON_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Maximum number of components to find
+<DT><EM>Default:</EM> 100 /ASK.
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000; max.value: 100000.000000.<P>
+Specify the maximum number of components to be cleaned. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__compon_log.html b/nclean/nclean__compon_log.html
new file mode 100644
index 0000000000000000000000000000000000000000..10a1e6506877812e9e801527a3f85f335e114170
--- /dev/null
+++ b/nclean/nclean__compon_log.html
@@ -0,0 +1,18 @@
+<TITLE>Description of COMPON_LOG (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword COMPON_LOG</H1> 
+
+<DT><EM>Prompt:</EM> Reporting interval for components found: | terminal, printer
+<DT><EM>Expected input:</EM> Integer number, 2 values; min.value: 0.000000.<P>
+You may give two numbers &lt;n&gt; here, indicating that every &lt;n&gt;-th component must 
+be reported. The first number applies to your terminal window, the second to 
+the log file. A value of 0 means 'no reporting at all. <P>
+Example: 
+        2, 0 specifies that every other component will be typed, and none 
+logged.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__cycle_depth.html b/nclean/nclean__cycle_depth.html
new file mode 100644
index 0000000000000000000000000000000000000000..707696de6edfd36c576ef99c59e366575e7da0f1
--- /dev/null
+++ b/nclean/nclean__cycle_depth.html
@@ -0,0 +1,15 @@
+<TITLE>Description of CYCLE_DEPTH (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword CYCLE_DEPTH</H1> 
+
+<DT><EM>Prompt:</EM> Major cycle depth
+<DT><EM>Default:</EM> .05 /ASK.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.001000; max.value: 1.000000.<P>
+Specify the level relative to the initial map maximum in the CLEAN window to 
+which you want to clean in one major cycle. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__data_factor.html b/nclean/nclean__data_factor.html
new file mode 100644
index 0000000000000000000000000000000000000000..473adc558b0264f5815698519b2c4c090e4a2cc8
--- /dev/null
+++ b/nclean/nclean__data_factor.html
@@ -0,0 +1,16 @@
+<TITLE>Description of DATA_FACTOR (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword DATA_FACTOR</H1> 
+
+<DT><EM>Prompt:</EM> Data multiplication factor
+<DT><EM>Default:</EM> 1. /ASK.
+<DT><EM>Expected input:</EM> Real number.<P>
+Specify the factor by which to multiply the input map-data. <P>
+This option is only relevant for DATA clean. The first input-map and all maps 
+created by DATA clean will be multiplied by this factor. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__deconvolution.html b/nclean/nclean__deconvolution.html
new file mode 100644
index 0000000000000000000000000000000000000000..b2e8f70aa5896e5b19f1ee30c2cd2056a68d8ac8
--- /dev/null
+++ b/nclean/nclean__deconvolution.html
@@ -0,0 +1,20 @@
+<TITLE>Description of DECONVOLUTION (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword DECONVOLUTION</H1> 
+
+<DT><EM>Prompt:</EM> Correct antenna pattern for mapping taper: YES/NO
+<DT><EM>Default:</EM> NO /NOASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+The gridding convolution in map-making is usually compensated for by 
+multiplying the output map and antenna pattern with a taper function that rises 
+toward the map edges. <P>
+If this is the case, answering YES here will instruct the program to account 
+for this effect; this will reduce the aliasing errors in the residual map,  
+allowing you to clean a somewhat larger part of the map. YES will in general 
+produce a result with less aliasing, NO the reverse. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__dmemory_use.html b/nclean/nclean__dmemory_use.html
new file mode 100644
index 0000000000000000000000000000000000000000..26d7d7d94960fa6e229b72c602f73dcb63443db8
--- /dev/null
+++ b/nclean/nclean__dmemory_use.html
@@ -0,0 +1,19 @@
+<TITLE>Description of DMEMORY_USE (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword DMEMORY_USE</H1> 
+
+<DT><EM>Prompt:</EM> Work memory size
+<DT><EM>Default:</EM> 300000.
+<DT><EM>Expected input:</EM> Integer number; min.value: 32000.000000; max.value: 32000000.000000.<P>
+The memory workspace in bytes needed is 12 times the size of the rectangle 
+enclosing all selected areas in the map plane. NCLEAN normally allocates up to 
+300 KB for this purpose. To satisfy the present need, you must either accept 
+the value suggested here or specify a smaller set of areas, or both. 
+!. 
+!NCLEAN will not accept a value in excess of 32000000 (32 MB). 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__grating_factor.html b/nclean/nclean__grating_factor.html
new file mode 100644
index 0000000000000000000000000000000000000000..814cb0b5b4707f65e09e3a27a7341ab722b73604
--- /dev/null
+++ b/nclean/nclean__grating_factor.html
@@ -0,0 +1,20 @@
+<TITLE>Description of GRATING_FACTOR (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword GRATING_FACTOR</H1> 
+
+<DT><EM>Prompt:</EM> Grating factor
+<DT><EM>Default:</EM> 1. /ASK.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+In the minor cycles of UVCOVER, DATA and COMPON clean, the maximum error made 
+in only subtracting part of the antenna pattern is estimated by &lt;number of 
+sources&gt; times &lt;ypical sidelobe level in antenna pattern&gt; times GRATING_FACTOR. <P>
+You may lower this latter factor if you are not worried about the effects of 
+far-out sidelobes on the minor-cycle cleaning process. A lower value will allow 
+more source components to be collected in minor cycles before a major cycle 
+must be started. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__loop_gain.html b/nclean/nclean__loop_gain.html
new file mode 100644
index 0000000000000000000000000000000000000000..2acfa977d89112e4658a864423b03dfddce0f3fb
--- /dev/null
+++ b/nclean/nclean__loop_gain.html
@@ -0,0 +1,17 @@
+<TITLE>Description of LOOP_GAIN (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword LOOP_GAIN</H1> 
+
+<DT><EM>Prompt:</EM> Clean loop-gain factor
+<DT><EM>Default:</EM> .4 /ASK.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.010000; max.value: 1.000000.<P>
+For each component found, the antenna pattern shifted to its position is 
+subtracted from the CLEAN window. To prevent overshoots, it is customary to 
+subtract not the complete component but only a fraction of it. The magnitude of 
+this fraction is defined here.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__map_factor.html b/nclean/nclean__map_factor.html
new file mode 100644
index 0000000000000000000000000000000000000000..0db960a47bf586dec55c2d4a22b927b42e0fa379
--- /dev/null
+++ b/nclean/nclean__map_factor.html
@@ -0,0 +1,16 @@
+<TITLE>Description of MAP_FACTOR (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword MAP_FACTOR</H1> 
+
+<DT><EM>Prompt:</EM> Multiplication factor
+<DT><EM>Default:</EM> 1. /ASK.
+<DT><EM>Expected input:</EM> Real number.<P>
+Specify the factor by which to multiply the residual map before restoring. <P>
+Normally one should use the default value of 1; a value of 0 serves to make a 
+map of the CLEAN components only. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__option.html b/nclean/nclean__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..b992ee3d90561559e94207ee1834bd6d74bcc067
--- /dev/null
+++ b/nclean/nclean__option.html
@@ -0,0 +1,43 @@
+<TITLE>Description of OPTION (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> BEAM, UVCOVER, DATA, UREST; COMPON, HISTO; QUIT Operation wanted
+<DT><EM>Expected input:</EM> Character(24).<P>
+CLEANing: <P>
+   BEAM         Hogbom clean: Use the map and the beam to clean. This 
+                 method is inaccurate away from the map centre due to the 
+                 aliasing associated with visibility gridding. <P>
+   UVCOVER      Standard Clark Clean: Find and provisionally subtract sources 
+                 in some map areas first (minor cycles), then properly subtract 
+                 the sources found (major cycle). The number of minor cycles 
+                 between major cycles is determined by the program; the user can 
+                 steer this through a few control parameters. 
+                The method suffers from the same limitations as BEAM, but is 
+                 faster for cleaning extended sources. <P>
+   DATA         Cotton-Schwab Clean: Find sources as in UVCOVER, but perform 
+                 the major cycle on the original SCN-file visibilities, making a 
+                 new map from the residuals as input for the next major cycle. 
+                 This method rigorously avoids the aliasing limitations of BEAM 
+                 and UVCOVER, at the price of being very much slower. <P>
+   UREST        Use a clean component list and a map to restore the clean 
+                 components in the map. <P>
+For exploring the data before committing more serious work: <P>
+   HISTO        Produce only a histogram of selected areas in the map and/or 
+                 antenna pattern <P>
+   COMPON       Execute minor cycles as for UVCOVER, but omit the following 
+                 major cycle. The result is a source model and a map in which 
+                 these sources are provisionally subtracted in selected areas. 
+                It is the fastest of the four CLEAN variants but produces an 
+                 inaccurate residual map. 
+                This option may be used to quickly get a feel for the 
+                 minor-cycle control of UVCOVER and DATA Clean, or to make an 
+                 initial data model for NCALIB SELFCAL or NMODEL UPDATE. <P>
+Other options: <P>
+   QUIT          Terminate NCLEAN. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__prussian_hat.html b/nclean/nclean__prussian_hat.html
new file mode 100644
index 0000000000000000000000000000000000000000..23583d007660dfae36c59dff23e7fbc5e7d8e6b2
--- /dev/null
+++ b/nclean/nclean__prussian_hat.html
@@ -0,0 +1,15 @@
+<TITLE>Description of PRUSSIAN_HAT (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword PRUSSIAN_HAT</H1> 
+
+<DT><EM>Prompt:</EM> Prussian hat value
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000; max.value: 0.500000.<P>
+For extended sources a prussian hat (i.e. a nominal additional peak value on 
+the central value of the antenna pattern) may give better clean results. Values 
+of .1 to .4 could be tried. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__residual.html b/nclean/nclean__residual.html
new file mode 100644
index 0000000000000000000000000000000000000000..31d0d19d3fbf2937622425212f4a4e0bc2596167
--- /dev/null
+++ b/nclean/nclean__residual.html
@@ -0,0 +1,20 @@
+<TITLE>Description of RESIDUAL (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword RESIDUAL</H1> 
+
+<DT><EM>Prompt:</EM> residual map?
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if the residual map must be written. <P>
+For BEAM and UVCOVER cleaning, this map is an automatic by-product of the 
+process and the choice is whether or not to write it to the .WMP file. The map 
+will be given the same indices as the input map except for an incremented 
+sequence number. <P>
+For UVDAT cleaning, the residual map must be constructed by making a new map 
+from the original visibilities, in which the CLEAN components just found are 
+subtracted. The new map will OVERWRITE the input map. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__restore.html b/nclean/nclean__restore.html
new file mode 100644
index 0000000000000000000000000000000000000000..07a8833d897c04ce70804b796dcf9dbe084a6368
--- /dev/null
+++ b/nclean/nclean__restore.html
@@ -0,0 +1,19 @@
+<TITLE>Description of RESTORE (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword RESTORE</H1> 
+
+<DT><EM>Prompt:</EM> restored map (YES/NO)?
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if a restored map must be written. <P>
+A restored map consists of the CLEAN components convolved with a hypothetical 
+beam that has no sidelobes, superimposed on the residuals. It is an 
+approximation to  what you would have observed with complete contiguous UV 
+coverage (hoth in hour angle and baseline) up to the longest baseline available. <P>
+You will be given the option to suppress the residuals (parameter MAP_FACTOR),  
+in which case you get a map of the CLEAN components only. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__restore_beam.html b/nclean/nclean__restore_beam.html
new file mode 100644
index 0000000000000000000000000000000000000000..25e1e593d975f2b9870799b21b99ebe72c1bc239
--- /dev/null
+++ b/nclean/nclean__restore_beam.html
@@ -0,0 +1,21 @@
+<TITLE>Description of RESTORE_BEAM (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword RESTORE_BEAM</H1> 
+
+<DT><EM>Prompt:</EM> dl, dm arcsec, pa deg
+<DT><EM>Expected input:</EM> Real number, 3 values.<P>
+Specify the restore beam width: <P>
+   dl      width of beam in arcsec (full-halfwidth) <P>
+   dm      width of beam in arcsec (full-halfwidth) <P>
+   pa      position angle of skewed beam in degrees (anti-clockwise; 
+            0 deg is horizontally to the right (+l direction) <P>
+The default beam is a two-dimensional Gaussian truncated at a level of .xx 
+relative to the maxiumum. If an antenna pattern for your map is available, the 
+l, m beam widths are derived from it; else a rule-of-thumb formula is used: <P>
+        half-width = 12 arcsec * 1400/frequency(MHz)  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nclean/nclean__wmp_sets0.html b/nclean/nclean__wmp_sets0.html
new file mode 100644
index 0000000000000000000000000000000000000000..76d4e5e360544c90b3d9573ddac588703e39ecbd
--- /dev/null
+++ b/nclean/nclean__wmp_sets0.html
@@ -0,0 +1,14 @@
+<TITLE>Description of WMP_SETS0 (NCLEAN)</TITLE>
+<H1>Program NCLEAN: private keyword WMP_SETS0</H1> 
+
+<DT><EM>Prompt:</EM> ONE input map: grp.fld.chn.pol.0.seq
+<DT><EM>Expected input:</EM> Character(32), 1 values.<P>
+Specify ONE input map (group.field.channel.polar.type(=0).sequence_number) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nclean/nclean_keys.html">List of keywords</A> for NCLEAN
+<LI>Description of the <A HREF="../wmp_descr/wmp_descr.html">WMP file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
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new file mode 100644
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@@ -0,0 +1,1446 @@
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diff --git a/nclean_descr/images.pl b/nclean_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nclean_descr/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nclean_descr/labels.pl b/nclean_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..422d289955f627fbb994384256eaba881beabefc
--- /dev/null
+++ b/nclean_descr/labels.pl
@@ -0,0 +1,18 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".missing"} ="$URL/nclean_descr.html"; 
+$external_labels{".beam.clean"} ="$URL/nclean_descr.html"; 
+$external_labels{".nclean.interface"} ="$URL/nclean_descr.html"; 
+$external_labels{".overview"} ="$URL/nclean_descr.html"; 
+$external_labels{".cycle.depth"} ="$URL/nclean_descr.html"; 
+$external_labels{".residual.maps"} ="$URL/nclean_descr.html"; 
+$external_labels{".contents"} ="$URL/nclean_descr.html"; 
+$external_labels{".uv.clean"} ="$URL/nclean_descr.html"; 
+$external_labels{".nclean.versus"} ="$URL/nclean_descr.html"; 
+$external_labels{".prussian.hat"} ="$URL/nclean_descr.html"; 
+$external_labels{".data.clean"} ="$URL/nclean_descr.html"; 
+$external_labels{".compon"} ="$URL/nclean_descr.html"; 
+$external_labels{".grating.factor"} ="$URL/nclean_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/nclean_descr/nclean_descr.html b/nclean_descr/nclean_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..7e995508fb2327c232838cf63c8c1f62086cfc2b
--- /dev/null
+++ b/nclean_descr/nclean_descr.html
@@ -0,0 +1,185 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The program NCLEAN</b>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nclean_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nclean_descr.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nclean_descr.html#SECTION0003000000000000000>  <b>NCLEAN versus NMODEL FIND</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nclean_descr.html#SECTION0003100000000000000>  <b>Beam Clean = H&#246;gbom Clean</b></A>
+<LI> <A NAME=tex2html5 HREF=nclean_descr.html#SECTION0003200000000000000>  <b>UV Clean = Clark Clean </b></A>
+<LI> <A NAME=tex2html6 HREF=nclean_descr.html#SECTION0003300000000000000>  <b>Data clean = Cotton-Schwab Clean</b></A>
+<LI> <A NAME=tex2html7 HREF=nclean_descr.html#SECTION0003400000000000000> <b>&quot;Component&quot; clean: A quick-and dirty Clean</b></A>
+</UL> 
+<LI> <A NAME=tex2html8 HREF=nclean_descr.html#SECTION0004000000000000000>  <b>Residual maps</b></A>
+<LI> <A NAME=tex2html9 HREF=nclean_descr.html#SECTION0005000000000000000> <b>Missing items to be added</b></A>
+</UL>
+<A NAME=.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        NCLEAN is a relatively simple implementation of a number of Clean algorithms.  According to its writer (WNB), more elaborate and versatile implementations exist in AIPS and GIPSY.
+<P>
+        NCLEAN makes extensive use of the 
+<A HREF="../nmodel_descr/nmodel_descr.html"><em>source model</em></A> facilities. A source model is a list of source components.  The user has considerable latitude in manipulating such models; for example, NCLEAN allows one to restore source components that were inserted in the model by mechanisms other than Clean and are not on grid points.  Since it is left to the user to decide what is &quot;correct&quot; and what not, such facilities should be used only by experts and with caution.
+<P>
+<A NAME=.nclean.interface><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the actions in NCLEAN. } 
+<A HREF="../fig/nclean_interface.ps"><STRONG>FIGURE</STRONG></A> 
+ .]{<i><A HREF=" #.nclean.interface">Figure</A> shows an overview of the options available in NCLEAN.  The program's basic Clean function is implemented in several forms to be discussed below.  In addition, there is a separate option to restore a map from a source model in a 
+<A HREF="../nmodel_descr/nmodel_descr.html"><em>MDL file</em></A>, and an option to produce a histogram of the intensities of a collection of map areas.
+<P>
+        The components found are stored in a source model in core. NCLEAN will ask the user for an MDL file to store the list; if he specifies none, the 
+<A HREF="../nmodel_descr/nmodel_descr.html"><em>NMODEL HANDLE</em></A> process will be activated to process the list.
+<P>
+<A NAME=.nclean.versus><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+</i><H1><A NAME=SECTION0003000000000000000>  <b>NCLEAN versus NMODEL FIND</b></A></H1>
+<P>
+        The Clean algorithm is fundamentally limited by its basic paradigm, <em>viz.</em> attempting to represent a continuous brightness contribution as a superposition of point sources on map-grid points. This approach is inadequate for small sources if dynamic ranges in excess of, say, 1000 are aimed for.
+<P>
+        On the other hand, Clean is the only mechanism available to construct models for extended sources that cannot be adequately represented by a model with at most a few parameters. Note, however, that Clean has difficulty guessing the missing information for extended sources which results in the notorious problem of <em>corrugations. Modifications to Clean's search algorithm have proved succesful in suppressing these corrugations (whichref&quot;SDI Clean&quot;), but they are not available in NCLEAN.
+<P>
+        As an alternative, Newstar has the option of FINDing sources with the program <A HREF="../nmodel_descr/nmodel_descr.html">NMODEL</A>.  This method is superior for sources of small extent, since it does not confine their positions to be on grid points and desribes their shapes in terms of an ellipse with three parameters (axes and orientation).  In doing this, FIND can also take the effects of bandwidth smearing and finite integration time into account.
+<P>
+        FIND is therefore the recommended way of building models of small sources.  Cleaning must be used for sources that do not fit the shape restrictions on FIND sources.  Obviously, Clean and FIND may have to be used in combination, in such a way that all source components in the model take the form that best fits their real appearance.
+<P>
+<A NAME=.beam.clean><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+</em><H2><A NAME=SECTION0003100000000000000>  <b>Beam Clean = H&#246;gbom Clean</b></A></H2>
+<P>
+        H&#246;gbom's original <b>Clean method is known in Newstar as <b>Beam Clean</b>.  It consists of repeatedly finding the highest point in (part of) a map (the <em>search area</em>) and subtracting a source component at that position from the entire map or some part of it (the <em>clean area</em>). The subtracted component consists of the antenna pattern shifted and multiplied by the peak intensity of the source and a <em>gain factor</em>.  This factor is usually chosen somewhat smaller then 1 to account for the fact that part of the intensity found may be due to sidelobes from other sources.
+<P>
+        The subtraction may be problematic in cases where the shifted antenna pattern does not cover the entire clean area.  Moreover, the edges of both the map and the antenna pattern are contaminated by aliasing effects.  For this reason cleaning is best restricted to an area somewhat less than the central half of the map in both dimensions.
+<P>
+        In the NEWSTAR version, the search area coincides with the clean area. It is defined as the union of at most 32 rectangles specified by the user. Since subtraction occurs only in the search area, sidelobes in the remainder of the map are not removed.  It is therefore not advisable to successively clean different areas; nor is it necessary, since NCLEAN allows you to specify all relevant areas simultaneously.
+<P>
+        H&#246;gbom Clean is controlled by the parameters
+<P>
+<UL><LI>   <A HREF="../nclean_private_keys/nclean_private_keys.html#.loop.gain"><b>LOOP_GAIN</b></A>: the gain factor;
+<P>
+<LI>   <A HREF="../nclean_private_keys/nclean_private_keys.html#.compon.limit"><b>COMPON_LIMIT</b></A>: the number of source components at which the process will stop;
+<P>
+<LI>   <A HREF="../nclean_private_keys/nclean_private_keys.html#.clean.limit"><b>CLEAN_LIMIT</b></A>: the absolute maximum intensity in the residual map at which the process will stop;
+<P>
+<LI>   <A HREF="../nclean_private_keys/nclean_private_keys.html#.area"><b>AREA</b></A> (prompt repeats until a null answer is given): the map areas in which source components are looked for 
+and subtracted. </UL>
+<P>
+<A NAME=.prussian.hat><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+        An additional parameter, 
+<A HREF="../nclean_private_keys/nclean_private_keys.html#.prussian.hat"><b>PRUSSIAN_HAT</b></A>, allows one to stick a delta-function peak on the centre of the antenna pattern, which in certain cases gives better results (Cornwell ...).
+<P>
+<A NAME=.uv.clean><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+</b><H2><A NAME=SECTION0003200000000000000>  <b>UV Clean = Clark Clean </b></A></H2>
+<P>
+        <b>UV Clean</b>, more hgenerally known as <b>Clark Clean speeds up the cleaning of extended sources which must be represented by a large number of closely spaced point-source components. Sources are found in the same way as for H&#246;gbom Clean.  But rather than subtracting them one by one in the entire search area, Clark Clean does only a provisional subtraction in a small <em>patch</em> around the source position.  Proper subtraction is done later by jointly convolving the sources collected with the antenna pattern and subtracting the result.
+<P>
+        The convolution is implemented through Fourier transformations and a multiplication in the visibility plane, which is considerably faster than a direct convolution in the map domain.  However, this method suffers from aliasing errors similar to those for Beam Clean and is therefore subject to the same limitations.
+<P>
+        In UV Clean <em>minor cycles</em>, in each of which a single source component is located and provisionally subtracted, alternate with <em>major cycles</em> in which the newly found sources are properly removed. The number of minor cycles between successive major cycles is controlled by an algorithm that estimates the buildup of deviations in the residual map due to the provisional nature of component subtractions.  The user has a few parameters to control this algorithm.
+<P>
+        UV Clean is controlled by the same parameters as H&#246;gbom Clean. In addition, the number of minor cycles to a major one is controlled by the parameters:
+<P>
+<UL><A NAME=.cycle.depth><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<LI>   <A HREF="../nclean_private_keys/nclean_private_keys.html#.cycle.depth"><b>CYCLE_DEPTH</b></A>: The lower limit to components to be found in minor cycles relative to the present absolute residual-map maximum.
+<P>
+<A NAME=.grating.factor><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<LI> <A HREF="../nclean_private_keys/nclean_private_keys.html#.grating.factor"><b>GRATING_FACTOR</b></A>: A multiplier to be applied to the estimate of the maximum error buildup in the minor cycles.  The default of 1 is supposed to guarantee that grating responses will not erroneously be mistaken for source components.  A lower value allows a larger number of minor cycles per major cycle, but should be used only to the extent that there is no danger of mistakes. The <A HREF="#.compon"><b>COMPON</b></A> clean option can be used to explore this effect prior to starting serious work.
+<P>
+</UL>
+<P>
+        In map-making, a taper rising toward the map edges may have been applied to the final map to componsate for the effect of the gridding convolution in the UV plane.  The parameter 
+<A HREF="../nclean_private_keys/nclean_private_keys.html#.deconvolution"><b>DECONVOLUTION</b></A> controls if the effect of this must be taken into account in cleaning.
+<P>
+<A NAME=.data.clean><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+</b><H2><A NAME=SECTION0003300000000000000>  <b>Data clean = Cotton-Schwab Clean</b></A></H2>
+<P>
+        &quot;Data&quot; Clean is the somewhat unfortunate name given to the &quot;Cotton-Schwab&quot; modification of <A HREF="#.uv.clean">Clark Clean</A>) in which the model subtraction is done in the <A HREF="../scn_descr/scn_descr.html">SCN file(s)</A> from which the map was originally made.  In this way aliasing effects are completely avoided, albeit at the expense of again much more processing.
+<P>
+        Since a Newstar map does not include a detailed bookkeeping of the SCN files and control parameters with which it was made, the user has to respecify them as part of the process.  This is not as bad as it may sound, because no harm will be done if the new map is made with different specifications provided only that a corresponding antenna pattern is generated along with it.  The user may actually take advantage of this, e.g.  by specifying a smaller map area if he has found that that is all he needs.
+<P>
+        Since the antenna beam plays no role in source subtraction, the 
+<A HREF="#.prussian.hat"><b>PRUSSIAN_HAT</b></A> parameter is not used in Data Clean.
+<P>
+        An important practical point to note is that <em>the residual map overwrites the input map</em>. This is discussed further 
+<A HREF="#.residual.maps">below</A>.
+<P>
+<A NAME=.compon><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003400000000000000> <b>&quot;Component&quot; clean: A quick-and dirty Clean</b></A></H2>
+<P>
+        Another Clean option is available in NCLEAN, in which only the minor-cycle part of a Clark or &quot;Data&quot; Clean is performed.  Since the minor-cycle source subtraction is of a sloppy nature, the residual map should <em>not</em> be used as a starting point for further investigations. However, the source model can be used, e.g.  as a starting point for 
+<A HREF="../ncalib/ncalib.html#.redun">Selfcal</A> or <A HREF="../nmodel_descr/nmodel_descr.html">NMODEL UPDATE</A>.
+<P>
+        Another possible use is to quickly explore the effect of the <b>CYCLE_DEPTH</b> and <b>GRATING_FACTOR</b> 
+<A HREF="#.cycle.depth">parameters</A> before embarking on a lengthy Clark or Data Clean.
+<P>
+<A NAME=.residual.maps><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>Residual maps</b></A></H1>
+<P>
+        Residual maps have the same size as their parent map. For H&#246;gbom and Clark Clean, they are stored in the .WMP file from which the input map was taken, under the index
+<P>
+        &lt;group&gt;.&lt;field&gt;.&lt;channel&gt;.&lt;polarisation&gt;.1.&lt;sequence_number&gt;
+<P>
+where &lt;group&gt;...  are the same as those of the input file, the type 1 indicates a map and &lt;sequence_number&gt; is the first new number available. Thus, derivatives of a map will form a contiguous sequence in the order in which they were created.
+<P>
+        For Data Clean the residual map is written in place of the original. The idea behind this is that, unlike for the other Clean modes, one may backtrack from a Data Clean operation without recourse to the input map: What one does instead is to discard the newly found model components and then regenerate the input map with the previous model.
+<P>
+        In whichever way one cleans, backtracking implies that one must keep track of which residual maps are rejected. There is (as yet?) no mechanism available to remove them from a .WMP file except for selectively 
+<A HREF="../nmap_descr/nmap_descr.html#.copy">copying</A> maps to a new .WMP file.
+<P>
+<A NAME=.missing><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>Missing items to be added</b></A></H1>
+<P>
+<UL><LI>   Litterature references 
+<LI>   Beam-patch calculation and other details of minor-cycle clean 
+<LI>   RESTORE details 
+</UL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nclean_keys/nclean_keys.html b/nclean_keys/nclean_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..7ae80364eff1f15986b1534da30d4b42dd56b461
--- /dev/null
+++ b/nclean_keys/nclean_keys.html
@@ -0,0 +1,105 @@
+<TITLE>Index of private keywords for NCLEAN </TITLE>
+<H1>Description of keywords for program NCLEAN</H1>
+
+<UL>
+<LI> <A HREF="../nclean/nclean__cmemory_use.html">
+  CMEMORY_USE</A>
+  UV-clean memory size
+<LI> <A HREF="../nclean/nclean__dmemory_use.html">
+  DMEMORY_USE</A>
+  Work memory size
+<LI> <A HREF="../nclean/nclean__option.html">
+  OPTION</A>
+  BEAM, UVCOVER, DATA, UREST; COMPON, HISTO; QUIT Operation wanted
+<LI> <A HREF="../nclean/nclean__wmp_sets0.html">
+  WMP_SETS0</A>
+  ONE input map: grp.fld.chn.pol.0.seq
+<LI> <A HREF="../nclean/nclean__ap_wmp_set.html">
+  AP_WMP_SET</A>
+  ONE antenna pattern (grp.fld.chn.pol.1.seq)
+<LI> <A HREF="../nclean/nclean__deconvolution.html">
+  DECONVOLUTION</A>
+  Correct antenna pattern for mapping taper: YES/NO
+<LI> <A HREF="../nclean/nclean__compon_log.html">
+  COMPON_LOG</A>
+  Reporting interval for components found: | terminal, printer
+<LI> <A HREF="../nclean/nclean__cycle_depth.html">
+  CYCLE_DEPTH</A>
+  Major cycle depth
+<LI> <A HREF="../nclean/nclean__data_factor.html">
+  DATA_FACTOR</A>
+  Data multiplication factor
+<LI> <A HREF="../nclean/nclean__map_factor.html">
+  MAP_FACTOR</A>
+  Multiplication factor
+<LI> <A HREF="../nclean/nclean__clean_limit.html">
+  CLEAN_LIMIT</A>
+  Limit in fraction of map maximum
+<LI> <A HREF="../nclean/nclean__compon_limit.html">
+  COMPON_LIMIT</A>
+  Maximum number of components to find
+<LI> <A HREF="../nclean/nclean__loop_gain.html">
+  LOOP_GAIN</A>
+  Clean loop-gain factor
+<LI> <A HREF="../nclean/nclean__area.html">
+  AREA</A>
+  Window area l, m, dl, dm
+<LI> <A HREF="../nclean/nclean__grating_factor.html">
+  GRATING_FACTOR</A>
+  Grating factor
+<LI> <A HREF="../nclean/nclean__prussian_hat.html">
+  PRUSSIAN_HAT</A>
+  Prussian hat value
+<LI> <A HREF="../nclean/nclean__residual.html">
+  RESIDUAL</A>
+  residual map?
+<LI> <A HREF="../nclean/nclean__restore.html">
+  RESTORE</A>
+  restored map (YES/NO)?
+<LI> <A HREF="../nclean/nclean__restore_beam.html">
+  RESTORE_BEAM</A>
+  dl, dm arcsec, pa deg
+<LI> <A HREF="../nclean/nclean__clip_area.html">
+  CLIP_AREA</A>
+  UV-radius range for clipping (m)
+<LI> <A HREF="../nclean/nclean__clip_levels.html">
+  CLIP_LEVELS</A>
+  Amplitude range to be discarded
+<P>
+
+<UL><LI>See also <A HREF="../nmap_comm/nmap_comm.html">NMAP</A> </UL>
+
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpnode_comm/wmpnode_comm.html">WMPNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpsets_comm/wmpsets_comm.html">WMPSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+
+<UL><LI>General keywords from <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A><UL>
+<LI><A HREF="../scnnode__scn_node/scnnode__scn_node.html">SCN_NODE</A>
+<P></UL></UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nclean_descr/nclean_descr.html">program NCLEAN</A>
+</UL>
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new file mode 100644
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nclean_private_intfc/images.pl b/nclean_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nclean_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nclean_private_intfc/labels.pl b/nclean_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..cf8e040b6df18f7a1285714df7fa824756a04611
--- /dev/null
+++ b/nclean_private_intfc/labels.pl
@@ -0,0 +1,29 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".compon.log"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".data.factor"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".public"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".loop.gain"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".cycle.depth"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".ap.wmp.set"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".cmemory.use"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".residual"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".deconvolution"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".map.factor"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".restore"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".clip.levels"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".restore.beam"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".area"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".dmemory.use"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".clean.limit"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".option"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".prussian.hat"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".wmp.sets0"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".compon.limit"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".clip.area"} ="$URL/nclean_private_intfc.html"; 
+$external_labels{".grating.factor"} ="$URL/nclean_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/nclean_private_intfc/nclean_private_intfc.html b/nclean_private_intfc/nclean_private_intfc.html
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@@ -0,0 +1,497 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NCLEAN</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nclean_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nclean_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nclean_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nclean_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nclean_private_intfc.html#SECTION0003200000000000000>  <b>Parameter AP_WMP_SET</b></A>
+<LI> <A NAME=tex2html6 HREF=nclean_private_intfc.html#SECTION0003300000000000000>  <b>Parameter AREA</b></A>
+<LI> <A NAME=tex2html7 HREF=nclean_private_intfc.html#SECTION0003400000000000000>  <b>Parameter CLEAN_LIMIT</b></A>
+<LI> <A NAME=tex2html8 HREF=nclean_private_intfc.html#SECTION0003500000000000000>  <b>Parameter CLIP_AREA</b></A>
+<LI> <A NAME=tex2html9 HREF=nclean_private_intfc.html#SECTION0003600000000000000>  <b>Parameter CLIP_LEVELS</b></A>
+<LI> <A NAME=tex2html10 HREF=nclean_private_intfc.html#SECTION0003700000000000000>  <b>Parameter CMEMORY_USE</b></A>
+<LI> <A NAME=tex2html11 HREF=nclean_private_intfc.html#SECTION0003800000000000000>  <b>Parameter COMPON_LIMIT</b></A>
+<LI> <A NAME=tex2html12 HREF=nclean_private_intfc.html#SECTION0003900000000000000>  <b>Parameter COMPON_LOG</b></A>
+<LI> <A NAME=tex2html13 HREF=nclean_private_intfc.html#SECTION00031000000000000000>  <b>Parameter CYCLE_DEPTH</b></A>
+<LI> <A NAME=tex2html14 HREF=nclean_private_intfc.html#SECTION00031100000000000000>  <b>Parameter DATA_FACTOR</b></A>
+<LI> <A NAME=tex2html15 HREF=nclean_private_intfc.html#SECTION00031200000000000000>  <b>Parameter DECONVOLUTION</b></A>
+<LI> <A NAME=tex2html16 HREF=nclean_private_intfc.html#SECTION00031300000000000000>  <b>Parameter DMEMORY_USE</b></A>
+<LI> <A NAME=tex2html17 HREF=nclean_private_intfc.html#SECTION00031400000000000000>  <b>Parameter GRATING_FACTOR</b></A>
+<LI> <A NAME=tex2html18 HREF=nclean_private_intfc.html#SECTION00031500000000000000>  <b>Parameter LOOP_GAIN</b></A>
+<LI> <A NAME=tex2html19 HREF=nclean_private_intfc.html#SECTION00031600000000000000>  <b>Parameter MAP_FACTOR</b></A>
+<LI> <A NAME=tex2html20 HREF=nclean_private_intfc.html#SECTION00031700000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html21 HREF=nclean_private_intfc.html#SECTION00031800000000000000>  <b>Parameter PRUSSIAN_HAT</b></A>
+<LI> <A NAME=tex2html22 HREF=nclean_private_intfc.html#SECTION00031900000000000000>  <b>Parameter RESIDUAL</b></A>
+<LI> <A NAME=tex2html23 HREF=nclean_private_intfc.html#SECTION00032000000000000000>  <b>Parameter RESTORE</b></A>
+<LI> <A NAME=tex2html24 HREF=nclean_private_intfc.html#SECTION00032100000000000000>  <b>Parameter RESTORE_BEAM</b></A>
+<LI> <A NAME=tex2html25 HREF=nclean_private_intfc.html#SECTION00032200000000000000>  <b>Parameter WMP_SETS0</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NCLEAN. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmap_public_intfc/nmap_public_intfc.html">NMAP</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../wmpnode_public_intfc/wmpnode_public_intfc.html">WMPNODE</A> public keywords 
+<LI> <A HREF="../wmpsets_public_intfc/wmpsets_public_intfc.html">WMPSETS</A> public keywords 
+</UL>
+<P>
+<A NAME=.ap.wmp.set><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter AP_WMP_SET</b></A></H2>
+<P>
+  <em>Prompt:</em> ONE antenna pattern (grp.fld.chn.pol.1.seq)<BR><em>Expected input:</em> Character *32:  1 to 1 values
+<P>
+    <PRE>
+Specify ONE antenna pattern
+                (group.field.channel.polarisation.type(=1).sequence_number)
+</PRE>
+<P>
+<A NAME=.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter AREA</b></A></H2>
+<P>
+<em>Prompt:</em> Window area l,m,dl,dm<BR><em>Expected input:</em> Integer:  1 to 4 values
+<P>
+  <PRE>
+The CLEAN window is defined as the union of up to 32 rectangular areas (which
+may arbitrarily overlap). For BEAM clean this is also the window within which
+source responses will be subtracted.
+</PRE>
+<P>
+  <PRE>
+You are being prompted for these areas one by one until you give a null reply
+(<CR> only). An area is specified by four numbers: l,m, dl,dm, where
+</PRE>
+<P>
+  <PRE>
+   l,m     l and m in grid points for the area centre; (l,m)=(0,0) at the map
+            centre, increasing toward the upper right (i.e. with decreasing RA
+            and increasing DEC)
+   dl,dm   width and height of the area in grid points
+</PRE>
+<P>
+<A NAME=.clean.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter CLEAN_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Limit in fraction of map maximum<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the level to which to clean in fraction of the initial map maximum.
+</PRE>
+<P>
+<A NAME=.clip.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter CLIP_AREA</b></A></H2>
+<P>
+<em>Prompt:</em> UV-radius range for clipping (m)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the (circular) UV-plane radii (in metres) between which you want to
+clip the data. The default is to clip everywhere.
+</PRE>
+<P>
+<A NAME=.clip.levels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter CLIP_LEVELS</b></A></H2>
+<P>
+<em>Prompt:</em> Amplitude range to be discarded<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify amplitude range (in Westerbork Units) of visibility magnitudes that you
+want to discard.
+</PRE>
+<P>
+  <PRE>
+In the annulus defined by CLIP_AREA, values between the limits you specify will
+be discarded.
+</PRE> 
+ <em>parameter <A HREF="#.clip.area">CLIP_AREA</A> </em>
+<P>
+  <PRE>
+NOTE: It would be more natural to define a range within which visibilities are
+considered valid. As it is, only the lower limit is actually useful, allowing
+you to define a rejection threshold for interference. To do so, specify your
+threshold for the lower and 'infinity' for the upper limit, e.g.
+</PRE>
+<P>
+  <PRE>
+                <threshold>,100000
+</PRE>
+<P>
+<A NAME=.cmemory.use><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter CMEMORY_USE</b></A></H2>
+<P>
+<em>Prompt:</em> UV-clean memory size<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the work memory size in bytes for the UV Clean option, to be allowed in
+defining the beam patch and to be used in executing the Fourier transforms.
+</PRE>
+<P>
+  <PRE>
+The default shown is normally adequate; a larger value may speed up the
+execution of major cycles in UV Clean.
+</PRE>
+<P>
+  <PRE>
+NCLEAN will not accept a value in excess of 4000000 (4 MB).
+</PRE>
+<P>
+<A NAME=.compon.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter COMPON_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Maximum number of components to find<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the maximum number of components to be cleaned.
+</PRE>
+<P>
+<A NAME=.compon.log><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter COMPON_LOG</b></A></H2>
+<P>
+<em>Prompt:</em> Reporting interval for components found: | terminal, printer<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+You may give two numbers <n> here, indicating that every <n>-th component must
+be reported. The first number applies to your terminal window, the second to
+the log file. A value of 0 means 'no reporting at all.
+</PRE>
+<P>
+  <PRE>
+Example:
+        2,0 specifies that every other component will be typed, and none logged.
+</PRE>
+<P>
+<A NAME=.cycle.depth><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter CYCLE_DEPTH</b></A></H2>
+<P>
+<em>Prompt:</em> Major cycle depth<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the level relative to the initial map maximum in the CLEAN window to
+which you want to clean in one major cycle.
+</PRE>
+<P>
+<A NAME=.data.factor><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter DATA_FACTOR</b></A></H2>
+<P>
+<em>Prompt:</em> Data multiplication factor<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the factor by which to multiply the input map-data.
+</PRE>
+<P>
+  <PRE>
+This option is only relevant for DATA clean. The first input-map and all maps
+created by DATA clean will be multiplied by this factor.
+</PRE>
+<P>
+<A NAME=.deconvolution><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter DECONVOLUTION</b></A></H2>
+<P>
+<em>Prompt:</em> Correct antenna pattern for mapping taper: YES/NO<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+The gridding convolution in map-making is usually compensated for by
+multiplying the output map and antenna pattern with a taper function that rises
+toward the map edges.
+</PRE>
+<P>
+  <PRE>
+If this is the case, answering YES here will instruct the program to account
+for this effect; this will reduce the aliasing errors in the residual map,
+allowing you to clean a somewhat larger part of the map. YES will in general
+produce a result with less aliasing, NO the reverse.
+</PRE>
+<P>
+<A NAME=.dmemory.use><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter DMEMORY_USE</b></A></H2>
+<P>
+<em>Prompt:</em> Work memory size<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+The memory workspace in bytes needed is 12 times the size of the rectangle
+enclosing all selected areas in the map plane. NCLEAN normally allocates up to
+300 KB for this purpose. To satisfy the present need, you must either accept
+the value suggested here or specify a smaller set of areas, or both.
+</PRE>
+<P>
+  <PRE>
+NCLEAN will not accept a value in excess of 4000000 (4 MB).
+</PRE>
+<P>
+<A NAME=.grating.factor><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter GRATING_FACTOR</b></A></H2>
+<P>
+<em>Prompt:</em> Grating factor<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+In the minor cycles of UVCOVER, DATA and COMPON clean, the maximum error made
+in only subtracting part of the antenna pattern is estimated by <number of
+sources> times <ypical sidelobe level in antenna pattern> times GRATING_FACTOR.
+</PRE>
+<P>
+  <PRE>
+You may lower this latter factor if you are not worried about the effects of
+far-out sidelobes on the minor-cycle cleaning process. A lower value will allow
+more source components to be collected in minor cycles before a major cycle
+must be started.
+</PRE>
+<P>
+<A NAME=.loop.gain><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter LOOP_GAIN</b></A></H2>
+<P>
+<em>Prompt:</em> Clean loop-gain factor<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+For each component found, the antenna pattern shifted to its position is
+subtracted from the CLEAN window. To prevent overshoots, it is customary to
+subtract not the complete component but only a fraction of it. The magnitude of
+this fraction is defined here.
+</PRE>
+<P>
+<A NAME=.map.factor><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter MAP_FACTOR</b></A></H2>
+<P>
+<em>Prompt:</em> Multiplication factor<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the factor by which to multiply the residual map before restoring.
+</PRE>
+<P>
+  <PRE>
+Normally one should use the default value of 1; a value of 0 serves to make a
+map of the CLEAN components only.
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Operation wanted<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+CLEANing:
+</PRE>
+<P>
+  <PRE>
+   BEAM         Hogbom clean: Use the map and the beam to clean. This
+                 method is inaccurate away from the map centre due to the
+                 aliasing associated with visibility gridding.
+</PRE>
+<P>
+  <PRE>
+   UVCOVER      Standard Clark Clean: Find and provisionally subtract sources
+                 in some map areas first (minor cycles), then properly subtract
+                 the sources found (major cycle). The number of minor cycles
+                 between major cycles is determined by the program; the user can
+                 steer this through a few control parameters.
+                The method suffers from the same limitations as BEAM, but is
+                 faster for cleaning extended sources.
+</PRE>
+<P>
+  <PRE>
+   DATA         Cotton-Schwab Clean: Find sources as in UVCOVER, but perform
+                 the major cycle on the original SCN-file visibilities, making a
+                 new map from the residuals as input for the next major cycle.
+                 This method rigorously avoids the aliasing limitations of BEAM
+                 and UVCOVER, at the price of being very much slower.
+</PRE>
+<P>
+  <PRE>
+   UREST        Use a clean component list and a map to restore the clean
+                 components in the map.
+</PRE>
+<P>
+  <PRE>
+For exploring the data before committing more serious work:
+</PRE>
+<P>
+  <PRE>
+   HISTO        Produce only a histogram of selected areas in the map and/or
+                 antenna pattern
+</PRE>
+<P>
+  <PRE>
+   COMPON       Execute minor cycles as for UVCOVER, but omit the following
+                 major cycle. The result is a source model and a map in which
+                 these sources are provisionally subtracted in selected areas.
+                It is the fastest of the four CLEAN variants but produces an
+                 inaccurate residual map.
+                This option may be used to quickly get a feel for the
+                 minor-cycle control of UVCOVER and DATA Clean, or to make an
+                 initial data model for NCALIB SELFCAL or NMODEL UPDATE.
+</PRE>
+<P>
+  <PRE>
+Other options:
+</PRE>
+<P>
+  <PRE>
+   QUIT          Terminate NCLEAN.
+</PRE>
+<P>
+<A NAME=.prussian.hat><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter PRUSSIAN_HAT</b></A></H2>
+<P>
+<em>Prompt:</em> Prussian hat value<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+For extended sources a prussian hat (i.e. a nominal additional peak value on
+the central value of the antenna pattern) may give better clean results. Values
+of .1 to .4 could be tried.
+</PRE> 
+                       Cornwell
+<P>
+<A NAME=.residual><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031900000000000000>  <b>Parameter RESIDUAL</b></A></H2>
+<P>
+ residual map?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if the residual map must be written.
+</PRE>
+<P>
+  <PRE>
+For BEAM and UVCOVER cleaning, this map is an automatic by-product of the
+process and the choice is whether or not to write it to the .WMP file. The map
+will be given the same indices as the input map except for an incremented
+sequence number.
+</PRE>
+<P>
+  <PRE>
+For UVDAT cleaning, the residual map must be constructed by making a new map
+from the original visibilities, in which the CLEAN components just found are
+subtracted. The new map will OVERWRITE the input map.
+</PRE> 
+               <em>See elsewhere for the 
+               <A HREF="../nclean_descr/nclean_descr.html#.residual.map">rationale</A> </em>
+<P>
+<A NAME=.restore><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032000000000000000>  <b>Parameter RESTORE</b></A></H2>
+<P>
+<em>Prompt:</em> restored map (YES/NO)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if a restored map must be written.
+</PRE>
+<P>
+  <PRE>
+A restored map consists of the CLEAN components convolved with a hypothetical
+beam that has no sidelobes, superimposed on the residuals. It is an
+approximation to  what you would have observed with complete contiguous UV
+coverage (hoth in hour angle and baseline) up to the longest baseline available.
+</PRE>
+<P>
+  <PRE>
+You will be given the option to suppress the residuals (parameter MAP_FACTOR),
+in which case you get a map of the CLEAN components only.
+</PRE>
+<P>
+<A NAME=.restore.beam><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032100000000000000>  <b>Parameter RESTORE_BEAM</b></A></H2>
+<P>
+<em>Prompt:</em> dl, dm arcsec, pa deg<BR><em>Expected input:</em> Real:  1 to 3 values
+<P>
+  <PRE>
+Specify the restore beam width:
+</PRE>
+<P>
+  <PRE>
+   dl      width of beam in arcsec (full-halfwidth)
+</PRE>
+<P>
+  <PRE>
+   dm      width of beam in arcsec (full-halfwidth)
+</PRE>
+<P>
+  <PRE>
+   pa      position angle of skewed beam in degrees (anti-clockwise;
+            0 deg is horizontally to the right (+l direction)
+</PRE>
+<P>
+  <PRE>
+The default beam is a two-dimensional Gaussian truncated at a level of .xx
+relative to the maxiumum. If an antenna pattern for your map is available, the
+l,m beam widths are derived from it; else a rule-of-thumb formula is used:
+</PRE>
+<P>
+  <PRE>
+        half-width = 12 arcsec * 1400/frequency(MHz)
+</PRE>
+<P>
+<A NAME=.wmp.sets0><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032200000000000000>  <b>Parameter WMP_SETS0</b></A></H2>
+<P>
+<em>Prompt:</em> ONE input map: grp.fld.chn.pol.0.seq<BR><em>Expected input:</em> Character *32:  1 to 1 values
+<P>
+  <PRE>
+Specify ONE input map (group.field.channel.polar.type(=0).sequence_number)
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
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+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ncopy/ncopy__copy_ifdata.html b/ncopy/ncopy__copy_ifdata.html
new file mode 100644
index 0000000000000000000000000000000000000000..2b7a979a6fee3c06aaa11d577de20f8ef5d6178f
--- /dev/null
+++ b/ncopy/ncopy__copy_ifdata.html
@@ -0,0 +1,14 @@
+<TITLE>Description of COPY_IFDATA (NCOPY)</TITLE>
+<H1>Program NCOPY: private keyword COPY_IFDATA</H1> 
+
+<DT><EM>Prompt:</EM> copy IF-data/Total Powers?
+<DT><EM>Expected input:</EM> Logical.<P>
+ Specify YES if you want to copy IF-data (Total Powers) together 
+with the data <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncopy/ncopy_keys.html">List of keywords</A> for NCOPY
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncopy_descr/ncopy_descr.html">program NCOPY</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncopy/ncopy__copy_model.html b/ncopy/ncopy__copy_model.html
new file mode 100644
index 0000000000000000000000000000000000000000..71a65e6f4748cbffba8297857ce77ca0c2811c91
--- /dev/null
+++ b/ncopy/ncopy__copy_model.html
@@ -0,0 +1,13 @@
+<TITLE>Description of COPY_MODEL (NCOPY)</TITLE>
+<H1>Program NCOPY: private keyword COPY_MODEL</H1> 
+
+<DT><EM>Prompt:</EM> copy model data?
+<DT><EM>Expected input:</EM> Logical.<P>
+ Specify YES if you want to copy the model together with the data <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncopy/ncopy_keys.html">List of keywords</A> for NCOPY
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncopy_descr/ncopy_descr.html">program NCOPY</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncopy/ncopy__option.html b/ncopy/ncopy__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..56fc926fc0eb7aed56c626c6d553467ba04ec72c
--- /dev/null
+++ b/ncopy/ncopy__option.html
@@ -0,0 +1,19 @@
+<TITLE>Description of OPTION (NCOPY)</TITLE>
+<H1>Program NCOPY: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> COPY, SHORTCOPY, OVERVIEW, QUIT
+<DT><EM>Expected input:</EM> Character(12), 1 values.<P>
+Actions: <P>
+  COPY          Copy sectors from one SCN file to another. 
+  SHORTCOPY     As copy, but only scans selected by scan number; this option 
+                 allows you to cut out the invalid trailing scan from a mosaic 
+                 sector <P>
+  OVERWIEW      Display and log an overview of all sectors in a SCN file 
+  QUIT          Exit from NCOPY  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncopy/ncopy_keys.html">List of keywords</A> for NCOPY
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncopy_descr/ncopy_descr.html">program NCOPY</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncopy/ncopy__polarisation.html b/ncopy/ncopy__polarisation.html
new file mode 100644
index 0000000000000000000000000000000000000000..5d7f8727dafbc4840186e666dad041f077dfd8b2
--- /dev/null
+++ b/ncopy/ncopy__polarisation.html
@@ -0,0 +1,19 @@
+<TITLE>Description of POLARISATION (NCOPY)</TITLE>
+<H1>Program NCOPY: private keyword POLARISATION</H1> 
+
+<DT><EM>Prompt:</EM> XYX, XY, X; [YX] Select polarisations
+<DT><EM>Default:</EM> XYX.
+<DT><EM>Expected input:</EM> Character(4).<P>
+Select polarisations to be copied: 
+        XYX:    XX, XY, YX, YY 
+        XY:     XX, YY only 
+        X:      XX only <P>
+        YX:     for special applications only: 
+                 overwrite XX with XY, YY with YX, then output as if XY  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncopy/ncopy_keys.html">List of keywords</A> for NCOPY
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncopy_descr/ncopy_descr.html">program NCOPY</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ncopy/ncopy__scans.html b/ncopy/ncopy__scans.html
new file mode 100644
index 0000000000000000000000000000000000000000..c2a7376d50513320f68f3e1298da54d1c2ee858c
--- /dev/null
+++ b/ncopy/ncopy__scans.html
@@ -0,0 +1,19 @@
+<TITLE>Description of SCANS (NCOPY)</TITLE>
+<H1>Program NCOPY: private keyword SCANS</H1> 
+
+<DT><EM>Prompt:</EM> First and last scan number from each sector
+<DT><EM>Default:</EM>  0, 10000.
+<DT><EM>Expected input:</EM> Integer number, 2 values.<P>
+From all sectors selected, only the scan numbers within the selected scan 
+number and HA ranges wiull be copied. E.g., the specification <P>
+                SCANS= 0, 4 <P>
+will remove the last scan (number 5) from allo sectors of a mosaic observation 
+that produces 6-scan sectors. <P>
+Remember that the first scan in a sector is numbered 0.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ncopy/ncopy_keys.html">List of keywords</A> for NCOPY
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ncopy_descr/ncopy_descr.html">program NCOPY</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
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new file mode 100644
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+%%EOF
diff --git a/ncopy_descr/images.pl b/ncopy_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ncopy_descr/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ncopy_descr/labels.pl b/ncopy_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..2db1179a871d6f998cbf3cfa10c132fea4711481
--- /dev/null
+++ b/ncopy_descr/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/ncopy_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/ncopy_descr/ncopy_descr.html b/ncopy_descr/ncopy_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..7c5e1a1c68942169391c61083e091b7e04ebfa61
--- /dev/null
+++ b/ncopy_descr/ncopy_descr.html
@@ -0,0 +1,97 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NCOPY</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncopy_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncopy_descr.html#SECTION0002000000000000000> <b>General</b></A>
+<LI> <A NAME=tex2html3 HREF=ncopy_descr.html#SECTION0003000000000000000> <b>NCOPY options and keywords</b></A>
+<LI> <A NAME=tex2html4 HREF=ncopy_descr.html#SECTION0004000000000000000> <b>Possible later extensions</b></A>
+</UL>
+<H1><A NAME=SECTION0002000000000000000> <b>General</b></A></H1>
+<P>
+        NCOPY is a program to selectively copy data from an input to an output SCN file. Its basic use is to condense SCN files by 
+<UL><LI>   selecting only those sectors, scans and polarisations that one wants to retain; 
+<LI>   eliminating &quot;holes&quot; in a file that are no longer used. 
+</UL> As an ancillary function, NCOPY can produce overviews of all sectors in a SCN file.
+<P>
+<H1><A NAME=SECTION0003000000000000000> <b>NCOPY options and keywords</b></A></H1>
+<P>
+<UL><LI>   OVERVIEW: Produce on terminal and in the log file a listing of all sectors in a file. In addition to the layout (as for NFLAG SHOW) and file size, the following is shown for each sector: 
+                <i>g.o.f.c.s</i> and absolute sector numbers; 
+                field name and WSRT observation number; 
+                frequency and bandwidth; 
+                hour-range and number of scans; 
+                numbers of interferometers and polarisations; 
+                technical information for testing/debugging purposes (subject to change).
+<P>
+The information relevant to the user is crammed into the width of a terminal window.
+<P>
+<LI>   COPY: Copy sectors. The following additional information is requested once for every time the COPY option is selected:
+<P>
+INPUT_SCAN<BR>OUTPUT_SCAN<BR>INPUT_SECTORS<BR>HA_RANGE<BR>POLARISATION <BR>Data will be appended to the output file. If the latter does not exist, a new file is created and its creation reported.
+<P>
+        A new output group is created for every input group, the remaining indices, o.f.c.s, being taken from the input. 
+</UL>
+<P>
+<H1><A NAME=SECTION0004000000000000000> <b>Possible later extensions</b></A></H1>
+<P>
+        As future options, to be realised only upon user demand, we consider: 
+<UL><LI>   integration of data over hour-angle intervals; 
+<LI>   selection of interferometers; 
+<LI>   definition of output sector numbers by the user and (partial) correction of the deficiencies noted above;
+<P>
+<LI>   permanent application of corrections to the stored data as foreseen in the original Newstar design.
+<P>
+</UL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ncopy_keys/ncopy_keys.html b/ncopy_keys/ncopy_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..5b7cdaaf95b884905a279366639c1b2a7f5b7729
--- /dev/null
+++ b/ncopy_keys/ncopy_keys.html
@@ -0,0 +1,81 @@
+<TITLE>Index of private keywords for NCOPY </TITLE>
+<H1>Description of keywords for program NCOPY</H1>
+
+<UL>
+<LI> <A HREF="../ncopy/ncopy__option.html">
+  OPTION</A>
+  COPY, SHORTCOPY, OVERVIEW, QUIT
+<P>
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>General keywords from <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A><UL>
+<LI><A HREF="../scnsets__scn_sets/scnsets__scn_sets.html">SCN_SETS</A>
+<LI><A HREF="../scnsets__overview/scnsets__overview.html">OVERVIEW</A>
+<P></UL></UL>
+
+
+<UL><LI>General keywords from <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A><UL>
+<LI><A HREF="../scnsets__scn_groups/scnsets__scn_groups.html">SCN_GROUPS</A>
+<LI><A HREF="../scnsets__scn_obss/scnsets__scn_obss.html">SCN_OBSS</A>
+<LI><A HREF="../scnsets__scn_fields/scnsets__scn_fields.html">SCN_FIELDS</A>
+<LI><A HREF="../scnsets__scn_channels/scnsets__scn_channels.html">SCN_CHANNELS</A>
+<LI><A HREF="../scnsets__scn_sectors/scnsets__scn_sectors.html">SCN_SECTORS</A>
+<P></UL></UL>
+
+
+<UL><LI>General keywords from <A HREF="../select_comm/select_comm.html">SELECT</A><UL>
+<LI><A HREF="../select__ha_range/select__ha_range.html">HA_RANGE</A>
+<LI><A HREF="../select__select_ifrs/select__select_ifrs.html">SELECT_IFRS</A>
+<P></UL></UL>
+
+<P><LI> <A HREF="../ncopy/ncopy__scans.html">
+  SCANS</A>
+  First and last scan number from each sector
+<LI> <A HREF="../ncopy/ncopy__polarisation.html">
+  POLARISATION</A>
+  XYX, XY, X; [YX] Select polarisations
+<LI> <A HREF="../ncopy/ncopy__copy_model.html">
+  COPY_MODEL</A>
+  copy model data?
+<LI> <A HREF="../ncopy/ncopy__copy_ifdata.html">
+  COPY_IFDATA</A>
+  copy IF-data/Total Powers?
+<P>
+
+<UL><LI>General keywords from <A HREF="../ngen_comm/ngen_comm.html">NGEN</A><UL>
+<LI><A HREF="../ngen__x_log/ngen__x_log.html">X_LOG</A>
+<LI><A HREF="../ngen__log/ngen__log.html">LOG</A>
+<LI><A HREF="../ngen__x_run/ngen__x_run.html">X_RUN</A>
+<LI><A HREF="../ngen__run/ngen__run.html">RUN</A>
+<LI><A HREF="../ngen__x_infix/ngen__x_infix.html">X_INFIX</A>
+<LI><A HREF="../ngen__infix/ngen__infix.html">INFIX</A>
+<LI><A HREF="../ngen__x_datab/ngen__x_datab.html">X_DATAB</A>
+<LI><A HREF="../ngen__datab/ngen__datab.html">DATAB</A>
+<P></UL></UL>
+
+
+<UL><LI>General keywords from <A HREF="../ngen_comm/ngen_comm.html">NGEN</A><UL>
+<LI><A HREF="../ngen__x_memory/ngen__x_memory.html">X_MEMORY</A>
+<LI><A HREF="../ngen__memory/ngen__memory.html">MEMORY</A>
+<P></UL></UL>
+
+
+<UL><LI>General keywords from <A HREF="../ngen_comm/ngen_comm.html">NGEN</A><UL>
+<LI><A HREF="../ngen__x_apply/ngen__x_apply.html">X_APPLY</A>
+<LI><A HREF="../ngen__apply/ngen__apply.html">APPLY</A>
+<LI><A HREF="../ngen__x_de_apply/ngen__x_de_apply.html">X_DE_APPLY</A>
+<LI><A HREF="../ngen__de_apply/ngen__de_apply.html">DE_APPLY</A>
+<LI><A HREF="../ngen__x_modelb/ngen__x_modelb.html">X_MODELB</A>
+<LI><A HREF="../ngen__modelb/ngen__modelb.html">MODELB</A>
+<P></UL></UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../ncopy_descr/ncopy_descr.html">program NCOPY</A>
+</UL>
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new file mode 100644
index 0000000000000000000000000000000000000000..36585ac1596fb56271786f0de519f59be693e102
--- /dev/null
+++ b/ncopy_private_intfc.ps
@@ -0,0 +1,578 @@
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/ncopy_private_intfc/images.pl b/ncopy_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ncopy_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ncopy_private_intfc/labels.pl b/ncopy_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..1d010ea17414b6c0b200ee9fd0bd2daf2d2f8fe8
--- /dev/null
+++ b/ncopy_private_intfc/labels.pl
@@ -0,0 +1,13 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".copy.model"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".polarisation"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".copy.ifdata"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".option"} ="$URL/ncopy_private_intfc.html"; 
+$external_labels{".scans"} ="$URL/ncopy_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/ncopy_private_intfc/ncopy_private_intfc.html b/ncopy_private_intfc/ncopy_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..dcbcea0edc58c3c4515644edf3ee478bbdcc1ef0
--- /dev/null
+++ b/ncopy_private_intfc/ncopy_private_intfc.html
@@ -0,0 +1,167 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NCOPY</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncopy_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncopy_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ncopy_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ncopy_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=ncopy_private_intfc.html#SECTION0003200000000000000>  <b>Parameter COPY_IFDATA</b></A>
+<LI> <A NAME=tex2html6 HREF=ncopy_private_intfc.html#SECTION0003300000000000000>  <b>Parameter COPY_MODEL</b></A>
+<LI> <A NAME=tex2html7 HREF=ncopy_private_intfc.html#SECTION0003400000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html8 HREF=ncopy_private_intfc.html#SECTION0003500000000000000>  <b>Parameter POLARISATION</b></A>
+<LI> <A NAME=tex2html9 HREF=ncopy_private_intfc.html#SECTION0003600000000000000>  <b>Parameter SCANS</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NCOPY. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show parameters that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+</UL>
+<P>
+<A NAME=.copy.ifdata><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter COPY_IFDATA</b></A></H2>
+<P>
+  <em>Prompt:</em> copy IF-data/Total Powers?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+    <PRE>
+        Specify YES if you want to copy IF-data (Total Powers) together
+with the data
+</PRE>
+<P>
+<A NAME=.copy.model><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter COPY_MODEL</b></A></H2>
+<P>
+<em>Prompt:</em> copy model data?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+        Specify YES if you want to copy the model together with the data
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Expected input:</em> Character *12:  1 value
+<P>
+  <PRE>
+Actions:
+</PRE>
+<P>
+  <PRE>
+  COPY          Copy sectors from one SCN file to another.
+  SHORTCOPY     As copy, but only scans selected by scan number; this option
+                 allows you to cut out the invalid trailing scan from a mosaic
+                 sector
+</PRE>
+<P>
+  <PRE>
+  OVERWIEW      Display and log an overview of all sectors in a SCN file
+  QUIT          Exit from NCOPY
+</PRE>
+<P>
+<A NAME=.polarisation><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter POLARISATION</b></A></H2>
+<P>
+<em>Prompt:</em> Select polarisations<BR><em>Expected input:</em> Character *4:  1 value
+<P>
+  <PRE>
+Select polarisations to be copied:
+        XYX:    XX, XY, YX, YY
+        XY:     XX, YY only
+        X:      XX only
+</PRE>
+<P>
+  <PRE>
+        YX:     for special applications only:
+                 overwrite XX with XY, YY with YX, then output as if XY
+</PRE>
+<P>
+<A NAME=.scans><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter SCANS</b></A></H2>
+<P>
+<em>Prompt:</em> First and last scan number from each sector<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+From all sectors selected, only the scan numbers within the selected scan
+number and HA ranges wiull be copied. E.g., the specification
+</PRE>
+<P>
+  <PRE>
+                SCANS= 0,4
+</PRE>
+<P>
+  <PRE>
+will remove the last scan (number 5) from allo sectors of a mosaic observation
+that produces 6-scan sectors.
+</PRE>
+<P>
+  <PRE>
+Remember that the first scan in a sector is numbered 0.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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@@ -0,0 +1,805 @@
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new file mode 100644
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+++ b/ncopy_progrmr/_10272_tex2html_wrap198.xbm
@@ -0,0 +1,5 @@
+#define noname_width 20
+#define noname_height 9
+static char noname_bits[] = {
+ 0x1c,0xf0,0x00,0x36,0xd8,0x00,0x1f,0xd8,0x00,0x03,0xc8,0x00,0xb3,0x49,0x0c,
+ 0x9e,0x79,0x0c,0x00,0x60,0x00,0x00,0x6c,0x00,0x00,0x3c,0x00};
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new file mode 100644
index 0000000000000000000000000000000000000000..80f8d166c62f01764e9b3f259e633adbb75bdfc3
--- /dev/null
+++ b/ncopy_progrmr/_10272_tex2html_wrap206.xbm
@@ -0,0 +1,6 @@
+#define noname_width 21
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x18,0x00,0x00,0x18,0x00,0x00,0x18,0x01,0x00,0x18,0x07,0x00,0x18,
+ 0x1c,0x00,0x18,0x70,0x00,0x18,0xc0,0x01,0x18,0xe0,0x00,0x18,0x38,0x00,0x18,
+ 0x0e,0x00,0x18,0x03,0x00,0x18,0x00,0x00,0x18,0x00,0x00,0x18,0x00,0x00,0x18};
diff --git a/ncopy_progrmr/_10272_tex2html_wrap208.png b/ncopy_progrmr/_10272_tex2html_wrap208.png
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new file mode 100644
index 0000000000000000000000000000000000000000..c3407d09ca3cc5b31d37ff3bc77659047b1faf44
--- /dev/null
+++ b/ncopy_progrmr/_10272_tex2html_wrap208.xbm
@@ -0,0 +1,6 @@
+#define noname_width 37
+#define noname_height 9
+static char noname_bits[] = {
+ 0x80,0x01,0x00,0x10,0x00,0xe0,0x00,0x00,0x70,0x00,0x38,0x80,0x7f,0xc0,0x01,
+ 0x0e,0x80,0xcd,0x00,0x07,0x03,0x00,0xff,0x00,0x1c,0x0f,0x80,0x0d,0x00,0x0e,
+ 0x3c,0xc0,0x8c,0x80,0x03,0xf0,0x80,0x7f,0xe0,0x00,0xc0,0x01,0x00,0x30,0x00};
diff --git a/ncopy_progrmr/images.pl b/ncopy_progrmr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..295777f8db3f947fd1a8a6e8e38f3672c9e614b2
--- /dev/null
+++ b/ncopy_progrmr/images.pl
@@ -0,0 +1,15 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$;html_special_mark_lt;;html_special_mark_gt;${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap208.xbm">'; 
+$key = q/{}$vs.${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap196.xbm">'; 
+$key = q/{}$e.g.${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap198.xbm">'; 
+$key = q/{}$;html_special_mark_lt;${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap192.xbm">'; 
+$key = q/{}$;html_special_mark_gt;|${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap206.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/ncopy_progrmr/labels.pl b/ncopy_progrmr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..c8c970f76d179c92da4f34bb5e6de5eaecec88cd
--- /dev/null
+++ b/ncopy_progrmr/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/ncopy_progrmr.html"; 
+
+1;
\ No newline at end of file
diff --git a/ncopy_progrmr/ncopy_progrmr.html b/ncopy_progrmr/ncopy_progrmr.html
new file mode 100644
index 0000000000000000000000000000000000000000..8c82195635a68635712af6a4822abebd7ce9366d
--- /dev/null
+++ b/ncopy_progrmr/ncopy_progrmr.html
@@ -0,0 +1,160 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>NCOPY programmmer's documentation</b>
+<P>
+<em>Contributed by JPH, 940208. <BR>Updates: 
+        JPH 941031      Clarify handling of APPLY/DEAPPLY masks before and after changes of October 1994. 
+<BR>JPH 941121      prefix underscores with slashes </em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ncopy_progrmr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ncopy_progrmr.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ncopy_progrmr.html#SECTION0003000000000000000>  <b>NCOCPY: Copy sectors </b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ncopy_progrmr.html#SECTION0003100000000000000>  <b>STH modifications </b></A>
+<LI> <A NAME=tex2html5 HREF=ncopy_progrmr.html#SECTION0003200000000000000>  <b>SCH modifications </b></A>
+<LI> <A NAME=tex2html6 HREF=ncopy_progrmr.html#SECTION0003300000000000000>  <b>NCOCPB: Make unique copy of a data structure </b></A>
+</UL> 
+<LI> <A NAME=tex2html7 HREF=ncopy_progrmr.html#SECTION0004000000000000000>  <b>Tests </b></A>
+<UL> 
+<LI> <A NAME=tex2html8 HREF=ncopy_progrmr.html#SECTION0004100000000000000> <b>Copying flags (9401..-940207) </b></A>
+<LI> <A NAME=tex2html9 HREF=ncopy_progrmr.html#SECTION0004200000000000000>  <b>Checklist overflow (de Bruijn, 940207) </b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        NCOPY Phase 2 is still a relatively straigthforward program. The structure follows standard Newstar practice, with a main dispatching routine NCOPY, initialisation and user-parameter input routines NCOINI and NCODAT, and routines NCO<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap192.png">xxx&gt; that do the actual work. Some parameter input may be done by the latter. 
+        There are currently two main options: 
+ <UL><LI>   COPY: To selectively copy (parts of) sectors. 
+<LI>   OVERVIEW: To display an overview of all sectors, one sector per line. 
+ </UL>
+<P>
+<H1><A NAME=SECTION0003000000000000000>  <b>NCOCPY: Copy sectors </b></A></H1>
+<P>
+.       For a number of variables and data structures, NCOCPY has an input and an output copy, which are distinguished by the prefixes I and O: IPLN <IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap196.png"> OPLN, etc. This is in anticipation of their I and O values being different, as some already may be, line ISCN and OSCN. Pairs that are currently identical are linked by EQUIVALENCEs, <IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap198.png"> INIFR and ONIFR. &quot;O&quot; variables that are not equivalenced must be explicitly assigned. 
+.       The basic logic of NCOPCPY is straightforward. NSCSTG is repeatedly called to read sectors. Each sector's HA range is checked against the user's range and first and last scan numbers to be copied, SCNFST and SCNLST, are established. The condition that the output need no more polarisations than present in the input is also checked. 
+.       ISTH is then copied to OSTH and written tentatively, with as many changes as possible already made; its address is saved for a later rewrite. Next, the IFR table is copied and the file address of the scans block established. 
+.       The WSRT headers are copied in an internal subroutine at label 2020. This routine consists of calls to: 
+ <UL><LI>   NSCSCR: read SCH; read raw uncorrected scan visibilities into 4-polarisation c/s and weight arrays, using STH and SCH dimension parameters such as PLN and NIFR.
+<P>
+<LI>   NSCSDW: write scan from these arrays, again using dimension parameters. 
+ </UL>  
+.       Modifications to the scan are made in between.
+<P>
+.       The model lists and visibilities are copied in an internal subroutine at label 2010.
+<P>
+.       Finally, the newly made sector is linked into the index structure. The code is patterned after that of NSCREG.
+<P>
+<H2><A NAME=SECTION0003100000000000000>  <b>STH modifications </b></A></H2>
+<P>
+        NCOCPY is responsible for the following OSTH fields that differ from their ISTH peers: 
+ <UL><LI>   HAB, SCN: reflect the user's HA selection. 
+<LI>   PLN: the number of polarisations in the output. 
+<LI>   NIFR: number of output interferometers (currently identical to input).
+<P>
+<LI>   SCNL: scan length (depends on NIFR, PLN).
+<P>
+<LI>   REDNS, ALGNS, OTHNS: zero the Y components if only XX data present.
+<P>
+<LI>   pointers to other data structures. 
+ </UL>
+<P>
+<H2><A NAME=SECTION0003200000000000000>  <b>SCH modifications </b></A></H2>
+<P>
+        NCOCPY is responsible for the following OSCH fields that differ from their ISCH peers: 
+ <UL><LI>   MAX: maximum of C/S values REDNS, ALGNS, OTHNS. 
+<LI>   OTHNS: zero the Y components if only XX data present. 
+ </UL>
+<P>
+<H2><A NAME=SECTION0003300000000000000>  <b>NCOCPB: Make unique copy of a data structure </b></A></H2>
+<P>
+        Several input data structures may be linked by more than one pointer, and each link might give rise to a separate copy. For copying such structures, NCOCPB must be used. It maintains a checklist of input file addresses of blocks it has already copied, with the corresponding output file addresses. The calling program is responsible for allocating a buffer for this list and initialising it through a special call to NCOCPB. Details of this and other variant calls are to be found in NCOCPB's header. 
+        Since there can(?) be no duplications of data structures between groups, the checklist is reinitialised for every new input group. 
+        The blocks that may have multiple references are: 
+ <UL><LI>   FDW for all sectors in a mosaic: 1 
+<LI>   OHW for all sectors in the same field: 128 fields 
+<LI>   SHW for all sectors at the same frequency: 8 frequencies. 
+<LI>   MDH for all sectors in the same field: 128 fields 
+ </UL>
+<P>
+<H1><A NAME=SECTION0004000000000000000>  <b>Tests </b></A></H1>
+<P>
+.       The following tests were made to check NCOPY: 
+ <UL><LI>   Copy sectors from the same input SCN file with various selection parameters. Check outputs with OVERVIEW and compare samples of headers and data with NCOPY SHOW. 
+<LI>   Copy one 4-polarisation input sector to three output sectors, selecting XYX, XY and X polarisations. Make 4 XX and 3 YY maps from the input amd output sectors and compare the map statistics through 
+. 
+        <i>sdiff -s -w 80 <IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap192.png">log1&gt; <IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap192.png">log2<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap206.png"> grep '-<IMG ALIGN=BOTTOM ALT="" SRC="_10272_tex2html_wrap208.png">'</i> 
+ </UL>
+<P>
+<H2><A NAME=SECTION0004100000000000000> <b>Copying flags (9401..-940207) </b></A></H2>
+<P>
+        Upon request of Ger de Bruijn, all input flags are also copied to the output. To this end, the calls to NSCSCR and NSCSCW have been changed to calls to NSCSCF and NSCSFW, respectively. These have an extra parameter in which the flag settings from the input are transferred to the output. 
+        The new entry points exist in the new version of NSCSCR and NSCSCW which are still being tested in JPH's shadow system. 
+        If desired, it is very simple to add code to suppress the copying of flags. 
+        Test: 
+        Use a 720-scan single-polarisation file. NFLAG, flag_optionDETERM, 
+ops_determPBAS, pbas_limits=0,200. This results in 18in a 270-scan single-polarisation file. flag_optionINSPECT, ops_inspectIFR gives an overview per interferometer. 
+        Copy the file with NCOPY and test the copy with NFLAG, flag_optionINSPECT, ops_inspectCOUNT, select_flagALL, sub_cubeNO. This gives the same result.
+<P>
+<H2><A NAME=SECTION0004200000000000000>  <b>Checklist overflow (de Bruijn, 940207) </b></A></H2>
+<P>
+Corrections: 
+ <UL><LI>   Do not use NCOCPB for STH addresses. Multiple references to STH can only occur due to a NSCAN REGROUP operation which is very rarely used. Multiple copies of an STH can not be prevented between COPY operations. The user is already responsible for avoiding those and now has the added responsibility of avoiding REGROUP duplications. 
+<LI>   Reinitialise checklist for each new input group. 
+<LI>   Souble checklist size to handle the largest predicted mosaic observation 
+ </UL>
+<P>
+Test: 
+        Copy a simple observation A to B, then B to C, and verify that overviews of B and C are identical.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/newstar-cookbook.pdf b/newstar-cookbook.pdf
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diff --git a/newstar-verheijen.pdf b/newstar-verheijen.pdf
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diff --git a/nfilt/nfilt__freq_select.html b/nfilt/nfilt__freq_select.html
new file mode 100644
index 0000000000000000000000000000000000000000..41286c4d1fb227dac1b910090b50f5da1dd1028a
--- /dev/null
+++ b/nfilt/nfilt__freq_select.html
@@ -0,0 +1,19 @@
+<TITLE>Description of FREQ_SELECT (NFILT)</TITLE>
+<H1>Program NFILT: private keyword FREQ_SELECT</H1> 
+
+<DT><EM>Prompt:</EM> Pairs of frequency (MHz) to select solution domain
+<DT><EM>Expected input:</EM> Real number, 16 values.<P>
+  	The actual solution of the continuum radiation will be based on a 
+subset of the input channels. The channels selected will be based on 
+pairs of frequencies, indicating a range. 
+E.g. 325, 327, 330, 332 will use channels with frequnecies in the ranges 
+325-327 and 330-332 MHz. <P>
+  	* indicates all channels. <P>
+Note that the corrections are saved for all selected input frequency sets. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nfilt/nfilt_keys.html">List of keywords</A> for NFILT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nfilt_descr/nfilt_descr.html">program NFILT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nfilt/nfilt__option.html b/nfilt/nfilt__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..8eda3ce575820091f61dbf0f80a6aedc0bcbc13a
--- /dev/null
+++ b/nfilt/nfilt__option.html
@@ -0,0 +1,24 @@
+<TITLE>Description of OPTION (NFILT)</TITLE>
+<H1>Program NFILT: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> CONTINUUM, QUIT Action
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the action to be performed by the program NFILT: <P>
+<DT><STRONG>  CONTINUUM</STRONG> make a UV-based estimate of the continuum in line data. The 
+		 algoritm used fits a polynomial to the sine and cosine 
+		 components of the residual corrected data, and stores it as 
+ 		 additive interferometer data. Second order effects could 
+		 necessitate an iteration for the cross-polarised channels to 
+	 	 properly cater for polarisation correctioons and Faraday 
+		 rotation. 
+		Although the program will handle any combination of input sets,  
+		 fastest operation is attained if loops are used to select the 
+		 fields. <P>
+<DT><STRONG>  QUIT:</STRONG>    	leave the program NSCAN 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nfilt/nfilt_keys.html">List of keywords</A> for NFILT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nfilt_descr/nfilt_descr.html">program NFILT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nfilt/nfilt__poly_degree.html b/nfilt/nfilt__poly_degree.html
new file mode 100644
index 0000000000000000000000000000000000000000..e389030eda28ba10fe523d8155f2fa4c4e4b64f1
--- /dev/null
+++ b/nfilt/nfilt__poly_degree.html
@@ -0,0 +1,14 @@
+<TITLE>Description of POLY_DEGREE (NFILT)</TITLE>
+<H1>Program NFILT: private keyword POLY_DEGREE</H1> 
+
+<DT><EM>Prompt:</EM> Polynomial degree
+<DT><EM>Expected input:</EM> Integer number; min.value: 0.000000; max.value: 6.000000.<P>
+Specify the degree of the polynomial to solve for: 0=constant; 1=slope 
+etc. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nfilt/nfilt_keys.html">List of keywords</A> for NFILT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nfilt_descr/nfilt_descr.html">program NFILT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nfilt_keys/nfilt_keys.html b/nfilt_keys/nfilt_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..6e2faf008b13e0d5bbbabd9c8cb702b42275e1a1
--- /dev/null
+++ b/nfilt_keys/nfilt_keys.html
@@ -0,0 +1,40 @@
+<TITLE>Index of private keywords for NFILT </TITLE>
+<H1>Description of keywords for program NFILT</H1>
+
+<UL>
+<LI> <A HREF="../nfilt/nfilt__option.html">
+  OPTION</A>
+  CONTINUUM, QUIT Action
+<LI> <A HREF="../nfilt/nfilt__poly_degree.html">
+  POLY_DEGREE</A>
+  Polynomial degree
+<LI> <A HREF="../nfilt/nfilt__freq_select.html">
+  FREQ_SELECT</A>
+  Pairs of frequency (MHz) to select solution domain
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nfilt_descr/nfilt_descr.html">program NFILT</A>
+</UL>
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new file mode 100644
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+++ b/nfilt_private_intfc.ps
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diff --git a/nfilt_private_intfc/images.pl b/nfilt_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nfilt_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nfilt_private_intfc/labels.pl b/nfilt_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..93c4f4c51a86f44bbb197a98e6fde8502ef185a2
--- /dev/null
+++ b/nfilt_private_intfc/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/nfilt_private_intfc.html"; 
+$external_labels{".freq.select"} ="$URL/nfilt_private_intfc.html"; 
+$external_labels{".poly.degree"} ="$URL/nfilt_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/nfilt_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/nfilt_private_intfc.html"; 
+$external_labels{".option"} ="$URL/nfilt_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/nfilt_private_intfc/nfilt_private_intfc.html b/nfilt_private_intfc/nfilt_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..4b331087472b4a05752454aeebd651625909b9c2
--- /dev/null
+++ b/nfilt_private_intfc/nfilt_private_intfc.html
@@ -0,0 +1,144 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NFILT</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nfilt_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nfilt_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nfilt_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nfilt_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nfilt_private_intfc.html#SECTION0003200000000000000>  <b>Parameter FREQ_SELECT</b></A>
+<LI> <A NAME=tex2html6 HREF=nfilt_private_intfc.html#SECTION0003300000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html7 HREF=nfilt_private_intfc.html#SECTION0003400000000000000>  <b>Parameter POLY_DEGREE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NFLAG. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show parameters that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+</UL>
+<P>
+<A NAME=.freq.select><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter FREQ_SELECT</b></A></H2>
+<P>
+  <em>Prompt:</em> Pairs of frequency (MHz) to select solution domain<BR><em>Expected input:</em> Real:  1 to 16 values
+<P>
+    <PRE>
+        The actual solution of the continuum radiation will be based on a
+subset of the input channels. The channels selected will be based on
+pairs of frequencies, indicating a range.
+E.g. 325,327,330,332 will use channels with frequnecies in the ranges
+325-327 and 330-332 MHz.
+</PRE>
+<P>
+  <PRE>
+        * indicates all channels.
+</PRE>
+<P>
+  <PRE>
+Note that the corrections are saved for all selected input frequency sets.
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Action<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the action to be performed by the program NFILT:
+</PRE>
+<P>
+  <PRE>
+  CONTINUUM     make a UV-based estimate of the continuum in line data. The
+                 algoritm used fits a polynomial to the sine and cosine
+                 components of the residual corrected data, and stores it as
+                 additive interferometer data. Second order effects could
+                 necessitate an iteration for the cross-polarised channels to
+                 properly cater for polarisation correctioons and Faraday
+                 rotation.
+                Although the program will handle any combination of input sets,
+                 fastest operation is attained if loops are used to select the
+                 fields.
+</PRE>
+<P>
+  <PRE>
+  QUIT:         leave the program NSCAN
+</PRE>
+<P>
+<A NAME=.poly.degree><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter POLY_DEGREE</b></A></H2>
+<P>
+<em>Prompt:</em> Polynomial degree<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the degree of the polynomial to solve for: 0=constant; 1=slope
+etc.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nflag/nflag__clip_limit.html b/nflag/nflag__clip_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..2dd2581c0ffd67876ac5ec16df8571080559362c
--- /dev/null
+++ b/nflag/nflag__clip_limit.html
@@ -0,0 +1,28 @@
+<TITLE>Description of CLIP_LIMIT (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword CLIP_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Clip threshold (W.U.)
+<DT><EM>Expected input:</EM> Real number.<P>
+ Specify the threshold value (W.U.) for the clipping criterion 
+selected. <P>
+The default value shown is three times the rms value calculated in a 'trial 
+run' through the first &lt;N&gt; valid (see Note below) scans in the 
+primary/secondary data cube. This is intended to be an educated guess at a 
+sensible 3-sigma threshold for your operation, but you must make your own 
+assessment of the probable suitability of this value. <P>
+Notes: 
+     The new setting of the target flag in each scan or data point will 
+      OVERRIDE the current one rather than being ORed into it. <P>
+     The number &lt;N&gt; of dry-run scans is defined by the parameter DRY_SCANS; the 
+      default is 25. <P>
+     The flags used in selecting valid scans are defined by parameter ? 
+SELECT_FLAGS; the default is ALL. 
+!               {\em see parameters \textref{DRY_SCANS}{.dry.scans},  
+!                \textref{SELECT_FLAG}{.select.flag} } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__clip_limits.html b/nflag/nflag__clip_limits.html
new file mode 100644
index 0000000000000000000000000000000000000000..b23fcb065d3928f4a4d90663e3ed70283a9e533c
--- /dev/null
+++ b/nflag/nflag__clip_limits.html
@@ -0,0 +1,31 @@
+<TITLE>Description of CLIP_LIMITS (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword CLIP_LIMITS</H1> 
+
+<DT><EM>Prompt:</EM> Clip limits
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+ Specify the range within which the test value will be accepted. 
+For values outside the range the flag will be set, for those within the range 
+it will be cleared. <P>
+The default value shown is three times the rms value calculated in a 'trial 
+run' through the first &lt;N&gt; valid (see Note below) scans in the 
+primary/secondary data cube. This is intended to be an educated guess at a 
+sensible 3-sigma threshold for your operation, but you must make your own 
+assessment of the probable suitability of this value. <P>
+Notes: 
+     The new setting of the target flag in each scan or data point will 
+      OVERRIDE the current one rather than being ORed into it. <P>
+     The number &lt;N&gt; of dry-run scans is defined by the parameter DRY_SCANS; the 
+      default is 25. <P>
+     The flags used in selecting valid scans are defined by parameter ? 
+SELECT_FLAGS; the default is ALL. 
+!               {\em see parameters \textref{DRY_SCANS}{.dry.scans},  
+!                \textref{SELECT_FLAG}{.select.flag} } 
+! 
+!!              rms, 3-sigma is not the right thing here - clarify 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__dry_scans.html b/nflag/nflag__dry_scans.html
new file mode 100644
index 0000000000000000000000000000000000000000..6f8789e25e6f65c2a8fa5225e38460c5c05d1a73
--- /dev/null
+++ b/nflag/nflag__dry_scans.html
@@ -0,0 +1,21 @@
+<TITLE>Description of DRY_SCANS (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword DRY_SCANS</H1> 
+
+<DT><EM>Prompt:</EM> Number of scans to use in trial runs
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000.<P>
+'Clipping' operations need (a) threshold value(s) that is (are) related to the 
+magnitude of the data at hand. <P>
+The program determines a 'rasonable' default for such cases by performing a 
+'trial run' on the first of the scans in the data cube selected. You may 
+specify their number here. The trial run evaluates the clipping criterion but 
+does NOT modify the .SCN file.  For data with reasonably stationary statistics,  
+the default number should be adequate. A larger number obviously will take more 
+time to process. If you specify a very large number, the trial run will include 
+the entire data cube selected.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__dt1_limit.html b/nflag/nflag__dt1_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..ea015abc45cf14de764103953d1db36352ac2285
--- /dev/null
+++ b/nflag/nflag__dt1_limit.html
@@ -0,0 +1,17 @@
+<TITLE>Description of DT1_LIMIT (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword DT1_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Discontinuity threshold (W.U. per 10 sec)
+<DT><EM>Expected input:</EM> Real number.<P>
+ The DT1 option looks for 'un-physical jumps' in time in the 
+cosine and sine values of the uv-data. The actual difference (in W.U.) between 
+successive time-samples is divided by the time that separates them, in units of 
+the integration time (e.g. 60 sec). The flag is set if this value exceeds the 
+threshold. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__elevation_limit.html b/nflag/nflag__elevation_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..855e352422403cc2356f81a4b1e235279bd13bd2
--- /dev/null
+++ b/nflag/nflag__elevation_limit.html
@@ -0,0 +1,14 @@
+<TITLE>Description of ELEVATION_LIMIT (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword ELEVATION_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Elevation lower limit (deg)
+<DT><EM>Expected input:</EM> Real number.<P>
+ Specify the lower limit for acceptable elevations. All points 
+corresponding to lower elevations are rejected. The default flag-type is SHADOW. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__flag_mode.html b/nflag/nflag__flag_mode.html
new file mode 100644
index 0000000000000000000000000000000000000000..7d73353415946a2c15f9760f8a23408f36b38f1a
--- /dev/null
+++ b/nflag/nflag__flag_mode.html
@@ -0,0 +1,54 @@
+<TITLE>Description of FLAG_MODE (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword FLAG_MODE</H1> 
+
+<DT><EM>Prompt:</EM>  HYPER, SECTORS, NODE; CORR, NOCORR, UFLAG;|-DRYRUN, NODRYRUN, SHOW, NOSHOW, NOTRACE, TRACE; QUIT  "Set ONE environment parameter at a time; QUIT or &lt;CR&gt; when done|" 
+<DT><EM>Default:</EM> QUIT.
+<DT><EM>Expected input:</EM> Character(24).<P>
+ You may select one of the options at a time. 
+ The logical ones, such as CORR/NOCORR will take effect immediately. For the 
+others, you will be prompted for (a) new value(s).  The values shown below as 
+defaults are the ones with which NFLAG starts up. <P>
+   Redefinition of the primary data cube: <P>
+        HYPER:    Change the primary data cube by selecting new polarisation,  
+                   interferometer and hour-angle ranges. 
+        SECTORS:  As HYPER but including a change of the SCN_SECTORS selection. 
+        NODE:     Completely new primary data cube (i.e. including new .SCN 
+                   file) <P>
+   Data-correction modes. Shown in parentheses is NFLAG's initial setting: <P>
+        CORR/NOCORR (=NOCORR): 
+                Reading mode for visibility data: without/with corrections 
+                 applied and ignoring/acknowledging flags. 
+                 (NOCORR mode will be ignored in those cases for which the use 
+                 of uncorrected data would be pointless, e.g. ARESID, RRESID). <P>
+        UFLAG (=ALL): 
+                Default flag types to be acknowledged when reading data in 
+                 CORR mode. <P>
+   Run modes: <P>
+        SHOW/NOSHOW (=SHOW): 
+                After each flagging operation, show/don't show a summary of the 
+                 new flag settings for the data cube and flag types selected 
+for 
+                 that operation. 
+                Note that in either mode the affected flags will be counted 
+                 anyway, so you can use INSPECT afterwards to show summatries 
+                 from various perspectives <P>
+        DRYRUN/NODRYRUN (=DRYRUN): 
+                For any operation that would change flags in the .SCN file,  
+                 do/don't do a 'trial run' first, - e.g. to get a feeling for 
+                 sensible default values for clip limits etc. 
+                 (For NODRYRUN safe default values will be chosen for such 
+                 limits so that nothing will happen until the user sets his own 
+                 values.) <P>
+        NOTRACE/TRACE (=NOTRACE): 
+                Dont't/do trace the flagging operations through messages on the 
+                 terminal. TRACE is likely to produce a lot of output and 
+                 intended for debugging purposes only. <P>
+   Navigation: <P>
+        QUIT:    Go back to FLAG_OPTION. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__flag_option.html b/nflag/nflag__flag_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..cb815f2719edb906b89964328e5d947ef9db4aa5
--- /dev/null
+++ b/nflag/nflag__flag_option.html
@@ -0,0 +1,41 @@
+<TITLE>Description of FLAG_OPTION (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword FLAG_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Type of flagging operation| CLIPDATA, DETERM; CLEAR, MANUAL, HASCANS, FCOPY;|-FLIST; MODE; INSPECT, STATIST, QUIT 
+<DT><EM>Default:</EM> INSPECT.
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify the type of flagging operation to be performed: <P>
+   Selective flagging on the basis of data/coordinate/statistics values: <P>
+        CLIPDATA  Flag data points according to a data-derived criterion 
+                   (amplitudes, selfcal residuals, etc.) 
+        DETERM    Flag data points on the basis of their coordinates (position,  
+                   elevation, etc.) <P>
+   Deterministic clearing, setting and copying of flags: <P>
+        CLEAR     Clear flags from scan headers and data (see also MANUAL) 
+        MANUAL    Manual flagging operations (includes CLEAR flags). 
+!!                      What is this about MANUAL vs CLEAR? 
+        HASCANS   Operations on the scan-header flags. These affect ENTIRE 
+                   scans, and in doing so IGNORE the interferometers (parameter 
+                   IFRS) and polarisations (parameter SELECT_XYX) selections 
+                   that you defined for your primary/secondary data cubes. 
+        FCOPY     Copy flags from one place in the hypercube to another. 
+!!                      From somewhere into the hypercube? 
+!!                      From the hypercube to somewhere else? <P>
+   Operation on the flag list in core: <P>
+        FLIST     Operations on the internal flag list 
+                   (including reading-from/writing-to a .FLF file). <P>
+   Define operating environment: <P>
+        MODE      Go to FLAG_MODE parameter to change 'environment' parameter 
+                   values. This includes re-definition of the primary data 
+cube. <P>
+   Navigation: <P>
+        INSPECT   Go to the flag-INSPECTion group of operations. 
+        STATIST   Go to the data-STATISTICS group of operations. <P>
+        QUIT      Return to primary OPTION.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ha.html b/nflag/nflag__ha.html
new file mode 100644
index 0000000000000000000000000000000000000000..33ed1902c16673027c2e42cbbbe7e3d5673aff7f
--- /dev/null
+++ b/nflag/nflag__ha.html
@@ -0,0 +1,14 @@
+<TITLE>Description of HA (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword HA</H1> 
+
+<DT><EM>Prompt:</EM> hour angle range to process (deg)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+ Specify the start and end of the HA-range to be processed. If 
+only one value is given, the end value will be the same. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__input_file.html b/nflag/nflag__input_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..4c63a571bf80f6a73270b7ce8b6b0e3684e1c378
--- /dev/null
+++ b/nflag/nflag__input_file.html
@@ -0,0 +1,14 @@
+<TITLE>Description of INPUT_FILE (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword INPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> Input .FLF file name (including extension)
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the full name of the input binary-flags file. The 
+recommended filename extension is .FLF. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__limit.html b/nflag/nflag__limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..3b1e998f02dc3dff9096bdf1a151c8a61a047a88
--- /dev/null
+++ b/nflag/nflag__limit.html
@@ -0,0 +1,14 @@
+<TITLE>Description of LIMIT (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Flagging threshold
+<DT><EM>Expected input:</EM> Real number.<P>
+ Specify the limit threshold value for the (un)flag criterion 
+selected. The units (e.g. W.U.) are those appropriate for the criterion. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__limits.html b/nflag/nflag__limits.html
new file mode 100644
index 0000000000000000000000000000000000000000..e4dd41f9a2398908c9333fd6e5e3d871a29bd28d
--- /dev/null
+++ b/nflag/nflag__limits.html
@@ -0,0 +1,40 @@
+<TITLE>Description of LIMITS (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword LIMITS</H1> 
+
+<DT><EM>Prompt:</EM> flagging limits
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+ Specify the LOWER and UPPER limiting values for the (un-)flag 
+criterion. The unit (e.g. W.U.) depends on the criterion under consideration. <P>
+! 
+!  Get flag limits 
+!       Ref:    NFLOPS 
+! 
+KEYWORD=ABCS_LIMITS 
+        DATA_TYP=R 
+        IO=I 
+        NVALUES=2 
+        SWITCHES=LOOP, VECTOR, NULL_VALUES 
+        SEARCH=L, P 
+        PROMPT="Acceptance range for ABS(cos), ABS(sin)  An ENTIRE scan will be flagged if for any valid data point in it 
+the modulus of either the real (cos) or imaginary (sin) part falls outside the 
+acceptance range. <P>
+This option allows you to reject scans containing interference peaks, or 'bad' 
+data (i.e. abnormally low amplitudes). <P>
+NOTES: <P>
+     The new setting of the target flag in each scan or data point will 
+      OVERRIDE the current one rather than being ORed into it. <P>
+     The flags used in selecting valid scans are defined by parameter ? 
+SELECT_FLAGS; the default is ALL. 
+!               {\em see parameters \textref{DRY_SCANS}{.dry.scans},  
+!                \textref{SELECT_FLAG}{.select.flag} } 
+! 
+!!              rms, 3-sigma is not the right thing here - clarify 
+NB: When new thresholds are given, all Scans in the specified data cube are 
+(un-)flagged accordingly, including the Scans that were flagged already.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_clipdata.html b/nflag/nflag__ops_clipdata.html
new file mode 100644
index 0000000000000000000000000000000000000000..5f1766f6cc96886c095ee2ec2506417136ff868c
--- /dev/null
+++ b/nflag/nflag__ops_clipdata.html
@@ -0,0 +1,62 @@
+<TITLE>Description of OPS_CLIPDATA (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_CLIPDATA</H1> 
+
+<DT><EM>Prompt:</EM> Select data-thresholding criterion | AMPL, COS, SIN; ARESID, RRESID; QXY, UXY, VXY; DT1;|-INSPECT, STATIST, MODE, CLEAR, QUIT | 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Remember that only the primary data cube is affected. <P>
+The following operations flag individual data points, according to a flagging 
+criterion that is derived from the visibilities themselves. You will be 
+prompted for an upper limit. For each visibility point exceeding the limit the 
+flag will be set if it exceeds the limit, for the others it will be cleared: 
+Current flags are NOT preserved. <P>
+The flag type is CLIP, unless you have defined your own type through the 
+USER_FLAGS parameter. <P>
+   Flagging on straight data values exceeding the threshold. These criteria are 
+   intended for use with CORRECTED data (Parameter FLAG_MODE=CORR). <P>
+        AMPL    Threshold applies to absolute value 
+        COS     Threshold applies to real (cosine) part. 
+        SIN     Threshold applies to imaginary (sine) part. <P>
+   Flagging on Selfcal/Redundancy residuals. You will be prompted to specify 
+the 
+   Selfcal source model used in the latest NCALIB SEFCAL/REDUN run. 
+   (NOTE that the residuals here are VECTOR differences between observation 
+    and source model; this definition is different from that used by NPLOT.) <P>
+        ARESID  Threshold applies to the magnitude of the residual 
+        RRESID  Threshold is the absolute difference of the residual's 
+magnitude 
+                 from the average magnitude of all residuals in the scan for 
+the 
+                 same baseline. (In short: This flags outliers in sets of 
+                 redundant baselines.) 
+                NOTE: This operation can be performed even on uncalibrated 
+data,  
+                 provided a source model is available. <P>
+   Flagging on polarisation-related criteria: <P>
+        QXY     Threshold applies to the magnitude of the difference between XX 
+                 and YY visibilities per interferometer (i.e. magnitude of 
+                 Stokes Q for parallel dipoles). 
+        UXY     Threshold applies to ABS(XY-YX) per interferometer 
+                 (i.e. ABS(U) if the dipoles are parallel). 
+        VXY     Threshold applies to ABS(j(XY+YX)) per interferometer 
+                 (i.e. ABS(V) if the dipoles are parallel). <P>
+                For unpolarised sources, this criterion should be as effective 
+                 as ARESID above. <P>
+   Flagging on discontinuities in time. The flags raised here serve only as an 
+   ALERT that there is a 'jump' in the data; you will have to decide yourself 
+   what to do about the problem. <P>
+        DT1     Threshold is the difference in amplitude of a data point with 
+                 its counterpart in the preceding scan. <P>
+  Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the environment MODE-control section of the 
+                 program 
+        CLEAR   Go to the CLEAR-flags operation. 
+        QUIT    Return to FLAG_OPTION.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_determ.html b/nflag/nflag__ops_determ.html
new file mode 100644
index 0000000000000000000000000000000000000000..265ffecfa1e0e6a64c245a8000b33acf38ac998b
--- /dev/null
+++ b/nflag/nflag__ops_determ.html
@@ -0,0 +1,36 @@
+<TITLE>Description of OPS_DETERM (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_DETERM</H1> 
+
+<DT><EM>Prompt:</EM> Select coordinate criterion | SHAD, PBAS , ELEVATION; REDUN, NONRED; INSPECT, STATIST, MODE, CLEAR, QUIT 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Remember that only the primary data cube is affected. <P>
+   Flagging of data points on the basis of their coordinates. The flag type is 
+   SHADOW, unless you have selected your own type (parameter FLAG_MODE). <P>
+        SHAD      In each scan, flag all data that are affected by 'shadowing',  
+                   i.e. all interferometers in which the aperture of either 
+                   telecope is partly blocked by another telescope in the line 
+                   of sight. <P>
+        PBAS      Flag all data for which the length of the projected baseline 
+                   is within a range (for which you will be prompted). This is 
+a 
+                   way to eliminate short baselines susceptible to 
+interference,  
+                   without losing more data than necessary. <P>
+        ELEVATION Flag all uv-data that have been taken at elevations below a 
+                   limit (for which you will be prompted). <P>
+        REDUN     Flag all redundant baselines. 
+        NONRED    Flag all non-redundant baselines. <P>
+   Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the enviornment MODE-control section of the 
+                 program 
+        CLEAR   Go to the CLEAR-flags operation. 
+        QUIT    Return to FLAG_OPTION.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_fcopy.html b/nflag/nflag__ops_fcopy.html
new file mode 100644
index 0000000000000000000000000000000000000000..4e6ec14e52fe31b4ff31cef04fb4a70daa80fba7
--- /dev/null
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@@ -0,0 +1,54 @@
+<TITLE>Description of OPS_FCOPY (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_FCOPY</H1> 
+
+<DT><EM>Prompt:</EM> Flag-copy operation TOTEL, TOPOL, TODATA, TOHEAD;|INSPECT, STATIST, MODE, CLEAR, QUIT 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ FCOPY propagates flags of the selected type from individual 
+interferometers to groups of interferometers that have something in common with 
+the flagged ones. <P>
+Flags are looked for in the entire primary data cube, but changes affect only 
+the primary/secondary cube. Make sure that you understand which of the 8 flag 
+types are affected! 
+!!              Primary/secondary: Correct? <P>
+   Operations that modify flags on individual data points: <P>
+        TOTEL  Copy flags from interferometers to telescopes: For each scan 
+                selected, flag all data that share a dipole (X or Y channel of 
+                a telescope) with any interferometer for which the flag 
+                selected is set. <P>
+        TOPOL  Copy flags to all polarisations: For each scan selected, flag 
+all 
+                polarisations of all telescope pairs for which the flag 
+selected 
+                is already set for at least one of them. (This is a sort of 
+                mini-PUT). 
+!!                      Each scan &lt;--&gt; primary data cube? <P>
+   Operations that affect ENTIRE scans. NOTE that these IGNORE ANY SELECTIONS 
+   you have defined for interferometers (parameter IFRS) and/or polarisations 
+   (parameter SELECT_XYX). 
+!               {\em see the dictinction between\ 
+!               \whichref{data and header flags}{} } <P>
+        TOHEAD  For each flag selected, set the scan-header flag if it is set 
+                 for more than a given number (paremeter TOH_LIMIT) of data 
+                 points. 
+                This invalidates the entire scan. The operation is reversible 
+                 (parameter OPS_MANUAL = CLHEAD); the individual data flags 
+                 are not affected. 
+!                       {\em See parameters \textref{TOH_LIMIT}{.toh.limit},  
+!                       \textref{OPS_MANUAL}{.ops.manual} } <P>
+        TODATA  Transfer flags of the type selected from the header of each 
+scan 
+                 to all the scan's data, deleting them in the headers. <P>
+   Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the enviornment MODE-control section of the 
+                 program 
+        CLEAR   Go to the CLEAR-flags operation. 
+        QUIT    Return to FLAG_OPTION.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_flist.html b/nflag/nflag__ops_flist.html
new file mode 100644
index 0000000000000000000000000000000000000000..06e85aaae1933567995e676e97e59cdf33d1115a
--- /dev/null
+++ b/nflag/nflag__ops_flist.html
@@ -0,0 +1,58 @@
+<TITLE>Description of OPS_FLIST (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_FLIST</H1> 
+
+<DT><EM>Prompt:</EM> Flag-list operation| DELETE, GET, PUT; LOAD, UNLOAD, READ, WRITE; HEADER, LIST, LCOUNT;|-INSPECT, STATIST, MODE, CLEAR, QUIT 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify operations on the internal flag list: The entries in 
+this list represent flagging instructions. Each entry contains a flag type, and 
+ranges for the secondary data cube (i.e. hour angle, polarisation,  
+interferometer and channel ranges) to which it applies. <P>
+   Flagging operations involving the internal flag list: <P>
+        DELETE  Clear the entire list. <P>
+        GET     Collect flags of specified type(s) from the specified primary 
+                 data cube, translate them into flaqg-list entries and merge 
+                 them into the list. 
+                The default flag type is ALL, but it can be changed (parameter 
+                 FLAG_MODE). 
+!                       {\em see \whichref{paremeter FLAG_MODE}{} } 
+!!                      correct? <P>
+        PUT     Use he entries in the internal flag list to set flags for 
+                 selected visibilities or scans. 
+                If an entry in the list results in setting the flags on all 
+data 
+                 points in a scan, the corresponding scan-header flag is set 
+                 instead for efficiency reasons. <P>
+   Transfer of the flag list to/from an external file. Two types of file may be 
+   used: <P>
+      The .FLF file is in a compact binary format that is efficient in both 
+      operating speed and disk-space. It is accessed through: 
+        LOAD    Merge contents of a .FLF file into the internal flag list 
+        UNLOAD  Write the internal flag list to a new .FLF file <P>
+     The list can also be stored in an ASCII file which you can inspect and 
+edit 
+     as you please. ASCII files are bulky and take much more time to process. 
+     They are accessed through: 
+        READ    Merge contents of an ASCII flag-list file into the internal 
+flag 
+                 list 
+        WRITE   Write the internal flag list to a new ASCII flag-list file <P>
+   Inspection: <P>
+        HEADER  Show the contents of the flag-list header. 
+        LIST    Show the contents of the flag-list (can be long!). 
+!!                       Implement control-C 
+        LCOUNT  Count the flags in the flag list (NOT in the data!). 
+                 These can be INSPECTed in various one-dimensional projections. <P>
+   Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the environment MODE-control section of the 
+                 program 
+        CLEAR   Go to the CLEAR-flags operation. 
+        QUIT    Go back to what you were doing before.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_inspect.html b/nflag/nflag__ops_inspect.html
new file mode 100644
index 0000000000000000000000000000000000000000..2e0595b003fed582ae570fc81deef131f17a6e27
--- /dev/null
+++ b/nflag/nflag__ops_inspect.html
@@ -0,0 +1,47 @@
+<TITLE>Description of OPS_INSPECT (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_INSPECT</H1> 
+
+<DT><EM>Prompt:</EM>  "Projection (COUNT, FTYP, TEL, IFR, HA) with optional '_' plus|-range modifier (X, Y, XY, YX, MAN, CLIP, NOISE, ADD, SHAD, U3, U2, U1, OLD)|-OR navigation control (STATIST, MODE)" 
+<DT><EM>Expected input:</EM> Character(24).<P>
+Count and inspect flags in the primary data cube. A complete reply consists of 
+one of the primary options plus a modifier suffix. <P>
+   Count flags (no modifier!): <P>
+        COUNT   Count the flags of all types that are set, for subsequent 
+                 inspection. 
+                You may define a secondary data cube for this operation 
+                By default, flags of all types are counted; you may change this 
+                 (parameter FLAG_MODE). <P>
+   Show the flag counts in various data-cube dimensions (&lt;mod&gt; stands for one 
+of 
+   the optional modifiers listed below): <P>
+        FTYP_&lt;mod&gt;  Show the counts per flag-type (data and headers). 
+        TEL_&lt;mod&gt;   Show the counts per telescope. 
+        IFR_&lt;mod&gt;   Show the counts per interferometer. 
+        HA_&lt;mod&gt;    Show the counts per hour-angle (total over all 
+                     interferometers and polarisations). 
+!!      CHAN_&lt;mod&gt;  Show the counts per frequency channel. <P>
+     Modifiers: You may limit the display of counts to a sub-set through one of 
+     the following modifiers (prefixed with an underscore, e.g. TEL_SHAD, or 
+     HA_XX). The display will be equivalent to that for a secondary cube 
+     covering the same selection. <P>
+        X, Y            XX alone, YY alone 
+        XY, YX          only XX and YY, only XY and YX 
+        MAN, CLIP, NOIS, ADD, SHAD, U3, U2, U1, OLD 
+                        for one flag type 
+        &lt;interferometer designation&gt; 
+                        for a (group of) interferometer(s), e.g. FTYP_9A, HA_8* 
+        &lt;telescope&gt; 
+                        for a (group of) telescope(s), e.g. FTYP_8 
+!!                      Implemented?? <P>
+   Navigation: <P>
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the enviornment MODE-control section of the 
+                 program 
+        QUIT    Back out from INSPECT: Return to what you were doing before.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_manual.html b/nflag/nflag__ops_manual.html
new file mode 100644
index 0000000000000000000000000000000000000000..4dd39fe857394328c059a9afcc8dbfd3f9251df0
--- /dev/null
+++ b/nflag/nflag__ops_manual.html
@@ -0,0 +1,45 @@
+<TITLE>Description of OPS_MANUAL (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_MANUAL</H1> 
+
+<DT><EM>Prompt:</EM> Manual-flagging operation| CLEAR, CLDAT, CLHEAD; UVDATA, HARANGE; INSPECT, STATIST, MODE, QUIT 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify one of the manual flagging operations. Remember that 
+only the selected primary/secondary data cube is affected. Make sure that you 
+understand which of the 8 flag types are affected. 
+!!                      Is it the secondary? <P>
+   Clear flags. You will be prompted for the flag-type(s) to be cleared: 
+   BEWARE! Much work can be undone with careless clearing! <P>
+        CLEAR   Clear all flags of the specified type(s) in both the 
+                 scan headers and the uv data of the selected cube. 
+!!                      What if a scan "protrudes" outside the cube? 
+        CLDAT   Clear flags on the visibilities only (i.e. leave scan headers 
+                 alone). 
+        CLHEAD  Clear flags in the scan headers only. <P>
+   Set flags: <P>
+        UVDATA  Set flags of the specified type(s) in the individual 
+                 visibilities, for selected interferometer(s) within the 
+primary 
+                 data cube. 
+                Default flag type is MANUAL, but can be overridden (parameter 
+                 FLAG_MODE). 
+        HARANGE Set flags of the specified type(s) on the individual 
+                 visibilities, for selected interferometer(s) within the 
+primary 
+                 data cube. 
+                Default flag type is MANUAL, but can be overridden (parameter 
+                 FLAG_MODE). 
+                You will be repeatedly prompted for an hour-angle range. <P>
+   Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the enviornment MODE-control section of the 
+                 program 
+        CLEAR   Go to the CLEAR-flags operation. 
+        QUIT    Return to FLAG_OPTION prompt.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_scans.html b/nflag/nflag__ops_scans.html
new file mode 100644
index 0000000000000000000000000000000000000000..38823dcfa2207eddcd27e3b237dc23c20f62417f
--- /dev/null
+++ b/nflag/nflag__ops_scans.html
@@ -0,0 +1,46 @@
+<TITLE>Description of OPS_SCANS (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_SCANS</H1> 
+
+<DT><EM>Prompt:</EM> Select scan-statistics flagging criterion | SCANS; MAXABCS; ANOISE, XAN, YAN, RNOISE, XRN, YRN;|-INSPECT, STATIST, MODE, CLEAR, QUIT 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ The operations available here flag scan headers and thereby 
+affect ENTIRE scans; in doing so they IGNORE ANY SELECTIONS you have defined 
+for interferometers (parameter IFRS) and/or polarisations (parameter 
+SELECT_XYX). Apart from this, only those scans that overlap with the primary 
+data cube are affected. <P>
+For each of the options an appropriate flag is selected, as noted below. If you 
+have defined your own selection through the USER_FLAGS parameter, that 
+selection will override NFLAG's defaults. 
+!                       {\em see \textref{FLAG_MODE}{.flag.mode} } <P>
+!               {\em see the dictinction between 
+!               \whichref{data and header flags}{} } <P>
+   Flagging the scans that you select. <P>
+        SCANS   Flag scans manually; you will be given the option to select a 
+                 secondary data cube for this operation. <P>
+   Flagging on data statistics. The default flag type is CLIP. <P>
+        MAXABCS Flag all scans in which the modulus of either the real (cosine) 
+                 or imaginary (sine) part of any visibility falls outside a 
+                 range to be specified. <P>
+   Flagging on noise statistics. The default flag type is NOISE. <P>
+        ANOISE  Flag all scans in which any of the four noise values (X/Y 
+                 gain/phase) recorded in the latest NCALIB ALIGN or SELFCAL 
+                 operation exceeds a threshold (yet to be prompted for). <P>
+        XAN, YAN As ANOISE, but checking only the X resp. Y noise values. <P>
+        RNOISE  Flag all scans in which any of the four noise values (X/Y 
+                 gain/phase) recorded in the latest NCALIB REDUN operation 
+                 exceeds a threshold (yet to be prompted for). <P>
+        XRN, YRN As RNOISE, but checking only the X resp. Y noise values. <P>
+   Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        STATIST Make detour into the (data) STATISTics section of the program 
+        MODE    Make detour into the enviornment MODE-control section of the 
+                 program 
+        CLEAR   Go to the CLEAR-flags operation. 
+        QUIT    Return to FLAG_OPTION.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__ops_statist.html b/nflag/nflag__ops_statist.html
new file mode 100644
index 0000000000000000000000000000000000000000..8802ea637dbda924cd869b5a8fd998676e87da94
--- /dev/null
+++ b/nflag/nflag__ops_statist.html
@@ -0,0 +1,47 @@
+<TITLE>Description of OPS_STATIST (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPS_STATIST</H1> 
+
+<DT><EM>Prompt:</EM> "Statistics operation - (ACC, SCANS, UVDAT, &lt;name&gt;;|-GROUPS, EXPLAIN; INSPECT, MODE, QUIT)" 
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Accumulate statistics from data and/or scan headers over the 
+primary or secondary data cube and display it. <P>
+   Accumulate: 
+        ACC     Accumulate statistics from data and scan headers, excluding 
+data 
+                 points/headers that are flagged. 
+                You may select a secondary data cube for this purpose 
+(parameter 
+                 XXX). <P>
+   Inspect the results of accumulation: <P>
+        SCANS   Show the collected scan-header statistics. 
+        UVDAT   Show the collected visibility statistics. 
+        &lt;name&gt;  Show the statistics of the named 'accumulation group' (use 
+                 GROUPS and EXPLAIN above to see what choices you have). <P>
+   These options will produce a Table with the following columns: <P>
+        &lt;name&gt;  The name of the quantity for which statistics have been 
+                 calculated. 
+        mean    Its average value 
+        rms     Its rms magnitude 
+        rmsms   Its rms deviation w.r.t. the mean. 
+        rmsvar  The rms difference, between pairs of successively processed 
+                 values. 
+        wtot    Total weight. Usually it indicates the total nr of samples. 
+        minval  Its minimum value. 
+        maxval  Its maximum value. 
+        &lt;unit&gt;  The units in which the above values (except wtot) are 
+expressed. <P>
+   Get some extra help: <P>
+        GROUPS  Show the names of the currently defined 'accumulation groups' 
+        EXPLAIN Show explanation of statistical quantities. <P>
+   Navigation: <P>
+        INSPECT Make detour into the (flag) INSPECTion section of the program 
+        MODE    Make detour into the enviornment MODE-control section of the 
+                 program 
+        QUIT    Go back to what you were doing before.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__option.html b/nflag/nflag__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..99f1c2f6129d0e61e4a7687e4cf30e796b86eb84
--- /dev/null
+++ b/nflag/nflag__option.html
@@ -0,0 +1,20 @@
+<TITLE>Description of OPTION (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> NFLAG main branch FLAG; SHOW, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify the nature of the operation you want to perform: <P>
+        FLAG:    Set, clear and/or browse data flags in a .SCN file 
+                  and/or browse its data statistics <P>
+        SHOW:    Show/edit data and header information in .SCN file. This 
+option 
+                  is a clone of the SHOW option in NSCAN and is available here 
+                  for convenience. <P>
+        QUIT:    Terminate NFLAG  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__output_file.html b/nflag/nflag__output_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..f7fac09473db599cb015ba628dbd3879399546ee
--- /dev/null
+++ b/nflag/nflag__output_file.html
@@ -0,0 +1,14 @@
+<TITLE>Description of OUTPUT_FILE (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword OUTPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> Output .FLF file name (including extension)
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the full name for the output binary-flags file. The 
+recommended filename extension is .FLF. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__pbas_limits.html b/nflag/nflag__pbas_limits.html
new file mode 100644
index 0000000000000000000000000000000000000000..1613d95dc1e8d98a0e3abd39c89a92fb4b19e3f7
--- /dev/null
+++ b/nflag/nflag__pbas_limits.html
@@ -0,0 +1,32 @@
+<TITLE>Description of PBAS_LIMITS (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword PBAS_LIMITS</H1> 
+
+<DT><EM>Prompt:</EM> Projected-baseline range to be flagged (m)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+ Specify the range of lengths of PROJECTED baseline to be 
+flagged. The default flag-type is SHADOW. <P>
+Short baselines are more sensitive to interference. In flagging them wholesale,  
+however, one also loses visibility data representing extended source structure; 
+a more selective procedure is to be preferred. <P>
+Another application of this parameter is to force a uv coverage that is more 
+nearly circular in the PROJECTED uv plane, and hence produces a more circularly 
+symmetric antenna pattern. To this end, set the lower limit less than or equal 
+to <P>
+        &lt;longest baseline&gt; * sin DEC <P>
+Instead of permanently modifying the .SCN file in this way, one may use the 
+NMAP parameters CWEIGHT_TYPE and CWEIGHT_VALUE to achieve a similar effect. 
+!               {\em see NMAP public paremeter 
+!                \textref{CWEIGHT_TYPE}{nmap_public_keys.cweight.type} } <P>
+Examples: 
+        PBAS_LIMITS = 0, 288 <P>
+   causes all projected baselines up to 288 m (inclusive) to be flagged. <P>
+   For a source at a declination of 30 deg,  <P>
+        PBAS_LIMITS = 1500, 10000 <P>
+   will flag projected baselines longer than 1500 m.   <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__put_expand_ch.html b/nflag/nflag__put_expand_ch.html
new file mode 100644
index 0000000000000000000000000000000000000000..ac810e7c12090707abc4299f4d20389e46b66348
--- /dev/null
+++ b/nflag/nflag__put_expand_ch.html
@@ -0,0 +1,23 @@
+<TITLE>Description of PUT_EXPAND_CH (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword PUT_EXPAND_CH</H1> 
+
+<DT><EM>Prompt:</EM> PUT expansion half-width in channel numbers
+<DT><EM>Expected input:</EM> Integer number; min.value: 0.000000.<P>
+ PUT performs flagging commands from the internal flag list on 
+your primary data cube. Each command consists of a flag/unflag mask plus ranges 
+in the frequency- 
+channel, interferometer, polarisation and hour-angle 'dimensions' of the TARGET 
+points to which it must be applied. <P>
+You have activated PUT's option to EXPAND, within the limits of the primary 
+data cube, the operation over a 4-dimensional volume of data around each target 
+point. You may now select the number of channels on either side of a target 
+channel over which you want to expand the flagging.  Example: 
+        If you reply 2, a total of 5 channels centered on each target channel 
+will be flagged: two above and two below the target.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__put_range.html b/nflag/nflag__put_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..ba89fd261c7ad986ea8a67ea25ff6ea5134ae144
--- /dev/null
+++ b/nflag/nflag__put_range.html
@@ -0,0 +1,46 @@
+<TITLE>Description of PUT_RANGE (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword PUT_RANGE</H1> 
+
+<DT><EM>Prompt:</EM> Ranges for expansion volume around PUT points:|-chan.HA.ifr.pol 
+<DT><EM>Expected input:</EM> Character(8), 4 values.<P>
+ PUT performs flagging commands from the internal flag list on 
+your primary data cube. Each command consists of a flag/unflag mask plus ranges 
+in the frequency- 
+channel, interferometer, polarisation and hour-angle 'dimensions' of the TARGET 
+points to which it must be applied. <P>
+PUT has the capability to EXPAND, within the limits of the primary data cube,  
+the operation over a 4-dimensional volume of data around each target point. 
+The extension volume is specified through RANGES along the channel, hour-angle,  
+interferometer and polarisation axes in this order. Except for interferometers,  
+a range is formulated in terms of units of sequential position rather than 
+physical coordinates. It can be one of the foloowing: <P>
+   .            do not extend along this axis 
+   *            extend to all positions along this axis 
+   &lt;n&gt; or &lt;n&gt;C  extend over &lt;n&gt;/2-1 positions on either side (incrementing &lt;n&gt; 
+                 if it is even) 
+   &lt;n&gt;L         extend over &lt;n&gt;-1 positions to the 'left' (i.e. toward lower 
+                 coordinates) 
+   &lt;n&gt;R         extend over &lt;n&gt;-1 fields to the 'right' (i.e. toward higher 
+                 coordinates) <P>
+   The following special notations can also be used in each dimension: <P>
+        &lt;n&gt;=0   suppress flagging altogether (length of the nextension cube is 
+                 zero) 
+        &lt;n&gt;=1   identical to . (length of extension cube is 1: no extension) 
+   The following shorthand can be used for the entire reply: <P>
+        *       short for 1, 1, 1, 1 or ., ., ., (You may do better to avoid this 
+                 form because this use of a wildcard character is anomalous.) <P>
+?  The interferometer range works on telescope basis, i.e. the given range is ? 
+  valid for both receptors (e.g. 0Y and AX). 
+!!              Clarify, it must be different from the other coordinates... <P>
+Example: 
+        If a particular ineterferometer is flagged in one of frequency 
+channels,  
+                PUT_RANGE= *, ., ., . 
+ will propagate the flag to all channels for that interferometer  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__select_flag.html b/nflag/nflag__select_flag.html
new file mode 100644
index 0000000000000000000000000000000000000000..b814be984100cbe96a7c6b9f63e7db9c95a8fc42
--- /dev/null
+++ b/nflag/nflag__select_flag.html
@@ -0,0 +1,30 @@
+<TITLE>Description of SELECT_FLAG (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword SELECT_FLAG</H1> 
+
+<DT><EM>Prompt:</EM> Flag type(s) to use in data selection| NONE, ALL, MAN, CLIP, NOISE, ADD, SHAD , U1, U2, U3; [OLD]
+<DT><EM>Expected input:</EM> Character(16), 16 values.<P>
+ Some operations test flags in selecting data. By default, NFLAG 
+selects the test flags appropriate to each operation; only those data are 
+accepted for which these flags are CLEAR. <P>
+You may define here an alternative (set of) flag type(s) to be used in ALL 
+subsequent testing operations; you may select more than one, separated by 
+commas. Reply NONE to revert to the default settings. <P>
+   ALL or *     test all flag types 
+   MAN          test the flag type for the MANUAL class of operations 
+   CLIP         test the flag type for the CLIP class of operations 
+   NOISE        test the flag type for the NOISE class of operations 
+   ADD          test the flag type for the ADDITIVE class of operations 
+   SHAD         test the flag type for the SHADOW class of operations 
+   U1, U2, U3   'user' flag types, i.e. types you may use as you please 
+   NONE         revert to NFLAG's default types per operation <P>
+   OLD          the flag type for the 'OLD' class (i.e. flagged before 
+                 930609, and converted with NVS option) 
+                 NB: OLD uses the same flag-bit as MAN 
+!!              I suppose this can now be removed. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__shadow_diam.html b/nflag/nflag__shadow_diam.html
new file mode 100644
index 0000000000000000000000000000000000000000..0c8172bbc46345ffa381ed50c5aed7a20091f256
--- /dev/null
+++ b/nflag/nflag__shadow_diam.html
@@ -0,0 +1,23 @@
+<TITLE>Description of SHADOW_DIAM (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword SHADOW_DIAM</H1> 
+
+<DT><EM>Prompt:</EM> Telescope shadowing diameter (metres)
+<DT><EM>Expected input:</EM> Real number.<P>
+ Specify the diameter (m) of the telescopes. <P>
+A telescope is 'shadowed' as soon as part of its aperture gets blocked by the 
+presence of another telecope in its line of sight. This condition occurs when 
+the projected baseline between the two telecopes becomes less than the 
+telescope diameter D (25 m for the WSRT). If you want to retain as much as 
+possible of your data, you may specify a somewhat smaller number (e.g. 0.8 D) 
+to take into account the fact that the edge of the aperture is only weakly 
+illuminated. <P>
+For the hour-angles at which a telescope is shadowed, all intreferometers are 
+flagged of which it is a part. The default flag-type is SHADOW. <P>
+  ? Another flag may be selected through the FLAG_MODE parameter.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__sub_cube.html b/nflag/nflag__sub_cube.html
new file mode 100644
index 0000000000000000000000000000000000000000..61591e3269d8112babece852865d3ba9928b83c2
--- /dev/null
+++ b/nflag/nflag__sub_cube.html
@@ -0,0 +1,28 @@
+<TITLE>Description of SUB_CUBE (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword SUB_CUBE</H1> 
+
+<DT><EM>Prompt:</EM> Type of secondary data cube YES, IFR, POL, HA; NO
+<DT><EM>Expected input:</EM> Character(24).<P>
+ You may define a 'secondary cube' that includes only part of the 
+primary data cube. The current flagging operation will affect only the cross 
+section of the primary and secondary cubes. <P>
+Unlike the primary cube (which can only be redefined through the FLAG_MODE 
+parameter), the secondary cube definition applies only to the current operation 
+and will evaporate when it completes. <P>
+Specify here how you want to define the secondary cube. You may give ONE option 
+at a time; the prompt will reappear until you reply with NO. <P>
+        YES  Polarisations, interferometers and hour-angle range. 
+        IFR  Interferometers 
+        POL  Polarisations 
+        HA   Hour-angle range 
+        NO   Accept the current settings 
+!!              Check volatility, interpretation of NO, one at a time and 
+!!              defaulting 
+!       \whichref{}{} 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__toh_limit.html b/nflag/nflag__toh_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..78bf543945544ee97842a248050435eafd944503
--- /dev/null
+++ b/nflag/nflag__toh_limit.html
@@ -0,0 +1,21 @@
+<TITLE>Description of TOH_LIMIT (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword TOH_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Maximum number of data flags to tolerate per scan
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000.<P>
+ NFLAG will check in each scan the number of points for which the 
+flag type selected is set. If that number exceeds this value you define here,  
+the entire scan will be flagged. This will subsequently result in faster 
+processing 
+(because individualdata points need not be tested) at the expense of the loss 
+of some healthy data. <P>
+The operation of setting header flags is reversible: The individual data flags 
+are retained so you can restore the present condition by clearing the header 
+flags.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__user_flag.html b/nflag/nflag__user_flag.html
new file mode 100644
index 0000000000000000000000000000000000000000..b2d89aa5add42e441023cbdb02b00e02d574ce8f
--- /dev/null
+++ b/nflag/nflag__user_flag.html
@@ -0,0 +1,27 @@
+<TITLE>Description of USER_FLAG (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword USER_FLAG</H1> 
+
+<DT><EM>Prompt:</EM> default flag type(s) NONE, ALL, MAN, CLIP, NOISE, ADD, SHAD, |U1, U2, U3; OLD 
+<DT><EM>Expected input:</EM> Character(16), 16 values.<P>
+ Specify the default flag type(s) for flagging operations. <P>
+    NONE:      no flag type specified (i.e. use default types) 
+    ALL or *   all flag types (not very useful) 
+    MAN        flag type for the MANUAL class of operations 
+    CLIP       flag type for the CLIP class of operations 
+    NOISE      flag type for the NOISE class of operations 
+    ADD        flag type for the ADDITIVE class of operations 
+    SHAD       flag type for the SHADOW class of operations 
+    U1, U2, U3 'user' flag types, i.e. types you may use as you please <P>
+Note:   Flags U1, U2, U3 can be used to experiment with some flagging operation 
+        without affecting the flag type that is 'officially' associated 
+        with the same operation. <P>
+    OLD        use the flag type for the 'OLD' class (i.e. flagged before 
+                930609, and converted with NVS option) 
+                NB: OLD uses the same flag-bit as MAN  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nflag/nflag__user_flags.html b/nflag/nflag__user_flags.html
new file mode 100644
index 0000000000000000000000000000000000000000..a828bc80b3aaed379e2b650ffee77c872d34b425
--- /dev/null
+++ b/nflag/nflag__user_flags.html
@@ -0,0 +1,21 @@
+<TITLE>Description of USER_FLAGS (NFLAG)</TITLE>
+<H1>Program NFLAG: private keyword USER_FLAGS</H1> 
+
+<DT><EM>Prompt:</EM> Select flag type(s) for ALL flagging operations| NONE, [ALL]; MAN, CLIP, NOISE, ADD, SHAD, U1, U2, U3; [OLD]
+<DT><EM>Expected input:</EM> Character(16), 16 values.<P>
+ Each flagging operation changes a specific flag type by default. 
+You may define here an alternative (set of) flag type(s) to be used in ALL 
+subsequent flagging operations. Reply NONE to revert to the default settings. <P>
+The purpose is to allow you to do experimental flagging with one of the USER 
+flags without messing up the flagging that you have already done. <P>
+        OLD     use the flag type for the 'OLD' class (i.e. flagged before 
+                 930609, and converted with NVS option) 
+                 NB: OLD uses the same flag-bit as MAN 
+!!              I suppose this can now be removed. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nflag/nflag_keys.html">List of keywords</A> for NFLAG
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
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new file mode 100644
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+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
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+
+
+1;
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diff --git a/nflag_descr/labels.pl b/nflag_descr/labels.pl
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+# Associate symbolic labels with physical files.
+
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+
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NFLAG</b>
+<P>
+<em>Contributed by Johan Hamaker, October 1995.<BR>Revision of original docyment by Jan Noordam, August 1993. </em>
+<P>
+<em>This is a preliminary version of a new document replacing the old version of August 1993 by J.E. Noordam. The information in it is thought to be accurate but known to be incomplete. It should, however, in its present from help the user to get to grips with NFLAG's overwhelming user interface and functionality. </em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nflag_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nflag_descr.html#SECTION0002000000000000000> <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nflag_descr.html#SECTION0003000000000000000>  <b>The <i>NEWSTAR </i> flags concept</b></A>
+<LI> <A NAME=tex2html4 HREF=nflag_descr.html#SECTION0004000000000000000>  <b>Flagging logistics</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=nflag_descr.html#SECTION0004100000000000000>  <b>Visibility and scan-header flags</b></A>
+</UL> 
+<LI> <A NAME=tex2html6 HREF=nflag_descr.html#SECTION0005000000000000000>  <b>Primary and secondary visibility (hyper)cubes</b></A>
+<LI> <A NAME=tex2html7 HREF=nflag_descr.html#SECTION0006000000000000000>  <b>The flagging branch of NFLAG</b></A>
+<LI> <A NAME=tex2html8 HREF=nflag_descr.html#SECTION0007000000000000000>  <b>The INSPECTion branch of NFLAG</b></A>
+<LI> <A NAME=tex2html9 HREF=nflag_descr.html#SECTION0008000000000000000>  <b>The STATISTics branch of NFLAG</b></A>
+<LI> <A NAME=tex2html10 HREF=nflag_descr.html#SECTION0009000000000000000>  <b>NFLAGS environment paremeters: The MODE branch</b></A>
+<LI> <A NAME=tex2html11 HREF=nflag_descr.html#SECTION00010000000000000000>  <b>Selection of bad visibilities on an X11 display </b></A>
+</UL>
+<A NAME=.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Overview</b></A></H1>
+<P>
+        The basic function of NFLAG is to mark visibility points in a .SCN file as faulty by 'flagging' them, i.e. by setting bits in the 'flag mask' associated with each point. In general, visibilities thus flagged will be considered no longer to exist; in this sense flagging is equivalent to deletion, but unlike deletion it is reversible, i.e. flag bits can be cleared at a later time. It is also possible to instruct processing programs to ignore flag bits and treat flagged visibilities as valid.
+<P>
+        A secondary function in NFLAG, not further described here, is the SHOW option through which one may explore the contents of a .SCN file. For a description, see the descriptions of <A HREF="../nscan_descr/nscan_descr.html">NSCAN</A> and its 
+<A HREF="../nscan_private_intfc/nscan_private_intfc.html">parameter interface</A>.
+<P>
+<A NAME=.flag.concept><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>The <i>NEWSTAR </i> flags concept</b></A></H1>
+<P>
+        The simplest way to get rid of bad visibilities is by <em>deleting</em> them. Typically this is done by replacing each bad value by a special value that processing programs recognise as an instruction to ignore the data point. Since its original value is overwritten, a deleted data point is irreversibly lost.
+<P>
+        The first step toward refinement is to <em>flag</em> visibilities as bad without overwriting them; processing programs ignore those data for which the flag is set. Since the original value is retained, is can be 'undeleted' by clearing the flag; flagging is therefore also known as 'reversible deletion'. This method is a well-known one, because it is implemented AIPS.
+<P>
+        In <i>NEWSTAR </i>, it is carried a step further by differentiating between a number of different reasons for which a visibility may be considered bad. Rather than a single flag, <i>NEWSTAR </i> associates a complete <em>flag byte</em> with each visibility point: Thus one has not a single bit to play with, but eight different ones.     The advantage of this approach is that different flagging operations can be treated independently of one another. This makes it possible in many cases to backtrack form a flagging operation that produced undesirable results and thus introduces an important margin of safety: For instance, a selection made in a laborious manual flagging session cannot be accidentally undone by a subsequent automatic clipping operation going wrong.
+<P>
+        Five of the eight bits in the flag byte are used by NFLAG, the user may use the remaining three in whichever way he wishes. By default, programs bypass all visibilities for which any one of the eight flags is set; it is also possible, however, to instruct a program to ignore certain flags. The three user-definable flag-types can be used for experiments with different selections of uv-data. (This is analogous to the use of different flag tables in AIPS.)
+<P>
+        Below is a list of the flags defined by <i>NEWSTAR </i>. The numbers shown in parentheses are the bit number (LSB=0) and hexadecimal values for these flags: 
+ <UL><LI>   MANUAL (bit 7, 80): NFLAG sets this flag when the user explicitly selects data points for flagging by specifying their coordinates (sector index, hour-angle range etc.)
+<P>
+<LI>   CLIP (bit 6, 40): This flag is set in operations that select bad data by comparing them against some limit, e.g. a maximum for their cos or sin components or their selfcal residual amplitiude.
+<P>
+<LI>   NOISE (bit 5, 20):  This flag is set in operations that select groups of bad data by checking their noise levels, e.g. those that NCALIB has calculated and stored in the .SCN file in a REDUN or 
+SELFCALperation.
+<P>
+<LI>   ADDitive (bit 4, 10):  This flag is set in operations that select groups of bad data by comparing their average value against some limits
+<P>
+<LI>   SHADowing (bit 3, 08):  This flag is set in operations that select bad data on the basis of some function of their coordinates, e.g. the length of the projected baseline or a geometry in which shadowing occurs.
+<P>
+ </UL>  The remaining three bits are known as U1 (bit 2, 04), U2 (bit 1, 02) and U3 (bit 0, 01).
+<P>
+        The <i>NEWSTAR </i> visibility flagging scheme gives the user unprecedented flexibility for reversible data-editing, although its very power makes it a little more difficult to understand and use than a simple scheme such as AIPS's.
+<P>
+<A NAME=.logistics><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>Flagging logistics</b></A></H1>
+<P>
+        The only program that actiually sets and clears flags is NFLAG. It contains a number of options to select bad data on a varied range of criteria and set flags accordingly. To verify the effect, it also offers the option to 
+count flags over various cross-sections or projections of the 
+<A HREF="../scn_file/scn_file.html#.hypercube">data hypercube</A> and tabulate the results.
+<P>
+        Another option is to select flags on a display of some two-dimensinal cross section through the hypercube, using the program NGIDS. NGIDS then produces a file with flagging commands which may subsequently be 
+read and executedy NFLAG.
+<P>
+        On a micro-level, it is possible to inspect the individual flag bytes in individual scans through the <A HREF="#.overview">SHOW</A> option.
+<P>
+<A NAME=.header.flags><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000>  <b>Visibility and scan-header flags</b></A></H2>
+<P>
+        In addition to the flag bytes associated with the individual visibilities, the <A HREF="../scn_file/scn_file.html#.scan">scan header</A> also contains a flag byte. Through the flags in this byte one may invalidate the scan as a whole. This is obviously a more expedient way to handle flagging, since a single computer instruction will flag or test the entire scan.
+<P>
+        In the present implementation of NFLAG, visibility flagging and scan-header flagging operate independently. That is, when the header is flagged the corresponding flags on the individual visibilities are left unchanged, and if the header is later unflagged those flags come back into force. On one hand this introduces some additional independence between different flagging operations as discussed <A HREF="#.flag.concept">above</A>. On the other hand it forces upon the user a technical distinction between two types of flagging that are functionally equivalent: The user must contend with such flagging operations as 
+<A HREF="../nflag_private_intfc/nflag_private_intfc.html#.ops.scans">HASCANS</A>, 
+<A HREF="../nflag_private_intfc/nflag_private_intfc.html#.ops.manual">CLHEAD</A>, 
+<A HREF="../nflag_private_intfc/nflag_private_intfc.html#.ops.fcopy">TOHEAD, TODATA</A>, statistics specifiers such as 
+<A HREF="../nflag_private_intfc/nflag_private_intfc.html#.ops.statist">SCANS</A>. (Unfortunately, the keywords used are not an example of clarity and consistency...)
+<P>
+<A NAME=.hypercubes><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000>  <b>Primary and secondary visibility (hyper)cubes</b></A></H1>
+<P>
+        We assume here that the concept of the visibility 
+<A HREF="../scn_file/scn_file.html#.hypercube">hypercube</A> is understood. We recall that the group/observation, mosaic-subfield, frequency-channel and (for a mosaic observation) the successive hour-angle 'cuts' are selected through the compound 
+<A HREF="../scn_file/scn_file.html#.SCNSUM.indices">sector index</A>; the scan's hour-angle, and within a scan the interferometer and polarisation are selected by direct specification.
+<P>
+        At the very start, NFLAG asks you to select a <em>primary data hypercube</em> to operate on, through the parameters 
+ <UL> 
+<LI><A HREF="../scnnode_public_intfc/scnnode_public_intfc.html#.scn.node"><b>SCN_NODE</b></A>: 
+        .SCN file; 
+<LI>   <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html#.scn.sets"><b>SCN_SETS</b></A>: 
+        sets of sectors, i.e. one ore more combinations of group, observation, 
+        mosaic subfield, frequency channels and hour angle cuts; 
+<LI>   <A HREF="../select_public_intfc/select_public_intfc.html#.ha.range"><b>HA_RANGE</b></A>: 
+        hour-angle range; 
+<LI>   <A HREF="../select_public_intfc/select_public_intfc.html#.select.ifrs"><b>SELECT_IFRS</b></A>: 
+        interferometers; 
+<LI>   <A HREF="../select_public_intfc/select_public_intfc.html#.select.xyx"><b>SELECT_XYX</b></A> 
+        polarisations. 
+ </UL>
+<P>
+This primary cube may later be redefined partly or completely through the MODE branch of NFLAG which is accessible from several places in the program.
+<P>
+        For certain operations, one may narrow down the range of visibilities to be operated on by defining a <em>secondary hypercube</em>; the data volume operated upon will then be the cross section of the primary and secondary cubes. Secondary-cube definition is limited to the latter three of the parameters listed above; note, in particular, that it is not presently possible to define a secondary frequency-channel range because that definition is part of the SCN_SETSparameter.
+<P>
+        A word of caution is in order about the effect of data-cube definitions in operations that affect the <A HREF="#.header.flags"><em>scan-header</em></A> flags. Since such actions operate on the entire scan, <em>the ranges of interferometers and polarisations (parameters <em>SELECT_IFRS</em> and 
+<em>SELECT_XYX</em>) that you defined for your hypercubes have no effect</em>.
+<P>
+<A NAME=.flagging.branch><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000>  <b>The flagging branch of NFLAG</b></A></H1>
+<P>
+<A NAME=.nflag.flag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/nflag_flag.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>Bird's eye view of the flagging branch of NFLAG, showing the four main branches and their interconnections. Regular text represents manpulation of program variables. Interactions with the user are shown in boldface; an arrow shows parameter input into a program variable. 
+<BR>Full-drawn lines represent the main-branch connections, dashed lines the detours from one main branch into another one; the user selects these routes through the nparameter inputs shown. 
+<BR>Dotted lines represent the return paths that are selected through a QUIT input in each of the branches. All returns are through label 101 in the top left; in the case where the return is from a detour, control is returned to the branch where the detour originated. </i>
+<P>
+<A NAME=.nflag.operate><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/nflag_operate.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>Schematic of the operations branch of NFLAG. 
+<BR>This branch contains options to set visibility or scan-header flags on the basis of a variety of criteria. See text for a description. </i>
+<P>
+        The flagging branch is where the actual work of NFLAG is done. All commands that change flag setting on visibility points or scan headers are to be found here. The flagging options are shown in the upper left box in 
+<A HREF=" #.nflag.flag">figure</A> A detailed overview of the branch is given in 
+<A HREF=" #.nflag.operate">figure</A>.
+<P>
+<A NAME=.inspection.branch><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0007000000000000000>  <b>The INSPECTion branch of NFLAG</b></A></H1>
+<P>
+<A NAME=.nflag.inspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/nflag_inspect.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>Schematic of the INSPECT branch of NFLAG. 
+<BR>By default NFLAG executes a COUNT operation at the end of each 
+flagging operation. The COUNT option is provided mainly for convenience, but must be executed if you want to display flagging statistics before doing anything else. </i>
+<P>
+        The purpose of the inspection branch is to provide overviews of the flags present. Generally speaking, the bulk of the visibilities is much too large for making useful graphic or tabular representations of the individual flag settings. For most purposes, however, the information one needs can be represented in the form of tables of flag counts along various cross-sections of the visibility hypercube. Such tables is what the inspection commands produce.
+<P>
+        A schematic overview of the branch is given in <A HREF=" #.nflag.inspect">figure</A>.
+<P>
+        From the INSPECT branch, it is possible also to make a detour into the 
+<A HREF="#.mode.branch">MODE</A> or <A HREF="#.statist.branch">STATISTICS</A> branch.
+<P>
+<A NAME=.statist.branch><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0008000000000000000>  <b>The STATISTics branch of NFLAG</b></A></H1>
+<P>
+<A NAME=.nflag.statist><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/nflag_statist.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>Schematic of the STATIST branch of NFLAG. 
+<BR>This branch accumulates statistical characteristics from the visibilities and/or the noise parameters in the scan headers and provides displays of the results in various formats. </i>
+<P>
+        The purpose of the statistics branch is to provide statistical overviews of the visibility data. Generally speaking, the bulk of the visibilities is much too large for making useful graphic or tabular representations of the individual values (except with NGIDS. For flagging purposes, however, much of the information one needs can be represented in the form of tables of data statistics along various cross-sections of the visibility hypercube. Such tables is what the statistics commands produce.
+<P>
+        A schematic overview of the branch is given in <A HREF=" #.nflag.statist">figure</A>.
+<P>
+        From the STATISTICS branch, it is possible also to make a detour into the INSPECT branch.
+<P>
+<A NAME=.mode.branch><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0009000000000000000>  <b>NFLAGS environment paremeters: The MODE branch</b></A></H1>
+<P>
+<A NAME=.x11><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION00010000000000000000>  <b>Selection of bad visibilities on an X11 display </b></A></H1>
+<P>
+<A NAME=.nflag.gids><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<A HREF="../fig/nflag_gids.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>The use of a flag file to transfer flagging commands into NFLAG. 
+<BR>Flag files contain flagging commands that NFLAG can read and execute. Both a compact binary form (the .FLF file) and a bulky text form are available. The latter form can be edited manually. 
+<BR>Flag files may be generated by NGIDS and through commands in the 
+FLIST branch of NFLAG. </i>
+<P>
+        For detailed point-by-point flagging of visibilities the flagging modes of NFLAG are much too cumbersome. For this purpose one may instead use a combination of 
+ <UL><LI>   NGIDS, to select data points with a cursor on a two-dimensional display of a cross section through the visibility hypercube in which data values are represented by colours;
+<P>
+<LI>   NFLAG, to do the actual flagging of the selected points. 
+ </UL>  The procedure is schematically represented in <A HREF=" #.nflag.gids">figure</A>.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nflag_keys/nflag_keys.html b/nflag_keys/nflag_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..5912dc4497e0804e3fb6245bb93da006dd48ba02
--- /dev/null
+++ b/nflag_keys/nflag_keys.html
@@ -0,0 +1,127 @@
+<TITLE>Index of private keywords for NFLAG </TITLE>
+<H1>Description of keywords for program NFLAG</H1>
+
+<UL>
+<LI> <A HREF="../nflag/nflag__option.html">
+  OPTION</A>
+  NFLAG main branch FLAG; SHOW, QUIT
+<LI> <A HREF="../nflag/nflag__sub_cube.html">
+  SUB_CUBE</A>
+  Type of secondary data cube YES, IFR, POL, HA; NO
+<LI> <A HREF="../nflag/nflag__input_file.html">
+  INPUT_FILE</A>
+  Input .FLF file name (including extension)
+<LI> <A HREF="../nflag/nflag__output_file.html">
+  OUTPUT_FILE</A>
+  Output .FLF file name (including extension)
+<LI> <A HREF="../nflag/nflag__flag_option.html">
+  FLAG_OPTION</A>
+  Type of flagging operation| CLIPDATA, DETERM; CLEAR, MANUAL, HASCANS, FCOPY;|-FLIST; MODE; INSPECT, STATIST, QUIT 
+<LI> <A HREF="../nflag/nflag__flag_mode.html">
+  FLAG_MODE</A>
+   HYPER, SECTORS, NODE; CORR, NOCORR, UFLAG;|-DRYRUN, NODRYRUN, SHOW, NOSHOW, NOTRACE, TRACE; QUIT  "Set ONE environment parameter at a time; QUIT or &lt;CR&gt; when done|" 
+<LI> <A HREF="../nflag/nflag__ops_flist.html">
+  OPS_FLIST</A>
+  Flag-list operation| DELETE, GET, PUT; LOAD, UNLOAD, READ, WRITE; HEADER, LIST, LCOUNT;|-INSPECT, STATIST, MODE, CLEAR, QUIT 
+<LI> <A HREF="../nflag/nflag__ops_manual.html">
+  OPS_MANUAL</A>
+  Manual-flagging operation| CLEAR, CLDAT, CLHEAD; UVDATA, HARANGE; INSPECT, STATIST, MODE, QUIT 
+<LI> <A HREF="../nflag/nflag__ops_fcopy.html">
+  OPS_FCOPY</A>
+  Flag-copy operation TOTEL, TOPOL, TODATA, TOHEAD;|INSPECT, STATIST, MODE, CLEAR, QUIT 
+<LI> <A HREF="../nflag/nflag__ops_scans.html">
+  OPS_SCANS</A>
+  Select scan-statistics flagging criterion | SCANS; MAXABCS; ANOISE, XAN, YAN, RNOISE, XRN, YRN;|-INSPECT, STATIST, MODE, CLEAR, QUIT 
+<LI> <A HREF="../nflag/nflag__ops_clipdata.html">
+  OPS_CLIPDATA</A>
+  Select data-thresholding criterion | AMPL, COS, SIN; ARESID, RRESID; QXY, UXY, VXY; DT1;|-INSPECT, STATIST, MODE, CLEAR, QUIT | 
+<LI> <A HREF="../nflag/nflag__ops_determ.html">
+  OPS_DETERM</A>
+  Select coordinate criterion | SHAD, PBAS , ELEVATION; REDUN, NONRED; INSPECT, STATIST, MODE, CLEAR, QUIT 
+<LI> <A HREF="../nflag/nflag__ops_statist.html">
+  OPS_STATIST</A>
+  "Statistics operation - (ACC, SCANS, UVDAT, &lt;name&gt;;|-GROUPS, EXPLAIN; INSPECT, MODE, QUIT)" 
+<LI> <A HREF="../nflag/nflag__ops_inspect.html">
+  OPS_INSPECT</A>
+   "Projection (COUNT, FTYP, TEL, IFR, HA) with optional '_' plus|-range modifier (X, Y, XY, YX, MAN, CLIP, NOISE, ADD, SHAD, U3, U2, U1, OLD)|-OR navigation control (STATIST, MODE)" 
+<LI> <A HREF="../nflag/nflag__user_flags.html">
+  USER_FLAGS</A>
+  Select flag type(s) for ALL flagging operations| NONE, [ALL]; MAN, CLIP, NOISE, ADD, SHAD, U1, U2, U3; [OLD]
+<LI> <A HREF="../nflag/nflag__user_flag.html">
+  USER_FLAG</A>
+  default flag type(s) NONE, ALL, MAN, CLIP, NOISE, ADD, SHAD, |U1, U2, U3; OLD 
+<LI> <A HREF="../nflag/nflag__select_flag.html">
+  SELECT_FLAG</A>
+  Flag type(s) to use in data selection| NONE, ALL, MAN, CLIP, NOISE, ADD, SHAD , U1, U2, U3; [OLD]
+<LI> <A HREF="../nflag/nflag__put_range.html">
+  PUT_RANGE</A>
+  Ranges for expansion volume around PUT points:|-chan.HA.ifr.pol 
+<LI> <A HREF="../nflag/nflag__put_expand_ch.html">
+  PUT_EXPAND_CH</A>
+  PUT expansion half-width in channel numbers
+<LI> <A HREF="../nflag/nflag__ha.html">
+  HA</A>
+  hour angle range to process (deg)
+<LI> <A HREF="../nflag/nflag__limit.html">
+  LIMIT</A>
+  Flagging threshold
+<LI> <A HREF="../nflag/nflag__clip_limit.html">
+  CLIP_LIMIT</A>
+  Clip threshold (W.U.)
+<LI> <A HREF="../nflag/nflag__clip_limits.html">
+  CLIP_LIMITS</A>
+  Clip limits
+<LI> <A HREF="../nflag/nflag__dt1_limit.html">
+  DT1_LIMIT</A>
+  Discontinuity threshold (W.U. per 10 sec)
+<LI> <A HREF="../nflag/nflag__limits.html">
+  LIMITS</A>
+  flagging limits
+<LI> <A HREF="../nflag/nflag__pbas_limits.html">
+  PBAS_LIMITS</A>
+  Projected-baseline range to be flagged (m)
+<LI> <A HREF="../nflag/nflag__shadow_diam.html">
+  SHADOW_DIAM</A>
+  Telescope shadowing diameter (metres)
+<LI> <A HREF="../nflag/nflag__toh_limit.html">
+  TOH_LIMIT</A>
+  Maximum number of data flags to tolerate per scan
+<LI> <A HREF="../nflag/nflag__dry_scans.html">
+  DRY_SCANS</A>
+  Number of scans to use in trial runs
+<LI> <A HREF="../nflag/nflag__elevation_limit.html">
+  ELEVATION_LIMIT</A>
+  Elevation lower limit (deg)
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nshow_comm/nshow_comm.html">NSHOW</A> </UL>
+
+
+<UL><LI>See also <A HREF="../flfnode_comm/flfnode_comm.html">FLFNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nflag_descr/nflag_descr.html">program NFLAG</A>
+</UL>
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new file mode 100644
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--- /dev/null
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
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--- /dev/null
+++ b/nflag_private_intfc/images.pl
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+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NFLAG</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nflag_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nflag_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nflag_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nflag_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nflag_private_intfc.html#SECTION0003200000000000000>  <b>Parameter ABCS_LIMITS</b></A>
+<LI> <A NAME=tex2html6 HREF=nflag_private_intfc.html#SECTION0003300000000000000>  <b>Parameter CLIP_LIMIT</b></A>
+<LI> <A NAME=tex2html7 HREF=nflag_private_intfc.html#SECTION0003400000000000000>  <b>Parameter CLIP_LIMITS</b></A>
+<LI> <A NAME=tex2html8 HREF=nflag_private_intfc.html#SECTION0003500000000000000>  <b>Parameter DRY_SCANS</b></A>
+<LI> <A NAME=tex2html9 HREF=nflag_private_intfc.html#SECTION0003600000000000000>  <b>Parameter DT1_LIMIT</b></A>
+<LI> <A NAME=tex2html10 HREF=nflag_private_intfc.html#SECTION0003700000000000000>  <b>Parameter ELEVATION_LIMIT</b></A>
+<LI> <A NAME=tex2html11 HREF=nflag_private_intfc.html#SECTION0003800000000000000>  <b>Parameter FLAG_MODE</b></A>
+<LI> <A NAME=tex2html12 HREF=nflag_private_intfc.html#SECTION0003900000000000000>  <b>Parameter FLAG_OPTION</b></A>
+<LI> <A NAME=tex2html13 HREF=nflag_private_intfc.html#SECTION00031000000000000000>  <b>Parameter HA</b></A>
+<LI> <A NAME=tex2html14 HREF=nflag_private_intfc.html#SECTION00031100000000000000>  <b>Parameter INPUT_FILE</b></A>
+<LI> <A NAME=tex2html15 HREF=nflag_private_intfc.html#SECTION00031200000000000000>  <b>Parameter LIMIT</b></A>
+<LI> <A NAME=tex2html16 HREF=nflag_private_intfc.html#SECTION00031300000000000000>  <b>Parameter LIMITS</b></A>
+<LI> <A NAME=tex2html17 HREF=nflag_private_intfc.html#SECTION00031400000000000000>  <b>Parameter OPS_CLIPDATA</b></A>
+<LI> <A NAME=tex2html18 HREF=nflag_private_intfc.html#SECTION00031500000000000000>  <b>Parameter OPS_DETERM</b></A>
+<LI> <A NAME=tex2html19 HREF=nflag_private_intfc.html#SECTION00031600000000000000>  <b>Parameter OPS_FCOPY</b></A>
+<LI> <A NAME=tex2html20 HREF=nflag_private_intfc.html#SECTION00031700000000000000>  <b>Parameter OPS_FLIST</b></A>
+<LI> <A NAME=tex2html21 HREF=nflag_private_intfc.html#SECTION00031800000000000000>  <b>Parameter OPS_INSPECT</b></A>
+<LI> <A NAME=tex2html22 HREF=nflag_private_intfc.html#SECTION00031900000000000000>  <b>Parameter OPS_MANUAL</b></A>
+<LI> <A NAME=tex2html23 HREF=nflag_private_intfc.html#SECTION00032000000000000000>  <b>Parameter OPS_SCANS</b></A>
+<LI> <A NAME=tex2html24 HREF=nflag_private_intfc.html#SECTION00032100000000000000>  <b>Parameter OPS_STATIST</b></A>
+<LI> <A NAME=tex2html25 HREF=nflag_private_intfc.html#SECTION00032200000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html26 HREF=nflag_private_intfc.html#SECTION00032300000000000000>  <b>Parameter OUTPUT_FILE</b></A>
+<LI> <A NAME=tex2html27 HREF=nflag_private_intfc.html#SECTION00032400000000000000>  <b>Parameter PBAS_LIMITS</b></A>
+<LI> <A NAME=tex2html28 HREF=nflag_private_intfc.html#SECTION00032500000000000000>  <b>Parameter PUT_EXPAND_CH</b></A>
+<LI> <A NAME=tex2html29 HREF=nflag_private_intfc.html#SECTION00032600000000000000>  <b>Parameter PUT_RANGE</b></A>
+<LI> <A NAME=tex2html30 HREF=nflag_private_intfc.html#SECTION00032700000000000000>  <b>Parameter SELECT_FLAG</b></A>
+<LI> <A NAME=tex2html31 HREF=nflag_private_intfc.html#SECTION00032800000000000000>  <b>Parameter SHADOW_DIAM</b></A>
+<LI> <A NAME=tex2html32 HREF=nflag_private_intfc.html#SECTION00032900000000000000>  <b>Parameter SUB_CUBE</b></A>
+<LI> <A NAME=tex2html33 HREF=nflag_private_intfc.html#SECTION00033000000000000000>  <b>Parameter TOH_LIMIT</b></A>
+<LI> <A NAME=tex2html34 HREF=nflag_private_intfc.html#SECTION00033100000000000000>  <b>Parameter USER_FLAG</b></A>
+<LI> <A NAME=tex2html35 HREF=nflag_private_intfc.html#SECTION00033200000000000000>  <b>Parameter USER_FLAGS</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NFLAG. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>.
+<P>
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../flfnode_public_intfc/flfnode_public_intfc.html">FLFNODE</A> public keywords 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../nshow_public_intfc/nshow_public_intfc.html">NSHOW</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+</UL>
+<P>
+<A NAME=.abcs.limits><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter ABCS_LIMITS</b></A></H2>
+<P>
+  <em>Prompt:</em> Acceptance range for ABS(cos), ABS(sin)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+    <PRE>
+        An ENTIRE scan will be flagged if for any valid data point in it
+the modulus of either the real (cos) or imaginary (sin) part falls outside the
+acceptance range.
+</PRE>
+<P>
+  <PRE>
+This option allows you to reject scans containing interference peaks, or 'bad'
+data (i.e. abnormally low amplitudes).
+</PRE>
+<P>
+  <PRE>
+NOTES:
+</PRE>
+<P>
+  <PRE>
+     The new setting of the target flag in each scan or data point will
+      OVERRIDE the current one rather than being ORed into it.
+</PRE>
+<P>
+  <PRE>
+     The flags used in selecting valid scans are defined by parameter ?
+SELECT_FLAGS; the default is ALL.
+</PRE> 
+               <em>see parameters <A HREF="#.dry.scans">DRY_SCANS</A>,
+                <A HREF="#.select.flag">SELECT_FLAG</A> </em>
+  <PRE>
+NB: When new thresholds are given, all Scans in the specified data cube are
+(un-)flagged accordingly, including the Scans that were flagged already.
+</PRE>
+<P>
+<A NAME=.clip.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter CLIP_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Clip threshold (W.U.)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+        Specify the threshold value (W.U.) for the clipping criterion
+selected.
+</PRE>
+<P>
+  <PRE>
+The default value shown is three times the rms value calculated in a 'trial
+run' through the first <N> valid (see Note below) scans in the
+primary/secondary data cube. This is intended to be an educated guess at a
+sensible 3-sigma threshold for your operation, but you must make your own
+assessment of the probable suitability of this value.
+</PRE>
+<P>
+  <PRE>
+Notes:
+     The new setting of the target flag in each scan or data point will
+      OVERRIDE the current one rather than being ORed into it.
+</PRE>
+<P>
+  <PRE>
+     The number <N> of dry-run scans is defined by the parameter DRY_SCANS; the
+      default is 25.
+</PRE>
+<P>
+  <PRE>
+     The flags used in selecting valid scans are defined by parameter ?
+SELECT_FLAGS; the default is ALL.
+</PRE> 
+               <em>see parameters <A HREF="#.dry.scans">DRY_SCANS</A>,
+                <A HREF="#.select.flag">SELECT_FLAG</A> </em>
+<P>
+<A NAME=.clip.limits><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter CLIP_LIMITS</b></A></H2>
+<P>
+<em>Prompt:</em> Clip limits<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+        Specify the range within which the test value will be accepted.
+For values outside the range the flag will be set, for those within the range
+it will be cleared.
+</PRE>
+<P>
+  <PRE>
+The default value shown is three times the rms value calculated in a 'trial
+run' through the first <N> valid (see Note below) scans in the
+primary/secondary data cube. This is intended to be an educated guess at a
+sensible 3-sigma threshold for your operation, but you must make your own
+assessment of the probable suitability of this value.
+</PRE>
+<P>
+  <PRE>
+Notes:
+     The new setting of the target flag in each scan or data point will
+      OVERRIDE the current one rather than being ORed into it.
+</PRE>
+<P>
+  <PRE>
+     The number <N> of dry-run scans is defined by the parameter DRY_SCANS; the
+      default is 25.
+</PRE>
+<P>
+  <PRE>
+     The flags used in selecting valid scans are defined by parameter ?
+SELECT_FLAGS; the default is ALL.
+</PRE> 
+               <em>see parameters <A HREF="#.dry.scans">DRY_SCANS</A>,
+                <A HREF="#.select.flag">SELECT_FLAG</A> </em>
+<P>
+<A NAME=.dry.scans><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter DRY_SCANS</b></A></H2>
+<P>
+<em>Prompt:</em> Number of scans to use in trial runs<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+'Clipping' operations need (a) threshold value(s) that is (are) related to the
+magnitude of the data at hand.
+</PRE>
+<P>
+  <PRE>
+The program determines a 'rasonable' default for such cases by performing a
+'trial run' on the first of the scans in the data cube selected. You may
+specify their number here. The trial run evaluates the clipping criterion but
+does NOT modify the .SCN file.  For data with reasonably stationary statistics,
+the default number should be adequate. A larger number obviously will take more
+time to process. If you specify a very large number, the trial run will include
+the entire data cube selected.
+</PRE>
+<P>
+<A NAME=.dt1.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter DT1_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Discontinuity threshold (W.U. per 10 sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+        The DT1 option looks for 'un-physical jumps' in time in the
+cosine and sine values of the uv-data. The actual difference (in W.U.) between
+successive time-samples is divided by the time that separates them, in units of
+the integration time (e.g. 60 sec). The flag is set if this value exceeds the
+threshold.
+</PRE>
+<P>
+<A NAME=.elevation.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter ELEVATION_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Elevation lower limit (deg)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+        Specify the lower limit for acceptable elevations. All points
+corresponding to lower elevations are rejected. The default flag-type is SHADOW.
+</PRE>
+<P>
+<A NAME=.flag.mode><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter FLAG_MODE</b></A></H2>
+<P>
+<em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        You may select one of the options at a time.
+ The logical ones, such as CORR/NOCORR will take effect immediately. For the
+others, you will be prompted for (a) new value(s).  The values shown below as
+defaults are the ones with which NFLAG starts up.
+</PRE>
+<P>
+  <PRE>
+   Redefinition of the primary data cube:
+</PRE>
+<P>
+  <PRE>
+        HYPER:    Change the primary data cube by selecting new polarisation,
+                   interferometer and hour-angle ranges.
+        SECTORS:  As HYPER but including a change of the SCN_SECTORS selection.
+        NODE:     Completely new primary data cube (i.e. including new .SCN
+                   file)
+</PRE>
+<P>
+  <PRE>
+   Data-correction modes. Shown in parentheses is NFLAG's initial setting:
+</PRE>
+<P>
+  <PRE>
+        CORR/NOCORR (=NOCORR):
+                Reading mode for visibility data: without/with corrections
+                 applied and ignoring/acknowledging flags.
+                 (NOCORR mode will be ignored in those cases for which the use
+                 of uncorrected data would be pointless, e.g. ARESID, RRESID).
+</PRE>
+<P>
+  <PRE>
+        UFLAG (=ALL):
+                Default flag types to be acknowledged when reading data in
+                 CORR mode.
+</PRE>
+<P>
+  <PRE>
+   Run modes:
+</PRE>
+<P>
+  <PRE>
+        SHOW/NOSHOW (=SHOW):
+                After each flagging operation, show/don't show a summary of the
+                 new flag settings for the data cube and flag types selected
+for
+                 that operation.
+                Note that in either mode the affected flags will be counted
+                 anyway, so you can use INSPECT afterwards to show summatries
+                 from various perspectives
+</PRE>
+<P>
+  <PRE>
+        DRYRUN/NODRYRUN (=DRYRUN):
+                For any operation that would change flags in the .SCN file,
+                 do/don't do a 'trial run' first, - e.g. to get a feeling for
+                 sensible default values for clip limits etc.
+                 (For NODRYRUN safe default values will be chosen for such
+                 limits so that nothing will happen until the user sets his own
+                 values.)
+</PRE>
+<P>
+  <PRE>
+        NOTRACE/TRACE (=NOTRACE):
+                Dont't/do trace the flagging operations through messages on the
+                 terminal. TRACE is likely to produce a lot of output and
+                 intended for debugging purposes only.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        QUIT:    Go back to FLAG_OPTION.
+</PRE>
+<P>
+<A NAME=.flag.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter FLAG_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Type of flagging operation|<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify the type of flagging operation to be performed:
+</PRE>
+<P>
+  <PRE>
+   Selective flagging on the basis of data/coordinate/statistics values:
+</PRE>
+<P>
+  <PRE>
+        CLIPDATA  Flag data points according to a data-derived criterion
+                   (amplitudes, selfcal residuals, etc.)
+        DETERM    Flag data points on the basis of their coordinates (position,
+                   elevation, etc.)
+</PRE>
+<P>
+  <PRE>
+   Deterministic clearing, setting and copying of flags:
+</PRE>
+<P>
+  <PRE>
+        CLEAR     Clear flags from scan headers and data (see also MANUAL)
+        MANUAL    Manual flagging operations (includes CLEAR flags).
+</PRE> 
+  <PRE>
+        HASCANS   Operations on the scan-header flags. These affect ENTIRE
+                   scans, and in doing so IGNORE the interferometers (parameter
+                   IFRS) and polarisations (parameter SELECT_XYX) selections
+                   that you defined for your primary/secondary data cubes.
+        FCOPY     Copy flags from one place in the hypercube to another.
+</PRE>
+<P>
+  <PRE>
+   Operation on the flag list in core:
+</PRE>
+<P>
+  <PRE>
+        FLIST     Operations on the internal flag list
+                   (including reading-from/writing-to a .FLF file).
+</PRE>
+<P>
+  <PRE>
+   Define operating environment:
+</PRE>
+<P>
+  <PRE>
+        MODE      Go to FLAG_MODE parameter to change 'environment' parameter
+                   values. This includes re-definition of the primary data
+cube.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT   Go to the flag-INSPECTion group of operations.
+        STATIST   Go to the data-STATISTICS group of operations.
+</PRE>
+<P>
+  <PRE>
+        QUIT      Return to primary OPTION.
+</PRE>
+<P>
+<A NAME=.ha><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter HA</b></A></H2>
+<P>
+<em>Prompt:</em> hour angle range to process (deg)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+        Specify the start and end of the HA-range to be processed. If
+only one value is given, the end value will be the same.
+</PRE>
+<P>
+<A NAME=.input.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter INPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> Input .FLF file name (including extension)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the full name of the input binary-flags file. The
+recommended filename extension is .FLF.
+</PRE>
+<P>
+<A NAME=.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Flagging threshold<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+        Specify the limit threshold value for the (un)flag criterion
+selected. The units (e.g. W.U.) are those appropriate for the criterion.
+</PRE>
+<P>
+<A NAME=.limits><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter LIMITS</b></A></H2>
+<P>
+<em>Prompt:</em> flagging limits<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+        Specify the LOWER and UPPER limiting values for the (un-)flag
+criterion. The unit (e.g. W.U.) depends on the criterion under consideration.
+</PRE>
+<P>
+<A NAME=.ops.clipdata><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter OPS_CLIPDATA</b></A></H2>
+<P>
+<em>Prompt:</em> elect data-thresholding criterion |<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Remember that only the primary data cube is affected.
+</PRE>
+<P>
+  <PRE>
+The following operations flag individual data points, according to a flagging
+criterion that is derived from the visibilities themselves. You will be
+prompted for an upper limit. For each visibility point exceeding the limit the
+flag will be set if it exceeds the limit, for the others it will be cleared:
+Current flags are NOT preserved.
+</PRE>
+<P>
+  <PRE>
+The flag type is CLIP, unless you have defined your own type through the
+USER_FLAGS parameter.
+</PRE>
+<P>
+  <PRE>
+   Flagging on straight data values exceeding the threshold. These criteria are
+   intended for use with CORRECTED data (Parameter FLAG_MODE=CORR).
+</PRE>
+<P>
+  <PRE>
+        AMPL    Threshold applies to absolute value
+        COS     Threshold applies to real (cosine) part.
+        SIN     Threshold applies to imaginary (sine) part.
+</PRE>
+<P>
+  <PRE>
+   Flagging on Selfcal/Redundancy residuals. You will be prompted to specify
+the
+   Selfcal source model used in the latest NCALIB SEFCAL/REDUN run.
+   (NOTE that the residuals here are VECTOR differences between observation
+    and source model; this definition is different from that used by NPLOT.)
+</PRE>
+<P>
+  <PRE>
+        ARESID  Threshold applies to the magnitude of the residual
+        RRESID  Threshold is the absolute difference of the residual's
+magnitude
+                 from the average magnitude of all residuals in the scan for
+the
+                 same baseline. (In short: This flags outliers in sets of
+                 redundant baselines.)
+                NOTE: This operation can be performed even on uncalibrated
+data,
+                 provided a source model is available.
+</PRE>
+<P>
+  <PRE>
+   Flagging on polarisation-related criteria:
+</PRE>
+<P>
+  <PRE>
+        QXY     Threshold applies to the magnitude of the difference between XX
+                 and YY visibilities per interferometer (i.e. magnitude of
+                 Stokes Q for parallel dipoles).
+        UXY     Threshold applies to ABS(XY-YX) per interferometer
+                 (i.e. ABS(U) if the dipoles are parallel).
+        VXY     Threshold applies to ABS(j(XY+YX)) per interferometer
+                 (i.e. ABS(V) if the dipoles are parallel).
+</PRE>
+<P>
+  <PRE>
+                For unpolarised sources, this criterion should be as effective
+                 as ARESID above.
+</PRE>
+<P>
+  <PRE>
+   Flagging on discontinuities in time. The flags raised here serve only as an
+   ALERT that there is a 'jump' in the data; you will have to decide yourself
+   what to do about the problem.
+</PRE>
+<P>
+  <PRE>
+        DT1     Threshold is the difference in amplitude of a data point with
+                 its counterpart in the preceding scan.
+</PRE>
+<P>
+  <PRE>
+  Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the environment MODE-control section of the
+                 program
+        CLEAR   Go to the CLEAR-flags operation.
+        QUIT    Return to FLAG_OPTION.
+</PRE>
+<P>
+<A NAME=.ops.determ><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter OPS_DETERM</b></A></H2>
+<P>
+<em>Prompt:</em> Select coordinate criterion |<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Remember that only the primary data cube is affected.
+</PRE>
+<P>
+  <PRE>
+   Flagging of data points on the basis of their coordinates. The flag type is
+   SHADOW, unless you have selected your own type (parameter FLAG_MODE).
+</PRE>
+<P>
+  <PRE>
+        SHAD      In each scan, flag all data that are affected by 'shadowing',
+                   i.e. all interferometers in which the aperture of either
+                   telecope is partly blocked by another telescope in the line
+                   of sight.
+</PRE>
+<P>
+  <PRE>
+        PBAS      Flag all data for which the length of the projected baseline
+                   is within a range (for which you will be prompted). This is
+a
+                   way to eliminate short baselines susceptible to
+interference,
+                   without losing more data than necessary.
+</PRE>
+<P>
+  <PRE>
+        ELEVATION Flag all uv-data that have been taken at elevations below a
+                   limit (for which you will be prompted).
+</PRE>
+<P>
+  <PRE>
+        REDUN     Flag all redundant baselines.
+        NONRED    Flag all non-redundant baselines.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the enviornment MODE-control section of the
+                 program
+        CLEAR   Go to the CLEAR-flags operation.
+        QUIT    Return to FLAG_OPTION.
+</PRE>
+<P>
+<A NAME=.ops.fcopy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter OPS_FCOPY</b></A></H2>
+<P>
+<em>Prompt:</em> Flag-copy operation<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        FCOPY propagates flags of the selected type from individual
+interferometers to groups of interferometers that have something in common with
+the flagged ones.
+</PRE>
+<P>
+  <PRE>
+Flags are looked for in the entire primary data cube, but changes affect only
+the primary/secondary cube. Make sure that you understand which of the 8 flag
+types are affected
+</PRE>
+<P>
+  <PRE>
+   Operations that modify flags on individual data points:
+</PRE>
+<P>
+  <PRE>
+        TOTEL  Copy flags from interferometers to telescopes: For each scan
+                selected, flag all data that share a dipole (X or Y channel of
+                a telescope) with any interferometer for which the flag
+                selected is set.
+</PRE>
+<P>
+  <PRE>
+        TOPOL  Copy flags to all polarisations: For each scan selected, flag
+all
+                polarisations of all telescope pairs for which the flag
+selected
+                is already set for at least one of them. (This is a sort of
+                mini-PUT).
+</PRE>
+<P>
+  <PRE>
+   Operations that affect ENTIRE scans. NOTE that these IGNORE ANY SELECTIONS
+   you have defined for interferometers (parameter IFRS) and/or polarisations
+   (parameter SELECT_XYX).
+</PRE> 
+               <em>see the dictinction between 
+               data and header flags </em>
+<P>
+  <PRE>
+        TOHEAD  For each flag selected, set the scan-header flag if it is set
+                 for more than a given number (paremeter TOH_LIMIT) of data
+                 points.
+                This invalidates the entire scan. The operation is reversible
+                 (parameter OPS_MANUAL = CLHEAD); the individual data flags
+                 are not affected.
+</PRE> 
+                       <em>See parameters <A HREF="#.toh.limit">TOH_LIMIT</A>,
+                       <A HREF="#.ops.manual">OPS_MANUAL</A> </em>
+<P>
+  <PRE>
+        TODATA  Transfer flags of the type selected from the header of each
+scan
+                 to all the scan's data, deleting them in the headers.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the enviornment MODE-control section of the
+                 program
+        CLEAR   Go to the CLEAR-flags operation.
+        QUIT    Return to FLAG_OPTION.
+</PRE>
+<P>
+<A NAME=.ops.flist><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter OPS_FLIST</b></A></H2>
+<P>
+<em>Prompt:</em> Flag-list operation|<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify operations on the internal flag list: The entries in
+this list represent flagging instructions. Each entry contains a flag type, and
+ranges for the secondary data cube (i.e. hour angle, polarisation,
+interferometer and channel ranges) to which it applies.
+</PRE>
+<P>
+  <PRE>
+   Flagging operations involving the internal flag list:
+</PRE>
+<P>
+  <PRE>
+        DELETE  Clear the entire list.
+</PRE>
+<P>
+  <PRE>
+        GET     Collect flags of specified type(s) from the specified primary
+                 data cube, translate them into flaqg-list entries and merge
+                 them into the list.
+                The default flag type is ALL, but it can be changed (parameter
+                 FLAG_MODE).
+</PRE> 
+                       <em>see paremeter FLAG_MODE</em>
+<P>
+  <PRE>
+        PUT     Use he entries in the internal flag list to set flags for
+                 selected visibilities or scans.
+                If an entry in the list results in setting the flags on all
+data
+                 points in a scan, the corresponding scan-header flag is set
+                 instead for efficiency reasons.
+</PRE>
+<P>
+  <PRE>
+   Transfer of the flag list to/from an external file. Two types of file may be
+   used:
+</PRE>
+<P>
+  <PRE>
+      The .FLF file is in a compact binary format that is efficient in both
+      operating speed and disk-space. It is accessed through:
+        LOAD    Merge contents of a .FLF file into the internal flag list
+        UNLOAD  Write the internal flag list to a new .FLF file
+</PRE>
+<P>
+  <PRE>
+     The list can also be stored in an ASCII file which you can inspect and
+edit
+     as you please. ASCII files are bulky and take much more time to process.
+     They are accessed through:
+        READ    Merge contents of an ASCII flag-list file into the internal
+flag
+                 list
+        WRITE   Write the internal flag list to a new ASCII flag-list file
+</PRE>
+<P>
+  <PRE>
+   Inspection:
+</PRE>
+<P>
+  <PRE>
+        HEADER  Show the contents of the flag-list header.
+        LIST    Show the contents of the flag-list (can be long).
+</PRE> 
+  <PRE>
+        LCOUNT  Count the flags in the flag list (NOT in the data).
+                 These can be INSPECTed in various one-dimensional projections.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the environment MODE-control section of the
+                 program
+        CLEAR   Go to the CLEAR-flags operation.
+        QUIT    Go back to what you were doing before.
+</PRE>
+<P>
+<A NAME=.ops.inspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter OPS_INSPECT</b></A></H2>
+<P>
+<em>Prompt:</em> &quot;-<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Count and inspect flags in the primary data cube. A complete reply consists of
+one of the primary options plus a modifier suffix.
+</PRE>
+<P>
+  <PRE>
+   Count flags (no modifier):
+</PRE>
+<P>
+  <PRE>
+        COUNT   Count the flags of all types that are set, for subsequent
+                 inspection.
+                You may define a secondary data cube for this operation
+                By default, flags of all types are counted; you may change this
+                 (parameter FLAG_MODE).
+</PRE>
+<P>
+  <PRE>
+   Show the flag counts in various data-cube dimensions (<mod> stands for one
+of
+   the optional modifiers listed below):
+</PRE>
+<P>
+  <PRE>
+        FTYP_<mod>  Show the counts per flag-type (data and headers).
+        TEL_<mod>   Show the counts per telescope.
+        IFR_<mod>   Show the counts per interferometer.
+        HA_<mod>    Show the counts per hour-angle (total over all
+                     interferometers and polarisations).
+</PRE>
+<P>
+  <PRE>
+     Modifiers: You may limit the display of counts to a sub-set through one of
+     the following modifiers (prefixed with an underscore, e.g. TEL_SHAD, or
+     HA_XX). The display will be equivalent to that for a secondary cube
+     covering the same selection.
+</PRE>
+<P>
+  <PRE>
+        X, Y            XX alone, YY alone
+        XY, YX          only XX and YY, only XY and YX
+        MAN, CLIP, NOIS, ADD, SHAD, U3, U2, U1, OLD
+                        for one flag type
+        <interferometer designation>
+                        for a (group of) interferometer(s), e.g. FTYP_9A, HA_8*
+        <telescope>
+                        for a (group of) telescope(s), e.g. FTYP_8
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the enviornment MODE-control section of the
+                 program
+        QUIT    Back out from INSPECT: Return to what you were doing before.
+</PRE>
+<P>
+<A NAME=.ops.manual><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031900000000000000>  <b>Parameter OPS_MANUAL</b></A></H2>
+<P>
+<em>Prompt:</em> Manual-flagging operation|<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify one of the manual flagging operations. Remember that
+only the selected primary/secondary data cube is affected. Make sure that you
+understand which of the 8 flag types are affected.
+</PRE>
+<P>
+  <PRE>
+   Clear flags. You will be prompted for the flag-type(s) to be cleared:
+   BEWARE! Much work can be undone with careless clearing
+</PRE>
+<P>
+  <PRE>
+        CLEAR   Clear all flags of the specified type(s) in both the
+                 scan headers and the uv data of the selected cube.
+</PRE> 
+  <PRE>
+        CLDAT   Clear flags on the visibilities only (i.e. leave scan headers
+                 alone).
+        CLHEAD  Clear flags in the scan headers only.
+</PRE>
+<P>
+  <PRE>
+   Set flags:
+</PRE>
+<P>
+  <PRE>
+        UVDATA  Set flags of the specified type(s) in the individual
+                 visibilities, for selected interferometer(s) within the
+primary
+                 data cube.
+                Default flag type is MANUAL, but can be overridden (parameter
+                 FLAG_MODE).
+        HARANGE Set flags of the specified type(s) on the individual
+                 visibilities, for selected interferometer(s) within the
+primary
+                 data cube.
+                Default flag type is MANUAL, but can be overridden (parameter
+                 FLAG_MODE).
+                You will be repeatedly prompted for an hour-angle range.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the enviornment MODE-control section of the
+                 program
+        CLEAR   Go to the CLEAR-flags operation.
+        QUIT    Return to FLAG_OPTION prompt.
+</PRE>
+<P>
+<A NAME=.ops.scans><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032000000000000000>  <b>Parameter OPS_SCANS</b></A></H2>
+<P>
+<em>Prompt:</em> elect scan-statistics flagging criterion |<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        The operations available here flag scan headers and thereby
+affect ENTIRE scans; in doing so they IGNORE ANY SELECTIONS you have defined
+for interferometers (parameter IFRS) and/or polarisations (parameter
+SELECT_XYX). Apart from this, only those scans that overlap with the primary
+data cube are affected.
+</PRE>
+<P>
+  <PRE>
+For each of the options an appropriate flag is selected, as noted below. If you
+have defined your own selection through the USER_FLAGS parameter, that
+selection will override NFLAG's defaults.
+</PRE> 
+                       <em>see <A HREF="#.flag.mode">FLAG_MODE</A> </em>
+<P>
+               <em>see the dictinction between
+               data and header flags </em>
+<P>
+  <PRE>
+   Flagging the scans that you select.
+</PRE>
+<P>
+  <PRE>
+        SCANS   Flag scans manually; you will be given the option to select a
+                 secondary data cube for this operation.
+</PRE>
+<P>
+  <PRE>
+   Flagging on data statistics. The default flag type is CLIP.
+</PRE>
+<P>
+  <PRE>
+        MAXABCS Flag all scans in which the modulus of either the real (cosine)
+                 or imaginary (sine) part of any visibility falls outside a
+                 range to be specified.
+</PRE>
+<P>
+  <PRE>
+   Flagging on noise statistics. The default flag type is NOISE.
+</PRE>
+<P>
+  <PRE>
+        ANOISE  Flag all scans in which any of the four noise values (X/Y
+                 gain/phase) recorded in the latest NCALIB ALIGN or SELFCAL
+                 operation exceeds a threshold (yet to be prompted for).
+</PRE>
+<P>
+  <PRE>
+        XAN,YAN As ANOISE, but checking only the X resp. Y noise values.
+</PRE>
+<P>
+  <PRE>
+        RNOISE  Flag all scans in which any of the four noise values (X/Y
+                 gain/phase) recorded in the latest NCALIB REDUN operation
+                 exceeds a threshold (yet to be prompted for).
+</PRE>
+<P>
+  <PRE>
+        XRN,YRN As RNOISE, but checking only the X resp. Y noise values.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        STATIST Make detour into the (data) STATISTics section of the program
+        MODE    Make detour into the enviornment MODE-control section of the
+                 program
+        CLEAR   Go to the CLEAR-flags operation.
+        QUIT    Return to FLAG_OPTION.
+</PRE>
+<P>
+<A NAME=.ops.statist><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032100000000000000>  <b>Parameter OPS_STATIST</b></A></H2>
+<P>
+<em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Accumulate statistics from data and/or scan headers over the
+primary or secondary data cube and display it.
+</PRE>
+<P>
+  <PRE>
+   Accumulate:
+        ACC     Accumulate statistics from data and scan headers, excluding
+data
+                 points/headers that are flagged.
+                You may select a secondary data cube for this purpose
+(parameter
+                 XXX).
+</PRE>
+<P>
+  <PRE>
+   Inspect the results of accumulation:
+</PRE>
+<P>
+  <PRE>
+        SCANS   Show the collected scan-header statistics.
+        UVDAT   Show the collected visibility statistics.
+        <name>  Show the statistics of the named 'accumulation group' (use
+                 GROUPS and EXPLAIN above to see what choices you have).
+</PRE>
+<P>
+  <PRE>
+   These options will produce a Table with the following columns:
+</PRE>
+<P>
+  <PRE>
+        <name>  The name of the quantity for which statistics have been
+                 calculated.
+        mean    Its average value
+        rms     Its rms magnitude
+        rmsms   Its rms deviation w.r.t. the mean.
+        rmsvar  The rms difference, between pairs of successively processed
+                 values.
+        wtot    Total weight. Usually it indicates the total nr of samples.
+        minval  Its minimum value.
+        maxval  Its maximum value.
+        <unit>  The units in which the above values (except wtot) are
+expressed.
+</PRE>
+<P>
+  <PRE>
+   Get some extra help:
+</PRE>
+<P>
+  <PRE>
+        GROUPS  Show the names of the currently defined 'accumulation groups'
+        EXPLAIN Show explanation of statistical quantities.
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+</PRE>
+<P>
+  <PRE>
+        INSPECT Make detour into the (flag) INSPECTion section of the program
+        MODE    Make detour into the enviornment MODE-control section of the
+                 program
+        QUIT    Go back to what you were doing before.
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032200000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> NFLAG main branch<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify the nature of the operation you want to perform:
+</PRE>
+<P>
+  <PRE>
+        FLAG:    Set, clear and/or browse data flags in a .SCN file
+                  and/or browse its data statistics
+</PRE>
+<P>
+  <PRE>
+        SHOW:    Show/edit data and header information in .SCN file. This
+option
+                  is a clone of the SHOW option in NSCAN and is available here
+                  for convenience.
+</PRE>
+<P>
+  <PRE>
+        QUIT:    Terminate NFLAG
+</PRE>
+<P>
+<A NAME=.output.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032300000000000000>  <b>Parameter OUTPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> Output .FLF file name (including extension)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the full name for the output binary-flags file. The
+recommended filename extension is .FLF.
+</PRE>
+<P>
+<A NAME=.pbas.limits><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032400000000000000>  <b>Parameter PBAS_LIMITS</b></A></H2>
+<P>
+<em>Prompt:</em> Projected-baseline range to be flagged (m)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+        Specify the range of lengths of PROJECTED baseline to be
+flagged. The default flag-type is SHADOW.
+</PRE>
+<P>
+  <PRE>
+Short baselines are more sensitive to interference. In flagging them wholesale,
+however, one also loses visibility data representing extended source structure;
+a more selective procedure is to be preferred.
+</PRE>
+<P>
+  <PRE>
+Another application of this parameter is to force a uv coverage that is more
+nearly circular in the PROJECTED uv plane, and hence produces a more circularly
+symmetric antenna pattern. To this end, set the lower limit less than or equal
+to
+</PRE>
+<P>
+  <PRE>
+        <longest baseline> * sin DEC
+</PRE>
+<P>
+  <PRE>
+Instead of permanently modifying the .SCN file in this way, one may use the
+NMAP parameters CWEIGHT_TYPE and CWEIGHT_VALUE to achieve a similar effect.
+</PRE> 
+               <em>see NMAP public paremeter
+                <A HREF="../nmap_public_keys/nmap_public_keys.html#.cweight.type">CWEIGHT_TYPE</A> </em>
+<P>
+  <PRE>
+Examples:
+        PBAS_LIMITS = 0, 288
+</PRE>
+<P>
+  <PRE>
+   causes all projected baselines up to 288 m (inclusive) to be flagged.
+</PRE>
+<P>
+  <PRE>
+   For a source at a declination of 30 deg,
+</PRE>
+<P>
+  <PRE>
+        PBAS_LIMITS = 1500, 10000
+</PRE>
+<P>
+  <PRE>
+   will flag projected baselines longer than 1500 m.
+</PRE>
+<P>
+<A NAME=.put.expand.ch><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032500000000000000>  <b>Parameter PUT_EXPAND_CH</b></A></H2>
+<P>
+<em>Prompt:</em> PUT expansion half-width in channel numbers<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+        PUT performs flagging commands from the internal flag list on
+your primary data cube. Each command consists of a flag/unflag mask plus ranges
+in the frequency-
+channel, interferometer, polarisation and hour-angle 'dimensions' of the TARGET
+points to which it must be applied.
+</PRE>
+<P>
+  <PRE>
+You have activated PUT's option to EXPAND, within the limits of the primary
+data cube, the operation over a 4-dimensional volume of data around each target
+point. You may now select the number of channels on either side of a target
+channel over which you want to expand the flagging.  Example:
+        If you reply 2, a total of 5 channels centered on each target channel
+will be flagged: two above and two below the target.
+</PRE>
+<P>
+<A NAME=.put.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032600000000000000>  <b>Parameter PUT_RANGE</b></A></H2>
+<P>
+<em>Expected input:</em> Character *8:  1 to 4 values
+<P>
+  <PRE>
+        PUT performs flagging commands from the internal flag list on
+your primary data cube. Each command consists of a flag/unflag mask plus ranges
+in the frequency-
+channel, interferometer, polarisation and hour-angle 'dimensions' of the TARGET
+points to which it must be applied.
+</PRE>
+<P>
+  <PRE>
+PUT has the capability to EXPAND, within the limits of the primary data cube,
+the operation over a 4-dimensional volume of data around each target point.
+The extension volume is specified through RANGES along the channel, hour-angle,
+interferometer and polarisation axes in this order. Except for interferometers,
+a range is formulated in terms of units of sequential position rather than
+physical coordinates. It can be one of the foloowing:
+</PRE>
+<P>
+  <PRE>
+   .            do not extend along this axis
+   *            extend to all positions along this axis
+   <n> or <n>C  extend over <n>/2-1 positions on either side (incrementing <n>
+                 if it is even)
+   <n>L         extend over <n>-1 positions to the 'left' (i.e. toward lower
+                 coordinates)
+   <n>R         extend over <n>-1 fields to the 'right' (i.e. toward higher
+                 coordinates)
+</PRE>
+<P>
+  <PRE>
+   The following special notations can also be used in each dimension:
+</PRE>
+<P>
+  <PRE>
+        <n>=0   suppress flagging altogether (length of the nextension cube is
+                 zero)
+        <n>=1   identical to . (length of extension cube is 1: no extension)
+   The following shorthand can be used for the entire reply:
+</PRE>
+<P>
+  <PRE>
+        *       short for 1,1,1,1 or .,.,., (You may do better to avoid this
+                 form because this use of a wildcard character is anomalous.)
+</PRE>
+<P>
+  <PRE>
+?  The interferometer range works on telescope basis, i.e. the given range is ?
+  valid for both receptors (e.g. 0Y and AX).
+</PRE>
+<P>
+  <PRE>
+Example:
+        If a particular ineterferometer is flagged in one of frequency
+channels,
+                PUT_RANGE= *,.,.,.
+ will propagate the flag to all channels for that interferometer
+</PRE>
+<P>
+<A NAME=.select.flag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032700000000000000>  <b>Parameter SELECT_FLAG</b></A></H2>
+<P>
+<em>Prompt:</em> Flag type(s) to use in data selection|<BR><em>Expected input:</em> Character *16:  1 to 16 values
+<P>
+  <PRE>
+        Some operations test flags in selecting data. By default, NFLAG
+selects the test flags appropriate to each operation; only those data are
+accepted for which these flags are CLEAR.
+</PRE>
+<P>
+  <PRE>
+You may define here an alternative (set of) flag type(s) to be used in ALL
+subsequent testing operations; you may select more than one, separated by
+commas. Reply NONE to revert to the default settings.
+</PRE>
+<P>
+  <PRE>
+   ALL or *     test all flag types
+   MAN          test the flag type for the MANUAL class of operations
+   CLIP         test the flag type for the CLIP class of operations
+   NOISE        test the flag type for the NOISE class of operations
+   ADD          test the flag type for the ADDITIVE class of operations
+   SHAD         test the flag type for the SHADOW class of operations
+   U1, U2, U3   'user' flag types, i.e. types you may use as you please
+   NONE         revert to NFLAG's default types per operation
+</PRE>
+<P>
+  <PRE>
+   OLD          the flag type for the 'OLD' class (i.e. flagged before
+                 930609, and converted with NVS option)
+                 NB: OLD uses the same flag-bit as MAN
+</PRE>
+<P>
+<A NAME=.shadow.diam><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032800000000000000>  <b>Parameter SHADOW_DIAM</b></A></H2>
+<P>
+<em>Prompt:</em> Telescope shadowing diameter (metres)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+        Specify the diameter (m) of the telescopes.
+</PRE>
+<P>
+  <PRE>
+A telescope is 'shadowed' as soon as part of its aperture gets blocked by the
+presence of another telecope in its line of sight. This condition occurs when
+the projected baseline between the two telecopes becomes less than the
+telescope diameter D (25 m for the WSRT). If you want to retain as much as
+possible of your data, you may specify a somewhat smaller number (e.g. 0.8 D)
+to take into account the fact that the edge of the aperture is only weakly
+illuminated.
+</PRE>
+<P>
+  <PRE>
+For the hour-angles at which a telescope is shadowed, all intreferometers are
+flagged of which it is a part. The default flag-type is SHADOW.
+</PRE>
+<P>
+  <PRE>
+  ? Another flag may be selected through the FLAG_MODE parameter.
+</PRE>
+<P>
+<A NAME=.sub.cube><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032900000000000000>  <b>Parameter SUB_CUBE</b></A></H2>
+<P>
+<em>Prompt:</em> Type of secondary data cube<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        You may define a 'secondary cube' that includes only part of the
+primary data cube. The current flagging operation will affect only the cross
+section of the primary and secondary cubes.
+</PRE>
+<P>
+  <PRE>
+Unlike the primary cube (which can only be redefined through the FLAG_MODE
+parameter), the secondary cube definition applies only to the current operation
+and will evaporate when it completes.
+</PRE>
+<P>
+  <PRE>
+Specify here how you want to define the secondary cube. You may give ONE option
+at a time; the prompt will reappear until you reply with NO.
+</PRE>
+<P>
+  <PRE>
+        YES  Polarisations, interferometers and hour-angle range.
+        IFR  Interferometers
+        POL  Polarisations
+        HA   Hour-angle range
+        NO   Accept the current settings
+</PRE>
+<P>
+<A NAME=.toh.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033000000000000000>  <b>Parameter TOH_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Maximum number of data flags to tolerate per scan<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+        NFLAG will check in each scan the number of points for which the
+flag type selected is set. If that number exceeds this value you define here,
+the entire scan will be flagged. This will subsequently result in faster
+processing
+(because individualdata points need not be tested) at the expense of the loss
+of some healthy data.
+</PRE>
+<P>
+  <PRE>
+The operation of setting header flags is reversible: The individual data flags
+are retained so you can restore the present condition by clearing the header
+flags.
+</PRE>
+<P>
+<A NAME=.user.flag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033100000000000000>  <b>Parameter USER_FLAG</b></A></H2>
+<P>
+<em>Prompt:</em> default flag type(s)<BR><em>Expected input:</em> Character *16:  1 to 16 values
+<P>
+  <PRE>
+        Specify the default flag type(s) for flagging operations.
+</PRE>
+<P>
+  <PRE>
+    NONE:      no flag type specified (i.e. use default types)
+    ALL or *   all flag types (not very useful)
+    MAN        flag type for the MANUAL class of operations
+    CLIP       flag type for the CLIP class of operations
+    NOISE      flag type for the NOISE class of operations
+    ADD        flag type for the ADDITIVE class of operations
+    SHAD       flag type for the SHADOW class of operations
+    U1, U2, U3 'user' flag types, i.e. types you may use as you please
+</PRE>
+<P>
+  <PRE>
+Note:   Flags U1, U2, U3 can be used to experiment with some flagging operation
+        without affecting the flag type that is 'officially' associated
+        with the same operation.
+</PRE>
+<P>
+  <PRE>
+    OLD        use the flag type for the 'OLD' class (i.e. flagged before
+                930609, and converted with NVS option)
+                NB: OLD uses the same flag-bit as MAN
+</PRE>
+<P>
+<A NAME=.user.flags><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033200000000000000>  <b>Parameter USER_FLAGS</b></A></H2>
+<P>
+<em>Prompt:</em> Select flag type(s) for ALL flagging operations|<BR><em>Expected input:</em> Character *16:  1 to 16 values
+<P>
+  <PRE>
+        Each flagging operation changes a specific flag type by default.
+You may define here an alternative (set of) flag type(s) to be used in ALL
+subsequent flagging operations. Reply NONE to revert to the default settings.
+</PRE>
+<P>
+  <PRE>
+The purpose is to allow you to do experimental flagging with one of the USER
+flags without messing up the flagging that you have already done.
+</PRE>
+<P>
+  <PRE>
+        OLD     use the flag type for the 'OLD' class (i.e. flagged before
+                 930609, and converted with NVS option)
+                 NB: OLD uses the same flag-bit as MAN
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+<TITLE>Newstar configuration management at NFRA</TITLE>
+
+<BR><STRONG>Subject:</STRONG> Newstar configuration management at NFRA
+<BR><STRONG>Author:</STRONG>  Marco de Vos (CMV) and Henk Vosmeyer (HjV)
+<BR><STRONG>To:</STRONG>      Newstar Support Team (HjV, CMV, JEN, JPH)
+<P> <STRONG>Date:</STRONG>    08/11/94 
+<P>
+<EM>Revision history</EM>
+<UL>
+<LI>22/01/96 - Change appendix 3
+<LI>11/11/94 - Add appendix 3
+<LI>08/11/94 - Typo's and minor changes
+<LI>02/11/94 - Separation of NFRA-Master and Export-Master
+<LI>04/03/94 - First release 
+<LI>21/02/94 - Prerelease
+</UL>
+
+
+<H1>Newstar configuration management at NFRA</H1>
+<PRE></PRE>
+
+
+<H2>General concerns</H2>
+
+The Newstar package is not a static product. Major and minor changes are 
+often being made to the software. These changes should affect the use of
+the package in a positive sense only. Therefore we need to guard the
+integrity of the package at NFRA and define clear procedures for external
+users on how to upgrade their implementation. This document describes
+those procedures. 
+<P>
+This document is limited to configuration management on the Unix systems.
+The VAX system will be no longer supported at NFRA from 15/03/94, and 
+can be maintained through the perl-scripts provided by WNB.
+<P>
+Reference to Newstar directories are made through the usual variables 
+$n_src, $n_root etc. Refer to Appendix 2 for the details. 
+<P>
+All commands assume one is logged in as the Newstar Master (newstar).
+<PRE></PRE>
+
+<H2>What makes up the Newstar configuration at NFRA</H2>
+
+The Newstar configuration at NFRA consists of the following:
+<P>
+<UL>
+  <LI><STRONG>The NFRA-Master system</STRONG> on the /newstar disk (below $n_root):
+  <OL>
+    <LI>The Master source tree (below $n_src)
+    <LI>The NFRA library and executable areas ($n_inc, $n_lib,
+             $n_exe and $n_tst for the various architectures)
+    <LI>The NFRA documentation area ($n_hlp)
+    <LI>The NFRA import area (below $n_import)
+  </OL>
+  <P>
+    Below /newstar/master we also have an installation of: (1) mongo (in
+    /newstar/master/mongo), of (2) perl (in /newstar/master/perl) and 
+    (3) a copy of the sources for the VAX-based Remote Tape Daemon (in
+    /newstar/master/rmtd).
+  <P>  
+    This is a working system, used by NFRA users and programmers.
+  <P>
+  <LI><STRONG>The Export-Master system</STRONG> on the /users disk of ftp.astron.nl:
+  <OL>
+    <LI>The Export Master source tree           (below $n_src)
+    <LI>The Server version of the documentation (below $n_www)
+      <UL>
+        <LI>server homepage            $n_www/homepage.html
+        <LI>documentation relevant to the Export Master source tree
+                                       $n_www/hlp/
+        <LI>user feedback system       $n_www/bug/
+        <LI>link to mail area          $n_www/mail/
+      </UL>
+    <LI>Some server programs for ftp.astron.nl    (below /users/newstar)
+    <LI>The import area for sites outside NFRA  (/users/ftp/newstar/import)
+  </OL>
+  <P>
+    This is a sources-only system which is never compiled.
+    The Export Master source tree and the documentation are kept
+    up-to-date from the NFRA Master system.
+  <P>
+  <LI><STRONG>The Newstar account</STRONG> on the NFRA Unix system (~newstar)
+  <OL>
+    <LI>Startup files for the newstar account (.cshrc and .login etc.). These 
+        files should not contain commands that are essential for the 
+        functioning of newstar apart from PATH settings and 
+        the startup command:
+<PRE>
+#
+# Initialise Newstar (either NFRA-Master or Export-Master)
+#
+if (-e  /newstar/master/src/sys/newstar_nfra.csh) then
+ source /newstar/master/src/sys/newstar_nfra.csh
+else if (-e /users/newstar/bin/newstar_init.csh) then
+ source     /users/newstar/bin/newstar_init.csh
+endif
+</PRE>
+
+    <LI>Mail environment (~/Mail and ~/.elm). The elm
+        alias friends_of_newstar is used to inform on updates. The Newstar
+        environment variable $n_master points to this eMail account.
+    <LI>Server interface (~/server). This directory is used to pass commands
+        to the server programs on ftp.astron.nl
+  </OL>
+  <P>
+    This account is the owner of the NFRA-Master and the Export-Master, and
+    is the only account that can modify them (apart from $n_import and the
+    locking database).
+</UL>
+<PRE></PRE>
+
+<H2>Relations between NFRA-Master and Export-Master</H2>
+
+The dynamic relations between Master systems (either the NFRA Master or
+another one) and Export-Master are as follows:
+<PRE>
++----------------------------------------------------------------------+
+|  Master:                                                             |
+|                 $n_src      <--------+                               |
+|                   |                  | nup build -U (in $n_import)   |
+|                   | nup build -U     |                               |
+|                   v                  |                               |
+|                 $n_exe, ... <--------+                               |
+|                                      |                               |
+|                 $n_import -->--------+                               |
+|                  | ^   ^^                                            |
+|                  | |   ||                                            |
+|                  | |   || (NFRA only)                                |
+|                  | |   |+--------------------+--<-- nsh in           |
+|                  | |   |                     |                       |
++----------------------------------------------------------------------+
+|  Export-Master:  | |   |                     |                       |
+|                  | |   | nup retrieve ...    | (NFRA and others)     |
+|                  | |   |  (NFRA only)        |                       |
+|      nup release | |   |                     |                       |
+|                  | | nup retrieve            |                       |
+|                  v |   |                     |                       |
+|                 $n_src |                     |                       |
+|                 $n_import <------------------+                       |
+|                                                                      |   
++----------------------------------------------------------------------+
+</PRE>
+Use of the "<TT>nup release</TT>" command is restricted to the NFRA-Master.
+Master systems outside NFRA use the "<TT>nup retrieve</TT>" command to get 
+updated files from the Export-Master. The "<TT>nup update</TT>" command 
+combines "<TT>nup retrieve</TT>" and "<TT>nup build -U</TT>".
+<BR>The NFRA-Master uses the "<TT>nup retrieve -import ...</TT>" to get 
+files from the Export-Master's $n_import (files checked in by 
+programmers outside the NFRA).
+<PRE></PRE>
+
+<H2>Definition of revisions and releases</H2>
+
+Every modification of files in the Master source tree results in a new
+<EM>revision</EM>, even if the modification does not involve changes in the
+executables. The procedure for merging modifications in the Master source
+tree is described in the next section.
+<P>
+A <EM>release</EM> is defined as a revision which involves one or more of the
+following items:
+<OL>
+  <LI>A change of fileformats, so you will have to use the 
+        NVS (New Version) option in some programs
+  <LI>A change in keyword syntax (so you will have to type different
+         things or change batch files in some cases) other than an 
+         additional keyword for which the default can be used.
+  <LI>Addition of a new program, or a major rewrite of an existing one.
+</OL>
+The issue of a new release has to be decided upon by at least two members 
+of the Newstar Project Team.
+<P>
+The updating of revision numbers is taken care of by the update script.
+Releases need to be explicitly indicated. The procedure for this is 
+described in a later section.
+<P>
+The version number of the current Newstar configuration is given
+by the file  $n_src/sys/version.idx
+<P>
+A full description of the current Newstar configuration is given by 
+the file  $n_src/sys/database.idx  after the command "<TT>nup check d</TT>"
+<P>
+A user-oriented decription of the configuration is given in the
+file  $n_src/doc/nnews.hlp  which is shown by the command "<TT>nnews</TT>"
+<P>
+The version number of the Newstar executables is given by the
+command 
+<BR>"<TT>what $n_exe/*.exe | grep %NST%</TT>"
+<P>
+<PRE></PRE>
+
+<H2>Checking-in modified files</H2>
+
+When programmers (in or outside the NFRA) want to make a change in files 
+in their Master source tree they have to use the "<TT>nsh in</TT>" command. 
+This will ask (among other things) for a list of files to be checked in, for 
+a comment and for the executables to be rebuilt (seprated by blanks). 
+<P>
+When programmers check in their modified files, these files are copied
+into their local $n_import directory, together with a groupfile listing
+the files and executables. The same files are copied into the $n_import
+directory of the Export-Master. If the "<TT>nsh in</TT>" command is issued for 
+(modified) files in a Master tree (presumably outside the NFRA), these 
+files are not copied to the local $n_import. They are copied into the 
+Export-Master. In all cases, a mail message describing the check-in is
+sent to $n_master (currently newstar@astron.nl).
+<P>
+Testing should be completed before check-in! At the NFRA, an executable 
+and/or ppd-file supplied by a programmer can at request be copied into 
+$n_tst for testing by a broader user-group. 
+<PRE></PRE>
+
+
+<H2>Merging modifications into the NFRA-Master source tree</H2>
+
+When mail concerning a check-in is received, the following actions
+should be taken:
+<P>
+
+<EM> 1e. If files originate from outside the NFRA, they should be 
+     received in $n_import of the NFRA-Master (more than one 
+     groupfile can be handled with a single update command):</EM>
+<PRE>
+  >>> nup retrieve -import updxxx.grp
+</PRE>
+<STRONG>Any file that has to be ftp'd with binary mode has to be retrieved
+separately.</STRONG>
+<P>
+<EM> 2e. Perform some elementary checks: </EM>
+<P>
+If psc/pin/pef-files are changed, they should be checked against 
+changes in keywords. If the meaning of existing keywords have been 
+changed, the revision should be treated as a release (see the previous 
+section). 
+<P>
+If keywords have been removed from a psc file, it should be checked wether
+they have been removed from the programs as well. In such cases, special
+care should be taken that executables are being rebuilt synchroneously
+with the ppd-files. In general, removal of keywords is discouraged for 
+revisions. 
+<P>
+NOTE: The synchronisation of exe/ppd files is not optimal in the present
+      structure for configuration management, but cannot be improved 
+      without structural changes in the coupling of exe and ppd files.
+<P>
+<EM> 3e. Update libraries and executables for all architectures:</EM>
+<PRE>
+  >>>  nup build -Update  updxxx.grp                   (on rzmws0)
+  >>>  nup build -Update  updxxx.grp                   (on rzmws5)
+</PRE>
+
+Any errors reported by the build command should be reported to 
+and repaired by the programmer. 
+<P>
+<EM> 4e. At successful compilation, merge the files in the source tree:</EM>
+<PRE>
+  >>>  nup build -Update -T:none -Merge updxxx.grp     (on rzmws0)
+</PRE>
+
+The revision number will be automatically updated in version.idx.
+<P>
+The subject from the groupfile(s) is copied in the nnews.hlp file, and a
+message to be sent to local Friends of Newstar is composed (so enter
+useful information). Both files will
+be presented in the MicroEmacs editor (change buffers with ^X X command,
+exit with Esc Z).
+Comments concerning programmers only should be removed from nnews.hlp, or
+be prefixed by "System: ". This checking of nnews.hlp is very important
+since most users rely on this file for their information on changes.
+The message is kept in $n_import/message.RR.rr where RR is the new Release,
+rr the new revision of Newstar.
+<P>
+The message is not yet sent, this is done after the Export-Master has been
+updated. 
+<BR>This is done with the "<TT>nup release</TT>" command, discussed later.
+A mail is sent to $n_master to remind you of this revision after three days.
+<PRE></PRE>
+
+<H2>Special procedure in case a groupfile needs to be deleted</H2>
+
+If a groupfile needs to be removed from the Master, it should be explicitly
+deleted using a command like 
+<BR>"<TT>rm $n_src/xxx/yyy.grp</TT>" followed by a reconstruction of the 
+database with  "<TT>nup check d</TT>".
+<P>
+At remote sides, the groupfile will be deleted automatically after the
+next update.
+<PRE></PRE>
+
+
+<H2>Special procedure for new releases</H2>
+
+If a modification is to be interpreted as a release, the following 
+special actions need to be taken:
+<OL>
+   <LI>Check out file  $n_src/sys/version.idx
+   <LI>Increase the release number by hand, set the revision number to 1
+   <LI>Check in file $n_src/sys/version.idx
+       <UL>
+        <LI>The comment should clearly indicate the new release
+        <LI>When asked for the executables to be rebuilt, answer:  @all
+       </UL>
+   <LI>Update the resulting groupfile in the master:
+       <UL>
+        <LI>Nnews should clearly reflect the new release
+        <LI>The mail message has to be edited to mention the release explicitly
+       </UL>
+   <LI>The file $n_root/updates.html should be edited
+       to reflect the new release. An example how to do this should be
+       taken from header of the previous release. It should be decided
+       wether the old revision history should still be kept in this file. 
+       If not, the revision information should be replaced by the remark
+<PRE>
+         &lt;EM&gt;Revision history not recorded&lt;/EM&gt;&lt;P&gt;
+</PRE>
+       The description of previous releases should not be removed.
+       Add a hypertext link to this release at the beginning of the file.
+</OL>
+<PRE></PRE>
+
+<H2>Merging changes into the Export-Master</H2>
+
+After the changes have been active in Dwingeloo, they have to be made 
+known to the outside world. This is typically done after three days (to 
+remind you, the above mentioned at-job is scheduled). 
+<P>
+The procedure to update the Export-Master is as follows:
+<P>
+<PRE>
+  >>>   telnet wsrt00
+  >>>   setenv n_remote rzmws0.astron.nl newstar /newstar/master/src
+  >>>   nup update
+</PRE>
+This will try to update the Westerbork installation from the NFRA-master.
+Any errors occurring here will almost certainly occur in other installtions
+as well, so they need to be repaired before the next step. Should you choose
+to make changes directly in the NFRA-Master, issue the following command
+<STRONG>at rzmws0</STRONG> before trying to update wsrt00 again:
+<PRE>
+  >>>  nup check d
+</PRE>
+This will make a fresh version of the database. Once installation on wsrt00
+is successfull, give the following command <STRONG>at rzmws0</STRONG>:
+<PRE>
+  >>>  nup release
+</PRE>
+This will rebuild the documentation, create a fresh database, pack
+all sources, libraries and executables and send them over to the
+Export-Master. It also tells the server program that files are waiting
+to be unpacked. Once this has been done, the message will be sent. In 
+case more than one release has been pending, a fresh message for the
+most recent revision will be composed, containing all the subjects 
+from previous revisions. The message will be sent to the Friends of Newstar.
+This relies on an elm alias friends_of_newstar. 
+<PRE></PRE>
+
+<H2>Maintenance of server programs for the Export-Master</H2>
+
+The server programs for the Export-Master are maintained outside the 
+normal Newstar routine. All sources (programs, scripts and text-files) 
+have to be in /users/newstar/src/. They have to be compiled or put in 
+their proper place by executing the "<TT>make</TT>" command in that directory.
+A "<TT>make</TT>" should be done after any change in files in /users/newstar/src.
+Refer to file /users/newstar/src/Makefile for details about requirements 
+for server programs.
+<PRE></PRE>
+
+<H2>Maintenance of the locking database</H2>
+
+The locking database is there mainly for administrative purposes.
+It warns users who check out a locked file, but still makes a copy for them.
+However, it will prohibit checking in locked files. Since users sometimes
+just delete files without unlocking them, the lock-file will get polluted.
+Therefore the weekly routine includes cleaning up of this file.
+<PRE></PRE>
+
+
+<H2>Weekly routines for the Newstar Master copy at NFRA</H2>
+
+Backups are made each Thursday afternoon or Friday morning. The procedure 
+for backups is:
+<PRE>
+  >>>   nup check d  
+</PRE>
+This will build a fresh version of file  database.idx  
+The database will be updated for any direct changes in the Master (that is:
+without proper checkin through $n_import). 
+<PRE>
+  >>>   nup save
+</PRE>
+This will make a backup of the entire master tree (all files below $n_root).
+Three DAT tapes are used for the backups (cyclic use of Newstar_A, Newstar_B
+and Newstar_C). The save command will run in the background and notify
+by mail when it is ready. 
+<P>
+The two most recent backups are stored at the Bank of Dwingeloo.
+Backups of the Export-Master are made as part of the Scissor backup
+routine.
+<P>
+
+After the backup, the following command should be entered:
+<PRE>
+  >>>   rm $n_exe/*.old $n_tst/*.old
+</PRE>
+This will throw away old versions, which can be restored from the backup
+tape if necessary.
+<PRE>
+  >>>   nup clear -Confirm
+</PRE>
+This will remove any obsolete files from the Master copy. See above for
+the deletion of obsolete groupfiles. Removing a file from a groupfile will
+cause a prompt for deletion here. In such cases, check wether the file
+has become really obsolete (e.g. by using a grep on the subroutine name).
+If the file has been accidentally removed from a groupfile, check out
+the groupfile, re-insert the file, check-in the groupfile and make a 
+maintenance revision.
+<PRE>
+  >>>   nup check  l        (on rzmws0)
+  >>>   nup check  l        (on rzmws5)
+</PRE>  
+This will check the current libraries. If faults are reported, the
+libraries should be updated through the groupfile produced by the
+check command (instructions are given by the command). The name of
+the groupfile will be  libyymmdd${n_arch}.grp.
+<PRE></PRE>
+
+
+<H2>Appendix 1: Terminology</H2>
+
+<DL>
+<DT> Site:<DD>
+             on or more computers that share a (Network) File System
+
+<DT> Master-systeem:<DD>
+   the officially installed Newstar version on a site
+
+<DT> NFRA-Master:<DD>
+      the master system at the Unix network of the NFRA,
+
+<DT> Export-Master:<DD>
+    the (sources-only) master system at the Unix network 
+                    of the NFRA, distribution is done from this master.
+
+<DT> User-systeem:<DD>
+     a (partial) version of Newstar that is made by a user/
+                    programmer based on the Master-system. When starting
+                    an executable, a version in the user-system has priority 
+                    over the Master.
+
+<DT> Binary-tree:<DD>
+      a directory tree in a Master or User system containing
+                    the executable files needed to run Newstar (NB: you 
+                    also need the startup scripts in $n_src/sys).
+
+<DT> Source-tree:<DD>
+      a directory tree in a Master or User system containing
+                    only all files needed to install a binary tree 
+                    (excluding the operating system and compilers...).
+
+<DT> Library-tree:<DD>
+     a directory tree in a Master or User system with libraries
+                    and (for a User system) object files; one directory in the
+                    library tree contains include files and system independent
+                    pre-processed files, all derived from the source tree.
+
+<DT> Work-directory:<DD>
+   a directory for temporary files, for listingss and for
+                    files needed for the debugger.
+</DL>
+<P>
+The Master system has two binary trees:
+<UL>
+   <LI>$n_root/exe     No debugging information.
+   <LI>$n_root/tst     Can be used for debugging, will usually be empty.
+</UL>
+<P>
+Executable files are looked for in the current directory first, then
+in $n_uexe (if it exists) and finally in $n_exe.
+<P>
+A user may decide to do "<TT>setenv n_uexe $n_tst</TT>" to get access to test versions,
+and programmers will set $n_uexe to the binary tree of their user system.
+<PRE></PRE>
+
+<H2>Appendix 2: Directory trees</H2>
+
+<PRE>
+Master (NFRA or elsewhere):
+---------------------------
+
+$n_root -+-- src           = $n_src       Source tree 
+         |
+         +-- lib -+-- inc  = $n_inc       Precompiled files 
+         |        +-- sun  = $n_lib       Object libraries
+         |        +-- hp
+         |
+         +-- exe -+-- sun  = $n_exe       Executables and ppd-files 
+         |        +-- hp
+         |        |
+         |        +-- html = $n_hlp       Hypertext help files (elsewhere)
+         |
+         +-- hlp           = $n_hlp       Hypertext help files (at NFRA)
+         |
+         +-- tst -+-- sun  = $n_tst       Test versions
+         |        +-- hp
+         |
+         +-- work -+-- sun = $n_work      Intermediate files, files
+         |         +-- hp                 necessary for debugging
+         |
+         +-- import        = $n_import    Import area for uploading of
+                                          revisions and programmers files.
+
+Sites outside NFRA can have other architectures in $n_lib and $n_exe. 
+At most sites outside NFRA $n_hlp is a subdirectory of $n_root/exe.
+
+This structure can be split over various filesystems. The tree can than
+be realised through symbolic links. Since all system commands use the
+environment variables this is not strictly necessary.
+		    
+Additional directories at NFRA only:          
+
+         |
+         +-- mongo                        Installation of mongo
+         +-- perl                         Executables for perl
+         +-- rmtd                         Sources for rmtd (VAX)
+
+Possible files in $n_root:  backups.txt  Log of backups
+                            updates.log  Log of update-commands
+                            updates.html Revision history (NFRA only)
+
+Source tree:
+
+   $n_src  -+-- sys                       Maintenance system
+            |
+            +-- doc -+- ...               Documents
+            |
+            +-- wng                       Precompiler, files, I/O etc.
+            +-- dwarf                     Parameter interface
+            +-- n*                        The various programs
+            | 
+            +-- data                      Calibrator models
+            | 
+            +-- batch                     Standard batch procedures
+
+Possible files in $n_src:  upd*.log      Compilation logs
+
+
+User system:
+------------
+
+~programmer +... $n_uroot -+-- lib -+-- inc = $n_uinc
+            :              |        +-- sun = $n_ulib
+            :              |
+                           +-- exe -+-- sun = $n_uexe
+                           |
+                           +-- work         = $n_work
+                           |
+                   [       +-- src          = $n_usrc  ]
+            :
+            +...                     Arbitrary directories with files
+                                          modified by the programmer.
+
+
+Logging in as the owner of $n_root (Newstar manager) causes $n_u... 
+to point to $n_..., $n_work will point to $n_root/work/$n_arch. 
+If the Newstar manager uses the -NUpdate switch for update, $n_uexe
+will be set to $n_tst, else it will be at $n_exe.
+
+It is confusing that there is no $n_uwork, this departure from the 
+general practice may be removed in future.
+
+
+Export Master (NFRA only, at ftp.astron.nl):
+------------------------------------------
+
+/users/ftp/newstar          = $n_root     Newstar ftp area
+/users/www/newstar          = $n_www      Newstar www area
+/users/newstar                            Newstar server programs
+
+$n_root -+-- src            = $n_src      Source tree 
+         |
+         +-- import         = $n_import   Import area for uploading of
+                                           revisions and programmers files
+                                           (also from non-NFRA sites).
+
+Files in $n_root: 
+   nstar_src.tar.Z                        Archive with sources
+   nstar_src_??.tar                       Archive with additional sources
+                                          for various architectures
+   nstar_hlp.tar.Z                        Archive with documentation
+   nstar_exe_??.tar.Z                     Archive with executables for
+                                          various architectures
+   nstar_lib_??.tar.Z                     Archive with libraries for
+                                          various architectures
+   nstar_lib_inc.tar.Z                    Archive with include files
+   
+
+
+$n_www  -+-- hlp                          Documentation (from nstar_hlp.tar)
+         |
+         +-- bug                          User Feedback System
+         |
+         +-- bin            = $n_cgi      httpd scripts for Newstar
+         |                                  (sources in /users/newstar/src)
+         |
+         +-- mail                         Link to Newstar mail area for HjV
+
+Files in $n_www:
+   homepage.html                          Homepage for the server area,
+                                          different from hlp/homepage.html
+   index.html                             Link to homepage.html, you get this
+                                          for http://www.astron.nl/newstar/
+   example.*                              Some sample images
+   updates.html                           Revision history (from NFRA master)
+
+
+/users/newstar -+-- src                   Server programs (sources)
+                +-- bin     = $n_bin      Server programs (executables)
+
+</PRE>
+<PRE></PRE>
+
+<H2>Appendix 3: Other programs and procedures related to Newstar</H2>
+
+<H3>Mails concerning Newstar</H3>
+
+A copy of all E-mail correspondention between the different members of the
+Newstar group should always be send to HjV (hjvosmeijer@astron.nl). He will
+extract those documents and put them in his Newstar mail directory
+(~hjv/public_html/newstar/mail). A printed version of the documents will be put in
+a special binder which will be kept in HjV's room.
+<BR>Every working-day at 07.00 AM a script will create an updated HTML
+file (<A HREF=http://www.astron.nl/~hjv/newstar/mail.html>mail.html</A>)
+which gives everyone the possibility to read the mails and search for 
+keywords using Mosaic. 
+
+
+
+<H3>Newstar use</H3>
+
+On every site where Newstar is installed, the programs will write an
+entry (with username, programname, date a.s.o.) in the file 
+$n_import/newstar.use. During an update of a site, this file is ftp'ed 
+to NFRA (/users/ftp/pub/incoming) and a new (empty) version is
+created on the updating site.
+<BR>At NFRA every working-day at 07.00 AM a script will take care for
+moving those new files to ~hjv/newstar/use, compressing the files and
+merge them with the already existing files per site, create quarterly 
+and monthly reports. The script will also update an HTML file 
+(<A HREF=http://www.astron.nl/~hjv/newstar/use.html>use.html</A>) 
+which which gives everyone the possibility to view those reports 
+by using Mosaic.  
+
+
diff --git a/nfra_config_management/nfra_config_management.html b/nfra_config_management/nfra_config_management.html
new file mode 100644
index 0000000000000000000000000000000000000000..6934202643367b5bf1597ab64ed7ff58105554de
--- /dev/null
+++ b/nfra_config_management/nfra_config_management.html
@@ -0,0 +1,652 @@
+<TITLE>Newstar configuration management at NFRA</TITLE>
+
+<BR><STRONG>Subject:</STRONG> Newstar configuration management at NFRA
+<BR><STRONG>Author:</STRONG>  Marco de Vos (CMV) and Henk Vosmeyer (HjV)
+<BR><STRONG>To:</STRONG>      Newstar Support Team (HjV, CMV, JEN, JPH)
+<P> <STRONG>Date:</STRONG>    08/11/94 
+<P>
+<EM>Revision history</EM>
+<UL>
+<LI>22/01/96 - Change appendix 3
+<LI>11/11/94 - Add appendix 3
+<LI>08/11/94 - Typo's and minor changes
+<LI>02/11/94 - Separation of NFRA-Master and Export-Master
+<LI>04/03/94 - First release 
+<LI>21/02/94 - Prerelease
+</UL>
+
+
+<H1>Newstar configuration management at NFRA</H1>
+<PRE></PRE>
+
+
+<H2>General concerns</H2>
+
+The Newstar package is not a static product. Major and minor changes are 
+often being made to the software. These changes should affect the use of
+the package in a positive sense only. Therefore we need to guard the
+integrity of the package at NFRA and define clear procedures for external
+users on how to upgrade their implementation. This document describes
+those procedures. 
+<P>
+This document is limited to configuration management on the Unix systems.
+The VAX system will be no longer supported at NFRA from 15/03/94, and 
+can be maintained through the perl-scripts provided by WNB.
+<P>
+Reference to Newstar directories are made through the usual variables 
+$n_src, $n_root etc. Refer to Appendix 2 for the details. 
+<P>
+All commands assume one is logged in as the Newstar Master (newstar).
+<PRE></PRE>
+
+<H2>What makes up the Newstar configuration at NFRA</H2>
+
+The Newstar configuration at NFRA consists of the following:
+<P>
+<UL>
+  <LI><STRONG>The NFRA-Master system</STRONG> on the /newstar disk (below $n_root):
+  <OL>
+    <LI>The Master source tree (below $n_src)
+    <LI>The NFRA library and executable areas ($n_inc, $n_lib,
+             $n_exe and $n_tst for the various architectures)
+    <LI>The NFRA documentation area ($n_hlp)
+    <LI>The NFRA import area (below $n_import)
+  </OL>
+  <P>
+    Below /newstar/master we also have an installation of: (1) mongo (in
+    /newstar/master/mongo), of (2) perl (in /newstar/master/perl) and 
+    (3) a copy of the sources for the VAX-based Remote Tape Daemon (in
+    /newstar/master/rmtd).
+  <P>  
+    This is a working system, used by NFRA users and programmers.
+  <P>
+  <LI><STRONG>The Export-Master system</STRONG> on the /users disk of ftp.nfra.nl:
+  <OL>
+    <LI>The Export Master source tree           (below $n_src)
+    <LI>The Server version of the documentation (below $n_www)
+      <UL>
+        <LI>server homepage            $n_www/homepage.html
+        <LI>documentation relevant to the Export Master source tree
+                                       $n_www/hlp/
+        <LI>user feedback system       $n_www/bug/
+        <LI>link to mail area          $n_www/mail/
+      </UL>
+    <LI>Some server programs for ftp.nfra.nl    (below /users/newstar)
+    <LI>The import area for sites outside NFRA  (/users/ftp/newstar/import)
+  </OL>
+  <P>
+    This is a sources-only system which is never compiled.
+    The Export Master source tree and the documentation are kept
+    up-to-date from the NFRA Master system.
+  <P>
+  <LI><STRONG>The Newstar account</STRONG> on the NFRA Unix system (~newstar)
+  <OL>
+    <LI>Startup files for the newstar account (.cshrc and .login etc.). These 
+        files should not contain commands that are essential for the 
+        functioning of newstar apart from PATH settings and 
+        the startup command:
+<PRE>
+#
+# Initialise Newstar (either NFRA-Master or Export-Master)
+#
+if (-e  /newstar/master/src/sys/newstar_nfra.csh) then
+ source /newstar/master/src/sys/newstar_nfra.csh
+else if (-e /users/newstar/bin/newstar_init.csh) then
+ source     /users/newstar/bin/newstar_init.csh
+endif
+</PRE>
+
+    <LI>Mail environment (~/Mail and ~/.elm). The elm
+        alias friends_of_newstar is used to inform on updates. The Newstar
+        environment variable $n_master points to this eMail account.
+    <LI>Server interface (~/server). This directory is used to pass commands
+        to the server programs on ftp.nfra.nl
+  </OL>
+  <P>
+    This account is the owner of the NFRA-Master and the Export-Master, and
+    is the only account that can modify them (apart from $n_import and the
+    locking database).
+</UL>
+<PRE></PRE>
+
+<H2>Relations between NFRA-Master and Export-Master</H2>
+
+The dynamic relations between Master systems (either the NFRA Master or
+another one) and Export-Master are as follows:
+<PRE>
++----------------------------------------------------------------------+
+|  Master:                                                             |
+|                 $n_src      <--------+                               |
+|                   |                  | nup build -U (in $n_import)   |
+|                   | nup build -U     |                               |
+|                   v                  |                               |
+|                 $n_exe, ... <--------+                               |
+|                                      |                               |
+|                 $n_import -->--------+                               |
+|                  | ^   ^^                                            |
+|                  | |   ||                                            |
+|                  | |   || (NFRA only)                                |
+|                  | |   |+--------------------+--<-- nsh in           |
+|                  | |   |                     |                       |
++----------------------------------------------------------------------+
+|  Export-Master:  | |   |                     |                       |
+|                  | |   | nup retrieve ...    | (NFRA and others)     |
+|                  | |   |  (NFRA only)        |                       |
+|      nup release | |   |                     |                       |
+|                  | | nup retrieve            |                       |
+|                  v |   |                     |                       |
+|                 $n_src |                     |                       |
+|                 $n_import <------------------+                       |
+|                                                                      |   
++----------------------------------------------------------------------+
+</PRE>
+Use of the "<TT>nup release</TT>" command is restricted to the NFRA-Master.
+Master systems outside NFRA use the "<TT>nup retrieve</TT>" command to get 
+updated files from the Export-Master. The "<TT>nup update</TT>" command 
+combines "<TT>nup retrieve</TT>" and "<TT>nup build -U</TT>".
+<BR>The NFRA-Master uses the "<TT>nup retrieve -import ...</TT>" to get 
+files from the Export-Master's $n_import (files checked in by 
+programmers outside the NFRA).
+<PRE></PRE>
+
+<H2>Definition of revisions and releases</H2>
+
+Every modification of files in the Master source tree results in a new
+<EM>revision</EM>, even if the modification does not involve changes in the
+executables. The procedure for merging modifications in the Master source
+tree is described in the next section.
+<P>
+A <EM>release</EM> is defined as a revision which involves one or more of the
+following items:
+<OL>
+  <LI>A change of fileformats, so you will have to use the 
+        NVS (New Version) option in some programs
+  <LI>A change in keyword syntax (so you will have to type different
+         things or change batch files in some cases) other than an 
+         additional keyword for which the default can be used.
+  <LI>Addition of a new program, or a major rewrite of an existing one.
+</OL>
+The issue of a new release has to be decided upon by at least two members 
+of the Newstar Project Team.
+<P>
+The updating of revision numbers is taken care of by the update script.
+Releases need to be explicitly indicated. The procedure for this is 
+described in a later section.
+<P>
+The version number of the current Newstar configuration is given
+by the file  $n_src/sys/version.idx
+<P>
+A full description of the current Newstar configuration is given by 
+the file  $n_src/sys/database.idx  after the command "<TT>nup check d</TT>"
+<P>
+A user-oriented decription of the configuration is given in the
+file  $n_src/doc/nnews.hlp  which is shown by the command "<TT>nnews</TT>"
+<P>
+The version number of the Newstar executables is given by the
+command 
+<BR>"<TT>what $n_exe/*.exe | grep %NST%</TT>"
+<P>
+<PRE></PRE>
+
+<H2>Checking-in modified files</H2>
+
+When programmers (in or outside the NFRA) want to make a change in files 
+in their Master source tree they have to use the "<TT>nsh in</TT>" command. 
+This will ask (among other things) for a list of files to be checked in, for 
+a comment and for the executables to be rebuilt (seprated by blanks). 
+<P>
+When programmers check in their modified files, these files are copied
+into their local $n_import directory, together with a groupfile listing
+the files and executables. The same files are copied into the $n_import
+directory of the Export-Master. If the "<TT>nsh in</TT>" command is issued for 
+(modified) files in a Master tree (presumably outside the NFRA), these 
+files are not copied to the local $n_import. They are copied into the 
+Export-Master. In all cases, a mail message describing the check-in is
+sent to $n_master (currently newstar@nfra.nl).
+<P>
+Testing should be completed before check-in! At the NFRA, an executable 
+and/or ppd-file supplied by a programmer can at request be copied into 
+$n_tst for testing by a broader user-group. 
+<PRE></PRE>
+
+
+<H2>Merging modifications into the NFRA-Master source tree</H2>
+
+When mail concerning a check-in is received, the following actions
+should be taken:
+<P>
+
+<EM> 1e. If files originate from outside the NFRA, they should be 
+     received in $n_import of the NFRA-Master (more than one 
+     groupfile can be handled with a single update command):</EM>
+<PRE>
+  >>> nup retrieve -import updxxx.grp
+</PRE>
+<STRONG>Any file that has to be ftp'd with binary mode has to be retrieved
+separately.</STRONG>
+<P>
+<EM> 2e. Perform some elementary checks: </EM>
+<P>
+If psc/pin/pef-files are changed, they should be checked against 
+changes in keywords. If the meaning of existing keywords have been 
+changed, the revision should be treated as a release (see the previous 
+section). 
+<P>
+If keywords have been removed from a psc file, it should be checked wether
+they have been removed from the programs as well. In such cases, special
+care should be taken that executables are being rebuilt synchroneously
+with the ppd-files. In general, removal of keywords is discouraged for 
+revisions. 
+<P>
+NOTE: The synchronisation of exe/ppd files is not optimal in the present
+      structure for configuration management, but cannot be improved 
+      without structural changes in the coupling of exe and ppd files.
+<P>
+<EM> 3e. Update libraries and executables for all architectures:</EM>
+<PRE>
+  >>>  nup build -Update  updxxx.grp                   (on rzmws0)
+  >>>  nup build -Update  updxxx.grp                   (on rzmws5)
+</PRE>
+
+Any errors reported by the build command should be reported to 
+and repaired by the programmer. 
+<P>
+<EM> 4e. At successful compilation, merge the files in the source tree:</EM>
+<PRE>
+  >>>  nup build -Update -T:none -Merge updxxx.grp     (on rzmws0)
+</PRE>
+
+The revision number will be automatically updated in version.idx.
+<P>
+The subject from the groupfile(s) is copied in the nnews.hlp file, and a
+message to be sent to local Friends of Newstar is composed (so enter
+useful information). Both files will
+be presented in the MicroEmacs editor (change buffers with ^X X command,
+exit with Esc Z).
+Comments concerning programmers only should be removed from nnews.hlp, or
+be prefixed by "System: ". This checking of nnews.hlp is very important
+since most users rely on this file for their information on changes.
+The message is kept in $n_import/message.RR.rr where RR is the new Release,
+rr the new revision of Newstar.
+<P>
+The message is not yet sent, this is done after the Export-Master has been
+updated. 
+<BR>This is done with the "<TT>nup release</TT>" command, discussed later.
+A mail is sent to $n_master to remind you of this revision after three days.
+<PRE></PRE>
+
+<H2>Special procedure in case a groupfile needs to be deleted</H2>
+
+If a groupfile needs to be removed from the Master, it should be explicitly
+deleted using a command like 
+<BR>"<TT>rm $n_src/xxx/yyy.grp</TT>" followed by a reconstruction of the 
+database with  "<TT>nup check d</TT>".
+<P>
+At remote sides, the groupfile will be deleted automatically after the
+next update.
+<PRE></PRE>
+
+
+<H2>Special procedure for new releases</H2>
+
+If a modification is to be interpreted as a release, the following 
+special actions need to be taken:
+<OL>
+   <LI>Check out file  $n_src/sys/version.idx
+   <LI>Increase the release number by hand, set the revision number to 1
+   <LI>Check in file $n_src/sys/version.idx
+       <UL>
+        <LI>The comment should clearly indicate the new release
+        <LI>When asked for the executables to be rebuilt, answer:  @all
+       </UL>
+   <LI>Update the resulting groupfile in the master:
+       <UL>
+        <LI>Nnews should clearly reflect the new release
+        <LI>The mail message has to be edited to mention the release explicitly
+       </UL>
+   <LI>The file $n_root/updates.html should be edited
+       to reflect the new release. An example how to do this should be
+       taken from header of the previous release. It should be decided
+       wether the old revision history should still be kept in this file. 
+       If not, the revision information should be replaced by the remark
+<PRE>
+         &lt;EM&gt;Revision history not recorded&lt;/EM&gt;&lt;P&gt;
+</PRE>
+       The description of previous releases should not be removed.
+       Add a hypertext link to this release at the beginning of the file.
+</OL>
+<PRE></PRE>
+
+<H2>Merging changes into the Export-Master</H2>
+
+After the changes have been active in Dwingeloo, they have to be made 
+known to the outside world. This is typically done after three days (to 
+remind you, the above mentioned at-job is scheduled). 
+<P>
+The procedure to update the Export-Master is as follows:
+<P>
+<PRE>
+  >>>   telnet wsrt00
+  >>>   setenv n_remote rzmws0.nfra.nl newstar /newstar/master/src
+  >>>   nup update
+</PRE>
+This will try to update the Westerbork installation from the NFRA-master.
+Any errors occurring here will almost certainly occur in other installtions
+as well, so they need to be repaired before the next step. Should you choose
+to make changes directly in the NFRA-Master, issue the following command
+<STRONG>at rzmws0</STRONG> before trying to update wsrt00 again:
+<PRE>
+  >>>  nup check d
+</PRE>
+This will make a fresh version of the database. Once installation on wsrt00
+is successfull, give the following command <STRONG>at rzmws0</STRONG>:
+<PRE>
+  >>>  nup release
+</PRE>
+This will rebuild the documentation, create a fresh database, pack
+all sources, libraries and executables and send them over to the
+Export-Master. It also tells the server program that files are waiting
+to be unpacked. Once this has been done, the message will be sent. In 
+case more than one release has been pending, a fresh message for the
+most recent revision will be composed, containing all the subjects 
+from previous revisions. The message will be sent to the Friends of Newstar.
+This relies on an elm alias friends_of_newstar. 
+<PRE></PRE>
+
+<H2>Maintenance of server programs for the Export-Master</H2>
+
+The server programs for the Export-Master are maintained outside the 
+normal Newstar routine. All sources (programs, scripts and text-files) 
+have to be in /users/newstar/src/. They have to be compiled or put in 
+their proper place by executing the "<TT>make</TT>" command in that directory.
+A "<TT>make</TT>" should be done after any change in files in /users/newstar/src.
+Refer to file /users/newstar/src/Makefile for details about requirements 
+for server programs.
+<PRE></PRE>
+
+<H2>Maintenance of the locking database</H2>
+
+The locking database is there mainly for administrative purposes.
+It warns users who check out a locked file, but still makes a copy for them.
+However, it will prohibit checking in locked files. Since users sometimes
+just delete files without unlocking them, the lock-file will get polluted.
+Therefore the weekly routine includes cleaning up of this file.
+<PRE></PRE>
+
+
+<H2>Weekly routines for the Newstar Master copy at NFRA</H2>
+
+Backups are made each Thursday afternoon or Friday morning. The procedure 
+for backups is:
+<PRE>
+  >>>   nup check d  
+</PRE>
+This will build a fresh version of file  database.idx  
+The database will be updated for any direct changes in the Master (that is:
+without proper checkin through $n_import). 
+<PRE>
+  >>>   nup save
+</PRE>
+This will make a backup of the entire master tree (all files below $n_root).
+Three DAT tapes are used for the backups (cyclic use of Newstar_A, Newstar_B
+and Newstar_C). The save command will run in the background and notify
+by mail when it is ready. 
+<P>
+The two most recent backups are stored at the Bank of Dwingeloo.
+Backups of the Export-Master are made as part of the Scissor backup
+routine.
+<P>
+
+After the backup, the following command should be entered:
+<PRE>
+  >>>   rm $n_exe/*.old $n_tst/*.old
+</PRE>
+This will throw away old versions, which can be restored from the backup
+tape if necessary.
+<PRE>
+  >>>   nup clear -Confirm
+</PRE>
+This will remove any obsolete files from the Master copy. See above for
+the deletion of obsolete groupfiles. Removing a file from a groupfile will
+cause a prompt for deletion here. In such cases, check wether the file
+has become really obsolete (e.g. by using a grep on the subroutine name).
+If the file has been accidentally removed from a groupfile, check out
+the groupfile, re-insert the file, check-in the groupfile and make a 
+maintenance revision.
+<PRE>
+  >>>   nup check  l        (on rzmws0)
+  >>>   nup check  l        (on rzmws5)
+</PRE>  
+This will check the current libraries. If faults are reported, the
+libraries should be updated through the groupfile produced by the
+check command (instructions are given by the command). The name of
+the groupfile will be  libyymmdd${n_arch}.grp.
+<PRE></PRE>
+
+
+<H2>Appendix 1: Terminology</H2>
+
+<DL>
+<DT> Site:<DD>
+             on or more computers that share a (Network) File System
+
+<DT> Master-systeem:<DD>
+   the officially installed Newstar version on a site
+
+<DT> NFRA-Master:<DD>
+      the master system at the Unix network of the NFRA,
+
+<DT> Export-Master:<DD>
+    the (sources-only) master system at the Unix network 
+                    of the NFRA, distribution is done from this master.
+
+<DT> User-systeem:<DD>
+     a (partial) version of Newstar that is made by a user/
+                    programmer based on the Master-system. When starting
+                    an executable, a version in the user-system has priority 
+                    over the Master.
+
+<DT> Binary-tree:<DD>
+      a directory tree in a Master or User system containing
+                    the executable files needed to run Newstar (NB: you 
+                    also need the startup scripts in $n_src/sys).
+
+<DT> Source-tree:<DD>
+      a directory tree in a Master or User system containing
+                    only all files needed to install a binary tree 
+                    (excluding the operating system and compilers...).
+
+<DT> Library-tree:<DD>
+     a directory tree in a Master or User system with libraries
+                    and (for a User system) object files; one directory in the
+                    library tree contains include files and system independent
+                    pre-processed files, all derived from the source tree.
+
+<DT> Work-directory:<DD>
+   a directory for temporary files, for listingss and for
+                    files needed for the debugger.
+</DL>
+<P>
+The Master system has two binary trees:
+<UL>
+   <LI>$n_root/exe     No debugging information.
+   <LI>$n_root/tst     Can be used for debugging, will usually be empty.
+</UL>
+<P>
+Executable files are looked for in the current directory first, then
+in $n_uexe (if it exists) and finally in $n_exe.
+<P>
+A user may decide to do "<TT>setenv n_uexe $n_tst</TT>" to get access to test versions,
+and programmers will set $n_uexe to the binary tree of their user system.
+<PRE></PRE>
+
+<H2>Appendix 2: Directory trees</H2>
+
+<PRE>
+Master (NFRA or elsewhere):
+---------------------------
+
+$n_root -+-- src           = $n_src       Source tree 
+         |
+         +-- lib -+-- inc  = $n_inc       Precompiled files 
+         |        +-- sun  = $n_lib       Object libraries
+         |        +-- hp
+         |
+         +-- exe -+-- sun  = $n_exe       Executables and ppd-files 
+         |        +-- hp
+         |        |
+         |        +-- html = $n_hlp       Hypertext help files (elsewhere)
+         |
+         +-- hlp           = $n_hlp       Hypertext help files (at NFRA)
+         |
+         +-- tst -+-- sun  = $n_tst       Test versions
+         |        +-- hp
+         |
+         +-- work -+-- sun = $n_work      Intermediate files, files
+         |         +-- hp                 necessary for debugging
+         |
+         +-- import        = $n_import    Import area for uploading of
+                                          revisions and programmers files.
+
+Sites outside NFRA can have other architectures in $n_lib and $n_exe. 
+At most sites outside NFRA $n_hlp is a subdirectory of $n_root/exe.
+
+This structure can be split over various filesystems. The tree can than
+be realised through symbolic links. Since all system commands use the
+environment variables this is not strictly necessary.
+		    
+Additional directories at NFRA only:          
+
+         |
+         +-- mongo                        Installation of mongo
+         +-- perl                         Executables for perl
+         +-- rmtd                         Sources for rmtd (VAX)
+
+Possible files in $n_root:  backups.txt  Log of backups
+                            updates.log  Log of update-commands
+                            updates.html Revision history (NFRA only)
+
+Source tree:
+
+   $n_src  -+-- sys                       Maintenance system
+            |
+            +-- doc -+- ...               Documents
+            |
+            +-- wng                       Precompiler, files, I/O etc.
+            +-- dwarf                     Parameter interface
+            +-- n*                        The various programs
+            | 
+            +-- data                      Calibrator models
+            | 
+            +-- batch                     Standard batch procedures
+
+Possible files in $n_src:  upd*.log      Compilation logs
+
+
+User system:
+------------
+
+~programmer +... $n_uroot -+-- lib -+-- inc = $n_uinc
+            :              |        +-- sun = $n_ulib
+            :              |
+                           +-- exe -+-- sun = $n_uexe
+                           |
+                           +-- work         = $n_work
+                           |
+                   [       +-- src          = $n_usrc  ]
+            :
+            +...                     Arbitrary directories with files
+                                          modified by the programmer.
+
+
+Logging in as the owner of $n_root (Newstar manager) causes $n_u... 
+to point to $n_..., $n_work will point to $n_root/work/$n_arch. 
+If the Newstar manager uses the -NUpdate switch for update, $n_uexe
+will be set to $n_tst, else it will be at $n_exe.
+
+It is confusing that there is no $n_uwork, this departure from the 
+general practice may be removed in future.
+
+
+Export Master (NFRA only, at ftp.nfra.nl):
+------------------------------------------
+
+/users/ftp/newstar          = $n_root     Newstar ftp area
+/users/www/newstar          = $n_www      Newstar www area
+/users/newstar                            Newstar server programs
+
+$n_root -+-- src            = $n_src      Source tree 
+         |
+         +-- import         = $n_import   Import area for uploading of
+                                           revisions and programmers files
+                                           (also from non-NFRA sites).
+
+Files in $n_root: 
+   nstar_src.tar.Z                        Archive with sources
+   nstar_src_??.tar                       Archive with additional sources
+                                          for various architectures
+   nstar_hlp.tar.Z                        Archive with documentation
+   nstar_exe_??.tar.Z                     Archive with executables for
+                                          various architectures
+   nstar_lib_??.tar.Z                     Archive with libraries for
+                                          various architectures
+   nstar_lib_inc.tar.Z                    Archive with include files
+   
+
+
+$n_www  -+-- hlp                          Documentation (from nstar_hlp.tar)
+         |
+         +-- bug                          User Feedback System
+         |
+         +-- bin            = $n_cgi      httpd scripts for Newstar
+         |                                  (sources in /users/newstar/src)
+         |
+         +-- mail                         Link to Newstar mail area for HjV
+
+Files in $n_www:
+   homepage.html                          Homepage for the server area,
+                                          different from hlp/homepage.html
+   index.html                             Link to homepage.html, you get this
+                                          for http://www.nfra.nl/newstar/
+   example.*                              Some sample images
+   updates.html                           Revision history (from NFRA master)
+
+
+/users/newstar -+-- src                   Server programs (sources)
+                +-- bin     = $n_bin      Server programs (executables)
+
+</PRE>
+<PRE></PRE>
+
+<H2>Appendix 3: Other programs and procedures related to Newstar</H2>
+
+<H3>Mails concerning Newstar</H3>
+
+A copy of all E-mail correspondention between the different members of the
+Newstar group should always be send to HjV (hjvosmeijer@nfra.nl). He will
+extract those documents and put them in his Newstar mail directory
+(~hjv/public_html/newstar/mail). A printed version of the documents will be put in
+a special binder which will be kept in HjV's room.
+<BR>Every working-day at 07.00 AM a script will create an updated HTML
+file (<A HREF=http://www.nfra.nl/~hjv/newstar/mail.html>mail.html</A>)
+which gives everyone the possibility to read the mails and search for 
+keywords using Mosaic. 
+
+
+
+<H3>Newstar use</H3>
+
+On every site where Newstar is installed, the programs will write an
+entry (with username, programname, date a.s.o.) in the file 
+$n_import/newstar.use. During an update of a site, this file is ftp'ed 
+to NFRA (/users/ftp/pub/incoming) and a new (empty) version is
+created on the updating site.
+<BR>At NFRA every working-day at 07.00 AM a script will take care for
+moving those new files to ~hjv/newstar/use, compressing the files and
+merge them with the already existing files per site, create quarterly 
+and monthly reports. The script will also update an HTML file 
+(<A HREF=http://www.nfra.nl/~hjv/newstar/use.html>use.html</A>) 
+which which gives everyone the possibility to view those reports 
+by using Mosaic.  
+
+
diff --git a/ngcalc/ngcalc__action.html b/ngcalc/ngcalc__action.html
new file mode 100644
index 0000000000000000000000000000000000000000..4efbf9266e7ee77b19ca623927e8ab68cd06e601
--- /dev/null
+++ b/ngcalc/ngcalc__action.html
@@ -0,0 +1,64 @@
+<TITLE>Description of ACTION (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword ACTION</H1> 
+
+<DT><EM>Prompt:</EM> type of action | EXTRACT, COPY, CALC, MERGE, COMBINE, TRANS, BASE, MONGO, PLOT, SHOW, BRIEF, FULL, DELETE, NODE, CVX, NVS, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the action to be performed: <P>
+   Creating cuts from external data: 
+	EXTRACT extract information from SCN file into cuts 
+	COPY    copy cuts to other NGF file, retaining their indices 
+		 (this action is mainly useful for discarding cuts no longer 
+		  needed and thereby freeing disk space) <P>
+   Viewing the contents of the .NGF file: 
+	SHOW    show information in cut headers and data 
+	BRIEF   show summary per group/field showing numbers of polarisations,  
+		interferometers, cuts and data points <P>
+   Calculations: 
+	CALC    Perform one of a set of predefined algorithms on individual cuts 
+	MERGE   Merge a number of cuts into a single new cut. 
+		NOTE: Overlapping points will be averaged so you may use MERGE 
+		      to average e.g. a set of interferometers with data points 
+		      at coincident hour angles. 
+	COMBINE Combine cut(s) in user-specified expression <P>
+   Sorting: 
+     Starting from a cut in the HA direction, these actions produce a new cut 
+in the frequency or baseline direction for each hour angle present in any of 
+the input cuts. Use the HA_RANGE parameter to limit the number of output cuts. 
+     The output cuts are in a primitive format in which the data are transposed 
+but NOT the coordinate axes. These wrong axes appear in plots of the transposed 
+cuts and must be interpreted as indicated below. In calculations, however,  
+coordinates will be interpreted correctly (provided you specify a sensible 
+calculation). <P>
+     Transposing a transposed group of cuts reproduces the original cuts. You 
+may also try to combine TRANS and BASE operations but sensible results are not 
+guaranteed. <P>
+	TRANS   transpose frequency and HA axes. 
+		In the transposed cuts, each channel is represented by an hour 
+		angle of &lt;channel number&gt;*0.125 deg. 
+		Each hour-angle bin of 0.125 deg is represented by a channel 
+		number, which starts at 0 for the lowest hour angle present. <P>
+	BASE    transpose interferometer and hour-angle axes. 
+		In the transposed cuts, each baseline bin of 10 metres is 
+		represented by an HA bin of .125 deg at HA = &lt;baseline&gt;/10*.125 
+		deg; baselines landing in the same bin are averaged. 
+		Each hour-angle bin of .125 deg is represented by a baseline 
+		sequence number of HA*.125. <P>
+   Plotting: 
+	MONGO   output cut data in a MONGO-readable file 
+	PLOT    plot data in NGF cut(s) <P>
+   Miscellaneous: 
+	DELETE  delete cuts. (Only the index linkage is removed but the cut data 
+		 remain in the file: Use COPY to free the file space.) 
+		BEWARE: This action is IRREVERSIBLE. 
+	NODE    switch to other NGF file 
+	QUIT    terminate NGCALC <P>
+   Data-format conversions: 
+	CVX     convert NGF file from other machine's format to local format 
+	NVS     update to latest NGF-file format  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__bas_range.html b/ngcalc/ngcalc__bas_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..ac73e783fc8ac7269613bf00f57164aba3f24e85
--- /dev/null
+++ b/ngcalc/ngcalc__bas_range.html
@@ -0,0 +1,14 @@
+<TITLE>Description of BAS_RANGE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword BAS_RANGE</H1> 
+
+<DT><EM>Prompt:</EM> Baseline range (metres)
+<DT><EM>Default:</EM> 0, 3000 M, KM.
+<DT><EM>Expected input:</EM> Real number in M, KM, 2 values; min.value: 0.000000; max.value: 0.000000.<P>
+Enter the the lower and upper ends of baseline range to plot. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__bas_scale.html b/ngcalc/ngcalc__bas_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..4e55bd307c7795d2b4b1fec71e9c7e418ef1d4d9
--- /dev/null
+++ b/ngcalc/ngcalc__bas_scale.html
@@ -0,0 +1,13 @@
+<TITLE>Description of BAS_SCALE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword BAS_SCALE</H1> 
+
+<DT><EM>Prompt:</EM> Baseline plot scale (metres/cm)
+<DT><EM>Default:</EM> 150..
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__calc_type.html b/ngcalc/ngcalc__calc_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..250b31ddcbd6e88ef7b4a9e6946d46d19f25d321
--- /dev/null
+++ b/ngcalc/ngcalc__calc_type.html
@@ -0,0 +1,36 @@
+<TITLE>Description of CALC_TYPE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword CALC_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> AVER, SMOOTH, POLY, CPOLY, DPOLY, SHIFT, NULL, QUIT calculation type
+<DT><EM>Default:</EM> QUIT.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the action to be performed on individual cut(s). <P>
+	AVER    average cut and report results <P>
+    The following actions will create a new cut for each input cut with the same 
+    index numbers except for a new SEQ number. <P>
+	SMOOTH  create new cut(s) by smoothing cut data with a triangular 
+		 function (whose halfwidth you will specify) <P>
+	POLY    fit N+1 coefficients of an Nth-order polynomial 
+		   P= c0 +c1*HA +c2*HA**2 +... +cN*HA**N 
+		through cut data and create new cut(s) from the residuals <P>
+	CPOLY   as POLY, but fitting only N selected coefficients of an 
+		 Mth-order polynomial. M&gt;N; the missing coefficients are held 
+		 at 0. (This method can be used, e.g., to fit a polynomial for 
+		 which you know a priori that it must be even.) <P>
+	DPOLY   subtract values of a polynomial (yet to be specified) from cut 
+		 data and create new cut(s) from the results <P>
+	SHIFT   create new cuts with visibility values transformed to a 
+		 different sky position <P>
+	NULL    create new cuts with data points in an HA range (yet to be 
+		 selected) deleted <P>
+	QUIT    leave CALC <P>
+Note:   All calculations are done with complex numbers. To use e.g. only 
+	amplitude, convert it first with an expression= AMPL(#..) in 
+	a COMBINE action. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__data_action.html b/ngcalc/ngcalc__data_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..994fb4db1fd1b884acd47ec752bfe57ccb80b339
--- /dev/null
+++ b/ngcalc/ngcalc__data_action.html
@@ -0,0 +1,17 @@
+<TITLE>Description of DATA_ACTION (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword DATA_ACTION</H1> 
+
+<DT><EM>Prompt:</EM> data representation SHOW, AMPLITUDE, PHASE, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify action to perform: <P>
+	SHOW    show detailed cut data <P>
+	AMPL    show amplitude of cut data 
+	PHASE   show phase of cut data <P>
+	QUIT    quit data part <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__expression.html b/ngcalc/ngcalc__expression.html
new file mode 100644
index 0000000000000000000000000000000000000000..487e8ff42809ab01df39184d9fe7d0202bf5d68d
--- /dev/null
+++ b/ngcalc/ngcalc__expression.html
@@ -0,0 +1,55 @@
+<TITLE>Description of EXPRESSION (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword EXPRESSION</H1> 
+
+<DT><EM>Prompt:</EM> expression
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the expression defining the new output cut. It is safest to enclose the 
+expression in double quotes. <P>
+Each data point in the output cut will be set to the value of your expression,  
+using the values of the corresponding data point in each of the input cuts in 
+the expression. Elements of an expression can be: <P>
+	References to input cuts of the form #&lt;number&gt; or ##&lt;number&gt; (see NOTE 
+	 below). You will be prompted later to identify one cut to be associated 
+	 with each of the numbers you use in the expression. For each output 
+	 point, a reference refers to the input point at the same hour angle. <P>
+	Real constants, e.g. 5, -1.23E-12 <P>
+	Symbolic constants 
+		PI [=3.14..], EE [=2.71..], CC [=light velocity in km/s],  
+		DRAD [=180/PI] <P>
+	Standard functions of real or complex argument (angles always in 
+	 degrees): 
+		SIN(x), COS(x), ASIN(x), ACOS(x), ATAN(x), ATAN(real, imag) 
+		EXP(x), EXP10(x), EXP2(x), LOG(x), LOG10(x), LOG2(x) 
+		ABS(X), SQRT(X( 
+		REAL(x), IMAG(x), AMPL(x), PHASE(x), IMUL(x) (mmultiply x by i) <P>
+	Standard functions of a real argument that will be performed separately 
+	 on the real and imaginary components of a complex argument 
+		FLOOR(x), CEIL(x), ROUND(x), INT(x), FRACT(x) <P>
+	Cut-data-point coordinates: 
+		RA [right-ascension], DEC [declination], HA [hour-angle],  
+		UT [univ.time], FQ [freq. in MHz], BL [baseline in m],  
+		UU [U in lambda], VV [V in lambda] <P>
+	Operators, in order of decreasing priority (results of logical and 
+	 relation expressions are 0. (False) or 1. (True)): <P>
+		unary +, - 
+		**, ^ (power) 
+		*, /, +, - 
+		&gt;=, &lt;=, =, &lt;, &gt;, &lt;&gt; (comparisons: if either value to be compared is 
+			   complex, absolute values are used in the comparison) 
+		&lt;&gt; (not)        &amp; (and)         ! (or) <P>
+Example: 
+	#1*(REAL(#1)&lt;0)+#2*(REAL(#2)&gt;0): for each hour angle, take the data 
+		value from cut #1 if it is &lt;0 and the data value from cut #2 if 
+		it is &gt;0, and add them to get the data point at the same hour 
+		angle in the output cut <P>
+NOTE: 
+	You may loop over sectors in the standard way. Each of the input 
+sectors in the expression will be incremented at the start of a new loop cycle. 
+You may, however, inhibit this incrementing by using a double '#', e.g. ##2. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__extract_type.html b/ngcalc/ngcalc__extract_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..1fb6a0d3ef35890530200d23053610b9b8adaf27
--- /dev/null
+++ b/ngcalc/ngcalc__extract_type.html
@@ -0,0 +1,22 @@
+<TITLE>Description of EXTRACT_TYPE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword EXTRACT_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> TCOR, ICOR, IFDATA, DATA, MODEL, WEIGHT, QUIT data type
+<DT><EM>Default:</EM> QUIT.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the type of data to extract: <P>
+	DATA    Observed visibilities 
+	WEIGHT  Visibility weights 
+	MODEL   Model visibilities <P>
+	TCOR    Telescope gain/phase corrections 
+	ICOR    Interferometer gain/phase corrections 
+	IFDATA  'IF' data: gain/system-temperature parameters from the WSRT 
+		 on-line system; you will be asked for details later. <P>
+	QUIT    quit EXTRACT action 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__ha_scale.html b/ngcalc/ngcalc__ha_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..0088e0f659b1e3321bae153e9e686e5f84972126
--- /dev/null
+++ b/ngcalc/ngcalc__ha_scale.html
@@ -0,0 +1,13 @@
+<TITLE>Description of HA_SCALE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword HA_SCALE</H1> 
+
+<DT><EM>Prompt:</EM> hour-angle plot scale degree/cm
+<DT><EM>Default:</EM> 15..
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__ha_width.html b/ngcalc/ngcalc__ha_width.html
new file mode 100644
index 0000000000000000000000000000000000000000..1faddf4ed3752557643af2461d38b68a5d56495f
--- /dev/null
+++ b/ngcalc/ngcalc__ha_width.html
@@ -0,0 +1,13 @@
+<TITLE>Description of HA_WIDTH (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword HA_WIDTH</H1> 
+
+<DT><EM>Prompt:</EM> smoothing width
+<DT><EM>Expected input:</EM> Real number in DEG.<P>
+Specify smoothing halfwidth of triangular smoothing function in degrees of HA. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__if_mode.html b/ngcalc/ngcalc__if_mode.html
new file mode 100644
index 0000000000000000000000000000000000000000..30899787452ef0e054466c4892898ff35cd21d06
--- /dev/null
+++ b/ngcalc/ngcalc__if_mode.html
@@ -0,0 +1,24 @@
+<TITLE>Description of IF_MODE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword IF_MODE</H1> 
+
+<DT><EM>Prompt:</EM> TPON, TPOFF, TNOISI, TSYS, TSYSI, GAIN, GNCAL, TSYSI, TNOISI, RGAINI type of IF data
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify type of 'IF' data to extract: <P>
+   Quantities related to telescope noise sources: 
+	TPON    total-power data for noise source on 
+	TPOFF   total-power data for noise source off 
+	TNOISI  constant noise source temperature <P>
+   Quanitities related to telescope system temperatiures: 
+	TSYS    system temperatures 
+	TSYSI   constant system temperature <P>
+   Quantities related to interferometer gain correction: 
+	GAIN    IF gains 
+	GNCAL   gain correction method 
+	RGAINI  constant receiver gain 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__max_base.html b/ngcalc/ngcalc__max_base.html
new file mode 100644
index 0000000000000000000000000000000000000000..c1ad4a2c95d84c56439e977faa3c0dbe940d249a
--- /dev/null
+++ b/ngcalc/ngcalc__max_base.html
@@ -0,0 +1,13 @@
+<TITLE>Description of MAX_BASE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword MAX_BASE</H1> 
+
+<DT><EM>Prompt:</EM> max. baseline to include (metres)
+<DT><EM>Expected input:</EM> Real number in M.<P>
+Specify maximum baseline to include in output cut. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__mongo_file.html b/ngcalc/ngcalc__mongo_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..21d764df3cf96bb14c5e1f507b6d302d5867a1fc
--- /dev/null
+++ b/ngcalc/ngcalc__mongo_file.html
@@ -0,0 +1,13 @@
+<TITLE>Description of MONGO_FILE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword MONGO_FILE</H1> 
+
+<DT><EM>Prompt:</EM> Mongo file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the name of the file to be used in Mongo plotting. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__ngf_node.html b/ngcalc/ngcalc__ngf_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..0c0ab574e2b8df41408991451a863538dd2f8c47
--- /dev/null
+++ b/ngcalc/ngcalc__ngf_node.html
@@ -0,0 +1,18 @@
+<TITLE>Description of NGF_NODE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword NGF_NODE</H1> 
+
+<DT><EM>Prompt:</EM> Input[+output] 'node' name
+<DT><EM>Expected input:</EM> Character(80).<P>
+This is the file from which input cuts will be read. <P>
+Except in COPY operations, it is also the file to which new cuts will be 
+written. <P>
+Enter ** (or e.g. /user0/mydata/**) to get a list of files, then enter #&lt;n&gt; to 
+select the &lt;n&gt;-th file from such that list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI>Description of the <A HREF="../ngf_descr/ngf_descr.html">NGF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__offset.html b/ngcalc/ngcalc__offset.html
new file mode 100644
index 0000000000000000000000000000000000000000..7bdaf48d79648dae64b762e0c4ffe65c269bf58d
--- /dev/null
+++ b/ngcalc/ngcalc__offset.html
@@ -0,0 +1,15 @@
+<TITLE>Description of OFFSET (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword OFFSET</H1> 
+
+<DT><EM>Prompt:</EM> plot offset (data units)
+<DT><EM>Default:</EM> 0..
+<DT><EM>Expected input:</EM> Real number.<P>
+Example: 
+	If you enter 100, &lt;data values&gt;-100 will be plotted. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__output_ngf_node.html b/ngcalc/ngcalc__output_ngf_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..c4e566e8df93fa00efe9701a25e098bf3cdbf5ac
--- /dev/null
+++ b/ngcalc/ngcalc__output_ngf_node.html
@@ -0,0 +1,17 @@
+<TITLE>Description of OUTPUT_NGF_NODE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword OUTPUT_NGF_NODE</H1> 
+
+<DT><EM>Prompt:</EM> Output 'node' name
+<DT><EM>Expected input:</EM> Character(80).<P>
+This is the file to which cuts will be copied. <P>
+The source and output files MUST be different. <P>
+Enter ** (or e.g. /user0/mydata/**) to get a list of files, enter #nn to select 
+the nn-th file from such a list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI>Description of the <A HREF="../ngf_descr/ngf_descr.html">NGF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__plot_type.html b/ngcalc/ngcalc__plot_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..20dd9c49fc069c54c6296397883fe4dbeb68ef35
--- /dev/null
+++ b/ngcalc/ngcalc__plot_type.html
@@ -0,0 +1,17 @@
+<TITLE>Description of PLOT_TYPE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword PLOT_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> COS, SIN, AMPLITUDE, PHASE cut-data component
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the data component for the output cut: <P>
+	COS     real part 
+	SIN     imaginary part 
+	AMPL    ABS(data) 
+	PHASE   ARG(data) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__poly_coef.html b/ngcalc/ngcalc__poly_coef.html
new file mode 100644
index 0000000000000000000000000000000000000000..3f2d3b88f053053fd9b3799ac9dff93e581c5163
--- /dev/null
+++ b/ngcalc/ngcalc__poly_coef.html
@@ -0,0 +1,14 @@
+<TITLE>Description of POLY_COEF (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword POLY_COEF</H1> 
+
+<DT><EM>Prompt:</EM> polynomial coefficients
+<DT><EM>Expected input:</EM> Real number, 11 values.<P>
+Specify the coefficients of the polynomial to be subtracted: <P>
+	P= c0 +c1*HA +c2*(HA**2) +... +cN*(HA**N) 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__poly_n.html b/ngcalc/ngcalc__poly_n.html
new file mode 100644
index 0000000000000000000000000000000000000000..2ab1583b33a359eec454981f834a619b98a25364
--- /dev/null
+++ b/ngcalc/ngcalc__poly_n.html
@@ -0,0 +1,16 @@
+<TITLE>Description of POLY_N (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword POLY_N</H1> 
+
+<DT><EM>Prompt:</EM> number of coefficients to fit
+<DT><EM>Expected input:</EM> Integer number; min.value: 0.000000; max.value: 10.000000.<P>
+Specify number of coefficients of the polynomial to be fitted to the data. <P>
+For CALC=POLY, this is 1 + the polynomial's degree. <P>
+For CALC=DPOLY it is the number of non-zero coefficients. You will be prompted 
+later for there orders. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__poly_use.html b/ngcalc/ngcalc__poly_use.html
new file mode 100644
index 0000000000000000000000000000000000000000..b6dae9457d5c187a2cdd63feb2bdc8ead6228fcd
--- /dev/null
+++ b/ngcalc/ngcalc__poly_use.html
@@ -0,0 +1,16 @@
+<TITLE>Description of POLY_USE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword POLY_USE</H1> 
+
+<DT><EM>Prompt:</EM> orders of coefficients to fit
+<DT><EM>Expected input:</EM> Integer number, 11 values.<P>
+Specify the orders of the polynomial coefficients to fit to. Default is 
+0, ..., &lt;N&gt;, where &lt;N&gt; is the number you gave for POLY_N. <P>
+Example: 
+    To fit a 6th-degree even polynomial, specify POLY_N=3 and POLY_USE=0, 2, 4, 6. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__scale.html b/ngcalc/ngcalc__scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..96feb674bc7dcb8aadb37136fe06e4da8b1b781a
--- /dev/null
+++ b/ngcalc/ngcalc__scale.html
@@ -0,0 +1,14 @@
+<TITLE>Description of SCALE (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword SCALE</H1> 
+
+<DT><EM>Prompt:</EM> plot scale (data units/mm)
+<DT><EM>Default:</EM> 10..
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the scale in units/mm. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__sector_action.html b/ngcalc/ngcalc__sector_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..ab07dd9a6d393ad4936a2e5886dacf4384c6b2db
--- /dev/null
+++ b/ngcalc/ngcalc__sector_action.html
@@ -0,0 +1,20 @@
+<TITLE>Description of SECTOR_ACTION (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword SECTOR_ACTION</H1> 
+
+<DT><EM>Prompt:</EM> Sector-header action | SHOW, EDIT; NEXT, CONT, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify interaction with this sector header: <P>
+   Show details of the sector header: 
+        SHOW    show entire sector header 
+        EDIT    edit fields (values) in the Sector header by name <P>
+   Navigation: 
+        NEXT:   proceed to the header for the next sector selected 
+        CONT:   descend into the scans of this sector 
+        QUIT:   return to the file-header level <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__select_xyx.html b/ngcalc/ngcalc__select_xyx.html
new file mode 100644
index 0000000000000000000000000000000000000000..7c3e3f6dabfc0e3fea15cab3fe098b301bece517
--- /dev/null
+++ b/ngcalc/ngcalc__select_xyx.html
@@ -0,0 +1,23 @@
+<TITLE>Description of SELECT_XYX (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword SELECT_XYX</H1> 
+
+<DT><EM>Prompt:</EM> XYX, XY, Y, X, YX, YYX, XXY polarisation(s)
+<DT><EM>Expected input:</EM> Character(4).<P>
+Select the polarisation(s) to be used. Your answer will be interpreted 
+according to the data type you will select hereafter <P>
+		Interferometer          Telescope 
+		==============          ========= 
+	XYX     XX, YX, YX and YY       X and Y 
+	XY      XX and YY               X and Y 
+	X       XX only                 X only 
+	Y       YY only                 Y only 
+	YX      XY and YX               none 
+	YYX     YX                      none 
+	XXY     XY                      none 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__shift.html b/ngcalc/ngcalc__shift.html
new file mode 100644
index 0000000000000000000000000000000000000000..4a5bc3e3943f9c7f1e15042550b33c1b0db8424b
--- /dev/null
+++ b/ngcalc/ngcalc__shift.html
@@ -0,0 +1,13 @@
+<TITLE>Description of SHIFT (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword SHIFT</H1> 
+
+<DT><EM>Prompt:</EM> l, m shifts to apply to data (arcsec)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the l, m shifts in arcsec to be applied to data <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc/ngcalc__use_ngf_set.html b/ngcalc/ngcalc__use_ngf_set.html
new file mode 100644
index 0000000000000000000000000000000000000000..4155d55c10dc153ae860beb109baf6992e61d57d
--- /dev/null
+++ b/ngcalc/ngcalc__use_ngf_set.html
@@ -0,0 +1,16 @@
+<TITLE>Description of USE_NGF_SET (NGCALC)</TITLE>
+<H1>Program NGCALC: private keyword USE_NGF_SET</H1> 
+
+<DT><EM>Prompt:</EM> Cut to use
+<DT><EM>Expected input:</EM> Character(32), 1 values.<P>
+Define the cut represented by each of the variables of the form 
+#&lt;n&gt; and ##&lt;n&gt; in your expression. You are being prompted for each such 
+variable that is present in the expression. Your reply must designate ONE cut. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngcalc/ngcalc_keys.html">List of keywords</A> for NGCALC
+<LI>Description of the <A HREF="../ngf_descr/ngf_descr.html">NGF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngcalc_descr/ngcalc_descr.html">program NGCALC</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngcalc_descr.ps b/ngcalc_descr.ps
new file mode 100644
index 0000000000000000000000000000000000000000..3a00e670396c621a3f7e4ea7cd216bf52c7d7f09
--- /dev/null
+++ b/ngcalc_descr.ps
@@ -0,0 +1,2461 @@
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+gs 1 -1 sc (ngcalc_display.fig 45%) col-1 show gr
+$F2psEnd
+restore
+
+%%EndDocument
+ @endspecial 117 2536 a Fd(Figure)14 b(4:)j Fg(NGCALC's)d(he)n
+(ader/data)i(display)f(interfac)n(e.Se)n(e)29 b(\014gur)n(e)15
+b(2)30 b(for)15 b(the)g(over)n(al)r(l)f(interfac)n(e.)935
+2995 y Fd(6)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/ngcalc_descr/_10534_tabular126.png b/ngcalc_descr/_10534_tabular126.png
new file mode 100644
index 0000000000000000000000000000000000000000..5486a2f6eaede020bebc43b9f674ca66bedba825
Binary files /dev/null and b/ngcalc_descr/_10534_tabular126.png differ
diff --git a/ngcalc_descr/_10534_tabular126.xbm b/ngcalc_descr/_10534_tabular126.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b5c4e62f8bb8dbf3b45cb0fbb77b48f7184762c8
--- /dev/null
+++ b/ngcalc_descr/_10534_tabular126.xbm
@@ -0,0 +1,105 @@
+#define noname_width 403
+#define noname_height 30
+static char noname_bits[] = {
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0xfe,0xc3,0x02,0x00,0x00,0x36,0xf2,0xc0,
+ 0xcc,0x36,0xcf,0x79,0x64,0x36,0x03,0x33,0xdb,0x9c,0x47,0xc0,0x88,0xcd,0xd8,
+ 0x0c,0x00,0x00,0x00,0x00,0x00,0x60,0xf4,0x3f,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0xff,0xc3,
+ 0x03,0x00,0x00,0x36,0x36,0xc0,0xfc,0xf6,0xbf,0x61,0x6c,0xf4,0x3f,0x23,0xde,
+ 0xfb,0x47,0xc0,0x08,0xcf,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x04,0x00,
+ 0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x10,0x00,0x80,0x01,0x00,0x00,0x36,0x36,0xc0,0x0e,0x36,0xfc,
+ 0x61,0x6c,0x34,0x3c,0x23,0xdb,0x1f,0x46,0xc0,0x88,0xcd,0xda,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x60,0x04,0x00,0x3a,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x80,0x01,0x00,0x00,
+ 0x36,0x32,0xc0,0x8e,0x36,0xc6,0x71,0x64,0x36,0x02,0xb3,0x79,0x1c,0x47,0xc0,
+ 0xc8,0xdc,0xce,0x0d,0x00,0x00,0x00,0x00,0x00,0x40,0xf6,0x3f,0x31,0x0c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0xff,0x83,0xc1,0x00,0x00,0xef,0x7b,0xc0,0x7b,0xef,0x7d,0xcf,0xe7,0xe3,
+ 0x01,0x1f,0xff,0xf7,0xfc,0x80,0x9f,0xdf,0xfb,0x0d,0x00,0x00,0x00,0x00,0x00,
+ 0xc0,0x06,0xc0,0xf3,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x7c,0x00,0xc0,0xc3,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x03,0x00,0x00,0x08,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ngcalc_descr/_18136_tabular130.png b/ngcalc_descr/_18136_tabular130.png
new file mode 100644
index 0000000000000000000000000000000000000000..5486a2f6eaede020bebc43b9f674ca66bedba825
Binary files /dev/null and b/ngcalc_descr/_18136_tabular130.png differ
diff --git a/ngcalc_descr/_18136_tabular130.xbm b/ngcalc_descr/_18136_tabular130.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b5c4e62f8bb8dbf3b45cb0fbb77b48f7184762c8
--- /dev/null
+++ b/ngcalc_descr/_18136_tabular130.xbm
@@ -0,0 +1,105 @@
+#define noname_width 403
+#define noname_height 30
+static char noname_bits[] = {
+ 0x1c,0x00,0xc0,0x00,0x00,0x00,0x38,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x03,
+ 0x00,0x00,0x60,0x00,0x06,0x00,0x00,0x00,0x00,0x80,0x01,0xc0,0x77,0xbe,0x03,
+ 0x00,0x00,0x08,0x00,0xbe,0xf3,0x38,0x00,0x03,0x00,0x8f,0x7f,0x07,0x00,0x00,
+ 0x38,0x00,0x78,0xfc,0x71,0x00,0x1e,0x00,0xc0,0x00,0x04,0x00,0x3c,0x00,0x00,
+ 0x00,0x00,0x08,0x00,0x00,0x03,0x00,0x00,0x40,0x00,0x04,0x40,0x00,0x00,0x00,
+ 0xc0,0x06,0x80,0x33,0x9c,0x01,0x00,0x00,0x0e,0x00,0x9c,0xe1,0x18,0x80,0x0d,
+ 0x00,0x8e,0x39,0x03,0x00,0x00,0x6c,0x00,0x70,0xcc,0x31,0x00,0x06,0x00,0x00,
+ 0x00,0x06,0x00,0x0c,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x03,0x00,0x00,0x40,
+ 0x00,0x04,0x60,0x00,0x00,0x00,0x40,0x06,0x00,0x17,0xb8,0x00,0x00,0x00,0x08,
+ 0x00,0xb8,0xc0,0x08,0xc0,0x0d,0x00,0x8c,0x70,0x01,0x00,0x00,0x6c,0x00,0x60,
+ 0x84,0x11,0x00,0x06,0x00,0x00,0x00,0x06,0x00,0x0c,0x00,0x00,0x00,0x00,0x0c,
+ 0x00,0x00,0x03,0x00,0x00,0x40,0x00,0x04,0x60,0x00,0x00,0x00,0x60,0x04,0x00,
+ 0x1e,0xf0,0x00,0x00,0x00,0x08,0x00,0xf0,0xc0,0x0d,0xc0,0x09,0x00,0xdc,0xe0,
+ 0x01,0x00,0x00,0x6c,0x00,0xe0,0x86,0x1b,0x00,0xef,0xfb,0xe0,0x7e,0xcf,0xfb,
+ 0xde,0xfb,0xbe,0xff,0xf1,0x1e,0xef,0x03,0x9f,0xe7,0xf3,0x7c,0xc0,0xc7,0xf3,
+ 0x3c,0x06,0x00,0x60,0xe4,0x3f,0x0e,0x70,0x00,0x00,0x00,0x08,0xff,0x71,0x80,
+ 0x05,0x00,0xcc,0x7f,0x58,0xe0,0x00,0x00,0x00,0x30,0xfe,0xc3,0x02,0x0b,0x06,
+ 0x36,0xf2,0xc0,0x4c,0x66,0xf6,0x6c,0xf6,0x23,0x33,0x9b,0x8d,0xd9,0x03,0xb3,
+ 0x6d,0x9a,0x47,0x60,0xc4,0x66,0x6c,0x06,0x00,0x60,0xf4,0x3f,0x0c,0x60,0x00,
+ 0x00,0x00,0x88,0xff,0x61,0x80,0x07,0x00,0xec,0x7f,0x78,0xc0,0x00,0x00,0x00,
+ 0x78,0xff,0xc3,0x03,0x0f,0x06,0x36,0x36,0xc0,0x4c,0xe6,0x37,0xec,0x37,0x63,
+ 0x33,0xfb,0x8d,0xdf,0x3c,0x23,0xef,0xf9,0x47,0x60,0x84,0x67,0x78,0x00,0x00,
+ 0x60,0x04,0x00,0x1e,0xf0,0x00,0x00,0x00,0x08,0x00,0xf0,0x00,0x03,0x00,0x06,
+ 0x00,0x30,0xe0,0x01,0x00,0x00,0x60,0x00,0x80,0x01,0x06,0x00,0x36,0x36,0xc0,
+ 0x4c,0x76,0x30,0x6c,0x30,0x63,0x33,0x1b,0xac,0xc1,0x3c,0xa3,0xed,0x1b,0x46,
+ 0x60,0xc4,0x66,0x6d,0x00,0x00,0x60,0x04,0x00,0x3a,0xd0,0x01,0x00,0x00,0x08,
+ 0x00,0xd0,0x01,0x03,0x00,0x0b,0x00,0x30,0xa0,0x03,0x00,0x00,0x6e,0x00,0x80,
+ 0x01,0x06,0x00,0x36,0x32,0xc0,0x4c,0x76,0x34,0x6c,0x34,0x23,0x33,0x1b,0xad,
+ 0xd1,0x00,0xf3,0x3c,0x1a,0x47,0x60,0x64,0x6e,0xe7,0x06,0x00,0x40,0xf6,0x3f,
+ 0x31,0x88,0x31,0x00,0x00,0x88,0xff,0x89,0x01,0x83,0x81,0xe9,0x7f,0x30,0x10,
+ 0xc3,0x00,0x00,0x6e,0xff,0x83,0x01,0x06,0x06,0xef,0x7b,0xe0,0xff,0xde,0x7b,
+ 0xde,0x7b,0xbe,0xff,0xf7,0x3c,0xef,0x01,0x9f,0xff,0xf3,0xfc,0xc0,0xcf,0xef,
+ 0xfd,0x06,0x00,0xc0,0x06,0xc0,0xf3,0x9e,0x37,0x00,0x00,0x3e,0x00,0x9e,0x87,
+ 0x87,0xc1,0x0f,0x00,0x78,0x3c,0xcf,0x00,0x00,0x6c,0x00,0xc0,0x03,0x0f,0x06,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x03,0x00,0x00,0x00,0x20,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,0x00,0x80,0x00,0x00,
+ 0x18,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,
+ 0x00,0x00,0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,
+ 0x00,0x07,0x00,0x00,0x00,0x00,0x80,0x03,0x00,0x00,0x60,0x00,0x0c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0xc0,0x77,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x78,
+ 0x1c,0x00,0x00,0x1e,0x00,0x80,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x03,0x00,
+ 0x00,0x40,0x00,0x08,0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x06,0x80,
+ 0x33,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x1c,0x00,0x70,0x0c,0x00,0x00,0x06,0x00,0xc0,0x00,0x06,0x00,
+ 0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x40,0x00,0x08,0xc0,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x40,0x06,0x00,0x17,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x60,0x04,0x00,0x00,
+ 0x06,0x00,0xc0,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x40,0x00,
+ 0x08,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x04,0x00,0x1e,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0xe0,0x06,0x00,0x00,0xef,0xfb,0xe0,0x79,0xe6,0x7d,0xdf,0xf7,0xe3,
+ 0x01,0x1f,0xcf,0xf7,0x7c,0x80,0x8f,0xe7,0x79,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x60,0xe4,0x3f,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x10,0xfe,0xc3,0x02,0x00,0x00,0x36,0xf2,0xc0,
+ 0xcc,0x36,0xcf,0x79,0x64,0x36,0x03,0x33,0xdb,0x9c,0x47,0xc0,0x88,0xcd,0xd8,
+ 0x0c,0x00,0x00,0x00,0x00,0x00,0x60,0xf4,0x3f,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0xff,0xc3,
+ 0x03,0x00,0x00,0x36,0x36,0xc0,0xfc,0xf6,0xbf,0x61,0x6c,0xf4,0x3f,0x23,0xde,
+ 0xfb,0x47,0xc0,0x08,0xcf,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x04,0x00,
+ 0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x10,0x00,0x80,0x01,0x00,0x00,0x36,0x36,0xc0,0x0e,0x36,0xfc,
+ 0x61,0x6c,0x34,0x3c,0x23,0xdb,0x1f,0x46,0xc0,0x88,0xcd,0xda,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x60,0x04,0x00,0x3a,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x10,0x00,0x80,0x01,0x00,0x00,
+ 0x36,0x32,0xc0,0x8e,0x36,0xc6,0x71,0x64,0x36,0x02,0xb3,0x79,0x1c,0x47,0xc0,
+ 0xc8,0xdc,0xce,0x0d,0x00,0x00,0x00,0x00,0x00,0x40,0xf6,0x3f,0x31,0x0c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0xff,0x83,0xc1,0x00,0x00,0xef,0x7b,0xc0,0x7b,0xef,0x7d,0xcf,0xe7,0xe3,
+ 0x01,0x1f,0xff,0xf7,0xfc,0x80,0x9f,0xdf,0xfb,0x0d,0x00,0x00,0x00,0x00,0x00,
+ 0xc0,0x06,0xc0,0xf3,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x7c,0x00,0xc0,0xc3,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x03,0x00,0x00,0x08,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/ngcalc_descr/images.pl b/ngcalc_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..58e0f492064876a93b23e3501a84f278398749b0
--- /dev/null
+++ b/ngcalc_descr/images.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{tabular}<<127>>lllll<<127>>;html_special_mark_amp;forinterferometer-baseddata:;html_special_mark_amp;0=XX,;html_special_mark_amp;1=XY,2=YX,;html_special_mark_amp;3=YY;;html_special_mark_amp;fortelescope-baseddata:;html_special_mark_amp;0=X,;html_special_mark_amp;;html_special_mark_amp;1=Y.{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10534_tabular126.xbm">'; 
+$key = q/{tabular}<<131>>lllll<<131>>;html_special_mark_amp;forinterferometer-baseddata:;html_special_mark_amp;0=XX,;html_special_mark_amp;1=XY,2=YX,;html_special_mark_amp;3=YY;;html_special_mark_amp;fortelescope-baseddata:;html_special_mark_amp;0=X,;html_special_mark_amp;;html_special_mark_amp;1=Y.{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_18136_tabular130.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/ngcalc_descr/labels.pl b/ngcalc_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..acff3699aa77925eacc954954e12a2462452f087
--- /dev/null
+++ b/ngcalc_descr/labels.pl
@@ -0,0 +1,19 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".inspect"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".ngcalc.display"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".extract"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".ngcalc.interface"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".ngf.file"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".ngf.scn.indices"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".combine"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".merge"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".contents"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".delete"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".general.features"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".ngcalc.extract"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".loops"} ="$URL/ngcalc_descr.html"; 
+$external_labels{".general"} ="$URL/ngcalc_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/ngcalc_descr/ngcalc_descr.html b/ngcalc_descr/ngcalc_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..c76f72941dfe5adb3e124c570469ac546f528d54
--- /dev/null
+++ b/ngcalc_descr/ngcalc_descr.html
@@ -0,0 +1,168 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NGCALC</b>  
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ngcalc_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ngcalc_descr.html#SECTION0002000000000000000>  <b>General</b></A>
+<LI> <A NAME=tex2html3 HREF=ngcalc_descr.html#SECTION0003000000000000000>  <b>The .NGF file</b></A>
+<LI> <A NAME=tex2html4 HREF=ngcalc_descr.html#SECTION0004000000000000000>  <b>General features of the parameter interface</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=ngcalc_descr.html#SECTION0004100000000000000>  <b>Special use of NGF_LOOPS</b></A>
+<LI> <A NAME=tex2html6 HREF=ngcalc_descr.html#SECTION0004200000000000000>  <b>The DELETE and COPY options</b></A>
+<LI> <A NAME=tex2html7 HREF=ngcalc_descr.html#SECTION0004300000000000000> <b>New cuts created by combining input cuts</b></A>
+<LI> <A NAME=tex2html8 HREF=ngcalc_descr.html#SECTION0004400000000000000>  <b>Inspecting the contents of an .NGF file</b></A>
+</UL> 
+<LI> <A NAME=tex2html9 HREF=ngcalc_descr.html#SECTION0005000000000000000>  <b>Extracting data from a .SCN file</b></A>
+<LI> <A NAME=tex2html10 HREF=ngcalc_descr.html#SECTION0006000000000000000>  <b>Merging cuts</b></A>
+</UL>
+<A NAME=.general><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000>  <b>General</b></A></H1>
+<P>
+        NGCALC is a program for extracting information from .SCN-file data and then manipulating it in a great variety of ways. The data may be either interferometer-based (visibilities) or telescope-based (e.g. corrections).
+<P>
+        This document is still far from complete, but it is hoped that it gives you somethging of a handle to start exploring on your own the many possibilities that NGCALC offers.
+<P>
+<A NAME=.ngf.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000>  <b>The .NGF file</b></A></H1>
+<P>
+        The extracted data are organised and manipulated in a special type of file, the <em>.NGF file</em>.
+<P>
+        The .NGF file contains a collection of <em>cuts</em> i.e. vectors representing the values of some quantity as a function of either hour angle or frequency. (You may still come across the term <em>plots</em> for these cuts, - and corresponding the the .NGF file may be referred to as a <em>plot file</em> -, but this unfortunate terminology is being phased out.) Each cut has a header containing relevant parameters such as interferometer designation, bandwidth, center frequency, hour-angle range etc.
+<P>
+        The cuts are organised in an index structure similar to that for sectors in a .SCN file and maps in the .WMP file. The order of the indices is
+<P>
+  &lt;grp&gt;.&lt;fld&gt;.&lt;chn&gt;.&lt;pol&gt;.&lt;iort&gt;.&lt;seq&gt;
+<P>
+For each cut, the index is derived automatically from the index of the sector from which the data are taken. This is shown schematically in  
+<A HREF=" #.ngf.scn.indices">figure</A> and explained below:
+<P>
+<A NAME=.ngf.scn.indices><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Derivation of .NGF-file cut indices from .SCN-file sector indices 
+<A HREF="../fig/ngf_scn_indices.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR>This diagram schematically indicates how the cut indices in the .NGF file are related to the sector indices in the .SCN file, - which in turn are derived from the hierarchical structure of the WSRT observation file. </i>
+<P>
+<UL><LI>   The &lt;grp&gt; (<em>group</em>) numbers are automatically assigned in sequential order. A group generally contains all cuts produced in a single run of NGCALC. In extracting data from a .SCN file, different input groups and/or observations are mapped to different output groups.  
+<LI>   &lt;fld&gt; (<em>field</em>) and  
+<LI>   &lt;chn&gt; (<em>channel</em>) are those for the data in the .SCN file from which the cut was made.  
+<LI>   &lt;pol&gt; (<em>polarisation</em>) is a fixed code:
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_18136_tabular130.png"><P>
+<P>
+<LI>   &lt;iort&gt; (<em>interferometer</em>for interferometer-based data) is a sequence number whose only function is to distinguish cuts for different interferometers. In general, you will use this index only in specifying 
+<A HREF="#.loops"><b>loops</b></A> to process interferometers one by one; for <em>selecting</em>interferometers, the SELECT_IFRSparameter is more convenient  
+<LI>   &lt;iort&gt; (<em>telecsope</em>for telecope-based data) is analogous to that for interferometers and the remarks made above on its use apply here as well; in particular, the index value does <em>not</em>necessarily correpond to the telescope number.  
+<LI>   &lt;seq&gt; (<em>sequence number</em>) is a number making it possible to have several different kinds of cut with all preceding indices identical.  
+</UL>
+<P>
+<A NAME=.ngcalc.interface><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of NGCALC's parameter interface. 
+<A HREF="../fig/ngcalc_interface.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See also: 
+<BR><A HREF=" #.ngcalc.extract">figure</A> for details of the <em>EXTRACT</em> operation 
+<BR><A HREF=" #.ngcalc.display">figure</A> for details of the display operations </i>
+<P>
+<A NAME=.ngcalc.extract><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> NGCALC's cut-extract interface. 
+<A HREF="../fig/ngcalc_extract.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See <A HREF=" #.ngcalc.interface">figure</A> for the overall interface. </i>
+<P>
+<A NAME=.ngcalc.display><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> NGCALC's header/data display interface. 
+<A HREF="../fig/ngcalc_display.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See <A HREF=" #.ngcalc.interface">figure</A> for the overall interface. </i>
+<P>
+<A NAME=.general.features><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>General features of the parameter interface</b></A></H1>
+<P>
+<A NAME=.loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000>  <b>Special use of NGF_LOOPS</b></A></H2>
+<P>
+        In certain operations, sets of input cuts are combined to produce some output, e.g. some statistic as in the CALC option, or a new cut as in the MERGE option. To process such sets per interferometer, the 
+NGF_LOOPS parameter may be used to loop over the interferometers one by one by specifying an increment for the <A HREF="#.ngf.file"><b>iort index</b></A>, e.g.
+<P>
+  NGF_LOOPS = 65, ....1
+<P>
+If you do not know the number of interferometers, you may have all of them processed by their number as 91 (the largest possible number) or higher.
+<P>
+<A NAME=.delete><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000>  <b>The DELETE and COPY options</b></A></H2>
+<P>
+        It is rather easy to make mistakes in defining operations that combine cuts. To get rid of the resultant clutter in an .NGF file, NGCALC offers the option to DELETE (sets of) cuts. The data are not actually deleted but simply disconnected from the index structure which makes them invisible; be careful: this process is <em>irrevrsible</em>!
+<P>
+        Deleted data may still occupy more disk space than you want. The 
+COPY operation may be used to create a new .NGF file from which the deleted data along with the corresponding index structures are actually removed.  The indices of valid data are copied unchanged, so e.g. the group numbers in the output file may form a non-contiguous series.
+<P>
+<A NAME=.combine><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004300000000000000> <b>New cuts created by combining input cuts</b></A></H2>
+<P>
+        Several options, such as MERGE and COMBINE, combine data from multiple input cuts to create new cuts. In such cases, NGCALC tries to assign sensible values to the output cut's header parameters, but one cannot rely blindly on them.
+<P>
+        The TRANS and BASE operations transpose data in the three-dimensional hour-angle/baseline/frequency-channel data cube. The cuts for the transposed data mostly use the same header parameters as the original cuts and some educated guessing may be necessary to figure out what these parameters mean.
+<P>
+<A NAME=.inspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004400000000000000>  <b>Inspecting the contents of an .NGF file</b></A></H2>
+<P>
+        The BRIEF and FULL options can be used to inspect the composition of your file. BRIEF provides a quick survey, FULL gives details per individual cuts. Since the number of cuts in a file may be quite large, the recommended way to explore a .NGF file is to start with  
+BRIEF and use FULL only to get details about one or a few cuts.
+<P>
+<A NAME=.extract><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000>  <b>Extracting data from a .SCN file</b></A></H1>
+<P>
+        The first step in using NGCALC is to extract the necessary data from one or more .SCN files and store it in an .NGF file. The number of output cuts equals the number of input sectors times the numer of selected interferometers; so in cases where the former is already considerable you should think carefully about what you need.
+<P>
+The mapping of the .SCN-file sector indices to .NGF-file cut indices is shown schematically in a diagram <A HREF=" #.ngf.scn.indices">figure</A>.
+<P>
+<A NAME=.merge><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000>  <b>Merging cuts</b></A></H1>
+<P>
+        The MERGE option enables you to merge a set of cuts into a new one; the NGF_LOOPS parameter may be used to execute a whole series of mergers in a single operation.
+<P>
+        In the merge algorithm, the input cut data are sorted in hour-angle bins .25 deg wide and averaged per bin. The resulting output is stored in a contiguous sequence of points equidistant at .25 deg, long enough to hold the data; see <A HREF=" #.ngcalc.merge">figure</A>.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ngcalc_keys/ngcalc_keys.html b/ngcalc_keys/ngcalc_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..e69de29bb2d1d6434b8b29ae775ad8c2e48c5391
diff --git a/ngcalc_lightcurve.txt b/ngcalc_lightcurve.txt
new file mode 100644
index 0000000000000000000000000000000000000000..a9e08acfe33de90ab86cf5f1616b96082ba049f6
--- /dev/null
+++ b/ngcalc_lightcurve.txt
@@ -0,0 +1,112 @@
+I,Q,U,V,p,angle lightcurves using NEWSTAR program NGCALC
+
+
+Ger de Bruyn 15-juni-1994
+
+The program NGCALC can extract 1-dimensional (Visibility data versus
+time/HA) data from a SCN-file. These can then be processed to yield
+lightcurves of all Stokes parameters for a range of baselines.
+
+A 'typical' run would go as follows:
+
+1) exe ngcalc/ask
+
+The /ask qualifier is only required if you wish to subtract the STORED
+selfcal MDL from the selfcal'ed visibility data.
+
+Input:
+ - the name of the NGF file you wish to create
+ - select option EXTRACT
+ - specify the name of the SCN-file
+ - select the SETS
+ - select the type of information you want to process (e.g. DATA)
+ - select the polarizations (specify XYX if you wish to form all
+   Stokes parameters)
+ - select the INTERFEROMETERS (e.g. FM)
+
+This is a slow program! It takes about 20 minutes CPU (on an HP710)
+for the extraction of 12 hours of data (720 scans of 1 minute) on 40
+baselines on one frequncy channel for each of the four XX,XY,YX,YY
+correlations. This then creates 40x4 files or 'plots' as they are called in
+the program.
+
+These plots will have a six-digit number containing information on the
+baselines, polarizations and frequency channel.
+
+2) Use the option MERGE to merge different HA-sections
+
+If the 12 hour observations was cut into more than one part, each
+HA-sector will get a separate file. You can then merge these two or
+more HA-slots into one file, where the appropriate HA information is
+preserved.
+
+You can use a double-loop here. One loop might run over polarization
+and one loop over baselines; e.g. 4,...1, 69,....1 if you had
+XX,XY,YX,YY and baselines from 9A (a 0 in the fifth digit) through 0D
+(a 68 in the fifth digit)
+
+
+3) Use option CALC, SHIFT to shift the visibilities to the source you
+wish to study
+
+Use the position (l,m in arcseconds) as given in your MODEL. You may
+(have to) use a loop again.
+
+
+4) Use the option MERGE to average all baselines you wish to use
+
+After the shift operation the source should be in the phase centre. This
+means that the source signal is contained in the COS part of the visibility.
+You can check, using the plotting facilities, whether indeed the SIN signal
+is consistent with noise around zero.
+
+You may wish to loop here over the fourth, polarization, index (e.g.
+4,...1)
+
+
+5) Use the COMBINE option to form Stokes I,Q,U and V
+
+Examples: 
+Q = (#0-#1)/2, where #0 is the YY file and #1 is the XX file.
+V = -0.5*imul(#0+#1) where #0 is the XY file and #1 is the YX file
+
+
+6) If required, smooth the data using option CALC, SMOOTH
+
+
+7) You can use the PLOT option at the various stages to see whether the
+results look as 'expected'
+
+8) Use option MON to dump the interesting files in an ASCII file for
+further processing with SUPERMONGO. The mongo file will contain as its first
+column the HA.
+
+  
+
+-----------------------------------------------------------
+N.B. There are a number of things to watch out for when using NGCALC
+
+1) Files can be addressed with the full six-digit index or with a # whichever
+you find more convenient. Note, however, that when using the #'s you can
+NOT use loops. 
+
+2) There is some logic to the index numbering system but it takes a while to
+get use to it. 
+
+3) When trying to form the polarization angle 0.5*atan(U/Q) you run into 
+the problem that this angle as calculated will be within the range -45 to
++45 degrees, while of course the true polarization angle is defined 
+within boundaries -90 and +90 degrees
+
+4) Unfortunately, the delete option does not yet work. If you have made a
+new file with erroneous specifications you would ideally like to
+throw it away because you might forget that it is unusable. 
+
+5) When using the loop system all the plotfiles that will be
+tried in the looping must be present.
+
+E.g. if you have 40 FM baselines in the NGF file they are numbered 0,2,8,9,....68
+with some numbers not occurring (This number is the order in which the
+baselines exist in the SCN file). Hence, if you wish to loop over baselines
+then you could say 69,....1 but then the program will stop after it has 
+done the first baseline, because baseline ....1 does not exist.
diff --git a/ngcalc_private_intfc.ps b/ngcalc_private_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..f4daddab713ab882a27ea4fa450813d63b3f220e
--- /dev/null
+++ b/ngcalc_private_intfc.ps
@@ -0,0 +1,2609 @@
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+
+%%EndDocument
+ @endspecial 117 2536 a Fg(Figure)14 b(3:)j Fj(NGCALC's)d(he)n
+(ader/data)i(display)f(interfac)n(e.Se)n(e)29 b(\014gur)n(e)15
+b(1)30 b(for)15 b(the)g(over)n(al)r(l)f(interfac)n(e.)924
+2995 y Fg(11)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/ngcalc_private_intfc/images.pl b/ngcalc_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ngcalc_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ngcalc_private_intfc/labels.pl b/ngcalc_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..1fd69fde27efdbaeb5eede338224826e112ddb13
--- /dev/null
+++ b/ngcalc_private_intfc/labels.pl
@@ -0,0 +1,35 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".extract.type"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".public"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".scale"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".ha.scale"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".ngcalc.interface"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".shift"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".max.base"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".output.ngf.node"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".data.action"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".bas.range"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".ngcalc.extract"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".expression"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".poly.n"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".mongo.file"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".action"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".plot.type"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".ngcalc.display"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".bas.scale"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".calc.type"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".offset"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".select.xyx"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".ha.width"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".use.ngf.set"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".ngf.node"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".sector.action"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".if.mode"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".poly.coef"} ="$URL/ngcalc_private_intfc.html"; 
+$external_labels{".poly.use"} ="$URL/ngcalc_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/ngcalc_private_intfc/ngcalc_private_intfc.html b/ngcalc_private_intfc/ngcalc_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..8dfa4c9b2e69bde70a3a5acef7d7fa45e4f7df7b
--- /dev/null
+++ b/ngcalc_private_intfc/ngcalc_private_intfc.html
@@ -0,0 +1,656 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NGCALC</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ngcalc_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<UL> 
+<LI> <A NAME=tex2html2 HREF=ngcalc_private_intfc.html#SECTION0001100000000000000>  <b>References to public interfaces</b></A>
+</UL> 
+<LI> <A NAME=tex2html3 HREF=ngcalc_private_intfc.html#SECTION0002000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ngcalc_private_intfc.html#SECTION0002100000000000000>  <b>Parameter ACTION</b></A>
+<LI> <A NAME=tex2html5 HREF=ngcalc_private_intfc.html#SECTION0002200000000000000>  <b>Parameter BAS_RANGE</b></A>
+<LI> <A NAME=tex2html6 HREF=ngcalc_private_intfc.html#SECTION0002300000000000000>  <b>Parameter BAS_SCALE</b></A>
+<LI> <A NAME=tex2html7 HREF=ngcalc_private_intfc.html#SECTION0002400000000000000>  <b>Parameter CALC_TYPE</b></A>
+<LI> <A NAME=tex2html8 HREF=ngcalc_private_intfc.html#SECTION0002500000000000000>  <b>Parameter DATA_ACTION</b></A>
+<LI> <A NAME=tex2html9 HREF=ngcalc_private_intfc.html#SECTION0002600000000000000>  <b>Parameter EXPRESSION</b></A>
+<LI> <A NAME=tex2html10 HREF=ngcalc_private_intfc.html#SECTION0002700000000000000>  <b>Parameter EXTRACT_TYPE</b></A>
+<LI> <A NAME=tex2html11 HREF=ngcalc_private_intfc.html#SECTION0002800000000000000>  <b>Parameter HA_SCALE</b></A>
+<LI> <A NAME=tex2html12 HREF=ngcalc_private_intfc.html#SECTION0002900000000000000>  <b>Parameter HA_WIDTH</b></A>
+<LI> <A NAME=tex2html13 HREF=ngcalc_private_intfc.html#SECTION00021000000000000000>  <b>Parameter IF_MODE</b></A>
+<LI> <A NAME=tex2html14 HREF=ngcalc_private_intfc.html#SECTION00021100000000000000>  <b>Parameter MAX_BASE</b></A>
+<LI> <A NAME=tex2html15 HREF=ngcalc_private_intfc.html#SECTION00021200000000000000>  <b>Parameter MONGO_FILE</b></A>
+<LI> <A NAME=tex2html16 HREF=ngcalc_private_intfc.html#SECTION00021300000000000000>  <b>Parameter NGF_NODE</b></A>
+<LI> <A NAME=tex2html17 HREF=ngcalc_private_intfc.html#SECTION00021400000000000000>  <b>Parameter OFFSET</b></A>
+<LI> <A NAME=tex2html18 HREF=ngcalc_private_intfc.html#SECTION00021500000000000000>  <b>Parameter OUTPUT_NGF_NODE</b></A>
+<LI> <A NAME=tex2html19 HREF=ngcalc_private_intfc.html#SECTION00021600000000000000>  <b>Parameter PLOT_TYPE</b></A>
+<LI> <A NAME=tex2html20 HREF=ngcalc_private_intfc.html#SECTION00021700000000000000>  <b>Parameter POLY_COEF</b></A>
+<LI> <A NAME=tex2html21 HREF=ngcalc_private_intfc.html#SECTION00021800000000000000>  <b>Parameter POLY_N</b></A>
+<LI> <A NAME=tex2html22 HREF=ngcalc_private_intfc.html#SECTION00021900000000000000>  <b>Parameter POLY_USE</b></A>
+<LI> <A NAME=tex2html23 HREF=ngcalc_private_intfc.html#SECTION00022000000000000000>  <b>Parameter SCALE</b></A>
+<LI> <A NAME=tex2html24 HREF=ngcalc_private_intfc.html#SECTION00022100000000000000>  <b>Parameter SECTOR_ACTION</b></A>
+<LI> <A NAME=tex2html25 HREF=ngcalc_private_intfc.html#SECTION00022200000000000000>  <b>Parameter SELECT_XYX</b></A>
+<LI> <A NAME=tex2html26 HREF=ngcalc_private_intfc.html#SECTION00022300000000000000>  <b>Parameter SHIFT</b></A>
+<LI> <A NAME=tex2html27 HREF=ngcalc_private_intfc.html#SECTION00022400000000000000>  <b>Parameter USE_NGF_SET</b></A>
+</UL>
+</UL>
+<A NAME=.ngcalc.interface><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of NGCALC's parameter interface. 
+<A HREF="../fig/ngcalc_interface.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See also: 
+<BR><A HREF=" #.ngcalc.extract">figure</A> for details of the <em>EXTRACT</em> operation 
+<BR><A HREF=" #.ngcalc.display">figure</A> for details of the display operations </i>
+<P>
+<A NAME=.ngcalc.extract><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> NGCALC's cut-extract interface. 
+<A HREF="../fig/ngcalc_extract.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See <A HREF=" #.ngcalc.interface">figure</A> for the overall interface. </i>
+<P>
+<A NAME=.ngcalc.display><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> NGCALC's header/data display interface. 
+<A HREF="../fig/ngcalc_display.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See <A HREF=" #.ngcalc.interface">figure</A> for the overall interface. </i>
+<P>
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0001100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../ngfsets_public_intfc/ngfsets_public_intfc.html">NGFSETS</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../nshow_public_intfc/nshow_public_intfc.html">NSHOW</A> public keywords 
+<LI> <A HREF="../plotter_public_intfc/plotter_public_intfc.html">PLOTTER</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+</UL>
+<P>
+<A NAME=.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002100000000000000>  <b>Parameter ACTION</b></A></H2>
+<P>
+  <em>Prompt:</em> type of action |<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+    <PRE>
+Specify the action to be performed:
+</PRE>
+<P>
+  <PRE>
+   Creating cuts from external data:
+        EXTRACT extract information from SCN file into cuts
+        COPY    copy cuts to other NGF file, retaining their indices
+                 (this action is mainly useful for discarding cuts no longer
+                  needed and thereby freeing disk space)
+</PRE>
+<P>
+  <PRE>
+   Viewing the contents of the .NGF file:
+        SHOW    show information in cut headers and data
+        BRIEF   show summary per group/field showing numbers of polarisations,
+                interferometers, cuts and data points
+</PRE>
+<P>
+  <PRE>
+   Calculations:
+        CALC    Perform one of a set of predefined algorithms on individual cuts
+        MERGE   Merge a number of cuts into a single new cut.
+                NOTE: Overlapping points will be averaged so you may use MERGE
+                      to average e.g. a set of interferometers with data points
+                      at coincident hour angles.
+        COMBINE Combine cut(s) in user-specified expression
+</PRE>
+<P>
+  <PRE>
+   Sorting:
+     Starting from a cut in the HA direction, these actions produce a new cut
+in the frequency or baseline direction for each hour angle present in any of
+the input cuts. Use the HA_RANGE parameter to limit the number of output cuts.
+     The output cuts are in a primitive format in which the data are transposed
+but NOT the coordinate axes. These wrong axes appear in plots of the transposed
+cuts and must be interpreted as indicated below. In calculations, however,
+coordinates will be interpreted correctly (provided you specify a sensible
+calculation).
+</PRE>
+<P>
+  <PRE>
+     Transposing a transposed group of cuts reproduces the original cuts. You
+may also try to combine TRANS and BASE operations but sensible results are not
+guaranteed.
+</PRE>
+<P>
+  <PRE>
+        TRANS   transpose frequency and HA axes.
+                In the transposed cuts, each channel is represented by an hour
+                angle of <channel number>*0.125 deg.
+                Each hour-angle bin of 0.125 deg is represented by a channel
+                number, which starts at 0 for the lowest hour angle present.
+</PRE>
+<P>
+  <PRE>
+        BASE    transpose interferometer and hour-angle axes.
+                In the transposed cuts, each baseline bin of 10 metres is
+                represented by an HA bin of .125 deg at HA = <baseline>/10*.125
+                deg; baselines landing in the same bin are averaged.
+                Each hour-angle bin of .125 deg is represented by a baseline
+                sequence number of HA*.125.
+</PRE>
+<P>
+  <PRE>
+   Plotting:
+        MONGO   output cut data in a MONGO-readable file
+        PLOT    plot data in NGF cut(s)
+</PRE>
+<P>
+  <PRE>
+   Miscellaneous:
+        DELETE  delete cuts. (Only the index linkage is removed but the cut data
+                 remain in the file: Use COPY to free the file space.)
+                BEWARE: This action is IRREVERSIBLE.
+        NODE    switch to other NGF file
+        QUIT    terminate NGCALC
+</PRE>
+<P>
+  <PRE>
+   Data-format conversions:
+        CVX     convert NGF file from other machine's format to local format
+        NVS     update to latest NGF-file format
+</PRE>
+<P>
+<A NAME=.bas.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002200000000000000>  <b>Parameter BAS_RANGE</b></A></H2>
+<P>
+<em>Prompt:</em> Baseline range (metres)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Enter the the lower and upper ends of baseline range to plot.
+</PRE>
+<P>
+<A NAME=.bas.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002300000000000000>  <b>Parameter BAS_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> Baseline plot scale (metres/cm)<BR><em>Expected input:</em> Real:  1 value
+<P>
+<A NAME=.calc.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002400000000000000>  <b>Parameter CALC_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> calculation type<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the action to be performed on individual cut(s).
+</PRE>
+<P>
+  <PRE>
+        AVER    average cut and report results
+</PRE>
+<P>
+  <PRE>
+    The following actions will create a new cut for each input cut with the same
+    index numbers except for a new SEQ number.
+</PRE>
+<P>
+  <PRE>
+        SMOOTH  create new cut(s) by smoothing cut data with a triangular
+                 function (whose halfwidth you will specify)
+</PRE>
+<P>
+  <PRE>
+        POLY    fit N+1 coefficients of an Nth-order polynomial
+                   P= c0 +c1*HA +c2*HA**2 +... +cN*HA**N
+                through cut data and create new cut(s) from the residuals
+</PRE>
+<P>
+  <PRE>
+        CPOLY   as POLY, but fitting only N selected coefficients of an
+                 Mth-order polynomial. M>N; the missing coefficients are held
+                 at 0. (This method can be used, e.g., to fit a polynomial for
+                 which you know a priori that it must be even.)
+</PRE>
+<P>
+  <PRE>
+        DPOLY   subtract values of a polynomial (yet to be specified) from cut
+                 data and create new cut(s) from the results
+</PRE>
+<P>
+  <PRE>
+        SHIFT   create new cuts with visibility values transformed to a
+                 different sky position
+</PRE>
+<P>
+  <PRE>
+        NULL    create new cuts with data points in an HA range (yet to be
+                 selected) deleted
+</PRE>
+<P>
+  <PRE>
+        QUIT    leave CALC
+Note:   All calculations are done with complex numbers. To use e.g. only
+        amplitude, convert it first with an expression= AMPL(#..) in
+        a COMBINE action.
+</PRE>
+<P>
+<A NAME=.data.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002500000000000000>  <b>Parameter DATA_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> data representation<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+        SHOW    show detailed cut data
+</PRE>
+<P>
+  <PRE>
+        AMPL    show amplitude of cut data
+        PHASE   show phase of cut data
+</PRE>
+<P>
+  <PRE>
+        QUIT    quit data part
+</PRE>
+<P>
+<A NAME=.expression><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002600000000000000>  <b>Parameter EXPRESSION</b></A></H2>
+<P>
+<em>Prompt:</em> expression<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the expression defining the new output cut. It is safest to enclose the
+expression in double quotes.
+</PRE>
+<P>
+  <PRE>
+Each data point in the output cut will be set to the value of your expression,
+using the values of the corresponding data point in each of the input cuts in
+the expression. Elements of an expression can be:
+</PRE>
+<P>
+  <PRE>
+        References to input cuts of the form #<number> or ##<number> (see NOTE
+         below). You will be prompted later to identify one cut to be associated
+         with each of the numbers you use in the expression. For each output
+         point, a reference refers to the input point at the same hour angle.
+</PRE>
+<P>
+  <PRE>
+        Real constants, e.g. 5, -1.23E-12
+</PRE>
+<P>
+  <PRE>
+        Symbolic constants
+                PI [=3.14..], EE [=2.71..], CC [=light velocity in km/s],
+                DRAD [=180/PI]
+</PRE>
+<P>
+  <PRE>
+        Standard functions of real or complex argument (angles always in
+         degrees):
+                SIN(x), COS(x), ASIN(x), ACOS(x), ATAN(x), ATAN(real,imag)
+                EXP(x), EXP10(x), EXP2(x), LOG(x), LOG10(x), LOG2(x)
+                ABS(X), SQRT(X(
+                REAL(x), IMAG(x), AMPL(x), PHASE(x), IMUL(x) (mmultiply x by i)
+</PRE>
+<P>
+  <PRE>
+        Standard functions of a real argument that will be performed separately
+         on the real and imaginary components of a complex argument
+                FLOOR(x), CEIL(x), ROUND(x), INT(x), FRACT(x)
+</PRE>
+<P>
+  <PRE>
+        Cut-data-point coordinates:
+                RA [right-ascension], DEC [declination], HA [hour-angle],
+                UT [univ.time], FQ [freq. in MHz], BL [baseline in m],
+                UU [U in lambda], VV [V in lambda]
+</PRE>
+<P>
+  <PRE>
+        Operators, in order of decreasing priority (results of logical and
+         relation expressions are 0. (False) or 1. (True)):
+</PRE>
+<P>
+  <PRE>
+                unary +,-
+                **,^ (power)
+                *, /, +, -
+                >=,<=,=,<,>,<> (comparisons: if either value to be compared is
+                           complex, absolute values are used in the comparison)
+                <> (not)        & (and)          (or)
+</PRE>
+<P>
+  <PRE>
+Example:
+        #1*(REAL(#1)<0)+#2*(REAL(#2)>0): for each hour angle, take the data
+                value from cut #1 if it is <0 and the data value from cut #2 if
+                it is >0, and add them to get the data point at the same hour
+                angle in the output cut
+</PRE>
+<P>
+  <PRE>
+NOTE:
+        You may loop over sectors in the standard way. Each of the input
+sectors in the expression will be incremented at the start of a new loop cycle.
+You may, however, inhibit this incrementing by using a double '#', e.g. ##2.
+</PRE>
+<P>
+<A NAME=.extract.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002700000000000000>  <b>Parameter EXTRACT_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> data type<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the type of data to extract:
+</PRE>
+<P>
+  <PRE>
+        DATA    Observed visibilities
+        WEIGHT  Visibility weights
+        MODEL   Model visibilities
+</PRE>
+<P>
+  <PRE>
+        TCOR    Telescope gain/phase corrections
+        ICOR    Interferometer gain/phase corrections
+        IFDATA  'IF' data: gain/system-temperature parameters from the WSRT
+                 on-line system; you will be asked for details later.
+</PRE>
+<P>
+  <PRE>
+        QUIT    quit EXTRACT action
+</PRE>
+<P>
+<A NAME=.ha.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002800000000000000>  <b>Parameter HA_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> hour-angle plot scale degree/cm<BR><em>Expected input:</em> Real:  1 value
+<P>
+<A NAME=.ha.width><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002900000000000000>  <b>Parameter HA_WIDTH</b></A></H2>
+<P>
+<em>Prompt:</em> smoothing width<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify smoothing halfwidth of triangular smoothing function in degrees of HA.
+</PRE>
+<P>
+<A NAME=.if.mode><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021000000000000000>  <b>Parameter IF_MODE</b></A></H2>
+<P>
+<em>Prompt:</em> type of IF data<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify type of 'IF' data to extract:
+</PRE>
+<P>
+  <PRE>
+   Quantities related to telescope noise sources:
+        TPON    total-power data for noise source on
+        TPOFF   total-power data for noise source off
+        TNOISI  constant noise source temperature
+</PRE>
+<P>
+  <PRE>
+   Quanitities related to telescope system temperatiures:
+        TSYS    system temperatures
+        TSYSI   constant system temperature
+</PRE>
+<P>
+  <PRE>
+   Quantities related to interferometer gain correction:
+        GAIN    IF gains
+        GNCAL   gain correction method
+        RGAINI  constant receiver gain
+</PRE>
+<P>
+<A NAME=.max.base><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021100000000000000>  <b>Parameter MAX_BASE</b></A></H2>
+<P>
+<em>Prompt:</em> max. baseline to include (metres)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify maximum baseline to include in output cut.
+</PRE>
+<P>
+<A NAME=.mongo.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021200000000000000>  <b>Parameter MONGO_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> Mongo file name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the name of the file to be used in Mongo plotting.
+</PRE>
+<P>
+<A NAME=.ngf.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021300000000000000>  <b>Parameter NGF_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> Input[+output] 'node' name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+This is the file from which input cuts will be read.
+</PRE>
+<P>
+  <PRE>
+Except in COPY operations, it is also the file to which new cuts will be
+written.
+</PRE>
+<P>
+  <PRE>
+Enter ** (or e.g. /user0/mydata/**) to get a list of files, then enter #<n> to
+select the <n>-th file from such that list.
+</PRE>
+<P>
+<A NAME=.offset><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021400000000000000>  <b>Parameter OFFSET</b></A></H2>
+<P>
+<em>Prompt:</em> plot offset (data units)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Example:
+        If you enter 100, <data values>-100 will be plotted.
+</PRE>
+<P>
+<A NAME=.output.ngf.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021500000000000000>  <b>Parameter OUTPUT_NGF_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> Output 'node' name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+This is the file to which cuts will be copied.
+The source and output files MUST be different.
+</PRE>
+<P>
+  <PRE>
+Enter ** (or e.g. /user0/mydata/**) to get a list of files, enter #nn to select
+the nn-th file from such a list.
+</PRE>
+<P>
+<A NAME=.plot.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021600000000000000>  <b>Parameter PLOT_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> cut-data component<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the data component for the output cut:
+</PRE>
+<P>
+  <PRE>
+        COS     real part
+        SIN     imaginary part
+        AMPL    ABS(data)
+        PHASE   ARG(data)
+</PRE>
+<P>
+<A NAME=.poly.coef><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021700000000000000>  <b>Parameter POLY_COEF</b></A></H2>
+<P>
+<em>Prompt:</em> polynomial coefficients<BR><em>Expected input:</em> Real:  1 to 11 values
+<P>
+  <PRE>
+Specify the coefficients of the polynomial to be subtracted:
+</PRE>
+<P>
+  <PRE>
+        P= c0 +c1*HA +c2*(HA**2) +... +cN*(HA**N)
+</PRE>
+<P>
+<A NAME=.poly.n><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021800000000000000>  <b>Parameter POLY_N</b></A></H2>
+<P>
+<em>Prompt:</em> number of coefficients to fit<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify number of coefficients of the polynomial to be fitted to the data.
+</PRE>
+<P>
+  <PRE>
+For CALC=POLY, this is 1 + the polynomial's degree.
+</PRE>
+<P>
+  <PRE>
+For CALC=DPOLY it is the number of non-zero coefficients. You will be prompted
+later for there orders.
+</PRE>
+<P>
+<A NAME=.poly.use><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021900000000000000>  <b>Parameter POLY_USE</b></A></H2>
+<P>
+<em>Prompt:</em> orders of coefficients to fit<BR><em>Expected input:</em> Integer:  1 to 11 values
+<P>
+  <PRE>
+Specify the orders of the polynomial coefficients to fit to. Default is
+0,...,<N>, where <N> is the number you gave for POLY_N.
+</PRE>
+<P>
+  <PRE>
+Example:
+    To fit a 6th-degree even polynomial, specify POLY_N=3 and POLY_USE=0,2,4,6.
+</PRE>
+<P>
+<A NAME=.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022000000000000000>  <b>Parameter SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> plot scale (data units/mm)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the scale in units/mm.
+</PRE>
+<P>
+<A NAME=.sector.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022100000000000000>  <b>Parameter SECTOR_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> Sector-header action |<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify interaction with this sector header:
+</PRE>
+<P>
+  <PRE>
+   Show details of the sector header:
+        SHOW    show entire sector header
+        EDIT    edit fields (values) in the Sector header by name
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+        NEXT:   proceed to the header for the next sector selected
+        CONT:   descend into the scans of this sector
+        QUIT:   return to the file-header level
+</PRE>
+<P>
+<A NAME=.select.xyx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022200000000000000>  <b>Parameter SELECT_XYX</b></A></H2>
+<P>
+<em>Prompt:</em> polarisation(s)<BR><em>Expected input:</em> Character *4:  1 value
+<P>
+  <PRE>
+Select the polarisation(s) to be used. Your answer will be interpreted
+according to the data type you will select hereafter
+</PRE>
+<P>
+  <PRE>
+                Interferometer          Telescope
+                ==============          =========
+        XYX     XX, YX, YX and YY       X and Y
+        XY      XX and YY               X and Y
+        X       XX only                 X only
+        Y       YY only                 Y only
+        YX      XY and YX               none
+        YYX     YX                      none
+        XXY     XY                      none
+</PRE>
+<P>
+<A NAME=.shift><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022300000000000000>  <b>Parameter SHIFT</b></A></H2>
+<P>
+<em>Prompt:</em> l,m shifts to apply to data (arcsec)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the l,m shifts in arcsec to be applied to data
+</PRE>
+<P>
+<A NAME=.use.ngf.set><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022400000000000000>  <b>Parameter USE_NGF_SET</b></A></H2>
+<P>
+<em>Prompt:</em> Cut to use<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Define the cut represented by each of the variables of the form
+#<n> and ##<n> in your expression. You are being prompted for each such
+variable that is present in the expression. Your reply must designate ONE cut.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ngen/ngen__apply.html b/ngen/ngen__apply.html
new file mode 100644
index 0000000000000000000000000000000000000000..95b9b01c2d71fb9c68e94f552ef339be2c499b38
--- /dev/null
+++ b/ngen/ngen__apply.html
@@ -0,0 +1,58 @@
+<TITLE>Description of APPLY (NGEN)</TITLE>
+<H1>Description of general keyword APPLY</H1>
+
+<DT><EM>Prompt:</EM> Specify visibility corrections  ALL;NORED, NOALG, NOOTH;NOEXT, NOREF, NOIREF, NOFAR;NOCLK, NOPOL;NOIFR, NOMIFR;|-NONE;  RED,  ALG,  OTH;  EXT,  REF,  IREF,  FAR;  CLK,  POL;  IFR,  MIFR|
+<DT><EM>Default:</EM> * /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 16 values.<P>
+In general, the uv data in a .SCN file are not physically modified. Instead,  
+correction parameters are stored in the sector and scan headers of the .SCN 
+file, to be applied 'on-the-fly' to the visibilities as they are read into 
+memory to be processed. <P>
+You may specify here the corrections to be applied by specifying a combination 
+of possible options (separated by commas). The prefix 'NO' indicates that a 
+correction must not be applied and would most likely be used in combination of 
+ALL. <P>
+        ALL or *       apply all available corrections 
+        NONE or ""     apply no corrections 
+        [NO]RED        redundancy corrections (telescope gain, phase) 
+        [NO]ALG        align corrections (telescope gain, phase) 
+        [NO]OTH        other telesc. gain/phase corrns (i.e. from calibrator) 
+        [NO]EXT        extinction correction (elevation-dependent gain) 
+        [NO]REF        refraction correction (elevation-dependent phase) 
+        [NO]IREF       ionospheric refracion 
+        [NO]CLK        clock correction 
+        [NO]POL        polarisation corrections (dipole angle, ellipticity) 
+        [NO]FAR        Faraday rotation 
+        [NO]MIFR       multiplicative interferometer errors <P>
+NOTES: 
+   1. If two options are mutually exclusive, the one specified last prevails,  
+e.g. 
+        NONE, CLK, POL    selects only the CLK and POL corrections; 
+        CLK, POL, NONE    selects no corrections at all. <P>
+   2. If a certain correction is to be disabled permanently, the safest way is 
+to zero it in the .SCN file itself, using NCALIB option SET ZERO. <P>
+. 
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] <P>
+Note: use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/APPLY=value (or: 
+                ='(val1, val2, ...)') 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__datab.html b/ngen/ngen__datab.html
new file mode 100644
index 0000000000000000000000000000000000000000..d9ab2adaa5d55812dfc0947ed1610af879f32a3d
--- /dev/null
+++ b/ngen/ngen__datab.html
@@ -0,0 +1,47 @@
+<TITLE>Description of DATAB (NGEN)</TITLE>
+<H1>Description of general keyword DATAB</H1>
+
+<DT><EM>Prompt:</EM> default directory name
+<DT><EM>Default:</EM> "" /NOASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+Directory names can be very long. In order to avoid having to type them fully 
+each time, the user may store it in the keyword DATAB (the name has historic 
+roots). From then on, node names (in the same $stream) are automatically 
+preceded by the contents of DATAB. <P>
+NB: On Unix systems, the value of DATAB has to end with a slash (eg ./) <P>
+If you set DATAB to "*", the DATAB keyword will be ignored completely (it will 
+not be changed if you use a directory name in the specification of a set etc.) <P>
+NB: In general, however, it is recommended to keep all files of a reduction 
+project in a single directory. In that case, no explicit directory name will be 
+needed in any case, if you run from this directory. <P>
+Example: if node name is preceded by a directory name: 
+        ../../wnb/wsrt/data/myproject/mynode the value of DATAB (for the 
+current $stream) will be: 
+        ../../wnb/wsrt/data/myproject/ Subsequently, typing 'othernode' will 
+produce the node name: 
+        ../../wnb/wsrt/data/myproject/othernode NB: IF THE NEWSTAR PROGRAM 
+CANNOT FIND A FILE (NODE), WHILE IT IS CLEARLY PRESENT IN THE CURRENT 
+DIRECTORY, CHECK THE VALUE OF DATAB!! <P>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] <P>
+Note: use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/DATAB='"value"' 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__de_apply.html b/ngen/ngen__de_apply.html
new file mode 100644
index 0000000000000000000000000000000000000000..7d9d82d680e7488fe6ad4f12aa42dc620ae630a9
--- /dev/null
+++ b/ngen/ngen__de_apply.html
@@ -0,0 +1,67 @@
+<TITLE>Description of DE_APPLY (NGEN)</TITLE>
+<H1>Description of general keyword DE_APPLY</H1>
+
+<DT><EM>Prompt:</EM> Specify visibility de-corrections  ALL; NOOTH; NOEXT, NOREF, NOIREF, NOFAR; NOCLK, NOPOL; NOIFR, NOMIFR;|-NONE;   OTH;   EXT,  REF,   IREF,  FAR;   CLK,  POL; IFR,  MIFR;|-SHFT, NOSHFT, MOD, NOMOD|
+<DT><EM>Default:</EM> NONE /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 16 values.<P>
+In general, the visibilties in a .SCN file are not physically modified. 
+Instead, correction parameters are stored in the sector and scan headers of the 
+.SCN file, to be applied 'on-the-fly' to the visibilities as they are read into 
+memory to be processed. <P>
+It is also possible, however, to make corrections more permanent by applying 
+them to the visibilities as stored in the .SCN file. The pertinent correction 
+parameters are reset to 0 in this process and their values transferred into a 
+second set of correction parameters, the "applied" corrections. Thus, for each 
+correction parameter &lt;xxx&gt; there is an 'applied' counterpart A&lt;xxx&gt;. <P>
+Just like it is possible to apply corrections on-the-fly, it is also possible 
+to     'de-apply' the 'applied' corrections on-the-fly. You may specify here 
+which 'applied' corrections you want to de-apply in this way. <P>
+The prefix 'NO' indicates that a correction must not be applied and would most 
+likely be used in combination of ALL. <P>
+        ALL or *       apply all available corrections 
+        NONE or ""     apply no corrections 
+        [NO]RED        redundancy corrections (telescope gain, phase) 
+        [NO]ALG        align corrections (telescope gain, phase) 
+        [NO]OTH        other telesc. gain/phase corrns (i.e. from calibrator) 
+        [NO]EXT        extinction correction (elevation-dependent gain) 
+        [NO]REF        refraction correction (elevation-dependent phase) 
+        [NO]IREF       ionospheric refracion 
+        [NO]CLK        clock correction 
+        [NO]POL        polarisation corrections (dipole angle, ellipticity) 
+        [NO]FAR        Faraday rotation 
+        [NO]MIFR       multiplicative interferometer errors 
+        [NO]SHFT       shift of centre of observations 
+        [NO]MOD        subtract model <P>
+NOTES: 
+   1. If two options are mutually exclusive, the one specified last prevails,  
+e.g. 
+        NONE, CLK, POL    selects only the CLK and POL corrections; 
+        CLK, POL, NONE    selects no corrections at all. <P>
+   2. The only DE_APPLY correction type that is ever different from zero so far 
+is MODEL. This type controls the subtraction of a source model strored 
+internally in .SCN-file sector. <P>
+. 
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] <P>
+Note: use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/DE_AP=value (or: 
+                '(val1, val2, ...)') 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__delete_node.html b/ngen/ngen__delete_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..38a10e3e4a7baaa0a814b446ba783a01ec714872
--- /dev/null
+++ b/ngen/ngen__delete_node.html
@@ -0,0 +1,13 @@
+<TITLE>Description of DELETE_NODE (NGEN)</TITLE>
+<H1>Description of general keyword DELETE_NODE</H1>
+
+<DT><EM>Prompt:</EM> Delete node (YES/NO)?
+<DT><EM>Default:</EM> NO /ASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify the deletion of a node (YES) or not (NO) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__display.html b/ngen/ngen__display.html
new file mode 100644
index 0000000000000000000000000000000000000000..b8d553f73a656baebd6fd4773d492f27cbb5c41a
--- /dev/null
+++ b/ngen/ngen__display.html
@@ -0,0 +1,24 @@
+<TITLE>Description of DISPLAY (NGEN)</TITLE>
+<H1>Description of general keyword DISPLAY</H1>
+
+<DT><EM>Prompt:</EM> Output Display
+<DT><EM>Default:</EM> * /NOASK.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the X-Display on which to produce output. E.g. if you are working from 
+a workstation or Xterminal called e.g. rzmwx5 on another machine (maybe a fast 
+processor, say rzmvfp); you can get the NGIDS display on your local machine by 
+giving as answer: rzmwx5:0.0 <P>
+If you specify a wildcard (*) or an empty answer, the display will be taken 
+from the environment variable DISPLAY; if this environment variable does not 
+exist, the default :0.0 will be assumed. <P>
+If your display machine is your working machine, give :0.0 (the default). <P>
+Note: Before being able to use your local display you should enable it by 
+typing while logged in on your local machine (rzmwx5) either: 
+        xhost + or: 
+        xhost +rzmfvp <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__infix.html b/ngen/ngen__infix.html
new file mode 100644
index 0000000000000000000000000000000000000000..171ef12223a6d8d4afd20d6e23801dda4515b7cd
--- /dev/null
+++ b/ngen/ngen__infix.html
@@ -0,0 +1,40 @@
+<TITLE>Description of INFIX (NGEN)</TITLE>
+<H1>Description of general keyword INFIX</H1>
+
+<DT><EM>Prompt:</EM> node name shorthand
+<DT><EM>Default:</EM> "" /NOASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+NEWSTAR file names can be very long. In order to avoid having to type them 
+fully each time, the user may store (part of) the node name in the keyword 
+INFIX. From then on, the user may specify node names in a short-hand notation 
+which contains a hash (#) character. The latter is automatically replaced by 
+the contents of INFIX, to produce the full file name. <P>
+Example: if part of the full node name is enclosed in brackets: 
+        mynode.21(cm.yesterday.s.x.c.d.file.d)d the value of INFIX (for the 
+current $stream) will be: 
+        cm.yesterday.s.x.c.d.file.d Subsequently, typing '92#e' will produce 
+the node name: 
+        mynode.92cm.yesterday.s.x.c.d.file.de <P>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] <P>
+Note: use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/INFIX=value 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__log.html b/ngen/ngen__log.html
new file mode 100644
index 0000000000000000000000000000000000000000..d39265f077d44b23e5b6208f0ba72744d9328495
--- /dev/null
+++ b/ngen/ngen__log.html
@@ -0,0 +1,44 @@
+<TITLE>Description of LOG (NGEN)</TITLE>
+<H1>Description of general keyword LOG</H1>
+
+<DT><EM>Prompt:</EM> log-file disposition NO, YES, SPOOL, CATEN
+<DT><EM>Default:</EM> YES /NOASK.
+<DT><EM>Expected input:</EM> Character(8).<P>
+For each run of a NEWSTAR program, logging information may be put into a 
+LOG-file, for subsequent inspection (and clogging up your room). LOG-files are 
+named with the first three letters of the program name (e.g. NCA), followed by 
+yymmddhhmmssA.LOG in the current working directory. E.g. NCA940305163412A.LOG 
+The most recent LOG-file for a program has an alias name equal to the program,  
+and the extension .LOG (e.g. NCALIB.LOG). <P>
+The LOG-file contains the values for all the parameter (keywords) that were 
+used for this particualr program run, including the 'hidden' ones. It will also 
+contain information about the program run itself, and any results. <P>
+Specify what to do with the logging output: 
+        NO:     Make no LOG-file (not recommended) 
+        YES:    Make a LOG-file (preferred option, no line-printer output) 
+        SPOOL:  Print the LOG-file on the printer at the end of the program run 
+        CATEN:  Add the new info to the existing LOG-file for this program <P>
+. 
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. 
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] Note: 
+use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/LOG=value 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__memory.html b/ngen/ngen__memory.html
new file mode 100644
index 0000000000000000000000000000000000000000..d9b958d586b3db7fff8d372ceb89f82233a98cb6
--- /dev/null
+++ b/ngen/ngen__memory.html
@@ -0,0 +1,33 @@
+<TITLE>Description of MEMORY (NGEN)</TITLE>
+<H1>Description of general keyword MEMORY</H1>
+
+<DT><EM>Prompt:</EM> Specify memory units
+<DT><EM>Default:</EM> 100000 /NOASK.
+<DT><EM>Expected input:</EM> Integer number.<P>
+Specify the amount of memory to be used per buffer for some applications. These 
+applications could run faster in some instances by increasing (if a lot of 
+physical memory present) or lowering (if a lot of swapping) this Value. <P>
+. 
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. 
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] Note: 
+use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/MEM=value 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__modelb.html b/ngen/ngen__modelb.html
new file mode 100644
index 0000000000000000000000000000000000000000..80d0c42426ba49ed20f54cd3f4c5934ff81c4024
--- /dev/null
+++ b/ngen/ngen__modelb.html
@@ -0,0 +1,36 @@
+<TITLE>Description of MODELB (NGEN)</TITLE>
+<H1>Description of general keyword MODELB</H1>
+
+<DT><EM>Prompt:</EM> default directory for model files
+<DT><EM>Default:</EM> "" /NOASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+For calibrator sources one usually want to use a generic model, and it is good 
+practice to collect such models in a single directory. <P>
+Newstar programs look for a calibrator model first in your 'preferred' 
+directory, then in the directory defined by MODELB, and finally in the 
+directory defined by the Unix environmant variable MODELB. The latter points to 
+the standard WSRT calibrator models that are part of Newstar. <P>
+NOTE: On Unix systems, the value of MODELB has to end with a slash (eg ./) <P>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] <P>
+Note: use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/MODELB='"value"' 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__pecify] ngen['$stream'].html b/ngen/ngen__pecify] ngen['$stream'].html
new file mode 100644
index 0000000000000000000000000000000000000000..81223e3027b60d70972f9eae6a2389593406214f
--- /dev/null
+++ b/ngen/ngen__pecify] ngen['$stream'].html	
@@ -0,0 +1,12 @@
+<TITLE>Description of pecify] NGEN['$stream'] (NGEN)</TITLE>
+<H1>Description of general keyword pecify] NGEN['$stream']</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__run.html b/ngen/ngen__run.html
new file mode 100644
index 0000000000000000000000000000000000000000..a035c8fe449ec975ae2125b3ca2d095b2188b74c
--- /dev/null
+++ b/ngen/ngen__run.html
@@ -0,0 +1,41 @@
+<TITLE>Description of RUN (NGEN)</TITLE>
+<H1>Description of general keyword RUN</H1>
+
+<DT><EM>Prompt:</EM> Exectute program after parameter setup (YES/NO)?
+<DT><EM>Default:</EM> YES /NOASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify the run mode of the NEWSTAR program: 
+        YES:   The NEWSTAR program will run normally 
+        NO:    The NEWSTAR program will prompt the user for all parameters 
+(keywords), but will then terminate. This mode should be used in conjunction 
+with the '/save' option, in which all the specified keyword values will be 
+saved in a .SAV file for later use (e.g. batch processing). <P>
+The /save option is invoked by starting the program in the following way: 
+        dwe 'program'[$'stream']/save (e.g. dwe ncalib$3/save). The saved 
+keyword values are used by running the program again: 
+        dwe 'program'[$'stream'] (e.g. dwe ncalib$3) <P>
+NB: An alternative approach is to use the '/norun' option: 
+        dwe 'program'[$'stream']/norun (e.g. dwe ncalib'$3'/norun) <P>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] <P>
+Note: use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/ASK=value 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__s during current login:.html b/ngen/ngen__s during current login:.html
new file mode 100644
index 0000000000000000000000000000000000000000..1bb25ad9f92148342519326e4c63f8c18bf5a753
--- /dev/null
+++ b/ngen/ngen__s during current login:.html	
@@ -0,0 +1,12 @@
+<TITLE>Description of s during current login: (NGEN)</TITLE>
+<H1>Description of general keyword s during current login:</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__uflag.html b/ngen/ngen__uflag.html
new file mode 100644
index 0000000000000000000000000000000000000000..31dae6a16cc8bd725333841f3e5e2d5bf6eaf3a1
--- /dev/null
+++ b/ngen/ngen__uflag.html
@@ -0,0 +1,53 @@
+<TITLE>Description of UFLAG (NGEN)</TITLE>
+<H1>Description of general keyword UFLAG</H1>
+
+<DT><EM>Prompt:</EM> Specify which flags you want to ignore | NONE, ALL; MAN, OLD, CLIP, NOIS, ADD, SHAD; U1, U2, U3|
+<DT><EM>Default:</EM> NONE /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 16 values.<P>
+Scan headers and data in a .SCN file can be flagged as invalid. There are 8 
+different flags distinguishing 8 different types of reasons for the flagging. 
+Flags can be set in a variety of ways, mostly through various options in NFLAG,  
+or by manual flagging in NGIDS. <P>
+By default, data points that have any one of the 8 flags set will be discarded. 
+You are given here the option to ignore specific types of flag, i.e. accept 
+data as valid even they have flags of these types set. You may give any 
+combination of options, separated by commas. <P>
+        NONE or ""     ignore none of the flags, i.e. discard all flagged data 
+        ALL or *       ignore all flags, i.e. accept all data 
+        MAN            ignore MANUAL flags 
+        CLIP           ignore CLIP flags 
+        NOIS           ignore NOISE flags 
+        SHAD           ignore SHADOW flags 
+        ADD            ignore ADDITIVE flags 
+        U1             ignore USER1 flags 
+        U2             ignore USER2 flags 
+        U3             ignore USER3 flags NOTES: 
+   1. If two options are mutually exclusive, the one specified last prevails,  
+e.g. 
+        NONE, CLIP, MAN   ignores the CLIP and MAN flags; 
+        CLIP, MAN, NONE   iognores none of the flags. <P>
+. 
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which 
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is 
+'hidden', i.e. the user is not prompted for it, but the default value is used. <P>
+Its value may be modified (for a given $stream) in several ways: 
+        Permanently for all programs and streams during current login: 
+                change the default value: dws[pecify] 'NGEN$0' 
+        Permanently for all programs in certain stream during current login: 
+                change the default value: dws[pecify] NGEN['$stream'] 
+        Permanently for certain program in all streams during current login: 
+                change the default value: dws[pecify] 'program$0' 
+        Permanently for certain program in certain stream during current login: 
+                change the default value: dws[pecify] program['$stream'] .Note: 
+use automatic saving in LOGOUT to pass on values beyond current login 
+        Incidentally for a certain incarnation of program[$stream]: 
+                run as: dwe program['$stream']/UFL=value (or: 
+                '(val1, val2, ...)') 
+        Incidentally for all hidden values: 
+                run a NEWSTAR program as: dwe program['$stream']/ASK <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_apply.html b/ngen/ngen__x_apply.html
new file mode 100644
index 0000000000000000000000000000000000000000..a1d28da483a27a55e37a8e2bfe89f70961428f6d
--- /dev/null
+++ b/ngen/ngen__x_apply.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_APPLY (NGEN)</TITLE>
+<H1>Description of general keyword X_APPLY</H1>
+
+<DT><EM>Prompt:</EM> |  ALL;NORED, NOALG, NOOTH;NOEXT, NOREF, NOIREF, NOFAR;NOCLK, NOPOL;NOIFR, NOMIFR;|-NONE;  RED,  ALG,  OTH;  EXT,  REF,  IREF,  FAR;  CLK,  POL;  IFR,  MIFR|
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 16 values.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_datab.html b/ngen/ngen__x_datab.html
new file mode 100644
index 0000000000000000000000000000000000000000..3709b0bc5b5c862c1cc8f2969fff17f0f9ab4ef4
--- /dev/null
+++ b/ngen/ngen__x_datab.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_DATAB (NGEN)</TITLE>
+<H1>Description of general keyword X_DATAB</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_de_apply.html b/ngen/ngen__x_de_apply.html
new file mode 100644
index 0000000000000000000000000000000000000000..6ce2d843c24a1798f5db45717ad1ed8da2f0aabc
--- /dev/null
+++ b/ngen/ngen__x_de_apply.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_DE_APPLY (NGEN)</TITLE>
+<H1>Description of general keyword X_DE_APPLY</H1>
+
+<DT><EM>Prompt:</EM> |  ALL; NOOTH; NOEXT, NOREF, NOIREF, NOFAR; NOCLK, NOPOL; NOIFR, NOMIFR;|-NONE;   OTH;   EXT,  REF,   IREF,  FAR;   CLK,  POL;   IFR,  MIFR;|-SHFT, NOSHFT, MOD, NOMOD|
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 16 values.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_infix.html b/ngen/ngen__x_infix.html
new file mode 100644
index 0000000000000000000000000000000000000000..7b3babbdb359290b92178ba8f641ca5e41bf342f
--- /dev/null
+++ b/ngen/ngen__x_infix.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_INFIX (NGEN)</TITLE>
+<H1>Description of general keyword X_INFIX</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_log.html b/ngen/ngen__x_log.html
new file mode 100644
index 0000000000000000000000000000000000000000..0bd3e26aec81790d20afaceee92556d2a005f88c
--- /dev/null
+++ b/ngen/ngen__x_log.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_LOG (NGEN)</TITLE>
+<H1>Description of general keyword X_LOG</H1>
+
+<DT><EM>Prompt:</EM> SPOOL, YES, NO, CATEN
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(8).<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_memory.html b/ngen/ngen__x_memory.html
new file mode 100644
index 0000000000000000000000000000000000000000..433b06b6369e1819bc143c8ee499f947ecbbfeb0
--- /dev/null
+++ b/ngen/ngen__x_memory.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_MEMORY (NGEN)</TITLE>
+<H1>Description of general keyword X_MEMORY</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Integer number.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_modelb.html b/ngen/ngen__x_modelb.html
new file mode 100644
index 0000000000000000000000000000000000000000..87fa839077d28325d5a258d2a0ab5cbaefed30d8
--- /dev/null
+++ b/ngen/ngen__x_modelb.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_MODELB (NGEN)</TITLE>
+<H1>Description of general keyword X_MODELB</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_run.html b/ngen/ngen__x_run.html
new file mode 100644
index 0000000000000000000000000000000000000000..588ac89fd22a67a0b2b1b0b5290417e7676e1770
--- /dev/null
+++ b/ngen/ngen__x_run.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_RUN (NGEN)</TITLE>
+<H1>Description of general keyword X_RUN</H1>
+
+<DT><EM>Prompt:</EM> 
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen/ngen__x_uflag.html b/ngen/ngen__x_uflag.html
new file mode 100644
index 0000000000000000000000000000000000000000..62f7db566962f386c43e52b404e9b3a22f2e505b
--- /dev/null
+++ b/ngen/ngen__x_uflag.html
@@ -0,0 +1,12 @@
+<TITLE>Description of X_UFLAG (NGEN)</TITLE>
+<H1>Description of general keyword X_UFLAG</H1>
+
+<DT><EM>Prompt:</EM> | NONE, ALL; MAN, OLD, CLIP, NOIS, ADD, SHAD; U1, U2, U3
+<DT><EM>Default:</EM> # /NOASK.
+<DT><EM>Expected input:</EM> Character(8), 16 values.<P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngen/ngen_comm.html">List of general keywords</A> for NGEN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngen_comm/ngen_comm.html b/ngen_comm/ngen_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..75757c155a6ccfb87ded068e197146008c422e67
--- /dev/null
+++ b/ngen_comm/ngen_comm.html
@@ -0,0 +1,71 @@
+<TITLE>Index of general keywords from NGEN</TITLE>
+<H1>Description of general keywords (NGEN)</H1>
+
+<UL>
+<LI> <A HREF="../ngen/ngen__x_log.html">
+  X_LOG</A>
+  SPOOL, YES, NO, CATEN
+<LI> <A HREF="../ngen/ngen__log.html">
+  LOG</A>
+  log-file disposition NO, YES, SPOOL, CATEN
+<LI> <A HREF="../ngen/ngen__x_run.html">
+  X_RUN</A>
+  
+<LI> <A HREF="../ngen/ngen__run.html">
+  RUN</A>
+  Exectute program after parameter setup (YES/NO)?
+<LI> <A HREF="../ngen/ngen__x_datab.html">
+  X_DATAB</A>
+  
+<LI> <A HREF="../ngen/ngen__datab.html">
+  DATAB</A>
+  default directory name
+<LI> <A HREF="../ngen/ngen__x_modelb.html">
+  X_MODELB</A>
+  
+<LI> <A HREF="../ngen/ngen__modelb.html">
+  MODELB</A>
+  default directory for model files
+<LI> <A HREF="../ngen/ngen__x_infix.html">
+  X_INFIX</A>
+  
+<LI> <A HREF="../ngen/ngen__infix.html">
+  INFIX</A>
+  node name shorthand
+<LI> <A HREF="../ngen/ngen__x_apply.html">
+  X_APPLY</A>
+  |  ALL;NORED, NOALG, NOOTH;NOEXT, NOREF, NOIREF, NOFAR;NOCLK, NOPOL;NOIFR, NOMIFR;|-NONE;  RED,  ALG,  OTH;  EXT,  REF,  IREF,  FAR;  CLK,  POL;  IFR,  MIFR|
+<LI> <A HREF="../ngen/ngen__apply.html">
+  APPLY</A>
+  Specify visibility corrections  ALL;NORED, NOALG, NOOTH;NOEXT, NOREF, NOIREF, NOFAR;NOCLK, NOPOL;NOIFR, NOMIFR;|-NONE;  RED,  ALG,  OTH;  EXT,  REF,  IREF,  FAR;  CLK,  POL;  IFR,  MIFR|
+<LI> <A HREF="../ngen/ngen__x_de_apply.html">
+  X_DE_APPLY</A>
+  |  ALL; NOOTH; NOEXT, NOREF, NOIREF, NOFAR; NOCLK, NOPOL; NOIFR, NOMIFR;|-NONE;   OTH;   EXT,  REF,   IREF,  FAR;   CLK,  POL;   IFR,  MIFR;|-SHFT, NOSHFT, MOD, NOMOD|
+<LI> <A HREF="../ngen/ngen__de_apply.html">
+  DE_APPLY</A>
+  Specify visibility de-corrections  ALL; NOOTH; NOEXT, NOREF, NOIREF, NOFAR; NOCLK, NOPOL; NOIFR, NOMIFR;|-NONE;   OTH;   EXT,  REF,   IREF,  FAR;   CLK,  POL; IFR,  MIFR;|-SHFT, NOSHFT, MOD, NOMOD|
+<LI> <A HREF="../ngen/ngen__x_uflag.html">
+  X_UFLAG</A>
+  | NONE, ALL; MAN, OLD, CLIP, NOIS, ADD, SHAD; U1, U2, U3
+<LI> <A HREF="../ngen/ngen__uflag.html">
+  UFLAG</A>
+  Specify which flags you want to ignore | NONE, ALL; MAN, OLD, CLIP, NOIS, ADD, SHAD; U1, U2, U3|
+<LI> <A HREF="../ngen/ngen__delete_node.html">
+  DELETE_NODE</A>
+  Delete node (YES/NO)?
+<LI> <A HREF="../ngen/ngen__x_memory.html">
+  X_MEMORY</A>
+  
+<LI> <A HREF="../ngen/ngen__memory.html">
+  MEMORY</A>
+  Specify memory units
+<LI> <A HREF="../ngen/ngen__display.html">
+  DISPLAY</A>
+  Output Display
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
diff --git a/ngen_keys/ngen_keys.html b/ngen_keys/ngen_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..8297d2088870645346f01390c2b7482bd547c5a4
--- /dev/null
+++ b/ngen_keys/ngen_keys.html
@@ -0,0 +1,15 @@
+<TITLE>Index of private keywords for NGEN </TITLE>
+<H1>Description of keywords for program NGEN</H1>
+
+<UL>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../ngen_descr/ngen_descr.html">program NGEN</A>
+</UL>
diff --git a/ngen_private_intfc.ps b/ngen_private_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..b9e91053ca6f92596a9924f92baaa49cbee02261
--- /dev/null
+++ b/ngen_private_intfc.ps
@@ -0,0 +1,329 @@
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+%%Title: ngen_private_intfc_tmp.dvi
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+b(v)n(alue)0 469 y Fb(2.19)74 b(P)n(arameter)18 b(X)p
+495 469 V 20 w(MODELB)0 571 y Fg(Exp)n(e)n(cte)n(d)d(input:)k
+Fd(Character)c(*80:)i(1)d(v)n(alue)0 724 y Fb(2.20)74
+b(P)n(arameter)18 b(X)p 495 724 V 20 w(R)n(UN)0 826 y
+Fg(Exp)n(e)n(cte)n(d)d(input:)k Fd(Y)m(es/No:)f(1)c(v)n(alue)0
+979 y Fb(2.21)74 b(P)n(arameter)18 b(X)p 495 979 V 20
+w(UFLA)n(G)935 2995 y Fd(9)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/ngen_public_intfc/images.pl b/ngen_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ngen_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ngen_public_intfc/labels.pl b/ngen_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..412f4e13a555444cf0c54aee6506b9bb39291007
--- /dev/null
+++ b/ngen_public_intfc/labels.pl
@@ -0,0 +1,28 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".modelb"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".delete.node"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".public"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.uflag"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.de.apply"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".display"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".apply"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.infix"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.memory"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.apply"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.run"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".run"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".datab"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".infix"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.log"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.datab"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".de.apply"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".x.modelb"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".memory"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".uflag"} ="$URL/ngen_public_intfc.html"; 
+$external_labels{".log"} ="$URL/ngen_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/ngen_public_intfc/ngen_public_intfc.html b/ngen_public_intfc/ngen_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..e4887d34dabc21730a3dbda57de280dc2e2a4fac
--- /dev/null
+++ b/ngen_public_intfc/ngen_public_intfc.html
@@ -0,0 +1,690 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group NGEN</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ngen_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ngen_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ngen_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ngen_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=ngen_public_intfc.html#SECTION0003200000000000000>  <b>Parameter APPLY</b></A>
+<LI> <A NAME=tex2html6 HREF=ngen_public_intfc.html#SECTION0003300000000000000>  <b>Parameter DATAB</b></A>
+<LI> <A NAME=tex2html7 HREF=ngen_public_intfc.html#SECTION0003400000000000000>  <b>Parameter DELETE_NODE</b></A>
+<LI> <A NAME=tex2html8 HREF=ngen_public_intfc.html#SECTION0003500000000000000>  <b>Parameter DE_APPLY</b></A>
+<LI> <A NAME=tex2html9 HREF=ngen_public_intfc.html#SECTION0003600000000000000>  <b>Parameter DISPLAY</b></A>
+<LI> <A NAME=tex2html10 HREF=ngen_public_intfc.html#SECTION0003700000000000000>  <b>Parameter INFIX</b></A>
+<LI> <A NAME=tex2html11 HREF=ngen_public_intfc.html#SECTION0003800000000000000>  <b>Parameter LOG</b></A>
+<LI> <A NAME=tex2html12 HREF=ngen_public_intfc.html#SECTION0003900000000000000>  <b>Parameter MEMORY</b></A>
+<LI> <A NAME=tex2html13 HREF=ngen_public_intfc.html#SECTION00031000000000000000>  <b>Parameter MODELB</b></A>
+<LI> <A NAME=tex2html14 HREF=ngen_public_intfc.html#SECTION00031100000000000000>  <b>Parameter RUN</b></A>
+<LI> <A NAME=tex2html15 HREF=ngen_public_intfc.html#SECTION00031200000000000000>  <b>Parameter UFLAG</b></A>
+<LI> <A NAME=tex2html16 HREF=ngen_public_intfc.html#SECTION00031300000000000000>  <b>Parameter X_APPLY</b></A>
+<LI> <A NAME=tex2html17 HREF=ngen_public_intfc.html#SECTION00031400000000000000>  <b>Parameter X_DATAB</b></A>
+<LI> <A NAME=tex2html18 HREF=ngen_public_intfc.html#SECTION00031500000000000000>  <b>Parameter X_DE_APPLY</b></A>
+<LI> <A NAME=tex2html19 HREF=ngen_public_intfc.html#SECTION00031600000000000000>  <b>Parameter X_INFIX</b></A>
+<LI> <A NAME=tex2html20 HREF=ngen_public_intfc.html#SECTION00031700000000000000>  <b>Parameter X_LOG</b></A>
+<LI> <A NAME=tex2html21 HREF=ngen_public_intfc.html#SECTION00031800000000000000>  <b>Parameter X_MEMORY</b></A>
+<LI> <A NAME=tex2html22 HREF=ngen_public_intfc.html#SECTION00031900000000000000>  <b>Parameter X_MODELB</b></A>
+<LI> <A NAME=tex2html23 HREF=ngen_public_intfc.html#SECTION00032000000000000000>  <b>Parameter X_RUN</b></A>
+<LI> <A NAME=tex2html24 HREF=ngen_public_intfc.html#SECTION00032100000000000000>  <b>Parameter X_UFLAG</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group NGEN, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter APPLY</b></A></H2>
+<P>
+  <em>Prompt:</em> Specify visibility corrections (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 to 16 values
+<P>
+    <PRE>
+In general, the uv data in a .SCN file are not physically modified. Instead,
+correction parameters are stored in the sector and scan headers of the .SCN
+file, to be applied 'on-the-fly' to the visibilities as they are read into
+memory to be processed.
+</PRE>
+<P>
+  <PRE>
+You may specify here the corrections to be applied by specifying a combination
+of possible options (separated by commas). The prefix 'NO' indicates that a
+correction must not be applied and would most likely be used in combination of
+ALL.
+</PRE>
+<P>
+  <PRE>
+        ALL or *       apply all available corrections
+        NONE or ""     apply no corrections
+        [NO]RED        redundancy corrections (telescope gain,phase)
+        [NO]ALG        align corrections (telescope gain,phase)
+        [NO]OTH        other telesc. gain/phase corrns (i.e. from calibrator)
+        [NO]EXT        extinction correction (elevation-dependent gain)
+        [NO]REF        refraction correction (elevation-dependent phase)
+        [NO]IREF       ionospheric refracion
+        [NO]CLK        clock correction
+        [NO]POL        polarisation corrections (dipole angle, ellipticity)
+        [NO]FAR        Faraday rotation
+        [NO]MIFR       multiplicative interferometer errors
+</PRE>
+<P>
+  <PRE>
+NOTES:
+   1. If two options are mutually exclusive, the one specified last prevails,
+e.g.
+        NONE,CLK,POL    selects only the CLK and POL corrections;
+        CLK,POL,NONE    selects no corrections at all.
+</PRE>
+<P>
+  <PRE>
+   2. If a certain correction is to be disabled permanently, the safest way is
+to zero it in the .SCN file itself, using NCALIB option SET ZERO.
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream']
+</PRE>
+<P>
+  <PRE>
+Note: use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/APPLY=value (or:
+                ='(val1,val2,...)')
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.datab><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter DATAB</b></A></H2>
+<P>
+<em>Prompt:</em> default directory name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Directory names can be very long. In order to avoid having to type them fully
+each time, the user may store it in the keyword DATAB (the name has historic
+roots). From then on, node names (in the same $stream) are automatically
+preceded by the contents of DATAB.
+</PRE>
+<P>
+  <PRE>
+NB: On Unix systems, the value of DATAB has to end with a slash (eg ./)
+</PRE>
+<P>
+  <PRE>
+If you set DATAB to "*", the DATAB keyword will be ignored completely (it will
+not be changed if you use a directory name in the specification of a set etc.)
+</PRE>
+<P>
+  <PRE>
+NB: In general, however, it is recommended to keep all files of a reduction
+project in a single directory. In that case, no explicit directory name will be
+needed in any case, if you run from this directory.
+</PRE>
+<P>
+  <PRE>
+Example: if node name is preceded by a directory name:
+        ../../wnb/wsrt/data/myproject/mynode the value of DATAB (for the
+current $stream) will be:
+        ../../wnb/wsrt/data/myproject/ Subsequently, typing 'othernode' will
+produce the node name:
+        ../../wnb/wsrt/data/myproject/othernode NB: IF THE NEWSTAR PROGRAM
+CANNOT FIND A FILE (NODE), WHILE IT IS CLEARLY PRESENT IN THE CURRENT
+DIRECTORY, CHECK THE VALUE OF DATAB!
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream']
+</PRE>
+<P>
+  <PRE>
+Note: use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/DATAB='"value"'
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.delete.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter DELETE_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> Delete node (YES/NO)? (<em>may vary per application</em>)<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify the deletion of a node (YES) or not (NO)
+</PRE>
+<P>
+<A NAME=.de.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter DE_APPLY</b></A></H2>
+<P>
+<em>Prompt:</em> Specify visibility de-corrections (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 to 16 values
+<P>
+  <PRE>
+In general, the visibilties in a .SCN file are not physically modified.
+Instead, correction parameters are stored in the sector and scan headers of the
+</PRE>
+<P>
+  <PRE>
+memory to be processed.
+</PRE>
+<P>
+  <PRE>
+It is also possible, however, to make corrections more permanent by applying
+them to the visibilities as stored in the .SCN file. The pertinent correction
+parameters are reset to 0 in this process and their values transferred into a
+second set of correction parameters, the "applied" corrections. Thus, for each
+correction parameter <xxx> there is an 'applied' counterpart A<xxx>.
+</PRE>
+<P>
+  <PRE>
+Just like it is possible to apply corrections on-the-fly, it is also possible
+to     'de-apply' the 'applied' corrections on-the-fly. You may specify here
+which 'applied' corrections you want to de-apply in this way.
+</PRE>
+<P>
+  <PRE>
+The prefix 'NO' indicates that a correction must not be applied and would most
+likely be used in combination of ALL.
+</PRE>
+<P>
+  <PRE>
+        ALL or *       apply all available corrections
+        NONE or ""     apply no corrections
+        [NO]RED        redundancy corrections (telescope gain,phase)
+        [NO]ALG        align corrections (telescope gain,phase)
+        [NO]OTH        other telesc. gain/phase corrns (i.e. from calibrator)
+        [NO]EXT        extinction correction (elevation-dependent gain)
+        [NO]REF        refraction correction (elevation-dependent phase)
+        [NO]IREF       ionospheric refracion
+        [NO]CLK        clock correction
+        [NO]POL        polarisation corrections (dipole angle, ellipticity)
+        [NO]FAR        Faraday rotation
+        [NO]MIFR       multiplicative interferometer errors
+        [NO]SHFT       shift of centre of observations
+        [NO]MOD        subtract model
+</PRE>
+<P>
+  <PRE>
+NOTES:
+   1. If two options are mutually exclusive, the one specified last prevails,
+e.g.
+        NONE,CLK,POL    selects only the CLK and POL corrections;
+        CLK,POL,NONE    selects no corrections at all.
+</PRE>
+<P>
+  <PRE>
+   2. The only DE_APPLY correction type that is ever different from zero so far
+is MODEL. This type controls the subtraction of a source model strored
+internally in .SCN-file sector.
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream']
+</PRE>
+<P>
+  <PRE>
+Note: use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/DE_AP=value (or:
+                '(val1,val2,...)')
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.display><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter DISPLAY</b></A></H2>
+<P>
+<em>Prompt:</em> Output Display (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the X-Display on which to produce output. E.g. if you are working from
+a workstation or Xterminal called e.g. rzmwx5 on another machine (maybe a fast
+processor, say rzmvfp); you can get the NGIDS display on your local machine by
+giving as answer: rzmwx5:0.0
+</PRE>
+<P>
+  <PRE>
+If you specify a wildcard (*) or an empty answer, the display will be taken
+from the environment variable DISPLAY; if this environment variable does not
+exist, the default :0.0 will be assumed.
+</PRE>
+<P>
+  <PRE>
+If your display machine is your working machine, give :0.0 (the default).
+</PRE>
+<P>
+  <PRE>
+Note: Before being able to use your local display you should enable it by
+typing while logged in on your local machine (rzmwx5) either:
+        xhost + or:
+        xhost +rzmfvp
+</PRE>
+<P>
+<A NAME=.infix><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter INFIX</b></A></H2>
+<P>
+<em>Prompt:</em> node name shorthand (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+NEWSTAR file names can be very long. In order to avoid having to type them
+fully each time, the user may store (part of) the node name in the keyword
+INFIX. From then on, the user may specify node names in a short-hand notation
+which contains a hash (#) character. The latter is automatically replaced by
+the contents of INFIX, to produce the full file name.
+</PRE>
+<P>
+  <PRE>
+Example: if part of the full node name is enclosed in brackets:
+        mynode.21(cm.yesterday.s.x.c.d.file.d)d the value of INFIX (for the
+current $stream) will be:
+        cm.yesterday.s.x.c.d.file.d Subsequently, typing '92#e' will produce
+the node name:
+        mynode.92cm.yesterday.s.x.c.d.file.de
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream']
+</PRE>
+<P>
+  <PRE>
+Note: use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/INFIX=value
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.log><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter LOG</b></A></H2>
+<P>
+<em>Prompt:</em> log-file disposition (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+For each run of a NEWSTAR program, logging information may be put into a
+LOG-file, for subsequent inspection (and clogging up your room). LOG-files are
+named with the first three letters of the program name (e.g. NCA), followed by
+yymmddhhmmssA.LOG in the current working directory. E.g. NCA940305163412A.LOG
+The most recent LOG-file for a program has an alias name equal to the program,
+and the extension .LOG (e.g. NCALIB.LOG).
+</PRE>
+<P>
+  <PRE>
+The LOG-file contains the values for all the parameter (keywords) that were
+used for this particualr program run, including the 'hidden' ones. It will also
+contain information about the program run itself, and any results.
+</PRE>
+<P>
+  <PRE>
+Specify what to do with the logging output:
+        NO:     Make no LOG-file (not recommended)
+        YES:    Make a LOG-file (preferred option, no line-printer output)
+        SPOOL:  Print the LOG-file on the printer at the end of the program run
+        CATEN:  Add the new info to the existing LOG-file for this program
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream'] Note:
+use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/LOG=value
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.memory><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter MEMORY</b></A></H2>
+<P>
+<em>Prompt:</em> Specify memory units (<em>may vary per application</em>)<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the amount of memory to be used per buffer for some applications. These
+applications could run faster in some instances by increasing (if a lot of
+physical memory present) or lowering (if a lot of swapping) this Value.
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream'] Note:
+use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/MEM=value
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.modelb><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter MODELB</b></A></H2>
+<P>
+<em>Prompt:</em> default directory for model files (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+For calibrator sources one usually want to use a generic model, and it is good
+practice to collect such models in a single directory.
+</PRE>
+<P>
+  <PRE>
+Newstar programs look for a calibrator model first in your 'preferred'
+directory, then in the directory defined by MODELB, and finally in the
+directory defined by the Unix environmant variable MODELB. The latter points to
+the standard WSRT calibrator models that are part of Newstar.
+NOTE: On Unix systems, the value of MODELB has to end with a slash (eg ./)
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream']
+</PRE>
+<P>
+  <PRE>
+Note: use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/MODELB='"value"'
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.run><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter RUN</b></A></H2>
+<P>
+<em>Prompt:</em> Exectute program after parameter setup (YES/NO)? (<em>may vary per application</em>)<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify the run mode of the NEWSTAR program:
+        YES:   The NEWSTAR program will run normally
+        NO:    The NEWSTAR program will prompt the user for all parameters
+(keywords), but will then terminate. This mode should be used in conjunction
+with the '/save' option, in which all the specified keyword values will be
+saved in a .SAV file for later use (e.g. batch processing).
+</PRE>
+<P>
+  <PRE>
+The /save option is invoked by starting the program in the following way:
+        dwe 'program'[$'stream']/save (e.g. dwe ncalib$3/save). The saved
+keyword values are used by running the program again:
+        dwe 'program'[$'stream'] (e.g. dwe ncalib$3)
+</PRE>
+<P>
+  <PRE>
+NB: An alternative approach is to use the '/norun' option:
+        dwe 'program'[$'stream']/norun (e.g. dwe ncalib'$3'/norun)
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream']
+</PRE>
+<P>
+  <PRE>
+Note: use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/ASK=value
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.uflag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter UFLAG</b></A></H2>
+<P>
+<em>Prompt:</em> Specify which flags you want to ignore | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 to 16 values
+<P>
+  <PRE>
+Scan headers and data in a .SCN file can be flagged as invalid. There are 8
+different flags distinguishing 8 different types of reasons for the flagging.
+Flags can be set in a variety of ways, mostly through various options in NFLAG,
+or by manual flagging in NGIDS.
+</PRE>
+<P>
+  <PRE>
+By default, data points that have any one of the 8 flags set will be discarded.
+You are given here the option to ignore specific types of flag, i.e. accept
+data as valid even they have flags of these types set. You may give any
+combination of options, separated by commas.
+</PRE>
+<P>
+  <PRE>
+        NONE or ""     ignore none of the flags, i.e. discard all flagged data
+        ALL or *       ignore all flags, i.e. accept all data
+        MAN            ignore MANUAL flags
+        CLIP           ignore CLIP flags
+        NOIS           ignore NOISE flags
+        SHAD           ignore SHADOW flags
+        ADD            ignore ADDITIVE flags
+        U1             ignore USER1 flags
+        U2             ignore USER2 flags
+        U3             ignore USER3 flags NOTES:
+   1. If two options are mutually exclusive, the one specified last prevails,
+e.g.
+        NONE,CLIP,MAN   ignores the CLIP and MAN flags;
+        CLIP,MAN,NONE   iognores none of the flags.
+</PRE>
+<P>
+  <PRE>
+This keyword is part of NGEN, i.e. it is a NEWSTAR 'environment keyword', which
+is available to all NEWSTAR programs. The switch /NOASK indicates that it is
+'hidden', i.e. the user is not prompted for it, but the default value is used.
+</PRE>
+<P>
+  <PRE>
+Its value may be modified (for a given $stream) in several ways:
+        Permanently for all programs and streams during current login:
+                change the default value: dws[pecify] 'NGEN$0'
+        Permanently for all programs in certain stream during current login:
+                change the default value: dws[pecify] NGEN['$stream']
+        Permanently for certain program in all streams during current login:
+                change the default value: dws[pecify] 'program$0'
+        Permanently for certain program in certain stream during current login:
+                change the default value: dws[pecify] program['$stream'] .Note:
+use automatic saving in LOGOUT to pass on values beyond current login
+        Incidentally for a certain incarnation of program[$stream]:
+                run as: dwe program['$stream']/UFL=value (or:
+                '(val1,val2,...)')
+        Incidentally for all hidden values:
+                run a NEWSTAR program as: dwe program['$stream']/ASK
+</PRE>
+<P>
+<A NAME=.x.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter X_APPLY</b></A></H2>
+<P>
+<em>Prompt:</em> | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 to 16 values
+<P>
+<A NAME=.x.datab><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter X_DATAB</b></A></H2>
+<P>
+<em>Expected input:</em> Character *80:  1 value
+<P>
+<A NAME=.x.de.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter X_DE_APPLY</b></A></H2>
+<P>
+<em>Prompt:</em> | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 to 16 values
+<P>
+<A NAME=.x.infix><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter X_INFIX</b></A></H2>
+<P>
+<em>Expected input:</em> Character *80:  1 value
+<P>
+<A NAME=.x.log><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter X_LOG</b></A></H2>
+<P>
+<em>Expected input:</em> Character *8:  1 value
+<P>
+<A NAME=.x.memory><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter X_MEMORY</b></A></H2>
+<P>
+<em>Expected input:</em> Integer:  1 value
+<P>
+<A NAME=.x.modelb><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031900000000000000>  <b>Parameter X_MODELB</b></A></H2>
+<P>
+<em>Expected input:</em> Character *80:  1 value
+<P>
+<A NAME=.x.run><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032000000000000000>  <b>Parameter X_RUN</b></A></H2>
+<P>
+<em>Expected input:</em> Yes/No:  1 value
+<P>
+<A NAME=.x.uflag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032100000000000000>  <b>Parameter X_UFLAG</b></A></H2>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ngfsets/ngfsets__ngf_sets.html b/ngfsets/ngfsets__ngf_sets.html
new file mode 100644
index 0000000000000000000000000000000000000000..c1bc667552ea146555a075e941c495d6b1ab3da3
--- /dev/null
+++ b/ngfsets/ngfsets__ngf_sets.html
@@ -0,0 +1,54 @@
+<TITLE>Description of NGF_SETS (NGFSETS)</TITLE>
+<H1>Description of general keyword NGF_SETS</H1>
+
+<DT><EM>Prompt:</EM> Sectors to do:  grp.fld.chn.pol.iort.seq 
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+	A NEWSTAR .NGF file contains visibilities and associated data for one 
+or more objects. The basic unit of data is the CUT, which is a one-dimensional 
+vector of some type of data extracted from a .SCN file. The data may be either 
+visibilities or associated data such as corrections; they may be associated 
+with an interferometer or with a telescope. Cuts are addressed through a CUT 
+INDEX which is a string of six integers separated by dots: <P>
+	grp.fld.chn.pol.iort.seq <P>
+	A GROUP is basically an administrative unit, allowing the user to 
+subdivide his data, e.g. per object. 
+	The FIELD and CHANNEL are the field and channel numbers in the .SCN 
+file of the observation from which the cut was taken. 
+	POL is a number indicating the polarisation. For interferometer data,  
+pol=0, 1, 2, 3 represents XX, XY, YX, YY. For telescope data pol=0, 1 represents X, Y. 
+	Depending on the type of data, IORT is the interferometer or telescope 
+number. (The former is difficult to interpret; rather use the SELECT_IFRS 
+parameter if you want to select interferometers.) 
+	The cut SEQuence number distinguishes cuts for which all five of the 
+preceding indices are identical. It is your responsibility to know what the 
+different seq values represent. <P>
+	Index values start at zero. (Remember that for the CHN index 0 is the 
+continuum channel.) <P>
+	You may select SETS of cuts for processing through [ranges of] values 
+for the ive indices, e.g. <P>
+		2.3-5:2.*.1-7.*.2 <P>
+The WILDCARD value '*' means 'all'. Each index may also be specified as a 
+RANGE: &lt;first&gt;-&lt;last&gt;[&lt;:increment&gt;]. Indices omitted are assumed to be '*',  
+i.e.  ...1.0  means *.*.*.1.0. For wildcards at the end the dots may also be 
+omitted, i.e. 1.0 means 1.0.*.*.* <P>
+	The notation 3-5:2 stands for 'from 3 through 5 in steps of 2'. The 
+step must be positive. If it is omitted, it is taken to be 1 (as in '1-7' 
+above). <P>
+	Multiple cut SETS may be specified, separated by comma's: 
+&lt;Set1&gt;, &lt;Set2&gt;, ... The associated NGF_LOOPS keyword allows even more looping 
+over index values. <P>
+IF YOU WANT TO BE REMINDED OF WHAT CUTS ARE IN YOUR FILE: 
+	Type O or L in response to this prompt to get an Overview or Layout 
+	of your .NGF file. <P>
+IF YOU DO NOT YET FEEL COMFORTABLE WITH THESE CONCEPTS MORE HELP IS PROVIDED: 
+	Type '@' or '&gt;' to be prompted for each of the 6 indices separately,  
+	with more specific explanation per index. <P>
+IF YOU GET BORED WITH 6-NUMBER INDICES: 
+	Absolute Cut nrs '#&lt;n&gt;' can be used as an alternative. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngfsets/ngfsets_comm.html">List of general keywords</A> for NGFSETS
+<LI>Description of the <A HREF="../ngf_descr/ngf_descr.html">NGF file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngfsets_comm/ngfsets_comm.html b/ngfsets_comm/ngfsets_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..26d0855002a74e776efc4266d39810242b8efbe3
--- /dev/null
+++ b/ngfsets_comm/ngfsets_comm.html
@@ -0,0 +1,35 @@
+<TITLE>Index of general keywords from NGFSETS</TITLE>
+<H1>Description of general keywords (NGFSETS)</H1>
+
+<UL>
+<LI> <A HREF="../ngfsets/ngfsets__ngf_sets.html">
+  NGF_SETS</A>
+  Sectors to do:  grp.fld.chn.pol.iort.seq 
+<LI> <A HREF="../ngfsets/ngfsets__ngf_loops.html">
+  NGF_LOOPS</A>
+  Loop specifications: nr of cycles, index increment per cycle
+<LI> <A HREF="../ngfsets/ngfsets__ngf_groups.html">
+  NGF_GROUPS</A>
+    1st index: grp = groups
+<LI> <A HREF="../ngfsets/ngfsets__ngf_fields.html">
+  NGF_FIELDS</A>
+    2nd index: field(s)
+<LI> <A HREF="../ngfsets/ngfsets__ngf_channels.html">
+  NGF_CHANNELS</A>
+  3rd index: channel(s)
+<LI> <A HREF="../ngfsets/ngfsets__ngf_polars.html">
+  NGF_POLARS</A>
+  4th index: polarisation(s)
+<LI> <A HREF="../ngfsets/ngfsets__ngf_ifrs.html">
+  NGF_IFRS</A>
+  5th index: iort = interferometers or telescopes
+<LI> <A HREF="../ngfsets/ngfsets__ngf_cuts.html">
+  NGF_CUTS</A>
+   6th index: cut(s)
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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new file mode 100644
index 0000000000000000000000000000000000000000..dd4d46d06b8e02b31883619e8bf9401f9cd35d6f
--- /dev/null
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+/w{0 rmoveto}B /l{p -4 w}B /m{p -3 w}B /n{p -2 w}B /o{p -1 w}B /q{p 1 w}
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+/bos{/SS save N}B /eos{SS restore}B end
+
+%%EndProcSet
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group NGFSETS</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ngfsets_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ngfsets_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ngfsets_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ngfsets_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=ngfsets_public_intfc.html#SECTION0003200000000000000>  <b>Parameter NGF_CHANNELS</b></A>
+<LI> <A NAME=tex2html6 HREF=ngfsets_public_intfc.html#SECTION0003300000000000000>  <b>Parameter NGF_CUTS</b></A>
+<LI> <A NAME=tex2html7 HREF=ngfsets_public_intfc.html#SECTION0003400000000000000>  <b>Parameter NGF_FIELDS</b></A>
+<LI> <A NAME=tex2html8 HREF=ngfsets_public_intfc.html#SECTION0003500000000000000>  <b>Parameter NGF_GROUPS</b></A>
+<LI> <A NAME=tex2html9 HREF=ngfsets_public_intfc.html#SECTION0003600000000000000>  <b>Parameter NGF_IFRS</b></A>
+<LI> <A NAME=tex2html10 HREF=ngfsets_public_intfc.html#SECTION0003700000000000000>  <b>Parameter NGF_LOOPS</b></A>
+<LI> <A NAME=tex2html11 HREF=ngfsets_public_intfc.html#SECTION0003800000000000000>  <b>Parameter NGF_POLARS</b></A>
+<LI> <A NAME=tex2html12 HREF=ngfsets_public_intfc.html#SECTION0003900000000000000>  <b>Parameter NGF_SETS</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group NGFSETS, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.ngf.channels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter NGF_CHANNELS</b></A></H2>
+<P>
+  <em>Prompt:</em> 3rd index: channel(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+    <PRE>
+Give the channel index (range) CHN of a cut-Set specification
+                                                (grp.fld.CHN.pol.iort.seq)
+</PRE>
+<P>
+  <PRE>
+Remember that channel 0 is the 'continuum' channel.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take the continuum channel
+        n1              take channel nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over channels n1 through n2 [step n3]
+        *               loop over all channels for the field (wildcard)
+        n1-[*]          loop over all channels for the field,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated NGF_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.ngf.cuts><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter NGF_CUTS</b></A></H2>
+<P>
+<em>Prompt:</em>  6th index: cut(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the sequence-number index (range) SEQ of a cut-Set
+                                specification (grp.fld.chn.pol.iort.SEQ).
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take the first cut
+        n1              take cut nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over cuts n1 through n2 [step n3]
+        *               loop over all
+                         (wildcard)
+        n1-[*]          loop over all cuts for the field and channel,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+The associated NGF_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.ngf.fields><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter NGF_FIELDS</b></A></H2>
+<P>
+<em>Prompt:</em>   2nd index: field(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the field index (range) FLD of a cut-Set specification
+                                                (grp.FLD.chn.pol.iort.seq)
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) field
+        n1              take field nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over fields n1 through n2 [step n3]
+        *               loop over all fields in the observation (wildcard)
+        n1-[*][:n3]     loop over all fields in the observation,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated NGF_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.ngf.groups><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter NGF_GROUPS</b></A></H2>
+<P>
+<em>Prompt:</em>   1st index: grp  (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the group index (range) GRP of a cut-Set specification
+                                                (GRP.fld.chn.pol.iort.seq)
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) group
+        n1              take group nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over groups n1 through n2 [step n3]
+        *               loop over all available groups (wildcard)
+        n1-[*][:n3]     loop over all available groups,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated NGF_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.ngf.ifrs><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter NGF_IFRS</b></A></H2>
+<P>
+<em>Prompt:</em> 5th index: iort  (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the interferometer or telescope index (range) IORT of a cut-Set
+specification
+                                                (grp.fld.chn.pol.IORT.seq)
+</PRE>
+<P>
+  <PRE>
+This index is most useful in loop specifications (parameter NGF_LOOPS).
+</PRE>
+<P>
+  <PRE>
+For interferometer data, iort is an interferometer sequence number which can
+not be easily interpreted. Therefore, this index is useful only in loop
+specifications (parameter NGF_LOOPS). Specify a wildcard ('*') here and rely on
+the SELECT_IFRS parameter for selecting interferometers.
+</PRE>
+<P>
+  <PRE>
+For telescope data, iort is the telescope number (A-D being represented by
+10-13). The selection possibilities are limited here and you may prefer to rely
+on the SELECT_TELS parameter.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) ifr|tel
+        n1              take ifr|tel nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over ifr|tels n1 through n2 [step n3]
+        *               loop over all available ifrs|tels (wildcard)
+        n1-[*][:n3]     loop over all available ifrs|tels,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated NGF_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.ngf.loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter NGF_LOOPS</b></A></H2>
+<P>
+<em>Prompt:</em> Loop specifications: nr of cycles, index increment per cycle (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 to 16 values
+<P>
+  <PRE>
+With the NGF_LOOPS keyword, you may specify repetitions of the operation you
+are currently defining, systematically incrementing the Group, Channel, Field
+etc. indices for each new cycle.
+</PRE>
+<P>
+  <PRE>
+This is done by specifying pairs of values:
+</PRE>
+<P>
+  <PRE>
+        niter1,index_incr1, niter2,index_incr2, ...
+</PRE>
+<P>
+  <PRE>
+In each pair, the first value (n_iter) indicates the number of times the loop
+has to execute; the second value (index_incr) indicates how the Cut index is to
+be changed at the start of a new cycle.
+</PRE>
+<P>
+  <PRE>
+Example:
+        The specification NGF_SETS = grp.fld.1-2.* would select the combination
+of all cuts of frequency channels 1 and 2 for the field grp.fld. If one wishes
+to process 32 sets of successive such pairs of frequency channels, you would
+have to type in the successive NGF_SETS specifications  by hand:
+</PRE>
+<P>
+  <PRE>
+        grp.fld.1-2, grp.fld.3-4, ....., grp.fld.63-64
+</PRE>
+<P>
+  <PRE>
+Instead, you may specify NGF_LOOPS=32, 0.0.2  This will cause the program to
+execute the present operation 32 times in a loop, starting with the NGF_SETS
+specification and then incrementing its indices by 0.0.2 for every iteration;
+this is equivalent to the above 32 separate runs of the program.
+</PRE>
+<P>
+  <PRE>
+        n_iter must be > 0, and the increment can be any index string with
+simple positive or negative integers. An increment of 0 may be omitted, i.e.
+the increment specifications 0.0.3.0 and ..3 are all equivalent.
+</PRE>
+<P>
+  <PRE>
+        Loops may be nested (to a limiting depth of 8 levels). A following loop
+specification is executed inside the preceding ones.
+</PRE>
+<P>
+  <PRE>
+Example of nested loops:
+        To run your program on group 3 for 64 fields (fld index), for 10 odd
+channels (chn index) per field, starting at channel 7 and combining all
+polarisations (pol index) every time, specify:
+</PRE>
+<P>
+  <PRE>
+                NGF_SETS=3.0.7.* (initial set of cuts)
+                NGF_LOOPS=64,.1, 10,..2
+</PRE>
+<P>
+  <PRE>
+The second loop is executed as an inner loop inside the first one, that is, for
+each mosaic subfield the channels are processed in a contiguous sequence.
+</PRE>
+<P>
+  <PRE>
+IF YOU WANT TO BE REMINDED OF WHAT CUTS ARE IN YOUR FILE:
+        Type O or L in response to this prompt to get an Overview or Layout
+        of the file for which you need to specify the sets.
+</PRE>
+<P>
+<A NAME=.ngf.polars><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter NGF_POLARS</b></A></H2>
+<P>
+<em>Prompt:</em> 4th index: polarisation(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the polarisation index (range) POL of a cut-Set specification
+                                                (grp.fld.chn.POL.iort.seq)
+</PRE>
+<P>
+  <PRE>
+        POL is a number indicating the polarisation. For interferometer data,
+pol=0,1,2,3 represents XX,XY,YX,YY. For telescope data pol=0,1 represents X,Y.
+</PRE>
+<P>
+  <PRE>
+This index is useful for defining loops (NGF_LOOPS parameter). Otherwise you
+may find the SELECT_XYX parameter more convenient.
+</PRE>
+<P>
+  <PRE>
+If you prefer to use NGF_POLAR here, examples of reasonable answers are:
+        For interferometer data
+                * (=XX,XY,YX,YY)        0-3:3 (=XX,YY)  0 (=XX) 3 (=YY)
+        For telescope data
+                * (=X,Y)        0 (=X)          1 (=Y)
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated NGF_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.ngf.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter NGF_SETS</b></A></H2>
+<P>
+<em>Prompt:</em> Sectors to do:  grp.fld.chn.pol.iort.seq (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+        A NEWSTAR .NGF file contains visibilities and associated data for one
+or more objects. The basic unit of data is the CUT, which is a one-dimensional
+vector of some type of data extracted from a .SCN file. The data may be either
+visibilities or associated data such as corrections; they may be associated
+with an interferometer or with a telescope. Cuts are addressed through a CUT
+INDEX which is a string of six integers separated by dots:
+</PRE>
+<P>
+  <PRE>
+        grp.fld.chn.pol.iort.seq
+</PRE>
+<P>
+  <PRE>
+        A GROUP is basically an administrative unit, allowing the user to
+subdivide his data, e.g. per object.
+        The FIELD and CHANNEL are the field and channel numbers in the .SCN
+file of the observation from which the cut was taken.
+        POL is a number indicating the polarisation. For interferometer data,
+pol=0,1,2,3 represents XX,XY,YX,YY. For telescope data pol=0,1 represents X,Y.
+        Depending on the type of data, IORT is the interferometer or telescope
+number. (The former is difficult to interpret; rather use the SELECT_IFRS
+parameter if you want to select interferometers.)
+        The cut SEQuence number distinguishes cuts for which all five of the
+preceding indices are identical. It is your responsibility to know what the
+different seq values represent.
+        Index values start at zero. (Remember that for the CHN index 0 is the
+continuum channel.)
+</PRE>
+<P>
+  <PRE>
+        You may select SETS of cuts for processing through [ranges of] values
+for the ive indices, e.g.
+</PRE>
+<P>
+  <PRE>
+                2.3-5:2.*.1-7.*.2
+</PRE>
+<P>
+  <PRE>
+The WILDCARD value '*' means 'all'. Each index may also be specified as a
+RANGE: <first>-<last>[<:increment>]. Indices omitted are assumed to be '*',
+i.e.  ...1.0  means *.*.*.1.0. For wildcards at the end the dots may also be
+omitted, i.e. 1.0 means 1.0.*.*.*
+</PRE>
+<P>
+  <PRE>
+        The notation 3-5:2 stands for 'from 3 through 5 in steps of 2'. The
+step must be positive. If it is omitted, it is taken to be 1 (as in '1-7'
+above).
+</PRE>
+<P>
+  <PRE>
+        Multiple cut SETS may be specified, separated by comma's:
+<Set1>,<Set2>,... The associated NGF_LOOPS keyword allows even more looping
+over index values.
+</PRE>
+<P>
+  <PRE>
+IF YOU WANT TO BE REMINDED OF WHAT CUTS ARE IN YOUR FILE:
+        Type O or L in response to this prompt to get an Overview or Layout
+        of your .NGF file.
+</PRE>
+<P>
+  <PRE>
+IF YOU DO NOT YET FEEL COMFORTABLE WITH THESE CONCEPTS MORE HELP IS PROVIDED:
+        type '' or '>' to be prompted for each of the 6 indices separately,
+        with more specific explanation per index.
+</PRE>
+<P>
+  <PRE>
+IF YOU GET BORED WITH 6-NUMBER INDICES:
+        Absolute Cut nrs '#<n>' can be used as an alternative.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ngids/ngids__all_chan.html b/ngids/ngids__all_chan.html
new file mode 100644
index 0000000000000000000000000000000000000000..9635bebf1b7ae601891c9e12413361754acbe079
--- /dev/null
+++ b/ngids/ngids__all_chan.html
@@ -0,0 +1,15 @@
+<TITLE>Description of ALL_CHAN (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword ALL_CHAN</H1> 
+
+<DT><EM>Prompt:</EM> Propagate flag changes to all channels (Yes/No)?
+<DT><EM>Expected input:</EM> Logical, 1 values.<P>
+If you answer Yes to this prompt, each flag will be set for all channels. That 
+is: If you set a flag in channel &lt;i&gt; it will be copied (in the flag list) to 
+the corresponding points in all other frequency channels. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__all_pols.html b/ngids/ngids__all_pols.html
new file mode 100644
index 0000000000000000000000000000000000000000..7aab13a52fcf64d7fae5d0521ea2632e2739e8dc
--- /dev/null
+++ b/ngids/ngids__all_pols.html
@@ -0,0 +1,15 @@
+<TITLE>Description of ALL_POLS (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword ALL_POLS</H1> 
+
+<DT><EM>Prompt:</EM> Propagate flag changes to all polarisations (Yes/No)?
+<DT><EM>Expected input:</EM> Logical, 1 values.<P>
+If you answer Yes to this prompt, each flag will be set for all polarisations. 
+That is: if you set a flag on an XX visibility it will be copied (in the flag 
+list) to the corresponding XY, YX and YY visibilities. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__area.html b/ngids/ngids__area.html
new file mode 100644
index 0000000000000000000000000000000000000000..a523f80c5d13a5542aca8fb5e134374dd4c06062
--- /dev/null
+++ b/ngids/ngids__area.html
@@ -0,0 +1,17 @@
+<TITLE>Description of AREA (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword AREA</H1> 
+
+<DT><EM>Prompt:</EM>  Display area (l, m, dl, dm)
+<DT><EM>Expected input:</EM> Integer number, 4 values.<P>
+Specify the map area to be displayed. The coordinates are in grid units. (0, 0) 
+is the map centre increase is toward the upper right (decreasing RA, incrasing 
+DEC). The area is defined by four values: <P>
+	l, m     area centre 
+	dl, dm   area size 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__blank_flags.html b/ngids/ngids__blank_flags.html
new file mode 100644
index 0000000000000000000000000000000000000000..480f64336661fce3f65c682040331223378a1376
--- /dev/null
+++ b/ngids/ngids__blank_flags.html
@@ -0,0 +1,17 @@
+<TITLE>Description of BLANK_FLAGS (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword BLANK_FLAGS</H1> 
+
+<DT><EM>Prompt:</EM> Blank flagged data-points (Yes/No)?
+<DT><EM>Expected input:</EM> Logical, 1 values.<P>
+If you answer YES to this prompt, data points that are flagged will be set to 
+blank in the GIDS window. <P>
+A single red overlay plane is used to display flagged data points. This plane 
+will contain the flags for the last plane loaded. The BLANK_FLAGS option allows 
+you to discern flagged data in other pictures. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__clip_level.html b/ngids/ngids__clip_level.html
new file mode 100644
index 0000000000000000000000000000000000000000..2d6e306192180c07654e510f1314e5831d25755e
--- /dev/null
+++ b/ngids/ngids__clip_level.html
@@ -0,0 +1,17 @@
+<TITLE>Description of CLIP_LEVEL (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword CLIP_LEVEL</H1> 
+
+<DT><EM>Prompt:</EM> Clip limit for flagging
+<DT><EM>Expected input:</EM> Real number, 1 values.<P>
+All visibilities that exceed the limit in the quantity displayed (cf. parameter 
+DATA_TYPE) will be flagged. Select a suitable level by consulting the display. 
+The colour bar to the left is annotated with values and you the pixel value 
+pointed at by the cursor is shown in the upper left corner. 
+!               {\em see parameter \textref{DATA_TYPE}{.data.type} } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__data_type.html b/ngids/ngids__data_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..ce2a82ed52021de59768da183106d3b80d78add7
--- /dev/null
+++ b/ngids/ngids__data_type.html
@@ -0,0 +1,14 @@
+<TITLE>Description of DATA_TYPE (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword DATA_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> AMPLITUDE, PHASE, COSINE, SINE Select visibility component to display
+<DT><EM>Default:</EM> AMPLITUDE.
+<DT><EM>Expected input:</EM> Character(16), 1 values.<P>
+Specify how to display complex visibility values <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__map_compress.html b/ngids/ngids__map_compress.html
new file mode 100644
index 0000000000000000000000000000000000000000..26542db599462d73eab08303793094780c5295de
--- /dev/null
+++ b/ngids/ngids__map_compress.html
@@ -0,0 +1,16 @@
+<TITLE>Description of MAP_COMPRESS (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword MAP_COMPRESS</H1> 
+
+<DT><EM>Prompt:</EM> display-size compression factor
+<DT><EM>Default:</EM> 1.
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000.<P>
+For a value N, the points in a N*N box are averaged into a single display 
+point. . Example: 
+	A 1024*1024 map loaded with N=2 will result in a 512*512 image. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__map_range.html b/ngids/ngids__map_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..96986068b6c4c8fd73d278714b380bb5477b87a5
--- /dev/null
+++ b/ngids/ngids__map_range.html
@@ -0,0 +1,16 @@
+<TITLE>Description of MAP_RANGE (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword MAP_RANGE</H1> 
+
+<DT><EM>Prompt:</EM> Data-value range for diaplay
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Data values outside the limuts will be truncated to the coresponding limit. <P>
+By choosing suitable limits you can concentrate the display on a particular 
+range of intensities in the map. The defaults shown are the extremes in the 
+image to be displayed. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__map_sequences.html b/ngids/ngids__map_sequences.html
new file mode 100644
index 0000000000000000000000000000000000000000..c8dac155dc6e6fa797507bb2f1ab7743cd9eb6c9
--- /dev/null
+++ b/ngids/ngids__map_sequences.html
@@ -0,0 +1,15 @@
+<TITLE>Description of MAP_SEQUENCES (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword MAP_SEQUENCES</H1> 
+
+<DT><EM>Prompt:</EM> Display-plane range to delete
+<DT><EM>Expected input:</EM> Integer number, 2 values; min.value: 1.000000.<P>
+The display planes are numbered sequentially in the order in which they were 
+loaded. You may specify here the first and last value for a range of planes 
+that will be removed from the GIDS display memory. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__next.html b/ngids/ngids__next.html
new file mode 100644
index 0000000000000000000000000000000000000000..223240635264e5bbbfe9dff208c5c1010f1f4e17
--- /dev/null
+++ b/ngids/ngids__next.html
@@ -0,0 +1,18 @@
+<TITLE>Description of NEXT (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword NEXT</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO, ALL Load next picture
+<DT><EM>Default:</EM> ALL.
+<DT><EM>Expected input:</EM> Character(5).<P>
+This prompt appears after the loading of a picture. NGIDS will wait for your 
+reply while you may manipulate the GIDS display. Your reply options are: <P>
+	YES     Load next picture, then return with this prompt 
+	NO      Quit loading, return to OPTION prompt 
+	ALL     Load all remaining pictures without intervening consultations 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__option.html b/ngids/ngids__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..ef21483479a4955dcccdb4201a236a8a8a968b6e
--- /dev/null
+++ b/ngids/ngids__option.html
@@ -0,0 +1,45 @@
+<TITLE>Description of OPTION (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> action MAP, DATA; DOFLAG, CLIPFLAG, FLAG; UNLOAD, WRITE, CLEAR;| -GCLEAR, NOFLAG, QUIT; POINT
+<DT><EM>Expected input:</EM> Character(24).<P>
+!!                      POINT?? 
+Specify the action to perform. <P>
+   Loading/unloading visibility data or images for half-tone/colour display. The 
+   visibility 'planes' or images that you select are stored in display memory 
+   for rapid access. The number of pictures that you can store is limited by the 
+   availablity of this memory. 
+!!                      Correct? <P>
+	MAP      Load images(s) from map (.WMP) files. 
+	DATA     Load (corrected) data from visibility (.SCN) files <P>
+   Select mode for flagging of visibility data on the display. The flags you set 
+   will not yet be written back to the .SCN file, so you can freely experiment. <P>
+	DOFLAG   Switch to Flagging mode for .SCN-file visibilities 
+	CLIPFLAG Switch to Flagging mode using cliplevels 
+	FLAG     Flagging in .WMP maps using the PGPLOT cursor in GIDS <P>
+!! In this mode, no maps will be stored in GIDS (this allows you to flag in a 
+!! lot of channels etc in a single command, without overloading the GIDS 
+!! memory). In normal display mode, consequtive images will be stored in GIDS 
+!! for playback (this sequence is reset with the GCLEAR command). 
+!!                      Is this relevant? <P>
+   Saving the flags you set on your display: <P>
+	UNLOAD   Save flags list in a .FLF (binary file), from which you can 
+		  then transfer to the .SCN file through NFLAG LOAD. 
+	WRITE    Save flags list in an ASCII file, which you may manually 
+		  edit before transferringt it to the .SCN file through NFLAG 
+		  READ. 
+	CLEAR    Clear flags list. 
+!                       {\em see 
+!                       \textref{NFLAG OPS_FLIST}{nflag_private_keys.ops.flist} 
+!                       parameter }\ <P>
+   Terminate current action sequence: <P>
+	GCLEAR   Remove a sequence of loaded pictures. 
+	NOFLAG   Switch back to normal display mode. 
+	QUIT     Leave NGIDS (the GIDS window will remain on the screen). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__output_file.html b/ngids/ngids__output_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..47cfbe339cbe4690827460c426849b7de4ae57a4
--- /dev/null
+++ b/ngids/ngids__output_file.html
@@ -0,0 +1,13 @@
+<TITLE>Description of OUTPUT_FILE (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword OUTPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> (output filename)
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the full name for the output disk-file. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__plot_type.html b/ngids/ngids__plot_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..eb21ad103ded1eddbc540f364b0c25f685850a7f
--- /dev/null
+++ b/ngids/ngids__plot_type.html
@@ -0,0 +1,27 @@
+<TITLE>Description of PLOT_TYPE (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword PLOT_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> IFRS, BASE, CHAN
+<DT><EM>Expected input:</EM> Character(16).<P>
+In displaying visibilities, you can choose between three two-dimensional cross 
+sections: <P>
+   IFRS   Hour angle (horizontal) versus interferometer (vertical), one picture 
+	   per frequency channel. Interferometers in the order 
+		.... <P>
+   BASE   As IFRS, but interferometers in order of increasing baseline, - and of 
+	   increasing East telecope number within sets of redundant baselines. <P>
+   CHAN   Hour angle (horizontal) versus frequency channel (vertical), one 
+	   picture per interferometer. <P>
+NOTE: 
+	You select the channels to be displayed through the SCN_SETS parameter,  
+in the form &lt;grp&gt;.&lt;obs&gt;.&lt;fld&gt;.&lt;CHN&gt;. You have the liberty to select SCN_SETS 
+with channels for more than one &lt;grp&gt;.&lt;obs&gt;.&lt;fld&gt;. You may think of some good 
+use of this option (e.g. displaying the same channel for all fields in a 
+mosaic). 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids/ngids__user_flag.html b/ngids/ngids__user_flag.html
new file mode 100644
index 0000000000000000000000000000000000000000..e46c778160e6269a57b10bcfb6beabef6b19e5b6
--- /dev/null
+++ b/ngids/ngids__user_flag.html
@@ -0,0 +1,28 @@
+<TITLE>Description of USER_FLAG (NGIDS)</TITLE>
+<H1>Program NGIDS: private keyword USER_FLAG</H1> 
+
+<DT><EM>Prompt:</EM> NONE, ALL; MAN, OLD, CLIP, NOISE, ADD, SHAD, U1, U2, U3 Flags to use
+<DT><EM>Expected input:</EM> Character(16), 16 values.<P>
+Each of the flagging modes (parameter OPTION, options FLAG, DOFLAG, CLIPFLAG) 
+uses a specific flag type by default. You may define here one ore more flags to 
+use instead. The use foreseen for this option is to experiment using one of 
+'user' flags without getting the experimental settings tangled up with settings 
+already in existence. 
+!               {\em see parameter \textref{OPTION}{.option} } <P>
+   NONE         revert to default types per flagging mode 
+   ALL or *     use all flag types (not a very sensible idea) <P>
+   MAN          use the flag type for the MANUAL class of operations 
+   CLIP         use the flag type for the CLIP class of operations 
+   NOISE        use the flag type for the NOISE class of operations 
+   SHAD         use the flag type for the SHADOW class of operations 
+   ADD          use the flag type for the ADDITIVE class of operations <P>
+   U1           use a separate flag for some user-defined operations 
+   U2           use a separate flag for some user-defined operations 
+   U3           use a separate flag for some user-defined operations 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../ngids/ngids_keys.html">List of keywords</A> for NGIDS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/ngids_descr.ps b/ngids_descr.ps
new file mode 100644
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+++ b/ngids_descr.ps
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diff --git a/ngids_descr/images.pl b/ngids_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ngids_descr/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ngids_descr/labels.pl b/ngids_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..438c17ed11251776b29d5ad6b7647db0c4f23482
--- /dev/null
+++ b/ngids_descr/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/ngids_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/ngids_descr/ngids_descr.html b/ngids_descr/ngids_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..d7f11a1d30ba32b3e919a8fbb9a9f6b77091bc71
--- /dev/null
+++ b/ngids_descr/ngids_descr.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>A few remarks on the program NGIDS <i>(Very incomplete)</i></b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ngids_descr.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ngids_keys/ngids_keys.html b/ngids_keys/ngids_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..2f6c00af14ec78dea56888805f3fe076a0af6f76
--- /dev/null
+++ b/ngids_keys/ngids_keys.html
@@ -0,0 +1,76 @@
+<TITLE>Index of private keywords for NGIDS </TITLE>
+<H1>Description of keywords for program NGIDS</H1>
+
+<UL>
+<LI> <A HREF="../ngids/ngids__option.html">
+  OPTION</A>
+  action MAP, DATA; DOFLAG, CLIPFLAG, FLAG; UNLOAD, WRITE, CLEAR;| -GCLEAR, NOFLAG, QUIT; POINT
+<LI> <A HREF="../ngids/ngids__map_compress.html">
+  MAP_COMPRESS</A>
+  display-size compression factor
+<LI> <A HREF="../ngids/ngids__map_range.html">
+  MAP_RANGE</A>
+  Data-value range for diaplay
+<LI> <A HREF="../ngids/ngids__plot_type.html">
+  PLOT_TYPE</A>
+  IFRS, BASE, CHAN
+<LI> <A HREF="../ngids/ngids__data_type.html">
+  DATA_TYPE</A>
+  AMPLITUDE, PHASE, COSINE, SINE Select visibility component to display
+<LI> <A HREF="../ngids/ngids__map_sequences.html">
+  MAP_SEQUENCES</A>
+  Display-plane range to delete
+<LI> <A HREF="../ngids/ngids__blank_flags.html">
+  BLANK_FLAGS</A>
+  Blank flagged data-points (Yes/No)?
+<LI> <A HREF="../ngids/ngids__output_file.html">
+  OUTPUT_FILE</A>
+  (output filename)
+<LI> <A HREF="../ngids/ngids__all_chan.html">
+  ALL_CHAN</A>
+  Propagate flag changes to all channels (Yes/No)?
+<LI> <A HREF="../ngids/ngids__all_pols.html">
+  ALL_POLS</A>
+  Propagate flag changes to all polarisations (Yes/No)?
+<LI> <A HREF="../ngids/ngids__user_flag.html">
+  USER_FLAG</A>
+  NONE, ALL; MAN, OLD, CLIP, NOISE, ADD, SHAD, U1, U2, U3 Flags to use
+<LI> <A HREF="../ngids/ngids__area.html">
+  AREA</A>
+   Display area (l, m, dl, dm)
+<LI> <A HREF="../ngids/ngids__next.html">
+  NEXT</A>
+  YES, NO, ALL Load next picture
+<LI> <A HREF="../ngids/ngids__clip_level.html">
+  CLIP_LEVEL</A>
+  Clip limit for flagging
+<P>
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpnode_comm/wmpnode_comm.html">WMPNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpsets_comm/wmpsets_comm.html">WMPSETS</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../ngids_descr/ngids_descr.html">program NGIDS</A>
+</UL>
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+eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/ngids_private_intfc/images.pl b/ngids_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/ngids_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/ngids_private_intfc/labels.pl b/ngids_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..a9a70a6b4ed69478a6d70fb2b18fb3ee231f8446
--- /dev/null
+++ b/ngids_private_intfc/labels.pl
@@ -0,0 +1,22 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".next"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".all.pols"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".public"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".all.chan"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".area"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".map.compress"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".data.type"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".option"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".map.range"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".map.sequences"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".clip.level"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".output.file"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".blank.flags"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".user.flag"} ="$URL/ngids_private_intfc.html"; 
+$external_labels{".plot.type"} ="$URL/ngids_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/ngids_private_intfc/ngids_private_intfc.html b/ngids_private_intfc/ngids_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..f47fded3a500e7f57139d8e8767dfd803bb3a34d
--- /dev/null
+++ b/ngids_private_intfc/ngids_private_intfc.html
@@ -0,0 +1,363 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NGIDS</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=ngids_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=ngids_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=ngids_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=ngids_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=ngids_private_intfc.html#SECTION0003200000000000000>  <b>Parameter ALL_CHAN</b></A>
+<LI> <A NAME=tex2html6 HREF=ngids_private_intfc.html#SECTION0003300000000000000>  <b>Parameter ALL_POLS</b></A>
+<LI> <A NAME=tex2html7 HREF=ngids_private_intfc.html#SECTION0003400000000000000>  <b>Parameter AREA</b></A>
+<LI> <A NAME=tex2html8 HREF=ngids_private_intfc.html#SECTION0003500000000000000>  <b>Parameter BLANK_FLAGS</b></A>
+<LI> <A NAME=tex2html9 HREF=ngids_private_intfc.html#SECTION0003600000000000000>  <b>Parameter CLIP_LEVEL</b></A>
+<LI> <A NAME=tex2html10 HREF=ngids_private_intfc.html#SECTION0003700000000000000>  <b>Parameter DATA_TYPE</b></A>
+<LI> <A NAME=tex2html11 HREF=ngids_private_intfc.html#SECTION0003800000000000000>  <b>Parameter MAP_COMPRESS</b></A>
+<LI> <A NAME=tex2html12 HREF=ngids_private_intfc.html#SECTION0003900000000000000>  <b>Parameter MAP_RANGE</b></A>
+<LI> <A NAME=tex2html13 HREF=ngids_private_intfc.html#SECTION00031000000000000000>  <b>Parameter MAP_SEQUENCES</b></A>
+<LI> <A NAME=tex2html14 HREF=ngids_private_intfc.html#SECTION00031100000000000000>  <b>Parameter NEXT</b></A>
+<LI> <A NAME=tex2html15 HREF=ngids_private_intfc.html#SECTION00031200000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html16 HREF=ngids_private_intfc.html#SECTION00031300000000000000>  <b>Parameter OUTPUT_FILE</b></A>
+<LI> <A NAME=tex2html17 HREF=ngids_private_intfc.html#SECTION00031400000000000000>  <b>Parameter PLOT_TYPE</b></A>
+<LI> <A NAME=tex2html18 HREF=ngids_private_intfc.html#SECTION00031500000000000000>  <b>Parameter USER_FLAG</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NGIDS. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>.
+<P>
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../wmpnode_public_intfc/wmpnode_public_intfc.html">WMPNODE</A> public keywords 
+<LI> <A HREF="../wmpsets_public_intfc/wmpsets_public_intfc.html">WMPSETS</A> public keywords 
+</UL>
+<P>
+<A NAME=.all.chan><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter ALL_CHAN</b></A></H2>
+<P>
+  <em>Prompt:</em> Propagate flag changes to all channels (Yes/No)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+    <PRE>
+If you answer Yes to this prompt, each flag will be set for all channels. That
+is: If you set a flag in channel <i> it will be copied (in the flag list) to
+the corresponding points in all other frequency channels.
+</PRE>
+<P>
+<A NAME=.all.pols><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter ALL_POLS</b></A></H2>
+<P>
+<em>Prompt:</em> Propagate flag changes to all polarisations (Yes/No)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+If you answer Yes to this prompt, each flag will be set for all polarisations.
+That is: if you set a flag on an XX visibility it will be copied (in the flag
+list) to the corresponding XY, YX and YY visibilities.
+</PRE>
+<P>
+<A NAME=.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter AREA</b></A></H2>
+<P>
+<em>Prompt:</em>  Display area (l,m, dl,dm)<BR><em>Expected input:</em> Integer:  1 to 4 values
+<P>
+  <PRE>
+Specify the map area to be displayed. The coordinates are in grid units. (0,0)
+is the map centre increase is toward the upper right (decreasing RA, incrasing
+DEC). The area is defined by four values:
+</PRE>
+<P>
+  <PRE>
+        l,m     area centre
+        dl,dm   area size
+</PRE>
+<P>
+<A NAME=.blank.flags><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter BLANK_FLAGS</b></A></H2>
+<P>
+<em>Prompt:</em> Blank flagged data-points (Yes/No)?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+If you answer YES to this prompt, data points that are flagged will be set to
+blank in the GIDS window.
+</PRE>
+<P>
+  <PRE>
+A single red overlay plane is used to display flagged data points. This plane
+will contain the flags for the last plane loaded. The BLANK_FLAGS option allows
+you to discern flagged data in other pictures.
+</PRE>
+<P>
+<A NAME=.clip.level><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter CLIP_LEVEL</b></A></H2>
+<P>
+<em>Prompt:</em> Clip limit for flagging<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+All visibilities that exceed the limit in the quantity displayed (cf. parameter
+DATA_TYPE) will be flagged. Select a suitable level by consulting the display.
+The colour bar to the left is annotated with values and you the pixel value
+pointed at by the cursor is shown in the upper left corner.
+</PRE> 
+               <em>see parameter <A HREF="#.data.type">DATA_TYPE</A> </em>
+<P>
+<A NAME=.data.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter DATA_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Select visibility component to display<BR><em>Expected input:</em> Character *16:  1 value
+<P>
+  <PRE>
+Specify how to display complex visibility values
+</PRE>
+<P>
+<A NAME=.map.compress><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter MAP_COMPRESS</b></A></H2>
+<P>
+<em>Prompt:</em> display-size compression factor<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+For a value N, the points in a N*N box are averaged into a single display
+point. . Example:
+        A 1024*1024 map loaded with N=2 will result in a 512*512 image.
+</PRE>
+<P>
+<A NAME=.map.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter MAP_RANGE</b></A></H2>
+<P>
+<em>Prompt:</em> Data-value range for diaplay<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Data values outside the limuts will be truncated to the coresponding limit.
+</PRE>
+<P>
+  <PRE>
+By choosing suitable limits you can concentrate the display on a particular
+range of intensities in the map. The defaults shown are the extremes in the
+image to be displayed.
+</PRE>
+<P>
+<A NAME=.map.sequences><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter MAP_SEQUENCES</b></A></H2>
+<P>
+<em>Prompt:</em> Display-plane range to delete<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+The display planes are numbered sequentially in the order in which they were
+loaded. You may specify here the first and last value for a range of planes
+that will be removed from the GIDS display memory.
+</PRE>
+<P>
+<A NAME=.next><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter NEXT</b></A></H2>
+<P>
+<em>Prompt:</em> Load next picture<BR><em>Expected input:</em> Character *5:  1 value
+<P>
+  <PRE>
+This prompt appears after the loading of a picture. NGIDS will wait for your
+reply while you may manipulate the GIDS display. Your reply options are:
+</PRE>
+<P>
+  <PRE>
+        YES     Load next picture, then return with this prompt
+        NO      Quit loading, return to OPTION prompt
+        ALL     Load all remaining pictures without intervening consultations
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> action<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the action to perform.
+</PRE>
+<P>
+  <PRE>
+   Loading/unloading visibility data or images for half-tone/colour display. The
+   visibility 'planes' or images that you select are stored in display memory
+   for rapid access. The number of pictures that you can store is limited by the
+   availablity of this memory.
+</PRE>
+<P>
+  <PRE>
+        MAP      Load images(s) from map (.WMP) files.
+        DATA     Load (corrected) data from visibility (.SCN) files
+</PRE>
+<P>
+  <PRE>
+   Select mode for flagging of visibility data on the display. The flags you set
+   will not yet be written back to the .SCN file, so you can freely experiment.
+</PRE>
+<P>
+  <PRE>
+        DOFLAG   Switch to Flagging mode for .SCN-file visibilities
+        CLIPFLAG Switch to Flagging mode using cliplevels
+        FLAG     Flagging in .WMP maps using the PGPLOT cursor in GIDS
+</PRE>
+<P>
+  <PRE>
+   Saving the flags you set on your display:
+</PRE>
+<P>
+  <PRE>
+        UNLOAD   Save flags list in a .FLF (binary file), from which you can
+                  then transfer to the .SCN file through NFLAG LOAD.
+        WRITE    Save flags list in an ASCII file, which you may manually
+                  edit before transferringt it to the .SCN file through NFLAG
+                  READ.
+        CLEAR    Clear flags list.
+</PRE> 
+                       <em>see
+                       <A HREF="../nflag_private_keys/nflag_private_keys.html#.ops.flist">NFLAG OPS_FLIST</A>
+                       parameter </em> 
+<P>
+  <PRE>
+   Terminate current action sequence:
+</PRE>
+<P>
+  <PRE>
+        GCLEAR   Remove a sequence of loaded pictures.
+        NOFLAG   Switch back to normal display mode.
+        QUIT     Leave NGIDS (the GIDS window will remain on the screen).
+</PRE>
+<P>
+<A NAME=.output.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter OUTPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> (output filename)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the full name for the output disk-file.
+</PRE>
+<P>
+<A NAME=.plot.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter PLOT_TYPE</b></A></H2>
+<P>
+<em>Expected input:</em> Character *16:  1 value
+<P>
+  <PRE>
+In displaying visibilities, you can choose between three two-dimensional cross
+sections:
+</PRE>
+<P>
+  <PRE>
+   IFRS   Hour angle (horizontal) versus interferometer (vertical), one picture
+           per frequency channel. Interferometers in the order
+                ....
+</PRE>
+<P>
+  <PRE>
+   BASE   As IFRS, but interferometers in order of increasing baseline, - and of
+           increasing East telecope number within sets of redundant baselines.
+</PRE>
+<P>
+  <PRE>
+   CHAN   Hour angle (horizontal) versus frequency channel (vertical), one
+           picture per interferometer.
+</PRE>
+<P>
+  <PRE>
+NOTE:
+        You select the channels to be displayed through the SCN_SETS parameter,
+in the form <grp>.<obs>.<fld>.<CHN>. You have the liberty to select SCN_SETS
+with channels for more than one <grp>.<obs>.<fld>. You may think of some good
+use of this option (e.g. displaying the same channel for all fields in a
+mosaic).
+</PRE>
+<P>
+<A NAME=.user.flag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter USER_FLAG</b></A></H2>
+<P>
+<em>Prompt:</em> Flags to use<BR><em>Expected input:</em> Character *16:  1 to 16 values
+<P>
+  <PRE>
+Each of the flagging modes (parameter OPTION, options FLAG, DOFLAG, CLIPFLAG)
+uses a specific flag type by default. You may define here one ore more flags to
+use instead. The use foreseen for this option is to experiment using one of
+'user' flags without getting the experimental settings tangled up with settings
+already in existence.
+</PRE> 
+               <em>see parameter <A HREF="#.option">OPTION</A> </em>
+<P>
+  <PRE>
+   NONE         revert to default types per flagging mode
+   ALL or *     use all flag types (not a very sensible idea)
+</PRE>
+<P>
+  <PRE>
+   MAN          use the flag type for the MANUAL class of operations
+   CLIP         use the flag type for the CLIP class of operations
+   NOISE        use the flag type for the NOISE class of operations
+   SHAD         use the flag type for the SHADOW class of operations
+   ADD          use the flag type for the ADDITIVE class of operations
+</PRE>
+<P>
+  <PRE>
+   U1           use a separate flag for some user-defined operations
+   U2           use a separate flag for some user-defined operations
+   U3           use a separate flag for some user-defined operations
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nmap/nmap__ the default one.html b/nmap/nmap__ the default one.html
new file mode 100644
index 0000000000000000000000000000000000000000..de03209f32469908d9e8cc96055b2be0b84593cd
--- /dev/null
+++ b/nmap/nmap__ the default one.html	
@@ -0,0 +1,23 @@
+<TITLE>Description of  the default one (NMAP)</TITLE>
+<H1>Program NMAP: private keyword  the default one</H1> 
+
+<DT><EM>Prompt:</EM> Correct map for convolution taper (Yes/No) ?
+<DT><EM>Default:</EM> YES.
+<DT><EM>Expected input:</EM> Logical.<P>
+The interpolation (convolution) in the visibility domain results in a 
+multiplication ('tapering') of the output map(s) and antenna pattern(s) by the 
+Fourier transform of the convolving function; i.e., toward the edge of the map 
+the sources, sidelobes and grating responses appear weaker than they actually 
+are. <P>
+By default this effect will be corrected for by dividing the map through the 
+taper. A side effect of this correction is that the noise, which is uniform 
+over the whole uncorrected map, is amplified toward the map edges. <P>
+Here you are given the option to bypass this correction. e.g. because uniform 
+noise is more important for your application than source fluxes. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__.html b/nmap/nmap__.html
new file mode 100644
index 0000000000000000000000000000000000000000..9f6e3584389771f6ebc9036b25b8fb3119519c35
--- /dev/null
+++ b/nmap/nmap__.html
@@ -0,0 +1,15 @@
+<TITLE>Description of  (NMAP)</TITLE>
+<H1>Program NMAP: private keyword </H1> 
+
+<DT><EM>Prompt:</EM> Map reference coordinates: RA, DEC (decimal deg)
+<DT><EM>Expected input:</EM> Double precision number, 2 values.<P>
+Specify (in decimal degrees) the RA and DEC of the reference coordinates to use 
+in producing the map. The coordinate system is B1950/J2000 or apparent as 
+defined by your value for parameter MAP_COORD. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__area.html b/nmap/nmap__area.html
new file mode 100644
index 0000000000000000000000000000000000000000..8e2510df29133f030a2d2d11607398387f2c49f8
--- /dev/null
+++ b/nmap/nmap__area.html
@@ -0,0 +1,17 @@
+<TITLE>Description of AREA (NMAP)</TITLE>
+<H1>Program NMAP: private keyword AREA</H1> 
+
+<DT><EM>Prompt:</EM> Area: l, m, dl, dm
+<DT><EM>Expected input:</EM> Integer number, 4 values.<P>
+Specify the area to be selected: <P>
+        l, m    position in grid spacings of centre of area 
+                0, 0 is the map centre, increaing toward the upper right (i.e. 
+                 with DEcreasing RA and INcreasing DEC) <P>
+        dl, dm  horizontal and vertical area sizes <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__bas_resolution.html b/nmap/nmap__bas_resolution.html
new file mode 100644
index 0000000000000000000000000000000000000000..69a480d33013f9240a9dc0506b6234d956891f2e
--- /dev/null
+++ b/nmap/nmap__bas_resolution.html
@@ -0,0 +1,17 @@
+<TITLE>Description of BAS_RESOLUTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword BAS_RESOLUTION</H1> 
+
+<DT><EM>Prompt:</EM> Baseline averaging interval (m)
+<DT><EM>Expected input:</EM> Real number; min.value: 9.000000; max.value: 300.000000.<P>
+Specify the width in metres of baseline over which visibilities will be 
+averaged. <P>
+The minimum value is 9, representing the smallest baseline increment ever 
+present in practice in a (set of) WSRT observation(s). The maximum is 
+(arbitrarily) fixed at 300. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__clip_area.html b/nmap/nmap__clip_area.html
new file mode 100644
index 0000000000000000000000000000000000000000..3dd60632d1c766c206a935652bac30c67f3107b1
--- /dev/null
+++ b/nmap/nmap__clip_area.html
@@ -0,0 +1,15 @@
+<TITLE>Description of CLIP_AREA (NMAP)</TITLE>
+<H1>Program NMAP: private keyword CLIP_AREA</H1> 
+
+<DT><EM>Prompt:</EM> UV-radius range for clipping (m)
+<DT><EM>Default:</EM> 0., 100000..
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.000000.<P>
+Specify the (circular) UV-plane radii (in metres) between which you want to 
+clip the data. The default is to clip everywhere. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__clip_levels.html b/nmap/nmap__clip_levels.html
new file mode 100644
index 0000000000000000000000000000000000000000..93ae70aad7154fd98b4bb31eadcc1a5a250d2fcc
--- /dev/null
+++ b/nmap/nmap__clip_levels.html
@@ -0,0 +1,23 @@
+<TITLE>Description of CLIP_LEVELS (NMAP)</TITLE>
+<H1>Program NMAP: private keyword CLIP_LEVELS</H1> 
+
+<DT><EM>Prompt:</EM> Amplitude range to be discarded
+<DT><EM>Default:</EM> 100000., 100000..
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify amplitude range (in Westerbork Units) of visibility magnitudes that you 
+want to discard. <P>
+In the annulus defined by CLIP_AREA, values between the limits you specify will 
+be discarded. 
+! {\em parameter \textref{CLIP_AREA}{.clip.area} } <P>
+NOTE: It would be more natural to define a range within which visibilities are 
+considered valid. As it is, only the lower limit is actually useful, allowing 
+you to define a rejection threshold for interference. To do so, specify your 
+threshold for the lower and 'infinity' for the upper limit, e.g. <P>
+                &lt;threshold&gt;, 100000  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__clipping.html b/nmap/nmap__clipping.html
new file mode 100644
index 0000000000000000000000000000000000000000..9293b70eca73b930daf87ec4b970dae804dc57ac
--- /dev/null
+++ b/nmap/nmap__clipping.html
@@ -0,0 +1,19 @@
+<TITLE>Description of CLIPPING (NMAP)</TITLE>
+<H1>Program NMAP: private keyword CLIPPING</H1> 
+
+<DT><EM>Prompt:</EM> Clipping?
+<DT><EM>Expected input:</EM> Logical.<P>
+'Clipping' means discarding data in a certain annulus that fall within a 
+certain range of values (yet to be specified). 
+! {\em parameters \textref{CLIP_AREA}{.clip.area},  
+!                 \textref{CLIP_LEVELS}{.clip.levels} } <P>
+It is a simple (and primitive) method of eliminating data affected by strong 
+interference. (Note that NFLAG provides a much wider scala of operations to 
+find and suppress interference.) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__comment.html b/nmap/nmap__comment.html
new file mode 100644
index 0000000000000000000000000000000000000000..8f0131981b1babe781eafeb2fbd211f93fa83344
--- /dev/null
+++ b/nmap/nmap__comment.html
@@ -0,0 +1,13 @@
+<TITLE>Description of COMMENT (NMAP)</TITLE>
+<H1>Program NMAP: private keyword COMMENT</H1> 
+
+<DT><EM>Prompt:</EM> FITS comment (&lt;=70 chars)
+<DT><EM>Expected input:</EM> Character(70).<P>
+The given text will be included as COMMENT in FITS output. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__convolve.html b/nmap/nmap__convolve.html
new file mode 100644
index 0000000000000000000000000000000000000000..7239f22d2033cdd2c88d13c15ad321843acee842
--- /dev/null
+++ b/nmap/nmap__convolve.html
@@ -0,0 +1,41 @@
+<TITLE>Description of CONVOLVE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword CONVOLVE</H1> 
+
+<DT><EM>Prompt:</EM> GAUSS, BOX, P4ROL, P6ROL, EXPSINC Convolution type
+<DT><EM>Expected input:</EM> Character(8).<P>
+This is the interpolation function to be used in horizontally and vertically 
+interpolating the observed visibilities onto the rectangular grid to be used in 
+the Fast Fourier Transform. <P>
+The choice of function determines the detailed aliasing properties of the 
+map(s). NMAP chooses appropriate horizontal and vertical width parameters for 
+each. You may specify one of the following functions: <P>
+   Gaussian-based: <P>
+        EXPSINC Sinc*exp on 6*6 grid points: An 'approximation' to the ideal 
+                 sinc (=sin(x)/x) function. This is the function selected as the 
+                 default for map-making after extensive experience with all of 
+                 the options available here. <P>
+        GAUSS   Gaussian type over 4*4 grid points: The function used in the 
+                 first years of WSRT operations; it was later replaced by the 
+                 prolate spheroids. The expense in computing time is the same as 
+                 for P4ROL. <P>
+   Prolate spheroids: These function minimise the 'power' (= the integral of the 
+    intensity squared) 'aliased in' from sources outside the map <P>
+        P4ROL   Prolate spheroidal function with 4*4 grid points. 
+        P6ROL   Prolate spheroidal function with 6*6 grid points: By using more 
+                 points in the interpolation, this function pushes the aliasing 
+                 down considerably, - at the expense of a factor two or more in 
+                 computing time for the interpolation <P>
+All the above functions may also be used in constructing a UV-plane for display 
+(UV_COORDINATES=UV). <P>
+For plotting visibilities versus baseline or interferometer 
+(UV_COORDINATES=BASHA or IFRHA), they are of little use, and the default one 
+would normally select is <P>
+        BOX     Shift to nearest grid point. 
+! {\em see parameter \textref{UV\_COORDINATES}{.uv.coordinates} } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__csum_factors.html b/nmap/nmap__csum_factors.html
new file mode 100644
index 0000000000000000000000000000000000000000..1904eaf14f461f2b7251b251b5d58d5c441b9672
--- /dev/null
+++ b/nmap/nmap__csum_factors.html
@@ -0,0 +1,21 @@
+<TITLE>Description of CSUM_FACTORS (NMAP)</TITLE>
+<H1>Program NMAP: private keyword CSUM_FACTORS</H1> 
+
+<DT><EM>Prompt:</EM> Summing multipliers
+<DT><EM>Expected input:</EM> Real number, 16 values.<P>
+Specify up to 8 complex weight factors by which the input maps have to be 
+multiplied. For each factor the real part should be given first, the imaginary 
+next. So 1, 0, 0, -1  means add the real part of the first map-pair to the 
+imagingary part of the second map-pair: <P>
+    (1+0*i)*(map1r + i*map1i) + (0-1*i)*(map2r + i*map2i) <P>
+If the number of weights you give is less than the number of maps  to be 
+combined, the weights will re-used in a cyclic fashion. Example: 
+        1, 1, -1, -1 will average the first, third, ... pairs in your WMP_SETS 
+specification with the negated second, fourth ... pairs. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__cubic.html b/nmap/nmap__cubic.html
new file mode 100644
index 0000000000000000000000000000000000000000..2c86b77717b2daf8689e223c586012e4e129b621
--- /dev/null
+++ b/nmap/nmap__cubic.html
@@ -0,0 +1,13 @@
+<TITLE>Description of CUBIC (NMAP)</TITLE>
+<H1>Program NMAP: private keyword CUBIC</H1> 
+
+<DT><EM>Prompt:</EM> Make line cube (Yes/No) ?
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want to output the FITS maps in one cube or in separate maps <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__cweight_type.html b/nmap/nmap__cweight_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..c78c1524fe8fa554aa16f07824a7a524aecacc74
--- /dev/null
+++ b/nmap/nmap__cweight_type.html
@@ -0,0 +1,23 @@
+<TITLE>Description of CWEIGHT_TYPE (NMAP)</TITLE>
+<H1>Description of general keyword CWEIGHT_TYPE</H1>
+
+<DT><EM>Prompt:</EM> GAUSS, LINEAR, NATURAL Circular weight type
+<DT><EM>Expected input:</EM> Character(8).<P>
+ON TOP of the standard taper function which is circular in the equatorial UV 
+plane, you nay specify a taper that is circular in the projected UV plane (i.e. 
+the plane as seen from the field centre). You can select one out of the 
+following functions: <P>
+	GAUSS   exp -(&lt;projected baseline&gt;/CWEIGHT_VALUE)**2 <P>
+	LINEAR  max (0, 1-&lt;projected baseline&gt;/CWEIGHT_VALUE) <P>
+	NATURAL unity weight everywhere, i.e. no circular taper <P>
+NOTE that the circular weighing does not replace the standard tapering, but is 
+applied as an EXTRA weight function. This is probably not what you want; you 
+may eliminate the normal tapering by specifying TAPER=NATURAL and 
+UNIFORM=STANDARD to take into account the radial density dependence of measured 
+visibilities. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__cweight_value.html b/nmap/nmap__cweight_value.html
new file mode 100644
index 0000000000000000000000000000000000000000..6661ffad7dcfcb03f08c52b3bcc6996d19348fd2
--- /dev/null
+++ b/nmap/nmap__cweight_value.html
@@ -0,0 +1,20 @@
+<TITLE>Description of CWEIGHT_VALUE (NMAP)</TITLE>
+<H1>Description of general keyword CWEIGHT_VALUE</H1>
+
+<DT><EM>Prompt:</EM> Circular-weight width (metres)
+<DT><EM>Default:</EM> 2548..
+<DT><EM>Expected input:</EM> Real number; min.value: 10.000000.<P>
+Specify the width for your circular weight function. <P>
+If you have selected a gaussian for the circular_weight function 
+(CWEIGHT_TYPE=GAUSS), the value you specify here will be the projected baseline 
+radius for which the weight is 1/e times its value in the origin. The default 
+value makes the weight equal to 1/4 at a projected baseline of 3000 m. <P>
+If you have selected a triangular weight function (CWEIGHT_TYPE=LINEAR), the 
+value you specify here is the projected baseline at which the weight reaches 
+zero. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__data_action.html b/nmap/nmap__data_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..d457ec8982900f532ee171255ef4040ec69117d3
--- /dev/null
+++ b/nmap/nmap__data_action.html
@@ -0,0 +1,17 @@
+<TITLE>Description of DATA_ACTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword DATA_ACTION</H1> 
+
+<DT><EM>Prompt:</EM> Action to perform on the data SHOW; NOISE, OFFSET; QUIT
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform: <P>
+        SHOW    show detailed map data <P>
+        NOISE   calculate noise 
+        OFFSET  calculate noise and offset <P>
+        QUIT    quit data part <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__data_type.html b/nmap/nmap__data_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..107af97a2855ee2056d9f362db106f1741ecda4c
--- /dev/null
+++ b/nmap/nmap__data_type.html
@@ -0,0 +1,20 @@
+<TITLE>Description of DATA_TYPE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword DATA_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> NORMAL, COS, SIN, AMPL, PHASE Data transformation for display
+<DT><EM>Default:</EM> NORMAL.
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify how to transform the complex input visibilities. NORMAL is the default; 
+the others are for special experiments and diagnostics only. <P>
+        NORMAL  Complex value <P>
+        COS     Real part 
+        SIN     Imaginary part <P>
+        AMPL    Amplitude 
+        PHASE   Phase  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__deconvolve.html b/nmap/nmap__deconvolve.html
new file mode 100644
index 0000000000000000000000000000000000000000..947bb76deb3c4023662e95800653e2fa60f7abbf
--- /dev/null
+++ b/nmap/nmap__deconvolve.html
@@ -0,0 +1,23 @@
+<TITLE>Description of DECONVOLVE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword DECONVOLVE</H1> 
+
+<DT><EM>Prompt:</EM> Correct map for convolution taper (Yes/No) ?
+<DT><EM>Default:</EM> YES.
+<DT><EM>Expected input:</EM> Logical.<P>
+The interpolation (convolution) in the visibility domain results in a 
+multiplication ('tapering') of the output map(s) and antenna pattern(s) by the 
+Fourier transform of the convolving function; i.e., toward the edge of the map 
+the sources, sidelobes and grating responses appear weaker than they actually 
+are. <P>
+By default this effect will be corrected for by dividing the map through the 
+taper. A side effect of this correction is that the noise, which is uniform 
+over the whole uncorrected map, is amplified toward the map edges. <P>
+Here you are given the option to bypass this correction. e.g. because uniform 
+noise is more important for your application than source fluxes.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__fiddle_option.html b/nmap/nmap__fiddle_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..c0d2271e54a0aa247b313032de446cc8840ead4f
--- /dev/null
+++ b/nmap/nmap__fiddle_option.html
@@ -0,0 +1,44 @@
+<TITLE>Description of FIDDLE_OPTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FIDDLE_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Fiddle action| BEAM, DEBEAM, FACTOR; EXTRACT, COPY, LOAD;|-ADD, AVER, POL, ANGLE; SUM, CSUM, RSUM, MOSCOM; QUIT
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform. <P>
+   In-place modifications: Modify data of (an) input image(s): <P>
+        BEAM    correct map for primary beam attenuation so it will represent 
+                 the 'true' sky 
+        DEBEAM  apply primary beam attenuation to map so it will reprsent the 
+                 product of the 'true' sky and the primary beam 
+        FACTOR  multiply image with a constant factor <P>
+   Unary operations: Create 1 new image from each input image: <P>
+        EXTRACT extract an area from (a) image(s) 
+        COPY    copy image(s) 
+        LOAD    read or write (an) image(s) in a foreign format (e.g. Holog) <P>
+   Binary combinations: make (a) new output image(s) from (a) pair(s) of input 
+   images: <P>
+        ADD     weighted sum of two images: F1*image1 + F2*image2 
+        AVER    weighted average of two images: 
+                        (F1*image1 + F2*image2) / [abs(F1) + abs(F2)] 
+        POL     degree of linear polarisation from Q and U maps: 
+                        sqrt (Qmap**2 + Umap**2)] 
+        ANGLE   polarisation orientation (radians) from Q and U maps: 
+                        0.5*atan (Umap / Qmap) <P>
+   Combinations of more than two images: <P>
+        SUM     weighted summation of (a) set(s) of images in a single .WMP file 
+                 (you will be prompted to select the weighing method) 
+        CSUM    weighted summation of pairs of images. You will be prompted 
+                 for (a) set(s) of "real" images and (a) set(s) of 
+                 "imaginary" images and complex weighting factors. 
+        RSUM    idem, but the complex weighting factors will be calculated 
+                 based on a specified rotation measure. 
+        MOSCOM  'mosaic combine': merge a set of maps (generally for different 
+                 field centres) into one output map <P>
+   Miscellaneous: <P>
+        QUIT    Return to OPTIONS level  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__field_centre.html b/nmap/nmap__field_centre.html
new file mode 100644
index 0000000000000000000000000000000000000000..f4f5217dbbf7370741c64df8df258917e8e0383e
--- /dev/null
+++ b/nmap/nmap__field_centre.html
@@ -0,0 +1,14 @@
+<TITLE>Description of FIELD_CENTRE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FIELD_CENTRE</H1> 
+
+<DT><EM>Prompt:</EM> Field centre: RA, DEC (decimal deg)
+<DT><EM>Expected input:</EM> Double precision number, 2 values.<P>
+Specify the map centre wanted in the apparent-coordinate frame. <P>
+Default is the fringe-stopping centre.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__field_shift.html b/nmap/nmap__field_shift.html
new file mode 100644
index 0000000000000000000000000000000000000000..6a4c739139007f294d2b5574aed085923d98efee
--- /dev/null
+++ b/nmap/nmap__field_shift.html
@@ -0,0 +1,22 @@
+<TITLE>Description of FIELD_SHIFT (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FIELD_SHIFT</H1> 
+
+<DT><EM>Prompt:</EM> l, m field shift (arcsec)
+<DT><EM>Default:</EM> 0., 0..
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the field-centre shift in l, m coordinates. <P>
+(l, m) are 'horizontal' and 'vertical' Cartesian coordinates in a plane tangent 
+to the celestial sphere at the reference centre. The coordinate system is 
+B1950/J2000 or apparent as defined by your value for parameter MAP_COORD. 
+!!      {\it See \textref{MAP_COORD}{.map.coord},  
+!!               \textref{REF_COORD}{.ref.coord} } <P>
+If you enter a null value (\ or ""), you will be prompted for a FIELD_CENTRE 
+instead. This option is intended for instrumental test programs only and has 
+not been tested for general applications; use it at your own risk if you wish.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__field_size.html b/nmap/nmap__field_size.html
new file mode 100644
index 0000000000000000000000000000000000000000..e88bd17d4e1455248db2e34ac537ddecaf2e883d
--- /dev/null
+++ b/nmap/nmap__field_size.html
@@ -0,0 +1,17 @@
+<TITLE>Description of FIELD_SIZE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FIELD_SIZE</H1> 
+
+<DT><EM>Prompt:</EM> Fieldsize l, m (deg)
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.001000; max.value: 180.000000.<P>
+Specify the l and m field size of the map to be transformed. The default will 
+produce a map with a resolution of about 3.5 grid intervals per 
+synthesized-beam half-width. <P>
+If you give a NULL answer (two double quotes), you will be prompted for the 
+grid steps.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__filename.html b/nmap/nmap__filename.html
new file mode 100644
index 0000000000000000000000000000000000000000..ae89a8c93ebed2739e592e0c8285cd62ca64aea5
--- /dev/null
+++ b/nmap/nmap__filename.html
@@ -0,0 +1,15 @@
+<TITLE>Description of FILENAME (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FILENAME</H1> 
+
+<DT><EM>Prompt:</EM> Name for output disk file
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (without an extension) to be used in creating a 
+pseudo-tape output file name (e.g. FITS write). <P>
+Specify a full filename otherwise (e.g. LOAD/UNLOAD in FIDDLE). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__fits_scale.html b/nmap/nmap__fits_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..8ebe4ee16d8384c3db2683963ef4813cfdf4f8a6
--- /dev/null
+++ b/nmap/nmap__fits_scale.html
@@ -0,0 +1,15 @@
+<TITLE>Description of FITS_SCALE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FITS_SCALE</H1> 
+
+<DT><EM>Prompt:</EM> JY, WU Units of source flux
+<DT><EM>Expected input:</EM> Character(4).<P>
+Specify the output units of the FITS data: <P>
+        JY      jansky per beam 
+        WU      Westerbork units (1 W.U. = 5 mJy) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__ft_size.html b/nmap/nmap__ft_size.html
new file mode 100644
index 0000000000000000000000000000000000000000..91b93b7ebbab3299e37540b1a92150198d5d8d39
--- /dev/null
+++ b/nmap/nmap__ft_size.html
@@ -0,0 +1,25 @@
+<TITLE>Description of FT_SIZE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword FT_SIZE</H1> 
+
+<DT><EM>Prompt:</EM> FFT size
+<DT><EM>Expected input:</EM> Integer number, 2 values; min.value: 4.000000; max.value: 8192.000000.<P>
+Specify the size of the Fourier transform in the horizontal and vertical 
+directions. Note that for 8k*8k maps the number of points/beam should 
+not be too close to 2 to stay within map size. <P>
+If the size in both direction is &lt;= 17, a Direct Fourier Transform (DFT) will 
+be made instead of the standard operation of interpolating onto a rectangular 
+grid followed by a Fast Fourier Transform (FFT). <P>
+The standard operation suffers from 'aliasing' artefacts associated with the 
+periodic nature of the FFT. These artefacts are suppressed, to a level that is 
+generally acceptable, through a very careful choice of the convolution function 
+used in the interpolstion to a rectangular grid, but they cannot be avoided 
+completely. <P>
+By avoiding the interpolation altogether, the DFT method is free from these 
+aliasing effects. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__grid_size.html b/nmap/nmap__grid_size.html
new file mode 100644
index 0000000000000000000000000000000000000000..affabd6dbe94da6e2866a560b5b0070de0edb71c
--- /dev/null
+++ b/nmap/nmap__grid_size.html
@@ -0,0 +1,19 @@
+<TITLE>Description of GRID_SIZE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword GRID_SIZE</H1> 
+
+<DT><EM>Prompt:</EM> Grid interval in l, m (arcsec)
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.001000; max.value: 180.000000.<P>
+Specify the l and m grid steps in arcseconds for the map to be made. <P>
+In most applications you may define GRID_SIZE as you please. NOTE however, that 
+any number of maps that you want to combine into a single mosaic (FIDDLE MOSCOM 
+option) must all share the same GRID_SIZE (as well as the same reference 
+coordinates, parameters MAP_COORD and REF_COORD) 
+!!      {\em See \textref{MAP_COORD}{.map.coord},  
+!!               \textref{REF_COORD}{.ref.coord} } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__ha_resolution.html b/nmap/nmap__ha_resolution.html
new file mode 100644
index 0000000000000000000000000000000000000000..ce41408f72591e95bce8ec7d0f2e76f0307dedfb
--- /dev/null
+++ b/nmap/nmap__ha_resolution.html
@@ -0,0 +1,19 @@
+<TITLE>Description of HA_RESOLUTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword HA_RESOLUTION</H1> 
+
+<DT><EM>Prompt:</EM> Hour-angle averaging interval (UT seconds)
+<DT><EM>Default:</EM> .50137.
+<DT><EM>Expected input:</EM> Real number; min.value: 0.040000; max.value: 15.000000.<P>
+Specify the width in UT degrees of hour angle over which visibilities will be 
+averaged (to reduce the noise per plotted point). <P>
+Note:   Observations are taken at multiples of 10 UT seconds and it is 
+        therefore convenient to specify this parameter in UT seconds as well. 
+        The number you specify will be converted to a sidereal hour-angle 
+        interval. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__ifr_resolution.html b/nmap/nmap__ifr_resolution.html
new file mode 100644
index 0000000000000000000000000000000000000000..782ec6f8cedee0e6e660603209e12a9e9b05c009
--- /dev/null
+++ b/nmap/nmap__ifr_resolution.html
@@ -0,0 +1,13 @@
+<TITLE>Description of IFR_RESOLUTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword IFR_RESOLUTION</H1> 
+
+<DT><EM>Prompt:</EM> Interferometer separation
+<DT><EM>Expected input:</EM> Real number; min.value: 0.100000; max.value: 16.000000.<P>
+Specify the vertical separation in grid points between interferometers <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__input_file.html b/nmap/nmap__input_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..fc9bda7c40f76812bc270ac249578a6ef46158c4
--- /dev/null
+++ b/nmap/nmap__input_file.html
@@ -0,0 +1,13 @@
+<TITLE>Description of INPUT_FILE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword INPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> Input file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (including extension) of the file to be converted. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__input_labels.html b/nmap/nmap__input_labels.html
new file mode 100644
index 0000000000000000000000000000000000000000..09384fb250f79af96d220fde139ed48a924ad8cd
--- /dev/null
+++ b/nmap/nmap__input_labels.html
@@ -0,0 +1,23 @@
+<TITLE>Description of INPUT_LABELS (NMAP)</TITLE>
+<H1>Program NMAP: private keyword INPUT_LABELS</H1> 
+
+<DT><EM>Prompt:</EM> Input tape labels
+<DT><EM>Expected input:</EM> Integer number, 256 values.<P>
+Specify the tape labels to be read. * specifies all labels on the tape. <P>
+Remember that WMP-file images are identified by indices grp.obs.fld.chn.seq). 
+Each of the selected tape labels will be stored in the WMP-file as a separate 
+field (FLD) in the group (GRP) being created. The CHN, POL and TYP indices will 
+reflect the nature of the input data, SEQ will be 0. <P>
+Example: 
+        INPUT_LABELS=3, 6, 8 will cause a new GRP to be created in which these 
+labels will be stored under the image indices <P>
+        &lt;newgrp&gt;. 0. &lt;chn for label 3&gt;. &lt;pol for label 3&gt;. &lt;typ for label 3&gt;. 0 
+        &lt;newgrp&gt;. 1. &lt;chn for label 6&gt;. &lt;pol for label 6&gt;. &lt;typ for label 6&gt;. 0 
+        &lt;newgrp&gt;. 2. &lt;chn for label 8&gt;. &lt;pol for label 8&gt;. &lt;typ for label 8&gt;. 0 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__lm_centre.html b/nmap/nmap__lm_centre.html
new file mode 100644
index 0000000000000000000000000000000000000000..d786a3cd464b0e65ffe0b424917f84bfa9aa3749
--- /dev/null
+++ b/nmap/nmap__lm_centre.html
@@ -0,0 +1,15 @@
+<TITLE>Description of LM_CENTRE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword LM_CENTRE</H1> 
+
+<DT><EM>Prompt:</EM> Output map centre
+<DT><EM>Expected input:</EM> Double precision number, 2 values.<P>
+Specify the centre of the output map in the l and m direction; in arcsec with 
+respect to the mosaic reference position. <P>
+If you specify an *, you will prompted for RA, DEC position <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__load_option.html b/nmap/nmap__load_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..7c3f768c3677899fd41a4e9a8ec34c63421b6fbc
--- /dev/null
+++ b/nmap/nmap__load_option.html
@@ -0,0 +1,22 @@
+<TITLE>Description of LOAD_OPTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword LOAD_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> WMP, UNLOAD; NEWHOLOG, [OLDHOLOG]; QUIT Load action/image type |
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify the type of foreign map and what to do with it: <P>
+        WMP      read WMP format maps from contiguous binary file 
+        UNLOAD   inverse of WMP: write WMP maps to contiguous binary file 
+                  this option can also be used to load in an SAOIMAGE file 
+                  (specify a data offset of 512) <P>
+        NEWHOLOG read HOLOG file from the WSRT (this option, synonymous with 
+                  WMP, was added to help the user) 
+        OLDHOLOG read a Holog map in old IBM-coded format (this option used to 
+                  be called HOLOG) <P>
+        QUIT    quit LOADing <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__ly for different.html b/nmap/nmap__ly for different.html
new file mode 100644
index 0000000000000000000000000000000000000000..b5da368eaee4e347a87301be2ff92c30d9ea0280
--- /dev/null
+++ b/nmap/nmap__ly for different.html	
@@ -0,0 +1,13 @@
+<TITLE>Description of ly for different (NMAP)</TITLE>
+<H1>Program NMAP: private keyword ly for different</H1> 
+
+<DT><EM>Prompt:</EM> Make line cube (Yes/No) ?
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want to output the FITS maps in one cube or in separate maps <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__map_coord.html b/nmap/nmap__map_coord.html
new file mode 100644
index 0000000000000000000000000000000000000000..8e74f4b56eb56610e57490f19afba8b94c00fbca
--- /dev/null
+++ b/nmap/nmap__map_coord.html
@@ -0,0 +1,41 @@
+<TITLE>Description of MAP_COORD (NMAP)</TITLE>
+<H1>Program NMAP: private keyword MAP_COORD</H1> 
+
+<DT><EM>Prompt:</EM> Map coordinate system|  B1950_J2000, APPARENT; REFERENCE, AREFERENCE
+<DT><EM>Expected input:</EM> Character(12).<P>
+Specify the coordinate system for the map. <P>
+There are two choices to be made: The first is whether the map is to be made in 
+apparent coordinates for the epoch of the observation or in fixed-epoch 
+coordinates. The latter are fixed for each instrument: B1950 for the WSRT,  
+J2000 for the ATNF. The second choice is whether the 'reference position' for 
+the map must coincide with the fringe-stopping centre or is to be specified by 
+you. <P>
+The reference position is the position at which the map plane is tangent to the 
+celestial sphere; it defines the geometry of the map's (l, m) grid in terms of 
+RA and DEC. <P>
+The reference position is important for mosaic mapping: The FIDDLE/MOSCOM 
+operation that combines mosaic subfields into a single large map will only work 
+if all input maps have the same reference. <P>
+For a single mosaic, the program by default uses the mosaic centre as the 
+reference for all subfield maps. However, if you intend to combine multiple 
+mosaics into a 'super-mosaic', only you can define the common reference centre 
+that will be needed. <P>
+You have the following options for your reply: <P>
+   Reference position defined by the observation (i.e. coinciding with the 
+    fringe stopping centre): <P>
+        B1950_J2000   in epoch coordinates for the epoch defined by the 
+                       instrument with which the observation was made: 
+                        B1950 for the WSRT 
+                        J2000 for the ATNF <P>
+        APPARENT      in apparent coordinates at the time of observation <P>
+   Reference position to be defined by the user through an additional parameter 
+    REF_COORD: <P>
+        REFER         in B1950_J2000 coordinates <P>
+        AREFER        in APPARENT coordinates. Note that this will not work for 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__map_factors.html b/nmap/nmap__map_factors.html
new file mode 100644
index 0000000000000000000000000000000000000000..706a28f95a4575a42c281c8ba427915d86939f73
--- /dev/null
+++ b/nmap/nmap__map_factors.html
@@ -0,0 +1,16 @@
+<TITLE>Description of MAP_FACTORS (NMAP)</TITLE>
+<H1>Program NMAP: private keyword MAP_FACTORS</H1> 
+
+<DT><EM>Prompt:</EM> Input-map multipliers
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the factors by which the input maps have to be multiplied. <P>
+You may specify up to 8 factors which will be used as multipliers in the 
+weighted summation the input maps you selected. If there are more maps to be 
+summed than factors specified, the factors will be cyclically re-used.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__map_level.html b/nmap/nmap__map_level.html
new file mode 100644
index 0000000000000000000000000000000000000000..7015b4670f0bef3e26b15f8b61bea959b644b812
--- /dev/null
+++ b/nmap/nmap__map_level.html
@@ -0,0 +1,15 @@
+<TITLE>Description of MAP_LEVEL (NMAP)</TITLE>
+<H1>Program NMAP: private keyword MAP_LEVEL</H1> 
+
+<DT><EM>Prompt:</EM> Polarisation threshold (W.U)
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the minimum level in Wetsrebork Units that is still to be considered 
+valid linear polarisation. Polarisation levels below this threshold will be set 
+to zero in the output map(s). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__map_polar.html b/nmap/nmap__map_polar.html
new file mode 100644
index 0000000000000000000000000000000000000000..8f131c14b1eaed1ec6b6e68b808af4f347a3d06e
--- /dev/null
+++ b/nmap/nmap__map_polar.html
@@ -0,0 +1,27 @@
+<TITLE>Description of MAP_POLAR (NMAP)</TITLE>
+<H1>Program NMAP: private keyword MAP_POLAR</H1> 
+
+<DT><EM>Prompt:</EM> Select 1 to 4 output-map polarisation(s)| XX, XY, YX, YY; I, L, Q, U, V; XXI, XYI, YXI, YYI; II, LI, QI, UI, VI
+<DT><EM>Default:</EM> XX.
+<DT><EM>Expected input:</EM> Character(4), 4 values.<P>
+Specify up to four polarisations for the maps to make: <P>
+        XX      XX only 
+        XY      XY only 
+        YX      YX only 
+        YY      YY only <P>
+        I       Stokes I 
+        L       'line' Stokes I: Incomplete input data (e.g. no valid XX or YY) 
+                 will be filled in aassuming that the field is unpolarised 
+                 (Q=U=V=0) 
+        Q       Stokes Q 
+        U       Stokes U 
+        V       Stokes V <P>
+Each of the above may be suffixed with 'I' to indicate that visibilities must 
+be pre-multiplied with sqrt(-1) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__memory_use.html b/nmap/nmap__memory_use.html
new file mode 100644
index 0000000000000000000000000000000000000000..eea0f17900f395f4f40d1b6bb3295793214ca119
--- /dev/null
+++ b/nmap/nmap__memory_use.html
@@ -0,0 +1,14 @@
+<TITLE>Description of MEMORY_USE (NMAP)</TITLE>
+<H1>Description of general keyword MEMORY_USE</H1>
+
+<DT><EM>Prompt:</EM> Work memory size
+<DT><EM>Default:</EM> 200000 /NOASK.
+<DT><EM>Expected input:</EM> Integer number; min.value: 20000.000000; max.value: 4000000.000000.<P>
+Specify an approximate value for the work memory size to be used in the 
+transform (bytes). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__old_dattyp.html b/nmap/nmap__old_dattyp.html
new file mode 100644
index 0000000000000000000000000000000000000000..2ca1802e64f379c1221ee1f77af8cef49c3eab01
--- /dev/null
+++ b/nmap/nmap__old_dattyp.html
@@ -0,0 +1,22 @@
+<TITLE>Description of OLD_DATTYP (NMAP)</TITLE>
+<H1>Program NMAP: private keyword OLD_DATTYP</H1> 
+
+<DT><EM>Prompt:</EM> Old R-series data format
+<DT><EM>Expected input:</EM> Integer number.<P>
+Specify the old R-series data type: <P>
+        0       local 
+        1       VAX, D_FORMAT 
+        2       VAX, G_FORMAT 
+        3       ALLIANT 
+        4       CONVEX 
+        5       IEEE 
+        6       DEC station 
+        7       SUN station 
+        8       HP  station <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__option.html b/nmap/nmap__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..63979d36c3f77b17842b8682567bde45d36b257f
--- /dev/null
+++ b/nmap/nmap__option.html
@@ -0,0 +1,31 @@
+<TITLE>Description of OPTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Action| MAKE, FIDDLE; W16FITS, W32FITS, WRLFITS, RFITS; SHOW; QUIT;|-[FROM_OLD, TO_OLD, CVX, NVS]
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform: <P>
+  Primary operations: 
+        MAKE      make map(s) from visibility data in .SCN file 
+        FIDDLE    combine or change maps in .WMP file <P>
+  FITS conversions: 
+        W16FITS   write FITS tape/disk with 16 bits data 
+        W32FITS   write FITS tape/disk with 32 bits data 
+        WRLFITS   write FITS tape/disk with 32 bits float data 
+        RFITS     read FITS tape/disk data <P>
+  Miscellaneous: 
+        SHOW      show/edit map data 
+        QUIT      finish <P>
+  Format conversions: 
+        CVX       convert a map file from other machine's format to local 
+                   machine's 
+        NVS       convert a map file to newest version. Needs to be run only if 
+                   indicated by program 
+        FROM_OLD  convert from R-series format 
+        TO_OLD    convert to R-series format  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__out_centre.html b/nmap/nmap__out_centre.html
new file mode 100644
index 0000000000000000000000000000000000000000..639f42f8edc35274b921929215a82cf53fa21fa3
--- /dev/null
+++ b/nmap/nmap__out_centre.html
@@ -0,0 +1,15 @@
+<TITLE>Description of OUT_CENTRE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword OUT_CENTRE</H1> 
+
+<DT><EM>Prompt:</EM> Output map centre
+<DT><EM>Expected input:</EM> Integer number, 2 values.<P>
+Specify the centre of the output map in the l and m direction in pixels with 
+respect to the mosaic reference position. <P>
+If you specify an *, you will be prompted for l, m and RA, DEC position <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__out_size.html b/nmap/nmap__out_size.html
new file mode 100644
index 0000000000000000000000000000000000000000..f7b8e189598fc11edf96903277bd379cf9384e45
--- /dev/null
+++ b/nmap/nmap__out_size.html
@@ -0,0 +1,14 @@
+<TITLE>Description of OUT_SIZE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword OUT_SIZE</H1> 
+
+<DT><EM>Prompt:</EM> Output map size
+<DT><EM>Expected input:</EM> Integer number, 2 values; min.value: 16.000000; max.value: 16384.000000.<P>
+Specify the size in grid points of the output map(s) in the horizontal and 
+vertical directions. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__output.html b/nmap/nmap__output.html
new file mode 100644
index 0000000000000000000000000000000000000000..f4ba4e78530cfc67703db4edc182ec9c25d11888
--- /dev/null
+++ b/nmap/nmap__output.html
@@ -0,0 +1,22 @@
+<TITLE>Description of OUTPUT (NMAP)</TITLE>
+<H1>Program NMAP: private keyword OUTPUT</H1> 
+
+<DT><EM>Prompt:</EM> MAP, AP; COVER; REAL, IMAG, AMPL, PHASE
+<DT><EM>Expected input:</EM> Character(8), 8 values.<P>
+Specify one or more output types: <P>
+   Standard image types for map-making: 
+        MAP     Output (a) map(s) 
+        AP      Output (an) antenna pattern(s) <P>
+   Visibility-domain outputs, for diagnostics only: 
+        COVER   Output the 'antenna-pattern' convolved visibilities <P>
+        REAL    Output the real part of the convolved visibilities 
+        IMAG    Output the imaginary part of the convolved visibilities <P>
+        AMPL    Output the amplitude of the convolved visibilities 
+        PHASE   Output the phase of the convolved visibilities <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__output_label.html b/nmap/nmap__output_label.html
new file mode 100644
index 0000000000000000000000000000000000000000..17df4301925c853fb86a8af0ccc603c09ac5020d
--- /dev/null
+++ b/nmap/nmap__output_label.html
@@ -0,0 +1,15 @@
+<TITLE>Description of OUTPUT_LABEL (NMAP)</TITLE>
+<H1>Program NMAP: private keyword OUTPUT_LABEL</H1> 
+
+<DT><EM>Prompt:</EM> Output label
+<DT><EM>Expected input:</EM> Integer number.<P>
+Specify the first output tape label. If this label already exists, it and all 
+the subsequent labels will be overwritten. <P>
+Specify * or 0 to write the new label behind all existing ones. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__qdatas.html b/nmap/nmap__qdatas.html
new file mode 100644
index 0000000000000000000000000000000000000000..0de48d05af72c8b55d78f50161fdfd326234c565
--- /dev/null
+++ b/nmap/nmap__qdatas.html
@@ -0,0 +1,24 @@
+<TITLE>Description of QDATAS (NMAP)</TITLE>
+<H1>Program NMAP: private keyword QDATAS</H1> 
+
+<DT><EM>Prompt:</EM> Special data selection (Yes/No) ?
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Logical.<P>
+Maps are normally made directly from the .SCN-file visibilities. Answering YES 
+here gives you access to some specials including <P>
+
+<DT>        - making a map from model visibilities in the .SCN file; 
+
+<DT>        - selecting visibilities from an annulus in the UV plane; 
+
+<DT>        - clipping extreme amplitudes in an annulus in the UV plane; 
+
+<DT>        - shifting the pointing centre to which the visibilities refer (and 
+           consequently the centre of the map to be made from them). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__qmaps.html b/nmap/nmap__qmaps.html
new file mode 100644
index 0000000000000000000000000000000000000000..b29cca66496ff84de9af5de4c9084ef6752a1841
--- /dev/null
+++ b/nmap/nmap__qmaps.html
@@ -0,0 +1,18 @@
+<TITLE>Description of QMAPS (NMAP)</TITLE>
+<H1>Description of general keyword QMAPS</H1>
+
+<DT><EM>Prompt:</EM> UV taper/convolution details?
+<DT><EM>Default:</EM> NO.
+<DT><EM>Expected input:</EM> Logical.<P>
+The standard defaults used for the taper and convolution functions in the 
+map-making process will produce maps of excellent quality for normal 
+applications at an acceptable expense of computing resources. <P>
+There may be particular situations, however, where a non-standard taper and/or 
+convolution function is more suitable. Answer YES if you want to make your own 
+selection out of the possible options. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__radec_centre.html b/nmap/nmap__radec_centre.html
new file mode 100644
index 0000000000000000000000000000000000000000..bf5f755f7d241315618c96a2f9c1208a11431d80
--- /dev/null
+++ b/nmap/nmap__radec_centre.html
@@ -0,0 +1,13 @@
+<TITLE>Description of RADEC_CENTRE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword RADEC_CENTRE</H1> 
+
+<DT><EM>Prompt:</EM> Output map centre: RA, DEC (decimal deg)
+<DT><EM>Expected input:</EM> Double precision number, 2 values.<P>
+Specify the centre of the output map: RA and DEC in decimal degrees. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__ref_coord.html b/nmap/nmap__ref_coord.html
new file mode 100644
index 0000000000000000000000000000000000000000..331c4eab5029775cbedee882fdf592758d7bdf2f
--- /dev/null
+++ b/nmap/nmap__ref_coord.html
@@ -0,0 +1,15 @@
+<TITLE>Description of REF_COORD (NMAP)</TITLE>
+<H1>Program NMAP: private keyword REF_COORD</H1> 
+
+<DT><EM>Prompt:</EM> Map reference coordinates: RA, DEC (decimal deg)
+<DT><EM>Expected input:</EM> Double precision number, 2 values.<P>
+Specify (in decimal degrees) the RA and DEC of the reference coordinates to use 
+in producing the map. The coordinate system is B1950/J2000 or apparent as 
+defined by your value for parameter MAP_COORD.   <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__rotation_measure.html b/nmap/nmap__rotation_measure.html
new file mode 100644
index 0000000000000000000000000000000000000000..e1887fd1bf85a88bccb1fa4078c6cd6ce0bf046e
--- /dev/null
+++ b/nmap/nmap__rotation_measure.html
@@ -0,0 +1,20 @@
+<TITLE>Description of ROTATION_MEASURE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword ROTATION_MEASURE</H1> 
+
+<DT><EM>Prompt:</EM> Rotation measure
+<DT><EM>Expected input:</EM> Real number, 512 values.<P>
+Specify one (or more) rotation measure(s) (RM). Pairs of input maps will be 
+phase-rotated to the the frequency of the first input map and averaged: <P>
+    THETAn = 2 * RM * ( (c/FRQn)**2 -  (c/FRQ1)**2 ) <P>
+    Qout = SUM( Wn * ( cos(THETAn)*Qn - sin(THETAn)*Un ) ) / SUM( Wn ) 
+    Uout = SUM( Wn * ( sin(THETAn)*Qn + cos(THETAn)*Un ) ) / SUM( Wn ) <P>
+A pair of Qout/Uout will be produced for each RM given. E.g. to get average Q/U 
+maps for rotation measures from 0 to 5 with intervals of 0.5, specify 
+ROTATION_MEASURE=0 TO 5 BY 0.5. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__subtract.html b/nmap/nmap__subtract.html
new file mode 100644
index 0000000000000000000000000000000000000000..c42a7b63a0710b8bd77c4eb380a90d576b5851a1
--- /dev/null
+++ b/nmap/nmap__subtract.html
@@ -0,0 +1,15 @@
+<TITLE>Description of SUBTRACT (NMAP)</TITLE>
+<H1>Program NMAP: private keyword SUBTRACT</H1> 
+
+<DT><EM>Prompt:</EM> Model subtraction (Yes/No) ?
+<DT><EM>Expected input:</EM> Logical.<P>
+Reply YES if you want to subtract a source model. You will then be prompted to 
+provide details on the model you want to subtract. 
+! {\em see the \textref{NMODEL HANDLE}{nmodel_public_intfc} interface } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__sum_factors.html b/nmap/nmap__sum_factors.html
new file mode 100644
index 0000000000000000000000000000000000000000..84aec4cf7cee90bec54ec8363a94b4f226cc4c90
--- /dev/null
+++ b/nmap/nmap__sum_factors.html
@@ -0,0 +1,20 @@
+<TITLE>Description of SUM_FACTORS (NMAP)</TITLE>
+<H1>Program NMAP: private keyword SUM_FACTORS</H1> 
+
+<DT><EM>Prompt:</EM> Summing multipliers
+<DT><EM>Expected input:</EM> Real number, 8 values.<P>
+Specify up to 8 weight factors by which the input maps have to be multiplied. 
+If the number of weights you give is less than the number of maps to be 
+combined, the weights will re-used in a cyclic fashion. <P>
+Example: 
+        1, -1 will average the first, third, ... maps in your WMP_SETS 
+specification with the negated second, fourth ... maps. <P>
+Note: When used together with the RSUM option, the weights will be used both 
+for the Real and Imaginary map (they are real weights). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__sum_option.html b/nmap/nmap__sum_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..e016ccbc505babcf5373427ed065e6d3a76f282e
--- /dev/null
+++ b/nmap/nmap__sum_option.html
@@ -0,0 +1,22 @@
+<TITLE>Description of SUM_OPTION (NMAP)</TITLE>
+<H1>Program NMAP: private keyword SUM_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> SUM, NSUM, NSSUM, BSUM, BNSUM, FSUM; QUIT Weighing method
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify the type of weight to use in the averaging. In all cases the summation 
+produces a weighted average map over all SETS_1, the weights depending on the 
+method you select: <P>
+        SUM     weight(i)= 1 
+        NSUM    weight(i)= normalisation factor of map(i) 
+        NSSUM   weight(i)= 1 / (&lt;noise in map(i)&gt;**2) <P>
+        BSUM    weight(i)= bandwidth of map(i) 
+        BNSUM   weight(i)= bandwidth * normalisation factor of map(i) <P>
+        FSUM    weight(i)= factors to be specified by you. <P>
+        QUIT    quit AVERaging <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__taper.html b/nmap/nmap__taper.html
new file mode 100644
index 0000000000000000000000000000000000000000..8e1b5e86cc3fab4f51b6e47da9e92f746f024ee3
--- /dev/null
+++ b/nmap/nmap__taper.html
@@ -0,0 +1,33 @@
+<TITLE>Description of TAPER (NMAP)</TITLE>
+<H1>Program NMAP: private keyword TAPER</H1> 
+
+<DT><EM>Prompt:</EM> GAUSS, LINEAR, OVERR, RGAUSS, NATURAL Taper type
+<DT><EM>Expected input:</EM> Character(8).<P>
+The taper is a function of baseline length used to de-emphasize the long 
+baselines and consequently reduce the near-in sidelobes of the synthesized beam. <P>
+You may specify the following functions, some of them to be supplemented later 
+with a baseline-scale parameter TAPER_VALUE: <P>
+! {\em see public parameter 
+!  \textref{TAPER_VALUE}{nmap_public_intfc.taper.value} } <P>
+        GAUSS    exp -(&lt;baseline&gt;/TAPER_VALUE)**2 
+                 standard WSRT beam: good compromise between near-in sidelobes,  
+                  beam width and noise <P>
+        LINEAR   max (0, 1-baseline/TAPER_VALUE) <P>
+        OVERR    1 / baseline   (no scale) <P>
+        RGAUSS   exp -(&lt;baseline&gt;/TAPER_VALUE)**2 / &lt;baseline&gt; 
+                 broader beam, very low near-in sidelobes, poorer noise <P>
+        NATURAL  no taper       (no scale) 
+                 optimum signal/noise ratio, narrower beam with very strong 
+                  near-in sidelobes <P>
+NOTES: - Unless you have specified UNIFORM=NATURAL for the UV coverage mode, the 
+        1/&lt;baseline&gt; density variation of measured visibility points is already 
+        being accounted for, so OVERR and RGAUSS should not be chosen. LINEAR 
+        does not combine very well with NATURAL either. <P>
+! {\em cf. parameter \textref{UNIFORM}{nmap_public_intfc.uniform} } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__taper_value.html b/nmap/nmap__taper_value.html
new file mode 100644
index 0000000000000000000000000000000000000000..35b7b981bc13944a78cfe49254cf2b26d2279bea
--- /dev/null
+++ b/nmap/nmap__taper_value.html
@@ -0,0 +1,15 @@
+<TITLE>Description of TAPER_VALUE (NMAP)</TITLE>
+<H1>Description of general keyword TAPER_VALUE</H1>
+
+<DT><EM>Prompt:</EM> Taper half-width (metres)
+<DT><EM>Expected input:</EM> Real number; min.value: 10.000000.<P>
+Specify the baseline in metres of the taper function at which the taper 
+function will fall to 1/e of its central value. <P>
+The default is defined such that the taper function you selected has a value of 
+1/4 for a baseline length of 3000 m. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__uniform.html b/nmap/nmap__uniform.html
new file mode 100644
index 0000000000000000000000000000000000000000..0388a9ff0aecc5879a2cd561d9403505fe124cf7
--- /dev/null
+++ b/nmap/nmap__uniform.html
@@ -0,0 +1,29 @@
+<TITLE>Description of UNIFORM (NMAP)</TITLE>
+<H1>Description of general keyword UNIFORM</H1>
+
+<DT><EM>Prompt:</EM> NATURAL, STANDARD, FULL Measure function for UV coverage
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify the way the UV coverage should be determined: <P>
+	STANDARD: Weigh each observed point with the track length it covers in 
+		   the UV plane, and average sets of redundant baselines. This 
+		   method accounts properly for the fact that the density of 
+		   measured points is inversely proportional to the baseline,  
+		   for the multiplicity of redundant baselines and for 
+		   variations in integration times. <P>
+	FULL:     Weigh each point according to the actual UV point density. In 
+		   this case care is also taken of all local UV plane density 
+		   enhancements, e.g. because there is overlap between 
+		   observations. <P>
+	NATURAL:  Take each individual measured point separately, without 
+		   weighing for the UV track covered by it. This option gives 
+		   the maximum possible signal/noise ratio in your map, but it 
+		   generally weighs the short baselines much too heavily which 
+		   results in a very fat synthesized beam. <P>
+Of these options, FULL gives the cleanest synthesized beam, but it is slower 
+because it necessitates an extra read pass over the .SCN-file data. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__use_noise.html b/nmap/nmap__use_noise.html
new file mode 100644
index 0000000000000000000000000000000000000000..1c8a246ffb418622d7f7dd9b11f82f58b000eeae
--- /dev/null
+++ b/nmap/nmap__use_noise.html
@@ -0,0 +1,14 @@
+<TITLE>Description of USE_NOISE (NMAP)</TITLE>
+<H1>Program NMAP: private keyword USE_NOISE</H1> 
+
+<DT><EM>Prompt:</EM> Weigh with noise (Yes/No) ?
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want the noise of the individual maps to be used as a weight in 
+the MOSCOM combination <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__user_comment.html b/nmap/nmap__user_comment.html
new file mode 100644
index 0000000000000000000000000000000000000000..93f6f72e77e356bbb6f56b30efbcb584cb7ea241
--- /dev/null
+++ b/nmap/nmap__user_comment.html
@@ -0,0 +1,13 @@
+<TITLE>Description of USER_COMMENT (NMAP)</TITLE>
+<H1>Program NMAP: private keyword USER_COMMENT</H1> 
+
+<DT><EM>Prompt:</EM> Comment to be included in map header(s) (&lt;=24 chars)|
+<DT><EM>Expected input:</EM> Character(24).<P>
+Give, optionally, a descriptive comment for the maps. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__user_data.html b/nmap/nmap__user_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..149784b43fc5cc2057095438a4d25172c335df0d
--- /dev/null
+++ b/nmap/nmap__user_data.html
@@ -0,0 +1,16 @@
+<TITLE>Description of USER_DATA (NMAP)</TITLE>
+<H1>Program NMAP: private keyword USER_DATA</H1> 
+
+<DT><EM>Prompt:</EM> STANDARD, MODEL Visibilities to use
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify the type of visibilities to use: <P>
+        STANDARD  observed visibilities <P>
+        MODEL     model visibilities (to be specified later with type=0 
+sources)  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__uv_area.html b/nmap/nmap__uv_area.html
new file mode 100644
index 0000000000000000000000000000000000000000..cd89e1706a92a06814733dee4fc3bcbf14902715
--- /dev/null
+++ b/nmap/nmap__uv_area.html
@@ -0,0 +1,25 @@
+<TITLE>Description of UV_AREA (NMAP)</TITLE>
+<H1>Description of general keyword UV_AREA</H1>
+
+<DT><EM>Prompt:</EM> projected UV radius range (metres)
+<DT><EM>Default:</EM> 0., 100000..
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.000000.<P>
+Specify the range of PROJECTED baselines for which you want to include the data. <P>
+You may use this option, - at the expense of throwing away data -, for such 
+purposes as <P>
+
+<DT>	- To make the projected synthesised aperture and hence the synthesised 
+	   beam somewhat more circularly symmetric. <P>
+
+<DT>	- To exclude noise from long projected baselines where you know there is 
+	   no signal of interest. <P>
+
+<DT>	- To eliminate data from the short baselines, e.g. to suppress 
+	   interference. <P>
+The default is not to eliminate any baselines. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_comm.html">List of general keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__uv_coordinates.html b/nmap/nmap__uv_coordinates.html
new file mode 100644
index 0000000000000000000000000000000000000000..9e0f69cf4a76245fb75c8e0cb9a09c1124349d0a
--- /dev/null
+++ b/nmap/nmap__uv_coordinates.html
@@ -0,0 +1,20 @@
+<TITLE>Description of UV_COORDINATES (NMAP)</TITLE>
+<H1>Program NMAP: private keyword UV_COORDINATES</H1> 
+
+<DT><EM>Prompt:</EM> UV coordinate system UV, BASHA, IFRHA
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify the type of UV coordinates wanted for UV-plane type output 
+! {\em \textref{OUTPUT}{.output}: COVER, REAL, IMAG, AMPL, PHASE options } <P>
+        UV      standard UV coordinates: interferometer tracks are ellipses <P>
+        BASHA   hour-angle (horizontal) and interferometer baseline (vertical) 
+                 coordinates: interferometer tracks are horizontal lines; 
+                 redundant baselines overlap <P>
+        IFRHA   as BASHA, but vertical axis is the interferometer ordinal number 
+                 in the sequence 01, 02, ..., 0D, 12, 13, ..., CD) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__wgt_limit.html b/nmap/nmap__wgt_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..fd949e70bd22c58a251d7054d7f041cf87b06c2d
--- /dev/null
+++ b/nmap/nmap__wgt_limit.html
@@ -0,0 +1,14 @@
+<TITLE>Description of WGT_LIMIT (NMAP)</TITLE>
+<H1>Program NMAP: private keyword WGT_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Relative weight limit
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000; max.value: 1.000000.<P>
+Specifies the relative weight as compared to the expected maximum weight of 
+data points combined on one line, below which no output will be generated <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__wmp_node_1.html b/nmap/nmap__wmp_node_1.html
new file mode 100644
index 0000000000000000000000000000000000000000..e61f7035bdc7e5d9d739b9f4527294361fd768c4
--- /dev/null
+++ b/nmap/nmap__wmp_node_1.html
@@ -0,0 +1,13 @@
+<TITLE>Description of WMP_NODE_1 (NMAP)</TITLE>
+<H1>Program NMAP: private keyword WMP_NODE_1</H1> 
+
+<DT><EM>Prompt:</EM> First WMP node name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the node name for the first Fiddle input set of images. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__wmp_node_2.html b/nmap/nmap__wmp_node_2.html
new file mode 100644
index 0000000000000000000000000000000000000000..82d895b166659d77a3c705b4bb7512e2cd1e1660
--- /dev/null
+++ b/nmap/nmap__wmp_node_2.html
@@ -0,0 +1,14 @@
+<TITLE>Description of WMP_NODE_2 (NMAP)</TITLE>
+<H1>Program NMAP: private keyword WMP_NODE_2</H1> 
+
+<DT><EM>Prompt:</EM> Second WMP node name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the node name for the second Fiddle input set of images. <P>
+Specify * if this is the same as the first node (NODE_1). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__wmp_set_1.html b/nmap/nmap__wmp_set_1.html
new file mode 100644
index 0000000000000000000000000000000000000000..aa71453f3c53a2ff1822f431baeb145c61350107
--- /dev/null
+++ b/nmap/nmap__wmp_set_1.html
@@ -0,0 +1,13 @@
+<TITLE>Description of WMP_SET_1 (NMAP)</TITLE>
+<H1>Program NMAP: private keyword WMP_SET_1</H1> 
+
+<DT><EM>Prompt:</EM> First image set(s) to be used: grp.fld.chn.pol.typ.seq
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+Specify the first image set(s) to be used. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap/nmap__wmp_set_2.html b/nmap/nmap__wmp_set_2.html
new file mode 100644
index 0000000000000000000000000000000000000000..30f53f6d1bb69ecfa77b775053ce923f2ef8a578
--- /dev/null
+++ b/nmap/nmap__wmp_set_2.html
@@ -0,0 +1,13 @@
+<TITLE>Description of WMP_SET_2 (NMAP)</TITLE>
+<H1>Program NMAP: private keyword WMP_SET_2</H1> 
+
+<DT><EM>Prompt:</EM> Second image set(s) to be used: grp.fld.chn.pol.typ.seq
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+Specify the second image Set(s) to be used <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmap/nmap_keys.html">List of keywords</A> for NMAP
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmap_comm/nmap_comm.html b/nmap_comm/nmap_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..0101baf396e95874c146ebc2eedb666bef0d9688
--- /dev/null
+++ b/nmap_comm/nmap_comm.html
@@ -0,0 +1,32 @@
+<TITLE>Index of general keywords from NMAP</TITLE>
+<H1>Description of general keywords (NMAP)</H1>
+
+<UL>
+<LI> <A HREF="../nmap/nmap__memory_use.html">
+  MEMORY_USE</A>
+  Work memory size
+<LI> <A HREF="../nmap/nmap__qmaps.html">
+  QMAPS</A>
+  UV taper/convolution details?
+<LI> <A HREF="../nmap/nmap__uniform.html">
+  UNIFORM</A>
+  NATURAL, STANDARD, FULL Measure function for UV coverage
+<LI> <A HREF="../nmap/nmap__taper_value.html">
+  TAPER_VALUE</A>
+  Taper half-width (metres)
+<LI> <A HREF="../nmap/nmap__cweight_type.html">
+  CWEIGHT_TYPE</A>
+  GAUSS, LINEAR, NATURAL Circular weight type
+<LI> <A HREF="../nmap/nmap__cweight_value.html">
+  CWEIGHT_VALUE</A>
+  Circular-weight width (metres)
+<LI> <A HREF="../nmap/nmap__uv_area.html">
+  UV_AREA</A>
+  projected UV radius range (metres)
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
diff --git a/nmap_descr.ps b/nmap_descr.ps
new file mode 100644
index 0000000000000000000000000000000000000000..2b8be015cf90525a288c36bfecbcefb2c22003ef
--- /dev/null
+++ b/nmap_descr.ps
@@ -0,0 +1,2027 @@
+%!PS-Adobe-2.0
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x80,0x11,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x81,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x19,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x18,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00};
diff --git a/nmap_descr/_10703_tex2html_wrap346.png b/nmap_descr/_10703_tex2html_wrap346.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d6996a744e2c6f126ad0d9a3495b6658489988d
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap346.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap346.xbm b/nmap_descr/_10703_tex2html_wrap346.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e5f0f4cd1d9a0eae65fa433649536345af2ee38a
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap346.xbm
@@ -0,0 +1,6 @@
+#define noname_width 31
+#define noname_height 10
+static char noname_bits[] = {
+ 0x10,0x00,0x00,0x10,0x18,0x00,0x00,0x18,0x18,0x00,0x00,0x18,0x1c,0x10,0x06,
+ 0x1c,0x16,0x30,0x03,0x16,0x12,0xe0,0x01,0x12,0x13,0xc0,0x00,0x13,0x7f,0xe0,
+ 0x01,0x7f,0x10,0x30,0x03,0x10,0x7c,0x10,0x06,0x7c};
diff --git a/nmap_descr/_10703_tex2html_wrap350.png b/nmap_descr/_10703_tex2html_wrap350.png
new file mode 100644
index 0000000000000000000000000000000000000000..147866ceaf288f5fde8a3b7f172fa276e19c1bac
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap350.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap350.xbm b/nmap_descr/_10703_tex2html_wrap350.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..c3e7243ef7b816b76d7ec3b2d4e029db25e0c29a
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap350.xbm
@@ -0,0 +1,6 @@
+#define noname_width 30
+#define noname_height 11
+static char noname_bits[] = {
+ 0x18,0x00,0x00,0x18,0x3c,0x00,0x00,0x3c,0x36,0x00,0x00,0x36,0x02,0x10,0x06,
+ 0x02,0x1f,0x30,0x03,0x1f,0x33,0xe0,0x01,0x33,0x23,0xc0,0x00,0x23,0x23,0xe0,
+ 0x01,0x23,0x32,0x30,0x03,0x32,0x36,0x10,0x06,0x36,0x1c,0x00,0x00,0x1c};
diff --git a/nmap_descr/_10703_tex2html_wrap352.png b/nmap_descr/_10703_tex2html_wrap352.png
new file mode 100644
index 0000000000000000000000000000000000000000..9e9df04499734988eb9c194a495fd6c57e762cc8
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap352.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap352.xbm b/nmap_descr/_10703_tex2html_wrap352.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e91af29cbdb1ca1dbeadfbae67c2274796bd52e4
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap352.xbm
@@ -0,0 +1,10 @@
+#define noname_width 63
+#define noname_height 13
+static char noname_bits[] = {
+ 0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x30,0x00,
+ 0x00,0x00,0xbc,0xf3,0xe3,0x81,0x19,0x78,0x77,0x3f,0xf6,0x7b,0xb3,0x01,0x0f,
+ 0xcc,0x1e,0x66,0x9e,0x31,0x1b,0x00,0x06,0xfc,0x1c,0x46,0xbe,0x31,0x1b,0x00,
+ 0x0f,0x0c,0x1c,0x46,0x93,0xb3,0x9d,0x81,0x19,0x8c,0x36,0x66,0x9f,0xb3,0xf3,
+ 0x80,0x30,0x78,0x77,0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0f};
diff --git a/nmap_descr/_10703_tex2html_wrap356.png b/nmap_descr/_10703_tex2html_wrap356.png
new file mode 100644
index 0000000000000000000000000000000000000000..3f59711c0aa9d5223483bfc68bd8e6148c7b7586
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap356.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap356.xbm b/nmap_descr/_10703_tex2html_wrap356.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..be628063cf682a2990fd0030c0419cc0dfb62f52
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap356.xbm
@@ -0,0 +1,7 @@
+#define noname_width 17
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0x01,0x01,0x00,0x01,0x01,0x00,0x01,0x01,0x00,0x01,0x61,0x0c,0x01,
+ 0x61,0x0c,0x01,0xe1,0x0e,0x01,0xc1,0x06,0x01,0xc1,0x06,0x01,0x81,0x07,0x01,
+ 0x81,0x03,0x01,0x81,0x03,0x01,0x81,0x01,0x01,0x81,0x01,0x01,0xe1,0x01,0x01,
+ 0xe1,0x00,0x01,0x01,0x00,0x01,0x01,0x00,0x01,0x01,0x00,0x01,0xff,0xff,0x01};
diff --git a/nmap_descr/_10703_tex2html_wrap358.png b/nmap_descr/_10703_tex2html_wrap358.png
new file mode 100644
index 0000000000000000000000000000000000000000..146b2b77be1883220532d0ed72b48d8e22705473
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap358.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap358.xbm b/nmap_descr/_10703_tex2html_wrap358.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d5a1672872ad6d589ce7d10051342b051dee6c87
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap358.xbm
@@ -0,0 +1,20 @@
+#define noname_width 152
+#define noname_height 13
+static char noname_bits[] = {
+ 0xf8,0x43,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x7f,0x0c,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0x30,0x73,0x00,0x00,0x00,0x00,0x00,0xc0,0x01,0x00,0x00,
+ 0x66,0x36,0x00,0x00,0x00,0x00,0x00,0xd8,0x18,0x42,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x01,0x10,0x00,0x43,0x37,0x00,0x00,0x00,0x00,0x00,0xdc,0x98,0x42,0x80,
+ 0x30,0x00,0x00,0x00,0x00,0x01,0x10,0x00,0x53,0x27,0x10,0x06,0x00,0x00,0x00,
+ 0x9c,0xd8,0x40,0x80,0x19,0xf0,0x3f,0x9e,0x1f,0x01,0x10,0x00,0x1b,0x30,0x30,
+ 0x03,0xff,0xe3,0xf1,0xc3,0xf8,0x40,0x00,0x0f,0x78,0x36,0xdb,0x1b,0x01,0x10,
+ 0x00,0x1f,0x30,0xe0,0x81,0x67,0xb3,0x79,0xc3,0x4c,0x40,0x00,0x06,0x30,0xb3,
+ 0x99,0x19,0x81,0xff,0x81,0x09,0x18,0xc0,0x00,0x33,0x9b,0x31,0x63,0x0c,0x40,
+ 0x00,0x0f,0x30,0xb3,0x99,0x19,0x01,0x10,0x80,0x01,0x2c,0xe0,0x01,0x33,0x9b,
+ 0x31,0xb3,0x0c,0x40,0x80,0x19,0x30,0xdb,0xa9,0x0d,0x01,0x10,0x80,0x01,0x26,
+ 0x30,0x03,0xb3,0x9d,0xb2,0x99,0x1f,0xf0,0x81,0x30,0x30,0x3b,0xbf,0xc7,0x07,
+ 0x10,0xe0,0x03,0x3f,0x10,0x06,0xb3,0xf3,0xf3,0xfc,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xc0,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x3c,0x00};
diff --git a/nmap_descr/_10703_tex2html_wrap360.png b/nmap_descr/_10703_tex2html_wrap360.png
new file mode 100644
index 0000000000000000000000000000000000000000..9d3ff2a4a70977260f78c6e7830751c2a6d3baf9
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap360.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap360.xbm b/nmap_descr/_10703_tex2html_wrap360.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..afacb4d869b712f9b9258fcbb32d48eab3f679fa
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap360.xbm
@@ -0,0 +1,40 @@
+#define noname_width 292
+#define noname_height 15
+static char noname_bits[] = {
+ 0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x00,0x41,0x00,0x00,0x80,0x00,0x00,0x04,0x00,0x00,
+ 0x00,0x00,0x00,0x01,0x00,0x08,0x01,0x84,0x3f,0x04,0x00,0x00,0x00,0x00,0x00,
+ 0x10,0x00,0x00,0xf0,0xc7,0x00,0x00,0x00,0x00,0x00,0x00,0x43,0x00,0x21,0x80,
+ 0x03,0x40,0xf8,0x43,0x08,0x00,0x00,0x00,0x07,0x80,0xf0,0xc7,0x10,0x02,0x06,
+ 0x33,0x07,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,0x60,0x66,0x03,0x00,0x00,
+ 0x00,0x00,0x80,0xcd,0x80,0x31,0x00,0x03,0x60,0x30,0x73,0x18,0x00,0x00,0x00,
+ 0x06,0xc0,0x60,0x66,0x33,0x06,0x82,0x21,0x04,0x00,0x00,0x00,0x00,0x00,0x10,
+ 0x00,0x01,0x30,0x74,0x03,0x00,0x00,0x00,0x00,0xc0,0x8d,0x80,0x11,0x80,0x01,
+ 0x20,0x18,0x42,0x10,0x80,0x00,0x00,0x03,0x40,0x30,0x74,0x23,0x04,0x83,0x29,
+ 0x04,0x08,0x03,0x00,0x00,0x00,0x10,0x00,0x01,0x30,0x75,0x02,0x61,0x00,0x00,
+ 0x00,0xc0,0x89,0x81,0x18,0x80,0x01,0x30,0x98,0x42,0x30,0x80,0x00,0x00,0x03,
+ 0x60,0x30,0x75,0x62,0x0c,0x83,0x0d,0x04,0x98,0x01,0xff,0xe3,0xf9,0x11,0x00,
+ 0x01,0xb0,0x01,0x03,0x33,0xe0,0x7f,0x3c,0x3f,0x8c,0xc1,0x18,0x9e,0xc7,0x33,
+ 0xd8,0x40,0x30,0x80,0x00,0x3c,0x8f,0x67,0xb0,0x01,0x63,0x0c,0x83,0x0f,0x04,
+ 0xf0,0x80,0x67,0xb3,0xbd,0x11,0x00,0x01,0xf0,0x01,0x03,0x1e,0xf0,0x6c,0xb6,
+ 0x37,0x8c,0x41,0x18,0x9b,0x6d,0x33,0xf8,0x40,0x30,0x80,0x00,0x36,0xdb,0x66,
+ 0xf0,0x01,0x63,0x0c,0xc3,0x04,0x04,0x60,0x00,0x33,0x9b,0x99,0x11,0xf8,0x1f,
+ 0x98,0x80,0x01,0x0c,0x60,0x66,0x33,0x33,0x86,0x41,0x98,0xd9,0xec,0x31,0x4c,
+ 0x40,0x30,0xfc,0x0f,0xb3,0xd9,0x63,0x98,0x80,0x61,0x0c,0xc3,0x00,0x04,0xf0,
+ 0x00,0x33,0x9b,0x99,0x11,0x00,0x01,0x18,0xc0,0x02,0x1e,0x60,0x66,0x33,0x33,
+ 0x8b,0x61,0x98,0xd9,0xe4,0x33,0x0c,0x40,0x30,0x80,0x00,0xb3,0xc9,0x67,0x18,
+ 0xc0,0x62,0x0c,0xc3,0x00,0x04,0x98,0x01,0xb3,0x9d,0xda,0x10,0x00,0x01,0x18,
+ 0x60,0x02,0x33,0x60,0xb6,0x53,0x9b,0x89,0x21,0x98,0xe9,0x36,0x31,0x0c,0x40,
+ 0x30,0x80,0x00,0xd3,0x6d,0x62,0x18,0x60,0x62,0x0c,0xf3,0x01,0x1f,0x08,0x03,
+ 0xb3,0xf3,0x7b,0x7c,0x00,0x01,0x3e,0xf0,0x03,0x61,0x60,0x76,0x7e,0xcf,0x8f,
+ 0x31,0x18,0xbf,0xf3,0x31,0x1f,0xf0,0x31,0x80,0x00,0x7e,0xe7,0x63,0x3e,0xf0,
+ 0x63,0x0c,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x80,0x30,0x10,0x00,0x00,0x20,0x00,0x00,0x10,
+ 0x80,0x00,0x00,0x00,0x40,0x00,0x00,0x20,0x04,0x06,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x0c,0x00,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0xc0,0x10,
+ 0x30,0x00,0x00,0x60,0x00,0x00,0x18,0x80,0x00,0x00,0x00,0xc0,0x00,0x00,0x30,
+ 0x06,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xc0,0x03,0xc0,0x18,0x30,0x00,0x00,0x60,0x00,0x00,0x18,0x00,
+ 0x00,0x00,0x00,0xc0,0x00,0x00,0x30,0x06,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x18,0x60,
+ 0x00,0x00,0xc0,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x18,0x03};
diff --git a/nmap_descr/_10703_tex2html_wrap362.png b/nmap_descr/_10703_tex2html_wrap362.png
new file mode 100644
index 0000000000000000000000000000000000000000..7824e292260eea7d3b760c36eef8c1ed2a69b8f3
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap362.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap362.xbm b/nmap_descr/_10703_tex2html_wrap362.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a31d7ecb8f2d05aebec6a4e03500fc208fd9b0e0
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap362.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 7
+static char noname_bits[] = {
+ 0x61,0x33,0x1e,0x0c,0x1e,0x33,0x61};
diff --git a/nmap_descr/_10703_tex2html_wrap364.png b/nmap_descr/_10703_tex2html_wrap364.png
new file mode 100644
index 0000000000000000000000000000000000000000..9d940304e3c2eba9aae0c75a34285a32d72319ed
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap364.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap364.xbm b/nmap_descr/_10703_tex2html_wrap364.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7e9a0bb8f1a5eccb70706966ad0fd2aa4e6b8be3
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap364.xbm
@@ -0,0 +1,15 @@
+#define noname_width 87
+#define noname_height 16
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x01,0x00,0x08,0x02,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x60,0x0b,0x04,0x08,0x01,0x00,0x00,0x00,0x00,0x80,
+ 0x00,0x60,0x13,0x07,0x8c,0x01,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x33,0x04,
+ 0x8c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x21,0x04,0xc4,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0xc0,0x62,0x04,0xc6,0xf8,0x1f,0x8f,0xdf,0x8f,0xe7,0x3c,
+ 0xee,0x63,0x04,0xc2,0x3c,0x9b,0xcd,0xfb,0xcd,0xf4,0x36,0x1b,0x60,0x04,0xc2,
+ 0x98,0xd9,0x8c,0xd9,0x6c,0x6c,0x9e,0x0f,0x60,0x04,0xc3,0x98,0xd9,0x8c,0xd9,
+ 0x6c,0x66,0xbe,0x01,0x60,0x04,0xc1,0x98,0xed,0x94,0xcd,0x76,0xe6,0x93,0x19,
+ 0x60,0x9f,0xc1,0x98,0x9d,0x9f,0xc7,0xce,0xe3,0x1f,0x0f,0x60,0x80,0x81,0x00,
+ 0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x20,0x80,0x80,0x01,0x00,0xc0,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0xc0,0x80,0x01,0x00,0xe0,0x01,0x00,0x00,0x00,0x00,0x30,
+ 0xc0,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18};
diff --git a/nmap_descr/_10703_tex2html_wrap366.png b/nmap_descr/_10703_tex2html_wrap366.png
new file mode 100644
index 0000000000000000000000000000000000000000..3e753a8800ab0fb2a61303df5d8c56db43e08fce
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap366.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap366.xbm b/nmap_descr/_10703_tex2html_wrap366.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e34bc8153fd6ab7c3a29c8affc4d934da8a7a5fb
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap366.xbm
@@ -0,0 +1,19 @@
+#define noname_width 110
+#define noname_height 17
+static char noname_bits[] = {
+ 0x00,0xf0,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x3f,0x00,
+ 0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,
+ 0x00,0x00,0x00,0x80,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x07,0x00,0x08,0x00,
+ 0x00,0x00,0xc4,0x06,0x00,0x00,0x00,0x00,0x00,0x8c,0x0d,0x00,0x0c,0x00,0x00,
+ 0x00,0xc7,0x06,0x00,0x00,0x00,0x00,0x00,0xb6,0x0d,0x00,0x04,0x00,0x00,0x00,
+ 0x04,0x06,0x10,0x00,0x00,0x00,0x00,0x37,0x0c,0x00,0x06,0x00,0x00,0x00,0x04,
+ 0x03,0x10,0x00,0x00,0x00,0x00,0x27,0x06,0x00,0xc2,0xff,0x78,0x7e,0x84,0x05,
+ 0x10,0xc0,0xff,0x78,0xfc,0x30,0x0b,0x02,0xe3,0xd9,0x6c,0x6f,0xc4,0x07,0x10,
+ 0xe0,0xd9,0x6c,0xde,0xb0,0x0f,0x07,0xc1,0xcc,0x66,0x66,0x04,0x80,0xff,0xc1,
+ 0xcc,0x66,0xcc,0x18,0x00,0x86,0xc1,0xcc,0x66,0x66,0x04,0x00,0x10,0xc0,0xcc,
+ 0x66,0xcc,0x2c,0x00,0x8c,0xc0,0x6c,0xa7,0x36,0x04,0x00,0x10,0xc0,0x6c,0xa7,
+ 0x6c,0x26,0x00,0xcc,0xc0,0xec,0xfc,0x1e,0x1f,0x00,0x10,0xc0,0xec,0xfc,0x3c,
+ 0x3f,0x00,0x58,0x00,0x00,0x00,0x03,0x00,0x00,0x10,0x00,0x00,0x00,0x06,0x00,
+ 0x00,0x78,0x00,0x00,0x00,0x03,0x00,0x00,0x10,0x00,0x00,0x00,0x06,0x00,0x00,
+ 0x30,0x00,0x00,0x80,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x0f,0x00,0x00,0x30,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/nmap_descr/_10703_tex2html_wrap368.png b/nmap_descr/_10703_tex2html_wrap368.png
new file mode 100644
index 0000000000000000000000000000000000000000..bc05642477c5d92ebf374e232cd47ff26b8db54a
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap368.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap368.xbm b/nmap_descr/_10703_tex2html_wrap368.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e139d521b03edc13a1eca9d3bb6bc483b1cc72c4
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap368.xbm
@@ -0,0 +1,8 @@
+#define noname_width 41
+#define noname_height 11
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0xf8,0x43,0x00,0x00,0x00,0x00,0x30,0x73,0x00,0x80,0x01,0x00,
+ 0x18,0x42,0x00,0xe0,0x00,0x00,0x98,0x42,0x00,0x38,0x80,0x7f,0xd8,0x40,0x00,
+ 0x0e,0x80,0xcd,0xf8,0x40,0x00,0x03,0x00,0xff,0x4c,0x40,0x00,0x0f,0x80,0x0d,
+ 0x0c,0x40,0x00,0x3c,0xc0,0x8c,0x0c,0x40,0x00,0xf0,0x80,0x7f,0x1f,0xf0,0x01,
+ 0xc0,0x01,0x00,0x00,0x00,0x00};
diff --git a/nmap_descr/_10703_tex2html_wrap370.png b/nmap_descr/_10703_tex2html_wrap370.png
new file mode 100644
index 0000000000000000000000000000000000000000..123f879bd1f9992b2b3b422fb4ecaea3d7ff043e
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap370.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap370.xbm b/nmap_descr/_10703_tex2html_wrap370.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a8621d006ea31b5b16f1618794d5dd965c5d5cb1
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap370.xbm
@@ -0,0 +1,23 @@
+#define noname_width 158
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x00,0x00,0x00,0x80,
+ 0x00,0x00,0x00,0x00,0x04,0x0c,0x90,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x40,
+ 0x00,0x00,0x00,0x40,0x80,0x00,0x00,0x00,0x60,0x08,0x36,0xf0,0x00,0x00,0x00,
+ 0x00,0x80,0x00,0x00,0x60,0x00,0x00,0x00,0x70,0xc0,0x00,0x00,0x00,0xb0,0x19,
+ 0x32,0x10,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x20,0x00,0x00,0x00,0x40,0xc0,
+ 0x00,0x00,0x00,0xb8,0x11,0x23,0x10,0x80,0x30,0x00,0x00,0xc0,0x00,0x00,0x30,
+ 0x00,0x00,0x00,0x40,0x40,0x00,0x00,0x00,0x38,0x31,0x23,0xf0,0x80,0x19,0xf0,
+ 0x7c,0xff,0x79,0x7e,0x30,0xfc,0x8f,0xe7,0x47,0x60,0xfc,0x8f,0xe7,0x87,0x31,
+ 0x23,0x90,0x01,0x0f,0xb0,0xf9,0xd9,0xd8,0x4c,0x30,0x9e,0xcd,0xf6,0x46,0x20,
+ 0x9e,0xcd,0xf6,0x86,0x31,0x23,0x80,0x01,0x06,0xe0,0x99,0xc1,0xf0,0x4c,0x30,
+ 0xcc,0x6c,0x66,0x46,0x20,0xcc,0x6c,0x66,0xc6,0x30,0x23,0x98,0x01,0x0f,0xb0,
+ 0x99,0xc1,0xda,0x4c,0x30,0xcc,0x6c,0x66,0x46,0x30,0xcc,0x6c,0x66,0x66,0x31,
+ 0x32,0x9b,0x81,0x19,0x98,0x9b,0xd1,0xce,0x4d,0x30,0xcc,0x76,0x6a,0x43,0x10,
+ 0xcc,0x76,0x6a,0x33,0x31,0x36,0xf3,0x81,0x30,0xf0,0x3f,0xcf,0xfb,0xff,0x30,
+ 0xcc,0xce,0xef,0xf1,0x19,0xcc,0xce,0xef,0xf9,0x31,0x1c,0x60,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x30,0x00,0x18,0x00,0x00,0x30,0x00,0x10,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x30,0x00,0x08,
+ 0x00,0x00,0x30,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x00,0x00,0x78,0x00,0x0c,0x00,0x00,0x78,0x00,0x18,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x0c};
diff --git a/nmap_descr/_10703_tex2html_wrap372.png b/nmap_descr/_10703_tex2html_wrap372.png
new file mode 100644
index 0000000000000000000000000000000000000000..545ab9e9498c34c150f7681d704c96153cafd47f
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap372.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap372.xbm b/nmap_descr/_10703_tex2html_wrap372.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..9b807a157eb40cb5497cd5aaffebbe6d55639253
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap372.xbm
@@ -0,0 +1,11 @@
+#define noname_width 77
+#define noname_height 11
+static char noname_bits[] = {
+ 0xf8,0x81,0x0f,0x1e,0x00,0x00,0x00,0x80,0x3f,0x04,0x30,0xc3,0x18,0x0c,0x00,
+ 0x00,0x00,0x00,0x33,0x07,0x18,0x63,0x18,0x06,0x00,0x18,0x00,0x80,0x21,0x04,
+ 0x18,0x33,0x18,0x06,0x00,0x0e,0x00,0x80,0x29,0x04,0x98,0x33,0x18,0x06,0x80,
+ 0x03,0xf8,0x87,0x0d,0x04,0xf8,0x39,0x18,0x06,0xe0,0x00,0xd8,0x8c,0x0f,0x04,
+ 0x0c,0x18,0x18,0x43,0x30,0x00,0xf0,0xcf,0x04,0x04,0x0c,0x18,0x0c,0x63,0xf0,
+ 0x00,0xd8,0xc0,0x00,0x04,0x0c,0x30,0x0e,0x23,0xc0,0x03,0xcc,0xc8,0x00,0x04,
+ 0x1f,0x70,0xc7,0x3f,0x00,0x0f,0xf8,0xf7,0x01,0x1f,0x00,0xc0,0x01,0x00,0x00,
+ 0x1c,0x00,0x00,0x00,0x00};
diff --git a/nmap_descr/_10703_tex2html_wrap374.png b/nmap_descr/_10703_tex2html_wrap374.png
new file mode 100644
index 0000000000000000000000000000000000000000..e8d6fef7502d4e37837b9fdc2d811d0d256e2e65
Binary files /dev/null and b/nmap_descr/_10703_tex2html_wrap374.png differ
diff --git a/nmap_descr/_10703_tex2html_wrap374.xbm b/nmap_descr/_10703_tex2html_wrap374.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..56b301ff148bc201f332ce67e4c4f77137f5258a
--- /dev/null
+++ b/nmap_descr/_10703_tex2html_wrap374.xbm
@@ -0,0 +1,10 @@
+#define noname_width 61
+#define noname_height 13
+static char noname_bits[] = {
+ 0xf8,0x43,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x73,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x18,0x42,0x00,0x00,0x00,0x00,0x00,0x00,0x98,0x42,0x80,0x30,0x00,0x00,
+ 0x00,0x00,0xd8,0x40,0x80,0x19,0xf0,0x3f,0x9e,0x1f,0xf8,0x40,0x00,0x0f,0x78,
+ 0x36,0xdb,0x1b,0x4c,0x40,0x00,0x06,0x30,0xb3,0x99,0x19,0x0c,0x40,0x00,0x0f,
+ 0x30,0xb3,0x99,0x19,0x0c,0x40,0x80,0x19,0x30,0xdb,0xa9,0x0d,0x1f,0xf0,0x81,
+ 0x30,0x30,0x3b,0xbf,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x01};
diff --git a/nmap_descr/images.pl b/nmap_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..25df85da6cf3ddc78a90a18c7ddf2509de83303d
--- /dev/null
+++ b/nmap_descr/images.pl
@@ -0,0 +1,39 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$1baseline${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap342.xbm">'; 
+$key = q/{}$F1timesmap1+F2timesmap2${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap358.xbm">'; 
+$key = q/{}$times${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap362.xbm">'; 
+$key = q/{}$0.5timesarctan<<245>>(map1map2)<<245>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap370.xbm">'; 
+$key = q/{}$;html_special_mark_lt;F1${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap368.xbm">'; 
+$key = q/{}$1(mapnoise^<<238>>2<<238>>)${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap364.xbm">'; 
+$key = q/{}$POL;html_special_mark_lt;F1${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap372.xbm">'; 
+$key = q/{}$sqrt<<309>>map1^<<242>>2<<242>>+map2^<<243>>2<<243>><<309>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap366.xbm">'; 
+$key = q/{}$6times6${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap350.xbm">'; 
+$key = q/{}$F1timesmap${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap374.xbm">'; 
+$key = q/{}$sqrt<<150>>-1<<150>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap338.xbm">'; 
+$key = q/{}fbox<<336>>largesfy<<336>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap356.xbm">'; 
+$key = q/{}$(F1timesmap1+F2timesmap2)(abs(F1)+abs(F2))${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap360.xbm">'; 
+$key = q/{}$4times4${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap346.xbm">'; 
+$key = q/{}$sinctimesexp${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap352.xbm">'; 
+$key = q/{}$exp(-baseline^<<193>>2<<193>>)${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap340.xbm">'; 
+$key = q/{}$exp(-baseline^<<199>>2<<199>>)baseline${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap344.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/nmap_descr/labels.pl b/nmap_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..85208cd477024029871305d7412e19f82b866e4e
--- /dev/null
+++ b/nmap_descr/labels.pl
@@ -0,0 +1,20 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".make.qmaps"} ="$URL/nmap_descr.html"; 
+$external_labels{".intro"} ="$URL/nmap_descr.html"; 
+$external_labels{".fiddle"} ="$URL/nmap_descr.html"; 
+$external_labels{".make.example"} ="$URL/nmap_descr.html"; 
+$external_labels{".contents"} ="$URL/nmap_descr.html"; 
+$external_labels{".options"} ="$URL/nmap_descr.html"; 
+$external_labels{".nmap.handle"} ="$URL/nmap_descr.html"; 
+$external_labels{".fits"} ="$URL/nmap_descr.html"; 
+$external_labels{".make.qdatas"} ="$URL/nmap_descr.html"; 
+$external_labels{".make.output"} ="$URL/nmap_descr.html"; 
+$external_labels{".nmap.make.q"} ="$URL/nmap_descr.html"; 
+$external_labels{".nmap.make"} ="$URL/nmap_descr.html"; 
+$external_labels{".copy"} ="$URL/nmap_descr.html"; 
+$external_labels{".make"} ="$URL/nmap_descr.html"; 
+$external_labels{".make.input"} ="$URL/nmap_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/nmap_descr/nmap_descr.html b/nmap_descr/nmap_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..bad10b12bb80390096ef9029d4bcd10cc2a7b0ac
--- /dev/null
+++ b/nmap_descr/nmap_descr.html
@@ -0,0 +1,273 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NMAP</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nmap_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nmap_descr.html#SECTION0002000000000000000>  <b>Introduction</b></A>
+<LI> <A NAME=tex2html3 HREF=nmap_descr.html#SECTION0003000000000000000> <b>Overview of NMAP options</b></A>
+<LI> <A NAME=tex2html4 HREF=nmap_descr.html#SECTION0004000000000000000> <b>Option MAKE: Making maps</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=nmap_descr.html#SECTION0004100000000000000> <b>Types of output images</b></A>
+<LI> <A NAME=tex2html6 HREF=nmap_descr.html#SECTION0004200000000000000> <b>Operations on the input data</b></A>
+</UL> 
+<LI> <A NAME=tex2html7 HREF=nmap_descr.html#SECTION0005000000000000000> <b>Option MAKE: example</b></A>
+<UL> 
+<LI> <A NAME=tex2html8 HREF=nmap_descr.html#SECTION0005100000000000000> <b>QMAPS: Hidden map options</b></A>
+<LI> <A NAME=tex2html9 HREF=nmap_descr.html#SECTION0005200000000000000> <b>QDATAS: Hidden map options</b></A>
+</UL> 
+<LI> <A NAME=tex2html10 HREF=nmap_descr.html#SECTION0006000000000000000> <b>Option FIDDLE: Operations on maps</b></A>
+<LI> <A NAME=tex2html11 HREF=nmap_descr.html#SECTION0007000000000000000> <b>Option FITS: Conversion to FITS format</b></A>
+</UL>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Introduction</b></A></H1>
+<P>
+        The <i>NEWSTAR </i> program NMAP makes maps (images) from the uv-data in a SCN-file, and stores them in a WMP-file. The input data may be combined in many different ways, to produce maps that range from simple to quite exotic.  As a by-product, antenna patterns may be calculated (and stored in the same .WMP file), for use in <A HREF="../nclean_descr/nclean_descr.html">NCLEAN</A>.
+<P>
+        The program NMAP also allows the user to manipulate maps in a .WMP file, and to convert them to other formats.
+<P>
+        A .WMP file may contain various kinds of maps that are <em>related in some way</em>, i.e. different frequency channels, polarisations, pointing centres (mosaicking), antenna patterns, CLEAN residuals, and even gridded uv-data. Each <em>image</em> in a .WMP file consists of a 2-dimensional array of pixel values, withj a header containing descriptive information. A 'hypercube' of images in a .WMP file can have maps of different sizes. For more information about the structure of the .WMP file, see the <A HREF="../wmp_descr/wmp_descr.html">.WMP file</A> description.
+<P>
+<A NAME=.options><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Overview of NMAP options</b></A></H1>
+<P>
+The program NMAP offers the following main options:
+<P>
+<UL><LI> <b>MAKE:</b>      Make map(s) and/or antenna patterns 
+<LI> <b>SHOW:</b>      Show/edit map (header) data. 
+                        See section on WMP File Description. 
+<LI> <b>FIDDLE:</b>    Perform all kinds of operations on maps. 
+<LI> <b>W16FITS:</b>   Write FITS tape/disk with 16 bits data. 
+<LI> <b>W32FITS:</b>   Write FITS tape/disk with 32 bits data. 
+<LI> <b>FROM_OLD:</b> Convert from old (R-series) format to WMP format. 
+<LI> <b>TO_OLD:</b>   Convert from WMP format to old (R-series) format. 
+<LI> <b>CVX:</b>       Convert a WMP-file from other machine's format 
+                        to local machine's. 
+<LI> <b>NVS:</b>       Convert a WMP file to newest version. 
+                        This option should be run if indicated by the program). 
+<LI> <b>QUIT:</b>      Quit the program NMAP. 
+</UL>
+<P>
+<A NAME=.make><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Option MAKE: Making maps</b></A></H1>
+<P>
+        An overview of the user interface for the MAKE option is shown in 
+<A HREF=" #.nmap.make">figure</A> and its companion <A HREF=" #.nmap.make.q">figure</A>.
+<P>
+<A NAME=.nmap.make><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of NMAP's map-making interface. 
+<A HREF="../fig/nmap_make.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See <A HREF=" #.nmap.make.q">figure</A> for the QMAPS and QDATS branches; by default, these branches are bypassed. 
+<BR><BR>(The rightmost column in the diagram is irrelevant for map-making in NMAP.) </i>
+<P>
+<A NAME=.make.output><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000> <b>Types of output images</b></A></H2>
+<P>
+        The program NMAP produces (multiple) images of the following types:
+<P>
+<UL><LI> <b>MAP:</b> Normal map of the uv-data or the uv-model (the uv-representation of the Selfcal model) from the SCN-file. Various linear combinations of the four measured polarisations can be specified with the keyword <b>MAP_POLAR</b>, to produce:
+<P>
+  <UL><LI> <b>XX, YY, XY or YX-maps:</b> Use XX, YY, XY or YX data only 
+  <LI> <b>I-map:</b>   (XX+YY)/2 
+  <LI> <b>Q-map:</b>   (-XX+YY)/2 
+  <LI> <b>U-map:</b>   (-XY+YX)/2 
+  <LI> <b>V-map:</b>   (XY+YX)*i/2 
+  <LI> <b>L-map:</b>   XX or YY or (XX+YY)/2 if both present 
+  <LI> <b>*I-map:</b>  any of the above, but multiplied with <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap338.png"> 
+  </UL>
+<P>
+NB: Note that parallel dipoles (++) are assumed here. Observations with `crossed' dipoles (+x) require linear combinations of all four polarisations. This can be done in the map plane (see NMAP option <b>FIDDLE_OPTION</b>).
+<P>
+<LI> <b>AP:</b>        Antenna pattern (Replace uv-data by 1's) 
+<LI> <b>COS:</b>       Assume input sines to be zero 
+<LI> <b>SIN:</b>       Assume input cosines to be zero 
+<LI> <b>AMPL:</b>      Assume input phases to be zero 
+<LI> <b>PHASE:</b>     Assume input amplitudes to be one 
+</UL>
+<P>
+It is also possible to store <b>uv-data</b> in a WMP file, for display purposes. The uv-data is `gridded' (convolved onto a rectangular grid).
+<P>
+<UL><LI> <b>COVER:</b>     Gridded uv-coverage (data replaced by 1's) 
+<LI> <b>REAL:</b>      Real part of the gridded uv-data 
+<LI> <b>IMAG:</b>      Imaginary part of the gridded uv-data 
+<LI> <b>AMPL:</b>      Amplitude of the gridded uv-data 
+<LI> <b>PHASE:</b>     Phases of the gridded uv-data 
+</UL>
+<P>
+<A NAME=.make.input><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000> <b>Operations on the input data</b></A></H2>
+<P>
+<A NAME=.nmap.make.q><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the optional detailed-question sequences of the map-making interface. This diagram expands the <em>QMAPS</em> and <em>QDATAS</em> stubs in 
+<A HREF="../fig/nmap_make_q.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><A HREF=" #.nmap.make">figure</A>. </i>
+<P>
+<UL><LI> <b>Data selection</b>: The uv-data that go into a map may be selected in various ways: 
+  <UL><LI> One or more SCN-files. 
+  <LI> Sets within a SCN-file (e.g. frequ channels, pointing centres). 
+  <LI> HA-Scans within each Set (HA-range). 
+  <LI> Polarisations (XX,YY,XY,YX). 
+  <LI> Individual iterferometers 
+  <LI> An area in the uv-plane 
+  <LI> Clip-level 
+  </UL>
+<P>
+<LI> <b>Data correction</b>: Various correction factors are stored in the Set and Scan headers of the SCN-file. They may be applied to the uv-data at the moment that they are read from disk for processing. Application of correction is controlled by the NGEN keywords <b>APPLY</b> and <b>DE_APPLY</b> (see the section `Common Features of <i>NEWSTAR </i> Programs' in this Cookbook).
+<P>
+<LI> <b>Data conversion</b>: The uv-data may be converted in various ways: 
+  <UL><LI> Subtraction of a source model. 
+  <LI> Combination of different polarisations (XX,YY,XY,YX). 
+  <LI> Conversion to amplitudes or phases. 
+  </UL>
+<P>
+<LI> <b>Data weighting:</b> 
+  <UL><LI>   NATURAL:  Take each individual measured point separately, 
+                        without weighting for the UV track covered by it. 
+  <LI>   STANDARD: Weight each observed point with the track length covered 
+                        on the UV plane, 
+                        and average redundant baselines on a per set basis. 
+  <i>(default)</i> 
+  <LI>   FULL:     Weight each point according to the actual UV point 
+                        density. In this case care is taken of all local UV 
+                        plane density enhancements, 
+                        but it necessitates an extra pass through the data. 
+  </UL>
+<P>
+<LI> <b>Data tapering:</b> 
+  <UL><LI>   GAUSS:      <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap340.png"> 
+  <i>(default)</i> 
+  <LI>   LINEAR:     max(0,1-baseline/taper_value) 
+  <LI>   NATURAL:    no taper 
+  <LI>   OVERR:      <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap342.png"> 
+  <LI>   RGAUSS:     <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap344.png"> 
+  </UL>
+<P>
+<LI> <b>Data convolution:</b> (onto a rectangular grid in the uv-plane) 
+  <UL><LI>   GAUSS:      Gaussian type with <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap346.png"> grid points 
+  <LI>   P4ROL:      Prolate spheroidal function with <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap346.png"> grid points 
+  <LI>   P6ROL:      Prolate spheroidal function with <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap350.png"> grid points 
+  <LI>   EXPSINC:    <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap352.png"> on <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap350.png"> grid points 
+  <i>(default)</i> 
+  <LI>   BOX:        A square box 
+  </UL> 
+</UL>
+<P>
+At this point, the data are either stored in the WMP file as gridded uv-data (usually for display purposes), or Fouries transformed into an image.
+<P>
+<A NAME=.make.example><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>Option MAKE: example</b></A></H1>
+<P>
+The following is an example of making a `normal' map (and its antenna pattern), using the program defaults. This is usually sufficient to get a satisfactory result. Experienced users may experiment with some of the more advanced options.
+<P>
+**** Put new script here ****
+<P>
+<A NAME=.make.qmaps><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005100000000000000> <b>QMAPS: Hidden map options</b></A></H2>
+<P>
+The more advanced map-making options are hidden behind the NMAP keyword <b>QMAPS</b>. If skipped, the (context-sensitive) default values will give a satisfactory result in most cases. Their values will be printed in the NMAP log-file. For more information on each of these keywords, see the on-line Help text (type `?'), which is also printed in the `Summary of NMAP keywords' in this Cookbook.
+<P>
+**** Put new script here ****
+<P>
+<A NAME=.make.qdatas><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000> <b>QDATAS: Hidden map options</b></A></H2>
+<P>
+The more advanced data-selection options are hidden behind the NMAP keyword <b>QDATA</b>. If skipped, the (context-sensitive) default values will give a satisfactory result in most cases. Their values will be printed in the NMAP log-file. For more information on each of these keywords, see the on-line Help text (type `?'), which is also printed in the `Summary of NMAP keywords' in this Cookbook.
+<P>
+ QDATAS 
+ (More data handling details?) 
+ = NO: 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap356.png">
+<P>
+(To be added later).
+<P>
+<A NAME=.fiddle><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0006000000000000000> <b>Option FIDDLE: Operations on maps</b></A></H1>
+<P>
+<A NAME=.nmap.handle><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of NMAP's map-handling interface. } 
+<A HREF="../fig/nmap_handle.ps"><STRONG>FIGURE</STRONG></A> 
+ .]{<i>The NMAP keyword <b>FIDDLE_OPTION</b> offers the user a wide range of possibilities to perform oparations on maps in WMP files:
+<P>
+All relevant data are copied from the first (or only) input map. If 2 maps are required (ADD,AVER,POL,ANGLE) all pairs of SETS_1and SETS_2will produce an output map. SUM will average all SETS_1maps. MOSCOM will produce a single output map from all specified input maps. The others will produce an output for each SETS_1. BEAM, DEBEAM and FACTOR will overwrite the input maps. F is a specified multiplication factor.
+<P>
+<UL><LI> <b>ADD:</b>  <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap358.png"> 
+<LI> <b>AVER:</b>  <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap360.png"> 
+<LI> <b>SUM:</b>  Various averages of maps. In all cases the summation produces a weighted average map over all SETS_1, the weight depending on the type: 
+  <UL><LI> <b>SUM:</b>  weight(i)= 1 
+  <LI> <b>NSUM:</b>  weight(i)= normalisation factor of map 
+  <LI> <b>BSUM:</b>  weight(i)= bandwidth 
+  <LI> <b>BNSUM:</b>  weight(i)= bandwidth <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap362.png"> normalisation factor 
+  <LI> <b>FSUM:</b>  weight(i)= factor given by the user. 
+                Up to 8 factors can be given, 
+                which will be used in a cyclic fashion if more needed 
+  <LI> <b>NSSUM:</b>  weight(i)= <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap364.png"> 
+  <LI> <b>QUIT:</b>  finished 
+  </UL> 
+<LI> <b>POL:</b>  <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap366.png">, 
+                unless <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap368.png">, then 0 
+<LI> <b>ANGLE:</b>  <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap370.png"> (radians), 
+                unless <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap372.png">, then 0 
+<LI> <b>EXTRACT:</b>  extract an area of maps 
+<A NAME=.copy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<LI> <b>COPY:</b>  copy maps 
+<LI> <b>BEAM:</b>  correct maps for primary beam 
+<LI> <b>DEBEAM:</b>  de-correct maps for primary beam 
+<LI> <b>FACTOR:</b>  <IMG ALIGN=BOTTOM ALT="" SRC="_10703_tex2html_wrap374.png"> 
+<LI> <b>MOSCOM:</b>  combine all specified maps 
+                (referenced to same mosaic position) into one output map. 
+                The noise of the individual maps may be used as weight. 
+<LI> <b>QUIT:</b>  quit the fiddle option. 
+</UL>
+<P>
+<A NAME=.fits><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+</i><H1><A NAME=SECTION0007000000000000000> <b>Option FITS: Conversion to FITS format</b></A></H1>
+<P>
+There are two separate NMAP options (<b>W16FITS</b> and <b>W32FITS</b>.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
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+
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+
+<P>.
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+<P>.
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+
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+
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+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+end
+%%EndProlog
+%%BeginSetup
+%%Feature: *Resolution 300dpi
+TeXDict begin
+%%PaperSize: a4
+
+%%EndSetup
+%%Page: 1 1
+1 0 bop 118 -41 a Fd(Printout)15 b(of)g(NEWST)m(AR)g(do)n(cument)h
+(chapter)f(-)f(June)i(13,)f(1997)0 59 y Fc(Adv)l(anced)23
+b(NMAP)f(examples)0 221 y(Con)n(ten)n(ts)0 320 y Fb(1)38
+b(Making)16 b(m)o(ultip)o(l)o(e)d(maps)1334 b(1)0 601
+y Fc(1)67 b(Making)23 b(m)n(ultiple)i(maps)0 716 y Fa(****)13
+b(Put)h(new)g(script)h(here)g(****)935 2995 y(1)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nmap_example/images.pl b/nmap_example/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nmap_example/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nmap_example/labels.pl b/nmap_example/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..4901387018aac4c5ce35e1722f08d5229e0b466c
--- /dev/null
+++ b/nmap_example/labels.pl
@@ -0,0 +1,7 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"nmap.example.makemult"} ="$URL/nmap_example.html"; 
+$external_labels{".contents"} ="$URL/nmap_example.html"; 
+
+1;
\ No newline at end of file
diff --git a/nmap_example/nmap_example.html b/nmap_example/nmap_example.html
new file mode 100644
index 0000000000000000000000000000000000000000..f075522c3fea3c8acd544d0e638e8217d8d90e91
--- /dev/null
+++ b/nmap_example/nmap_example.html
@@ -0,0 +1,63 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Advanced NMAP examples</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nmap_example.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nmap_example.html#SECTION0002000000000000000> <b>Making multiple maps</b></A>
+</UL>
+<A NAME=nmap.example.makemult><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Making multiple maps</b></A></H1>
+<P>
+**** Put new script here ****
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nmap_keys/nmap_keys.html b/nmap_keys/nmap_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..156aa0f32da9da6cb0f36e563aa6a6adc77a06c4
--- /dev/null
+++ b/nmap_keys/nmap_keys.html
@@ -0,0 +1,205 @@
+<TITLE>Index of private keywords for NMAP </TITLE>
+<H1>Description of keywords for program NMAP</H1>
+
+<UL>
+<LI> <A HREF="../nmap/nmap__option.html">
+  OPTION</A>
+  Action| MAKE, FIDDLE; W16FITS, W32FITS, WRLFITS, RFITS; SHOW; QUIT;|-[FROM_OLD, TO_OLD, CVX, NVS]
+<LI> <A HREF="../nmap/nmap__fiddle_option.html">
+  FIDDLE_OPTION</A>
+  Fiddle action| BEAM, DEBEAM, FACTOR; EXTRACT, COPY, LOAD;|-ADD, AVER, POL, ANGLE; SUM, CSUM, RSUM, MOSCOM; QUIT
+<LI> <A HREF="../nmap/nmap__cubic.html">
+  CUBIC</A>
+  Make line cube (Yes/No) ?
+<LI> <A HREF="../nmap/nmap__use_noise.html">
+  USE_NOISE</A>
+  Weigh with noise (Yes/No) ?
+<LI> <A HREF="../nmap/nmap__wgt_limit.html">
+  WGT_LIMIT</A>
+  Relative weight limit
+<LI> <A HREF="../nmap/nmap__sum_option.html">
+  SUM_OPTION</A>
+  SUM, NSUM, NSSUM, BSUM, BNSUM, FSUM; QUIT Weighing method
+<LI> <A HREF="../nmap/nmap__load_option.html">
+  LOAD_OPTION</A>
+  WMP, UNLOAD; NEWHOLOG, [OLDHOLOG]; QUIT Load action/image type |
+<LI> <A HREF="../nmap/nmap__map_factors.html">
+  MAP_FACTORS</A>
+  Input-map multipliers
+<LI> <A HREF="../nmap/nmap__sum_factors.html">
+  SUM_FACTORS</A>
+  Summing multipliers
+<LI> <A HREF="../nmap/nmap__csum_factors.html">
+  CSUM_FACTORS</A>
+  Summing multipliers
+<LI> <A HREF="../nmap/nmap__rotation_measure.html">
+  ROTATION_MEASURE</A>
+  Rotation measure
+<LI> <A HREF="../nmap/nmap__map_level.html">
+  MAP_LEVEL</A>
+  Polarisation threshold (W.U)
+<LI> <A HREF="../nmap/nmap__comment.html">
+  COMMENT</A>
+  FITS comment (&lt;=70 chars)
+<LI> <A HREF="../nmap/nmap__fits_scale.html">
+  FITS_SCALE</A>
+  JY, WU Units of source flux
+<LI> <A HREF="../nmap/nmap__input_file.html">
+  INPUT_FILE</A>
+  Input file name
+<LI> <A HREF="../nmap/nmap__filename.html">
+  FILENAME</A>
+  Name for output disk file
+<LI> <A HREF="../nmap/nmap__input_labels.html">
+  INPUT_LABELS</A>
+  Input tape labels
+<LI> <A HREF="../nmap/nmap__output_label.html">
+  OUTPUT_LABEL</A>
+  Output label
+<LI> <A HREF="../nmap/nmap__wmp_node_1.html">
+  WMP_NODE_1</A>
+  First WMP node name
+<LI> <A HREF="../nmap/nmap__wmp_node_2.html">
+  WMP_NODE_2</A>
+  Second WMP node name
+<LI> <A HREF="../nmap/nmap__wmp_set_1.html">
+  WMP_SET_1</A>
+  First image set(s) to be used: grp.fld.chn.pol.typ.seq
+<LI> <A HREF="../nmap/nmap__wmp_set_2.html">
+  WMP_SET_2</A>
+  Second image set(s) to be used: grp.fld.chn.pol.typ.seq
+<LI> <A HREF="../nmap/nmap__area.html">
+  AREA</A>
+  Area: l, m, dl, dm
+<LI> <A HREF="../nmap/nmap__data_action.html">
+  DATA_ACTION</A>
+  Action to perform on the data SHOW; NOISE, OFFSET; QUIT
+<LI> <A HREF="../nmap/nmap__map_polar.html">
+  MAP_POLAR</A>
+  Select 1 to 4 output-map polarisation(s)| XX, XY, YX, YY; I, L, Q, U, V; XXI, XYI, YXI, YYI; II, LI, QI, UI, VI
+<LI> <A HREF="../nmap/nmap__map_coord.html">
+  MAP_COORD</A>
+  Map coordinate system|  B1950_J2000, APPARENT; REFERENCE, AREFERENCE
+<LI> <A HREF="../nmap/nmap__ref_coord.html">
+  REF_COORD</A>
+  Map reference coordinates: RA, DEC (decimal deg)
+<LI> <A HREF="../nmap/nmap__user_comment.html">
+  USER_COMMENT</A>
+  Comment to be included in map header(s) (&lt;=24 chars)|
+<LI> <A HREF="../nmap/nmap__uv_coordinates.html">
+  UV_COORDINATES</A>
+  UV coordinate system UV, BASHA, IFRHA
+<LI> <A HREF="../nmap/nmap__ha_resolution.html">
+  HA_RESOLUTION</A>
+  Hour-angle averaging interval (UT seconds)
+<LI> <A HREF="../nmap/nmap__bas_resolution.html">
+  BAS_RESOLUTION</A>
+  Baseline averaging interval (m)
+<LI> <A HREF="../nmap/nmap__ifr_resolution.html">
+  IFR_RESOLUTION</A>
+  Interferometer separation
+<LI> <A HREF="../nmap/nmap__ft_size.html">
+  FT_SIZE</A>
+  FFT size
+<LI> <A HREF="../nmap/nmap__out_size.html">
+  OUT_SIZE</A>
+  Output map size
+<LI> <A HREF="../nmap/nmap__out_centre.html">
+  OUT_CENTRE</A>
+  Output map centre
+<LI> <A HREF="../nmap/nmap__lm_centre.html">
+  LM_CENTRE</A>
+  Output map centre
+<LI> <A HREF="../nmap/nmap__radec_centre.html">
+  RADEC_CENTRE</A>
+  Output map centre: RA, DEC (decimal deg)
+<LI> <A HREF="../nmap/nmap__field_size.html">
+  FIELD_SIZE</A>
+  Fieldsize l, m (deg)
+<LI> <A HREF="../nmap/nmap__grid_size.html">
+  GRID_SIZE</A>
+  Grid interval in l, m (arcsec)
+<LI> <A HREF="../nmap/nmap__taper.html">
+  TAPER</A>
+  GAUSS, LINEAR, OVERR, RGAUSS, NATURAL Taper type
+<LI> <A HREF="../nmap/nmap__convolve.html">
+  CONVOLVE</A>
+  GAUSS, BOX, P4ROL, P6ROL, EXPSINC Convolution type
+<LI> <A HREF="../nmap/nmap__deconvolve.html">
+  DECONVOLVE</A>
+  Correct map for convolution taper (Yes/No) ?
+<LI> <A HREF="../nmap/nmap__qdatas.html">
+  QDATAS</A>
+  Special data selection (Yes/No) ?
+<LI> <A HREF="../nmap/nmap__user_data.html">
+  USER_DATA</A>
+  STANDARD, MODEL Visibilities to use
+<LI> <A HREF="../nmap/nmap__clipping.html">
+  CLIPPING</A>
+  Clipping?
+<LI> <A HREF="../nmap/nmap__clip_area.html">
+  CLIP_AREA</A>
+  UV-radius range for clipping (m)
+<LI> <A HREF="../nmap/nmap__clip_levels.html">
+  CLIP_LEVELS</A>
+  Amplitude range to be discarded
+<LI> <A HREF="../nmap/nmap__subtract.html">
+  SUBTRACT</A>
+  Model subtraction (Yes/No) ?
+<LI> <A HREF="../nmap/nmap__field_shift.html">
+  FIELD_SHIFT</A>
+  l, m field shift (arcsec)
+<LI> <A HREF="../nmap/nmap__field_centre.html">
+  FIELD_CENTRE</A>
+  Field centre: RA, DEC (decimal deg)
+<LI> <A HREF="../nmap/nmap__data_type.html">
+  DATA_TYPE</A>
+  NORMAL, COS, SIN, AMPL, PHASE Data transformation for display
+<LI> <A HREF="../nmap/nmap__output.html">
+  OUTPUT</A>
+  MAP, AP; COVER; REAL, IMAG, AMPL, PHASE
+<LI> <A HREF="../nmap/nmap__old_dattyp.html">
+  OLD_DATTYP</A>
+  Old R-series data format
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nshow_comm/nshow_comm.html">NSHOW</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmap_comm/nmap_comm.html">NMAP</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpnode_comm/wmpnode_comm.html">WMPNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpsets_comm/wmpsets_comm.html">WMPSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../unit_comm/unit_comm.html">UNIT</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nmap_descr/nmap_descr.html">program NMAP</A>
+</UL>
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index 0000000000000000000000000000000000000000..1c4b3ea79a7a5c87975460f6e6ab183c49fd2675
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NMAP</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nmap_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nmap_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nmap_private_intfc.html#SECTION0003000000000000000>  <b>Interface diagrams</b></A>
+<LI> <A NAME=tex2html4 HREF=nmap_private_intfc.html#SECTION0004000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=nmap_private_intfc.html#SECTION0004100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html6 HREF=nmap_private_intfc.html#SECTION0004200000000000000>  <b>Parameter AREA</b></A>
+<LI> <A NAME=tex2html7 HREF=nmap_private_intfc.html#SECTION0004300000000000000>  <b>Parameter BAS_RESOLUTION</b></A>
+<LI> <A NAME=tex2html8 HREF=nmap_private_intfc.html#SECTION0004400000000000000>  <b>Parameter CLIPPING</b></A>
+<LI> <A NAME=tex2html9 HREF=nmap_private_intfc.html#SECTION0004500000000000000>  <b>Parameter CLIP_AREA</b></A>
+<LI> <A NAME=tex2html10 HREF=nmap_private_intfc.html#SECTION0004600000000000000>  <b>Parameter CLIP_LEVELS</b></A>
+<LI> <A NAME=tex2html11 HREF=nmap_private_intfc.html#SECTION0004700000000000000>  <b>Parameter COMMENT</b></A>
+<LI> <A NAME=tex2html12 HREF=nmap_private_intfc.html#SECTION0004800000000000000>  <b>Parameter CONVOLVE</b></A>
+<LI> <A NAME=tex2html13 HREF=nmap_private_intfc.html#SECTION0004900000000000000>  <b>Parameter CSUM_FACTORS</b></A>
+<LI> <A NAME=tex2html14 HREF=nmap_private_intfc.html#SECTION00041000000000000000>  <b>Parameter CUBIC</b></A>
+<LI> <A NAME=tex2html15 HREF=nmap_private_intfc.html#SECTION00041100000000000000>  <b>Parameter DATA_ACTION</b></A>
+<LI> <A NAME=tex2html16 HREF=nmap_private_intfc.html#SECTION00041200000000000000>  <b>Parameter DATA_TYPE</b></A>
+<LI> <A NAME=tex2html17 HREF=nmap_private_intfc.html#SECTION00041300000000000000>  <b>Parameter DECONVOLVE</b></A>
+<LI> <A NAME=tex2html18 HREF=nmap_private_intfc.html#SECTION00041400000000000000>  <b>Parameter FIDDLE_OPTION</b></A>
+<LI> <A NAME=tex2html19 HREF=nmap_private_intfc.html#SECTION00041500000000000000>  <b>Parameter FIELD_CENTRE</b></A>
+<LI> <A NAME=tex2html20 HREF=nmap_private_intfc.html#SECTION00041600000000000000>  <b>Parameter FIELD_SHIFT</b></A>
+<LI> <A NAME=tex2html21 HREF=nmap_private_intfc.html#SECTION00041700000000000000>  <b>Parameter FIELD_SIZE</b></A>
+<LI> <A NAME=tex2html22 HREF=nmap_private_intfc.html#SECTION00041800000000000000>  <b>Parameter FILENAME</b></A>
+<LI> <A NAME=tex2html23 HREF=nmap_private_intfc.html#SECTION00041900000000000000>  <b>Parameter FITS_SCALE</b></A>
+<LI> <A NAME=tex2html24 HREF=nmap_private_intfc.html#SECTION00042000000000000000>  <b>Parameter FT_SIZE</b></A>
+<LI> <A NAME=tex2html25 HREF=nmap_private_intfc.html#SECTION00042100000000000000>  <b>Parameter GRID_SIZE</b></A>
+<LI> <A NAME=tex2html26 HREF=nmap_private_intfc.html#SECTION00042200000000000000>  <b>Parameter HA_RESOLUTION</b></A>
+<LI> <A NAME=tex2html27 HREF=nmap_private_intfc.html#SECTION00042300000000000000>  <b>Parameter IFR_RESOLUTION</b></A>
+<LI> <A NAME=tex2html28 HREF=nmap_private_intfc.html#SECTION00042400000000000000>  <b>Parameter INPUT_FILE</b></A>
+<LI> <A NAME=tex2html29 HREF=nmap_private_intfc.html#SECTION00042500000000000000>  <b>Parameter INPUT_LABELS</b></A>
+<LI> <A NAME=tex2html30 HREF=nmap_private_intfc.html#SECTION00042600000000000000>  <b>Parameter LM_CENTRE</b></A>
+<LI> <A NAME=tex2html31 HREF=nmap_private_intfc.html#SECTION00042700000000000000>  <b>Parameter LOAD_OPTION</b></A>
+<LI> <A NAME=tex2html32 HREF=nmap_private_intfc.html#SECTION00042800000000000000>  <b>Parameter MAP_COORD</b></A>
+<LI> <A NAME=tex2html33 HREF=nmap_private_intfc.html#SECTION00042900000000000000>  <b>Parameter MAP_FACTORS</b></A>
+<LI> <A NAME=tex2html34 HREF=nmap_private_intfc.html#SECTION00043000000000000000>  <b>Parameter MAP_LEVEL</b></A>
+<LI> <A NAME=tex2html35 HREF=nmap_private_intfc.html#SECTION00043100000000000000>  <b>Parameter MAP_POLAR</b></A>
+<LI> <A NAME=tex2html36 HREF=nmap_private_intfc.html#SECTION00043200000000000000>  <b>Parameter OLD_DATTYP</b></A>
+<LI> <A NAME=tex2html37 HREF=nmap_private_intfc.html#SECTION00043300000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html38 HREF=nmap_private_intfc.html#SECTION00043400000000000000>  <b>Parameter OUTPUT</b></A>
+<LI> <A NAME=tex2html39 HREF=nmap_private_intfc.html#SECTION00043500000000000000>  <b>Parameter OUTPUT_LABEL</b></A>
+<LI> <A NAME=tex2html40 HREF=nmap_private_intfc.html#SECTION00043600000000000000>  <b>Parameter OUT_CENTRE</b></A>
+<LI> <A NAME=tex2html41 HREF=nmap_private_intfc.html#SECTION00043700000000000000>  <b>Parameter OUT_SIZE</b></A>
+<LI> <A NAME=tex2html42 HREF=nmap_private_intfc.html#SECTION00043800000000000000>  <b>Parameter QDATAS</b></A>
+<LI> <A NAME=tex2html43 HREF=nmap_private_intfc.html#SECTION00043900000000000000>  <b>Parameter RADEC_CENTRE</b></A>
+<LI> <A NAME=tex2html44 HREF=nmap_private_intfc.html#SECTION00044000000000000000>  <b>Parameter REF_COORD</b></A>
+<LI> <A NAME=tex2html45 HREF=nmap_private_intfc.html#SECTION00044100000000000000>  <b>Parameter ROTATION_MEASURE</b></A>
+<LI> <A NAME=tex2html46 HREF=nmap_private_intfc.html#SECTION00044200000000000000>  <b>Parameter SUBTRACT</b></A>
+<LI> <A NAME=tex2html47 HREF=nmap_private_intfc.html#SECTION00044300000000000000>  <b>Parameter SUM_FACTORS</b></A>
+<LI> <A NAME=tex2html48 HREF=nmap_private_intfc.html#SECTION00044400000000000000>  <b>Parameter SUM_OPTION</b></A>
+<LI> <A NAME=tex2html49 HREF=nmap_private_intfc.html#SECTION00044500000000000000>  <b>Parameter TAPER</b></A>
+<LI> <A NAME=tex2html50 HREF=nmap_private_intfc.html#SECTION00044600000000000000>  <b>Parameter USER_COMMENT</b></A>
+<LI> <A NAME=tex2html51 HREF=nmap_private_intfc.html#SECTION00044700000000000000>  <b>Parameter USER_DATA</b></A>
+<LI> <A NAME=tex2html52 HREF=nmap_private_intfc.html#SECTION00044800000000000000>  <b>Parameter USE_NOISE</b></A>
+<LI> <A NAME=tex2html53 HREF=nmap_private_intfc.html#SECTION00044900000000000000>  <b>Parameter UV_COORDINATES</b></A>
+<LI> <A NAME=tex2html54 HREF=nmap_private_intfc.html#SECTION00045000000000000000>  <b>Parameter WGT_LIMIT</b></A>
+<LI> <A NAME=tex2html55 HREF=nmap_private_intfc.html#SECTION00045100000000000000>  <b>Parameter WMP_NODE_1</b></A>
+<LI> <A NAME=tex2html56 HREF=nmap_private_intfc.html#SECTION00045200000000000000>  <b>Parameter WMP_NODE_2</b></A>
+<LI> <A NAME=tex2html57 HREF=nmap_private_intfc.html#SECTION00045300000000000000>  <b>Parameter WMP_SET_1</b></A>
+<LI> <A NAME=tex2html58 HREF=nmap_private_intfc.html#SECTION00045400000000000000>  <b>Parameter WMP_SET_2</b></A>
+</UL>
+</UL>
+<A NAME=.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NMAP. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>.
+<P>
+        Apart from a number of utility options, the main functions of NMAP are the making of maps from .SCN files (option MAKE) and manipulating these maps in various ways (option FIDDLE).
+<P>
+        &quot;Roadmap&quot;-style overviews for the entire parameter interface are shown in <A HREF="#.diagrams">below</A>.
+<P>
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.diagrams><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Interface diagrams</b></A></H1>
+<P>
+        The first diagram, an synopsis of NMAP's parameter interface, does not yet exist. Following that diagram several sub-diagrams are planned, of which those for the FIDDLE and utility options still have to be made.
+<P>
+        <A HREF=" #.nmap.make">Figure</A> shows the parameter interface for MAKE. Two detours in this interface, for parameters QMAPS and QDATAS, are normally bypassed; they are shown in <A HREF=" #.nmap.make.q">figure</A>.
+<P>
+        Included in these diagrams are NMAP's public parameters. These are interleaved with the private ones so they can not be diagrammed as a separate unit. In fact, the only reason that they are public is that the NCLEAN 
+<A HREF="../nclean_descr/nclean_descr.html#.data.clean">'data clean'</A> operation uses them. This use is indicated on the right-hand side of <A HREF=" #.nmap.make">figure</A> and 
+<A HREF=" #.nmap.make.q">figure</A>.
+<P>
+<A NAME=.nmap.make><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of NMAP's map-making interface. 
+<A HREF="../fig/nmap_make.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR><BR>See <A HREF=" #.nmap.make.q">figure</A> for the QMAPS and QDATS branches; by default, these branches are bypassed. 
+<BR><BR>(The rightmost column in the diagram is irrelevant for map-making in NMAP.) </i>
+<P>
+<A NAME=.nmap.make.q><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the optional detailed-question sequences of the map-making interface. This diagram expands the <em>QMAPS</em> and <em>QDATAS</em> stubs in 
+<A HREF="../fig/nmap_make_q.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><A HREF=" #.nmap.make">figure</A>. </i>
+<P>
+<A NAME=.nmap.handle><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of NMAP's map-handling interface. } 
+<A HREF="../fig/nmap_handle.ps"><STRONG>FIGURE</STRONG></A> 
+ .]{<i><A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+</i><H1><A NAME=SECTION0004000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmap_public_intfc/nmap_public_intfc.html">NMAP</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../nshow_public_intfc/nshow_public_intfc.html">NSHOW</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../unit_public_intfc/unit_public_intfc.html">UNIT</A> public keywords 
+<LI> <A HREF="../wmpnode_public_intfc/wmpnode_public_intfc.html">WMPNODE</A> public keywords 
+<LI> <A HREF="../wmpsets_public_intfc/wmpsets_public_intfc.html">WMPSETS</A> public keywords 
+</UL>
+<P>
+<A NAME=.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0004200000000000000>  <b>Parameter AREA</b></A></H2>
+<P>
+  <em>Prompt:</em> Area: l,m, dl,dm<BR><em>Expected input:</em> Integer:  1 to 4 values
+<P>
+    <PRE>
+Specify the area to be selected:
+</PRE>
+<P>
+  <PRE>
+        l, m    position in grid spacings of centre of area
+                0,0 is the map centre, increaing toward the upper right (i.e.
+                 with DEcreasing RA and INcreasing DEC)
+</PRE>
+<P>
+  <PRE>
+        dl, dm  horizontal and vertical area sizes
+</PRE>
+<P>
+<A NAME=.bas.resolution><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004300000000000000>  <b>Parameter BAS_RESOLUTION</b></A></H2>
+<P>
+<em>Prompt:</em> Baseline averaging interval (m)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the width in metres of baseline over which visibilities will be
+averaged.
+</PRE>
+<P>
+  <PRE>
+The minimum value is 9, representing the smallest baseline increment ever
+present in practice in a (set of) WSRT observation(s). The maximum is
+(arbitrarily) fixed at 300.
+</PRE>
+<P>
+<A NAME=.clipping><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004400000000000000>  <b>Parameter CLIPPING</b></A></H2>
+<P>
+<em>Prompt:</em> Clipping?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+'Clipping' means discarding data in a certain annulus that fall within a
+certain range of values (yet to be specified).
+</PRE> 
+ <em>parameters <A HREF="#.clip.area">CLIP_AREA</A>,
+                 <A HREF="#.clip.levels">CLIP_LEVELS</A> </em>
+<P>
+  <PRE>
+It is a simple (and primitive) method of eliminating data affected by strong
+interference. (Note that NFLAG provides a much wider scala of operations to
+find and suppress interference.)
+</PRE>
+<P>
+<A NAME=.clip.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004500000000000000>  <b>Parameter CLIP_AREA</b></A></H2>
+<P>
+<em>Prompt:</em> UV-radius range for clipping (m)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the (circular) UV-plane radii (in metres) between which you want to
+clip the data. The default is to clip everywhere.
+</PRE>
+<P>
+<A NAME=.clip.levels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004600000000000000>  <b>Parameter CLIP_LEVELS</b></A></H2>
+<P>
+<em>Prompt:</em> Amplitude range to be discarded<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify amplitude range (in Westerbork Units) of visibility magnitudes that you
+want to discard.
+</PRE>
+<P>
+  <PRE>
+In the annulus defined by CLIP_AREA, values between the limits you specify will
+be discarded.
+</PRE> 
+ <em>parameter <A HREF="#.clip.area">CLIP_AREA</A> </em>
+<P>
+  <PRE>
+NOTE: It would be more natural to define a range within which visibilities are
+considered valid. As it is, only the lower limit is actually useful, allowing
+you to define a rejection threshold for interference. To do so, specify your
+threshold for the lower and 'infinity' for the upper limit, e.g.
+</PRE>
+<P>
+  <PRE>
+                <threshold>,100000
+</PRE>
+<P>
+<A NAME=.comment><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004700000000000000>  <b>Parameter COMMENT</b></A></H2>
+<P>
+<em>Prompt:</em> FITS comment (<IMG ALIGN=BOTTOM ALT="" SRC="_26913_tex2html_wrap580.png"><BR><em>Expected input:</em> Character *70:  1 value
+<P>
+  <PRE>
+The given text will be included as COMMENT in FITS output.
+</PRE>
+<P>
+<A NAME=.convolve><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004800000000000000>  <b>Parameter CONVOLVE</b></A></H2>
+<P>
+<em>Prompt:</em> Convolution type<BR><em>Expected input:</em> Character:  1 value
+<P>
+  <PRE>
+This is the interpolation function to be used in horizontally and vertically
+interpolating the observed visibilities onto the rectangular grid to be used in
+the Fast Fourier Transform.
+</PRE>
+<P>
+  <PRE>
+The choice of function determines the detailed aliasing properties of the
+map(s). NMAP chooses appropriate horizontal and vertical width parameters for
+each. You may specify one of the following functions:
+</PRE>
+<P>
+  <PRE>
+   Gaussian-based:
+</PRE>
+<P>
+  <PRE>
+        EXPSINC Sinc*exp on 6*6 grid points: An 'approximation' to the ideal
+                 sinc (=sin(x)/x) function. This is the function selected as the
+                 default for map-making after extensive experience with all of
+                 the options available here.
+        GAUSS   Gaussian type over 4*4 grid points: The function used in the
+                 first years of WSRT operations; it was later replaced by the
+                 prolate spheroids. The expense in computing time is the same as
+                 for P4ROL.
+</PRE>
+<P>
+  <PRE>
+   Prolate spheroids: These function minimise the 'power' (= the integral of the
+    intensity squared) 'aliased in' from sources outside the map
+</PRE>
+<P>
+  <PRE>
+        P4ROL   Prolate spheroidal function with 4*4 grid points.
+        P6ROL   Prolate spheroidal function with 6*6 grid points: By using more
+                 points in the interpolation, this function pushes the aliasing
+                 down considerably, - at the expense of a factor two or more in
+                 computing time for the interpolation
+</PRE>
+<P>
+  <PRE>
+All the above functions may also be used in constructing a UV-plane for display
+(UV_COORDINATES=UV).
+</PRE>
+<P>
+  <PRE>
+For plotting visibilities versus baseline or interferometer
+(UV_COORDINATES=BASHA or IFRHA), they are of little use, and the default one
+would normally select is
+</PRE>
+<P>
+  <PRE>
+        BOX     Shift to nearest grid point.
+</PRE> 
+ <em>see parameter <A HREF="#.uv.coordinates">UV_COORDINATES</A> </em>
+<P>
+<A NAME=.csum.factors><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0004900000000000000>  <b>Parameter CSUM_FACTORS</b></A></H2>
+<P>
+<em>Prompt:</em> Summing multipliers<BR><em>Expected input:</em> Real:  1 to 16 values
+<P>
+  <PRE>
+Specify up to 8 complex weight factors by which the input maps have to be
+multiplied. For each factor the real part should be given first, the imaginary
+next. So 1,0,0,-1  means add the real part of the first map-pair to the
+imagingary part of the second map-pair:
+</PRE>
+<P>
+  <PRE>
+    (1+0*i)*(map1r + i*map1i) + (0-1*i)*(map2r + i*map2i)
+</PRE>
+<P>
+  <PRE>
+If the number of weights you give is less than the number of maps  to be
+combined, the weights will re-used in a cyclic fashion. Example:
+        1,1,-1,-1 will average the first, third, ... pairs in your WMP_SETS
+specification with the negated second, fourth ... pairs.
+</PRE>
+<P>
+<A NAME=.cubic><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041000000000000000>  <b>Parameter CUBIC</b></A></H2>
+<P>
+<em>Prompt:</em> Make line cube (Yes/No) ?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want to output the FITS maps in one cube or in separate maps
+</PRE>
+<P>
+<A NAME=.data.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041100000000000000>  <b>Parameter DATA_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> Action to perform on the data<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+        SHOW    show detailed map data
+</PRE>
+<P>
+  <PRE>
+        NOISE   calculate noise
+        OFFSET  calculate noise and offset
+</PRE>
+<P>
+  <PRE>
+        QUIT    quit data part
+</PRE>
+<P>
+<A NAME=.data.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041200000000000000>  <b>Parameter DATA_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Data transformation for display<BR><em>Expected input:</em> Character:  1 value
+<P>
+  <PRE>
+Specify how to transform the complex input visibilities. NORMAL is the default;
+the others are for special experiments and diagnostics only.
+</PRE>
+<P>
+  <PRE>
+        NORMAL  Complex value
+</PRE>
+<P>
+  <PRE>
+        COS     Real part
+        SIN     Imaginary part
+</PRE>
+<P>
+  <PRE>
+        AMPL    Amplitude
+        PHASE   Phase
+</PRE>
+<P>
+<A NAME=.deconvolve><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041300000000000000>  <b>Parameter DECONVOLVE</b></A></H2>
+<P>
+<em>Prompt:</em> Correct map for convolution taper (Yes/No) ?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+The interpolation (convolution) in the visibility domain results in a
+multiplication ('tapering') of the output map(s) and antenna pattern(s) by the
+Fourier transform of the convolving function; i.e., toward the edge of the map
+the sources, sidelobes and grating responses appear weaker than they actually
+are.
+</PRE>
+<P>
+  <PRE>
+By default this effect will be corrected for by dividing the map through the
+taper. A side effect of this correction is that the noise, which is uniform
+over the whole uncorrected map, is amplified toward the map edges.
+</PRE>
+<P>
+  <PRE>
+Here you are given the option to bypass this correction. e.g. because uniform
+noise is more important for your application than source fluxes.
+</PRE>
+<P>
+<A NAME=.fiddle.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041400000000000000>  <b>Parameter FIDDLE_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Fiddle action|<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify action to perform.
+</PRE>
+<P>
+  <PRE>
+   In-place modifications: Modify data of (an) input image(s):
+</PRE>
+<P>
+  <PRE>
+        BEAM    correct map for primary beam attenuation so it will represent
+                 the 'true' sky
+        DEBEAM  apply primary beam attenuation to map so it will reprsent the
+                 product of the 'true' sky and the primary beam
+        FACTOR  multiply image with a constant factor
+</PRE>
+<P>
+  <PRE>
+   Unary operations: Create 1 new image from each input image:
+</PRE>
+<P>
+  <PRE>
+        EXTRACT extract an area from (a) image(s)
+        COPY    copy image(s)
+        LOAD    read or write (an) image(s) in a foreign format (e.g. Holog)
+</PRE>
+<P>
+  <PRE>
+   Binary combinations: make (a) new output image(s) from (a) pair(s) of input
+   images:
+</PRE>
+<P>
+  <PRE>
+        ADD     weighted sum of two images: F1*image1 + F2*image2
+        AVER    weighted average of two images:
+                        (F1*image1 + F2*image2) / [abs(F1) + abs(F2)]
+        POL     degree of linear polarisation from Q and U maps:
+                        sqrt (Qmap**2 + Umap**2)]
+        ANGLE   polarisation orientation (radians) from Q and U maps:
+                        0.5*atan (Umap / Qmap)
+</PRE>
+<P>
+  <PRE>
+   Combinations of more than two images:
+</PRE>
+<P>
+  <PRE>
+        SUM     weighted summation of (a) set(s) of images in a single .WMP file
+                 (you will be prompted to select the weighing method)
+        CSUM    weighted summation of pairs of images. You will be prompted
+                 for (a) set(s) of "real" images and (a) set(s) of
+                 "imaginary" images and complex weighting factors.
+        RSUM    idem, but the complex weighting factors will be calculated
+                 based on a specified rotation measure.
+        MOSCOM  'mosaic combine': merge a set of maps (generally for different
+                 field centres) into one output map
+</PRE>
+<P>
+  <PRE>
+   Miscellaneous:
+</PRE>
+<P>
+  <PRE>
+        QUIT    Return to OPTIONS level
+</PRE>
+<P>
+<A NAME=.field.centre><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041500000000000000>  <b>Parameter FIELD_CENTRE</b></A></H2>
+<P>
+<em>Prompt:</em> Field centre: RA,DEC (decimal deg)<BR><em>Expected input:</em> DoublePrecision:  1 to 2 values
+<P>
+  <PRE>
+Specify the map centre wanted in the apparent-coordinate frame.
+Default is the fringe-stopping centre.
+</PRE>
+<P>
+<A NAME=.field.shift><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041600000000000000>  <b>Parameter FIELD_SHIFT</b></A></H2>
+<P>
+<em>Prompt:</em> l,m field shift (arcsec)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the field-centre shift in l,m coordinates.
+</PRE>
+<P>
+  <PRE>
+(l,m) are 'horizontal' and 'vertical' Cartesian coordinates in a plane tangent
+to the celestial sphere at the reference centre. The coordinate system is
+B1950/J2000 or apparent as defined by your value for parameter MAP_COORD.
+</PRE> 
+      <i>See <A HREF="#.map.coord">MAP_COORD</A>,
+               <A HREF="#.ref.coord">REF_COORD</A> </i>
+<P>
+  <PRE>
+If you enter a null value (\ or ""), you will be prompted for a FIELD_CENTRE
+instead. This option is intended for instrumental test programs only and has
+not been tested for general applications; use it at your own risk if you wish.
+</PRE>
+<P>
+<A NAME=.field.size><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041700000000000000>  <b>Parameter FIELD_SIZE</b></A></H2>
+<P>
+<em>Prompt:</em> Fieldsize l,m (deg)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the l and m field size of the map to be transformed. The default will
+produce a map with a resolution of about 3.5 grid intervals per
+synthesized-beam half-width.
+</PRE>
+<P>
+  <PRE>
+If you give a NULL answer (two double quotes), you will be prompted for the
+grid steps.
+</PRE>
+<P>
+<A NAME=.filename><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041800000000000000>  <b>Parameter FILENAME</b></A></H2>
+<P>
+<em>Prompt:</em> Name for output disk file<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the file name (without an extension) to be used in creating a
+pseudo-tape output file name (e.g. FITS write).
+</PRE>
+<P>
+  <PRE>
+Specify a full filename otherwise (e.g. LOAD/UNLOAD in FIDDLE).
+</PRE>
+<P>
+<A NAME=.fits.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00041900000000000000>  <b>Parameter FITS_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> Units of source flux<BR><em>Expected input:</em> Character *4:  1 value
+<P>
+  <PRE>
+Specify the output units of the FITS data:
+</PRE>
+<P>
+  <PRE>
+        JY      jansky per beam
+        WU      Westerbork units (1 W.U. = 5 mJy)
+</PRE>
+<P>
+<A NAME=.ft.size><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042000000000000000>  <b>Parameter FT_SIZE</b></A></H2>
+<P>
+<em>Prompt:</em> FFT size<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+Specify the size of the Fourier transform in the horizontal and vertical
+directions.
+</PRE>
+<P>
+  <PRE>
+If the size in both direction is <= 17, a Direct Fourier Transform (DFT) will
+be made instead of the standard operation of interpolating onto a rectangular
+grid followed by a Fast Fourier Transform (FFT).
+</PRE>
+<P>
+  <PRE>
+The standard operation suffers from 'aliasing' artefacts associated with the
+periodic nature of the FFT. These artefacts are suppressed, to a level that is
+generally acceptable, through a very careful choice of the convolution function
+used in the interpolstion to a rectangular grid, but they cannot be avoided
+completely.
+</PRE>
+<P>
+  <PRE>
+By avoiding the interpolation altogether, the DFT method is free from these
+aliasing effects.
+</PRE>
+<P>
+<A NAME=.grid.size><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042100000000000000>  <b>Parameter GRID_SIZE</b></A></H2>
+<P>
+<em>Prompt:</em> Grid interval in l,m (arcsec)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the l and m grid steps in arcseconds for the map to be made.
+In most applications you may define GRID_SIZE as you please. NOTE however, that
+any number of maps that you want to combine into a single mosaic (FIDDLE MOSCOM
+option) must all share the same GRID_SIZE (as well as the same reference
+coordinates, parameters MAP_COORD and REF_COORD)
+</PRE> 
+      <em>See <A HREF="#.map.coord">MAP_COORD</A>,
+               <A HREF="#.ref.coord">REF_COORD</A> </em>
+<P>
+<A NAME=.ha.resolution><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042200000000000000>  <b>Parameter HA_RESOLUTION</b></A></H2>
+<P>
+<em>Prompt:</em> Hour-angle averaging interval (UT seconds)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the width in UT degrees of hour angle over which visibilities will be
+averaged (to reduce the noise per plotted point).
+</PRE>
+<P>
+  <PRE>
+Note:   Observations are taken at multiples of 10 UT seconds and it is
+        therefore convenient to specify this parameter in UT seconds as well.
+        The number you specify will be converted to a sidereal hour-angle
+        interval.
+</PRE>
+<P>
+<A NAME=.ifr.resolution><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042300000000000000>  <b>Parameter IFR_RESOLUTION</b></A></H2>
+<P>
+<em>Prompt:</em> Interferometer separation<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the vertical separation in grid points between interferometers
+</PRE>
+<P>
+<A NAME=.input.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042400000000000000>  <b>Parameter INPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> Input file name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the file name (including extension) of the file to be converted.
+</PRE>
+<P>
+<A NAME=.input.labels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042500000000000000>  <b>Parameter INPUT_LABELS</b></A></H2>
+<P>
+<em>Prompt:</em> Input tape labels<BR><em>Expected input:</em> Integer:  1 to 256 values
+<P>
+  <PRE>
+Specify the tape labels to be read. * specifies all labels on the tape.
+</PRE>
+<P>
+  <PRE>
+Remember that WMP-file images are identified by indices grp.obs.fld.chn.seq).
+Each of the selected tape labels will be stored in the WMP-file as a separate
+field (FLD) in the group (GRP) being created. The CHN, POL and TYP indices will
+reflect the nature of the input data, SEQ will be 0.
+</PRE>
+<P>
+  <PRE>
+Example:
+        INPUT_LABELS=3,6,8 will cause a new GRP to be created in which these
+labels will be stored under the image indices
+</PRE>
+<P>
+  <PRE>
+        <newgrp>. 0. <chn for label 3>. <pol for label 3>. <typ for label 3>. 0
+        <newgrp>. 1. <chn for label 6>. <pol for label 6>. <typ for label 6>. 0
+        <newgrp>. 2. <chn for label 8>. <pol for label 8>. <typ for label 8>. 0
+</PRE>
+<P>
+<A NAME=.lm.centre><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042600000000000000>  <b>Parameter LM_CENTRE</b></A></H2>
+<P>
+<em>Prompt:</em> Output map centre<BR><em>Expected input:</em> DoublePrecision:  1 to 2 values
+<P>
+  <PRE>
+Specify the centre of the output map in the l and m direction; in arcsec with
+respect to the mosaic reference position.
+</PRE>
+<P>
+  <PRE>
+If you specify an *, you will prompted for RA,DEC position
+</PRE>
+<P>
+<A NAME=.load.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042700000000000000>  <b>Parameter LOAD_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Load action/image type |<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify the type of foreign map and what to do with it:
+</PRE>
+<P>
+  <PRE>
+        WMP      read WMP format maps from contiguous binary file
+        UNLOAD   inverse of WMP: write WMP maps to contiguous binary file
+                  this option can also be used to load in an SAOIMAGE file
+                  (specify a data offset of 512)
+</PRE>
+<P>
+  <PRE>
+        NEWHOLOG read HOLOG file from the WSRT (this option, synonymous with
+                  WMP, was added to help the user)
+        OLDHOLOG read a Holog map in old IBM-coded format (this option used to
+                  be called HOLOG)
+</PRE>
+<P>
+  <PRE>
+        QUIT    quit LOADing
+</PRE>
+<P>
+<A NAME=.map.coord><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042800000000000000>  <b>Parameter MAP_COORD</b></A></H2>
+<P>
+<em>Prompt:</em> Map coordinate system|<BR><em>Expected input:</em> Character *12:  1 value
+<P>
+  <PRE>
+Specify the coordinate system for the map.
+</PRE>
+<P>
+  <PRE>
+There are two choices to be made: The first is whether the map is to be made in
+apparent coordinates for the epoch of the observation or in fixed-epoch
+coordinates. The latter are fixed for each instrument: B1950 for the WSRT,
+J2000 for the ATNF. The second choice is whether the 'reference position' for
+the map must coincide with the fringe-stopping centre or is to be specified by
+you.
+</PRE>
+<P>
+  <PRE>
+The reference position is the position at which the map plane is tangent to the
+celestial sphere; it defines the geometry of the map's (l,m) grid in terms of
+RA and DEC.
+</PRE>
+<P>
+  <PRE>
+The reference position is important for mosaic mapping: The FIDDLE/MOSCOM
+operation that combines mosaic subfields into a single large map will only work
+if all input maps have the same reference.
+</PRE>
+<P>
+  <PRE>
+For a single mosaic, the program by default uses the mosaic centre as the
+reference for all subfield maps. However, if you intend to combine multiple
+mosaics into a 'super-mosaic', only you can define the common reference centre
+that will be needed.
+</PRE>
+<P>
+  <PRE>
+You have the following options for your reply:
+</PRE>
+<P>
+  <PRE>
+   Reference position defined by the observation (i.e. coinciding with the
+    fringe stopping centre):
+</PRE>
+<P>
+  <PRE>
+        B1950_J2000   in epoch coordinates for the epoch defined by the
+                       instrument with which the observation was made:
+                        B1950 for the WSRT
+                        J2000 for the ATNF
+</PRE>
+<P>
+  <PRE>
+        APPARENT      in apparent coordinates at the time of observation
+</PRE>
+<P>
+  <PRE>
+   Reference position to be defined by the user through an additional parameter
+    REF_COORD:
+</PRE>
+<P>
+  <PRE>
+        REFER         in B1950_J2000 coordinates
+</PRE>
+<P>
+  <PRE>
+        AREFER        in APPARENT coordinates. Note that this will not work for
+</PRE>
+<P>
+<A NAME=.map.factors><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00042900000000000000>  <b>Parameter MAP_FACTORS</b></A></H2>
+<P>
+<em>Prompt:</em> Input-map multipliers<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the factors by which the input maps have to be multiplied.
+</PRE>
+<P>
+  <PRE>
+You may specify up to 8 factors which will be used as multipliers in the
+weighted summation the input maps you selected. If there are more maps to be
+summed than factors specified, the factors will be cyclically re-used.
+</PRE>
+<P>
+<A NAME=.map.level><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043000000000000000>  <b>Parameter MAP_LEVEL</b></A></H2>
+<P>
+<em>Prompt:</em> Polarisation threshold (W.U)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the minimum level in Wetsrebork Units that is still to be considered
+valid linear polarisation. Polarisation levels below this threshold will be set
+to zero in the output map(s).
+</PRE>
+<P>
+<A NAME=.map.polar><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043100000000000000>  <b>Parameter MAP_POLAR</b></A></H2>
+<P>
+<em>Prompt:</em> Select 1 to 4 output-map polarisation(s)|<BR><em>Expected input:</em> Character *4:  1 to 4 values
+<P>
+  <PRE>
+Specify up to four polarisations for the maps to make:
+</PRE>
+<P>
+  <PRE>
+        XX      XX only
+        XY      XY only
+        YX      YX only
+        YY      YY only
+</PRE>
+<P>
+  <PRE>
+        I       Stokes I
+        L       'line' Stokes I: Incomplete input data (e.g. no valid XX or YY)
+                 will be filled in aassuming that the field is unpolarised
+                 (Q=U=V=0)
+        Q       Stokes Q
+        U       Stokes U
+        V       Stokes V
+</PRE>
+<P>
+  <PRE>
+Each of the above may be suffixed with 'I' to indicate that visibilities must
+be pre-multiplied with sqrt(-1)
+</PRE>
+<P>
+<A NAME=.old.dattyp><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043200000000000000>  <b>Parameter OLD_DATTYP</b></A></H2>
+<P>
+<em>Prompt:</em> Old R-series data format<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the old R-series data type:
+</PRE>
+<P>
+  <PRE>
+        0       local
+        1       VAX, D_FORMAT
+        2       VAX, G_FORMAT
+        3       ALLIANT
+        4       CONVEX
+        5       IEEE
+        6       DEC station
+        7       SUN station
+        8       HP  station
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043300000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Action|<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+  Primary operations:
+        MAKE      make map(s) from visibility data in .SCN file
+        FIDDLE    combine or change maps in .WMP file
+</PRE>
+<P>
+  <PRE>
+  FITS conversions:
+        W16FITS   write FITS tape/disk with 16 bits data
+        W32FITS   write FITS tape/disk with 32 bits data
+        WRLFITS   write FITS tape/disk with 32 bits float data
+        RFITS     read FITS tape/disk data
+</PRE>
+<P>
+  <PRE>
+  Miscellaneous:
+        SHOW      show/edit map data
+        QUIT      finish
+</PRE>
+<P>
+  <PRE>
+  Format conversions:
+        CVX       convert a map file from other machine's format to local
+                   machine's
+        NVS       convert a map file to newest version. Needs to be run only if
+                   indicated by program
+        FROM_OLD  convert from R-series format
+        TO_OLD    convert to R-series format
+</PRE>
+<P>
+<A NAME=.output><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043400000000000000>  <b>Parameter OUTPUT</b></A></H2>
+<P>
+<em>Expected input:</em> Character *8:  1 to 8 values
+<P>
+  <PRE>
+Specify one or more output types:
+</PRE>
+<P>
+  <PRE>
+   Standard image types for map-making:
+        MAP     Output (a) map(s)
+        AP      Output (an) antenna pattern(s)
+</PRE>
+<P>
+  <PRE>
+   Visibility-domain outputs, for diagnostics only:
+        COVER   Output the 'antenna-pattern' convolved visibilities
+</PRE>
+<P>
+  <PRE>
+        REAL    Output the real part of the convolved visibilities
+        IMAG    Output the imaginary part of the convolved visibilities
+</PRE>
+<P>
+  <PRE>
+        AMPL    Output the amplitude of the convolved visibilities
+        PHASE   Output the phase of the convolved visibilities
+</PRE>
+<P>
+<A NAME=.output.label><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043500000000000000>  <b>Parameter OUTPUT_LABEL</b></A></H2>
+<P>
+<em>Prompt:</em> Output label<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the first output tape label. If this label already exists, it and all
+the subsequent labels will be overwritten.
+Specify * or 0 to write the new label behind all existing ones.
+</PRE>
+<P>
+<A NAME=.out.centre><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043600000000000000>  <b>Parameter OUT_CENTRE</b></A></H2>
+<P>
+<em>Prompt:</em> Output map centre<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+Specify the centre of the output map in the l and m direction in pixels with
+respect to the mosaic reference position.
+</PRE>
+<P>
+  <PRE>
+If you specify an *, you will be prompted for l,m and RA,DEC position
+</PRE>
+<P>
+<A NAME=.out.size><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043700000000000000>  <b>Parameter OUT_SIZE</b></A></H2>
+<P>
+<em>Prompt:</em> Output map size<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+Specify the size in grid points of the output map(s) in the horizontal and
+vertical directions.
+</PRE>
+<P>
+<A NAME=.qdatas><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043800000000000000>  <b>Parameter QDATAS</b></A></H2>
+<P>
+<em>Prompt:</em> Special data selection (Yes/No) ?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Maps are normally made directly from the .SCN-file visibilities. Answering YES
+here gives you access to some specials including
+</PRE>
+<P>
+  <PRE>
+        - making a map from model visibilities in the .SCN file;
+        - selecting visibilities from an annulus in the UV plane;
+        - clipping extreme amplitudes in an annulus in the UV plane;
+        - shifting the pointing centre to which the visibilities refer (and
+           consequently the centre of the map to be made from them).
+</PRE>
+<P>
+<A NAME=.radec.centre><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00043900000000000000>  <b>Parameter RADEC_CENTRE</b></A></H2>
+<P>
+<em>Prompt:</em> Output map centre: RA,DEC (decimal deg)<BR><em>Expected input:</em> DoublePrecision:  1 to 2 values
+<P>
+  <PRE>
+Specify the centre of the output map: RA and DEC in decimal degrees.
+</PRE>
+<P>
+<A NAME=.ref.coord><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044000000000000000>  <b>Parameter REF_COORD</b></A></H2>
+<P>
+<em>Prompt:</em> Map reference coordinates: RA,DEC (decimal deg)<BR><em>Expected input:</em> DoublePrecision:  1 to 2 values
+<P>
+  <PRE>
+Specify (in decimal degrees) the RA and DEC of the reference coordinates to use
+in producing the map. The coordinate system is B1950/J2000 or apparent as
+defined by your value for parameter MAP_COORD.
+</PRE>
+<P>
+<A NAME=.rotation.measure><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044100000000000000>  <b>Parameter ROTATION_MEASURE</b></A></H2>
+<P>
+<em>Prompt:</em> Rotation measure<BR><em>Expected input:</em> Real:  1 to 64 values
+<P>
+  <PRE>
+Specify one (or more) rotation measure(s) (RM). Pairs of input maps will be
+phase-rotated to the the frequency of the first input map and averaged:
+    THETAn = 2 * RM * ( (c/FRQn)**2 -  (c/FRQ1)**2 )
+    Qout = SUM( Wn * ( cos(THETAn)*Qn - sin(THETAn)*Un ) ) / SUM( Wn )
+    Uout = SUM( Wn * ( sin(THETAn)*Qn + cos(THETAn)*Un ) ) / SUM( Wn )
+A pair of Qout/Uout will be produced for each RM given. E.g. to get average Q/U
+maps for rotation measures from 0 to 5 with intervals of 0.5, specify
+ROTATION_MEASURE=0 TO 5 BY 0.5.
+</PRE>
+<P>
+<A NAME=.subtract><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044200000000000000>  <b>Parameter SUBTRACT</b></A></H2>
+<P>
+<em>Prompt:</em> Model subtraction (Yes/No) ?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Reply YES if you want to subtract a source model. You will then be prompted to
+provide details on the model you want to subtract.
+</PRE> 
+ <em>see the <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL HANDLE</A> interface </em>
+<P>
+<A NAME=.sum.factors><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044300000000000000>  <b>Parameter SUM_FACTORS</b></A></H2>
+<P>
+<em>Prompt:</em> Summing multipliers<BR><em>Expected input:</em> Real:  1 to 8 values
+<P>
+  <PRE>
+Specify up to 8 weight factors by which the input maps have to be multiplied.
+If the number of weights you give is less than the number of maps to be
+combined, the weights will re-used in a cyclic fashion.
+</PRE>
+<P>
+  <PRE>
+Example:
+        1,-1 will average the first, third, ... maps in your WMP_SETS
+specification with the negated second, fourth ... maps.
+</PRE>
+<P>
+  <PRE>
+Note: When used together with the RSUM option, the weights will be used both
+for the Real and Imaginary map (they are real weights).
+</PRE>
+<P>
+<A NAME=.sum.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044400000000000000>  <b>Parameter SUM_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Weighing method<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify the type of weight to use in the averaging. In all cases the summation
+produces a weighted average map over all SETS_1, the weights depending on the
+method you select:
+</PRE>
+<P>
+  <PRE>
+        SUM     weight(i)= 1
+        NSUM    weight(i)= normalisation factor of map(i)
+        NSSUM   weight(i)= 1 / (<noise in map(i)>**2)
+</PRE>
+<P>
+  <PRE>
+        BSUM    weight(i)= bandwidth of map(i)
+        BNSUM   weight(i)= bandwidth * normalisation factor of map(i)
+</PRE>
+<P>
+  <PRE>
+        FSUM    weight(i)= factors to be specified by you.
+</PRE>
+<P>
+  <PRE>
+        QUIT    quit AVERaging
+</PRE>
+<P>
+<A NAME=.taper><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044500000000000000>  <b>Parameter TAPER</b></A></H2>
+<P>
+<em>Prompt:</em> Taper type<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+The taper is a function of baseline length used to de-emphasize the long
+baselines and consequently reduce the near-in sidelobes of the synthesized beam.
+</PRE>
+<P>
+  <PRE>
+You may specify the following functions, some of them to be supplemented later
+with a baseline-scale parameter TAPER_VALUE:
+</PRE> 
+ <em>see public parameter
+  <A HREF="../nmap_public_intfc/nmap_public_intfc.html#.taper.value">TAPER_VALUE</A> </em>
+<P>
+  <PRE>
+        GAUSS    exp -(<baseline>/TAPER_VALUE)**2
+                 standard WSRT beam: good compromise between near-in sidelobes,
+                  beam width and noise
+</PRE>
+<P>
+  <PRE>
+        LINEAR   max (0, 1-baseline/TAPER_VALUE)
+</PRE>
+<P>
+  <PRE>
+        OVERR    1 / baseline   (no scale)
+</PRE>
+<P>
+  <PRE>
+        RGAUSS   exp -(<baseline>/TAPER_VALUE)**2 / <baseline>
+                 broader beam, very low near-in sidelobes, poorer noise
+</PRE>
+<P>
+  <PRE>
+        NATURAL  no taper       (no scale)
+                 optimum signal/noise ratio, narrower beam with very strong
+                  near-in sidelobes
+</PRE>
+<P>
+  <PRE>
+NOTES: - Unless you have specified UNIFORM=NATURAL for the UV coverage mode, the
+        1/<baseline> density variation of measured visibility points is already
+        being accounted for, so OVERR and RGAUSS should not be chosen. LINEAR
+        does not combine very well with NATURAL either.
+</PRE> 
+ <em>cf. parameter <A HREF="../nmap_public_intfc/nmap_public_intfc.html#.uniform">UNIFORM</A> </em>
+<P>
+<A NAME=.user.comment><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044600000000000000>  <b>Parameter USER_COMMENT</b></A></H2>
+<P>
+<em>Prompt:</em> Comment to be included in map header(s) (<IMG ALIGN=BOTTOM ALT="" SRC="_26913_tex2html_wrap580.png"><BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Give, optionally, a descriptive comment for the maps.
+</PRE>
+<P>
+<A NAME=.user.data><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044700000000000000>  <b>Parameter USER_DATA</b></A></H2>
+<P>
+<em>Prompt:</em> Visibilities to use<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify the type of visibilities to use:
+</PRE>
+<P>
+  <PRE>
+        STANDARD  observed visibilities
+</PRE>
+<P>
+  <PRE>
+        MODEL     model visibilities (to be specified later with type=0
+sources)
+</PRE>
+<P>
+<A NAME=.use.noise><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044800000000000000>  <b>Parameter USE_NOISE</b></A></H2>
+<P>
+<em>Prompt:</em> Weigh with noise (Yes/No) ?<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want the noise of the individual maps to be used as a weight in
+the MOSCOM combination
+</PRE>
+<P>
+<A NAME=.uv.coordinates><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00044900000000000000>  <b>Parameter UV_COORDINATES</b></A></H2>
+<P>
+<em>Prompt:</em> UV coordinate system<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify the type of UV coordinates wanted for UV-plane type output
+</PRE> 
+ <em><A HREF="#.output">OUTPUT</A>: COVER, REAL, IMAG, AMPL, PHASE options </em>
+<P>
+  <PRE>
+        UV      standard UV coordinates: interferometer tracks are ellipses
+</PRE>
+<P>
+  <PRE>
+        BASHA   hour-angle (horizontal) and interferometer baseline (vertical)
+                 coordinates: interferometer tracks are horizontal lines;
+                 redundant baselines overlap
+</PRE>
+<P>
+  <PRE>
+        IFRHA   as BASHA, but vertical axis is the interferometer ordinal number
+                 in the sequence 01,02,...,0D,12,13,...,CD)
+</PRE>
+<P>
+<A NAME=.wgt.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00045000000000000000>  <b>Parameter WGT_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Relative weight limit<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specifies the relative weight as compared to the expected maximum weight of
+data points combined on one line, below which no output will be generated
+</PRE>
+<P>
+<A NAME=.wmp.node.1><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00045100000000000000>  <b>Parameter WMP_NODE_1</b></A></H2>
+<P>
+<em>Prompt:</em> First WMP node name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the node name for the first Fiddle input set of images.
+</PRE>
+<P>
+<A NAME=.wmp.node.2><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00045200000000000000>  <b>Parameter WMP_NODE_2</b></A></H2>
+<P>
+<em>Prompt:</em> Second WMP node name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the node name for the second Fiddle input set of images.
+</PRE>
+<P>
+  <PRE>
+Specify * if this is the same as the first node (NODE_1).
+</PRE>
+<P>
+<A NAME=.wmp.set.1><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00045300000000000000>  <b>Parameter WMP_SET_1</b></A></H2>
+<P>
+<em>Prompt:</em> First image set(s) to be used: grp.fld.chn.pol.typ.seq<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+Specify the first image set(s) to be used.
+</PRE>
+<P>
+<A NAME=.wmp.set.2><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00045400000000000000>  <b>Parameter WMP_SET_2</b></A></H2>
+<P>
+<em>Prompt:</em> Second image set(s) to be used: grp.fld.chn.pol.typ.seq<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+Specify the second image Set(s) to be used
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+%!PS-Adobe-2.0
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+gs 1 -1 sc (*) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+1800 5700 m
+gs 1 -1 sc (*) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 5700 m
+gs 1 -1 sc (TAPER_VALUE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5100 5700 m
+gs 1 -1 sc (Taper width) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+3000 6000 m
+gs 1 -1 sc (set  TAPVAL) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 6600 m
+gs 1 -1 sc (CWEIGHT_TYPE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5100 6600 m
+gs 1 -1 sc (Circular taper function \(i.e. circular in the plane of the field\)) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+3000 7200 m
+gs 1 -1 sc (CWGTYP=1) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+2700 6900 m
+gs 1 -1 sc (NONE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+4500 6900 m
+gs 1 -1 sc (GAUSS) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+6600 6900 m
+gs 1 -1 sc (LINEAR) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+4800 7200 m
+gs 1 -1 sc (CWGTYP=2) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+6900 7200 m
+gs 1 -1 sc (CWGTYP=3) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+1800 6600 m
+gs 1 -1 sc (*) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 9900 m
+gs 1 -1 sc (DECONVOLVE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5100 9900 m
+gs 1 -1 sc (Undo map taper due to convolution?) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+10200 9900 m
+gs 1 -1 sc (set DECVL) col-1 show gr
+/Times-Italic findfont 300.00 scalefont setfont
+9300 2400 m
+gs 1 -1 sc (is selected) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+7200 2400 m
+gs 1 -1 sc (QMAPS=YES) col-1 show gr
+/Times-Italic findfont 300.00 scalefont setfont
+2700 2400 m
+gs 1 -1 sc (The following prompts appear only if  ) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 12900 m
+gs 1 -1 sc (USER_DATA) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 12900 m
+gs 1 -1 sc (Observed or model visibilities) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+2700 13200 m
+gs 1 -1 sc (STANDARD) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5100 13200 m
+gs 1 -1 sc (MODEL) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 14100 m
+gs 1 -1 sc (UV_AREA) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 14100 m
+gs 1 -1 sc (UV annulus selection) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 15000 m
+gs 1 -1 sc (UV annulus for clipping) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 14700 m
+gs 1 -1 sc (Clip visibilities with extreme amplitudes?) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+2700 15300 m
+gs 1 -1 sc (CLIP_LEVELS) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2700 15000 m
+gs 1 -1 sc (CLIP_AREA) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 15300 m
+gs 1 -1 sc (Lower and upper limits for valid visibility amplitudes) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 15900 m
+gs 1 -1 sc (FIELD_SHIFT) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 16200 m
+gs 1 -1 sc (Map centre) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 15900 m
+gs 1 -1 sc (Map shift) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2700 16200 m
+gs 1 -1 sc (FIELD_CENTRE) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+2400 16800 m
+gs 1 -1 sc (DATA_TYPE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+5700 16800 m
+gs 1 -1 sc (Visibility transformation) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+2700 17100 m
+gs 1 -1 sc (NORMAL) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+4800 17100 m
+gs 1 -1 sc (COSINE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+6900 17100 m
+gs 1 -1 sc (SINE) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+9000 17100 m
+gs 1 -1 sc (AMPL) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+11100 17100 m
+gs 1 -1 sc (PHASE) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+3000 17400 m
+gs 1 -1 sc (DATTYP=1) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+5100 17400 m
+gs 1 -1 sc (DATTYP=2) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+7200 17400 m
+gs 1 -1 sc (DATTYP=3) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+9300 17400 m
+gs 1 -1 sc (DATTYP=4) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+11400 17400 m
+gs 1 -1 sc (DATTYP=5) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+7800 16200 m
+gs 1 -1 sc (LSHIFT=-1, set CENTRE) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+7800 15900 m
+gs 1 -1 sc (LSHIFT=1, set SHIFT) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+12300 15300 m
+gs 1 -1 sc (set CLPLEV) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+9300 15000 m
+gs 1 -1 sc (set CLPRAD) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+9300 14100 m
+gs 1 -1 sc (set  UVRAD) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+5400 13500 m
+gs 1 -1 sc (UVDTP=1) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+3000 13500 m
+gs 1 -1 sc (UVDTP=0) col-1 show gr
+/Times-Bold findfont 240.00 scalefont setfont
+2400 14700 m
+gs 1 -1 sc (CLIPPING) col-1 show gr
+/Times-Italic findfont 300.00 scalefont setfont
+2700 12000 m
+gs 1 -1 sc (The following prompts appear only if  ) col-1 show gr
+/Times-Roman findfont 300.00 scalefont setfont
+7200 12000 m
+gs 1 -1 sc (QDATAS=YES) col-1 show gr
+/Times-Italic findfont 300.00 scalefont setfont
+9300 12000 m
+gs 1 -1 sc (is selected) col-1 show gr
+/Times-Italic findfont 300.00 scalefont setfont
+2400 600 m
+gs 1 -1 sc (UV-plane  or map-making mode  \(see previous figure\)) col-1 show gr
+/Times-Roman findfont 150.00 scalefont setfont
+11700 600 m
+gs 1 -1 sc (nmap_make_q.fig 50%) col-1 show gr
+/Times-Bold findfont 300.00 scalefont setfont
+1800 14175 m
+gs 1 -1 sc (*) col-1 show gr
+$F2psEnd
+restore
+
+%%EndDocument
+ @endspecial 0 2538 a Fg(Figure)11 b(1:)16 b Fj(Overview)11
+b(of)h(the)g(optional)h(detaile)n(d-question)f(se)n(quenc)n(es)h(of)f
+(the)g(map-making)h(interfac)n(e.)k(This)12 b(diagr)n(am)0
+2587 y(exp)n(ands)k(the)f Fg(QMAPS)h Fj(and)f Fg(QD)o(A)m(T)m(AS)f
+Fj(stubs)h(in)30 b(\014gur)n(e)15 b(1.7)g(.)935 2995
+y Fg(4)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nmap_public_intfc/images.pl b/nmap_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nmap_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nmap_public_intfc/labels.pl b/nmap_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..4e59fa21e8b9cbb984ba3a3ffc8c026f777d1396
--- /dev/null
+++ b/nmap_public_intfc/labels.pl
@@ -0,0 +1,16 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".uniform"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".overview"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".qmaps"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".cweight.value"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".uv.area"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".nmap.make.q"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".taper.value"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".nmap.make"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".cweight.type"} ="$URL/nmap_public_intfc.html"; 
+$external_labels{".memory.use"} ="$URL/nmap_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/nmap_public_intfc/nmap_public_intfc.html b/nmap_public_intfc/nmap_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..3c13945758d9606dac12b9257782c06ca9b3ec5b
--- /dev/null
+++ b/nmap_public_intfc/nmap_public_intfc.html
@@ -0,0 +1,252 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group NMAP</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nmap_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nmap_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<UL> 
+<LI> <A NAME=tex2html3 HREF=nmap_public_intfc.html#SECTION0002100000000000000>  <b>Parameter CWEIGHT_TYPE</b></A>
+<LI> <A NAME=tex2html4 HREF=nmap_public_intfc.html#SECTION0002200000000000000>  <b>Parameter CWEIGHT_VALUE</b></A>
+<LI> <A NAME=tex2html5 HREF=nmap_public_intfc.html#SECTION0002300000000000000>  <b>Parameter MEMORY_USE</b></A>
+<LI> <A NAME=tex2html6 HREF=nmap_public_intfc.html#SECTION0002400000000000000>  <b>Parameter QMAPS</b></A>
+<LI> <A NAME=tex2html7 HREF=nmap_public_intfc.html#SECTION0002500000000000000>  <b>Parameter TAPER_VALUE</b></A>
+<LI> <A NAME=tex2html8 HREF=nmap_public_intfc.html#SECTION0002600000000000000>  <b>Parameter UNIFORM</b></A>
+<LI> <A NAME=tex2html9 HREF=nmap_public_intfc.html#SECTION0002700000000000000>  <b>Parameter UV_AREA</b></A>
+</UL>
+</UL>
+<A NAME=.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group NMAP.This group is a subset of the map-making control parameters, viz. thoseparameters that are also used by NCLEAN in its 
+<A HREF="../nclean_descr/nclean_descr.html#.data.clean">"dataclean"</A> operation.
+<P>
+        The accompanying diagrams are to be found in the document describingNMAP's <A HREF="../nmap_private_intfc/nmap_private_intfc.html">private parameters</A>. This document contiansonly the descriptions of the individual parameters in alphabetical order. Thesecenter on the Help texts, which have been designed to guide the user to theproper choice at each junction, even if his knowledge of the overall workingsof the program is only superficial.
+<P>
+        The prompt and help texts defined for these parameters are those for NMAP. In the data-clean application, these may be overridden by texts more appropriate there. Unfortunately, the present architecture of 
+<i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.nmap.make.q><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the optional detailed-question sequences of the map-making interface. This diagram expands the <em>QMAPS</em> and <em>QDATAS</em> stubs in 
+<A HREF="../fig/nmap_make_q.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><A HREF=" #.nmap.make">figure</A>. </i>
+<P>
+        <A HREF=" #.nmap.make.q">Figure</A> gives a schematic overview of this part of NMAP'sparameter interface. (The companion diagram to which the figure refers is irrelevant in the present context, but you may find it in the description of NMAP's  <A HREF="../nmap_private_intfc/nmap_private_intfc.html#.nmap.make">private interface</A>.)
+<P>
+<A NAME=.cweight.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002100000000000000>  <b>Parameter CWEIGHT_TYPE</b></A></H2>
+<P>
+  <em>Prompt:</em> Circular weight type (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+    <PRE>
+ON TOP of the standard taper function which is circular in the equatorial UV
+plane, you nay specify a taper that is circular in the projected UV plane (i.e.
+the plane as seen from the field centre). You can select one out of the
+following functions:
+</PRE>
+<P>
+  <PRE>
+        GAUSS   exp -(<projected baseline>/CWEIGHT_VALUE)**2
+</PRE>
+<P>
+  <PRE>
+        LINEAR  max (0, 1-<projected baseline>/CWEIGHT_VALUE)
+</PRE>
+<P>
+  <PRE>
+        NATURAL unity weight everywhere, i.e. no circular taper
+</PRE>
+<P>
+  <PRE>
+NOTE that the circular weighing does not replace the standard tapering, but is
+applied as an EXTRA weight function. This is probably not what you want; you
+may eliminate the normal tapering by specifying TAPER=NATURAL and
+UNIFORM=STANDARD to take into account the radial density dependence of measured
+visibilities.
+</PRE>
+<P>
+<A NAME=.cweight.value><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002200000000000000>  <b>Parameter CWEIGHT_VALUE</b></A></H2>
+<P>
+<em>Prompt:</em> Circular-weight width (metres) (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the width for your circular weight function.
+</PRE>
+<P>
+  <PRE>
+If you have selected a gaussian for the circular_weight function
+(CWEIGHT_TYPE=GAUSS), the value you specify here will be the projected baseline
+radius for which the weight is 1/e times its value in the origin. The default
+value makes the weight equal to 1/4 at a projected baseline of 3000 m.
+</PRE>
+<P>
+  <PRE>
+If you have selected a triangular weight function (CWEIGHT_TYPE=LINEAR), the
+value you specify here is the projected baseline at which the weight reaches
+zero.
+</PRE>
+<P>
+<A NAME=.memory.use><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002300000000000000>  <b>Parameter MEMORY_USE</b></A></H2>
+<P>
+<em>Prompt:</em> Work memory size (<em>may vary per application</em>)<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify an approximate value for the work memory size to be used in the
+transform (bytes).
+</PRE>
+<P>
+<A NAME=.qmaps><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002400000000000000>  <b>Parameter QMAPS</b></A></H2>
+<P>
+<em>Prompt:</em> UV taper/convolution details? (<em>may vary per application</em>)<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+The standard defaults used for the taper and convolution functions in the
+map-making process will produce maps of excellent quality for normal
+applications at an acceptable expense of computing resources.
+</PRE>
+<P>
+  <PRE>
+There may be particular situations, however, where a non-standard taper and/or
+convolution function is more suitable. Answer YES if you want to make your own
+selection out of the possible options.
+</PRE>
+<P>
+<A NAME=.taper.value><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002500000000000000>  <b>Parameter TAPER_VALUE</b></A></H2>
+<P>
+<em>Prompt:</em> Taper half-width (metres) (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the baseline in metres of the taper function at which the taper
+function will fall to 1/e of its central value.
+</PRE>
+<P>
+  <PRE>
+The default is defined such that the taper function you selected has a value of
+1/4 for a baseline length of 3000 m.
+</PRE>
+<P>
+<A NAME=.uniform><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002600000000000000>  <b>Parameter UNIFORM</b></A></H2>
+<P>
+<em>Prompt:</em> Measure function for UV coverage (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify the way the UV coverage should be determined:
+</PRE>
+<P>
+  <PRE>
+        STANDARD: Weigh each observed point with the track length it covers in
+                   the UV plane, and average sets of redundant baselines. This
+                   method accounts properly for the fact that the density of
+                   measured points is inversely proportional to the baseline,
+                   for the multiplicity of redundant baselines and for
+                   variations in integration times.
+</PRE>
+<P>
+  <PRE>
+        FULL:     Weigh each point according to the actual UV point density. In
+                   this case care is also taken of all local UV plane density
+                   enhancements, e.g. because there is overlap between
+                   observations.
+</PRE>
+<P>
+  <PRE>
+        NATURAL:  Take each individual measured point separately, without
+                   weighing for the UV track covered by it. This option gives
+                   the maximum possible signal/noise ratio in your map, but it
+                   generally weighs the short baselines much too heavily which
+                   results in a very fat synthesized beam.
+</PRE>
+<P>
+  <PRE>
+Of these options, FULL gives the cleanest synthesized beam, but it is slower
+because it necessitates an extra read pass over the .SCN-file data.
+</PRE>
+<P>
+<A NAME=.uv.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002700000000000000>  <b>Parameter UV_AREA</b></A></H2>
+<P>
+<em>Prompt:</em> projected UV radius range (metres) (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the range of PROJECTED baselines for which you want to include the data.
+</PRE>
+<P>
+  <PRE>
+You may use this option, - at the expense of throwing away data -, for such
+purposes as
+</PRE>
+<P>
+  <PRE>
+        - To make the projected synthesised aperture and hence the synthesised
+           beam somewhat more circularly symmetric.
+</PRE>
+<P>
+  <PRE>
+        - To exclude noise from long projected baselines where you know there is
+           no signal of interest.
+</PRE>
+<P>
+  <PRE>
+        - To eliminate data from the short baselines, e.g. to suppress
+           interference.
+</PRE>
+<P>
+  <PRE>
+The default is not to eliminate any baselines.
+</PRE>
+<P>
+<A NAME=.nmap.make><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>      
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nmodel/nmodel__action.html b/nmodel/nmodel__action.html
new file mode 100644
index 0000000000000000000000000000000000000000..d2ff6f36173fb3a1abf6d7bfe8a403c22d7730de
--- /dev/null
+++ b/nmodel/nmodel__action.html
@@ -0,0 +1,43 @@
+<TITLE>Description of ACTION (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword ACTION</H1> 
+
+<DT><EM>Prompt:</EM> Action HELP, HANDLE; SAVE, GET; FIND, UPDATE; |-CONVERT, EDIT, REDIT, FEDIT , BEAM, DEBEAM; FROM_OLD, TO_OLD, NVS, CVXL; QUIT|
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify action to perform: <P>
+   General: <P>
+        HELP      show some explanation on model lists 
+        HANDLE    select general model-handling branch <P>
+   Model construction: <P>
+        FIND    find sources in map (.WMP file) 
+        UPDATE  update sources by comparison with visibilities (.SCN file) <P>
+   Transfer of model to/from .SCN file: <P>
+        SAVE      save model data in .SCN file 
+        GET       get model from .SCN file <P>
+   Wholescale conversions of model list: <P>
+        CONVERT   Convert model list from epoch to epoch or coordinate to 
+                   coordinate with conversion of l, m coordinates and intensities 
+                   if necessary 
+        EDIT      Change model-list overall parameters without conversion of 
+                   coordinates and intensity (except possible field rotation if 
+                   converting from apparant &lt;-&gt; epoch) 
+        REDIT     Change reference coordinates and frequency. Intensities will 
+                   be corrected for spectral index only. 
+        FEDIT     As REDIT, but intensities will also be corrected for the 
+                   effect of different beams at different frequencies 
+!!                      Primary or synthesised? 
+        BEAM      Correct sources for attenuation by primary beam 
+        DEBEAM    Apply primary-beam attenuation to sources <P>
+   Utilities: <P>
+        FROM_OLD  convert old format source list (use B1950 or Apparent by 
+                   preference) 
+        TO_OLD    convert to old format source list 
+        NVS       make new version of model file if necessary 
+        CVXL      convert formats between machines <P>
+        QUIT    finish <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__area.html b/nmodel/nmodel__area.html
new file mode 100644
index 0000000000000000000000000000000000000000..fcf0892d9068cc4f4eeefb50d5b2c77ddf3b6ec8
--- /dev/null
+++ b/nmodel/nmodel__area.html
@@ -0,0 +1,17 @@
+<TITLE>Description of AREA (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword AREA</H1> 
+
+<DT><EM>Prompt:</EM> Map area: l, m, dl, dm
+<DT><EM>Expected input:</EM> Integer number, 4 values.<P>
+Specify the map area to be selected: <P>
+        l, m    position in grid spacings of centre of area 
+                0, 0 is the map centre, increaing toward the upper right (i.e. 
+                 with DEcreasing RA and INcreasing DEC) <P>
+        dl, dm  horizontal and vertical area sizes  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__beam_descr.html b/nmodel/nmodel__beam_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..f159583942f46ed5c7f1b95dc5cc784e05495b8f
--- /dev/null
+++ b/nmodel/nmodel__beam_descr.html
@@ -0,0 +1,29 @@
+<TITLE>Description of BEAM_DESCR (NMODEL)</TITLE>
+<H1>Description of general keyword BEAM_DESCR</H1>
+
+<DT><EM>Prompt:</EM> Beam descriptors
+<DT><EM>Default:</EM> 0, 0, 1, 6, 1, 1, 4, 4 /NOASK.
+<DT><EM>Expected input:</EM> Integer number, 32 values.<P>
+Describe the primary beam for an instrument other than the WSRT or the ATCA. 
+Here you specify the formula to be used; later you will be asked for values for 
+the coefficients. <P>
+Each instrument (up to 8) is decribed by four numbers, with (in order) the 
+following meaning: <P>
+
+<DT>  - the value of the * in BEAM_FREQ_* and BEAM_FACTOR_* to use <P>
+
+<DT>  - the type of formula: 
+        0= cos(factor*freq(MHz)*angle(degree))**6; 
+        1= 1/(1+fac1*(freq(GHz)*angle(arcmin))**2+fac2*...); 
+        2= 1+fac1*(freq(GHz)*angel(arcmin))**2+fac2*...) <P>
+
+<DT>  - the number of factors per frequency range in BEAM_FACTOR_* <P>
+
+<DT>  - the number of frequency ranges specified in BEAM_FREQ_* <P>
+Instruments are: first WSRT, second ATCA  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__beam_factor_0.html b/nmodel/nmodel__beam_factor_0.html
new file mode 100644
index 0000000000000000000000000000000000000000..4a857e890ccf78cf8ebfa0b2f1e82ff58b6e493d
--- /dev/null
+++ b/nmodel/nmodel__beam_factor_0.html
@@ -0,0 +1,14 @@
+<TITLE>Description of BEAM_FACTOR_0 (NMODEL)</TITLE>
+<H1>Description of general keyword BEAM_FACTOR_0</H1>
+
+<DT><EM>Prompt:</EM> Beam feed factors
+<DT><EM>Default:</EM> .0629, .065, .065, .065, .065, .065 /NOASK.
+<DT><EM>Expected input:</EM> Real number, 64 values.<P>
+Specify per frequency band specified in BEAM_FREQ_0 the factors to be used in 
+the primary beam calculation formula (see BEAM_DESCR). This is for WSRT cos**6 <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__beam_factor_1.html b/nmodel/nmodel__beam_factor_1.html
new file mode 100644
index 0000000000000000000000000000000000000000..4432849f7cfd1a5b030d22cedcebb910fdfaded7
--- /dev/null
+++ b/nmodel/nmodel__beam_factor_1.html
@@ -0,0 +1,15 @@
+<TITLE>Description of BEAM_FACTOR_1 (NMODEL)</TITLE>
+<H1>Description of general keyword BEAM_FACTOR_1</H1>
+
+<DT><EM>Prompt:</EM> Beam feed factors
+<DT><EM>Default:</EM> 8.99E-4, 2.15E-6, -2.23E-09, 1.56E-12,                1.02E-3, 9.48E-7, -3.68E-10, 4.88E-13, -                1.08E-3, 1.31E-6, -1.17E-09, 1.07E-12, -                1.04E-3, 8.36E-7, -4.68E-10, 5.50E-13 /NOASK.
+<DT><EM>Expected input:</EM> Real number, 64 values.<P>
+Specify per frequency band specified in BEAM_FREQ_1 the factors to be used in 
+the primary beam calculation formula (see BEAM_DESCR). This is for ATCA 
+1/(1+ai.x**2i) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__beam_freq_0.html b/nmodel/nmodel__beam_freq_0.html
new file mode 100644
index 0000000000000000000000000000000000000000..a9c04d802e955957e822c6bfd683aceefaf3de0d
--- /dev/null
+++ b/nmodel/nmodel__beam_freq_0.html
@@ -0,0 +1,16 @@
+<TITLE>Description of BEAM_FREQ_0 (NMODEL)</TITLE>
+<H1>Description of general keyword BEAM_FREQ_0</H1>
+
+<DT><EM>Prompt:</EM> Beam feed frequencies
+<DT><EM>Default:</EM> 500, 1000, 2000, 4000, 8000, 100000 /NOASK.
+<DT><EM>Expected input:</EM> Real number, 8 values.<P>
+Specify in increasing order the frequency bands to be used in calculating the 
+primary beam. For each value there should be a corresponding set of values in 
+BEAM_FACTOR_0 (the number of values in BEAM_DESCR).These factors will be used 
+up to the corresponding frequency specified. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__beam_freq_1.html b/nmodel/nmodel__beam_freq_1.html
new file mode 100644
index 0000000000000000000000000000000000000000..9bebcec9b2607627ef33482029861cfc610ca6c8
--- /dev/null
+++ b/nmodel/nmodel__beam_freq_1.html
@@ -0,0 +1,16 @@
+<TITLE>Description of BEAM_FREQ_1 (NMODEL)</TITLE>
+<H1>Description of general keyword BEAM_FREQ_1</H1>
+
+<DT><EM>Prompt:</EM> Beam feed frequencies
+<DT><EM>Default:</EM> 2000, 4000, 8000, 100000 /NOASK.
+<DT><EM>Expected input:</EM> Real number, 8 values.<P>
+Specify in increasing order the frequency bands to be used in calculating the 
+primary beam. For each value there should be a corresponding set of values in 
+BEAM_FACTOR_1 (the number of values in BEAM_DESCR).These factors will be used 
+up to the specified corresponding frequency (MHz). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__beam_scale.html b/nmodel/nmodel__beam_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..3243c95dc6642386c745a474a3daf66e84a23101
--- /dev/null
+++ b/nmodel/nmodel__beam_scale.html
@@ -0,0 +1,15 @@
+<TITLE>Description of BEAM_SCALE (NMODEL)</TITLE>
+<H1>Description of general keyword BEAM_SCALE</H1>
+
+<DT><EM>Prompt:</EM> Scale factor for primary-beam width
+<DT><EM>Default:</EM> 1. /NOASK.
+<DT><EM>Expected input:</EM> Real number.<P>
+Specify a scaling factor for the primary beam calculations. If, e.g. a beam has 
+been defined (by BEAM_FACTOR) for a 25 m dish, it can be used for a 20 m dish 
+by specifying here 20./25. (or 0.8)  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__calibrators.html b/nmodel/nmodel__calibrators.html
new file mode 100644
index 0000000000000000000000000000000000000000..97583f92745a6cbedeeeddab8878e1950421ab4d
--- /dev/null
+++ b/nmodel/nmodel__calibrators.html
@@ -0,0 +1,14 @@
+<TITLE>Description of CALIBRATORS (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword CALIBRATORS</H1> 
+
+<DT><EM>Prompt:</EM> List of sources or *
+<DT><EM>Expected input:</EM> Integer number, 128 values.<P>
+Specify up to 128 numbers of sources in the model list that you want to use as 
+calibrators. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__clear_ref.html b/nmodel/nmodel__clear_ref.html
new file mode 100644
index 0000000000000000000000000000000000000000..2b3ce65fd0bfda34dfe304686650185f4d24cf53
--- /dev/null
+++ b/nmodel/nmodel__clear_ref.html
@@ -0,0 +1,13 @@
+<TITLE>Description of CLEAR_REF (NMODEL)</TITLE>
+<H1>Description of general keyword CLEAR_REF</H1>
+
+<DT><EM>Prompt:</EM> Clear reference coordinates (Yes/No)?
+<DT><EM>Expected input:</EM> Logical, 1 values.<P>
+If you answer YES to this prompt, the reference coordinates of the model will 
+be reset. Otherwise, only the number of components will be set to zero.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__convert_to.html b/nmodel/nmodel__convert_to.html
new file mode 100644
index 0000000000000000000000000000000000000000..2c0805524f14976bc8725a5b5fef9f709fdec648
--- /dev/null
+++ b/nmodel/nmodel__convert_to.html
@@ -0,0 +1,18 @@
+<TITLE>Description of CONVERT_TO (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword CONVERT_TO</H1> 
+
+<DT><EM>Prompt:</EM> B1950, J2000, APPARENT, LOCAL Target coordinate system
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the coordinate system for the output model-list. <P>
+If you are CONVERTing, the output model list's coordinates and intensities will 
+reflect the new type, frequency, instrument and central coordinates. <P>
+If you are EDITing, the new data will be copied only, but the coordinates will 
+be rotated to the new Pole if you are converting between apparent and epoch. 
+!!              ??? 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__delete_area.html b/nmodel/nmodel__delete_area.html
new file mode 100644
index 0000000000000000000000000000000000000000..3ca2bad73f607b069e75f772b42143e2f4c7c720
--- /dev/null
+++ b/nmodel/nmodel__delete_area.html
@@ -0,0 +1,14 @@
+<TITLE>Description of DELETE_AREA (NMODEL)</TITLE>
+<H1>Description of general keyword DELETE_AREA</H1>
+
+<DT><EM>Prompt:</EM> Area l, m, dl, dm (arcsec)
+<DT><EM>Expected input:</EM> Real number, 4 values.<P>
+Specify the area in which all sources should be deleted: <P>
+        l, m     area centre (0, 0 = map centre) 
+        dl, dm   area size  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__delete_level.html b/nmodel/nmodel__delete_level.html
new file mode 100644
index 0000000000000000000000000000000000000000..48f79415dcc6f174715794bb45b457aea0f34f01
--- /dev/null
+++ b/nmodel/nmodel__delete_level.html
@@ -0,0 +1,13 @@
+<TITLE>Description of DELETE_LEVEL (NMODEL)</TITLE>
+<H1>Description of general keyword DELETE_LEVEL</H1>
+
+<DT><EM>Prompt:</EM> Lower flux limit
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Source whose absolute flux is below the value specified here will be deleted 
+from the model list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__edit_field.html b/nmodel/nmodel__edit_field.html
new file mode 100644
index 0000000000000000000000000000000000000000..fb251725c56638752d700aecd00a2f5bf4d90e96
--- /dev/null
+++ b/nmodel/nmodel__edit_field.html
@@ -0,0 +1,30 @@
+<TITLE>Description of EDIT_FIELD (NMODEL)</TITLE>
+<H1>Description of general keyword EDIT_FIELD</H1>
+
+<DT><EM>Prompt:</EM> Source attribute to edit| L, M; I, SI, RM, Q, U, V; LA, SA, PA; ID, BITS, TYP, CCBM, TP2
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify the source attribute that you want to edit: <P>
+   Source coordinates: <P>
+        L, M          coordinates relative to reference (arcsec) <P>
+   Properties of the source: <P>
+        I             ampitude 
+        SI            spectral index 
+        RM            intrinsic rotation measure 
+        Q, U, V       Stokes parameters in % of I 
+        LA, SA, PA    long axis short axis, position angle of elliptic-Gaussian 
+                       extended-source model <P>
+   Administrative attributes in the model list: <P>
+        ID            identification 
+        BITS          bits mask (if source is extended, has polarisation) 
+!                       \whichref{}{} 
+        TYP           source type (0 is the standard) 
+!                       \whichref{}{} 
+        CCBM          clean component (1) and beam-corrected (8) 
+!                       \whichref{}{} 
+        TP2           reserved  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__edit_value.html b/nmodel/nmodel__edit_value.html
new file mode 100644
index 0000000000000000000000000000000000000000..c5c9fe3ee9d1a2d3b00896a3abfddef2e6d486d0
--- /dev/null
+++ b/nmodel/nmodel__edit_value.html
@@ -0,0 +1,12 @@
+<TITLE>Description of EDIT_VALUE (NMODEL)</TITLE>
+<H1>Description of general keyword EDIT_VALUE</H1>
+
+<DT><EM>Prompt:</EM> New value
+<DT><EM>Expected input:</EM> Real number.<P>
+Specify the value to set in specified edit field. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__find_type.html b/nmodel/nmodel__find_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..ece4e195ca70164a966811f481c1308f784ebca9
--- /dev/null
+++ b/nmodel/nmodel__find_type.html
@@ -0,0 +1,19 @@
+<TITLE>Description of FIND_TYPE (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword FIND_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> Finding mode POS, ABS, MANUAL; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify how to select candidate sources: <P>
+        POS     Select sources with highest positive brightness 
+        ABS     Select sources with highest absolute brightness 
+        MANUAL  Select sources manually with the cursor on a GIDS screen. 
+                 Sources are selected by pushing MB1; MB3 will finish; 
+                 MB2 will not calculate position, but put grid point as clean 
+                 source <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__gids_sources.html b/nmodel/nmodel__gids_sources.html
new file mode 100644
index 0000000000000000000000000000000000000000..1492fa810bb4d4f09c7788333991a5bb24896765
--- /dev/null
+++ b/nmodel/nmodel__gids_sources.html
@@ -0,0 +1,13 @@
+<TITLE>Description of GIDS_SOURCES (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword GIDS_SOURCES</H1> 
+
+<DT><EM>Prompt:</EM> Select sources on GIDS display (Yes/No)?"
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if you want to point at sources on the GIDS display for the current map <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__id_start.html b/nmodel/nmodel__id_start.html
new file mode 100644
index 0000000000000000000000000000000000000000..d3a17f34d72288211e44c0129a2ecf250650e62b
--- /dev/null
+++ b/nmodel/nmodel__id_start.html
@@ -0,0 +1,13 @@
+<TITLE>Description of ID_START (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword ID_START</H1> 
+
+<DT><EM>Prompt:</EM> Start identification number
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000.<P>
+Specify the start of the ID number to be used in the source list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__ion of model file if necessary.html b/nmodel/nmodel__ion of model file if necessary.html
new file mode 100644
index 0000000000000000000000000000000000000000..16f8f0a768105b0872cee57a659d33e0d25ddb5e
--- /dev/null
+++ b/nmodel/nmodel__ion of model file if necessary.html	
@@ -0,0 +1,19 @@
+<TITLE>Description of ion of model file if necessary (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword ion of model file if necessary</H1> 
+
+<DT><EM>Prompt:</EM> Finding mode POS, ABS, MANUAL; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify how to select candidate sources: <P>
+        POS     Select sources with highest positive brightness 
+        ABS     Select sources with highest absolute brightness 
+        MANUAL  Select sources manually with the cursor on a GIDS screen. 
+                 Sources are selected by pushing MB1; MB3 will finish; 
+                 MB2 will not calculate position, but put grid point as clean 
+                 source <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__map_limit.html b/nmodel/nmodel__map_limit.html
new file mode 100644
index 0000000000000000000000000000000000000000..459fc660fc89969bb3e6ed2bfb155486fbdff8a8
--- /dev/null
+++ b/nmodel/nmodel__map_limit.html
@@ -0,0 +1,14 @@
+<TITLE>Description of MAP_LIMIT (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword MAP_LIMIT</H1> 
+
+<DT><EM>Prompt:</EM> Lower relative intensity limit
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000; max.value: 1.000000.<P>
+Specify the lowest limit with respect to the maximum in the map that will be 
+considered a valid source <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__max_number.html b/nmodel/nmodel__max_number.html
new file mode 100644
index 0000000000000000000000000000000000000000..7e71c19c348bccb5f3381f89df444d3d43edb986
--- /dev/null
+++ b/nmodel/nmodel__max_number.html
@@ -0,0 +1,13 @@
+<TITLE>Description of MAX_NUMBER (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword MAX_NUMBER</H1> 
+
+<DT><EM>Prompt:</EM> Maximum number of sources to add
+<DT><EM>Expected input:</EM> Integer number; min.value: 1.000000; max.value: 200.000000.<P>
+Specify the maximum number of sources that will be found.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__merge_radius.html b/nmodel/nmodel__merge_radius.html
new file mode 100644
index 0000000000000000000000000000000000000000..eae6687098303a6b7c7cf4f1f9cf42df47c26267
--- /dev/null
+++ b/nmodel/nmodel__merge_radius.html
@@ -0,0 +1,14 @@
+<TITLE>Description of MERGE_RADIUS (NMODEL)</TITLE>
+<H1>Description of general keyword MERGE_RADIUS</H1>
+
+<DT><EM>Prompt:</EM> Coincidence radii dl, dm (arcsec)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Point sources that are within (dl, dm) arcsec of each other are combined. The 
+suggested default values are approximately half the synthesised  beam radius in 
+l and m directions. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__model_action.html b/nmodel/nmodel__model_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..e69de29bb2d1d6434b8b29ae775ad8c2e48c5391
diff --git a/nmodel/nmodel__model_modify.html b/nmodel/nmodel__model_modify.html
new file mode 100644
index 0000000000000000000000000000000000000000..f00ea91af66b9bb58efd6ada0db7447b3c77345e
--- /dev/null
+++ b/nmodel/nmodel__model_modify.html
@@ -0,0 +1,42 @@
+<TITLE>Description of MODEL_MODIFY (NMODEL)</TITLE>
+<H1>Description of general keyword MODEL_MODIFY</H1>
+
+<DT><EM>Prompt:</EM> Model-handling action MERGE, RMERGE, SORT, FSORT; CALIB, EDIT, FEDIT, FLUX_KNOWN;| -DEL, DNCLOW, DCLOW, DAREA; SHOW, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify what you want to do with the model list in core: <P>
+   Consolidating/rearranging the list: <P>
+        MERGE   Combine (point-) sources at the same position. 
+                 Must have the same spectral index and rotation measure. 
+                 Stokes Q, U, V are properly taken into account. 
+                 CLEAN components are NOT combined with non-CLEAN comp. 
+                 Extended sources are ignored. 
+        RMERGE  As MERGE, but within specified radius (which may be 0). 
+                 The (l, m) position of the strongest source is taken. 
+                 CLEAN components are combined if at the same position. 
+!!               Discard duplicates or add fluxes? See MODEL_ACTION MERGE 
+!!               below 
+        SORT    Sort source list in decreasing amplitude. (This will be done 
+                 automatically when you write the list back to a .MDL file.) 
+        FSORT   Sort on a specified field in source list (for subsequent 
+                 display) <P>
+   Modifying sources in the list: <P>
+        CALIB   Calibrate the source list to a new amplitude and/or position 
+        EDIT    Edit source list (an amplitude of zero will delete the source) 
+        FEDIT   Edit a field in a range of sources 
+        FLUX_KNOWN Toggle the 'unknown-flux' bit. When this bit is off, NCALIB 
+                 will by default refrain from attempting a Selfcan gain 
+                 solution. <P>
+   Deleting sources in the list: <P>
+        DEL     Delete sources 
+        DNCLOW  Delete non-clean sources with low amplitudes 
+        DCLOW   Delete clean components with low amplitudes 
+        DAREA   Delete sources in specified area <P>
+   Miscellaneous: <P>
+        SHOW       Show the list. (You will be prompted for details) <P>
+        QUIT       Quit model-handling.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__model_option.html b/nmodel/nmodel__model_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..db0b66efad2e6764faab637e30cacc9c6b3e3824
--- /dev/null
+++ b/nmodel/nmodel__model_option.html
@@ -0,0 +1,48 @@
+<TITLE>Description of MODEL_OPTION (NMODEL)</TITLE>
+<H1>Description of general keyword MODEL_OPTION</H1>
+
+<DT><EM>Prompt:</EM> Model-list action| READ, WRITE, INTERN; CLEAR, ADD, MODIFY, SHOW; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the action to be taken on the internal model list: <P>
+   Transfers between the internal list and an external file: <P>
+        READ   Read the components from a .MDL file on disk into the 
+                program's model list. The default filename is the name of 
+                the calibrator belonging to the most recently read sector,  
+                derived from the fieldname and the frequency. .MDL files are 
+                first searched for in the current directory or the directory 
+                defined by parameter DATAB. If this fails, the file is looked 
+                for in the directory defined by parameter MODELB and finally by 
+                that defined by the Unix environment variable MODELB. <P>
+               NOTE that reading is INCREMENTAL, so if you read the same 
+                .MDL file twice, you will get every component doubled... <P>
+        WRITE  Write the program's model list to a .MDL file. <P>
+        INTERN This does not affect the list, but selects 
+                the model stored in the scan-file(s). Selecting INTERN is 
+                equivalent to setting DE_APPLY=MODEL. 
+                You may use this internal model in combination with 
+                components in the program's model list. 
+!!                      To be sorted out... <P>
+   Modification and display of the internal list: <P>
+        CLEAR  Empty the program's model list and optionally its reference 
+                coordinates. <P>
+        ADD    Manual input of sources to add the list <P>
+        MODIFY Enter a submenu with options to modify the model list: 
+
+<DT>                  - by deleting sources from the list; 
+
+<DT>                  - by editing entries manually; 
+
+<DT>                  - by sorting (for subsequent display) the list: you will be 
+                     prompted for a definition of the sort order; 
+
+<DT>                  - by calibrating. 
+!!                      What?? How?? <P>
+        SHOW   Show the program's model list, you will be prompted for details. <P>
+. 
+        QUIT   Exit from model-handling.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__model_show.html b/nmodel/nmodel__model_show.html
new file mode 100644
index 0000000000000000000000000000000000000000..57e3a3efdd6518fde395257b3e67e6a3796f44e7
--- /dev/null
+++ b/nmodel/nmodel__model_show.html
@@ -0,0 +1,18 @@
+<TITLE>Description of MODEL_SHOW (NMODEL)</TITLE>
+<H1>Description of general keyword MODEL_SHOW</H1>
+
+<DT><EM>Prompt:</EM> Model listing mode SHOW, LIST, RSHOW, RLIST, TOTAL; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify what type of listing you want, and where it should be shown: <P>
+   LIST   Show the program's model list in the log file. 
+   SHOW   Idem, but both on the terminal and in the log file. <P>
+   RLIST  Show the program's model list in RA/DEC coordinates in the log file. 
+   RSHOW  Idem, but both on the terminal and in the log file. <P>
+   TOTAL  Show the statistics of the program's model list. <P>
+   QUIT   Back to MODEL_OPTION. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__names_file.html b/nmodel/nmodel__names_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..c7f491d691693750caec1b69b47e5206e8f57061
--- /dev/null
+++ b/nmodel/nmodel__names_file.html
@@ -0,0 +1,15 @@
+<TITLE>Description of NAMES_FILE (NMODEL)</TITLE>
+<H1>Description of general keyword NAMES_FILE</H1>
+
+<DT><EM>Prompt:</EM> File with source names
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the full name of the input disk-file. The file should contain lines 
+with Ra, Dec and Name, separated by white space. Comments may be added starting 
+with an exclamation mark. A NULL answer (two double quotes) will ignore the 
+name-list: no file will be opened. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__old_file.html b/nmodel/nmodel__old_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..82088156290065f7f3746106d350a03c136828b4
--- /dev/null
+++ b/nmodel/nmodel__old_file.html
@@ -0,0 +1,14 @@
+<TITLE>Description of OLD_FILE (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword OLD_FILE</H1> 
+
+<DT><EM>Prompt:</EM> old model filename
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the filename (includinhg extension) the an old-format RMODEL file to be 
+read or written.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__ref_scn_node.html b/nmodel/nmodel__ref_scn_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..04de35a5f8e7359fd7f7b49901f2ce9bdfa51839
--- /dev/null
+++ b/nmodel/nmodel__ref_scn_node.html
@@ -0,0 +1,33 @@
+<TITLE>Description of REF_SCN_NODE (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword REF_SCN_NODE</H1> 
+
+<DT><EM>Prompt:</EM> File name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the node name with the model overall coordinates to use. <P>
+Instead of a file name you may reply with a '*'. You will then be prompted for 
+'manual' inpout of data, unless you are CONVRTing between apparent and epoch 
+coordinates. 
+!!                      ??? 
+!!. 
+!!Note that the node name can be preceded with dev:[dir..] (or /dev/dir... if 
+!!Unix). The specified dev and/or directories will become the default 
+!!database for all node related names. Atstart of program the default is the 
+!!current directory. The database specified should be an existing directory. 
+!!. 
+!!By placing part of the node name in parentheses (), the string defined 
+!!in such a way can in subsequent node questions be referenced with a #. 
+!!Hence the following inputs will translate as: 
+!!. 
+!!  ngc1204.21cm.long                   ngc1204.21cm.long 
+!!  [dwl.ger.ngc1204]ngc1204.90cm.short [dwl.ger.ngc1204]ngc1204.90cm.short 
+!!  (ngc1204.21cm.)long                 [dwl.ger.ngc1204]ngc1204.21cm.long 
+!!  a.#long                             [dwl.ger.ngc1204]a.ngc1204.21cm.long 
+!!              Is this of any use? If so, why specifically here? 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__ref_scn_set.html b/nmodel/nmodel__ref_scn_set.html
new file mode 100644
index 0000000000000000000000000000000000000000..c040954d7d61ec798ec7469e831c4f9b420ab32b
--- /dev/null
+++ b/nmodel/nmodel__ref_scn_set.html
@@ -0,0 +1,16 @@
+<TITLE>Description of REF_SCN_SET (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword REF_SCN_SET</H1> 
+
+<DT><EM>Prompt:</EM> ONE sector for reference coordinates: grp.obs.fld.chn.seq
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+Specify ONE .SCN-file sector from which the reference coordinates (RA, DEC,  
+frequency) are to be taken. <P>
+grp.obs.fld.chn.seq = group.obs.field.channel.sequence_number  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__reference_data.html b/nmodel/nmodel__reference_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..a71a2a29226f588938a603c43a8ffa5897e22089
--- /dev/null
+++ b/nmodel/nmodel__reference_data.html
@@ -0,0 +1,18 @@
+<TITLE>Description of REFERENCE_DATA (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword REFERENCE_DATA</H1> 
+
+<DT><EM>Prompt:</EM> RA, DEC, Freq, rot., instr.
+<DT><EM>Expected input:</EM> Double precision number, 5 values.<P>
+Specify <P>
+        RA, DEC (decimal degrees) 
+        precession rotation angle (degrees) 
+        spectral-index reference frequency (MHz) 
+        instrument code (0=WSRT; 1=ATCA) <P>
+for the new reference source list position.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__reference_freq.html b/nmodel/nmodel__reference_freq.html
new file mode 100644
index 0000000000000000000000000000000000000000..6b1426d787eafa6017cdc3e883d128886d1fd9ca
--- /dev/null
+++ b/nmodel/nmodel__reference_freq.html
@@ -0,0 +1,13 @@
+<TITLE>Description of REFERENCE_FREQ (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword REFERENCE_FREQ</H1> 
+
+<DT><EM>Prompt:</EM> Reference frequency (MHz)
+<DT><EM>Expected input:</EM> Double precision number.<P>
+Specify the spectral index reference frequency (MHz). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__sort_centre.html b/nmodel/nmodel__sort_centre.html
new file mode 100644
index 0000000000000000000000000000000000000000..77d2c663e7b15d62930f6bec91871139b9202b3a
--- /dev/null
+++ b/nmodel/nmodel__sort_centre.html
@@ -0,0 +1,13 @@
+<TITLE>Description of SORT_CENTRE (NMODEL)</TITLE>
+<H1>Description of general keyword SORT_CENTRE</H1>
+
+<DT><EM>Prompt:</EM> Reference coordinates l, m|-
+for distance sort (arcsec)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the reference coordinates for the distance sort that you selected. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__sort_field.html b/nmodel/nmodel__sort_field.html
new file mode 100644
index 0000000000000000000000000000000000000000..2f579e557a77a665ddd4d5a4da04617ef93607d0
--- /dev/null
+++ b/nmodel/nmodel__sort_field.html
@@ -0,0 +1,33 @@
+<TITLE>Description of SORT_FIELD (NMODEL)</TITLE>
+<H1>Description of general keyword SORT_FIELD</H1>
+
+<DT><EM>Prompt:</EM> Sort criterion L, M, LM, ML, DIST; I, SI, POL, RM, Q, U, V; LA, SA, PA;| -ID, BITS, TYP, CCBM, TP2
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify sourfce attribute on which to sort: <P>
+   Source coordinates: <P>
+        L, M          l or m, arbitrary order for the other 
+        LM, ML        l and then m, or m and then l 
+        DIST          distance to a specified reference point <P>
+   Properties of the source: <P>
+        I             ampitude 
+        SI            spectral index 
+        POL           polarised intensity 
+        RM            intrinsic rotation measure 
+        Q, U, V       Stokes parameters in % of I 
+        LA, SA, PA    long axis short axis, position angle of elliptic-Gaussian 
+                       extended-source model <P>
+   Administrative attributes in the model list: <P>
+        ID            identification 
+        BITS          bits mask (if source is extended, has polarisation) 
+!                       \whichref{}{} 
+        TYP           source type (0 is the standard) 
+!                       \whichref{}{} 
+        CCBM          clean component (1) and beam-corrected (8) 
+!                       \whichref{}{} 
+        TP2           reserved  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__sort_type.html b/nmodel/nmodel__sort_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..0907cc6125976fa227b81792a2573965efa51d50
--- /dev/null
+++ b/nmodel/nmodel__sort_type.html
@@ -0,0 +1,12 @@
+<TITLE>Description of SORT_TYPE (NMODEL)</TITLE>
+<H1>Description of general keyword SORT_TYPE</H1>
+
+<DT><EM>Prompt:</EM> INCREASING, DECREASING
+<DT><EM>Expected input:</EM> Character(24).<P>
+ Specify the polarity of the sort <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__source.html b/nmodel/nmodel__source.html
new file mode 100644
index 0000000000000000000000000000000000000000..61e6c825b4f26afcd75a72280bcef5c850cbabb3
--- /dev/null
+++ b/nmodel/nmodel__source.html
@@ -0,0 +1,31 @@
+<TITLE>Description of SOURCE (NMODEL)</TITLE>
+<H1>Description of general keyword SOURCE</H1>
+
+<DT><EM>Prompt:</EM> I, l, m, id, Q, U, V, lax, sax, pa, si, rm, rs
+<DT><EM>Expected input:</EM> Real number, 13 values.<P>
+Specify the source parameters in order shown. <P>
+   I            intensity (W.U.) 
+   l, m         coordinates w.r.t. reference (arcsec) 
+   id           identification number (see below) 
+   Q            Stokes Q relative to I (%) 
+   U            Stokes U relative to I (%) 
+   V            Stokes V relative to I (%) 
+   lax          long-axis full halfwidth (arcsec, =0 for a point source) 
+   sax          short-axis full halfwidth (arcsec, =0 for a point source) 
+   pa           position angle of long axis (degrees, North through East) 
+   si           spectral index 
+   rm           intrinsic rotation measure ( rad/m**2 at 1 Ghz) 
+   rs           reserved <P>
+You may omit values that you want to leave alone, but not the commas that 
+delimit them. Trailing values and commas may be omitted. <P>
+    Example: 
+        , , 3 will set m to 3 and leave all other parameters unchanged. <P>
+The identification number is of the form <P>
+        &lt;sequence number&gt;-&lt;mask byte&gt; 
+  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__source_factors.html b/nmodel/nmodel__source_factors.html
new file mode 100644
index 0000000000000000000000000000000000000000..ce5cd9c941fd1246f85b64e0ecda3dd2f9663dc4
--- /dev/null
+++ b/nmodel/nmodel__source_factors.html
@@ -0,0 +1,15 @@
+<TITLE>Description of SOURCE_FACTORS (NMODEL)</TITLE>
+<H1>Description of general keyword SOURCE_FACTORS</H1>
+
+<DT><EM>Prompt:</EM> Amlitude ratio Anew/Aold, | shift dl, dm (arcsec)
+<DT><EM>Expected input:</EM> Real number, 3 values.<P>
+Specify the calibration parameters in te order shown: 
+  An/Ao new/old amplitude 
+  dl    new-old l in arcsec 
+  dm    new-old m in arcsec  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__source_list.html b/nmodel/nmodel__source_list.html
new file mode 100644
index 0000000000000000000000000000000000000000..f58bf3afd8923a10451de4397b03207b3c1a73de
--- /dev/null
+++ b/nmodel/nmodel__source_list.html
@@ -0,0 +1,13 @@
+<TITLE>Description of SOURCE_LIST (NMODEL)</TITLE>
+<H1>Description of general keyword SOURCE_LIST</H1>
+
+<DT><EM>Prompt:</EM> Source number list
+<DT><EM>Expected input:</EM> Integer number, 128 values.<P>
+Specify a list of individual source numbers to be acted upon. If you want to 
+spaecfy a range, reply '*' here and wait for the next prompt <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__source_number.html b/nmodel/nmodel__source_number.html
new file mode 100644
index 0000000000000000000000000000000000000000..fc13f48c73ed6ff60998f9f0bb5c49fc246bf50b
--- /dev/null
+++ b/nmodel/nmodel__source_number.html
@@ -0,0 +1,12 @@
+<TITLE>Description of SOURCE_NUMBER (NMODEL)</TITLE>
+<H1>Description of general keyword SOURCE_NUMBER</H1>
+
+<DT><EM>Prompt:</EM> Source number
+<DT><EM>Expected input:</EM> Integer number.<P>
+Specify the number of the source to be acted upon. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__source_range.html b/nmodel/nmodel__source_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..9b6a1e30b12d8fd9302930895108fda0d1e8d7e6
--- /dev/null
+++ b/nmodel/nmodel__source_range.html
@@ -0,0 +1,15 @@
+<TITLE>Description of SOURCE_RANGE (NMODEL)</TITLE>
+<H1>Description of general keyword SOURCE_RANGE</H1>
+
+<DT><EM>Prompt:</EM> Source number range
+<DT><EM>Expected input:</EM> Integer number, 2 values.<P>
+Specify the first and last source number to process. * indicates 'all'. If you 
+want all sources from some number &lt;N&gt; upward, reply <P>
+        '&lt;N&gt;-&lt;some very large number&gt;'. 
+!!              Does * work? 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_comm.html">List of general keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__update_cluster.html b/nmodel/nmodel__update_cluster.html
new file mode 100644
index 0000000000000000000000000000000000000000..f6a50636e94b9d7ad78dad6476ae94a0d4f0c3fe
--- /dev/null
+++ b/nmodel/nmodel__update_cluster.html
@@ -0,0 +1,13 @@
+<TITLE>Description of UPDATE_CLUSTER (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword UPDATE_CLUSTER</H1> 
+
+<DT><EM>Prompt:</EM> Update cluster size in arcsec (l, m)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the cluster size for update in arcsec in the l and m direction.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__update_mode.html b/nmodel/nmodel__update_mode.html
new file mode 100644
index 0000000000000000000000000000000000000000..5e21476e9c33e2b99086fe45192c92d6fdee3f10
--- /dev/null
+++ b/nmodel/nmodel__update_mode.html
@@ -0,0 +1,24 @@
+<TITLE>Description of UPDATE_MODE (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword UPDATE_MODE</H1> 
+
+<DT><EM>Prompt:</EM> Update type SEPARATE; CLUSTER, LCLUSTER; COMBINED, LCOMBINED;|CONSTRAINED, LCONSTRAINED; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify how the update process should proceed: <P>
+        SEPARATE        each source to be updated is looked at separately,  
+                         and they are fiddled to cater for close sources <P>
+        CLUSTER         sources are clustered to bypass closeness problems <P>
+        COMBINED        all sources solved in one go, with sub-clustering <P>
+        CONSTRAINED     use constraints and clustering. The standard 
+                         constraint used is to fix all variables for all 
+                         but the lowest intensity source <P>
+        L&lt;type&gt;         Loop up to 20 cycles till convergence: 
+                         Note that the loop option does not always 
+                         work, and is very slow. Preferably use for a 
+                         small number of well separated sources/clusters.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel/nmodel__update_type.html b/nmodel/nmodel__update_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..3dc66f528a58b1ab7e93b98104e945802f432749
--- /dev/null
+++ b/nmodel/nmodel__update_type.html
@@ -0,0 +1,46 @@
+<TITLE>Description of UPDATE_TYPE (NMODEL)</TITLE>
+<H1>Program NMODEL: private keyword UPDATE_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> Update mode I, LM, ILM, SILM; EXTEND; QUV, PESTIMATE;|X00, X01, X02, X03 ; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the parameters to be redetermined per source in the update process. <P>
+   Position and flux: 
+        I       Intensity only 
+        LM      Position only 
+        ILM     Intensity and position 
+        SILM    Intensity, spectral index and position (requires a multichannel 
+                 observation with &lt;bandwidth per channel&gt;/&lt;frequency&gt; greater 
+                 than ..) 
+!                       ?? <P>
+   Source size: 
+        EXTEND  Intensity and size parameters for elliptic-Gaussian model 
+                 (major/minor axes, position angle) <P>
+   Source polarisation: 
+        QUV     Stokes Q/I, U/I, V/I 
+        PESTIM  Estimate the total linear polarisation, and store it as Stokes 
+                 Q. NOTE that this improper use of the model list is not 
+                 recorded, so you it is your responsibility to interpret this 
+                 kluge correctly. <P>
+   Specially programmed updates -- ask AGdB about details 
+<DT><STRONG>	X00</STRONG> Type extra 0 
+<DT><STRONG>	X01</STRONG> Type extra 1 
+<DT><STRONG>	X02</STRONG> Type extra 2 
+<DT><STRONG>	X03</STRONG> Type extra 3 <P>
+NOTES: 
+        1. All sources in the model are taken into account in determining the 
+residual visibilities on which the update fit is performed. However, no updates 
+are attempted for sources of type other than 0 nor for CLEAN components. <P>
+        If you want to protect one or more sources from being updated, you can 
+do so by temporarily changing their type (OPTION=MODIFY, MODIFY_OPTION=FEDIT,  
+see the Help text there). 
+!               \whichref{}{} <P>
+        2. It is recommended that you use a set of interferometers that gives a 
+uniform baseline coverage, e.g. by selecting fixed-movable (FM) interferometers 
+only.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nmodel/nmodel_keys.html">List of keywords</A> for NMODEL
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nmodel_comm/nmodel_comm.html b/nmodel_comm/nmodel_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..e69de29bb2d1d6434b8b29ae775ad8c2e48c5391
diff --git a/nmodel_descr.ps b/nmodel_descr.ps
new file mode 100644
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+%%EndDocument
+ @endspecial 0 1963 a Fa(Figure)14 b(3:)k Fb(Overview)c(of)g(the)h(p)n
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+%%Trailer
+end
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+%%EOF
diff --git a/nmodel_descr/images.pl b/nmodel_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nmodel_descr/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nmodel_descr/labels.pl b/nmodel_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..ee045a3b65b36d096635e3d40ea15fe3bda21d0d
--- /dev/null
+++ b/nmodel_descr/labels.pl
@@ -0,0 +1,8 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".nmodel.handle"} ="$URL/nmodel_descr.html"; 
+$external_labels{".nmodel.convert"} ="$URL/nmodel_descr.html"; 
+$external_labels{".nmodel.interface"} ="$URL/nmodel_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/nmodel_descr/nmodel_descr.html b/nmodel_descr/nmodel_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..9836063e2a889c56087246ea0d32723c57855d34
--- /dev/null
+++ b/nmodel_descr/nmodel_descr.html
@@ -0,0 +1,69 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <i>This is a dummy replacing the original Cookbook version that got lost. Since that version contained very little true information, no attempt has been made to restore it.
+<P>
+        A new version is planned.
+<P>
+        Shown below are the interface diagrams that do exist
+<P>
+<A NAME=.nmodel.interface><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the actions in NMODEL. <BR><A HREF="../fig/nmodel_interface.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>See the companion diagrams for details of the  model-handling (<A HREF=" #.nmodel.handle">figure</A>) and model-conversion (<A HREF=" #.nmodel.convert">figure</A>) interfaces  </i>
+<P>
+<A NAME=.nmodel.handle><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the parameter interface for the model-manipulation branch of NMODEL. <BR><A HREF="../fig/nmodel_handle.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i>This diagram expands the HANDLE branch in the overview diagram (<A HREF=" #.nmodel.interface">figure</A>) of NMODEL's parameter interface. 
+<BR>The same model-handling facilities are also available from several other programs. 
+ </i>
+<P>
+<A NAME=.nmodel.convert><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Overview of the parameter interface for the model-conversion branch of NMODEL. 
+<A HREF="../fig/nmodel_convert.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR>This diagram expands the corresponding branch in the overview diagram (<A HREF=" #.nmodel.interface">figure</A>) of NMODEL's parameter interface. </i>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+</i><HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nmodel_keys/nmodel_keys.html b/nmodel_keys/nmodel_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..06d5f62bfb1cf8da4b452d44c00c6aba2b192035
--- /dev/null
+++ b/nmodel_keys/nmodel_keys.html
@@ -0,0 +1,88 @@
+<TITLE>Index of private keywords for NMODEL </TITLE>
+<H1>Description of keywords for program NMODEL</H1>
+
+<UL>
+<LI> <A HREF="../nmodel/nmodel__action.html">
+  ACTION</A>
+  Action HELP, HANDLE; SAVE, GET; FIND, UPDATE; |-CONVERT, EDIT, REDIT, FEDIT , BEAM, DEBEAM; FROM_OLD, TO_OLD, NVS, CVXL; QUIT|
+<LI> <A HREF="../nmodel/nmodel__find_type.html">
+  FIND_TYPE</A>
+  Finding mode POS, ABS, MANUAL; QUIT
+<LI> <A HREF="../nmodel/nmodel__update_type.html">
+  UPDATE_TYPE</A>
+  Update mode I, LM, ILM, SILM; EXTEND; QUV, PESTIMATE;|X00, X01, X02, X03 ; QUIT
+<LI> <A HREF="../nmodel/nmodel__update_mode.html">
+  UPDATE_MODE</A>
+  Update type SEPARATE; CLUSTER, LCLUSTER; COMBINED, LCOMBINED;|CONSTRAINED, LCONSTRAINED; QUIT
+<LI> <A HREF="../nmodel/nmodel__update_cluster.html">
+  UPDATE_CLUSTER</A>
+  Update cluster size in arcsec (l, m)
+<LI> <A HREF="../nmodel/nmodel__gids_sources.html">
+  GIDS_SOURCES</A>
+  Select sources on GIDS display (Yes/No)?"
+<LI> <A HREF="../nmodel/nmodel__old_file.html">
+  OLD_FILE</A>
+  old model filename
+<LI> <A HREF="../nmodel/nmodel__calibrators.html">
+  CALIBRATORS</A>
+  List of sources or *
+<LI> <A HREF="../nmodel/nmodel__convert_to.html">
+  CONVERT_TO</A>
+  B1950, J2000, APPARENT, LOCAL Target coordinate system
+<LI> <A HREF="../nmodel/nmodel__ref_scn_node.html">
+  REF_SCN_NODE</A>
+  File name
+<LI> <A HREF="../nmodel/nmodel__ref_scn_set.html">
+  REF_SCN_SET</A>
+  ONE sector for reference coordinates: grp.obs.fld.chn.seq
+<LI> <A HREF="../nmodel/nmodel__reference_data.html">
+  REFERENCE_DATA</A>
+  RA, DEC, Freq, rot., instr.
+<LI> <A HREF="../nmodel/nmodel__reference_freq.html">
+  REFERENCE_FREQ</A>
+  Reference frequency (MHz)
+<LI> <A HREF="../nmodel/nmodel__area.html">
+  AREA</A>
+  Map area: l, m, dl, dm
+<LI> <A HREF="../nmodel/nmodel__map_limit.html">
+  MAP_LIMIT</A>
+  Lower relative intensity limit
+<LI> <A HREF="../nmodel/nmodel__max_number.html">
+  MAX_NUMBER</A>
+  Maximum number of sources to add
+<LI> <A HREF="../nmodel/nmodel__id_start.html">
+  ID_START</A>
+  Start identification number
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpnode_comm/wmpnode_comm.html">WMPNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpsets_comm/wmpsets_comm.html">WMPSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nmodel_descr/nmodel_descr.html">program NMODEL</A>
+</UL>
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diff --git a/nmodel_private_intfc/images.pl b/nmodel_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nmodel_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nmodel_private_intfc/labels.pl b/nmodel_private_intfc/labels.pl
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index 0000000000000000000000000000000000000000..f9c180a7dc66e310f311a1d67dba734a24e99169
--- /dev/null
+++ b/nmodel_private_intfc/labels.pl
@@ -0,0 +1,25 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
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+$external_labels{".public"} ="$URL/nmodel_private_intfc.html"; 
+$external_labels{".convert.to"} ="$URL/nmodel_private_intfc.html"; 
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+$external_labels{".action"} ="$URL/nmodel_private_intfc.html"; 
+$external_labels{".max.number"} ="$URL/nmodel_private_intfc.html"; 
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+$external_labels{".update.cluster"} ="$URL/nmodel_private_intfc.html"; 
+$external_labels{".ref.scn.node"} ="$URL/nmodel_private_intfc.html"; 
+
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diff --git a/nmodel_private_intfc/nmodel_private_intfc.html b/nmodel_private_intfc/nmodel_private_intfc.html
new file mode 100644
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--- /dev/null
+++ b/nmodel_private_intfc/nmodel_private_intfc.html
@@ -0,0 +1,441 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NMODEL</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nmodel_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nmodel_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nmodel_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nmodel_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nmodel_private_intfc.html#SECTION0003200000000000000>  <b>Parameter ACTION</b></A>
+<LI> <A NAME=tex2html6 HREF=nmodel_private_intfc.html#SECTION0003300000000000000>  <b>Parameter AREA</b></A>
+<LI> <A NAME=tex2html7 HREF=nmodel_private_intfc.html#SECTION0003400000000000000>  <b>Parameter CALIBRATORS</b></A>
+<LI> <A NAME=tex2html8 HREF=nmodel_private_intfc.html#SECTION0003500000000000000>  <b>Parameter CONVERT_TO</b></A>
+<LI> <A NAME=tex2html9 HREF=nmodel_private_intfc.html#SECTION0003600000000000000>  <b>Parameter FIND_TYPE</b></A>
+<LI> <A NAME=tex2html10 HREF=nmodel_private_intfc.html#SECTION0003700000000000000>  <b>Parameter GIDS_SOURCES</b></A>
+<LI> <A NAME=tex2html11 HREF=nmodel_private_intfc.html#SECTION0003800000000000000>  <b>Parameter ID_START</b></A>
+<LI> <A NAME=tex2html12 HREF=nmodel_private_intfc.html#SECTION0003900000000000000>  <b>Parameter MAP_LIMIT</b></A>
+<LI> <A NAME=tex2html13 HREF=nmodel_private_intfc.html#SECTION00031000000000000000>  <b>Parameter MAX_NUMBER</b></A>
+<LI> <A NAME=tex2html14 HREF=nmodel_private_intfc.html#SECTION00031100000000000000>  <b>Parameter OLD_FILE</b></A>
+<LI> <A NAME=tex2html15 HREF=nmodel_private_intfc.html#SECTION00031200000000000000>  <b>Parameter REFERENCE_DATA</b></A>
+<LI> <A NAME=tex2html16 HREF=nmodel_private_intfc.html#SECTION00031300000000000000>  <b>Parameter REFERENCE_FREQ</b></A>
+<LI> <A NAME=tex2html17 HREF=nmodel_private_intfc.html#SECTION00031400000000000000>  <b>Parameter REF_SCN_NODE</b></A>
+<LI> <A NAME=tex2html18 HREF=nmodel_private_intfc.html#SECTION00031500000000000000>  <b>Parameter REF_SCN_SET</b></A>
+<LI> <A NAME=tex2html19 HREF=nmodel_private_intfc.html#SECTION00031600000000000000>  <b>Parameter UPDATE_CLUSTER</b></A>
+<LI> <A NAME=tex2html20 HREF=nmodel_private_intfc.html#SECTION00031700000000000000>  <b>Parameter UPDATE_MODE</b></A>
+<LI> <A NAME=tex2html21 HREF=nmodel_private_intfc.html#SECTION00031800000000000000>  <b>Parameter UPDATE_TYPE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NMODEL. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show parameters that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../wmpnode_public_intfc/wmpnode_public_intfc.html">WMPNODE</A> public keywords 
+<LI> <A HREF="../wmpsets_public_intfc/wmpsets_public_intfc.html">WMPSETS</A> public keywords 
+</UL>
+<P>
+<A NAME=.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter ACTION</b></A></H2>
+<P>
+  <em>Prompt:</em> Action<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+    <PRE>
+        Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+   General:
+</PRE>
+<P>
+  <PRE>
+        HELP      show some explanation on model lists
+        HANDLE    select general model-handling branch
+</PRE>
+<P>
+  <PRE>
+   Model construction:
+</PRE>
+<P>
+  <PRE>
+        FIND    find sources in map (.WMP file)
+        UPDATE  update sources by comparison with visibilities (.SCN file)
+</PRE>
+<P>
+  <PRE>
+   Transfer of model to/from .SCN file:
+</PRE>
+<P>
+  <PRE>
+        SAVE      save model data in .SCN file
+        GET       get model from .SCN file
+</PRE>
+<P>
+  <PRE>
+   Wholescale conversions of model list:
+</PRE>
+<P>
+  <PRE>
+        CONVERT   Convert model list from epoch to epoch or coordinate to
+                   coordinate with conversion of l,m coordinates and intensities
+                   if necessary
+        EDIT      Change model-list overall parameters without conversion of
+                   coordinates and intensity (except possible field rotation if
+                   converting from apparant <-> epoch)
+        REDIT     Change reference coordinates and frequency. Intensities will
+                   be corrected for spectral index only.
+        FEDIT     As REDIT, but intensities will also be corrected for the
+                   effect of different beams at different frequencies
+</PRE> 
+  <PRE>
+        BEAM      Correct sources for attenuation by primary beam
+        DEBEAM    Apply primary-beam attenuation to sources
+</PRE>
+<P>
+  <PRE>
+   Utilities:
+</PRE>
+<P>
+  <PRE>
+        FROM_OLD  convert old format source list (use B1950 or Apparent by
+                   preference)
+        TO_OLD    convert to old format source list
+        NVS       make new version of model file if necessary
+        CVXL      convert formats between machines
+</PRE>
+<P>
+  <PRE>
+        QUIT    finish
+</PRE>
+<P>
+<A NAME=.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter AREA</b></A></H2>
+<P>
+<em>Prompt:</em> Map area: l,m, dl,dm<BR><em>Expected input:</em> Integer:  1 to 4 values
+<P>
+  <PRE>
+Specify the map area to be selected:
+</PRE>
+<P>
+  <PRE>
+        l, m    position in grid spacings of centre of area
+                0,0 is the map centre, increaing toward the upper right (i.e.
+                 with DEcreasing RA and INcreasing DEC)
+</PRE>
+<P>
+  <PRE>
+        dl, dm  horizontal and vertical area sizes
+</PRE>
+<P>
+<A NAME=.calibrators><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter CALIBRATORS</b></A></H2>
+<P>
+<em>Prompt:</em> List of sources or *<BR><em>Expected input:</em> Integer:  1 to 128 values
+<P>
+  <PRE>
+Specify up to 128 numbers of sources in the model list that you want to use as
+calibrators.
+</PRE>
+<P>
+<A NAME=.convert.to><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter CONVERT_TO</b></A></H2>
+<P>
+<em>Prompt:</em> Target coordinate system<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the coordinate system for the output model-list.
+</PRE>
+<P>
+  <PRE>
+If you are CONVERTing, the output model list's coordinates and intensities will
+reflect the new type, frequency, instrument and central coordinates.
+</PRE>
+<P>
+  <PRE>
+If you are EDITing, the new data will be copied only, but the coordinates will
+be rotated to the new Pole if you are converting between apparent and epoch.
+</PRE>
+<P>
+<A NAME=.find.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter FIND_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Finding mode<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify how to select candidate sources:
+</PRE>
+<P>
+  <PRE>
+        POS     Select sources with highest positive brightness
+        ABS     Select sources with highest absolute brightness
+        MANUAL  Select sources manually with the cursor on a GIDS screen.
+                 Sources are selected by pushing MB1; MB3 will finish;
+                 MB2 will not calculate position, but put grid point as clean
+                 source
+</PRE>
+<P>
+<A NAME=.gids.sources><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter GIDS_SOURCES</b></A></H2>
+<P>
+<em>Prompt:</em> Select sources on GIDS display (Yes/No)?&quot;<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if you want to point at sources on the GIDS display for the current map
+</PRE>
+<P>
+<A NAME=.id.start><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter ID_START</b></A></H2>
+<P>
+<em>Prompt:</em> Start identification number<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the start of the ID number to be used in the source list.
+</PRE>
+<P>
+<A NAME=.map.limit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter MAP_LIMIT</b></A></H2>
+<P>
+<em>Prompt:</em> Lower relative intensity limit<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the lowest limit with respect to the maximum in the map that will be
+considered a valid source
+</PRE>
+<P>
+<A NAME=.max.number><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter MAX_NUMBER</b></A></H2>
+<P>
+<em>Prompt:</em> Maximum number of sources to add<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the maximum number of sources that will be found.
+</PRE>
+<P>
+<A NAME=.old.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter OLD_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> old model filename<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the filename (includinhg extension) the an old-format RMODEL file to be
+read or written.
+</PRE>
+<P>
+<A NAME=.reference.data><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter REFERENCE_DATA</b></A></H2>
+<P>
+<em>Prompt:</em> RA, DEC, Freq, rot.,instr.<BR><em>Expected input:</em> DoublePrecision:  1 to 5 values
+<P>
+  <PRE>
+Specify
+</PRE>
+<P>
+  <PRE>
+        RA, DEC (decimal degrees)
+        precession rotation angle (degrees)
+        spectral-index reference frequency (MHz)
+        instrument code (0=WSRT; 1=ATCA)
+</PRE>
+<P>
+  <PRE>
+for the new reference source list position.
+</PRE>
+<P>
+<A NAME=.reference.freq><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter REFERENCE_FREQ</b></A></H2>
+<P>
+<em>Prompt:</em> Reference frequency (MHz)<BR><em>Expected input:</em> DoublePrecision:  1 value
+<P>
+  <PRE>
+Specify the spectral index reference frequency (MHz).
+</PRE>
+<P>
+<A NAME=.ref.scn.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter REF_SCN_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> File name<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the node name with the model overall coordinates to use.
+</PRE>
+<P>
+  <PRE>
+Instead of a file name you may reply with a '*'. You will then be prompted for
+'manual' inpout of data, unless you are CONVRTing between apparent and epoch
+coordinates.
+</PRE>
+<P>
+<A NAME=.ref.scn.set><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter REF_SCN_SET</b></A></H2>
+<P>
+<em>Prompt:</em> ONE sector for reference coordinates: grp.obs.fld.chn.seq<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+Specify ONE .SCN-file sector from which the reference coordinates (RA, DEC,
+frequency) are to be taken.
+</PRE>
+<P>
+  <PRE>
+grp.obs.fld.chn.seq = group.obs.field.channel.sequence_number
+</PRE>
+<P>
+<A NAME=.update.cluster><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter UPDATE_CLUSTER</b></A></H2>
+<P>
+<em>Prompt:</em> Update cluster size in arcsec (l,m)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the cluster size for update in arcsec in the l and m direction.
+</PRE>
+<P>
+<A NAME=.update.mode><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter UPDATE_MODE</b></A></H2>
+<P>
+<em>Prompt:</em> Update type<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify how the update process should proceed:
+</PRE>
+<P>
+  <PRE>
+        SEPARATE        each source to be updated is looked at separately,
+                         and they are fiddled to cater for close sources
+</PRE>
+<P>
+  <PRE>
+        CLUSTER         sources are clustered to bypass closeness problems
+</PRE>
+<P>
+  <PRE>
+        COMBINED        all sources solved in one go, with sub-clustering
+</PRE>
+<P>
+  <PRE>
+        CONSTRAINED     use constraints and clustering. The standard
+                         constraint used is to fix all variables for all
+                         but the lowest intensity source
+</PRE>
+<P>
+  <PRE>
+        L<type>         Loop up to 20 cycles till convergence:
+                         Note that the loop option does not always
+                         work, and is very slow. Preferably use for a
+                         small number of well separated sources/clusters.
+</PRE>
+<P>
+<A NAME=.update.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter UPDATE_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Update mode<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the parameters to be redetermined per source in the update process.
+</PRE>
+<P>
+  <PRE>
+   Position and flux:
+        I       Intensity only
+        LM      Position only
+        ILM     Intensity and position
+        SILM    Intensity, spectral index and position (requires a multichannel
+                 observation with <bandwidth per channel>/<frequency> greater
+                 than ..)
+</PRE>
+<P>
+  <PRE>
+   Source size:
+        EXTEND  Intensity and size parameters for elliptic-Gaussian model
+                 (major/minor axes, position angle)
+</PRE>
+<P>
+  <PRE>
+   Source polarisation:
+        QUV     Stokes Q/I, U/I, V/I
+        PESTIM  Estimate the total linear polarisation, and store it as Stokes
+                 Q. NOTE that this improper use of the model list is not
+                 recorded, so you it is your responsibility to interpret this
+                 kluge correctly.
+</PRE>
+<P>
+  <PRE>
+NOTES:
+        1. All sources in the model are taken into account in determining the
+residual visibilities on which the update fit is performed. However, no updates
+are attempted for sources of type other than 0 nor for CLEAN components.
+        If you want to protect one or more sources from being updated, you can
+do so by temporarily changing their type (OPTION=MODIFY, MODIFY_OPTION=FEDIT,
+see the Help text there).
+</PRE>
+<P>
+  <PRE>
+        2. It is recommended that you use a set of interferometers that gives a
+uniform baseline coverage, e.g. by selecting fixed-movable (FM) interferometers
+only.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nmodel_public_intfc/images.pl b/nmodel_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nmodel_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nmodel_public_intfc/labels.pl b/nmodel_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..2628fec1d4b7de2eed266b1554c70c534bead334
--- /dev/null
+++ b/nmodel_public_intfc/labels.pl
@@ -0,0 +1,31 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".beam.descr"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".beam.freq.0"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".edit.field"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".beam.freq.1"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".edit.value"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".names.file"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".clear.ref"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".merge.radius"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".source.list"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".sort.type"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".model.option"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".source.number"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".delete.area"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".beam.scale"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".beam.factor.0"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".sort.centre"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".source.range"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".model.show"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".source"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".beam.factor.1"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".sort.field"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".delete.level"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".source.factors"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".model.action"} ="$URL/nmodel_public_intfc.html"; 
+$external_labels{".model.modify"} ="$URL/nmodel_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/nmodel_public_intfc/nmodel_public_intfc.html b/nmodel_public_intfc/nmodel_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..eccc1aeddea7f70b1044a605bcd818b4b7b829b0
--- /dev/null
+++ b/nmodel_public_intfc/nmodel_public_intfc.html
@@ -0,0 +1,732 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group NMODEL</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nmodel_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nmodel_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<UL> 
+<LI> <A NAME=tex2html3 HREF=nmodel_public_intfc.html#SECTION0002100000000000000>  <b>Parameter BEAM_DESCR</b></A>
+<LI> <A NAME=tex2html4 HREF=nmodel_public_intfc.html#SECTION0002200000000000000>  <b>Parameter BEAM_FACTOR_0</b></A>
+<LI> <A NAME=tex2html5 HREF=nmodel_public_intfc.html#SECTION0002300000000000000>  <b>Parameter BEAM_FACTOR_1</b></A>
+<LI> <A NAME=tex2html6 HREF=nmodel_public_intfc.html#SECTION0002400000000000000>  <b>Parameter BEAM_FREQ_0</b></A>
+<LI> <A NAME=tex2html7 HREF=nmodel_public_intfc.html#SECTION0002500000000000000>  <b>Parameter BEAM_FREQ_1</b></A>
+<LI> <A NAME=tex2html8 HREF=nmodel_public_intfc.html#SECTION0002600000000000000>  <b>Parameter BEAM_SCALE</b></A>
+<LI> <A NAME=tex2html9 HREF=nmodel_public_intfc.html#SECTION0002700000000000000>  <b>Parameter CLEAR_REF</b></A>
+<LI> <A NAME=tex2html10 HREF=nmodel_public_intfc.html#SECTION0002800000000000000>  <b>Parameter DELETE_AREA</b></A>
+<LI> <A NAME=tex2html11 HREF=nmodel_public_intfc.html#SECTION0002900000000000000>  <b>Parameter DELETE_LEVEL</b></A>
+<LI> <A NAME=tex2html12 HREF=nmodel_public_intfc.html#SECTION00021000000000000000>  <b>Parameter EDIT_FIELD</b></A>
+<LI> <A NAME=tex2html13 HREF=nmodel_public_intfc.html#SECTION00021100000000000000>  <b>Parameter EDIT_VALUE</b></A>
+<LI> <A NAME=tex2html14 HREF=nmodel_public_intfc.html#SECTION00021200000000000000>  <b>Parameter MERGE_RADIUS</b></A>
+<LI> <A NAME=tex2html15 HREF=nmodel_public_intfc.html#SECTION00021300000000000000>  <b>Parameter MODEL_ACTION</b></A>
+<LI> <A NAME=tex2html16 HREF=nmodel_public_intfc.html#SECTION00021400000000000000>  <b>Parameter MODEL_MODIFY</b></A>
+<LI> <A NAME=tex2html17 HREF=nmodel_public_intfc.html#SECTION00021500000000000000>  <b>Parameter MODEL_OPTION</b></A>
+<LI> <A NAME=tex2html18 HREF=nmodel_public_intfc.html#SECTION00021600000000000000>  <b>Parameter MODEL_SHOW</b></A>
+<LI> <A NAME=tex2html19 HREF=nmodel_public_intfc.html#SECTION00021700000000000000>  <b>Parameter NAMES_FILE</b></A>
+<LI> <A NAME=tex2html20 HREF=nmodel_public_intfc.html#SECTION00021800000000000000>  <b>Parameter SORT_CENTRE</b></A>
+<LI> <A NAME=tex2html21 HREF=nmodel_public_intfc.html#SECTION00021900000000000000>  <b>Parameter SORT_FIELD</b></A>
+<LI> <A NAME=tex2html22 HREF=nmodel_public_intfc.html#SECTION00022000000000000000>  <b>Parameter SORT_TYPE</b></A>
+<LI> <A NAME=tex2html23 HREF=nmodel_public_intfc.html#SECTION00022100000000000000>  <b>Parameter SOURCE</b></A>
+<LI> <A NAME=tex2html24 HREF=nmodel_public_intfc.html#SECTION00022200000000000000>  <b>Parameter SOURCE_FACTORS</b></A>
+<LI> <A NAME=tex2html25 HREF=nmodel_public_intfc.html#SECTION00022300000000000000>  <b>Parameter SOURCE_LIST</b></A>
+<LI> <A NAME=tex2html26 HREF=nmodel_public_intfc.html#SECTION00022400000000000000>  <b>Parameter SOURCE_NUMBER</b></A>
+<LI> <A NAME=tex2html27 HREF=nmodel_public_intfc.html#SECTION00022500000000000000>  <b>Parameter SOURCE_RANGE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group NMODEL, (part of) which is included in all those <i>NEWSTAR </i> programs that manipulate models in .MDL and/or .SCN files.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.beam.descr><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0002100000000000000>  <b>Parameter BEAM_DESCR</b></A></H2>
+<P>
+  <em>Prompt:</em> Beam descriptors (<em>may vary per application</em>)<BR><em>Expected input:</em> Integer:  1 to 32 values
+<P>
+    <PRE>
+Describe the primary beam for an instrument other than the WSRT or the ATCA.
+Here you specify the formula to be used; later you will be asked for values for
+the coefficients.
+</PRE>
+<P>
+  <PRE>
+Each instrument (up to 8) is decribed by four numbers, with (in order) the
+following meaning:
+</PRE>
+<P>
+  <PRE>
+  - the value of the * in BEAM_FREQ_* and BEAM_FACTOR_* to use
+</PRE>
+<P>
+  <PRE>
+  - the type of formula:
+        0= cos(factor*freq(MHz)*angle(degree))**6;
+        1= 1/(1+fac1*(freq(GHz)*angle(arcmin))**2+fac2*...);
+        2= 1+fac1*(freq(GHz)*angel(arcmin))**2+fac2*...)
+</PRE>
+<P>
+  <PRE>
+  - the number of factors per frequency range in BEAM_FACTOR_*
+</PRE>
+<P>
+  <PRE>
+  - the number of frequency ranges specified in BEAM_FREQ_*
+</PRE>
+<P>
+  <PRE>
+Instruments are: first WSRT, second ATCA
+</PRE>
+<P>
+<A NAME=.beam.factor.0><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002200000000000000>  <b>Parameter BEAM_FACTOR_0</b></A></H2>
+<P>
+<em>Prompt:</em> Beam feed factors (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 64 values
+<P>
+  <PRE>
+Specify per frequency band specified in BEAM_FREQ_0 the factors to be used in
+the primary beam calculation formula (see BEAM_DESCR). This is for WSRT cos**6
+</PRE>
+<P>
+<A NAME=.beam.factor.1><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002300000000000000>  <b>Parameter BEAM_FACTOR_1</b></A></H2>
+<P>
+<em>Prompt:</em> Beam feed factors (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 64 values
+<P>
+  <PRE>
+Specify per frequency band specified in BEAM_FREQ_1 the factors to be used in
+the primary beam calculation formula (see BEAM_DESCR). This is for ATCA
+1/(1+ai.x**2i)
+</PRE>
+<P>
+<A NAME=.beam.freq.0><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002400000000000000>  <b>Parameter BEAM_FREQ_0</b></A></H2>
+<P>
+<em>Prompt:</em> Beam feed frequencies (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 8 values
+<P>
+  <PRE>
+Specify in increasing order the frequency bands to be used in calculating the
+primary beam. For each value there should be a corresponding set of values in
+BEAM_FACTOR_0 (the number of values in BEAM_DESCR).These factors will be used
+up to the corresponding frequency specified.
+</PRE>
+<P>
+<A NAME=.beam.freq.1><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002500000000000000>  <b>Parameter BEAM_FREQ_1</b></A></H2>
+<P>
+<em>Prompt:</em> Beam feed frequencies (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 8 values
+<P>
+  <PRE>
+Specify in increasing order the frequency bands to be used in calculating the
+primary beam. For each value there should be a corresponding set of values in
+BEAM_FACTOR_1 (the number of values in BEAM_DESCR).These factors will be used
+up to the specified corresponding frequency (MHz).
+</PRE>
+<P>
+<A NAME=.beam.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002600000000000000>  <b>Parameter BEAM_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> Scale factor for primary-beam width (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify a scaling factor for the primary beam calculations. If, e.g. a beam has
+been defined (by BEAM_FACTOR) for a 25 m dish, it can be used for a 20 m dish
+by specifying here 20./25. (or 0.8)
+</PRE>
+<P>
+<A NAME=.clear.ref><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002700000000000000>  <b>Parameter CLEAR_REF</b></A></H2>
+<P>
+<em>Prompt:</em> Clear reference coordinates (Yes/No)? (<em>may vary per application</em>)<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+If you answer YES to this prompt, the reference coordinates of the model will
+be reset. Otherwise, only the number of components will be set to zero.
+</PRE>
+<P>
+<A NAME=.delete.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002800000000000000>  <b>Parameter DELETE_AREA</b></A></H2>
+<P>
+<em>Prompt:</em> Area l,m, dl,dm (arcsec) (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 4 values
+<P>
+  <PRE>
+Specify the area in which all sources should be deleted:
+</PRE>
+<P>
+  <PRE>
+        l,m     area centre (0,0 = map centre)
+        dl,dm   area size
+</PRE>
+<P>
+<A NAME=.delete.level><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0002900000000000000>  <b>Parameter DELETE_LEVEL</b></A></H2>
+<P>
+<em>Prompt:</em> Lower flux limit (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Source whose absolute flux is below the value specified here will be deleted
+from the model list.
+</PRE>
+<P>
+<A NAME=.edit.field><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021000000000000000>  <b>Parameter EDIT_FIELD</b></A></H2>
+<P>
+<em>Prompt:</em> Source attribute to edit| (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify the source attribute that you want to edit:
+</PRE>
+<P>
+  <PRE>
+   Source coordinates:
+</PRE>
+<P>
+  <PRE>
+        L, M          coordinates relative to reference (arcsec)
+</PRE>
+<P>
+  <PRE>
+   Properties of the source:
+</PRE>
+<P>
+  <PRE>
+        I             ampitude
+        SI            spectral index
+        RM            intrinsic rotation measure
+        Q, U, V       Stokes parameters in %
+        LA, SA, PA    long axis short axis, position angle of elliptic-Gaussian
+                       extended-source model
+</PRE>
+<P>
+  <PRE>
+   Administrative attributes in the model list:
+</PRE>
+<P>
+  <PRE>
+        ID            identification
+        BITS          bits mask (if source is extended, has polarisation)
+</PRE>
+<P>
+  <PRE>
+        TYP           source type (0 is the standard)
+</PRE>
+<P>
+  <PRE>
+        CCBM          clean component (1) and beam-corrected (8)
+</PRE>
+<P>
+  <PRE>
+        TP2           reserved
+</PRE>
+<P>
+<A NAME=.edit.value><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021100000000000000>  <b>Parameter EDIT_VALUE</b></A></H2>
+<P>
+<em>Prompt:</em> New value (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the value to set in specified edit field.
+</PRE>
+<P>
+<A NAME=.merge.radius><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021200000000000000>  <b>Parameter MERGE_RADIUS</b></A></H2>
+<P>
+<em>Prompt:</em> Coincidence radii dl,dm (arcsec) (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Point sources that are within (dl,dm) arcsec of each other are combined. The
+suggested default values are approximately half the synthesised  beam radius in
+l and m directions.
+</PRE>
+<P>
+<A NAME=.model.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021300000000000000>  <b>Parameter MODEL_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> specify model disposition and format in the order shown,|- (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 to 5 values
+<P>
+  <PRE>
+NOTE:
+        The defaults proposed have been chosen to minimise the time needed for
+the lengthy (re)calculations of model visibilities. The price you pay for this
+is a near-doubling of the size of the sectors in your .SCN file in which you
+store a model. Your priorities may be different, but before choosing
+non-default options make sure you understand the consequences.
+</PRE>
+<P>
+  <PRE>
+        In principle, the model list now in memory will be used to calculate
+the model sources' visibilities in your observation(s).
+</PRE>
+<P>
+  <PRE>
+        To avoid this lengthy calculation where possible, the program will try
+to use model visibilities stored earlier in the .SCN file. To this end, it will
+read the model list from the .SCN file and combine it with the list in core,
+then (re)calculate the visibilities only for those components that are not
+represented correctly in the .SCN file. Having done that, the program may or
+may not save the combined model and its visibilities back into the .SCN file.
+</PRE>
+<P>
+  <PRE>
+        You must select ONE of the following options for the combination and
+subsequent storage:
+</PRE>
+<P>
+  <PRE>
+   MERGE       Merge the model in the .SCN file with the one in core discarding
+                duplicates, i.e. components with identical position, extent and
+                flux; store the combined model in the .SCN file.
+               This option is suitable in the most common situations, viz.:
+                  - the list in core is an extension containing the list in the
+                    .SCN file as a subset; or
+                  - the list in core is an incremental update, i.e. a list of
+                    aditional components.
+</PRE>
+<P>
+  <PRE>
+   INCREMENT   As MERGE, but retain the resultant model IN CORE ONLY without
+                changing the .SCN file
+</PRE>
+<P>
+  <PRE>
+   NEW         Overwrite the model in the SCN file with the model in core.
+</PRE>
+<P>
+  <PRE>
+   TEMPORARY   Use the model in core, ignoring the one in the SCN file.
+</PRE>
+<P>
+  <PRE>
+   ADD         As MERGE, but without discarding any components, i.e. fluxes
+                of coincident sources are added.
+               This option will produce the same effect as MERGE in the case
+                that the list in core is an incremental update. Its use is
+                recommended for special applications only.
+</PRE>
+<P>
+  <PRE>
+        Separately from the above, you may define which effects must be
+accounted for in the visibility calculations. The four items below must be
+specified in the order shown. You may select the default by skipping the item,
+typing only the delimiter comma; for example ',,\BEAM' will select the
+defaults for the first four items.
+</PRE>
+<P>
+  <PRE>
+   BAND/NOBAND   To correct or not correct the radial extent of your model
+                  components for the smearing due to your finite observing
+                  bandwidth
+</PRE>
+<P>
+  <PRE>
+   TIME/NOTIME   To correct or not correct the tangential extent of your model
+                  model components for the smearing due to the finite
+                  integration time of your observation
+</PRE>
+<P>
+  <PRE>
+   INPOL/NOINPOL To correct or not correct the polarisation components
+                  Q,U,V of your model for the effect of position-dependent
+                  primary-beam polarisation.
+                 (NOTE: The iNPOL option is currently disabled.)
+</PRE>
+<P>
+  <PRE>
+   BEAM/NOBEAM   To correct or not correct your model fluxes for the
+                  position-dependent gain of the primary beam.
+</PRE>
+<P>
+  <PRE>
+NOTE that specifying options different from those used earlier in calculating
+the model visibilities that are noe now in the .SCN file will result in a
+partial or complete recalculation of the visibilities.
+</PRE>
+<P>
+<A NAME=.model.modify><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021400000000000000>  <b>Parameter MODEL_MODIFY</b></A></H2>
+<P>
+<em>Prompt:</em> Model-handling action (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify what you want to do with the model list in core:
+</PRE>
+<P>
+  <PRE>
+   Consolidating/rearranging the list:
+</PRE>
+<P>
+  <PRE>
+        MERGE   Combine (point-) sources at the same position.
+                 Must have the same spectral index and rotation measure.
+                 Stokes Q,U,V are properly taken into account.
+                 CLEAN components are NOT combined with non-CLEAN comp.
+                 Extended sources are ignored.
+        RMERGE  As MERGE, but within specified radius (which may be 0).
+                 The (l,m) position of the strongest source is taken.
+                 CLEAN components are combined if at the same position.
+</PRE> 
+  <PRE>
+        SORT    Sort source list in decreasing amplitude. (This will be done
+                 automatically when you write the list back to a .MDL file.)
+        FSORT   Sort on a specified field in source list (for subsequent
+                 display)
+</PRE>
+<P>
+  <PRE>
+   Modifying sources in the list:
+</PRE>
+<P>
+  <PRE>
+        CALIB   Calibrate the source list to a new amplitude and/or position
+        EDIT    Edit source list (an amplitude of zero will delete the source)
+        FEDIT   Edit a field in a range of sources
+        FLUX_KNOWN Toggle the 'unknown-flux' bit. When this bit is off, NCALIB
+                 will by default refrain from attempting a Selfcan gain
+                 solution.
+</PRE>
+<P>
+  <PRE>
+   Deleting sources in the list:
+</PRE>
+<P>
+  <PRE>
+        DEL     Delete sources
+        DNCLOW  Delete non-clean sources with low amplitudes
+        DCLOW   Delete clean components with low amplitudes
+        DAREA   Delete sources in specified area
+</PRE>
+<P>
+  <PRE>
+   Miscellaneous:
+</PRE>
+<P>
+  <PRE>
+        SHOW       Show the list. (You will be prompted for details)
+</PRE>
+<P>
+  <PRE>
+        QUIT       Quit model-handling.
+</PRE>
+<P>
+<A NAME=.model.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021500000000000000>  <b>Parameter MODEL_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Model-list action| (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the action to be taken on the internal model list:
+</PRE>
+<P>
+  <PRE>
+   Transfers between the internal list and an external file:
+</PRE>
+<P>
+  <PRE>
+        READ   Read the components from a .MDL file on disk into the
+                program's model list. The default filename is the name of
+                the calibrator belonging to the most recently read sector,
+                derived from the fieldname and the frequency. .MDL files are
+                first searched for in the current directory or the directory
+                defined by parameter DATAB. If this fails, the file is looked
+                for in the directory defined by parameter MODELB and finally by
+                that defined by the Unix environment variable MODELB.
+</PRE>
+<P>
+  <PRE>
+               NOTE that reading is INCREMENTAL, so if you read the same
+                .MDL file twice, you will get every component doubled...
+</PRE>
+<P>
+  <PRE>
+        WRITE  Write the program's model list to a .MDL file.
+</PRE>
+<P>
+  <PRE>
+        INTERN This does not affect the list, but selects
+                the model stored in the scan-file(s). Selecting INTERN is
+                equivalent to setting DE_APPLY=MODEL.
+                You may use this internal model in combination with
+                components in the program's model list.
+</PRE>
+<P>
+  <PRE>
+   Modification and display of the internal list:
+</PRE>
+<P>
+  <PRE>
+        CLEAR  Empty the program's model list and optionally its reference
+                coordinates.
+</PRE>
+<P>
+  <PRE>
+        ADD    Manual input of sources to add the list
+</PRE>
+<P>
+  <PRE>
+        MODIFY Enter a submenu with options to modify the model list:
+                  - by deleting sources from the list;
+                  - by editing entries manually;
+                  - by sorting (for subsequent display) the list: you will be
+                     prompted for a definition of the sort order;
+                  - by calibrating.
+</PRE>
+<P>
+  <PRE>
+        SHOW   Show the program's model list, you will be prompted for details.
+</PRE>
+<P>
+  <PRE>
+        QUIT   Exit from model-handling.
+</PRE>
+<P>
+<A NAME=.model.show><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021600000000000000>  <b>Parameter MODEL_SHOW</b></A></H2>
+<P>
+<em>Prompt:</em> Model listing mode (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify what type of listing you want, and where it should be shown:
+</PRE>
+<P>
+  <PRE>
+   LIST   Show the program's model list in the log file.
+   SHOW   Idem, but both on the terminal and in the log file.
+</PRE>
+<P>
+  <PRE>
+   RLIST  Show the program's model list in RA/DEC coordinates in the log file.
+   RSHOW  Idem, but both on the terminal and in the log file.
+</PRE>
+<P>
+  <PRE>
+   TOTAL  Show the statistics of the program's model list.
+</PRE>
+<P>
+  <PRE>
+   QUIT   Back to MODEL_OPTION.
+</PRE>
+<P>
+<A NAME=.names.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021700000000000000>  <b>Parameter NAMES_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> File with source names (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the full name of the input disk-file. The file should contain lines
+with Ra, Dec and Name, separated by white space. Comments may be added starting
+with an exclamation mark. A NULL answer (two double quotes) will ignore the
+name-list: no file will be opened.
+</PRE>
+<P>
+<A NAME=.sort.centre><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021800000000000000>  <b>Parameter SORT_CENTRE</b></A></H2>
+<P>
+<em>Prompt:</em> Reference coordinates l,m|- (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the reference coordinates for the distance sort that you selected.
+</PRE>
+<P>
+<A NAME=.sort.field><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00021900000000000000>  <b>Parameter SORT_FIELD</b></A></H2>
+<P>
+<em>Prompt:</em> Sort criterion (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify sourfce attribute on which to sort:
+</PRE>
+<P>
+  <PRE>
+   Source coordinates:
+</PRE>
+<P>
+  <PRE>
+        L, M          l or m, arbitrary order for the other
+        LM, ML        l and then m, or m and then l
+        DIST          distance to a specified reference point
+</PRE>
+<P>
+  <PRE>
+   Properties of the source:
+</PRE>
+<P>
+  <PRE>
+        I             ampitude
+        SI            spectral index
+        POL           polarised intensity
+        RM            intrinsic rotation measure
+        Q, U, V       Stokes parameters in %
+        LA, SA, PA    long axis short axis, position angle of elliptic-Gaussian
+                       extended-source model
+</PRE>
+<P>
+  <PRE>
+   Administrative attributes in the model list:
+</PRE>
+<P>
+  <PRE>
+        ID            identification
+        BITS          bits mask (if source is extended, has polarisation)
+</PRE>
+<P>
+  <PRE>
+        TYP           source type (0 is the standard)
+</PRE>
+<P>
+  <PRE>
+        CCBM          clean component (1) and beam-corrected (8)
+</PRE>
+<P>
+  <PRE>
+        TP2           reserved
+</PRE>
+<P>
+<A NAME=.sort.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022000000000000000>  <b>Parameter SORT_TYPE</b></A></H2>
+<P>
+<em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+        Specify the polarity of the sort
+</PRE>
+<P>
+<A NAME=.source><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022100000000000000>  <b>Parameter SOURCE</b></A></H2>
+<P>
+<em>Prompt:</em> I,l,m,id,Q,U,V,lax,sax,pa,si,rm,rs (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 13 values
+<P>
+  <PRE>
+Specify the source parameters in order shown.
+</PRE>
+<P>
+  <PRE>
+   I            intensity (W.U.)
+   l, m         coordinates w.r.t. reference (arcsec)
+   id           identification number (see below)
+   Q            Stokes Q relative to I (%
+   U            Stokes U relative to I (%
+   V            Stokes V relative to I (%
+   lax          long-axis full halfwidth (arcsec, =0 for a point source)
+   sax          short-axis full halfwidth (arcsec, =0 for a point source)
+   pa           position angle of long axis (degrees, North through East)
+   si           spectral index
+   rm           intrinsic rotation measure ( rad/m**2 at 1 Ghz)
+   rs           reserved
+</PRE>
+<P>
+  <PRE>
+You may omit values that you want to leave alone, but not the commas that
+delimit them. Trailing values and commas may be omitted.
+</PRE>
+<P>
+  <PRE>
+    Example:
+        ,,3 will set m to 3 and leave all other parameters unchanged.
+</PRE>
+<P>
+  <PRE>
+The identification number is of the form
+</PRE>
+<P>
+  <PRE>
+        <sequence number>-<mask byte>
+</PRE>
+<P>
+<A NAME=.source.factors><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022200000000000000>  <b>Parameter SOURCE_FACTORS</b></A></H2>
+<P>
+<em>Prompt:</em> Amlitude ratio Anew/Aold, | shift dl,dm (arcsec) (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 3 values
+<P>
+  <PRE>
+Specify the calibration parameters in te order shown:
+  An/Ao new/old amplitude
+  dl    new-old l in arcsec
+  dm    new-old m in arcsec
+</PRE>
+<P>
+<A NAME=.source.list><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022300000000000000>  <b>Parameter SOURCE_LIST</b></A></H2>
+<P>
+<em>Prompt:</em> Source number list (<em>may vary per application</em>)<BR><em>Expected input:</em> Integer:  1 to 128 values
+<P>
+  <PRE>
+Specify a list of individual source numbers to be acted upon. If you want to
+spaecfy a range, reply '*' here and wait for the next prompt
+</PRE>
+<P>
+<A NAME=.source.number><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022400000000000000>  <b>Parameter SOURCE_NUMBER</b></A></H2>
+<P>
+<em>Prompt:</em> Source number (<em>may vary per application</em>)<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the number of the source to be acted upon.
+</PRE>
+<P>
+<A NAME=.source.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00022500000000000000>  <b>Parameter SOURCE_RANGE</b></A></H2>
+<P>
+<em>Prompt:</em> Source number range (<em>may vary per application</em>)<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+Specify the first and last source number to process. * indicates 'all'. If you
+want all sources from some number <N> upward, reply
+</PRE>
+<P>
+  <PRE>
+        '<N>-<some very large number>'.
+</PRE>
+<P>
+
+<P>.
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+<P>.
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+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nnews.txt b/nnews.txt
new file mode 100644
index 0000000000000000000000000000000000000000..5cc4c64e68184fb046cfc4c969eb1d8c218f7bda
--- /dev/null
+++ b/nnews.txt
@@ -0,0 +1,730 @@
+1 NNews
+ 1000929 Allow reading leiden data from CD-ROM
+ 1000929 Repair problem locating MDL files
+ 1000929 Correct bug in COR data display; add stepping over sets in SCAN display
+ 1000922 Correct double 29 in DCB data from MS
+ 1000922 Solved rounding problem when flagging mosaic data using CHAN
+ 1000922 Added the display of polarisation channels if no ap solution
+ 1000921 Repair milennium bug in update procedure
+ 000309 NSCAN: Allow for CD-ROM directories
+ 000309        Add 99A, 99B for project numbers
+ 000309 NPLOT: phase continuity added
+ 000309        Changed the MXNCH to 8192 to plot long 10s files
+ 000309 ALL: Default for MODEL_ACTION now uses BEAM instead of NOBEAM
+ 000309 NCALIB: fix FCA used for reading data for vzero calculation
+ 000309         solves a problem with DZB data reported by AGB
+ 000309         Added loops to SET -- INIT
+ 000309 NGCALC: Corrected a missing argument that made ngcalc plot crash
+ 000309 NMODEL: Add extra model update modes (but not implement them yet)
+ 000309         Add messages that X* updates not yet implemented.
+ 000309         Corrected update convergence for 'I' only case
+ 000309 NMAP: [C]MEMORY_USE max. 4 --> 32 MB (request by AGB)
+ 980707 System: Various changes for logbook and CD-ROM stuff
+                NFRA: remove ws4, ws5, ws7 stuff, use daw18 for compile/linking
+                add script to read WSRT-logbook
+ 980707 NPLOT: change dot pattern for connecting lines
+ 980707        phase continuity; better connecting lines
+ 980707 NCALIB: For better calculating MIFR
+ 970728 NPLOT: modification related to remove control-C plot control
+ 970605 NPLOT: Make default coordinate contouring grid size 256
+               Some changes for plotting exactly on pole
+ 970530 NPLOT: Correct plotting of coordinates and ticks near pole.
+               A selectable precision (COORD_PREC) possible.
+ 970529 NSCAN UVFITS: Allow multiple BITPIXes, 
+                      better grouping of sets in labels
+                      Extra prompt for BITPIX
+ 970529 System: Included check for non-existent conversion from DEC,L to RA,M
+ 970529 NPLOT: Coordinate plotting near pole
+ 970509 NSCAN/NFLAG: improve formatting of X/Y arrays
+ 970509 NCOPY: add new option SHORTCOPY
+ 970509 NPLOT: plot control through control-C
+  	       SPECIAL options:
+	  	   alternatives for HA scale
+	 	   hour-angle integration
+		   annotation text
+	       new SORT=INVERT option: transposed interferometer order
+	       new data types AGAIN, PGAIN: ampl. and phase of data/model
+	       plot order XXgain, XXphase ... i.s.o. XXgain, YYgain ...
+	       raster lines on tel/interfmr plots
+	       increase font size for 'PLUVO' plots
+	       nonlinear gain scale to accomodate very large and very small gains
+               modification related to control-C plot control in NPLOT
+               correct scales for BAND mode
+ 970509 NCALIB: New algorithm for VZERO calculation
+                Add USIGN to resolve sign ambiguity in Stokes U
+                Calculate and report GZD
+                Revise gain normalisation algorithm (had never been tested!)
+                Revise ME calculation in ncalib.for
+                extend GAIN_NORM help text to include -1 option
+ 970509 System NFRA: do  'setenv LPDEST jet5'  to use new printer
+               Fixes/changes in record/replay
+               Small changes for LICK and WSRT
+               Changes for RUG (add Solaris)
+               Add IONOST for HP
+ 970509 NSCAN: Give error-message in case WNFRD return an error  - bug 229 
+ 970509 All: Filename-problem on Solaris solved  - bug 224 
+             Logging of selected IFRs also in logfile  - bug 228 
+ 970509 NMAP: problem in FITS maps created by NMAP solved  - bug 221 
+ 970509 NCLEAN: fixed crash problem when reading visibility data  - bug 226 
+ 961108 NSCAN: Corrections for archive 
+ 961017 NCOPY: add special option for holographic beam measurements
+ 961017 NCALIB: fix loose ends from earlier change of dispatching codes
+                CCOPY should now work as advertised
+                Renormalisation: Leave undefined corrections (TCOR=0) undefined
+ 961017 NSCAN: Correct use of band8 bandwidth for versions<46
+ 961017 NSCAN UVFITS: Use RR,LL etc instead of XX,YY because of problems with UVLOD in AIPS
+ 961017 All: use . i.s.o. - in interfm display for better visual appearance
+ 960813 NCALIB: correct VZERO calculation
+                suppress 'XY constrains' output in log file
+                correct code for SETCLK (was treated as SETMIFR)
+                correct SHOW output format
+ 960813 NPLOT: correct misleading comment
+ 960813 NSCAN: Add bytecount for CHECK
+ 960813 System: add files for site LICK, add Dec-Alpha/OSF1 in Bonn
+ 960626 NPLOT: change plot annotaion format
+               change interface to ST plot options: ST_ prefix in IFR_MODE
+               replaced by S_ prefix in OPTION
+               new keyword HA_MODE for special effects in vertical scale
+ 960626 NCALIB: For REDUN option: Take all interferometers. (Also 00, 11 etc.)
+ 960626 NMODEL: show RA and DEC in show header also in decimal format
+ 960626 NSCAN/NFLAG: fine-tune overview formatting
+               bug fix in MAXD calculation for NSCSCF
+ 960626 NSCAN: Read correct OH-length for mosaik observations
+ 960626 NCOPY: Fix serious bugs - must have been there for several months!
+               zero IFRMC, IFRAC, emit user message  - bug 141 
+ 960626 System: add files for Solaris system
+                Situation at RUU changed
+ 960520 NCALIB: extend help texts for BASEL_xxx parameters
+ 960513 NCOPY/NPLOT/NGIDS/NCLEAN: warning if /NORUN
+ 960502 Documentation: Several small bugs fixed
+ 960422 NMAP: RA,DEC in header within proper ranges
+              emergency bandage for the HOLOG mess: new keywords OLDHOLOG and NEWHOLOG
+              report filename on open failures
+              find free label if * specified (previously * was equivalent to 1)
+              return to nmadat after most actions
+                 (in batch mode, input EOF will cause nmap to QUIT as before)
+ 960422 NMODEL: option RMERGE: merges model components that are within radius
+                removed bug from UPDATE option QUV
+ 960422 NPLOT: Do not ask IFR_MODE when OPTION=TELESCOPE  - bug 161 
+               Correct MB3 or X exit loop  - bug 200 
+               add plot modes STNORM, STSORT: using ST i.s.o. HA
+ 960422 NSCAN/NFLAG: Type text for COR/UNCOR and if something NOT present  - bug 169 
+ 960422 NSCAN: corrected a bug in precession angle calculation  - bug 0217 
+               Add pol.code for DXB/DCB IF-sets, Increase max number of sets
+ 960422 NFLAG: new options: UXY and VXY 
+ 960422 NCOPY: interferometer selection, SELECT_IFRS parameter
+ 960422 NCALIB: Correct Copy MIFR corrections (SET_OPTION=ICOPY)  - bug 181 
+ 960422 IONOS: Changed averaging (first days, then hours)
+ 960422 All: truncate '.<number>' in mosaic field name to get correct default MDL name
+ 960422 System: add I_HPWSRT.CSH
+                new routine for calculating sidereal time
+                add dwrec|p|n aliases
+ 960130 NMAP RFITS: Do not abort when error in FITS header found
+ 960130 System: correct problem with unlocking of files  - bug 142 
+        System: some small updates, mainly for NFRA purpose
+ 960130 Documentation: remove FULL command in ndoc: replaced by ALL
+ 960130 NCLEAN: Move comments to new line
+ 960130 NSCAN: Change name for Scissor: CONTLINE now OBSMODE
+ 960130 NMODEL: Reminder if INTERN is on  - bug 156 
+ 960130 NFLAG: Explanation for STATISTICS GROUPS option, correct flow, 
+               IFR output  - bug 149 151 153 189 190 
+ 960130 NCALIB: Add message concerning model selection for REDUN  - bug 178 
+                Reset Scan counter for SET ZERO  - bug 185 
+ 960130 NSCAN: Some explanation for layout  - bug 172 
+ 960130 NMAP: REF_COORD RA always positive  - bug 193 
+              RFITS: Message if Disk files not found
+ 960130 NPLOT: merge HjV 941031, 950711, 950718 with my own changes.
+               Fix help text for IFR_MODE  - bug 201 
+ 960130 NFLAG: Comments; add detour into MODE from STATIST branch;  - bug 190 
+               add labels 183, 193 (CMV's fix for bug 190)
+ 960130 All programs: add OVERVIEW=ALTOBS option
+ 960130 System: implements the dwre? commands; 
+ 960130 System: Add LD_LIBRARY_PATH for site UCSB
+ 951215 System: Add new site: AIRUB (Bonn)
+ 951213 Correct REF_COORD backtrack error  - bug 194 
+ 951213 System: Add environment n_www
+                Used to specify your favorite WWW browser.
+                If you don't define it, xmosaic (part of Newstar
+                distibution) will be used.
+                You may change n_www in your newstar_<site>.csh
+                When changing this file, please check it in with: nsh in
+ 951205 SYSTEM: Add site IRABO, add some missing files
+ 951205 MODELS:Adding a new model file for 1127-145 at 21cm
+ 951205        New improved model for 3C295 at 21cm from reduction group
+ 951205        New improved models for 325 MHz (92cm)
+ 951205 NMAP: correction of logic for FIELD_SHIFT/FIELD_CENTRE  - bug 139
+ 951205 NSCAN: Made Scissor interface more robust
+ 951205 NCALIB: correct REDUN output: last column I (= nr of iterns) decimal
+ 951205 Correct scaling of errors (/10 instead of *10)
+ 921205 PPD: Donot remember ?? request, so user retains access to terminal
+             help trough ?  - bug 154 
+ 951205 System: add DAT-device for DAW13 (NFRA-only)
+ 951205 NFLAG: correct EXPLAIN bug showing RMS 3 times 
+ 951205 Documentation: 
+           1. Revision of documentation system - various bug fixes
+              - more robust - better cross-referencing
+           2. groundwork for batch recording system
+ 951205 NMAP: Implement complex summing/rotation measures
+ 951205 NSCAN: Add ARC option for LEIDEN tapes
+        Therefore WARC changed to ARC and added two new sub-options for ARC
+ 950822 New Newstar release: 6.1
+ 950821 NCALIB SET IREF Help text corrected
+ 950821 Scissor: Improve options for ionos, add filpo option
+ 950821 NMAP: Rough trial to produce P^2 maps (pol type LI)
+              Prepare improved polarised intensity map
+ 950714 NCALIB: Include MIFR setting
+                New least squares: better mean errors in polarisation calculations
+                Improved 'complex' solutions for calibration
+                Change in writing interferometer errors for missing telescopes
+                Add option ICOPY for SET_OPTION (Copy MIFR-corrections)
+ 950714 NCLEAN DATA Clean: correct restored map when using DataFactor (new keyword)
+ 950714 NSCAN: Add MDLNODE_PEF (model keyword was missing)
+               Add NSCSCY to NSCSCR for UVLIN type operations
+ 950714 NPLOT: Re-open SCN-file for update when models found  - bug 127 
+               Plot all PHASE residuals in W.U.
+               Add (hidden) keyword PLOT_HEADING (Def. YES / NOASK)
+ 950714 NGCALC: Change SET_ACTION in SECTOR_ACTION, add EDIT
+ 950714 NPLOT/NGCALC: Add A0-plotter, therefore changed options for 
+                    keyword PLOTTER and added keyword PLOT_FORMAT
+ 950714 NMODEL: Update option extended with, a.o., clustering, position only
+                Add constrained update
+                Model update correction for constrained clusters of more 
+                    than 2 sources
+                Added looped updates: not always perfect; slow, and most 
+                    useful for small number of well separated sources/clusters
+ 950714 System: some changes for use in Leiden
+ 950714 Documentation: Use latex2html stuff from Newstar account
+                       Correct some typo's in tex-files
+                       Add plotter_public_intfc.tex and change some other
+ 950714 NFILT: Create the program to calculate continuum from the UV data
+ 950714 NGEN: Change (DE_)APPLY so it has the same options as X_(DE_)APPLY
+ 950530 NSCAN/WARC: Correct handling of Mosaic positions
+ 950530 Update the LSQ test program twnm.for
+ 950516 NSCAN: fixed problem with wrong 0X total power.  - bug 122
+ 950516 Scan-file remembers whether REDUN was done with /DE_APPLY=OTH
+ 950516 NCLEAN: Add keyword DATA_FACTOR for DATA-clean option
+ 950503 TWNM: A new set of least squares routines, incorporating proper error 
+        handling and non-linear solutions are provided. 
+        Documentation is available in lsq.tex/lsq.ps
+ 950502 NCLEAN: DATA clean: HA_RANGE works once more
+ 950502 NCLEAN: Better error message in case outputfile readonly
+ 950502 NCLEAN: Data clean: clip_area back again
+ 950502 NSCAN: Correct AOTH correction if telescopes deleted
+ 950502 NMAP MAKE: correct binning if position of C,D is zero
+ 950502 NSCAN: Add option to read LEIDEN-tapes
+ 950502 Scissor: More client commands, add ionosphere stuff
+ 950502 Scissor: no messages about succesfull connection
+ 950502 NSCAN: Check if IF is present
+ 950303 NSCAN: DE_APPLY corrections set properly if telescope missing
+ 950224 Add test program TWNM for non-linear and complex LSQ testing
+ 950224 When elm NOT available, do  elm alias '/usr/ucb/mail'
+ 950224 Make sure that if still logged in after 7 days with
+        intermediate logins, you can re-init symbol file
+ 950221 NCALIB: Different limits for manual gain
+        NCALIB: Account for /DE_APPLY=OTH in different way when writing back corrections
+ 950220 NPLOT: correction for plotting mosaic IFDATA
+ 950220 NCALIB: larger range for gain corrections (SET MANUAL etc)
+        NCALIB: Do not create non-existing SCN files
+ 950220 NSCAN etc: Giving HA_RANGE=* is equivalent to default range
+ 950220 NSCAN PFITS: Option for shortlist of multiple labels
+ 950220 bug fix: allow for comment following '\' null reply
+ 950220 alert user if he tries to process .psc files
+ 950220 744 --> 644: data files are not executable
+ 950220 update of doc system
+ 950202 NCALIB: restore printing logic to situation before 940912(request by AGB)
+ 950202 NGEN: Add shift and model again
+ 950202 System: Use $HOME in directories i.s.o. tilde
+ 950202 NCALIB: default modelfile back again
+ 950202 Scissor: improved archiving procedures
+ 950202 NSCAN WARC: also pass calculated size of label to MEDIAD
+ 950202 NMAP: RFITS several small bugs fixed  - bug 134 
+ 950126 NSCAN (NFRA): Archiving options
+ 950126 changes in user interface accumulated over several months
+        the algorithms have not been touched
+        minor corrections to prompt/help formatting
+        format and help-text changes
+ 950123 ATNF: do not keep old executables (-NKeep switch)
+ 950123 Correct renaming of log-files etc
+ 950123 NMAP on Alpha: correct alignment
+        NMAP on Alpha: Correct RFITS
+ 950123 complete backtracking on ctrl-D, fix omissions in closing files
+ 950123 NPLOT: Correct HA_SCALE
+ 950123 Correct plotting of Y telescope errors  - bug 135 
+ 950123 Correct alignment errors in NMAP common
+ 950123 NSCAN DUMP: correct size of copied labels
+ 950112 correct scan number for model visibilities in HA-integration
+        this fixes a bug reported to JPH personally by AGB
+ 950112 system: test if we have to rebuild sys_bldppd.exe before 
+                processing psc/pin files
+ 950111 NSCAN: Option WARC updates Scissor
+        NSCAN: Put WSRT Gain corrections in DE_APPY OTHERS
+ 950111 NSCAN: Correction for WARC
+ 950111 NSCAN: Correct WARC for Mosaic observations
+ 950111 donot give an error message for wildcard disk input
+ 950111 NPLOT: Correct scale for pol.vectors
+ 950111 NPLOT: Fix bug with RA =~ 0.0 (No coordinates plotted)
+        NATNF: Select all interf. (Not asked anywhere)
+        System: Add scripts for ESTEC
+        Documentation: Newstar maintenance inside/outside NFRA as html-file
+ 950111 NSCAN DUMP: Pass correct size to Scissor
+ 950111 NMODEL: Option _CONVERT is CONVERT again
+ 950111 show prompt only on terminal or if environment var N_PSCTEST=1
+ 941121 NPLOT: Correct handling of # at WMP_LOOPS
+ 941121 NFLAG: Correct bug in psc-file, occurring at GET option
+ 941115 Documentation: include link to Scissor in homepage
+ 941115 new organisation of program-parameter documentation
+ 941115 adapt hypertext program-parameter help to new organisation
+        add sync mechanism to xmosaic restarting
+ 941115 NFRA: More Scissor commands
+ 941115 NFRA: Allow override of Owner for medium adminitstration
+ 941115 prompt-format control in .psc files, see psc_guide.txt
+ 941115 correct units for correction tables: deg --> rad
+ 941110 NMAP WFITS: Correct bug in CDELT3
+ 941110 NGIDS: Include FLFNODE
+ 941110 All: allow tape-directories on disk
+ 941110 NSCAN: update mediumadm. in Scissor for option DUMP
+ 941110 System: Interface to Scissor
+ 941031 NCALIB: Repair yet another bug in psc-file
+ 941031 PPD: Add missing pef-files in psc-files, typo's in for-files
+ 941027 New Newstar release: 5.1
+ 941027 NMAP FIDDLE: Open/close file when asking WMP_SET_2
+ 941019 NMAP FIDDLE EXTRACT: Correct fieldsize of extracted map
+ 941019 NPLOT: Correct default option after IFDATA choosen
+ 941019 NCOPY: add option to apply corrections to data being copied
+        (request of AGB; primitive implementation only)
+ 941019 NMAP: add FIELD_CENTRE for map-making
+ 940930 NGIDS: Correct plotting of maps with odd-axis length
+ 940930 NMAP: Corrections in RFITS (for FITS files not produced by NMAP)
+ 940930 NCALIB: Bug in COPY repaired
+ 940928 NFLAG: Can use CLIPDATA=2*RMS etc. again.
+               solved problem with write-protected files
+ 940928 NMAP: No longer overwrite tapes when aborted  - bug 125 
+ 940928 All: correct default model-file for broadband 92 cm observations
+ 940928 NCALIB: SET DX etc is now SET OTHERS DX
+        NCALIB: Option SET OTHERS MULTIPLY added
+ 940928 NPLOT: Prompts for scales accept * (=default)
+ 940908 NFLAG: bug in `dryrun' statistics fixed
+        New NFLAG option RT1 (CLIPDATA group)
+ 940901 NMODEL: Changed NMODEL UPDATE to include Polarisation
+        and Linear pol estimator (not written yet)
+ 940901 NGIDS: New flagging mode CLIPFLAG  - bug 115 
+ 940901 All: specifying SELECT_IFRS= -* also switches off autocorrelations
+ 940901 Files opened for writing/updating are now write-locked
+        to prevent multiple writes to the same file
+ 940901 System: changes in X11 interface  - bug 120 
+ 940901 NPLOT: Keep old user-input as default for next plot, 
+        option to abort a series of plots on X11.
+ 940901 No more confusing messages about DWARF symbols
+ 940901 User interface:
+          LOOPS before SETS like everywhere
+          Replace reporting of individual cuts by summaries per 100
+ 940901 ALL: Improve user interface and list output for LAYOUT/OVERVIEW
+ 940901 NMODEL: Correction for pol update
+ 940901 NPLOT: Ask tick-type also if no pixel coordinates asked
+ 940901 NPLOT: Correct bug in overlay of contour map and pol. vectors
+ 940901 NSCAN: Load datasets with 512 channels (or more)
+ 940901 NSCAN/NMAP: UNIT-* now really lists units
+ 940901 NFILT: Tested writing of IFR errors with Qubes
+        Still missing: secondary corrections
+ 940901 NMAP Write FITS: Correct bu causing core dump, correct scale for AP
+ 940901 NPLOT: More space between annotation and axis
+ 940821 NFILT: Add interferometer error writing to Qube options
+ 940821 NMAP: No error if #.. set-specification in FIDDLE
+ 940821 NSCAN LOAD: Use proper channel numbers for observations <1983
+ 940821 NPLOT MAP: Options to suppress annotation with pixel coordinates
+ 940821 NGCALC: Add BASE option to make plots as function of baseline
+        NGCALC CALC: Add CPOLY to make plot with data from fit
+ 940821 NCALIB REDUN: MODEL_OPTION no longer accepts INTERNAL  - bug 121 
+ 940821 NFLAG FLAG: DETERM option ELEVATION added  - bug 111 
+ 940812 NMAP FIDDLE COPY: Keep original comment in map header
+ 940812 All: NODE specification from list (** first, then #nn)
+        Giving * as tapeunit generates list of known ones
+ 940812 NCLEAN: No max. limit on memory size
+ 940803 NCLEAN: prompt for DMEMORY_SIZE with a default value
+        (not tested because this code is not normally executed)
+ 940803 NCLEAN: Bug 67 (Data Clean overwrites input map).  - bug 67 
+        This behaviour is intentional. An explanation
+        is given in the NCLEAN program description.
+ 940721 DEC/Alpha: get rid of <unaligned access> from qsort routine
+ 940721 NFRA: add tape-unit MAG0 (1600 bpi) and MAG1 (6250 bpi) for rzmws0
+ 940721 NGCALC: add DEL function  - bug 117
+ 940721 NPLOT: Add option ISYS to IFDATA to plot Tsys X+Y
+ 940721 NGCALC: Correct extract of IF-data
+        NGCALC: Correct bug in subtraction of poly-fit, show also 
+        for HA in hours
+ 940721 NFLAG: Add MANUAL option HARANGE with repeated prompt  - bug 118 
+ 940721 NMAP: Correct centre of extracted map (FIDDLE EXTRACT)  - bug 114 
+ 940721 NCALIB: bug in SET INIT corrected  - bug 116 
+ 940721 NFLAG: Improved statistics options
+ 940721 NMAP: Add option to read FITS-files  - bug 104 
+        Only tested on FITS-files written with Newstar
+ 940721 ndoc Hyper: respect user's Xmosaic window-size settings
+ 940721 NPLOT: Increase buffers for large DATA plots
+ 940623 NMAP: Correction in Job Summary
+ 940623 NMAP: Correct grouping in output map
+ 940623 WSRT batches: smaller plots
+ 940623 NGCALC: Correct data copy buffer pointer  - bug 113 
+ 940623 NMAP: Correct for crash during MOSCOM
+ 940623 NGIDS: Really set data to BLANK if BLANK_FLAGS=YES
+ 940623 NPLOT: Handle INTERNAL model correctly for RESIDUAL and MODEL - bug 99 
+        NPLOT: Correct default HA scale for X11  - bug 112 
+        NPLOT MAP: Option EDIT for PLOT_POSITIONS
+        NPLOT: Option INTERFEROMETER (corrections per ifr.)
+ 940613 nhyper: Mosaic 2.4 for DEC workstaton
+ 940613 NPLOT: different data-types on one page possible
+ 940613 NMAP: Add job summary log
+ 940613 NSCAN: Make available for old VAX R-series files
+ 940524 NMAP: Also symbol SD=Sin(Dec) defined
+ 940524 NFLAG: Define DWARF symbol RMS after dryrun, this allows
+        specifications like CLIP_LIMIT=5*rms
+ 940524 NCALIB SET INIT: Option to select interferometers  - bug 110 
+ 940524 NCOPY: Copy IF-data, option to strip Model, does not complain - bug 109
+        if data has less polarisations than expected
+ 940524 NPLOT: More sensible default for HA-range
+ 940524 NSCAN LOAD: Adapt for some weird tape-errors
+ 940524 NPLOT on X11: no more accidental "incorrect datatype" messages
+ 940524 NMAP: Make available for old VAX R-series files
+ 940524 NMAP: Extra spaces in output summary (for ABF scripts)
+ 940524 NSCAN: Small error with LOADIF on HP/WSRT solved
+ 940516 Prompts for NODE: ** option also matches lowercase files
+ 940516 NCALIB COPY/SHOW/CCOPY: Hidden keyword CAL_EQUAL to make all
+        input sectors of equal length (=weight)
+ 940516 nhyer: Mosaic 2.4 for Sun and Hp
+ 940516 NMAP FIDDLE MOSCOM: Max. number of input maps increased
+ 940516 NSCAN LIST: Print duration of measurement
+ 940516 NSCAN: Correct CATEG output for RUG/sw
+ 940509 NSCAN: LOADIF option to load Total Power data with uv-data
+        NSCAN SHOW: TP/GN option for SCAN_ACTION to show T.P./Tsys
+ 940509 NSCAN/NFLAG SHOW OVERVIEW: Correct bug in listing
+ 940509 Extensions are now accepted with nodenames (e.g. M31.SCN i.s.o. M31)
+        Warning if node needs to be converted with CVX
+        System: allow global DWARF symbols to be defined by Newstar programs
+        NMAP:  handle flaw of Sun tapeunits when winding up to end-of-file
+        NSCAN: properly handle End-of-File on some Sun tapeunits
+ 940509 NMAP: Declination stored in DWARF symbol PCDEC
+        This allows you to specify e.g. GRID_SIZE=4,4/SIN(PCDEC)
+ 940509 NPLOT: Add option IFDATA (keyword: OPTION) and 
+               keyword IF_MODE to plot Total Power data
+ 940509 NSCAN LOADIF: Various bugs corrected
+ 940509 NGCALC: Add option IFDATA (keyword: OPTION) and 
+                keyword IF_MODE to extract Total Power data
+ 940509 NPLOT: Option to label sources with proper names in map-plot
+ 940509 All: You can get a list of matching nodes by giving **
+        or name_of_directory/*
+ 940509 NMAP: Increase size of output map for MOSCOM
+ 940509 NGIDS: Increase buffer size for large MOSCOM maps
+ 940509 NCALIB SET: Options IFR and MIFR for interf. corrections  - bug 98 
+        NSCAN/NFLAG SHOW: SCAN_OPTION Ifr to list these corrections
+ 940509 NPLOT: Freq.bands back in plots with IFR_MODE=BAND
+ 940425 NSCAN UVFITS: Correct labeling of polarisations  - bug 88 
+ 940425 NCLEAN UVCOVER: No crash if Mapsize<FFTsize
+ 940425 NPLOT: Option to plot identification with sources in maps
+ 940425 All: proper correction for Faraday rotation once more  - bug 102 
+ 940425 NMAP: Bug removed from NVS and CVX 
+ 940418 NSCAN LOAD: Warning if Leiden tape, comments for old tape versions
+ 940418 NPLOT MODEL: default model file, INTERN handled correctly
+ 940418 NMODEL etc: Change in SHOW submenu, SHOW option in MODIFY
+ 940418 NMAP: Warning if input data with different pointing centra selected
+        NMAP: Do not create non-existing SCN files
+        NMAP: INTERN option works with MODEL_OPTION
+ 940418 System: DWARF startup more reliable, default dir. for models
+ 940418 NSCAN/NFLAG: Corrected bug in NSCSCM (in NSCSCR)
+ 940418 NSCAN/NFLAG SHOW: bug in T option corrected, phase shown unscaled
+ 940418 NGIDS DATA: Phases in range -180,180 (used to be 0,360)  - bug 77 
+ 940418 NGIDS: better text if INTERN option used  - bug 94 
+ 940411 DWARF: Unix environment variables (setenv) now recognised as symbols
+ 940411 NCALIB: Selection of telescopes possible for ZERO and COPY/CCOPY
+ 940411 NMAP: Show flux in areas with option SHOW CONT CONT D/N/O
+ 940411 NPLOT: Solved some little problems
+ 940411 NSCAN: Reading data period july 1978 - january 1984 possible - bug 73 
+ 940329 NMODEL/NCALIB: Solved HP bug at WSRT
+        NSCAN: Proper sequence number in LIST option
+ 940329 DWARF: ?? also works if you were reading something on a server
+ 940317 NFLAG: removed bug which caused an extra Scan
+        NFLAG: added option QXY (to CLIPDATA group)
+        NFLAG: added switch (use MODE) to disable 'dry-run'
+ 940317 NSCAN: Do not ask OVERVIEW question for Layout...
+ 940316 NGIDS: Correct handling of INTERN option for models  - bug 79 
+ 940316 NSCAN: Levels in Overview 
+ 940315 DWARF: proper handling of paths in restore and save
+ 940304 NMAP etc: Proper sign of V in model subtraction  -  bug 74 
+ 940303 NSCAN LIST: Proper date/time
+ 940303 NSCAN/NFLAG SHOW: Correct negative phases
+ 940301 NCALIB: Add space between HA and Pol. in output list
+ 940301 Models: Correct test for equality U,Q,V
+ 940301 NCALIB: "Flux-unknown" bit in model header determines default 
+        for SOLVE gain
+ 940301 NSCAN/NFLAG SHOW: Option to display corrected data  - bug 53
+ 940228 All: Propoer Faraday rotation, model for x+ etc dipoles
+ 940228 NCOPY: Bug causing segmentation violation removed
+ 940228 NMODEL: Changed MODEL_OPTION user interface,
+        default file for READ model is calibrator model
+ 940228 NCALIB: added (linear) differential shifts
+ 940228 NGEN: New keyword MODELB: search directory for models
+ 940224 NPLOT: Problems with mosaick observations solved
+ 940224 DWARF: Correct handling of quotes and slashes in qualifiers 
+        passed to dwe
+ 940224 NSCAN: New command LIST to list contents of WSRT tapes
+ 940223 NSCAN: Proper conversions for reading WSRT data on DECStations
+ 940223 DWARF: Streams work again
+ 940223 DWARF: DATAB feature switched off if DATAB set to "*" (including the
+        quotes, use dws ngen to set this)
+ 940221 NCOPY now copies all flags i.s.o. removing them
+ 940218 DWARF: Show version when program is started
+ 940218 NGIDS: Option to blank flagged datapoints
+ 940218 NCALIB: Changed format of log-line (tag for Reduce scripts)
+ 940218 NSCAN Remote tapes: tell server who is calling
+ 940216 NGEN: Add keyword MEMORY 
+ 940215 NMAP: Default HA-range -90,90 for WSRT  - bug 4
+        NMAP: Allow specification of Grid size (give "" at FIELD_SIZE) - bug 5 
+        NCALIB: SOLVE and COMPLEX always asked  - bug 60 
+        NSCAN/NFLAG Show: Give category/type in printout
+ 940214 NCOPY: remove relics of simulation
+ 940208 NSCAN: Remote tape-units
+ 940203 NGIDS: New keyword ALL_POLS, no empty flag files, 
+               Name of input Node and Sets in (ASCII) flag files.
+ 940203 NMAP: Suppress unnecessary creation of new groups when looping
+ 940203 Fitting NPLOT to the needs of the reduction group  - bug 59
+        which means: Plot AP or CS on one page (= 'old' PLOTAP)
+                     More plots on one page
+        NPLOT: add BANDPASS option to make (ifr, ch) plots - bug 26
+ 940202 DWARF/System: Changes for DEC Alpha/OSF1 and general cleanup  - bug 57 
+ 940126 NGIDS: Increase effective size of buffer
+ 940120 NFLAG: Extended IHAMIN,IHAMAX to 180 degr
+ 940120 DWARF: open ppd-file readonly
+ 940117 NGIDS: Correct bug in data-range/model subtraction, better min/max
+ 940117 NSCAN/NFLAG: Better printing of FREQ in Sector header (no 0.xxxE04)
+ 931223 NPLOT: Keyword SCN_LOOPS included
+ 931221 NGIDS: Correct some SUN specific Fortran and typos
+ 931221 NGIDS: Correct zoom and HA step, some more on-line help
+ 931220 NSCAN, NMAP, NGCALC: New EDIT format, new OVERVIEW option for SHOW.
+        Answer L or O to any ???_SETS/LOOPS prompt to get the Layout or an
+        overview of the corresponding file.
+ 931217 NSCAN: report which interferometer in case of Format error
+ 931217 NGIDS: Read SCN files directly and flag them with gids regions - bug 65 
+ 931216 General: old logfiles (>5 days) no longer purged
+ 931216 NFLAG: Fully reworked new version
+ 931216 All: Make LOOPS more specific (SCN_LOOPS etc)  - bug 3 
+ 931215 All: Read special (ACORM=0) tapes
+ 931215 NCALIB: cater for possible phase ambiguities in complex gain averaging
+ 931215 NCALIB: Make Complex solution (only a possibility) and some small
+                text changes
+ 931215 New (931117) version of giplib and gids for cv
+ 931215 NMODEL: Add REDIT, FEDIT model action
+ 931206 NGEN: New dummy program NGEN for use in batch scripts
+ 931206 NMAP: Changed text  - bug 42 
+ 931202 System: Problem solved with character entry (for HP-UX 09.01)
+ 931202 NPLOT/X11: Plot crosses in maps (again)  - bug 40 
+ 931130 NGIDS allows SLICE
+ 931130 NSCAN: correct default label for output disk files
+ 931130 NSCAN: report old and new indices for each new index being made
+ 931124 NSCAN/NFLAG: W option shows all weights including values of 0
+ 931123 Error with structures in WNTINC. Recompile some DSC  - bug 63
+ 931123 WNTINC: Proper _T for multiple sub-structures
+ 931123 NMAP Show: Layout extended (and some minor changes)
+ 931123 NPLOT: starts with white display
+ 931117 NCLEAN: Better userinteraction for AREA=, INST corrected in Beam Clean
+ 931117 System: xmosaic 2.0 and various minor improvements
+ 931116 DWARF: can now use . as well as $ for stream, dwv: new option /SHORT
+ 931116 NSCAN/NFLAG SHOW: Sector action does not stop in batch  - bug 61 
+ 931112 All: bug fix to clock correction
+ 931111 Fire off X11 window right at the beginning and keep it.  - bug 27 
+ 931110 NCALIB: baseline-pole correction fixed
+ 931105 NSCAN/NFLAG: Changed default for SECTOR_ACTION to NEXT
+ 931102 Models: Default option for MODEL_ACTION is now NOBEAM!!!!
+ 931008 Models: Automatic correction for beam shape at different frequencies,
+		positions, instruments has been included in all model
+		handling and calculations.
+		NMODEL EDIT option has been added to be able to change the
+		model header without conversion (part of the old CONVERT),
+		NMODEL CONVERT will convert everything
+		In model data calculations the automatic beaming can be
+		suppressed by the MODEL_ACTION NOBEAM. Note that if you
+		specify BEAM with an existing (old) calculated model, the
+		complete model will be recalculated.
+ 930924 NGCALC: Bug with 1D plots fixed
+ 930922 NSCAN: Option SHOW is back in NSCAN (but it also remains in NFLAG)
+ 930913 NSCAN: Correction of UVFITS output for incomplete data
+ 930826 NFLAG: New options TOPOL, STAT, ... New sequence in OPERATION_...
+               (now goes back to FLAG_MODE, OPERATION_0).
+               Bug in interferometer coding for ASCII files corrected.
+ 930825 NPLOT: Bug in PS output corrected. Also, printing to A3 should 
+               now switch back to A4 properly
+ 930806 NFLAG: Option ARESID for flaggin on Selfcal/Align residuals
+        NFLAG: Option PUT repaired 
+ 930802 NSCAN: NVS handles IQUV to XYX conversion properly for more than
+               one channel, proper weight check.
+ 930722 NPLOT: Changed keyword PLUVO in IFR_MODE(normal,spectral,sort)
+             normal: plot ifr vs ha, ifr order (00,01,...,dd)
+             spectral: spectral channel vs ha, per ifr (old PLUVO)
+             sort: ifr vs ha, baseline sort
+ 930706 NPLOT: RULE plots will now be plotted horizontal (C10)
+ 930701	New version of NGCALC with more expression functions and SHIFT
+	Calculate option. The new features can only be used for freshly
+	extracted data; there is no possibility to add the necessary
+	data to the existing NGF files by, e.g. NVS option. Old data
+	can still be used for all other options.
+ 930628	New NPLOT (NGCALC) X11 driver. You can now select the plotsize as
+	fraction of screen (default 0.75; value > 0.0, <= 1.0) by:
+		setenv PGPLOT_XW_WIDTH value
+	and get all plots without waiting (and without seeing end result) by:
+		setenv PGPLOT_XW_CLICKLEFT 0
+ 930622	New NFLAG SHOW SCAN T option to guess calibrator phases selfcal start
+ 930622	Add some flagging possibilities to NGIDS for UV data
+ 930619	A new program: NFLAG contains now the SHOW and FLAG(DELETE) options
+	originally in NSCAN
+ 930616	New option added to set a field shift in SCN (in NCALIB), and to
+	"de-"apply it if wanted (all programs)
+ 930610	Flagging in NSCAN has been redefined, and options added. Read ? text
+	for details
+ 930608	The data format has been changed to cater for multiple flagging layers
+	and absolute (rather than relative) weights per data point.
+	SCN files made before this date will give a message:
+	"run NSCAN/NMAP NVS first". Run NSCAN NVS to convert the data to the
+	new format.
+	"DELETE" is now called "FLAGGING", and a new NGEN keyword UFLAG has
+	been introduced to be able to selectively include flagged data in
+	your processing. Like other NGEN keywords (e.g. APPLY) it can be
+	set as a switch on dwe; a dws NGEN or dws "program" or by
+	dwe "program"/ASK.
+	NSCAN SHOW has been extended to show the flags set for the DATA W
+	option, and a SET_ACTION FLAGS has been added to give an overview
+	of flags per cube slice.
+ 930606	Added ionospheric refraction, baseline pole, d(x,y,x), clock and
+	frequency correction.
+	Limited edges of mosaic output to suppress noisy data
+ 930524 Many keywords now have a more meaningfull name.
+ 930519 Read/Write to DAT-devices on HP now possible
+ 930513 NCALIB/NGCALC: New method for complex Least Squares
+        NPLOT:  Solved problem when plotting with one (positive or negative) 
+                contour causes crashes. (A42)
+        Problem with keyword DELETE_NODE solved (came in a loop). (A47)
+        NGIDS:  Reorganised the program for future (interactive deleting)
+        NMODEL: New option: FIND to find sources in map
+ 930503 NMODEL: Problem with core-dump when type-error solved (A40)
+                Model update was wrong for fields with negative declination.
+        NSCAN:  Problem with flagging of two polarisations corrected (A41)
+        NSCAN/NCALIB: Message will be printed when the program creates a new
+                SCN-file. Happens when name of non existing-file typed in (A43)
+        NCLEAN: Problems solved with noise values in the latest restore-step of
+                data-clean (came from original iso. residual map). (A44)
+        NGIDS:  now totally independent from GIPSY (A49)
+        NATNF:  Phase problem solved (A50)
+ 930304 NMAP:   Writing cubes contiguous
+ 930210 NPLOT:  Default contours now available.
+                Default PLOTTER will now be PSP, default SIZE will be 1.3, 1.3
+ 920205 The problems on the HP with default value 0 have been solved.
+        Also some printout on the screen will fit on one line.
+ 921222 NPLOT:  Display option X11 now partly available for UNIX machines
+                (Do NOT use halftone; some options will NOT work correct yet)
+ 921218 Changed KEYWORD=LOG. All programs have now default YES iso. SPOOL
+ 921106 Programs changed for J2000 and allow HA outside -90 - +90 degrees.
+ 921022 NATNF, NSCAN and NMAP are now able to use mag-tapes on UNIX system.
+        Do a setenv to see which mag-tapes are available.
+        NPLOT and NGCALC can now plot on A3-plotter (B17).
+ 920903 Many problems solved by WNB during his stay in Dwingeloo
+        NGCALC: New program for data calculation and plotting (C2)
+        NATNF:  New program to handle RPFITS files
+        NSCAN:  Split mosaic data (B1)
+                Error in old WSRT-tapes (1987) .. pointing set (A33)
+                Wrong MJD when not correct ended WSRT observation (A34)
+                Faster mosaic splitsing (2 times faster) (A35)
+                Conversion LINOBS (I,Q,U,V) to XX,XY,YX,YY (B14)
+        NMAP:   UV circular weighting function (B5)
+                A option/loop (in FIDDLE/ADD) for line-data (B6)
+                MOSCOM option to use noise as weight (B11)
+                Extended NMAP fits header (B12)
+                Change coordinates if shift (A23)
+                Noise for extract/copy in NMAP (A28)
+                Precission angle calculation (A30)
+                Calculate offsets in map (A32)
+                Logics MAP statistics (A36)
+        NMODEL: Delete of non-clean components (B3)
+                Delete of sources inside dl,dm box (B13)
+                Merge source models: sometimes recalculate everything (A31)
+                RSHOW problem solved (A22)
+        NPLOT:  Option to plot hourangle against frequency for a baseline 
+                polarisation (C7)
+                Halftone plotting problem solved (A19)
+                Plot message by selfcal/align residuals with model (A24)
+                On SUN: Problem plots bigger than A4 solved (A26)
+        NCLEAN: Changed sign restore beam angle (A20)
+ 920728 NGIDS:  New program to load maps into GIDS
+                (GIDS = Groningen Image Display System)
+ 920714 NSCAN updated for Online System nr. 63 (Change in extended FD)
+ 920626 New delete option DCLOW, same as DNCLOW, but for cleaning components
+        NMAP:   Problem with Beam-option correctred (B4)
+                Problem with fsum corrected (A18)
+                Problem with model subtraction for polarisation sources 
+                with RM corrected (A16)
+ 920623 Name of software-pakket changed from N-series into NEWSTAR
+        (Netherlands East West Synthesis Telescope Array Reduction-package)
+ 920609 NSCAN:  Problem with flagging of two polarisations corrected (A12)
+                Layout for MJD(start) corrected (A14)
+        NMAP:   Problem with source subtraction corrected (A15)
+                Problem with "LAYOUT" option for WMP-file corrected (A13)
+ 920504 NMAP:   Problem with data in HA-baseline format corrected.
+        NSCAN:  Problem with delete options (Rnoise Anoise) corrected (A11)
+ 920407 Problem with option CVX to DEC-workstation corrected.
+        NPLOT:  Use of double loops for plotting a MAP corrected (A5)
+                Plotting more than one 'data', 'residuals' or 
+                'telescope corrections' problem corrected.
+        NMODEL: Symmetirc extended sources problem corrected (A6)
+        NCLEAN: Epoche problem corrected (A9)
+        NMAP:   Writing REAL or AMP data from .WMP file to grey-scale
+                problem corrected.
+ 920131 NCLEAN with an unsaved residual map corrected
+ 920131 NCLEAN major cycle statistics printout corrected
+ 920130 NPLOT re-write to use full page in portrait mode
+ 920129 NPLOT output to EPS and EPP can be viewed on the DECstation (if files
+        produced there or ftp'ed) with the command: dxpsview &
+        or with the PostScript preview application
+        These files can also be incorporated in WordMarc (and other) documents
+ 920128 Spool error PS plots
+ 920128 Change prompt error in NMAP FIDDLE
+ 920119 NMODEL UPDATE corrected for use of B1950 models
+ 920119 NCALIB SELFCAL corrected for use of B1950 models
+ 920117 NCLEN COMPON option
+ 920117 NCLEAN restoring for extended sources
+ 920117 NCLEAN restoring for non-clean point sources
+ 920116 NCLEAN URESTore option for clean components
+ 920116 NPLOT large plots now ok
+ 920115 NCLEAN UVCOVER with restore option
+ 920109 NSCAN UVFITS memory related crashes for large jobs solved
+ 920109 NMODEL option to delete low-level non-clean changed in definition
+ 920108 NCLEAN Clark type clean (UVCOVER) please test and comments
+ 911230 NMODEL UPDATE corrected for logical error for clean components
+ 911230 NMODEL new option DNCLOW to delete low-level non-clean components
+ 911230 NPLOT better RA, DEC coordinates
+ 911227 NPLOT renewed with ruled surface and polarisation vector possibilities
+ 911227 Correct conversion to/from other coordinates in NMODEL
+ 911219 A new set of Plot routines incorporated in NPLOT (maybe problems)
+ 911209 Correct interferometer selection POL NCALIB
+ 911115 All (de-)beams have a maximum limit of a factor 100   
+ 911105 MAPs made before today at 10:00 will not properly combine in MOSCOM
+ 911105 NMAP FIDDLE MOSCOM will combine mosaic fields properly weighted
+ 911104 Correct de-selection of clean components (X)UPDATE in NMODEL
+ 911031 WERR option NSCAN will correct mosaic HA tape error
+ 911025 All HA's on WSRT tape for mosaic wrong
+ 911024 NMAP reference coordinate (mosaic) option checked
+ 911023 NPLOT RES definition changed for Ampl and Phase
+ 911014 NSCAN DELETE new CLIP option
+ 911009 NCALIB: SET RENORM option added
+ 911009 NMAP: correct multiple polarisations output
+ 911008 Default: No complex for NCALIB pure redundancy
+ 911007 Instrumental polarisation in first version
+ 911004 NCALIB POLAR VZERO options CALC APPLY MANUAL ASK in first version
+ 911003 The ncopy command will transfer and convert files from VAX
+ 910930 NPLOT: repair logics
+ 910930 NCALIB POLAR COPY has loops
+ 910930 NCALIB REDUN check on extreme values
+ 910927 Multiple input sets ok in NMAP; NPLOT option order reversed
+ 910923 Add SET,COPY,EDIT option to POLAR option in NCALIB
+ 910923 Correct sign of shift in NMAP
+ 910918 Add option to NPLOT to only plot XY,YX
+ 910918 quota directory|filename ... gives size (may have wildcards) (Alliant)
+ 910917 Correct bug in all programs that mistreated APPLY and DE_APPLY
+ 910917 Status of options as described in ITR198a
+        Can be printed (on VAX) by: $ wm/print user5:[wnb.itr]itr2a.wnb
+ 910917 The following programs exist:
+        NSCAN, NMODEL, NCALIB, NMAP, NCLEAN, NPLOT (+NGEN for parameters only)
diff --git a/nplot/nplot__angle_wmp_set.html b/nplot/nplot__angle_wmp_set.html
new file mode 100644
index 0000000000000000000000000000000000000000..40b32595ddbb7c4c05c03ceea2a23d1849667a37
--- /dev/null
+++ b/nplot/nplot__angle_wmp_set.html
@@ -0,0 +1,17 @@
+<TITLE>Description of ANGLE_WMP_SET (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword ANGLE_WMP_SET</H1> 
+
+<DT><EM>Prompt:</EM> ONE position-angle map: grp.fld.chn.pol.0.seq
+<DT><EM>Expected input:</EM> Character(32), 1 values.<P>
+Select a .WMP-file image holding polarisation position angles. If the image you 
+specify contains anything else, your plot will be garbage. <P>
+The .WMP-file indices are: <P>
+        group.field.channel.polarisation.type(=0).sequence_number <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI>Description of the <A HREF="../wmp_descr/wmp_descr.html">WMP file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__annotation.html b/nplot/nplot__annotation.html
new file mode 100644
index 0000000000000000000000000000000000000000..e158cc263cca1aa2c1279ed515d1f130082f291c
--- /dev/null
+++ b/nplot/nplot__annotation.html
@@ -0,0 +1,13 @@
+<TITLE>Description of ANNOTATION (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword ANNOTATION</H1> 
+
+<DT><EM>Prompt:</EM> Annotation text, up to 80 characters in double quotes
+<DT><EM>Expected input:</EM> Character(80).<P>
+This text will be displayed on all plots for this NPLOT run until you change it 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__area.html b/nplot/nplot__area.html
new file mode 100644
index 0000000000000000000000000000000000000000..81771bebd9f07182277b5f85abffdd995bdfc92b
--- /dev/null
+++ b/nplot/nplot__area.html
@@ -0,0 +1,17 @@
+<TITLE>Description of AREA (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword AREA</H1> 
+
+<DT><EM>Prompt:</EM> Area centre (l, m) and width (dl, dm) in grid units
+<DT><EM>Expected input:</EM> Integer number, 4 values.<P>
+Specify an area of a map: <P>
+        l, m     grid coordinates of area centre: 0, 0 is the map centre,  
+                 increasing to the upper right (i.e. with DEcreasing 
+                 right ascension and INcreasing declination) <P>
+        dl, dm   area width and height  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__coord.html b/nplot/nplot__coord.html
new file mode 100644
index 0000000000000000000000000000000000000000..36843de22b0e2278d9f1209d62dd11e1baca730a
--- /dev/null
+++ b/nplot/nplot__coord.html
@@ -0,0 +1,33 @@
+<TITLE>Description of COORD (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword COORD</H1> 
+
+<DT><EM>Prompt:</EM> | NONE;  LM,  DEGREE, RADEC;  DLM,  DDEGREE, DRADEC;|-ONONE; OLM, ODEGREE, ORADEC; ODLM, ODDEGREE, ODRADEC Axis annotation style
+<DT><EM>Default:</EM> NONE /ASK.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Select ONE style of axis annotations: <P>
+        NONE     no annotation (only pixel coordinates) <P>
+   Relative quasi-Cartesian coordinates: <P>
+        LM       l, m in arcsec with respect to map centre 
+                  (or annotation for UV-plane plots) 
+        DLM      l, m in arcsec with respect to centre of plot 
+                  (or annotation for UV-plane plots) <P>
+   Equatorial coordinates: <P>
+        DEGREE   right ascension and declination in decimal degrees 
+        RADEC    right ascension (hhmmss) and declination (ddmmss) 
+        DDEGREE  relative right ascension and declination in decimal degrees 
+                  w.r.t.  centre of plot 
+        DRADEC   relative right ascension (hhmmss) and declination (ddmmss) 
+                  w.r.t. centre of plot <P>
+These annotations will be printed along the left and bottom sides of the plot. <P>
+By default, (l, m) pixel-coordinates are shown along the top and right axes side 
+irrespective of what you select. You may suppress these, by prefixing any of 
+the above options with an O for 'Only'. <P>
+Example: 
+        ONONE will suppress all annotations.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__coord_prec.html b/nplot/nplot__coord_prec.html
new file mode 100644
index 0000000000000000000000000000000000000000..67e546a39e418d09421fb9f22d68c5d8a688d873
--- /dev/null
+++ b/nplot/nplot__coord_prec.html
@@ -0,0 +1,15 @@
+<TITLE>Description of COORD_PREC (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword COORD_PREC</H1> 
+
+<DT><EM>Prompt:</EM> Number of steps for coordinate contouring near pole
+<DT><EM>Default:</EM> 256 /NOASK.
+<DT><EM>Expected input:</EM> Integer number; min.value: 8.000000; max.value: 32768.000000.<P>
+Specify the number of steps across the map to use in defining the 
+coordinate grid for contouring of coordinates near the pole. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__coord_type.html b/nplot/nplot__coord_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..fe2bf6ebe7efda2cf24381aec8b72de853115f7a
--- /dev/null
+++ b/nplot/nplot__coord_type.html
@@ -0,0 +1,17 @@
+<TITLE>Description of COORD_TYPE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword COORD_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> TICK, DOTTED, FULL Coordinate grid style
+<DT><EM>Default:</EM> TICK /ASK.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Select the style for plotting coordinate grid lines: <P>
+   TICK          give along plot edges only 
+   DOTTED        dotted grid 
+   FULL          full-drawn grid  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__data_type.html b/nplot/nplot__data_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..7c143e0171f0c4a1b8e601c4dc6863360dda1df1
--- /dev/null
+++ b/nplot/nplot__data_type.html
@@ -0,0 +1,18 @@
+<TITLE>Description of DATA_TYPE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword DATA_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> DATA; SLOPE data types to plot
+<DT><EM>Default:</EM> DATA /ASK.
+<DT><EM>Expected input:</EM> Character(16).<P>
+Specify the data type(s) to be plotted. <P>
+   DATA or *    plot the data as given in the map 
+   SLOPE        plot the horizontal slope of the data (This option is still 
+                 experimental!) 
+!!                      purpose? 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__data_types.html b/nplot/nplot__data_types.html
new file mode 100644
index 0000000000000000000000000000000000000000..4ae038765b73912bbdc556f252b32bab32d5b449
--- /dev/null
+++ b/nplot/nplot__data_types.html
@@ -0,0 +1,31 @@
+<TITLE>Description of DATA_TYPES (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword DATA_TYPES</H1> 
+
+<DT><EM>Prompt:</EM> Visibility component to plot AMPLITUDE, PHASE; AGAIN, PGAIN; COSINE, SINE;  AP, CS
+<DT><EM>Default:</EM> AMPLITUDE.
+<DT><EM>Expected input:</EM> Character(16), 6 values.<P>
+Specify the visibility component to be plotted. <P>
+        The quantity plotted depends on the data selected.  For TEL or INTERF 
+and for redund. RES       :       gain-1(%), phase(deg) For DATA: 
+                  ampl (WU), phase(deg For Selfcal RES with external model: <P>
+. 
+   Standard representations of complex data: <P>
+                        Model           Resid           Int.model 
+        AMPLITUDE 
+        PHASE 
+        COSINE 
+        SINE <P>
+   Instrumental gain/phase for DATA_TYPE=RES: 
+        AGAIN   Re log(data/model) * 100 = gain in % 
+        PGAIN   Im log(data/model) * 180/pi = phase in deg <P>
+   Old WSRT 'PLOTAP' formats: <P>
+        AP         amplitude/phase plots, one pair per page 
+        CS         cosine/sine plots, one pair per page <P>
+ 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__dot_cont.html b/nplot/nplot__dot_cont.html
new file mode 100644
index 0000000000000000000000000000000000000000..6fc4c8d6bbc412df93d82cbd665734a2da279292
--- /dev/null
+++ b/nplot/nplot__dot_cont.html
@@ -0,0 +1,13 @@
+<TITLE>Description of DOT_CONT (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword DOT_CONT</H1> 
+
+<DT><EM>Prompt:</EM> Dotted-contour levels
+<DT><EM>Expected input:</EM> Real number, 32 values.<P>
+Specify up to 32 values of the contours to be drawn as dotted lines.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__full_cont.html b/nplot/nplot__full_cont.html
new file mode 100644
index 0000000000000000000000000000000000000000..774a78487a735ebb4a179046eb666acd28ada315
--- /dev/null
+++ b/nplot/nplot__full_cont.html
@@ -0,0 +1,13 @@
+<TITLE>Description of FULL_CONT (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword FULL_CONT</H1> 
+
+<DT><EM>Prompt:</EM> Full-contour levels
+<DT><EM>Expected input:</EM> Real number, 32 values.<P>
+Specify up to 32 values of the contours to be drawn as full lines.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__ha_integration.html b/nplot/nplot__ha_integration.html
new file mode 100644
index 0000000000000000000000000000000000000000..31fceeb2170322c2b2d23d74465ac0eafe10eb9d
--- /dev/null
+++ b/nplot/nplot__ha_integration.html
@@ -0,0 +1,17 @@
+<TITLE>Description of HA_INTEGRATION (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword HA_INTEGRATION</H1> 
+
+<DT><EM>Prompt:</EM> Integration time (sec)
+<DT><EM>Expected input:</EM> Real number; max.value: 3600.000000.<P>
+Specify the time interval over which you want to integrate (if possible) before 
+calibrating. The value you specify will be rounded down to a multiple of the 
+hour-angle interval between successive scans. <P>
+'*' and '0' mean do not integrate, i.e. calibrate per scan. <P>
+The largest value allowed is 3600 (= 1 hour).  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__ha_mode.html b/nplot/nplot__ha_mode.html
new file mode 100644
index 0000000000000000000000000000000000000000..3a33320b16419b2b7da3aa2c722c3bf120263a94
--- /dev/null
+++ b/nplot/nplot__ha_mode.html
@@ -0,0 +1,34 @@
+<TITLE>Description of HA_MODE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword HA_MODE</H1> 
+
+<DT><EM>Prompt:</EM> Special HA plot coordinates ST, IST, SEQUENCE, ISEQUENCE
+<DT><EM>Expected input:</EM> Character(10).<P>
+This parameter selects a coordinate conversion for the vertical (HA) plot 
+coordinate in plots of .SCN-file entities. <P>
+    ST          Sidereal time i.s.o. HA. This is useful for plotting a series of 
+                 observations (e.g. calibrators-object-calibrators) in a time 
+                 sequence, e.g. to survey interference. Vertical coordinate is 
+                 ST in degrees <P>
+    SEQUENCE    Pseudo sidereal time: Sidereal time is forced into an ascending 
+                 sequence: When the start ST for a sector is less than that of 
+                 the one just plotted, it is changed to make the new sector 
+                 follow the previous one contiguously. Within each sector,  
+                 vertical scale size is that of HA or ST, but the sectors are 
+                 displaced in ST. Sectors are plotted in order of their index. 
+                This mode is useful to stuff a lot of information into a single 
+                 plot, e.g. to check for interference, but the plot may become 
+                 too confusing. <P>
+    I&lt;xxx&gt;      The prefix I indicates that you want to integrate scans; you 
+                 will be prompted for the HA interval over which to integrate. 
+                 As currently implemented, this mode is effective only for plots 
+                 that have HA or (pseudo)ST as vertical coordinate. The plot 
+                 scale for this coordinate will not be affected. <P>
+NPLOT will set plotting mode according to your reply and return to the OPTION 
+prompt. The mode will remain in force until you change it or NPLOT exits.    <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__ha_scale.html b/nplot/nplot__ha_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..13773806fa51d1369fcc1b2eef1a52fa5b3894a0
--- /dev/null
+++ b/nplot/nplot__ha_scale.html
@@ -0,0 +1,14 @@
+<TITLE>Description of HA_SCALE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword HA_SCALE</H1> 
+
+<DT><EM>Prompt:</EM> HA plot scale (degree/cm)
+<DT><EM>Default:</EM> 1..
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the hour-angle scale in degree/cm. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__halftone.html b/nplot/nplot__halftone.html
new file mode 100644
index 0000000000000000000000000000000000000000..f071f9256b0aaa8e2af2ddb81bd0c3cba7330f80
--- /dev/null
+++ b/nplot/nplot__halftone.html
@@ -0,0 +1,36 @@
+<TITLE>Description of HALFTONE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword HALFTONE</H1> 
+
+<DT><EM>Prompt:</EM> NONE, CONTINUE; STEP, PATTERN Halftone transfer function
+<DT><EM>Default:</EM> NONE /ASK.
+<DT><EM>Expected input:</EM> Character(24).<P>
+At this point, data values have been normalised to lie within the interval 
+[0, 1]. Halftones are represented by the same interval: 0=white, 1=black. You 
+are now to define the transfer function F for mapping data values onto 
+halftones: <P>
+        halftone = F (normalised data value) <P>
+   Continuous functions: <P>
+        CONTINUE  a quadratic function (you will be prompted for the 
+                   coefficients) 
+        NONE      direct mapping: halftone level = normalised data value <P>
+   Discontinuous functions: <P>
+        STEP      F is a staircase function; halftone shades are generated by a 
+                   stochastic algorithm 
+        PATTERN   as STEP, but halftone shades are represented by a set of 
+                   fixed patterns <P>
+In selecting a method, bear in mind that the human eye is quite sensitive to 
+density variations in light shades while very poorly perceiving the same 
+variations in the dark shades; in other words, its response to density 
+variations is quasi-logarithmic. <P>
+To compensate for this, a quasi-exponential transfer function is suitable. The 
+best approximation to this available here is a steeply quadratic function (i.e. 
+specify CONTINUE here and consult the on-line help for the TRANSFORM parameter). <P>
+You may judge the quality of your transfer function from the grey-scale wedge 
+that will appear side by side with your plot.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__if_mode.html b/nplot/nplot__if_mode.html
new file mode 100644
index 0000000000000000000000000000000000000000..89215ff23dab929094cce9f0084240e1d61b6047
--- /dev/null
+++ b/nplot/nplot__if_mode.html
@@ -0,0 +1,24 @@
+<TITLE>Description of IF_MODE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword IF_MODE</H1> 
+
+<DT><EM>Prompt:</EM> Parameter to plot TPON, TPOFF, TSYS, ISYS, GAIN;  GNCAL, TSYSI, TNOISI, RGAINI
+<DT><EM>Expected input:</EM> Character(8).<P>
+Specify action to perform: <P>
+   Telescope parameters: <P>
+        TPON          total power data (noise source off) 
+        TPOFF         total power data (noise source on) 
+        TSYS          system temperatures 
+        ISYS          system temperatures (X+Y) 
+        GAIN          IF gains <P>
+   Interferometer parameters: <P>
+        GNCAL         gain correction method 
+        TSYSI         constant system temperature 
+        TNOISI        constant noise source temperature 
+        RGAINI        constant receiver gain <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__ifr_mode.html b/nplot/nplot__ifr_mode.html
new file mode 100644
index 0000000000000000000000000000000000000000..bfc3cc874e08daa0b2d80df9f6cd348f4cb27768
--- /dev/null
+++ b/nplot/nplot__ifr_mode.html
@@ -0,0 +1,33 @@
+<TITLE>Description of IFR_MODE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword IFR_MODE</H1> 
+
+<DT><EM>Prompt:</EM> NORMAL, INVERT, SORT;  SPECTRAL, BAND Select data cross-section
+<DT><EM>Expected input:</EM> Character(16).<P>
+Specify the cross section through the visibility data cube to be plotted: 
+        Consider the interferometers arranged in an upper-triangular matrix: <P>
+                00 01 02 ... 0B 0C 0D 
+                   11 12 ... 1B 1C 1D 
+                      22 ... 2B 2C 2D 
+                             :  :  : 
+                             BB BC BD 
+                                CC CD 
+                                   DD <P>
+Then the possible plotting modes are <P>
+    visibilities as function of hour angle per interferometer: <P>
+        NORMAL  interferometer order in the matrix is row by row <P>
+        INVERT  interferometer order in the matrix is column by column  . 
+        SORT    interferometers in order of ascending baseline <P>
+    other cross sections of the hour-angle/interferometer/channel cube: <P>
+        SPECTRAL visibilities as function of spectral channel and hour angle,  
+                  per interferometer (the WSRT 'PLUVO' format) 
+!!                      i.e. one plot per ifr? <P>
+        BAND    visibilities as function of channel and interferometer,  
+                 interferometer order as for NORMAL 
+!!                      for one HA or averaged? 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__option.html b/nplot/nplot__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..d557c0b458cd0bffafc5a3c5c6b567c447c77729
--- /dev/null
+++ b/nplot/nplot__option.html
@@ -0,0 +1,32 @@
+<TITLE>Description of OPTION (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Type of data to plot|  MAP; DATA, RESID, MODEL; TELESC, INTERFM, IFDATA;|SPECIAL; QUIT
+<DT><EM>Default:</EM> QUIT.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify type of data to plot: <P>
+   .WMP-file data: <P>
+        MAP              image(s) from .WMP file <P>
+   .SCN-file visibilities: 
+        DATA             observed visibilities 
+        MODEL            model visibilities 
+        RESIDUAL         visibility residuals (after correction of all known 
+                          errors and division by the visibilities of a source 
+                          model (yet to be specified) 
+                                (sets I=1, QUV=0) <P>
+   .SCN-file correction parameters: <P>
+        TELESCOPE        telescope phase/gain corrections 
+        INTERFEROMETER   interferometer phase/gain corrections (i.e. all 
+                          corrections combined per interferometer) 
+! I rechecked this 960523 - JPH 
+        IFDATA           IF-data: total powers, system temperatures etc. <P>
+   Plotting versus sidereal time i.s.o. hour angle: <P>
+        SPECIAL          will prompt for a special mode <P>
+        QUIT             terminate NPLOT  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__plot_heading.html b/nplot/nplot__plot_heading.html
new file mode 100644
index 0000000000000000000000000000000000000000..d230538a9a4acc3594ea301859613a1ad826c488
--- /dev/null
+++ b/nplot/nplot__plot_heading.html
@@ -0,0 +1,14 @@
+<TITLE>Description of PLOT_HEADING (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword PLOT_HEADING</H1> 
+
+<DT><EM>Prompt:</EM> YES, NO Plot heading (Yes/No) ?
+<DT><EM>Default:</EM> YES /NOASK.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify if you want to have a MAP plot with or without the heading. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__plot_positions.html b/nplot/nplot__plot_positions.html
new file mode 100644
index 0000000000000000000000000000000000000000..dbe97730da285612b87fb45a6cad5d886f0f9013
--- /dev/null
+++ b/nplot/nplot__plot_positions.html
@@ -0,0 +1,26 @@
+<TITLE>Description of PLOT_POSITIONS (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword PLOT_POSITIONS</H1> 
+
+<DT><EM>Prompt:</EM> NO, YES, NAMES; EDIT Mark source positions
+<DT><EM>Default:</EM> NO /ASK.
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify if you want model-source positions marked in your plot. The answers may 
+be: <P>
+        NO 
+        YES     position markers only 
+        MAMES   position markers annotated with their IDs from the model list <P>
+The marker symbol used is determined per source by its Type (which is the 
+suffix number in its ID). <P>
+        EDIT    invoke model-handling code to modify model-components' Types,  
+                 (FEDIT option), then return to this prompt. This path also 
+                 allows you to define additional annotations. 
+!\whichref{NMODEL HANDLE/EDIT}{nmodel_public_keys.} 
+!\whichref{parameter SOURCES}{} 
+!\whichref{parameter TEXT}{} 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__plot_type.html b/nplot/nplot__plot_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..af2c4e28638722f2559e28e4d5746e68a9fc4dca
--- /dev/null
+++ b/nplot/nplot__plot_type.html
@@ -0,0 +1,22 @@
+<TITLE>Description of PLOT_TYPE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword PLOT_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> Data representation(s) CONTOUR, HALFTONE, RULED;  POLARISATION
+<DT><EM>Expected input:</EM> Character(16), 4 values.<P>
+Specify the (combination of) data representations: <P>
+        CONTOUR      Contour plot 
+        HALFTONE     Halftone plot 
+        *            Equivalent to CONTOUR, HALFTONE 
+        RULED        Ruled-surface <P>
+        POLARISATION Pseudo-vectors of linear polarisation. This requires two 
+                      input maps, one holding polarisation strengths 
+                      sqrt(Q*Q+U*U) and the other position angles atan(U/Q)/2. 
+!               {\em Such maps are prepared with 
+!                \whichref{NMAP FIDDLE xxx}{} } 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__plots_per_page.html b/nplot/nplot__plots_per_page.html
new file mode 100644
index 0000000000000000000000000000000000000000..f6027dafbcd6d55932eda53bcd2f39b43b0fb077
--- /dev/null
+++ b/nplot/nplot__plots_per_page.html
@@ -0,0 +1,14 @@
+<TITLE>Description of PLOTS_PER_PAGE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword PLOTS_PER_PAGE</H1> 
+
+<DT><EM>Prompt:</EM> Number of plots per page in hor. and vert. directions
+<DT><EM>Default:</EM> 1, 1 /ASK.
+<DT><EM>Expected input:</EM> Integer number, 2 values; min.value: 1.000000; max.value: 5.000000.<P>
+Specify number of plots to be plotted on one page. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__pol_range.html b/nplot/nplot__pol_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..a600ed0af450b219bda7a128c0d21b04deac287e
--- /dev/null
+++ b/nplot/nplot__pol_range.html
@@ -0,0 +1,16 @@
+<TITLE>Description of POL_RANGE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword POL_RANGE</H1> 
+
+<DT><EM>Prompt:</EM> Polarised-flux limits (W.U.)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+No polarisation pseudo-vector will be drown if the intensity of linear 
+polarisation is below the lower limit (and therefore mainly noise); above the 
+upper limit it will be truncated to that limit. <P>
+Please specify the limits in Westerbork Units.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__pol_scale.html b/nplot/nplot__pol_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..978d09ea9e609d3efb264bb6947061b3b4a671a5
--- /dev/null
+++ b/nplot/nplot__pol_scale.html
@@ -0,0 +1,13 @@
+<TITLE>Description of POL_SCALE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword POL_SCALE</H1> 
+
+<DT><EM>Prompt:</EM> Polarisation pseudo-vector length scale W.U./cm
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the polarisation pseudo-vector length scale in Westerbork Units /cm. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__pol_type.html b/nplot/nplot__pol_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..2f96403e669be882598773c1c116270a2e68e841
--- /dev/null
+++ b/nplot/nplot__pol_type.html
@@ -0,0 +1,13 @@
+<TITLE>Description of POL_TYPE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword POL_TYPE</H1> 
+
+<DT><EM>Prompt:</EM> POL, MAG Polarisation representation
+<DT><EM>Expected input:</EM> Character(16).<P>
+Specify if polarisation (POL) or magnetic field (MAG) should be plotted <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__range.html b/nplot/nplot__range.html
new file mode 100644
index 0000000000000000000000000000000000000000..c42e87ff384e92b4b489d7db8991b1e086d54761
--- /dev/null
+++ b/nplot/nplot__range.html
@@ -0,0 +1,19 @@
+<TITLE>Description of RANGE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword RANGE</H1> 
+
+<DT><EM>Prompt:</EM> Halftone saturation limits
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the range of values to be covered by the full range of halftone shades. <P>
+The first value is the minimum to be represented by 'white', the second value 
+the to be represented by 'black'. <P>
+NOTES: 
+        Values outside this range will always be white. (If you think this is a 
+bad idea, please submit a Bug Report.) 
+        It is not possible to invert the scale by specifying a maximum&lt;minimum. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__rule_range.html b/nplot/nplot__rule_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..e0801a928c407eb374a4a6c8ed4402966c16bbb1
--- /dev/null
+++ b/nplot/nplot__rule_range.html
@@ -0,0 +1,14 @@
+<TITLE>Description of RULE_RANGE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword RULE_RANGE</H1> 
+
+<DT><EM>Prompt:</EM> Ruled-surface intensity range (W.U.)
+<DT><EM>Expected input:</EM> Real number, 2 values.<P>
+Specify the intensity limits in Westerbork Units for the ruled surface plot. 
+Values outside the limits will be truncated. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__rule_scale.html b/nplot/nplot__rule_scale.html
new file mode 100644
index 0000000000000000000000000000000000000000..247d20026ba0d05c54247462d1fe83f3e1c589d7
--- /dev/null
+++ b/nplot/nplot__rule_scale.html
@@ -0,0 +1,13 @@
+<TITLE>Description of RULE_SCALE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword RULE_SCALE</H1> 
+
+<DT><EM>Prompt:</EM> Ruled-surface height scale (W.U./cm)
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the ruled-surface height scale in Westerbork Units /cm. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__scale_ampl.html b/nplot/nplot__scale_ampl.html
new file mode 100644
index 0000000000000000000000000000000000000000..f00fa06c9b1ed58b7ffa06676fbc569bbd88f006
--- /dev/null
+++ b/nplot/nplot__scale_ampl.html
@@ -0,0 +1,20 @@
+<TITLE>Description of SCALE_AMPL (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword SCALE_AMPL</H1> 
+
+<DT><EM>Prompt:</EM> Magnitude scale (W.U./mm or %/mm)
+<DT><EM>Default:</EM> 10..
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the magnitude scale: <P>
+  in Westerbork Units /mm       for source/model visibilities and visibility 
+                                 residuals 
+  in percent/mm                 for telescope corrections <P>
+The ugly default for DATA_TYPE=RES is 4 times the maximum of the Redun/Align 
+amplitude noises recorded in the sector headers selected. For other DATA_TYPEs 
+it is a value that is likely to give reasonable output.   <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__scale_phase.html b/nplot/nplot__scale_phase.html
new file mode 100644
index 0000000000000000000000000000000000000000..be753c62903cf610bf308bd15a8caa65ea01425e
--- /dev/null
+++ b/nplot/nplot__scale_phase.html
@@ -0,0 +1,18 @@
+<TITLE>Description of SCALE_PHASE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword SCALE_PHASE</H1> 
+
+<DT><EM>Prompt:</EM> Phase scale (W.U./mm or deg/mm)
+<DT><EM>Default:</EM> 1..
+<DT><EM>Expected input:</EM> Real number; min.value: 0.000000.<P>
+Specify the phase scale: <P>
+  in Westerbork Units /mm  for residuals 
+  in degrees/mm            for source/model visibilities; for telescope 
+                            corrections. <P>
+The default is a value that is likely to give reasonable output.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__size.html b/nplot/nplot__size.html
new file mode 100644
index 0000000000000000000000000000000000000000..66fe80a66facb5432ee3eaa3d6fa1a0b102b77b4
--- /dev/null
+++ b/nplot/nplot__size.html
@@ -0,0 +1,19 @@
+<TITLE>Description of SIZE (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword SIZE</H1> 
+
+<DT><EM>Prompt:</EM> Plot scaling factors (horizontal, vertical)
+<DT><EM>Default:</EM> 1., 1. /ASK.
+<DT><EM>Expected input:</EM> Real number, 2 values; min.value: 0.001000; max.value: 5.000000.<P>
+At this point, the plot has been dimensioned to fit on a single plotter page or 
+terminal screen, but will not necessarily fill it. You may blow it up in either 
+or both dimensions with the factors you specify here. <P>
+If necessary, the blown-up plot will be distributed over more tham one page. 
+!!              Explain default size 
+!!              ''(i.e. a QMS plot of a power of 2 length will be 12.8 cm).'' 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__sources.html b/nplot/nplot__sources.html
new file mode 100644
index 0000000000000000000000000000000000000000..ff1f368879217700a970c1c2477203f88031c4cd
--- /dev/null
+++ b/nplot/nplot__sources.html
@@ -0,0 +1,16 @@
+<TITLE>Description of SOURCES (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword SOURCES</H1> 
+
+<DT><EM>Prompt:</EM> Source pair for annotation
+<DT><EM>Default:</EM> * /ASK.
+<DT><EM>Expected input:</EM> Character(10), 2 values.<P>
+Give the names of two sources that you have selected for plotting. A connecting 
+line will be drawn between them. You will be prompted for an annotation, which 
+defaults to the separation in degrees. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__text.html b/nplot/nplot__text.html
new file mode 100644
index 0000000000000000000000000000000000000000..fb97650be0e1f7f8297adc891a40855fcb8c0861
--- /dev/null
+++ b/nplot/nplot__text.html
@@ -0,0 +1,14 @@
+<TITLE>Description of TEXT (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword TEXT</H1> 
+
+<DT><EM>Prompt:</EM> Annotation for source pair
+<DT><EM>Default:</EM> * /ASK.
+<DT><EM>Expected input:</EM> Character(80).<P>
+The annotation (max 80 characters) for the source pair just selected <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nplot/nplot__transform.html b/nplot/nplot__transform.html
new file mode 100644
index 0000000000000000000000000000000000000000..5d9c29e01c68a49e028dfa984ad5c7fc89a29cc6
--- /dev/null
+++ b/nplot/nplot__transform.html
@@ -0,0 +1,38 @@
+<TITLE>Description of TRANSFORM (NPLOT)</TITLE>
+<H1>Program NPLOT: private keyword TRANSFORM</H1> 
+
+<DT><EM>Prompt:</EM> Grey-scale transfer coefficients:|-
+up to 5 groups of 2 limits plus 3 coefficients of quadratic|
+<DT><EM>Expected input:</EM> Real number, 5 values, min: 3.<P>
+Specify the range coefficients for the CONTINUOUS quadratic transfer function 
+that you selected. 
+!               {\em parameter \textref{HALFTONE}{.halftone} } <P>
+Remember that the data at this point have been normalised to the range [0, 1]. 
+You may specify 5 values, of which the first three are REQUIRED: <P>
+        m, M     Range of normalised data values to be represented by the full 
+                 halftone range. Values outside this range will be truncated. 
+        a, b, c   The 0-th through 2nd-order coefficients in the transfer 
+                 quadratic. <P>
+The result will be ('ndv' = normalised data value): <P>
+        ndv &lt; m:         OUT = 0                         (white) 
+        m &lt; ndv &lt; M:     OUT = a + b*IN + c*IN*IN        (grey scale) 
+        ndv &gt; M:         OUT = 1                         (black) <P>
+You may break the IN range up into partial ranges by specifying multiple sets 
+of m, M, a, b, c separated by semicolons, or specifying the sets one by one as the 
+prompt is repeated. Input will be considered complete when you give no new 
+reply. <P>
+Examples: 
+        standard linear, halftone=ndv:  0, 1, 0, 1 
+        ndv distance from .5:           0, .5, 1, -2; .5, 1, -1, 2 
+        four grey levels:               0, .25, 0; .25, .5, .25; .5, .75, .5; .75, 1, 1 
+        an approximation to an exp 
+         that seeks to match the 
+         quasi-logarithic response 
+         of the human eye:              0, 1, 0, .1, .9  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nplot/nplot_keys.html">List of keywords</A> for NPLOT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
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new file mode 100644
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+++ b/nplot_descr.ps
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new file mode 100644
index 0000000000000000000000000000000000000000..f64a3d2075f60ae2c5fa5c1b3e4f6a70db3788ce
--- /dev/null
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@@ -0,0 +1,5 @@
+#define noname_width 15
+#define noname_height 14
+static char noname_bits[] = {
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+ 0x61,0x63,0x63,0x36,0x36,0x1e,0x3c,0x0c,0x18,0x38,0x0e,0xf0,0x07};
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--- /dev/null
+++ b/nplot_descr/_11065_tex2html_wrap213.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0xc1,0x07,0x02,0xc1,0x07,0x02,0x01,0x0c,0x02,0x01,0x0e,0x02,0x01,0x07,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0x81,0x01,0x02,0x81,0x01,0x02,0x01,0x00,0x02,
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diff --git a/nplot_descr/images.pl b/nplot_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..31f991fff14fae9e966a3f8cffd98368dbae0a93
--- /dev/null
+++ b/nplot_descr/images.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}fbox<<209>>largesf?<<209>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11065_tex2html_wrap213.xbm">'; 
+$key = q/{}$bigotimes${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11065_tex2html_wrap211.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/nplot_descr/labels.pl b/nplot_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..4840c35bb199554bd5f0235c0c72c57e9be142e1
--- /dev/null
+++ b/nplot_descr/labels.pl
@@ -0,0 +1,12 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".options"} ="$URL/nplot_descr.html"; 
+$external_labels{".data.normal"} ="$URL/nplot_descr.html"; 
+$external_labels{".output"} ="$URL/nplot_descr.html"; 
+$external_labels{".pluvo"} ="$URL/nplot_descr.html"; 
+$external_labels{".data"} ="$URL/nplot_descr.html"; 
+$external_labels{".map"} ="$URL/nplot_descr.html"; 
+$external_labels{".contents"} ="$URL/nplot_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/nplot_descr/nplot_descr.html b/nplot_descr/nplot_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..b79340fd5b2deb0f7f042475abcbacb581e68b8b
--- /dev/null
+++ b/nplot_descr/nplot_descr.html
@@ -0,0 +1,130 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NPLOT</b>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nplot_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nplot_descr.html#SECTION0002000000000000000> <b>Overview of NPLOT options</b></A>
+<LI> <A NAME=tex2html3 HREF=nplot_descr.html#SECTION0003000000000000000> <b>NPLOT output</b></A>
+<LI> <A NAME=tex2html4 HREF=nplot_descr.html#SECTION0004000000000000000> <b>Plotting a map from a WMP file</b></A>
+<LI> <A NAME=tex2html5 HREF=nplot_descr.html#SECTION0005000000000000000> <b>Plotting uv-data from a SCN-file</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=nplot_descr.html#SECTION0005100000000000000> <b>NORMAL: interferometers vs time (HA)</b></A>
+<LI> <A NAME=tex2html7 HREF=nplot_descr.html#SECTION0005200000000000000> <b>PLUVO: frequency channels vs time (HA)</b></A>
+</UL>
+</UL>
+<A NAME=.options><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000> <b>Overview of NPLOT options</b></A></H1>
+<P>
+The program NPLOT has the following main options:
+<P>
+<UL><LI> <b>MAP:</b>        Plot map(s) of various types (from WMP-file)  
+<LI> <b>DATA:</b>       Plot uv-data from SCN-file  
+<LI> <b>MODEL:</b>      Plot uv-model from SCN-file   
+        (i.e. the uv-representation of a Selfcal model,   
+        calculated for the uv-coordinates of the uv-data in the SCN-file)  
+<LI> <b>TELESCOPE:</b>  Plot telescope errors  
+<LI> <b>RESIDUAL:</b>   Plot interferometer residuals  
+        (i.e. the residual scatter of redundant spacing data after a  
+        Redundancy solution, or the residual differences with the   
+        source model after a Selfcal solution.  
+<LI> <b>QUIT:</b>       Quit the program NPLOT  
+</UL>
+<P>
+<A NAME=.output><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>NPLOT output</b></A></H1>
+<P>
+After selecting an NPLOT option, the <b>PLOTTER</b> question is asked:
+<P>
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_11065_tex2html_wrap211.png"> <b>PLOTTER</b>  
+ (QMS,QMSP,REGIS,FREGIS,EPS,EPP,PSL,PSP,...)  
+ = PSP:  
+ <IMG ALIGN=BOTTOM ALT="" SRC="_11065_tex2html_wrap213.png">
+<P>
+Produces QMS formatted files, for which currenlty no printers are available<BR><tt>QMS    QMS laser printer in landscape orientation</tt><BR><tt>QMSP   QMS laser printer in portrait orientation</tt><BR>Produces output on VT terminal:<BR><tt>REGIS  graphics VT terminal (e.g. VT330)</tt><BR><tt>FREGIS (*) REGIS to file</tt><BR>Produces PostScript files on disk (which may fill up quickly!):<BR><tt>EPS    encapsulated PostScript for use in textprocessors etc</tt><BR><tt>EPP    EPS in portrait mode</tt><BR><tt>EAL    encapsulated PostScript A3 plotter landscape</tt><BR><tt>EAP    EPS A3 in portrait mode</tt><BR>Produces PostScript files, and prints them automatically (if you are lucky)<BR>on the New PostScript laser printer in the Dwingeloo computer room:<BR><tt>PSL    Postscript (do not use halftone: slow!)</tt><BR><tt>PSP    PostScript in portrait mode</tt><BR><tt>PAL    Postscript A3 (do not use halftone: slow!)</tt><BR><tt>PAP    PostScript A3 in portrait mode</tt><BR>Bit maps:<BR><tt>BIT1   (*) bitmap for 100 dpi</tt><BR><tt>BIT2   (*) bitmap for 200 dpi</tt><BR><tt>BIT3   (*) bitmap for 300 bpi</tt><BR>Produces a X11-plot on the Workstation (or X-terminal) screen.<BR><tt>X11    X11 terminal</tt><BR><tt>(*) = not implemented yet.</tt>
+<P>
+All plot file names start with the 3-4 letters of the selected option (e.g. EPS), followed by a unique combination of characters based on the time and the date. All plot files have the extension .PLT.
+<P>
+<A NAME=.map><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000> <b>Plotting a map from a WMP file</b></A></H1>
+<P>
+NPLOT option MAP can be used to make <b>contour plots</b> or <b>greyscale plots</b> of 2-dimensional pixel-arrays stored in a  WMP-file.  These may be maps, antenna-patterns, residuals etc, but also gridded uv-data (see the description of the program NMAP, and the WMP file).  They can also be displayed (and analysed) as a color image on the X11 screen with the program NGIDS.
+<P>
+*** Put new script here ****
+<P>
+The plot is now made, and sent to the laser plotter automatically if that has been specified. The program will then prompt the user for the next plot  to be specified.
+<P>
+**** Put new script here ****
+<P>
+It is also possible to make `ruled-surface' plots, halftone plots and plots in polar coordinates (gridded uv-data).
+<P>
+<A NAME=.data><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000> <b>Plotting uv-data from a SCN-file</b></A></H1>
+<P>
+<A NAME=.data.normal><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005100000000000000> <b>NORMAL: interferometers vs time (HA)</b></A></H2>
+<P>
+**** Put new script here ****
+<P>
+The plot is now made, and sent to the laser plotter automatically if that has been specified. The program will then prompt the user for the next plot  to be specified.
+<P>
+**** Put new script here ****
+<P>
+<A NAME=.pluvo><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005200000000000000> <b>PLUVO: frequency channels vs time (HA)</b></A></H2>
+<P>
+**** Put new script here ****
+<P>
+Etc...
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nplot_keys/nplot_keys.html b/nplot_keys/nplot_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..df201ec052b9ae735c3c397e29057d5ce4811127
--- /dev/null
+++ b/nplot_keys/nplot_keys.html
@@ -0,0 +1,140 @@
+<TITLE>Index of private keywords for NPLOT </TITLE>
+<H1>Description of keywords for program NPLOT</H1>
+
+<UL>
+
+<UL><LI>See also <A HREF="../plotter_comm/plotter_comm.html">PLOTTER</A> </UL>
+
+<P><LI> <A HREF="../nplot/nplot__option.html">
+  OPTION</A>
+  Type of data to plot|  MAP; DATA, RESID, MODEL; TELESC, INTERFM, IFDATA;|SPECIAL; QUIT
+<LI> <A HREF="../nplot/nplot__ha_mode.html">
+  HA_MODE</A>
+  Special HA plot coordinates ST, IST, SEQUENCE, ISEQUENCE
+<LI> <A HREF="../nplot/nplot__ha_integration.html">
+  HA_INTEGRATION</A>
+  Integration time (sec)
+<LI> <A HREF="../nplot/nplot__annotation.html">
+  ANNOTATION</A>
+  Annotation text, up to 80 characters in double quotes
+<LI> <A HREF="../nplot/nplot__if_mode.html">
+  IF_MODE</A>
+  Parameter to plot TPON, TPOFF, TSYS, ISYS, GAIN;  GNCAL, TSYSI, TNOISI, RGAINI
+<LI> <A HREF="../nplot/nplot__ifr_mode.html">
+  IFR_MODE</A>
+  NORMAL, INVERT, SORT;  SPECTRAL, BAND Select data cross-section
+<LI> <A HREF="../nplot/nplot__angle_wmp_set.html">
+  ANGLE_WMP_SET</A>
+  ONE position-angle map: grp.fld.chn.pol.0.seq
+<LI> <A HREF="../nplot/nplot__data_types.html">
+  DATA_TYPES</A>
+  Visibility component to plot AMPLITUDE, PHASE; AGAIN, PGAIN; COSINE, SINE;  AP, CS
+<LI> <A HREF="../nplot/nplot__plots_per_page.html">
+  PLOTS_PER_PAGE</A>
+  Number of plots per page in hor. and vert. directions
+<LI> <A HREF="../nplot/nplot__data_type.html">
+  DATA_TYPE</A>
+  DATA; SLOPE data types to plot
+<LI> <A HREF="../nplot/nplot__plot_type.html">
+  PLOT_TYPE</A>
+  Data representation(s) CONTOUR, HALFTONE, RULED;  POLARISATION
+<LI> <A HREF="../nplot/nplot__scale_ampl.html">
+  SCALE_AMPL</A>
+  Magnitude scale (W.U./mm or %/mm)
+<LI> <A HREF="../nplot/nplot__scale_phase.html">
+  SCALE_PHASE</A>
+  Phase scale (W.U./mm or deg/mm)
+<LI> <A HREF="../nplot/nplot__ha_scale.html">
+  HA_SCALE</A>
+  HA plot scale (degree/cm)
+<LI> <A HREF="../nplot/nplot__pol_scale.html">
+  POL_SCALE</A>
+  Polarisation pseudo-vector length scale W.U./cm
+<LI> <A HREF="../nplot/nplot__rule_scale.html">
+  RULE_SCALE</A>
+  Ruled-surface height scale (W.U./cm)
+<LI> <A HREF="../nplot/nplot__area.html">
+  AREA</A>
+  Area centre (l, m) and width (dl, dm) in grid units
+<LI> <A HREF="../nplot/nplot__size.html">
+  SIZE</A>
+  Plot scaling factors (horizontal, vertical)
+<LI> <A HREF="../nplot/nplot__full_cont.html">
+  FULL_CONT</A>
+  Full-contour levels
+<LI> <A HREF="../nplot/nplot__dot_cont.html">
+  DOT_CONT</A>
+  Dotted-contour levels
+<LI> <A HREF="../nplot/nplot__halftone.html">
+  HALFTONE</A>
+  NONE, CONTINUE; STEP, PATTERN Halftone transfer function
+<LI> <A HREF="../nplot/nplot__range.html">
+  RANGE</A>
+  Halftone saturation limits
+<LI> <A HREF="../nplot/nplot__transform.html">
+  TRANSFORM</A>
+  Grey-scale transfer coefficients:|-
+up to 5 groups of 2 limits plus 3 coefficients of quadratic|
+<LI> <A HREF="../nplot/nplot__pol_range.html">
+  POL_RANGE</A>
+  Polarised-flux limits (W.U.)
+<LI> <A HREF="../nplot/nplot__pol_type.html">
+  POL_TYPE</A>
+  POL, MAG Polarisation representation
+<LI> <A HREF="../nplot/nplot__rule_range.html">
+  RULE_RANGE</A>
+  Ruled-surface intensity range (W.U.)
+<LI> <A HREF="../nplot/nplot__coord.html">
+  COORD</A>
+  | NONE;  LM,  DEGREE, RADEC;  DLM,  DDEGREE, DRADEC;|-ONONE; OLM, ODEGREE, ORADEC; ODLM, ODDEGREE, ODRADEC Axis annotation style
+<LI> <A HREF="../nplot/nplot__coord_type.html">
+  COORD_TYPE</A>
+  TICK, DOTTED, FULL Coordinate grid style
+<LI> <A HREF="../nplot/nplot__plot_positions.html">
+  PLOT_POSITIONS</A>
+  NO, YES, NAMES; EDIT Mark source positions
+<LI> <A HREF="../nplot/nplot__sources.html">
+  SOURCES</A>
+  Source pair for annotation
+<LI> <A HREF="../nplot/nplot__text.html">
+  TEXT</A>
+  Annotation for source pair
+<LI> <A HREF="../nplot/nplot__plot_heading.html">
+  PLOT_HEADING</A>
+  YES, NO Plot heading (Yes/No) ?
+<LI> <A HREF="../nplot/nplot__coord_prec.html">
+  COORD_PREC</A>
+  Number of steps for coordinate contouring near pole
+<P>
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpnode_comm/wmpnode_comm.html">WMPNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../wmpsets_comm/wmpsets_comm.html">WMPSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nplot_descr/nplot_descr.html">program NPLOT</A>
+</UL>
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new file mode 100644
index 0000000000000000000000000000000000000000..04e6dd740ccf97818d8023bb4465915820581bb9
--- /dev/null
+++ b/nplot_private_intfc.ps
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+(here.)0 2392 y(If)j(necessary)o(,)e(the)h(blown-up)f(plot)h(will)g(be)
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+(the)h(separatio)o(n)e(in)h(degrees.)935 2995 y Fi(9)p
+eop
+%%Page: 10 10
+10 9 bop 0 -41 a Fh(2.33)74 b(P)n(arameter)18 b(TEXT)0
+60 y Fl(Pr)n(ompt:)g Fi(Annotation)13 b(for)h(source)h(pair)0
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+(range)f([0,1].)0 814 y(You)g(may)h(specify)e(5)i(values,)e(of)i(which)
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+(c*IN*IN)154 b(\(grey)18 b(scale\))157 1279 y(ndv)g(>)i(M:)175
+b(OUT)19 b(=)g(1)490 b(\(black\))0 1357 y(You)18 b(may)h(break)f(the)g
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+(complete)f(when)i(you)h(give)f(no)h(new)0 1494 y(reply.)0
+1573 y(Examples:)157 1619 y(standard)d(linear,)h(halftone=n)o(dv:)36
+b(0,1,)18 b(0,1)157 1665 y(ndv)g(distance)f(from)h(.5:)215
+b(0,.5,)17 b(1,-2;)h(.5,1,)g(-1,2)157 1710 y(four)g(grey)g(levels:)292
+b(0,.25,0;)16 b(.25,.5,.25)o(;)g(.5,.75,.5;)g(.75,1,1)157
+1756 y(an)j(approxima)o(tio)o(n)d(to)j(an)g(exp)177 1802
+y(that)f(seeks)f(to)i(match)f(the)177 1847 y(quasi-lo)o(gar)o(ith)o(ic)
+e(response)177 1893 y(of)i(the)h(human)f(eye:)273 b(0,1,)18
+b(0,.1,.9)924 2995 y Fi(10)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nplot_private_intfc/images.pl b/nplot_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nplot_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nplot_private_intfc/labels.pl b/nplot_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..646b921ed69371454b4cf1886d53fb0f1bfc6c69
--- /dev/null
+++ b/nplot_private_intfc/labels.pl
@@ -0,0 +1,41 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".plot.heading"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".data.types"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".public"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".text"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".pol.scale"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".ha.scale"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".annotation"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".ha.integration"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".coord.type"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".contents"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".dot.cont"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".ha.mode"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".data.type"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".scale.phase"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".coord.prec"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".plots.per.page"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".rule.range"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".plot.type"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".plot.positions"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".size"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".sources"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".area"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".full.cont"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".pol.type"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".scale.ampl"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".range"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".if.mode"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".pol.range"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".option"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".transform"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".ifr.mode"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".rule.scale"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".coord"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".angle.wmp.set"} ="$URL/nplot_private_intfc.html"; 
+$external_labels{".halftone"} ="$URL/nplot_private_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/nplot_private_intfc/nplot_private_intfc.html b/nplot_private_intfc/nplot_private_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..5cf757e5e7c0b1821aad589c8467b28632cafd5a
--- /dev/null
+++ b/nplot_private_intfc/nplot_private_intfc.html
@@ -0,0 +1,850 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NPLOT</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nplot_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nplot_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nplot_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nplot_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nplot_private_intfc.html#SECTION0003200000000000000>  <b>Parameter ANGLE_WMP_SET</b></A>
+<LI> <A NAME=tex2html6 HREF=nplot_private_intfc.html#SECTION0003300000000000000>  <b>Parameter ANNOTATION</b></A>
+<LI> <A NAME=tex2html7 HREF=nplot_private_intfc.html#SECTION0003400000000000000>  <b>Parameter AREA</b></A>
+<LI> <A NAME=tex2html8 HREF=nplot_private_intfc.html#SECTION0003500000000000000>  <b>Parameter COORD</b></A>
+<LI> <A NAME=tex2html9 HREF=nplot_private_intfc.html#SECTION0003600000000000000>  <b>Parameter COORD_PREC</b></A>
+<LI> <A NAME=tex2html10 HREF=nplot_private_intfc.html#SECTION0003700000000000000>  <b>Parameter COORD_TYPE</b></A>
+<LI> <A NAME=tex2html11 HREF=nplot_private_intfc.html#SECTION0003800000000000000>  <b>Parameter DATA_TYPE</b></A>
+<LI> <A NAME=tex2html12 HREF=nplot_private_intfc.html#SECTION0003900000000000000>  <b>Parameter DATA_TYPES</b></A>
+<LI> <A NAME=tex2html13 HREF=nplot_private_intfc.html#SECTION00031000000000000000>  <b>Parameter DOT_CONT</b></A>
+<LI> <A NAME=tex2html14 HREF=nplot_private_intfc.html#SECTION00031100000000000000>  <b>Parameter FULL_CONT</b></A>
+<LI> <A NAME=tex2html15 HREF=nplot_private_intfc.html#SECTION00031200000000000000>  <b>Parameter HALFTONE</b></A>
+<LI> <A NAME=tex2html16 HREF=nplot_private_intfc.html#SECTION00031300000000000000>  <b>Parameter HA_INTEGRATION</b></A>
+<LI> <A NAME=tex2html17 HREF=nplot_private_intfc.html#SECTION00031400000000000000>  <b>Parameter HA_MODE</b></A>
+<LI> <A NAME=tex2html18 HREF=nplot_private_intfc.html#SECTION00031500000000000000>  <b>Parameter HA_SCALE</b></A>
+<LI> <A NAME=tex2html19 HREF=nplot_private_intfc.html#SECTION00031600000000000000>  <b>Parameter IFR_MODE</b></A>
+<LI> <A NAME=tex2html20 HREF=nplot_private_intfc.html#SECTION00031700000000000000>  <b>Parameter IF_MODE</b></A>
+<LI> <A NAME=tex2html21 HREF=nplot_private_intfc.html#SECTION00031800000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html22 HREF=nplot_private_intfc.html#SECTION00031900000000000000>  <b>Parameter PLOTS_PER_PAGE</b></A>
+<LI> <A NAME=tex2html23 HREF=nplot_private_intfc.html#SECTION00032000000000000000>  <b>Parameter PLOT_HEADING</b></A>
+<LI> <A NAME=tex2html24 HREF=nplot_private_intfc.html#SECTION00032100000000000000>  <b>Parameter PLOT_POSITIONS</b></A>
+<LI> <A NAME=tex2html25 HREF=nplot_private_intfc.html#SECTION00032200000000000000>  <b>Parameter PLOT_TYPE</b></A>
+<LI> <A NAME=tex2html26 HREF=nplot_private_intfc.html#SECTION00032300000000000000>  <b>Parameter POL_RANGE</b></A>
+<LI> <A NAME=tex2html27 HREF=nplot_private_intfc.html#SECTION00032400000000000000>  <b>Parameter POL_SCALE</b></A>
+<LI> <A NAME=tex2html28 HREF=nplot_private_intfc.html#SECTION00032500000000000000>  <b>Parameter POL_TYPE</b></A>
+<LI> <A NAME=tex2html29 HREF=nplot_private_intfc.html#SECTION00032600000000000000>  <b>Parameter RANGE</b></A>
+<LI> <A NAME=tex2html30 HREF=nplot_private_intfc.html#SECTION00032700000000000000>  <b>Parameter RULE_RANGE</b></A>
+<LI> <A NAME=tex2html31 HREF=nplot_private_intfc.html#SECTION00032800000000000000>  <b>Parameter RULE_SCALE</b></A>
+<LI> <A NAME=tex2html32 HREF=nplot_private_intfc.html#SECTION00032900000000000000>  <b>Parameter SCALE_AMPL</b></A>
+<LI> <A NAME=tex2html33 HREF=nplot_private_intfc.html#SECTION00033000000000000000>  <b>Parameter SCALE_PHASE</b></A>
+<LI> <A NAME=tex2html34 HREF=nplot_private_intfc.html#SECTION00033100000000000000>  <b>Parameter SIZE</b></A>
+<LI> <A NAME=tex2html35 HREF=nplot_private_intfc.html#SECTION00033200000000000000>  <b>Parameter SOURCES</b></A>
+<LI> <A NAME=tex2html36 HREF=nplot_private_intfc.html#SECTION00033300000000000000>  <b>Parameter TEXT</b></A>
+<LI> <A NAME=tex2html37 HREF=nplot_private_intfc.html#SECTION00033400000000000000>  <b>Parameter TRANSFORM</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NPLOT. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show parameters that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../wmpnode_public_intfc/wmpnode_public_intfc.html">WMPNODE</A> public keywords 
+<LI> <A HREF="../wmpsets_public_intfc/wmpsets_public_intfc.html">WMPSETS</A> public keywords 
+</UL>
+<P>
+<A NAME=.angle.wmp.set><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter ANGLE_WMP_SET</b></A></H2>
+<P>
+  <em>Prompt:</em> ONE position-angle map: grp.fld.chn.pol.0.seq<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+    <PRE>
+Select a .WMP-file image holding polarisation position angles. If the image you
+specify contains anything else, your plot will be garbage.
+</PRE>
+<P>
+  <PRE>
+The .WMP-file indices are:
+</PRE>
+<P>
+  <PRE>
+        group.field.channel.polarisation.type(=0).sequence_number
+</PRE>
+<P>
+<A NAME=.annotation><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter ANNOTATION</b></A></H2>
+<P>
+<em>Prompt:</em> Annotation text, up to 80 characters in double quotes<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+This text will be displayed on all plots for this NPLOT run until you change it
+</PRE>
+<P>
+<A NAME=.area><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter AREA</b></A></H2>
+<P>
+<em>Prompt:</em> Area centre (l,m) and width (dl,dm) in grid units<BR><em>Expected input:</em> Integer:  1 to 4 values
+<P>
+  <PRE>
+Specify an area of a map:
+</PRE>
+<P>
+  <PRE>
+        l,m     grid coordinates of area centre: 0,0 is the map centre,
+                 increasing to the upper right (i.e. with DEcreasing
+                 right ascension and INcreasing declination)
+</PRE>
+<P>
+  <PRE>
+        dl,dm   area width and height
+</PRE>
+<P>
+<A NAME=.coord><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter COORD</b></A></H2>
+<P>
+<em>Prompt:</em> Axis annotation style<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Select ONE style of axis annotations:
+</PRE>
+<P>
+  <PRE>
+        NONE     no annotation (only pixel coordinates)
+</PRE>
+<P>
+  <PRE>
+   Relative quasi-Cartesian coordinates:
+</PRE>
+<P>
+  <PRE>
+        LM       l, m in arcsec with respect to map centre
+                  (or annotation for UV-plane plots)
+        DLM      l, m in arcsec with respect to centre of plot
+                  (or annotation for UV-plane plots)
+</PRE>
+<P>
+  <PRE>
+   Equatorial coordinates:
+</PRE>
+<P>
+  <PRE>
+        DEGREE   right ascension and declination in decimal degrees
+        RADEC    right ascension (hhmmss) and declination (ddmmss)
+        DDEGREE  relative right ascension and declination in decimal degrees
+                  w.r.t.  centre of plot
+        DRADEC   relative right ascension (hhmmss) and declination (ddmmss)
+                  w.r.t. centre of plot
+</PRE>
+<P>
+  <PRE>
+These annotations will be printed along the left and bottom sides of the plot.
+</PRE>
+<P>
+  <PRE>
+By default, (l,m) pixel-coordinates are shown along the top and right axes side
+irrespective of what you select. You may suppress these, by prefixing any of
+the above options with an O for 'Only'.
+</PRE>
+<P>
+  <PRE>
+Example:
+        ONONE will suppress all annotations.
+</PRE>
+<P>
+<A NAME=.coord.prec><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter COORD_PREC</b></A></H2>
+<P>
+<em>Prompt:</em> Number of steps for coordinate contouring near pole<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the number of steps across the map to use in defining the
+coordinate grid for contouring of coordinates near the pole.
+</PRE>
+<P>
+<A NAME=.coord.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter COORD_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Coordinate grid style<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Select the style for plotting coordinate grid lines:
+</PRE>
+<P>
+  <PRE>
+   TICK          give along plot edges only
+   DOTTED        dotted grid
+   FULL          full-drawn grid
+</PRE>
+<P>
+<A NAME=.data.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter DATA_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> data types to plot<BR><em>Expected input:</em> Character *16:  1 value
+<P>
+  <PRE>
+Specify the data type(s) to be plotted.
+</PRE>
+<P>
+  <PRE>
+   DATA or *    plot the data as given in the map
+   SLOPE        plot the horizontal slope of the data (This option is still
+                 experimental)
+</PRE>
+<P>
+<A NAME=.data.types><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter DATA_TYPES</b></A></H2>
+<P>
+<em>Prompt:</em> Visibility component to plot<BR><em>Expected input:</em> Character *16:  1 to 6 values
+<P>
+  <PRE>
+Specify the visibility component to be plotted.
+</PRE>
+<P>
+  <PRE>
+        The quantity plotted depends on the data selected.  For TEL or INTERF
+and for redund. RES       :       gain-1(%
+                  ampl (WU), phase(deg For Selfcal RES with external model:
+</PRE>
+<P>
+  <PRE>
+   Standard representations of complex data:
+</PRE>
+<P>
+  <PRE>
+                        Model           Resid           Int.model
+        AMPLITUDE
+        PHASE
+        COSINE
+        SINE
+</PRE>
+<P>
+  <PRE>
+        AGAIN   Re log(data/model) * 100 = gain in %
+        PGAIN   Im log(data/model) * 180/pi = phase in deg
+</PRE>
+<P>
+  <PRE>
+   Old WSRT 'PLOTAP' formats:
+</PRE>
+<P>
+  <PRE>
+        AP         amplitude/phase plots, one pair per page
+        CS         cosine/sine plots, one pair per page
+</PRE>
+<P>
+<em>Expected input:</em> Real *16:  1 to 6 values
+<P>
+<A NAME=.dot.cont><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter DOT_CONT</b></A></H2>
+<P>
+<em>Prompt:</em> Dotted-contour levels<BR><em>Expected input:</em> Real:  1 to 32 values
+<P>
+  <PRE>
+Specify up to 32 values of the contours to be drawn as dotted lines.
+</PRE>
+<P>
+<A NAME=.full.cont><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter FULL_CONT</b></A></H2>
+<P>
+<em>Prompt:</em> Full-contour levels<BR><em>Expected input:</em> Real:  1 to 32 values
+<P>
+  <PRE>
+Specify up to 32 values of the contours to be drawn as full lines.
+</PRE>
+<P>
+<A NAME=.halftone><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter HALFTONE</b></A></H2>
+<P>
+<em>Prompt:</em> Halftone transfer function<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+At this point, data values have been normalised to lie within the interval
+[0,1]. Halftones are represented by the same interval: 0=white, 1=black. You
+are now to define the transfer function F for mapping data values onto
+halftones:
+</PRE>
+<P>
+  <PRE>
+        halftone = F (normalised data value)
+</PRE>
+<P>
+  <PRE>
+   Continuous functions:
+</PRE>
+<P>
+  <PRE>
+        CONTINUE  a quadratic function (you will be prompted for the
+                   coefficients)
+        NONE      direct mapping: halftone level = normalised data value
+</PRE>
+<P>
+  <PRE>
+   Discontinuous functions:
+</PRE>
+<P>
+  <PRE>
+        STEP      F is a staircase function; halftone shades are generated by a
+                   stochastic algorithm
+        PATTERN   as STEP, but halftone shades are represented by a set of
+                   fixed patterns
+</PRE>
+<P>
+  <PRE>
+In selecting a method, bear in mind that the human eye is quite sensitive to
+density variations in light shades while very poorly perceiving the same
+variations in the dark shades; in other words, its response to density
+variations is quasi-logarithmic.
+</PRE>
+<P>
+  <PRE>
+To compensate for this, a quasi-exponential transfer function is suitable. The
+best approximation to this available here is a steeply quadratic function (i.e.
+specify CONTINUE here and consult the on-line help for the TRANSFORM parameter).
+</PRE>
+<P>
+  <PRE>
+You may judge the quality of your transfer function from the grey-scale wedge
+that will appear side by side with your plot.
+</PRE>
+<P>
+<A NAME=.ha.integration><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter HA_INTEGRATION</b></A></H2>
+<P>
+<em>Prompt:</em> Integration time (sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the time interval over which you want to integrate (if possible) before
+calibrating. The value you specify will be rounded down to a multiple of the
+hour-angle interval between successive scans.
+</PRE>
+<P>
+  <PRE>
+'*' and '0' mean do not integrate, i.e. calibrate per scan.
+</PRE>
+<P>
+  <PRE>
+The largest value allowed is 3600 (= 1 hour).
+</PRE>
+<P>
+<A NAME=.ha.mode><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter HA_MODE</b></A></H2>
+<P>
+<em>Prompt:</em> Special HA plot coordinates<BR><em>Expected input:</em> Character *10:  1 value
+<P>
+  <PRE>
+This parameter selects a coordinate conversion for the vertical (HA) plot
+coordinate in plots of .SCN-file entities.
+</PRE>
+<P>
+  <PRE>
+    ST          Sidereal time i.s.o. HA. This is useful for plotting a series of
+                 observations (e.g. calibrators-object-calibrators) in a time
+                 sequence, e.g. to survey interference. Vertical coordinate is
+                 ST in degrees
+</PRE>
+<P>
+  <PRE>
+    SEQUENCE    Pseudo sidereal time: Sidereal time is forced into an ascending
+                 sequence: When the start ST for a sector is less than that of
+                 the one just plotted, it is changed to make the new sector
+                 follow the previous one contiguously. Within each sector,
+                 vertical scale size is that of HA or ST, but the sectors are
+                 displaced in ST. Sectors are plotted in order of their index.
+                This mode is useful to stuff a lot of information into a single
+                 plot, e.g. to check for interference, but the plot may become
+                 too confusing.
+</PRE>
+<P>
+  <PRE>
+    I<xxx>      The prefix I indicates that you want to integrate scans; you
+                 will be prompted for the HA interval over which to integrate.
+                 As currently implemented, this mode is effective only for plots
+                 that have HA or (pseudo)ST as vertical coordinate. The plot
+                 scale for this coordinate will not be affected.
+</PRE>
+<P>
+  <PRE>
+NPLOT will set plotting mode according to your reply and return to the OPTION
+prompt. The mode will remain in force until you change it or NPLOT exits.
+</PRE>
+<P>
+<A NAME=.ha.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter HA_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> HA plot scale (degree/cm)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the hour-angle scale in degree/cm.
+</PRE>
+<P>
+<A NAME=.ifr.mode><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter IFR_MODE</b></A></H2>
+<P>
+<em>Prompt:</em> Select data cross-section<BR><em>Expected input:</em> Character *16:  1 value
+<P>
+  <PRE>
+Specify the cross section through the visibility data cube to be plotted:
+        Consider the interferometers arranged in an upper-triangular matrix:
+</PRE>
+<P>
+  <PRE>
+                00 01 02 ... 0B 0C 0D
+                   11 12 ... 1B 1C 1D
+                      22 ... 2B 2C 2D
+                             :  :  :
+                             BB BC BD
+                                CC CD
+                                   DD
+</PRE>
+<P>
+  <PRE>
+Then the possible plotting modes are
+</PRE>
+<P>
+  <PRE>
+    visibilities as function of hour angle per interferometer:
+</PRE>
+<P>
+  <PRE>
+        NORMAL  interferometer order in the matrix is row by row
+</PRE>
+<P>
+  <PRE>
+        INVERT  interferometer order in the matrix is column by column  .
+        SORT    interferometers in order of ascending baseline
+</PRE>
+<P>
+  <PRE>
+    other cross sections of the hour-angle/interferometer/channel cube:
+</PRE>
+<P>
+  <PRE>
+        SPECTRAL visibilities as function of spectral channel and hour angle,
+                  per interferometer (the WSRT 'PLUVO' format)
+</PRE>
+<P>
+  <PRE>
+        BAND    visibilities as function of channel and interferometer,
+                 interferometer order as for NORMAL
+</PRE>
+<P>
+<A NAME=.if.mode><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter IF_MODE</b></A></H2>
+<P>
+<em>Prompt:</em> Parameter to plot<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+  <PRE>
+Specify action to perform:
+</PRE>
+<P>
+  <PRE>
+   Telescope parameters:
+</PRE>
+<P>
+  <PRE>
+        TPON          total power data (noise source off)
+        TPOFF         total power data (noise source on)
+        TSYS          system temperatures
+        ISYS          system temperatures (X+Y)
+        GAIN          IF gains
+</PRE>
+<P>
+  <PRE>
+   Interferometer parameters:
+</PRE>
+<P>
+  <PRE>
+        GNCAL         gain correction method
+        TSYSI         constant system temperature
+        TNOISI        constant noise source temperature
+        RGAINI        constant receiver gain
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Type of data to plot|<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify type of data to plot:
+</PRE>
+<P>
+  <PRE>
+   .WMP-file data:
+</PRE>
+<P>
+  <PRE>
+        MAP              image(s) from .WMP file
+</PRE>
+<P>
+  <PRE>
+   .SCN-file visibilities:
+        DATA             observed visibilities
+        MODEL            model visibilities
+        RESIDUAL         visibility residuals (after correction of all known
+                          errors and division by the visibilities of a source
+                          model (yet to be specified)
+                                (sets I=1, QUV=0)
+</PRE>
+<P>
+  <PRE>
+   .SCN-file correction parameters:
+</PRE>
+<P>
+  <PRE>
+        TELESCOPE        telescope phase/gain corrections
+        INTERFEROMETER   interferometer phase/gain corrections (i.e. all
+                          corrections combined per interferometer)
+</PRE> 
+  <PRE>
+        IFDATA           IF-data: total powers, system temperatures etc.
+</PRE>
+<P>
+  <PRE>
+   Plotting versus sidereal time i.s.o. hour angle:
+</PRE>
+<P>
+  <PRE>
+        SPECIAL          will prompt for a special mode
+</PRE>
+<P>
+  <PRE>
+        QUIT             terminate NPLOT
+</PRE>
+<P>
+<A NAME=.plots.per.page><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031900000000000000>  <b>Parameter PLOTS_PER_PAGE</b></A></H2>
+<P>
+<em>Prompt:</em> Number of plots per page in hor. and vert. directions<BR><em>Expected input:</em> Integer:  1 to 2 values
+<P>
+  <PRE>
+Specify number of plots to be plotted on one page.
+</PRE>
+<P>
+<A NAME=.plot.heading><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032000000000000000>  <b>Parameter PLOT_HEADING</b></A></H2>
+<P>
+<em>Prompt:</em> Plot heading (Yes/No) ?<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify if you want to have a MAP plot with or without the heading.
+</PRE>
+<P>
+<A NAME=.plot.positions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032100000000000000>  <b>Parameter PLOT_POSITIONS</b></A></H2>
+<P>
+<em>Prompt:</em> Mark source positions<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify if you want model-source positions marked in your plot. The answers may
+be:
+</PRE>
+<P>
+  <PRE>
+        NO
+        YES     position markers only
+        MAMES   position markers annotated with their IDs from the model list
+</PRE>
+<P>
+  <PRE>
+The marker symbol used is determined per source by its Type (which is the
+suffix number in its ID).
+</PRE>
+<P>
+  <PRE>
+        EDIT    invoke model-handling code to modify model-components' Types,
+                 (FEDIT option), then return to this prompt. This path also
+                 allows you to define additional annotations.
+</PRE> 
+NMODEL HANDLE/EDIT
+parameter SOURCES
+parameter TEXT
+<P>
+<A NAME=.plot.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032200000000000000>  <b>Parameter PLOT_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Data representation(s)<BR><em>Expected input:</em> Character *16:  1 to 4 values
+<P>
+  <PRE>
+Specify the (combination of) data representations:
+</PRE>
+<P>
+  <PRE>
+        CONTOUR      Contour plot
+        HALFTONE     Halftone plot
+        *            Equivalent to CONTOUR,HALFTONE
+        RULED        Ruled-surface
+</PRE>
+<P>
+  <PRE>
+        POLARISATION Pseudo-vectors of linear polarisation. This requires two
+                      input maps, one holding polarisation strengths
+                      sqrt(Q*Q+U*U) and the other position angles atan(U/Q)/2.
+</PRE> 
+               <em>Such maps are prepared with
+                NMAP FIDDLE xxx </em>
+<P>
+<A NAME=.pol.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032300000000000000>  <b>Parameter POL_RANGE</b></A></H2>
+<P>
+<em>Prompt:</em> Polarised-flux limits (W.U.)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+No polarisation pseudo-vector will be drown if the intensity of linear
+polarisation is below the lower limit (and therefore mainly noise); above the
+upper limit it will be truncated to that limit.
+</PRE>
+<P>
+  <PRE>
+Please specify the limits in Westerbork Units.
+</PRE>
+<P>
+<A NAME=.pol.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032400000000000000>  <b>Parameter POL_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> Polarisation pseudo-vector length scale W.U./cm<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the polarisation pseudo-vector length scale in Westerbork Units /cm.
+</PRE>
+<P>
+<A NAME=.pol.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032500000000000000>  <b>Parameter POL_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Polarisation representation<BR><em>Expected input:</em> Character *16:  1 value
+<P>
+  <PRE>
+Specify if polarisation (POL) or magnetic field (MAG) should be plotted
+</PRE>
+<P>
+<A NAME=.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032600000000000000>  <b>Parameter RANGE</b></A></H2>
+<P>
+<em>Prompt:</em> Halftone saturation limits<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the range of values to be covered by the full range of halftone shades.
+</PRE>
+<P>
+  <PRE>
+The first value is the minimum to be represented by 'white', the second value
+the to be represented by 'black'.
+</PRE>
+<P>
+  <PRE>
+NOTES:
+        Values outside this range will always be white. (If you think this is a
+bad idea, please submit a Bug Report.)
+        It is not possible to invert the scale by specifying a maximum<minimum.
+</PRE>
+<P>
+<A NAME=.rule.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032700000000000000>  <b>Parameter RULE_RANGE</b></A></H2>
+<P>
+<em>Prompt:</em> Ruled-surface intensity range (W.U.)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+Specify the intensity limits in Westerbork Units for the ruled surface plot.
+Values outside the limits will be truncated.
+</PRE>
+<P>
+<A NAME=.rule.scale><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032800000000000000>  <b>Parameter RULE_SCALE</b></A></H2>
+<P>
+<em>Prompt:</em> Ruled-surface height scale (W.U./cm)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the ruled-surface height scale in Westerbork Units /cm.
+</PRE>
+<P>
+<A NAME=.scale.ampl><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032900000000000000>  <b>Parameter SCALE_AMPL</b></A></H2>
+<P>
+<em>Prompt:</em> Magnitude scale (W.U./mm or <em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the magnitude scale:
+</PRE>
+<P>
+  <PRE>
+  in Westerbork Units /mm       for source/model visibilities and visibility
+                                 residuals
+  in percent/mm                 for telescope corrections
+</PRE>
+<P>
+  <PRE>
+amplitude noises recorded in the sector headers selected. For other DATA_TYPEs
+it is a value that is likely to give reasonable output.
+</PRE>
+<P>
+<em>Expected input:</em> Real:  1 value
+<P>
+<A NAME=.scale.phase><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033000000000000000>  <b>Parameter SCALE_PHASE</b></A></H2>
+<P>
+<em>Prompt:</em> Phase scale (W.U./mm or deg/mm)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the phase scale:
+</PRE>
+<P>
+  <PRE>
+  in Westerbork Units /mm  for residuals
+  in degrees/mm            for source/model visibilities; for telescope
+                            corrections.
+</PRE>
+<P>
+  <PRE>
+The default is a value that is likely to give reasonable output.
+</PRE>
+<P>
+<A NAME=.size><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033100000000000000>  <b>Parameter SIZE</b></A></H2>
+<P>
+<em>Prompt:</em> Plot scaling factors (horizontal, vertical)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+  <PRE>
+At this point, the plot has been dimensioned to fit on a single plotter page or
+terminal screen, but will not necessarily fill it. You may blow it up in either
+or both dimensions with the factors you specify here.
+</PRE>
+<P>
+  <PRE>
+If necessary, the blown-up plot will be distributed over more tham one page.
+</PRE>
+<P>
+<A NAME=.sources><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033200000000000000>  <b>Parameter SOURCES</b></A></H2>
+<P>
+<em>Prompt:</em> Source pair for annotation<BR><em>Expected input:</em> Character *10:  1 to 2 values
+<P>
+  <PRE>
+Give the names of two sources that you have selected for plotting. A connecting
+line will be drawn between them. You will be prompted for an annotation, which
+defaults to the separation in degrees.
+</PRE>
+<P>
+<A NAME=.text><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033300000000000000>  <b>Parameter TEXT</b></A></H2>
+<P>
+<em>Prompt:</em> Annotation for source pair<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+The annotation (max 80 characters) for the source pair just selected
+</PRE>
+<P>
+<A NAME=.transform><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00033400000000000000>  <b>Parameter TRANSFORM</b></A></H2>
+<P>
+<em>Prompt:</em> Grey-scale transfer coefficients:|-<BR><em>Expected input:</em> Real:  1 to 3 values
+<P>
+  <PRE>
+Specify the range coefficients for the CONTINUOUS quadratic transfer function
+that you selected.
+</PRE> 
+               <em>parameter <A HREF="#.halftone">HALFTONE</A> </em>
+<P>
+  <PRE>
+Remember that the data at this point have been normalised to the range [0,1].
+You may specify 5 values, of which the first three are REQUIRED:
+</PRE>
+<P>
+  <PRE>
+        m,M     Range of normalised data values to be represented by the full
+                 halftone range. Values outside this range will be truncated.
+        a,b,c   The 0-th through 2nd-order coefficients in the transfer
+                 quadratic.
+</PRE>
+<P>
+  <PRE>
+The result will be ('ndv' = normalised data value):
+</PRE>
+<P>
+  <PRE>
+        ndv < m:         OUT = 0                         (white)
+        m < ndv < M:     OUT = a + b*IN + c*IN*IN        (grey scale)
+        ndv > M:         OUT = 1                         (black)
+</PRE>
+<P>
+  <PRE>
+You may break the IN range up into partial ranges by specifying multiple sets
+of m,M,a,b,c separated by semicolons, or specifying the sets one by one as the
+prompt is repeated. Input will be considered complete when you give no new
+reply.
+</PRE>
+<P>
+  <PRE>
+Examples:
+        standard linear, halftone=ndv:  0,1, 0,1
+        ndv distance from .5:           0,.5, 1,-2; .5,1, -1,2
+        four grey levels:               0,.25,0; .25,.5,.25; .5,.75,.5; .75,1,1
+        an approximation to an exp
+         that seeks to match the
+         quasi-logarithic response
+         of the human eye:              0,1, 0,.1,.9
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nscan/nscan__arc_option.html b/nscan/nscan__arc_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..3d4e0f66f588b089cebca20cda47b9c3da28509d
--- /dev/null
+++ b/nscan/nscan__arc_option.html
@@ -0,0 +1,17 @@
+<TITLE>Description of ARC_OPTION (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword ARC_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> ARC Action CHECK, ARCHIVE
+<DT><EM>Expected input:</EM> Character(24).<P>
+Checking in a WSRT tape has two phases. In the first phase, the ARC option 
+CHECK is used to verify the general integrity of the tape. The tape is listed 
+and all blocks are read. In the second phase labels are copied to the archive 
+medium (with the DUMP option) and the Scissor database is updated through ARC 
+option ARCHIVE. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__bitpix.html b/nscan/nscan__bitpix.html
new file mode 100644
index 0000000000000000000000000000000000000000..bd0d3757cd9b6f70e70319ab79667bcef6019998
--- /dev/null
+++ b/nscan/nscan__bitpix.html
@@ -0,0 +1,18 @@
+<TITLE>Description of BITPIX (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword BITPIX</H1> 
+
+<DT><EM>Prompt:</EM> Precision for writing UVFITS output
+<DT><EM>Default:</EM> 16.
+<DT><EM>Expected input:</EM> Integer number, 1 values.<P>
+Specify the precision for writing UVFITS data. <P>
+   16     2 bytes integers 
+   32     4 bytes integers 
+
+<DT>  -32     IEEE Floating point values (not yet supported) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__channels.html b/nscan/nscan__channels.html
new file mode 100644
index 0000000000000000000000000000000000000000..4c62fea691e53e61dfa73727779632bd4df6fd95
--- /dev/null
+++ b/nscan/nscan__channels.html
@@ -0,0 +1,23 @@
+<TITLE>Description of CHANNELS (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword CHANNELS</H1> 
+
+<DT><EM>Prompt:</EM> frequency channel number(s)
+<DT><EM>Expected input:</EM> Integer number, 512 values.<P>
+Select the frequency channels/bands to be included. NOTE that the WSRT 
+continuum channel (i.e. the sum of all channels) always has number 0 <P>
+   '*' selects all channels <P>
+   '&lt;begin&gt; TO &lt;end&gt;&gt; BY &lt;step&gt;' selects channels &lt;begin&gt;, &lt;begin&gt;+&lt;step&gt;, ... 
+        up to &lt;end&gt;. The 'BY &lt;step&gt;' part may be omitted. 
+   BEWARE: The notation &lt;begin&gt;-&lt;end&gt;:&lt;step&gt; will be interpreted as an 
+        expression and give incorrect results <P>
+Each of the selected channels will be stored in the .SCN file as a separate 
+'channel' (chn) under the current 'group', 'observation' and 'field' 
+grp.obs.fld. (Remember that .SCN file 'sectors' are identified by indices 
+grp.obs.fld.chn.seq).  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__hab_offset.html b/nscan/nscan__hab_offset.html
new file mode 100644
index 0000000000000000000000000000000000000000..d7f8267088d25ffc91676f6b17c253bb5092fe08
--- /dev/null
+++ b/nscan/nscan__hab_offset.html
@@ -0,0 +1,19 @@
+<TITLE>Description of HAB_OFFSET (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword HAB_OFFSET</H1> 
+
+<DT><EM>Prompt:</EM> Start-offset (sec)
+<DT><EM>Expected input:</EM> Real number.<P>
+Specify the time-offset from the start of an observation, at which the 
+integration for the output scans should start. Example: an offset of n will 
+throw away the first n (rounded up to a multiple of 10) seconds of data. <P>
+NOTE: This feature was useful in early mosaic experiments in which the slewing 
+between fields occurred in the first integration interval(s) on the new field. 
+It is now standard practice to slew during the final integration interval on 
+the old source.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__iat_utc.html b/nscan/nscan__iat_utc.html
new file mode 100644
index 0000000000000000000000000000000000000000..45315178aa2741e622d0c3b199452bbf32c612dd
--- /dev/null
+++ b/nscan/nscan__iat_utc.html
@@ -0,0 +1,17 @@
+<TITLE>Description of IAT_UTC (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword IAT_UTC</H1> 
+
+<DT><EM>Prompt:</EM> MJD, leap seconds, ...
+<DT><EM>Default:</EM> 48257, 26, 900000, 27, 900000, 27, 900000, 27, 900000, 27,                 900000, 27, 900000, 27, 900000, 27, 900000, 27, 900000, 27 /NOASK.
+<DT><EM>Expected input:</EM> Real number, 20 values.<P>
+Specify the IAT-UTC values as pair(s) of numbers: <P>
+   MJD at which the leap seconds occur 
+   The total number of leap seconds as from that date. <P>
+The first value is for 1 Jan 1991. Values before that are known by the program. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__ifsets.html b/nscan/nscan__ifsets.html
new file mode 100644
index 0000000000000000000000000000000000000000..6fad1dfc124a8e79004a886c62119acb3ae844c4
--- /dev/null
+++ b/nscan/nscan__ifsets.html
@@ -0,0 +1,13 @@
+<TITLE>Description of IFSETS (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword IFSETS</H1> 
+
+<DT><EM>Prompt:</EM> integration time for total-power data
+<DT><EM>Expected input:</EM> Integer number; min.value: 0.000000; max.value: 3600.000000.<P>
+Specify the desired integration time for IF sets with Total Power data. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__input_file.html b/nscan/nscan__input_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..a9bce045adc818ae4dcea8d8850c3935432a830d
--- /dev/null
+++ b/nscan/nscan__input_file.html
@@ -0,0 +1,17 @@
+<TITLE>Description of INPUT_FILE (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword INPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> input filename
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the input disk-file name. <P>
+For the NSCAN LOAD-from-disk option, or for the NSCAN PFITS option, don't 
+specify a file extension: it will be made by the program on the basis of the 
+tape label number. <P>
+In the case of other NSCAN options, give the full file name. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__input_labels.html b/nscan/nscan__input_labels.html
new file mode 100644
index 0000000000000000000000000000000000000000..408c6ac34eb46d6009d6d32ba1f693d3a81000dc
--- /dev/null
+++ b/nscan/nscan__input_labels.html
@@ -0,0 +1,24 @@
+<TITLE>Description of INPUT_LABELS (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword INPUT_LABELS</H1> 
+
+<DT><EM>Prompt:</EM> input tape labels
+<DT><EM>Expected input:</EM> Integer number, 256 values.<P>
+Specify the tape labels to be read. <P>
+   '*' selects all labels <P>
+   '&lt;begin&gt; TO &lt;end&gt;&gt; BY &lt;step&gt;' selects labels &lt;begin&gt;, &lt;begin&gt;+&lt;step&gt;, ... 
+        up to &lt;end&gt;. The 'BY &lt;step&gt;' part may be omitted. 
+   BEWARE: The notation &lt;begin&gt;-&lt;end&gt;:&lt;step&gt; will be interpreted as an 
+        expression and give incorrect results <P>
+Each of the selected labels will be stored in the .SCN file as a separate 
+'observation' (obs) in the current 'group' grp. (Remember that .SCN file 
+'sectors' are identified by indices grp.obs.fld.chn.seq). <P>
+Example: 
+        If the current group nr is &lt;g&gt;, the selected input labels will be 
+stored sequentially in the .SCN file as observations &lt;g&gt;.0, &lt;g&gt;.1, &lt;g&gt;.2  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__integration_time.html b/nscan/nscan__integration_time.html
new file mode 100644
index 0000000000000000000000000000000000000000..8fc9fa69282fe63ea657ad8b19dea65ae59a3c5c
--- /dev/null
+++ b/nscan/nscan__integration_time.html
@@ -0,0 +1,37 @@
+<TITLE>Description of INTEGRATION_TIME (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword INTEGRATION_TIME</H1> 
+
+<DT><EM>Prompt:</EM> integration time (sec)
+<DT><EM>Default:</EM> 120.
+<DT><EM>Expected input:</EM> Integer number; min.value: 10.000000; max.value: 3600.000000.<P>
+Specify the desired integration time per output scan in seconds. <P>
+120 sec is a good default; a lower value should be selected if visibilities 
+vary rapidly as a consequence of the source distribution in the observed field,  
+atmospheric conditions or interference. <P>
+For standard observations, the number must be a multiple of the basic 
+integration time used for the observation (which is some multiple of 10 sec). <P>
+In WSRT mosaic observations, slewing occurs in the last 10 sec of the dwell 
+time on each subfield. The integration time you specify must therefore at most 
+be &lt;dwell time&gt; minus 10 sec. You may also use a submultiple of this value 
+without losing data. <P>
+    Example: 
+        If the dwell time is 90 sec, there is 80 sec of valid data. HA_INT = 80,  
+    40, 20 or 10 will use it all. However, HA_INT = 30 or 60 will result in the 
+    loss of the last 20 sec. <P>
+        The volume of your data in the .SCN depends primarily on the 
+integration time. For each integration interval a 'scan' is created which 
+consists of <P>
+        &lt;nr of polarisations&gt; * &lt;nr of interferometers&gt; * 12 + 1024 bytes <P>
+Model visibilities which may be added later will occupy another <P>
+        4 * &lt;nr of interferometers&gt; * 12 bytes .                 NOTE: 
+        The WSRT runs on Universal Time; the quantum of integration time is 
+therefore 10 UT seconds, and a full 12-sidereal-hour observation contains 
+somewhat less than 12*360 of these quanta. You can mostly ignore this subtlety,  
+but the difference may be of practical importance in some situations.   <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__ngle for atnf.html b/nscan/nscan__ngle for atnf.html
new file mode 100644
index 0000000000000000000000000000000000000000..b5c27c3bb303820cb09be504289e9c370e1a34d6
--- /dev/null
+++ b/nscan/nscan__ngle for atnf.html	
@@ -0,0 +1,14 @@
+<TITLE>Description of ngle for ATNF (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword ngle for ATNF</H1> 
+
+<DT><EM>Prompt:</EM> Which type tape WSRT, LEIDEN
+<DT><EM>Expected input:</EM> Character(6).<P>
+Specify the type of the tape. <P>
+Currently we support two types: WSRT and LEIDEN. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__old_dattyp.html b/nscan/nscan__old_dattyp.html
new file mode 100644
index 0000000000000000000000000000000000000000..5c23ec9239e41c24f5c4055a0ba7fd36e72bc9bb
--- /dev/null
+++ b/nscan/nscan__old_dattyp.html
@@ -0,0 +1,22 @@
+<TITLE>Description of OLD_DATTYP (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword OLD_DATTYP</H1> 
+
+<DT><EM>Prompt:</EM> Old R-series data format
+<DT><EM>Expected input:</EM> Integer number.<P>
+Specify the old R-series data type: <P>
+        0= local 
+        1= VAX, D_FORMAT 
+        2= VAX, G_FORMAT 
+        3= ALLIANT 
+        4= CONVEX 
+        5= IEEE 
+        6= DEC station 
+        7= SUN station 
+        8= HP  station <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__option.html b/nscan/nscan__option.html
new file mode 100644
index 0000000000000000000000000000000000000000..1ce4bbabde0cd39d47b9e71a3f01acdbc05867d6
--- /dev/null
+++ b/nscan/nscan__option.html
@@ -0,0 +1,55 @@
+<TITLE>Description of OPTION (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword OPTION</H1> 
+
+<DT><EM>Prompt:</EM> Action QUIT; LOAD, IFLOAD, LEIDEN, LIST, ARC, DUMP; UVFITS, PFITS; | -SHOW; [CVX, NVS, NOPT; REGROUP; FROM_OLD, WERR, AERR, VFIX]
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify the action to be performed by the program NSCAN: <P>
+   Operations on WSRT 'circle' observation files (on classical, DAT or Exabyte 
+   tape, magnetic or optical disk): <P>
+        LOAD     transfer observed visibilities into a .SCN file. 
+        IFLOAD   same, but also transfer the 'IF' data (total powers etc). The 
+                  extra data will enlarge the .SCN file by some 30%; you need 
+                  them only if you suspect that the on-line gain calibration has 
+                  been incorrect. 
+        LEIDEN   transfer observed visibilities from standard LEIDEN file into a 
+                  .SCN file 
+        LIST     show contents of selected labels 
+        ARC      as list, but update the Scissor database if at NFRA 
+        DUMP     copy selected label(s) byte for byte into a disk file <P>
+   Conversion to and listing of data in FITS format <P>
+        UVFITS   convert .SCN file to UVFITS tape/disk file for use in AIPS 
+        PFITS    print AIPS-like FITS info (but also other) from UVFITS file 
+                   header <P>
+   Display and editing of .SCN files: <P>
+        SHOW     show/edit data and header information in .SCN file. (This 
+                   option is duplicated in NFLAG.) <P>
+   Utilities: <P>
+        QUIT     leave the program NSCAN <P>
+        CVX      convert a .SCN file from other machine's number format 
+        NVS      convert a .SCN file to newest version. Needs only to be run if 
+                   programs report that the data has the wrong version 
+
+<DT>                  - calculates parallactic angle for ATNF 
+        NOPT     update contents of sector/scan headers and polarisation format 
+                  of visibility data: 
+
+<DT>                   - convert input data in Stokes parameter format to XX format 
+
+<DT>                   - calculate UT start 
+
+<DT>                   - calculate precession rotation angle if not filled 
+
+<DT>                   - recalculate MJD for observations aborted at Wbork 
+        REGROUP  create a second index for each of one or more sets of sector.! <P>
+   One-time fixes: <P>
+        FROM_OLD convert old (R-series) uv-data file into NEWSTAR .SCN file 
+        WERR     correct one-time mosaic WSRT tape errors (1991 data only) 
+        AERR     change sign of phases 
+        VFIX     recalculate velocities <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__output_file.html b/nscan/nscan__output_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..14f9b2bb890e76e0c10a9359bb63d4d48e9428ff
--- /dev/null
+++ b/nscan/nscan__output_file.html
@@ -0,0 +1,16 @@
+<TITLE>Description of OUTPUT_FILE (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword OUTPUT_FILE</H1> 
+
+<DT><EM>Prompt:</EM> output filename
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the full name for the output disk file. <P>
+For the NSCAN DUMP option, don't specify a file extension: it will be made by 
+the program on the basis of the label number. <P>
+For the other NSCAN options, specify a full file-name. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__output_label.html b/nscan/nscan__output_label.html
new file mode 100644
index 0000000000000000000000000000000000000000..1a2a13c538c52df0c54059c513b10e5cd3087279
--- /dev/null
+++ b/nscan/nscan__output_label.html
@@ -0,0 +1,14 @@
+<TITLE>Description of OUTPUT_LABEL (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword OUTPUT_LABEL</H1> 
+
+<DT><EM>Prompt:</EM> output tape label
+<DT><EM>Expected input:</EM> Integer number.<P>
+ Specify the first output tape label. 
+* or 0 indicates the end of the tape (i.e. append the new labels at the end). <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__pointing_sets.html b/nscan/nscan__pointing_sets.html
new file mode 100644
index 0000000000000000000000000000000000000000..75af02294d6b77a4e44fab3fb4f09605b210f946
--- /dev/null
+++ b/nscan/nscan__pointing_sets.html
@@ -0,0 +1,31 @@
+<TITLE>Description of POINTING_SETS (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword POINTING_SETS</H1> 
+
+<DT><EM>Prompt:</EM> Mosaic field sequence number(s)
+<DT><EM>Expected input:</EM> Integer number, 512 values.<P>
+ Select the SEQUENCE numbers of the fields (= mosaic 'pointing 
+centres') to be selected. (see Note below). <P>
+NOTE that WSRT mosaic fields are numbered starting at 1 <P>
+   '*' selects all fields <P>
+   '&lt;begin&gt; TO &lt;end&gt;&gt; BY &lt;step&gt;' selects fields &lt;begin&gt;, &lt;begin&gt;+&lt;step&gt;, ... 
+        up to &lt;end&gt;. The 'BY &lt;step&gt;' part may be omitted. 
+   BEWARE: The notation &lt;begin&gt;-&lt;end&gt;:&lt;step&gt; will be interpreted as an 
+        expression and give incorrect results <P>
+Each of the selected fields will be stored in the .SCN file as a separate 
+'field' (fld) under the current 'group' and 'observation' grp.obs. (Remember 
+that .SCN file 'sectors' are identified by indices grp.obs.fld.chn.seq). <P>
+NOTE: 
+        The numbers you specify refer to the SEQUENCE (starting with 0) in 
+which the mosaic fields aqppear on the tape. Normally, an observation starts 
+with field 0 and the sequence numbers equal the field numbers. However, if your 
+observation starts 'somehere in the middle', this is no longer the case and you 
+must be careful in selecting your fields. Example: <P>
+        Your observation starts at field 19. To select fields 19 through 24,  
+specify POINTING_SETS= 0 TO 5.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__scn_set_pattern.html b/nscan/nscan__scn_set_pattern.html
new file mode 100644
index 0000000000000000000000000000000000000000..8d0cc6d334e3b8e67dd0a57d385f694585da07cd
--- /dev/null
+++ b/nscan/nscan__scn_set_pattern.html
@@ -0,0 +1,21 @@
+<TITLE>Description of SCN_SET_PATTERN (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword SCN_SET_PATTERN</H1> 
+
+<DT><EM>Prompt:</EM> new index pattern (grp.obs.fld.chn.seq)
+<DT><EM>Expected input:</EM> Character(32), 1 values.<P>
+Specify a new index pattern (group.observation.field.channel.sequence_number) 
+into which to change the index pattern of the input Set of uv-data Sectors. <P>
+Each index in the pattern that contains an * is copied from the input Set. 
+Other fields are used as is (true for the first four fields, i.e. 
+grp.obs.fld.chn.) <P>
+Example: To change the indices of the Set 
+        0.*.15283.* to 
+        0.*.0    .* <P>
+give the first selection as the input Set, and the second as the pattern. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__select_iqxy.html b/nscan/nscan__select_iqxy.html
new file mode 100644
index 0000000000000000000000000000000000000000..46d17f8871894e3ac89c62870a219fa8db2ebb70
--- /dev/null
+++ b/nscan/nscan__select_iqxy.html
@@ -0,0 +1,27 @@
+<TITLE>Description of SELECT_IQXY (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword SELECT_IQXY</H1> 
+
+<DT><EM>Prompt:</EM> output polarisations (ONE 'value') |  I, Q, U, V, IQ, UV, IQUV, X, XXY, YYX, Y, XY, YX, XYX
+<DT><EM>Expected input:</EM> Character(4).<P>
+Specify the polarisation(s) to be written: <P>
+        I:      I only 
+        Q:      Q only 
+        U:      U only 
+        V:      V only <P>
+        IQ:     I and Q 
+        UV:     U and V 
+        IQUV:   I, Q, U and V <P>
+        X:      XX only 
+        XXY:    XY only 
+        YYX:    YX only 
+        Y:      YY only <P>
+        XY:     XX and YY 
+        YX:     XY and YX 
+        XYX:    all four: XX, XY, YX, YY <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__type_tape.html b/nscan/nscan__type_tape.html
new file mode 100644
index 0000000000000000000000000000000000000000..b00e878a9c1db8c4de533c6d44dfe3d65c3afb39
--- /dev/null
+++ b/nscan/nscan__type_tape.html
@@ -0,0 +1,14 @@
+<TITLE>Description of TYPE_TAPE (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword TYPE_TAPE</H1> 
+
+<DT><EM>Prompt:</EM> Which type tape WSRT, LEIDEN
+<DT><EM>Expected input:</EM> Character(6).<P>
+Specify the type of the tape. <P>
+Currently we support two types: WSRT and LEIDEN. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__werr_ha.html b/nscan/nscan__werr_ha.html
new file mode 100644
index 0000000000000000000000000000000000000000..e614ded991938dae8514b3b4ec03791a53e2ed42
--- /dev/null
+++ b/nscan/nscan__werr_ha.html
@@ -0,0 +1,15 @@
+<TITLE>Description of WERR_HA (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword WERR_HA</H1> 
+
+<DT><EM>Prompt:</EM> Hour-angle correction (deg)
+<DT><EM>Expected input:</EM> Double precision number in DEG, RAD, CIR, HMS.<P>
+Specify the angle to be added to all hour angles in the .SCN file <P>
+NOTE: This is a special feature to be used only to correct errors made in the 
+on-line observation.  <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__werr_option.html b/nscan/nscan__werr_option.html
new file mode 100644
index 0000000000000000000000000000000000000000..43485d6de1267acd66d8d9f60276cf49067d8fb1
--- /dev/null
+++ b/nscan/nscan__werr_option.html
@@ -0,0 +1,17 @@
+<TITLE>Description of WERR_OPTION (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword WERR_OPTION</H1> 
+
+<DT><EM>Prompt:</EM> WERR action WE0, WE1; QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify correction to be performed: <P>
+   WE0:   correct Hour angles for tape error in splitted mosaic tapes before 
+           online version 62 
+   WE1:   correct all Hour angles with a constant offset 
+   QUIT:  no more <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nscan/nscan__werr_ra.html b/nscan/nscan__werr_ra.html
new file mode 100644
index 0000000000000000000000000000000000000000..5100357c9bcffb5d3fe875b7b6b0a2ceab5b2991
--- /dev/null
+++ b/nscan/nscan__werr_ra.html
@@ -0,0 +1,13 @@
+<TITLE>Description of WERR_RA (NSCAN)</TITLE>
+<H1>Program NSCAN: private keyword WERR_RA</H1> 
+
+<DT><EM>Prompt:</EM> RA of mosaic centre
+<DT><EM>Expected input:</EM> Double precision number in DEG, RAD, CIR, HMS.<P>
+Specify the Right Ascension of the centre of the mosaic area <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nscan/nscan_keys.html">List of keywords</A> for NSCAN
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
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new file mode 100644
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x0e,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/nscan_descr/_11156_tabbing135.png b/nscan_descr/_11156_tabbing135.png
new file mode 100644
index 0000000000000000000000000000000000000000..527b49d75fa4b6fdaf7efcfd2f320c3019a89ad5
Binary files /dev/null and b/nscan_descr/_11156_tabbing135.png differ
diff --git a/nscan_descr/_11156_tabbing135.xbm b/nscan_descr/_11156_tabbing135.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5e146a603c534659dcfc5c7bcb02d3cfc8b352d5
--- /dev/null
+++ b/nscan_descr/_11156_tabbing135.xbm
@@ -0,0 +1,293 @@
+#define noname_width 546
+#define noname_height 63
+static char noname_bits[] = {
+ 0xff,0x01,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x38,0x1e,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x00,0x80,0x03,0x00,0x00,0x00,0x38,0xc0,0x00,0x33,0x01,0x00,0x00,0x70,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x07,0x80,0x03,0xe0,0x00,0xf8,0x38,0x00,0x1c,0x00,
+ 0x0c,0x06,0x80,0x03,0xf0,0x01,0x00,0x1c,0x00,0x0c,0x80,0x03,0xe0,0xe3,0x00,
+ 0x70,0x00,0x30,0x18,0x00,0x0e,0xc0,0x07,0x00,0x00,0x00,0x00,0x70,0x0c,0x80,
+ 0x00,0x00,0x00,0x00,0x08,0x03,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x30,0x60,0x03,0x31,0x03,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x80,0x0f,
+ 0xc0,0x07,0xf0,0x01,0xf8,0x7c,0x00,0x3e,0x00,0x1e,0x07,0xc0,0x07,0xf0,0x01,
+ 0x00,0x3e,0x00,0x0c,0xc0,0x07,0xe0,0xf3,0x01,0xf8,0x00,0x78,0x1c,0x00,0x1f,
+ 0xc0,0x07,0x00,0x00,0x00,0x00,0xf0,0x08,0xc0,0x00,0x00,0x00,0x00,0x0c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x30,0x20,0x03,0x31,0x02,0x00,
+ 0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x80,0x0d,0xc0,0x06,0xb0,0x01,0x08,0x66,
+ 0x00,0x36,0x00,0x1b,0x07,0xc0,0x06,0x10,0x00,0x00,0x36,0x00,0x0f,0xc0,0x06,
+ 0x20,0x98,0x01,0xd8,0x00,0x6c,0x1c,0x00,0x1b,0x40,0x00,0x00,0x00,0x00,0x00,
+ 0xd0,0x09,0xc0,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x03,
+ 0x00,0x00,0x00,0x30,0x30,0x02,0x30,0x3c,0x3f,0x1e,0x40,0x18,0x00,0x00,0x00,
+ 0x00,0xc0,0x18,0x60,0x0c,0x18,0x03,0x08,0xc6,0x00,0x63,0x80,0x8f,0x05,0x60,
+ 0x0c,0x10,0x00,0x00,0x63,0x00,0x0f,0x60,0x0c,0x20,0x18,0x03,0x8c,0x01,0x3e,
+ 0x16,0x80,0x31,0x40,0x00,0x00,0x00,0x00,0x00,0x90,0x89,0xef,0x79,0xc0,0xf7,
+ 0xfd,0x9e,0xfb,0xdd,0xdc,0xfe,0x07,0x7c,0x1f,0xcf,0xef,0xc7,0x33,0x30,0x02,
+ 0x30,0x6c,0x66,0x33,0x40,0x18,0x00,0x00,0x00,0x00,0xc0,0x18,0x60,0x0c,0x18,
+ 0xfb,0xfb,0xee,0x00,0xe3,0xbf,0xdf,0x05,0x60,0xfc,0xf7,0x01,0x00,0x63,0x00,
+ 0x0c,0x60,0xec,0xef,0xbb,0x03,0x8c,0xff,0x7e,0x17,0x80,0xf1,0xdf,0x07,0x00,
+ 0x00,0x00,0x00,0x90,0xcb,0xc8,0xcc,0x60,0x1e,0x99,0x0c,0x33,0x99,0x98,0xcc,
+ 0x0c,0x66,0x13,0x9b,0xc9,0x64,0x36,0x30,0x02,0x30,0x78,0x46,0x3f,0x40,0x00,
+ 0x00,0x00,0x00,0x00,0xc0,0x18,0x60,0x0c,0x18,0xfb,0xdb,0xfd,0x00,0xe3,0xbf,
+ 0xf1,0x1f,0x60,0xfc,0xb7,0x03,0x00,0x63,0x00,0x0c,0x60,0xec,0x6f,0xf7,0x03,
+ 0x8c,0xff,0xc6,0x7f,0x80,0xf1,0xdf,0x0e,0x00,0x00,0x00,0x00,0x10,0xcf,0xd8,
+ 0xfc,0x60,0x18,0x9b,0x0c,0x33,0x99,0x98,0xcc,0x0c,0x06,0x13,0x9e,0xc9,0xe4,
+ 0x37,0x30,0x02,0x30,0x6c,0x46,0x03,0x40,0x00,0x00,0x00,0x00,0x00,0xc0,0x18,
+ 0x60,0x0c,0x18,0x03,0x8c,0x45,0x00,0x63,0x80,0xf1,0x1f,0x60,0x0c,0x18,0x03,
+ 0x00,0x63,0x00,0x0c,0x60,0x0c,0x30,0x16,0x01,0x8c,0x01,0xc6,0x7f,0x80,0x31,
+ 0x60,0x0c,0x00,0x00,0x00,0x00,0x10,0xce,0xd8,0x0e,0x60,0x18,0x9b,0x2c,0x33,
+ 0x99,0x98,0xcc,0x0c,0x06,0x13,0x9b,0xc9,0x64,0x30,0x30,0x02,0x30,0xe6,0x66,
+ 0x23,0x40,0x18,0x00,0x00,0x00,0x00,0x80,0x8d,0xc3,0xc6,0xb1,0x01,0xdc,0x7d,
+ 0x38,0x36,0x00,0x3b,0x84,0xc3,0x06,0xb8,0xe3,0x00,0x36,0x0e,0x0c,0xc7,0x06,
+ 0x70,0xf7,0xe1,0xd8,0x00,0xec,0x10,0x0e,0x1b,0xe0,0x0e,0x00,0x00,0x00,0x00,
+ 0x10,0xce,0xc8,0x8e,0x60,0x1c,0x99,0x2c,0x33,0xd9,0xd8,0xcc,0x0c,0x46,0x93,
+ 0xb9,0xc9,0x64,0x34,0x20,0x03,0xfc,0xfc,0x3e,0x1e,0xf0,0x19,0x00,0x00,0x00,
+ 0x00,0x80,0x8f,0xc3,0xc7,0xf1,0x01,0xf8,0x3c,0x38,0x3e,0x00,0x1f,0x9f,0xc3,
+ 0x07,0xf0,0xe1,0x00,0x3e,0x0e,0x1f,0xc7,0x07,0xe0,0xf3,0xe0,0xf8,0x00,0x7c,
+ 0x7c,0x0e,0x1f,0xc0,0x07,0x00,0x00,0x00,0x00,0x78,0x8c,0xcf,0x7b,0xc0,0xf3,
+ 0xfd,0xbd,0xff,0xfb,0xf9,0xff,0x1f,0xbc,0x3f,0xff,0xff,0xcf,0x7b,0x60,0x03,
+ 0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x01,0x00,0x00,0x06,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xff,0x01,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x33,0x01,0x00,
+ 0x00,0xb0,0x01,0x00,0x00,0x00,0x00,0x00,0x06,0x80,0x03,0xe0,0xe0,0x00,0x7c,
+ 0x38,0x00,0x0e,0x00,0x06,0x03,0xc0,0x01,0xc0,0x60,0x00,0x00,0x0c,0x00,0x03,
+ 0xc0,0x01,0xe0,0x70,0x00,0x38,0x00,0x0c,0x0c,0x80,0x03,0x80,0xc1,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x31,0x03,0x00,0x00,0xb8,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x06,0xc0,0x07,0xf0,0xf1,0x01,0x7c,0x7c,0x00,0x1f,0x00,0x8f,0x03,
+ 0xe0,0x03,0xc0,0x60,0x00,0x00,0x0c,0x00,0x03,0xe0,0x03,0xf0,0xf9,0x00,0x7c,
+ 0x00,0x1e,0x0e,0xc0,0x07,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x31,0x02,0x00,0x00,0x38,0x01,0x00,0x00,0x00,0x00,0x80,0x07,0xc0,0x06,0x30,
+ 0xb1,0x01,0x04,0x66,0x00,0x1b,0x80,0x8d,0x03,0x60,0x03,0xf0,0x78,0x00,0x00,
+ 0x0f,0xc0,0x03,0x60,0x03,0x18,0xcf,0x00,0x6c,0x00,0x1b,0x0e,0xc0,0x06,0xe0,
+ 0xf1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x3c,0x3f,0x1e,0x80,0x19,
+ 0x00,0x00,0x00,0x00,0x80,0x07,0x60,0x0c,0x80,0x19,0x03,0x04,0xc6,0x80,0x31,
+ 0xc0,0xc7,0x02,0x30,0x06,0xf0,0x78,0x00,0x00,0x0f,0xc0,0x03,0x30,0x06,0x10,
+ 0x8f,0x01,0xc6,0x80,0x0f,0x0b,0x60,0x0c,0xe0,0xf1,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0x6c,0x66,0x33,0x80,0x19,0x00,0x00,0x00,0x00,0x00,0x06,
+ 0x60,0x0c,0xe0,0x19,0xff,0x7d,0xee,0x80,0xb1,0xff,0xef,0x02,0x30,0xfe,0xc3,
+ 0x60,0x00,0x00,0x0c,0x00,0x03,0x30,0xfe,0x83,0xdd,0x01,0xc6,0xff,0x9f,0x0b,
+ 0x60,0xec,0x8f,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x78,0x46,
+ 0x3f,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x60,0x0c,0x80,0x19,0xff,0xed,
+ 0xfc,0x80,0xb1,0xff,0xf8,0x0f,0x30,0xfe,0xc3,0x60,0x00,0x00,0x0c,0x00,0x03,
+ 0x30,0xfe,0xc3,0xf9,0x01,0xc6,0xff,0xb1,0x3f,0x60,0xec,0x8f,0xc1,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x6c,0x46,0x03,0x60,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x06,0x60,0x0c,0x10,0x1b,0x03,0xc6,0x44,0x80,0x31,0xc0,0xf8,0x0f,
+ 0x30,0x06,0xc0,0x60,0x00,0x00,0x0c,0x00,0x03,0x30,0x06,0xe0,0x88,0x00,0xc6,
+ 0x80,0xb1,0x3f,0x60,0x0c,0x80,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x31,0x02,0x00,
+ 0x00,0xe0,0x00,0x00,0x00,0x00,0x00,0x80,0x09,0xc0,0x06,0xb0,0x01,0x08,0x66,
+ 0x00,0x36,0x00,0x1b,0x07,0xc0,0x06,0xf0,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x3c,0x3f,0x1e,0xb0,0x18,0x00,0x00,0x00,
+ 0x00,0x00,0x0c,0x60,0x0c,0x18,0x03,0x08,0xc6,0x00,0x63,0x80,0x8f,0x05,0x60,
+ 0x0c,0xf0,0xf0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x30,0x6c,0x66,0x33,0x90,0x18,0x00,0x00,0x00,0x00,0x00,0x0f,0x60,0x0c,0x18,
+ 0xfb,0xfb,0xee,0x00,0xe3,0xbf,0xdf,0x05,0x60,0xfc,0xc7,0xc0,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x78,0x46,0x3f,0x98,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x0c,0x60,0x0c,0x18,0xfb,0xdb,0xfd,0x00,0xe3,0xbf,
+ 0xf1,0x1f,0x60,0xfc,0xc7,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0x6c,0x46,0x03,0xf8,0x03,0x00,0x00,0x00,0x00,0x80,0x18,
+ 0x60,0x0c,0x18,0x03,0x8c,0x45,0x00,0x63,0x80,0xf1,0x1f,0x60,0x0c,0xc0,0xc0,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xe6,0x66,
+ 0x23,0x80,0x18,0x00,0x00,0x00,0x00,0xc0,0x9d,0xc3,0xc6,0xb1,0x01,0xdc,0x7d,
+ 0x38,0x36,0x00,0x3b,0x84,0xc3,0x06,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xfc,0xfc,0x3e,0x1e,0xe0,0x1b,0x00,0x00,0x00,
+ 0x00,0x80,0x8f,0xc3,0xc7,0xf1,0x01,0xf8,0x3c,0x38,0x3e,0x00,0x1f,0x9f,0xc3,
+ 0x07,0xf0,0xf1,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/nscan_descr/images.pl b/nscan_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..be7b7652a91ca0de9e4dbcaf067c78b4407fb405
--- /dev/null
+++ b/nscan_descr/images.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{tabbing}+++++=++++++++=++++++++=+++++=+++++=+++++=+++++=+++++=+++++=kill>Tape1:><<136>>tt0.0.0-59.0-64.0-5,0.1.0-59.0-64.0-5<<136>>>>>>>Notecontinuumchannel0>Tape2:><<137>>tt1.0.30-59.0-64.0-11,1.1.0-29.0-64.0-11<<137>>>Tape3:><<138>>tt2.0.0-59.0-64.0-11<<138>>>Tape4:><<139>>tt3.0.0-59.0-64.0-11<<139>>{tabbing}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11156_tabbing135.xbm">'; 
+$key = q/{tabbing}+++++=++++++++=++++++++=+++++=+++++=+++++=+++++=+++++=+++++=kill>Tape1:>label1:>6hours,spacing9Ais36m>>label2:>6hours,36m>Tape2:>label1:>12hoursforfields30-59,72m>>label2:>12hoursforfields0-29,72m>Tape3:>label1:>12hoursallfieldsfor48m>Tape4:>label1:>12hoursallfieldsfor90m{tabbing}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11156_tabbing131.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/nscan_descr/labels.pl b/nscan_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..734274a621d79a3e7fe933217703566da71a7588
--- /dev/null
+++ b/nscan_descr/labels.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"nscan.descr.load"} ="$URL/nscan_descr.html"; 
+$external_labels{"nscan.descr.options"} ="$URL/nscan_descr.html"; 
+$external_labels{".contents"} ="$URL/nscan_descr.html"; 
+$external_labels{"nscan.descr.delete"} ="$URL/nscan_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/nscan_descr/nscan_descr.html b/nscan_descr/nscan_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..b11314e54d49540c4d4cf65c73da6ef2bd79d12e
--- /dev/null
+++ b/nscan_descr/nscan_descr.html
@@ -0,0 +1,119 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The Program NSCAN</b>  
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nscan_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nscan_descr.html#SECTION0002000000000000000> <b>Overview of NCSAN options</b></A>
+<LI> <A NAME=tex2html3 HREF=nscan_descr.html#SECTION0003000000000000000> <b>Option LOAD</b></A>
+<LI> <A NAME=tex2html4 HREF=nscan_descr.html#SECTION0004000000000000000> <b>Option DELETE</b></A>
+</UL>
+<A NAME=nscan.descr.options><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000> <b>Overview of NCSAN options</b></A></H1>
+<P>
+The program NSCAN allows the user to interact with the uv-data file (SCN-file).  The structure of this file is explained in detail in a separate section of this cookbook. The program NSCAN offers the following main options:
+<P>
+<UL><LI> <b>LOAD:</b>  Load WSRT uv-data (in WSRT circle format) from tape, disk, DAT or optical disk into a SCN-file.  The input may be from multiple tapes and/or labels.  The user may select data, and change the integration time.
+<P>
+<LI> <b>DUMP:</b>  Dump WSRT data (in WSRT circle format) from tape or DAT or optical disk to a disk file (in WSRT circle format).
+<P>
+<LI> <b>FROM_OLD:</b>  Convert an old (R-series format) SCN-file into a <i>NEWSTAR </i> SCN-file.
+<P>
+<LI> <b>TO_OLD:</b>  Convert a <i>NEWSTAR </i> SCN-file into an old (R-series format) SCN-file.
+<P>
+<LI> <b>SHOW:</b>  Show/edit the contents of a SCN-file: layout, header information  (incl corrections), uv-data and uv-model.  This is demonstrated in the section `Description of the SCN-file' in this Cookbook.
+<P>
+<LI> <b>DELETE:</b>  Delete (or un-delete) uv-data in a SCN-file, according to certain selection criteria. Actually, the data is only disabled (flagged) reversibly by making the attached weight-factor negative.
+<P>
+<LI> <b>COPY:</b> (not yet available)  Copy selected Sets from a SCN file to a new (secondary) SCN-file. The uv-data may be physically modified (e.g. corrections, model subtraction, change of integration time) in this process.  This option will probably be implemented in a separate program NCOPY.
+<P>
+<LI> <b>REGROUP:</b>  Select and reorganise the data in a SCN-file.  Make a new group directory entry (job tree) with specified Sets in it.
+<P>
+<LI> <b>UVFITS:</b>  Convert a SCN-file into a UVFITS file (tape/disk) for further image analysis in AIPS.  It is recommended to do all WSRT uv-data processing first in <i>NEWSTAR </i>, since AIPS uv-data processing is rather VLA-oriented, and does not do justice to WSRT data.
+<P>
+<LI> <b>PFITS:</b>  Print a summary of a UVFITS (AIPS) tape/disk file, showing all keywords and a limited set of data.
+<P>
+<LI> <b>CVX:</b>  Convert a SCN file from other machine's format to local machine's.
+<P>
+<LI> <b>NVS:</b>  Convert a SCN file to newest version.  This should be run if SCN file made before the dates:  
+ <BR>910417: add MJD to set header.  
+ <BR>900907: add precession rotation angle.  
+ <BR>900220: add polarisation corrections.  
+ <BR>920828: recalculate MJD for observations aborted at Wbork.
+<P>
+<LI> <b>WERR:</b>  Correct mosaic tape errors. This only concerns mosaic data taken in 1991.
+<P>
+<LI> <b>QUIT:</b>  Exit the program NSCAN  
+</UL>
+<P>
+<A NAME=nscan.descr.load><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>Option LOAD</b></A></H1>
+<P>
+<b>An example:</b>  Let us assume we have a mosaicking observations at 4 settings of ABCD of 60 fields, 64 line channels. There will thus be 12 spokes per 12 hour per field.  These data are on 4 tapes:
+<P>
+                                 <P><IMG ALIGN=BOTTOM ALT="" SRC="_11156_tabbing131.png"><P>
+<P>
+The Set numbers will be unknown, but the indices generated are (if they are read in in order of tape and label):
+<P>
+                                 <P><IMG ALIGN=BOTTOM ALT="" SRC="_11156_tabbing135.png"><P>
+<P>
+If a map is wanted of field 31 using spacings 36 m and 72 m averaging all odd channels between 17 and 25, the data could be specified as:
+<P>
+ <PRE> 
+    0..31.17-25:2,1..31.17-25:2
+or  0-1.*.31.17-25:2 
+</PRE>
+<P>
+<A NAME=nscan.descr.delete><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Option DELETE</b></A></H1>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nscan_keys/nscan_keys.html b/nscan_keys/nscan_keys.html
new file mode 100644
index 0000000000000000000000000000000000000000..f60ae4b7e920e7ca8aca6a7e74993974a045a12d
--- /dev/null
+++ b/nscan_keys/nscan_keys.html
@@ -0,0 +1,100 @@
+<TITLE>Index of private keywords for NSCAN </TITLE>
+<H1>Description of keywords for program NSCAN</H1>
+
+<UL>
+<LI> <A HREF="../nscan/nscan__option.html">
+  OPTION</A>
+  Action QUIT; LOAD, IFLOAD, LEIDEN, LIST, ARC, DUMP; UVFITS, PFITS; | -SHOW; [CVX, NVS, NOPT; REGROUP; FROM_OLD, WERR, AERR, VFIX]
+<LI> <A HREF="../nscan/nscan__type_tape.html">
+  TYPE_TAPE</A>
+  Which type tape WSRT, LEIDEN
+<LI> <A HREF="../nscan/nscan__arc_option.html">
+  ARC_OPTION</A>
+  ARC Action CHECK, ARCHIVE
+<LI> <A HREF="../nscan/nscan__werr_option.html">
+  WERR_OPTION</A>
+  WERR action WE0, WE1; QUIT
+<LI> <A HREF="../nscan/nscan__input_file.html">
+  INPUT_FILE</A>
+  input filename
+<LI> <A HREF="../nscan/nscan__integration_time.html">
+  INTEGRATION_TIME</A>
+  integration time (sec)
+<LI> <A HREF="../nscan/nscan__output_file.html">
+  OUTPUT_FILE</A>
+  output filename
+<LI> <A HREF="../nscan/nscan__input_labels.html">
+  INPUT_LABELS</A>
+  input tape labels
+<LI> <A HREF="../nscan/nscan__output_label.html">
+  OUTPUT_LABEL</A>
+  output tape label
+<LI> <A HREF="../nscan/nscan__pointing_sets.html">
+  POINTING_SETS</A>
+  Mosaic field sequence number(s)
+<LI> <A HREF="../nscan/nscan__channels.html">
+  CHANNELS</A>
+  frequency channel number(s)
+<LI> <A HREF="../nscan/nscan__ifsets.html">
+  IFSETS</A>
+  integration time for total-power data
+<LI> <A HREF="../nscan/nscan__iat_utc.html">
+  IAT_UTC</A>
+  MJD, leap seconds, ...
+<LI> <A HREF="../nscan/nscan__bitpix.html">
+  BITPIX</A>
+  Precision for writing UVFITS output
+<LI> <A HREF="../nscan/nscan__werr_ra.html">
+  WERR_RA</A>
+  RA of mosaic centre
+<LI> <A HREF="../nscan/nscan__werr_ha.html">
+  WERR_HA</A>
+  Hour-angle correction (deg)
+<LI> <A HREF="../nscan/nscan__werr_vel.html">
+  WERR_VEL</A>
+  Reference velocity (m/sec)
+<LI> <A HREF="../nscan/nscan__hab_offset.html">
+  HAB_OFFSET</A>
+  Start-offset (sec)
+<LI> <A HREF="../nscan/nscan__scn_set_pattern.html">
+  SCN_SET_PATTERN</A>
+  new index pattern (grp.obs.fld.chn.seq)
+<LI> <A HREF="../nscan/nscan__old_dattyp.html">
+  OLD_DATTYP</A>
+  Old R-series data format
+<LI> <A HREF="../nscan/nscan__select_iqxy.html">
+  SELECT_IQXY</A>
+  output polarisations (ONE 'value') |  I, Q, U, V, IQ, UV, IQUV, X, XXY, YYX, Y, XY, YX, XYX
+<P>
+
+<UL><LI>See also <A HREF="../nshow_comm/nshow_comm.html">NSHOW</A> </UL>
+
+
+<UL><LI>See also <A HREF="../ngen_comm/ngen_comm.html">NGEN</A> </UL>
+
+
+<UL><LI>See also <A HREF="../unit_comm/unit_comm.html">UNIT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnnode_comm/scnnode_comm.html">SCNNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../scnsets_comm/scnsets_comm.html">SCNSETS</A> </UL>
+
+
+<UL><LI>See also <A HREF="../select_comm/select_comm.html">SELECT</A> </UL>
+
+
+<UL><LI>See also <A HREF="../mdlnode_comm/mdlnode_comm.html">MDLNODE</A> </UL>
+
+
+<UL><LI>See also <A HREF="../nmodel_comm/nmodel_comm.html">NMODEL</A> </UL>
+
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+<LI>Description of <A HREF="../nscan_descr/nscan_descr.html">program NSCAN</A>
+</UL>
diff --git a/nscan_private_intfc.ps b/nscan_private_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..0ee19cfaca150c263a5839df624556af099fb401
--- /dev/null
+++ b/nscan_private_intfc.ps
@@ -0,0 +1,983 @@
+%!PS-Adobe-2.0
+%%Creator: dvipsk 5.66a Copyright 1986-97 Radical Eye Software (www.radicaleye.com)
+%%Title: nscan_private_intfc_tmp.dvi
+%%Pages: 7
+%%PageOrder: Ascend
+%%BoundingBox: 0 0 596 842
+%%EndComments
+%DVIPSCommandLine: dvips -o /newstar/master/hlp/nscan_private_intfc.ps
+%+ nscan_private_intfc_tmp.dvi
+%DVIPSParameters: dpi=300, compressed
+%DVIPSSource:  TeX output 1997.06.13:0925
+%%BeginProcSet: texc.pro
+%!
+/TeXDict 250 dict def TeXDict begin /N{def}def /B{bind def}N /S{exch}N
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+ifelse 0 0 0]concat}if 72 Resolution div 72 VResolution div neg scale
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+TR[matrix currentmatrix{dup dup round sub abs 0.00001 lt{round}if}
+forall round exch round exch]setmatrix}N /@landscape{/isls true N}B
+/@manualfeed{statusdict /manualfeed true put}B /@copies{/#copies X}B
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nscan_private_intfc/images.pl b/nscan_private_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nscan_private_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nscan_private_intfc/labels.pl b/nscan_private_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..76734175830912eaeb06abb5fb85a89cd5410e3e
--- /dev/null
+++ b/nscan_private_intfc/labels.pl
@@ -0,0 +1,28 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".werr.option"} ="$URL/nscan_private_intfc.html"; 
+$external_labels{".public"} ="$URL/nscan_private_intfc.html"; 
+$external_labels{".bitpix"} ="$URL/nscan_private_intfc.html"; 
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+$external_labels{".contents"} ="$URL/nscan_private_intfc.html"; 
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+$external_labels{".hab.offset"} ="$URL/nscan_private_intfc.html"; 
+$external_labels{".old.dattyp"} ="$URL/nscan_private_intfc.html"; 
+$external_labels{".input.labels"} ="$URL/nscan_private_intfc.html"; 
+$external_labels{".type.tape"} ="$URL/nscan_private_intfc.html"; 
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+$external_labels{".select.iqxy"} ="$URL/nscan_private_intfc.html"; 
+$external_labels{".iat.utc"} ="$URL/nscan_private_intfc.html"; 
+
+1;
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new file mode 100644
index 0000000000000000000000000000000000000000..a63af688ed6c4ebe9936b7ae2ce607eebbecf514
--- /dev/null
+++ b/nscan_private_intfc/nscan_private_intfc.html
@@ -0,0 +1,596 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Private parameters for program NSCAN</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nscan_private_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nscan_private_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nscan_private_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nscan_private_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nscan_private_intfc.html#SECTION0003200000000000000>  <b>Parameter ARC_OPTION</b></A>
+<LI> <A NAME=tex2html6 HREF=nscan_private_intfc.html#SECTION0003300000000000000>  <b>Parameter BITPIX</b></A>
+<LI> <A NAME=tex2html7 HREF=nscan_private_intfc.html#SECTION0003400000000000000>  <b>Parameter CHANNELS</b></A>
+<LI> <A NAME=tex2html8 HREF=nscan_private_intfc.html#SECTION0003500000000000000>  <b>Parameter HAB_OFFSET</b></A>
+<LI> <A NAME=tex2html9 HREF=nscan_private_intfc.html#SECTION0003600000000000000>  <b>Parameter IAT_UTC</b></A>
+<LI> <A NAME=tex2html10 HREF=nscan_private_intfc.html#SECTION0003700000000000000>  <b>Parameter IFSETS</b></A>
+<LI> <A NAME=tex2html11 HREF=nscan_private_intfc.html#SECTION0003800000000000000>  <b>Parameter INPUT_FILE</b></A>
+<LI> <A NAME=tex2html12 HREF=nscan_private_intfc.html#SECTION0003900000000000000>  <b>Parameter INPUT_LABELS</b></A>
+<LI> <A NAME=tex2html13 HREF=nscan_private_intfc.html#SECTION00031000000000000000>  <b>Parameter INTEGRATION_TIME</b></A>
+<LI> <A NAME=tex2html14 HREF=nscan_private_intfc.html#SECTION00031100000000000000>  <b>Parameter OLD_DATTYP</b></A>
+<LI> <A NAME=tex2html15 HREF=nscan_private_intfc.html#SECTION00031200000000000000>  <b>Parameter OPTION</b></A>
+<LI> <A NAME=tex2html16 HREF=nscan_private_intfc.html#SECTION00031300000000000000>  <b>Parameter OUTPUT_FILE</b></A>
+<LI> <A NAME=tex2html17 HREF=nscan_private_intfc.html#SECTION00031400000000000000>  <b>Parameter OUTPUT_LABEL</b></A>
+<LI> <A NAME=tex2html18 HREF=nscan_private_intfc.html#SECTION00031500000000000000>  <b>Parameter POINTING_SETS</b></A>
+<LI> <A NAME=tex2html19 HREF=nscan_private_intfc.html#SECTION00031600000000000000>  <b>Parameter SCN_SET_PATTERN</b></A>
+<LI> <A NAME=tex2html20 HREF=nscan_private_intfc.html#SECTION00031700000000000000>  <b>Parameter SELECT_IQXY</b></A>
+<LI> <A NAME=tex2html21 HREF=nscan_private_intfc.html#SECTION00031800000000000000>  <b>Parameter TYPE_TAPE</b></A>
+<LI> <A NAME=tex2html22 HREF=nscan_private_intfc.html#SECTION00031900000000000000>  <b>Parameter WERR_HA</b></A>
+<LI> <A NAME=tex2html23 HREF=nscan_private_intfc.html#SECTION00032000000000000000>  <b>Parameter WERR_OPTION</b></A>
+<LI> <A NAME=tex2html24 HREF=nscan_private_intfc.html#SECTION00032100000000000000>  <b>Parameter WERR_RA</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the parameter interface of the program NSCAN. The program also uses a number of public interfaces; references to these are also <A HREF="#.public">listed</A>. 
+show parameters that 
+        The remainder of the document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<em>See also:</em> 
+<UL><LI> <A HREF="../introduction/introduction.html#.user.interface">DWARF</A> user interface 
+<LI> <A HREF="../mdlnode_public_intfc/mdlnode_public_intfc.html">MDLNODE</A> public keywords 
+<LI> <A HREF="../ngen_public_intfc/ngen_public_intfc.html">NGEN</A> public keywords 
+<LI> <A HREF="../nmodel_public_intfc/nmodel_public_intfc.html">NMODEL</A> public keywords 
+<LI> <A HREF="../nshow_public_intfc/nshow_public_intfc.html">NSHOW</A> public keywords 
+<LI> <A HREF="../scnnode_public_intfc/scnnode_public_intfc.html">SCNNODE</A> public keywords 
+<LI> <A HREF="../scnsets_public_intfc/scnsets_public_intfc.html">SCNSETS</A> public keywords 
+<LI> <A HREF="../select_public_intfc/select_public_intfc.html">SELECT</A> public keywords 
+<LI> <A HREF="../unit_public_intfc/unit_public_intfc.html">UNIT</A> public keywords 
+</UL>
+<P>
+<A NAME=.arc.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter ARC_OPTION</b></A></H2>
+<P>
+  <em>Prompt:</em> ARC Action<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+    <PRE>
+Checking in a WSRT tape has two phases. In the first phase, the ARC option
+CHECK is used to verify the general integrity of the tape. The tape is listed
+and all blocks are read. In the second phase labels are copied to the archive
+medium (with the DUMP option) and the Scissor database is updated through ARC
+option ARCHIVE.
+</PRE>
+<P>
+<A NAME=.bitpix><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter BITPIX</b></A></H2>
+<P>
+<em>Prompt:</em> Precision for writing UVFITS output<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the precision for writing UVFITS data.
+</PRE>
+<P>
+  <PRE>
+   16     2 bytes integers
+   32     4 bytes integers
+  -32     IEEE Floating point values (not yet supported)
+</PRE>
+<P>
+<A NAME=.channels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter CHANNELS</b></A></H2>
+<P>
+<em>Prompt:</em> frequency channel number(s)<BR><em>Expected input:</em> Integer:  1 to 512 values
+<P>
+  <PRE>
+Select the frequency channels/bands to be included. NOTE that the WSRT
+continuum channel (i.e. the sum of all channels) always has number 0
+</PRE>
+<P>
+  <PRE>
+   '*' selects all channels
+</PRE>
+<P>
+  <PRE>
+   '<begin> TO <end>> BY <step>' selects channels <begin>, <begin>+<step>, ...
+        up to <end>. The 'BY <step>' part may be omitted.
+   BEWARE: The notation <begin>-<end>:<step> will be interpreted as an
+        expression and give incorrect results
+</PRE>
+<P>
+  <PRE>
+Each of the selected channels will be stored in the .SCN file as a separate
+'channel' (chn) under the current 'group', 'observation' and 'field'
+grp.obs.fld. (Remember that .SCN file 'sectors' are identified by indices
+grp.obs.fld.chn.seq).
+</PRE>
+<P>
+<A NAME=.hab.offset><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter HAB_OFFSET</b></A></H2>
+<P>
+<em>Prompt:</em> Start-offset (sec)<BR><em>Expected input:</em> Real:  1 value
+<P>
+  <PRE>
+Specify the time-offset from the start of an observation, at which the
+integration for the output scans should start. Example: an offset of n will
+throw away the first n (rounded up to a multiple of 10) seconds of data.
+</PRE>
+<P>
+  <PRE>
+NOTE: This feature was useful in early mosaic experiments in which the slewing
+between fields occurred in the first integration interval(s) on the new field.
+It is now standard practice to slew during the final integration interval on
+the old source.
+</PRE>
+<P>
+<A NAME=.iat.utc><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter IAT_UTC</b></A></H2>
+<P>
+<em>Prompt:</em> MJD, leap seconds,...<BR><em>Expected input:</em> Real:  1 to 20 values
+<P>
+  <PRE>
+Specify the IAT-UTC values as pair(s) of numbers:
+</PRE>
+<P>
+  <PRE>
+   MJD at which the leap seconds occur
+   The total number of leap seconds as from that date.
+</PRE>
+<P>
+  <PRE>
+The first value is for 1 Jan 1991. Values before that are known by the program.
+</PRE>
+<P>
+<A NAME=.ifsets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter IFSETS</b></A></H2>
+<P>
+<em>Prompt:</em> integration time for total-power data<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the desired integration time for IF sets with Total Power data.
+</PRE>
+<P>
+<A NAME=.input.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter INPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> input filename<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the input disk-file name.
+</PRE>
+<P>
+  <PRE>
+For the NSCAN LOAD-from-disk option, or for the NSCAN PFITS option, don't
+specify a file extension: it will be made by the program on the basis of the
+tape label number.
+</PRE>
+<P>
+  <PRE>
+In the case of other NSCAN options, give the full file name.
+</PRE>
+<P>
+<A NAME=.input.labels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter INPUT_LABELS</b></A></H2>
+<P>
+<em>Prompt:</em> input tape labels<BR><em>Expected input:</em> Integer:  1 to 256 values
+<P>
+  <PRE>
+Specify the tape labels to be read.
+</PRE>
+<P>
+  <PRE>
+   '*' selects all labels
+</PRE>
+<P>
+  <PRE>
+   '<begin> TO <end>> BY <step>' selects labels <begin>, <begin>+<step>, ...
+        up to <end>. The 'BY <step>' part may be omitted.
+   BEWARE: The notation <begin>-<end>:<step> will be interpreted as an
+        expression and give incorrect results
+</PRE>
+<P>
+  <PRE>
+Each of the selected labels will be stored in the .SCN file as a separate
+'observation' (obs) in the current 'group' grp. (Remember that .SCN file
+'sectors' are identified by indices grp.obs.fld.chn.seq).
+</PRE>
+<P>
+  <PRE>
+Example:
+        If the current group nr is <g>, the selected input labels will be
+stored sequentially in the .SCN file as observations <g>.0, <g>.1, <g>.2
+</PRE>
+<P>
+<A NAME=.integration.time><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031000000000000000>  <b>Parameter INTEGRATION_TIME</b></A></H2>
+<P>
+<em>Prompt:</em> integration time (sec)<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the desired integration time per output scan in seconds.
+120 sec is a good default; a lower value should be selected if visibilities
+vary rapidly as a consequence of the source distribution in the observed field,
+atmospheric conditions or interference.
+</PRE>
+<P>
+  <PRE>
+For standard observations, the number must be a multiple of the basic
+integration time used for the observation (which is some multiple of 10 sec).
+</PRE>
+<P>
+  <PRE>
+In WSRT mosaic observations, slewing occurs in the last 10 sec of the dwell
+time on each subfield. The integration time you specify must therefore at most
+be <dwell time> minus 10 sec. You may also use a submultiple of this value
+without losing data.
+</PRE>
+<P>
+  <PRE>
+    Example:
+        If the dwell time is 90 sec, there is 80 sec of valid data. HA_INT = 80,
+    40, 20 or 10 will use it all. However, HA_INT = 30 or 60 will result in the
+    loss of the last 20 sec.
+</PRE>
+<P>
+  <PRE>
+        The volume of your data in the .SCN depends primarily on the
+integration time. For each integration interval a 'scan' is created which
+consists of
+</PRE>
+<P>
+  <PRE>
+        <nr of polarisations> * <nr of interferometers> * 12 + 1024 bytes
+</PRE>
+<P>
+  <PRE>
+Model visibilities which may be added later will occupy another
+</PRE>
+<P>
+  <PRE>
+        4 * <nr of interferometers> * 12 bytes .                 NOTE:
+        The WSRT runs on Universal Time; the quantum of integration time is
+therefore 10 UT seconds, and a full 12-sidereal-hour observation contains
+somewhat less than 12*360 of these quanta. You can mostly ignore this subtlety,
+but the difference may be of practical importance in some situations.
+</PRE>
+<P>
+<A NAME=.old.dattyp><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031100000000000000>  <b>Parameter OLD_DATTYP</b></A></H2>
+<P>
+<em>Prompt:</em> Old R-series data format<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+Specify the old R-series data type:
+</PRE>
+<P>
+  <PRE>
+        0= local
+        1= VAX, D_FORMAT
+        2= VAX, G_FORMAT
+        3= ALLIANT
+        4= CONVEX
+        5= IEEE
+        6= DEC station
+        7= SUN station
+        8= HP  station
+</PRE>
+<P>
+<A NAME=.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031200000000000000>  <b>Parameter OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> Action<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify the action to be performed by the program NSCAN:
+</PRE>
+<P>
+  <PRE>
+   Operations on WSRT 'circle' observation files (on classical, DAT or Exabyte
+   tape, magnetic or optical disk):
+</PRE>
+<P>
+  <PRE>
+        LOAD     transfer observed visibilities into a .SCN file.
+        IFLOAD   same, but also transfer the 'IF' data (total powers etc). The
+                  extra data will enlarge the .SCN file by some 30%
+                  them only if you suspect that the on-line gain calibration has
+                  been incorrect.
+        LEIDEN   transfer observed visibilities from standard LEIDEN file into a
+                  .SCN file
+        LIST     show contents of selected labels
+        ARC      as list, but update the Scissor database if at NFRA
+        DUMP     copy selected label(s) byte for byte into a disk file
+</PRE>
+<P>
+  <PRE>
+   Conversion to and listing of data in FITS format
+</PRE>
+<P>
+  <PRE>
+        UVFITS   convert .SCN file to UVFITS tape/disk file for use in AIPS
+        PFITS    print AIPS-like FITS info (but also other) from UVFITS file
+                   header
+</PRE>
+<P>
+  <PRE>
+   Display and editing of .SCN files:
+</PRE>
+<P>
+  <PRE>
+        SHOW     show/edit data and header information in .SCN file. (This
+                   option is duplicated in NFLAG.)
+</PRE>
+<P>
+  <PRE>
+   Utilities:
+</PRE>
+<P>
+  <PRE>
+        QUIT     leave the program NSCAN
+</PRE>
+<P>
+  <PRE>
+        CVX      convert a .SCN file from other machine's number format
+        NVS      convert a .SCN file to newest version. Needs only to be run if
+                   programs report that the data has the wrong version
+                  - calculates parallactic angle for ATNF
+        NOPT     update contents of sector/scan headers and polarisation format
+                  of visibility data:
+                   - convert input data in Stokes parameter format to XX format
+                   - calculate UT start
+                   - calculate precession rotation angle if not filled
+                   - recalculate MJD for observations aborted at Wbork
+        REGROUP  create a second index for each of one or more sets of sector.
+</PRE>
+<P>
+  <PRE>
+   One-time fixes:
+</PRE>
+<P>
+  <PRE>
+        FROM_OLD convert old (R-series) uv-data file into NEWSTAR .SCN file
+        WERR     correct one-time mosaic WSRT tape errors (1991 data only)
+        AERR     change sign of phases
+</PRE>
+<P>
+<A NAME=.output.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031300000000000000>  <b>Parameter OUTPUT_FILE</b></A></H2>
+<P>
+<em>Prompt:</em> output filename<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the full name for the output disk file.
+</PRE>
+<P>
+  <PRE>
+For the NSCAN DUMP option, don't specify a file extension: it will be made by
+the program on the basis of the label number.
+</PRE>
+<P>
+  <PRE>
+For the other NSCAN options, specify a full file-name.
+</PRE>
+<P>
+<A NAME=.output.label><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031400000000000000>  <b>Parameter OUTPUT_LABEL</b></A></H2>
+<P>
+<em>Prompt:</em> output tape label<BR><em>Expected input:</em> Integer:  1 value
+<P>
+  <PRE>
+        Specify the first output tape label.
+* or 0 indicates the end of the tape (i.e. append the new labels at the end).
+</PRE>
+<P>
+<A NAME=.pointing.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031500000000000000>  <b>Parameter POINTING_SETS</b></A></H2>
+<P>
+<em>Prompt:</em> Mosaic field sequence number(s)<BR><em>Expected input:</em> Integer:  1 to 512 values
+<P>
+  <PRE>
+        Select the SEQUENCE numbers of the fields (= mosaic 'pointing
+centres') to be selected. (see Note below).
+</PRE>
+<P>
+  <PRE>
+NOTE that WSRT mosaic fields are numbered starting at 1
+</PRE>
+<P>
+  <PRE>
+   '*' selects all fields
+</PRE>
+<P>
+  <PRE>
+   '<begin> TO <end>> BY <step>' selects fields <begin>, <begin>+<step>, ...
+        up to <end>. The 'BY <step>' part may be omitted.
+   BEWARE: The notation <begin>-<end>:<step> will be interpreted as an
+        expression and give incorrect results
+</PRE>
+<P>
+  <PRE>
+Each of the selected fields will be stored in the .SCN file as a separate
+'field' (fld) under the current 'group' and 'observation' grp.obs. (Remember
+that .SCN file 'sectors' are identified by indices grp.obs.fld.chn.seq).
+</PRE>
+<P>
+  <PRE>
+NOTE:
+        The numbers you specify refer to the SEQUENCE (starting with 0) in
+which the mosaic fields aqppear on the tape. Normally, an observation starts
+with field 0 and the sequence numbers equal the field numbers. However, if your
+observation starts 'somehere in the middle', this is no longer the case and you
+must be careful in selecting your fields. Example:
+</PRE>
+<P>
+  <PRE>
+        Your observation starts at field 19. To select fields 19 through 24,
+specify POINTING_SETS= 0 TO 5.
+</PRE>
+<P>
+<A NAME=.scn.set.pattern><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031600000000000000>  <b>Parameter SCN_SET_PATTERN</b></A></H2>
+<P>
+<em>Prompt:</em> new index pattern (grp.obs.fld.chn.seq)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Specify a new index pattern (group.observation.field.channel.sequence_number)
+into which to change the index pattern of the input Set of uv-data Sectors.
+</PRE>
+<P>
+  <PRE>
+Each index in the pattern that contains an * is copied from the input Set.
+Other fields are used as is (true for the first four fields, i.e.
+grp.obs.fld.chn.)
+</PRE>
+<P>
+  <PRE>
+Example: To change the indices of the Set
+        0.*.15283.* to
+        0.*.0    .*
+</PRE>
+<P>
+  <PRE>
+give the first selection as the input Set, and the second as the pattern.
+</PRE>
+<P>
+<A NAME=.select.iqxy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031700000000000000>  <b>Parameter SELECT_IQXY</b></A></H2>
+<P>
+<em>Prompt:</em> output polarisations (ONE 'value') |<BR><em>Expected input:</em> Character *4:  1 value
+<P>
+  <PRE>
+Specify the polarisation(s) to be written:
+</PRE>
+<P>
+  <PRE>
+        I:      I only
+        Q:      Q only
+        U:      U only
+        V:      V only
+</PRE>
+<P>
+  <PRE>
+        IQ:     I and Q
+        UV:     U and V
+        IQUV:   I, Q, U and V
+</PRE>
+<P>
+  <PRE>
+        X:      XX only
+        XXY:    XY only
+        YYX:    YX only
+        Y:      YY only
+</PRE>
+<P>
+  <PRE>
+        XY:     XX and YY
+        YX:     XY and YX
+        XYX:    all four: XX,XY,YX,YY
+</PRE>
+<P>
+<A NAME=.type.tape><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031800000000000000>  <b>Parameter TYPE_TAPE</b></A></H2>
+<P>
+<em>Prompt:</em> Which type tape<BR><em>Expected input:</em> Character *6:  1 value
+<P>
+  <PRE>
+Specify the type of the tape.
+</PRE>
+<P>
+  <PRE>
+Currently we support two types: WSRT and LEIDEN.
+</PRE>
+<P>
+<A NAME=.werr.ha><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00031900000000000000>  <b>Parameter WERR_HA</b></A></H2>
+<P>
+<em>Prompt:</em> Hour-angle correction (deg)<BR><em>Expected input:</em> DoublePrecision:  1 value
+<P>
+  <PRE>
+Specify the angle to be added to all hour angles in the .SCN file
+</PRE>
+<P>
+  <PRE>
+NOTE: This is a special feature to be used only to correct errors made in the
+on-line observation.
+</PRE>
+<P>
+<A NAME=.werr.option><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032000000000000000>  <b>Parameter WERR_OPTION</b></A></H2>
+<P>
+<em>Prompt:</em> WERR action<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify correction to be performed:
+</PRE>
+<P>
+  <PRE>
+   WE0:   correct Hour angles for tape error in splitted mosaic tapes before
+           online version 62
+   WE1:   correct all Hour angles with a constant offset
+   QUIT:  no more
+</PRE>
+<P>
+<A NAME=.werr.ra><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION00032100000000000000>  <b>Parameter WERR_RA</b></A></H2>
+<P>
+<em>Prompt:</em> RA of mosaic centre<BR><em>Expected input:</em> DoublePrecision:  1 value
+<P>
+  <PRE>
+Specify the Right Ascension of the centre of the mosaic area
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/nshow/nshow__edit.html b/nshow/nshow__edit.html
new file mode 100644
index 0000000000000000000000000000000000000000..dc34e6a635de968537e817e5c1311dcbfb5f47f3
--- /dev/null
+++ b/nshow/nshow__edit.html
@@ -0,0 +1,48 @@
+<TITLE>Description of EDIT (NSHOW)</TITLE>
+<H1>Description of general keyword EDIT</H1>
+
+<DT><EM>Prompt:</EM> Edit: name [offset][/length][:format] , val [, ...]
+<DT><EM>Expected input:</EM> Character(80), 16 values.<P>
+The preceding sequence of parameter values that you provided defines one header 
+or data structure being processed. The EDIT parameter now allows you show 
+and/or edit the values of individual (goups of) fields in this structure. All 
+fields may be modified, except for the pointers that define the structure of 
+the file. <P>
+NOTE: Although EDITing may be used to patch up a file, it is really intended 
+only for debugging/testing purposes! 
+        Newstar programs provide a number of manual-input operations that cover 
+all situations expected in normal practice. In the rare cases that a file is 
+systematically corrupted in a curable way (e.g. because of an error in the WSRT 
+on-line program), the preferred course is to have an ad-hoc extension made to a 
+Newstar program to process the damaged file(s). <P>
+The following operations are available: <P>
+   *                 show values of all fields in the structure 
+   :                 show format information for all fields in the structure 
+   &lt;name&gt;            show value(s) of field &lt;name&gt; in the structure 
+   &lt;name&gt;:           show format information for field &lt;name&gt; in the structure 
+   &lt;name&gt;, &lt;value&gt;, .. write &lt;valye&gt; in filed &lt;name&gt; in the structure <P>
+   Instead of &lt;name&gt; you may specify a hex number (absolute address in the file) 
+   or a hex number preceded by a '.' (address in the file relative to the origin 
+   of the current structure) <P>
+. 
+Values are assumed to be in format of printout. Radix can be changed by 
+prefixing with %X, %B, %O or %D. Angles are in degrees, but can be given as 
+hh:[mm[:ss[.ttt]]] or dd.mm.[ss.ttt] <P>
+'name' can be followed by (offset) to start at position offset in multi-valued 
+list; and/or /number to limit number of values in same <P>
+A full name specification can be followed with either: 
+   :format               to change printing and reading format. (format can be 
+                        e.g. {USX}{BIJ}  {ED}[n[.m]] {EC|DC}[n[.m]] 
+   ::type[(off)][/n]     where type specifies a header type (e.g. STH) to format 
+                        the indicated disk area as this type 
+                        Single letter types are dummy header types for simple 
+                        formats 
+  ::                    gives all known header types 
+! {\em see the \textref{SHOW/EDIT}{show_edit} manual for a more elaborate 
+! \ description} 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nshow/nshow_comm.html">List of general keywords</A> for NSHOW
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nshow/nshow__file_action.html b/nshow/nshow__file_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..c1eb937dac21a3278ac3faf3af25340098beca60
--- /dev/null
+++ b/nshow/nshow__file_action.html
@@ -0,0 +1,21 @@
+<TITLE>Description of FILE_ACTION (NSHOW)</TITLE>
+<H1>Description of general keyword FILE_ACTION</H1>
+
+<DT><EM>Prompt:</EM> file-header action LAYOUT, OVERVIEW; SHOW, EDIT; CONT, QUIT |
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify interaction with the file header: <P>
+   Summarise contents of the file: 
+        LAYOUT    show counts of groups, fields and channels in the file 
+        OVERVIEW  give overview of all sector headers <P>
+   Details of the file header: 
+        SHOW:     display the file header in full 
+        EDIT:     edit fields in the file header <P>
+   Navigation: 
+        CONT      go down one level, to interact with Sector headers 
+        QUIT      exit from SHOW/EDIT option <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nshow/nshow_comm.html">List of general keywords</A> for NSHOW
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nshow/nshow__map_action.html b/nshow/nshow__map_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..ea6f01598cca1425a9548af5a33821b07ef33b50
--- /dev/null
+++ b/nshow/nshow__map_action.html
@@ -0,0 +1,21 @@
+<TITLE>Description of MAP_ACTION (NSHOW)</TITLE>
+<H1>Description of general keyword MAP_ACTION</H1>
+
+<DT><EM>Prompt:</EM> NEXT, JOB, SHOW, EDIT, CONT, QUIT image-header action
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify interaction with image header: <P>
+   Show details of the image header: 
+        SHOW    Display the entire image header 
+        EDIT    Edit fields in the image header <P>
+   Show details associated with the current image: 
+        JOB     Job summary sheet (if available) <P>
+   Navigation: 
+        NEXT    Proceed to the header for the next image selected 
+        CONT    Pescend into the scans of this image 
+        QUIT    Return to the file-header level <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nshow/nshow_comm.html">List of general keywords</A> for NSHOW
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nshow/nshow__ply} }.html b/nshow/nshow__ply} }.html
new file mode 100644
index 0000000000000000000000000000000000000000..135e7b8e0b30b78ccab334725eea1ae5325691bc
--- /dev/null
+++ b/nshow/nshow__ply} }.html	
@@ -0,0 +1,21 @@
+<TITLE>Description of ply} } (NSHOW)</TITLE>
+<H1>Description of general keyword ply} }</H1>
+
+<DT><EM>Prompt:</EM> NEXT, JOB, SHOW, EDIT, CONT, QUIT image-header action
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify interaction with image header: <P>
+   Show details of the image header: 
+        SHOW    Display the entire image header 
+        EDIT    Edit fields in the image header <P>
+   Show details associated with the current image: 
+        JOB     Job summary sheet (if available) <P>
+   Navigation: 
+        NEXT    Proceed to the header for the next image selected 
+        CONT    Pescend into the scans of this image 
+        QUIT    Return to the file-header level <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nshow/nshow_comm.html">List of general keywords</A> for NSHOW
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nshow/nshow__scan_action.html b/nshow/nshow__scan_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..786451ceab892f6713c1cea4a51c93f6890aad77
--- /dev/null
+++ b/nshow/nshow__scan_action.html
@@ -0,0 +1,55 @@
+<TITLE>Description of SCAN_ACTION (NSHOW)</TITLE>
+<H1>Description of general keyword SCAN_ACTION</H1>
+
+<DT><EM>Prompt:</EM> Scan action, one of |-
+(header:)       Show, Edit, Ifr; |-
+(navigate:)     nn.nn, &gt;/&lt;, &gt;n/&lt;n, Quit; |-
+(data select:)  XX, XY, YX, YY, TP, GN; COR/UNCOR; |-
+(data display:) Data, A_phi, Weight; |-
+(miscell:)      Tel
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify interaction with the scan's header or data: <P>
+   Details of the scan header and associated tables: <P>
+        SHOW    Show entire header for selected scan 
+        EDIT    Edit fields in the scan header 
+        IFR     Show table of interferometer corrections <P>
+   Navigation. The hour angle/scan you select remains in force until you select 
+   a new one or QUIT. Initial selection is the first scan in this sector. For a 
+   non-existent hour-angle, the nearest existing one is selected instead. <P>
+        nn.nn   Select scan at hour angle nearest to this value 
+        &gt;, &lt;    Select the next (&gt;) or preceding (&lt;) scan 
+        &gt;n, &lt;n  Select the n-th next (&gt;) or preceding (&lt;) scan 
+        Q[uit]  Return to sector-header level <P>
+Mode switches. The values you select remain in force until you change them or 
+QUIT. <P>
+   Data-stream selection; the initial setting is XX. 
+        XX/XY/YX/YY 
+                Select polarisation 
+        TP      Select Total Power mode (noise source on/off) 
+        GN      Select Gain correction mode <P>
+   Correction mode. Visibility data will be displayed accordingly. Initial 
+   setting is UNCOR. <P>
+        UNCOR   Display 'raw' data 
+        COR     Display the data corrected as specified by the APPLY 
+                and DE_APPLY parameters. These parameters are normally set 
+                automatically for you. (This may result in the program 
+                requesting additional information.) 
+! {\em see the parameter description for \textref{APPLY}{ngen.apply} and 
+! \textref{DE_APPLY}{ngen.de.apply} } <P>
+Data display for the selected scan and polarisation: <P>
+        D[ata]   Complex visibilities (real and imaginary parts) 
+        A[mpl]   Visibilities represented as amplitude and phase 
+        W[eight] Weights and flags associated with the visibilities <P>
+Miscellaneous functions:\. 
+        T[el]   Calculate and show an estimate (based on a point source model) 
+                for the telescope gains/phases. In those rare cases where NCALIB 
+                REDUN fails to correctly resolve 180-deg phase ambiguities, you 
+                may use the phases displayed here as initial values for the 
+                corrections, through the NCALIB SET MANUAL option. 
+! {\em see the NCALIB \textref{SET MANUAL}{ncalib.set} parameter description} 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nshow/nshow_comm.html">List of general keywords</A> for NSHOW
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nshow/nshow__sector_action.html b/nshow/nshow__sector_action.html
new file mode 100644
index 0000000000000000000000000000000000000000..b7b95a14f95207a7c97bdc28d4bdf9672934f2d5
--- /dev/null
+++ b/nshow/nshow__sector_action.html
@@ -0,0 +1,25 @@
+<TITLE>Description of SECTOR_ACTION (NSHOW)</TITLE>
+<H1>Description of general keyword SECTOR_ACTION</H1>
+
+<DT><EM>Prompt:</EM> Sector-header action | SHOW, EDIT; NAME, IFRS, IFH, FLAGS; NEXT, CONT, QUIT
+<DT><EM>Expected input:</EM> Character(24).<P>
+Specify interaction with this sector header: <P>
+   Show details of the sector header: 
+        SHOW    show entire sector header 
+        EDIT    edit fields (values) in the Sector header by name <P>
+   Show details associated with the current sector: 
+        NAME    index 'name' of the current Sector (if #nr specified) 
+        IFRS    the interferometer table 
+        IFH:    header of 'IF' data (Total Powers etc) 
+        FLAGS:  show the nr of flags per interferometer that are set in the 
+                 current Sector <P>
+   Navigation: 
+        NEXT:   proceed to the header for the next sector selected 
+        CONT:   descend into the scans of this sector 
+        QUIT:   return to the file-header level <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../nshow/nshow_comm.html">List of general keywords</A> for NSHOW
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/nshow_comm/nshow_comm.html b/nshow_comm/nshow_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..a45898a4ed85924dd69edce4ecc415a3c469daa9
--- /dev/null
+++ b/nshow_comm/nshow_comm.html
@@ -0,0 +1,31 @@
+<TITLE>Index of general keywords from NSHOW</TITLE>
+<H1>Description of general keywords (NSHOW)</H1>
+
+<UL>
+<LI> <A HREF="../nshow/nshow__file_action.html">
+  FILE_ACTION</A>
+  file-header action LAYOUT, OVERVIEW; SHOW, EDIT; CONT, QUIT |
+<LI> <A HREF="../nshow/nshow__sector_action.html">
+  SECTOR_ACTION</A>
+  Sector-header action | SHOW, EDIT; NAME, IFRS, IFH, FLAGS; NEXT, CONT, QUIT
+<LI> <A HREF="../nshow/nshow__scan_action.html">
+  SCAN_ACTION</A>
+  Scan action, one of |-
+(header:)       Show, Edit, Ifr; |-
+(navigate:)     nn.nn, &gt;/&lt;, &gt;n/&lt;n, Quit; |-
+(data select:)  XX, XY, YX, YY, TP, GN; COR/UNCOR; |-
+(data display:) Data, A_phi, Weight; |-
+(miscell:)      Tel
+<LI> <A HREF="../nshow/nshow__map_action.html">
+  MAP_ACTION</A>
+  NEXT, JOB, SHOW, EDIT, CONT, QUIT image-header action
+<LI> <A HREF="../nshow/nshow__edit.html">
+  EDIT</A>
+  Edit: name [offset][/length][:format] , val [, ...]
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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+b(APPL)m(Y)710 1655 y Fb(2)740 1671 y Fc(and)g(DE)p 886
+1671 12 2 v 14 w(APPL)m(Y)1029 1655 y Fb(3)0 1746 y Fd(Data)18
+b(display)f(for)h(the)h(selected)d(scan)i(and)h(polarisat)o(ion)o(:)157
+1825 y(D[ata])56 b(Complex)17 b(visibiliti)o(es)f(\(real)i(and)g
+(imaginary)f(parts\))157 1870 y(A[mpl])56 b(Visibilitie)o(s)16
+b(represented)g(as)j(amplitude)d(and)i(phase)157 1916
+y(W[eight])e(Weights)h(and)i(flags)e(associated)f(with)i(the)h
+(visibilit)o(ies)0 1995 y(Miscellane)o(ou)o(s)e(functions)o(:\\)o(.)157
+2040 y(T[el])57 b(Calculate)16 b(and)i(show)g(an)h(estimate)e(\(based)g
+(on)i(a)g(point)f(source)f(model\))314 2086 y(for)h(the)h(telescope)d
+(gains/pha)o(ses)o(.)g(In)j(those)f(rare)g(cases)g(where)f(NCALIB)314
+2132 y(REDUN)h(fails)f(to)i(correctly)d(resolve)h(180-deg)g(phase)h
+(ambiguiti)o(es)o(,)f(you)314 2177 y(may)h(use)h(the)f(phases)f
+(displayed)g(here)h(as)h(initial)d(values)i(for)g(the)314
+2223 y(correctio)o(ns,)e(through)h(the)h(NCALIB)f(SET)i(MANUAL)e
+(option.)0 2302 y Fc(se)n(e)c(the)f(NCALIB)27 b(SET)14
+b(MANUAL)567 2286 y Fb(4)596 2302 y Fc(p)n(ar)n(ameter)f(description)0
+2456 y Fe(2.6)74 b(P)n(arameter)18 b(SECTOR)p 656 2456
+17 2 v 20 w(A)n(CTION)0 2557 y Fj(Pr)n(ompt:)g Fg(Sector-header)e
+(action)d(|)h(\()p Fj(may)h(vary)g(p)n(er)f(applic)n(ation)p
+Fg(\))0 2607 y Fj(Exp)n(e)n(cte)n(d)h(input:)k Fg(Character)c(*24:)i(1)
+d(v)n(alue)0 2682 y Fd(Specify)j(interacti)o(on)f(with)i(this)g(sector)
+g(header:)p 0 2721 756 2 v 46 2747 a Fb(2)64 2759 y Fa($n)p
+104 2759 11 2 v 11 w(hlp/ngen.ps:.a)o(pp)o(ly)46 2787
+y Fb(3)64 2799 y Fa($n)p 104 2799 V 11 w(hlp/ngen.ps:.d)o(e.a)o(pp)o
+(ly)46 2827 y Fb(4)64 2838 y Fa($n)p 104 2838 V 11 w(hlp/ncalib.ps:)o
+(.set)935 2995 y Fg(3)p eop
+%%Page: 4 4
+4 3 bop 59 0 a Fd(Show)18 b(details)f(of)i(the)f(sector)f(header:)157
+46 y(SHOW)77 b(show)18 b(entire)f(sector)g(header)157
+92 y(EDIT)77 b(edit)18 b(fields)f(\(values\))g(in)i(the)f(Sector)f
+(header)h(by)g(name)59 171 y(Show)g(details)f(associate)o(d)g(with)h
+(the)g(current)f(sector:)157 216 y(NAME)77 b(index)18
+b('name')f(of)i(the)f(current)f(Sector)g(\(if)i(#nr)f(specified\))157
+262 y(IFRS)77 b(the)18 b(interferom)o(ete)o(r)e(table)157
+308 y(IFH:)77 b(header)17 b(of)i('IF')f(data)g(\(Total)f(Powers)h
+(etc\))157 353 y(FLAGS:)37 b(show)18 b(the)g(nr)h(of)g(flags)f(per)g
+(interferom)o(ete)o(r)e(that)i(are)h(set)f(in)h(the)333
+399 y(current)e(Sector)59 478 y(Navigatio)o(n:)157 523
+y(NEXT:)57 b(proceed)17 b(to)i(the)f(header)f(for)i(the)f(next)g
+(sector)g(selected)157 569 y(CONT:)57 b(descend)17 b(into)h(the)g
+(scans)g(of)h(this)f(sector)157 615 y(QUIT:)57 b(return)17
+b(to)i(the)f(file-header)e(level)935 2995 y Fg(4)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/nshow_public_intfc/images.pl b/nshow_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/nshow_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/nshow_public_intfc/labels.pl b/nshow_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..25dd877b040cc20f177ee84ee939eb557b5b9bd3
--- /dev/null
+++ b/nshow_public_intfc/labels.pl
@@ -0,0 +1,13 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".map.action"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".file.action"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".public"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".edit"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".sector.action"} ="$URL/nshow_public_intfc.html"; 
+$external_labels{".scan.action"} ="$URL/nshow_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/nshow_public_intfc/nshow_public_intfc.html b/nshow_public_intfc/nshow_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..306a364208716602f75fab95b25b00ca1d0003f6
--- /dev/null
+++ b/nshow_public_intfc/nshow_public_intfc.html
@@ -0,0 +1,312 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group NSHOW</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=nshow_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=nshow_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=nshow_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=nshow_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=nshow_public_intfc.html#SECTION0003200000000000000>  <b>Parameter EDIT</b></A>
+<LI> <A NAME=tex2html6 HREF=nshow_public_intfc.html#SECTION0003300000000000000>  <b>Parameter FILE_ACTION</b></A>
+<LI> <A NAME=tex2html7 HREF=nshow_public_intfc.html#SECTION0003400000000000000>  <b>Parameter MAP_ACTION</b></A>
+<LI> <A NAME=tex2html8 HREF=nshow_public_intfc.html#SECTION0003500000000000000>  <b>Parameter SCAN_ACTION</b></A>
+<LI> <A NAME=tex2html9 HREF=nshow_public_intfc.html#SECTION0003600000000000000>  <b>Parameter SECTOR_ACTION</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group NSHOW, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter EDIT</b></A></H2>
+<P>
+  <em>Prompt:</em> Edit: name [offset][/length][:format] , val [,...] (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 to 16 values
+<P>
+    <PRE>
+The preceding sequence of parameter values that you provided defines one header
+or data structure being processed. The EDIT parameter now allows you show
+and/or edit the values of individual (goups of) fields in this structure. All
+fields may be modified, except for the pointers that define the structure of
+the file.
+</PRE>
+<P>
+  <PRE>
+NOTE: Although EDITing may be used to patch up a file, it is really intended
+only for debugging/testing purposes
+        Newstar programs provide a number of manual-input operations that cover
+all situations expected in normal practice. In the rare cases that a file is
+systematically corrupted in a curable way (e.g. because of an error in the WSRT
+on-line program), the preferred course is to have an ad-hoc extension made to a
+Newstar program to process the damaged file(s).
+</PRE>
+<P>
+  <PRE>
+The following operations are available:
+</PRE>
+<P>
+  <PRE>
+   *                 show values of all fields in the structure
+   :                 show format information for all fields in the structure
+   <name>            show value(s) of field <name> in the structure
+   <name>:           show format information for field <name> in the structure
+   <name>,<value>,.. write <valye> in filed <name> in the structure
+</PRE>
+<P>
+  <PRE>
+   Instead of <name> you may specify a hex number (absolute address in the file)
+   or a hex number preceded by a '.' (address in the file relative to the origin
+   of the current structure)
+</PRE>
+<P>
+  <PRE>
+Values are assumed to be in format of printout. Radix can be changed by
+prefixing with %
+hh:[mm[:ss[.ttt]]] or dd.mm.[ss.ttt]
+</PRE>
+<P>
+  <PRE>
+'name' can be followed by (offset) to start at position offset in multi-valued
+list; and/or /number to limit number of values in same
+</PRE>
+<P>
+  <PRE>
+A full name specification can be followed with either:
+   :format               to change printing and reading format. (format can be
+                        e.g. {USX}{BIJ}  {ED}[n[.m]] {EC|DC}[n[.m]]
+   ::type[(off)][/n]     where type specifies a header type (e.g. STH) to format
+                        the indicated disk area as this type
+                        Single letter types are dummy header types for simple
+                        formats
+  ::                    gives all known header types
+</PRE> 
+ <em>see the <A HREF="../show_edit/show_edit.html">SHOW/EDIT</A> manual for a more elaborate
+  description</em>
+<P>
+<A NAME=.file.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter FILE_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> file-header action (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify interaction with the file header:
+</PRE>
+<P>
+  <PRE>
+   Summarise contents of the file:
+        LAYOUT    show counts of groups, fields and channels in the file
+        OVERVIEW  give overview of all sector headers
+</PRE>
+<P>
+  <PRE>
+   Details of the file header:
+        SHOW:     display the file header in full
+        EDIT:     edit fields in the file header
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+        CONT      go down one level, to interact with Sector headers
+        QUIT      exit from SHOW/EDIT option
+</PRE>
+<P>
+<A NAME=.map.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter MAP_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> image-header action (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify interaction with image header:
+</PRE>
+<P>
+  <PRE>
+   Show details of the image header:
+        SHOW    Display the entire image header
+        EDIT    Edit fields in the image header
+</PRE>
+<P>
+  <PRE>
+   Show details associated with the current image:
+        JOB     Job summary sheet (if available)
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+        NEXT    Proceed to the header for the next image selected
+        CONT    Pescend into the scans of this image
+        QUIT    Return to the file-header level
+</PRE>
+<P>
+<A NAME=.scan.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter SCAN_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> Scan action, one of |- (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify interaction with the scan's header or data:
+</PRE>
+<P>
+  <PRE>
+   Details of the scan header and associated tables:
+</PRE>
+<P>
+  <PRE>
+        SHOW    Show entire header for selected scan
+        EDIT    Edit fields in the scan header
+        IFR     Show table of interferometer corrections
+</PRE>
+<P>
+  <PRE>
+   Navigation. The hour angle/scan you select remains in force until you select
+   a new one or QUIT. Initial selection is the first scan in this sector. For a
+   non-existent hour-angle, the nearest existing one is selected instead.
+</PRE>
+<P>
+  <PRE>
+        nn.nn   Select scan at hour angle nearest to this value
+        >, <    Select the next (>) or preceding (<) scan
+        >n, <n  Select the n-th next (>) or preceding (<) scan
+        Q[uit]  Return to sector-header level
+</PRE>
+<P>
+  <PRE>
+Mode switches. The values you select remain in force until you change them or
+QUIT.
+</PRE>
+<P>
+  <PRE>
+   Data-stream selection; the initial setting is XX.
+        XX/XY/YX/YY
+                Select polarisation
+        TP      Select Total Power mode (noise source on/off)
+        GN      Select Gain correction mode
+</PRE>
+<P>
+  <PRE>
+   Correction mode. Visibility data will be displayed accordingly. Initial
+   setting is UNCOR.
+</PRE>
+<P>
+  <PRE>
+        UNCOR   Display 'raw' data
+        COR     Display the data corrected as specified by the APPLY
+                and DE_APPLY parameters. These parameters are normally set
+                automatically for you. (This may result in the program
+                requesting additional information.)
+</PRE> 
+ <em>see the parameter description for <A HREF="../ngen/ngen.html#.apply">APPLY</A> and
+ <A HREF="../ngen/ngen.html#.de.apply">DE_APPLY</A> </em>
+<P>
+  <PRE>
+Data display for the selected scan and polarisation:
+</PRE>
+<P>
+  <PRE>
+        D[ata]   Complex visibilities (real and imaginary parts)
+        A[mpl]   Visibilities represented as amplitude and phase
+        W[eight] Weights and flags associated with the visibilities
+</PRE>
+<P>
+  <PRE>
+Miscellaneous functions:\.
+        T[el]   Calculate and show an estimate (based on a point source model)
+                for the telescope gains/phases. In those rare cases where NCALIB
+                REDUN fails to correctly resolve 180-deg phase ambiguities, you
+                may use the phases displayed here as initial values for the
+                corrections, through the NCALIB SET MANUAL option.
+</PRE> 
+ <em>see the NCALIB <A HREF="../ncalib/ncalib.html#.set">SET MANUAL</A> parameter description</em>
+<P>
+<A NAME=.sector.action><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter SECTOR_ACTION</b></A></H2>
+<P>
+<em>Prompt:</em> Sector-header action | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *24:  1 value
+<P>
+  <PRE>
+Specify interaction with this sector header:
+</PRE>
+<P>
+  <PRE>
+   Show details of the sector header:
+        SHOW    show entire sector header
+        EDIT    edit fields (values) in the Sector header by name
+</PRE>
+<P>
+  <PRE>
+   Show details associated with the current sector:
+        NAME    index 'name' of the current Sector (if #nr specified)
+        IFRS    the interferometer table
+        IFH:    header of 'IF' data (Total Powers etc)
+        FLAGS:  show the nr of flags per interferometer that are set in the
+                 current Sector
+</PRE>
+<P>
+  <PRE>
+   Navigation:
+        NEXT:   proceed to the header for the next sector selected
+        CONT:   descend into the scans of this sector
+        QUIT:   return to the file-header level
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/obscure_bugs.txt b/obscure_bugs.txt
new file mode 100644
index 0000000000000000000000000000000000000000..fb821540ca2edceb402d15d0710bc909b43d15f9
--- /dev/null
+++ b/obscure_bugs.txt
@@ -0,0 +1,26 @@
+obscure_bugs.txt
+
+A collection of obscure Newstar bugs and their antidotes
+--------------------------------------------------------
+
+	Like any system its size, Newstar is sensitive to programming errors
+that are eaily made. Some of these may result in very obscure behaviour that
+may be difficult to diagnose. This document is meant to formalise our
+collective knowledge in this area. Anyone who solves a problem of this type is
+invited to record his experience here so others after him may benefit from it.
+
+
+Symptom: When exiting, the program emits a series of messages
+-------
+	mv: <file name> is identical to <filename>
+
+Cause: The first argument in a WNCTXT call should be a bitmask (normally F_T or
+F_TP). Omitting it or putting something else in its place may cause this type
+of behaviour.
+(JPH 940909)
+
+
+Symptom: Program crashes with IOT 6 (?)
+-------
+Cause: Division by 0 (and probably other arithmetic exceptions)
+(JPH 940909)
diff --git a/people.ps b/people.ps
new file mode 100644
index 0000000000000000000000000000000000000000..9691bdaba2f1a55b1e24e0b608098b004bb40e48
--- /dev/null
+++ b/people.ps
@@ -0,0 +1,258 @@
+%!PS-Adobe-2.0
+%%Creator: dvipsk 5.66a Copyright 1986-97 Radical Eye Software (www.radicaleye.com)
+%%Title: people_tmp.dvi
+%%Pages: 1
+%%PageOrder: Ascend
+%%BoundingBox: 0 0 596 842
+%%EndComments
+%DVIPSCommandLine: dvips -o /newstar/master/hlp/people.ps people_tmp.dvi
+%DVIPSParameters: dpi=300, compressed
+%DVIPSSource:  TeX output 1997.06.13:0915
+%%BeginProcSet: texc.pro
+%!
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+mul N /landplus90{false}def /@rigin{isls{[0 landplus90{1 -1}{-1 1}
+ifelse 0 0 0]concat}if 72 Resolution div 72 VResolution div neg scale
+isls{landplus90{VResolution 72 div vsize mul 0 exch}{Resolution -72 div
+hsize mul 0}ifelse TR}if Resolution VResolution vsize -72 div 1 add mul
+TR[matrix currentmatrix{dup dup round sub abs 0.00001 lt{round}if}
+forall round exch round exch]setmatrix}N /@landscape{/isls true N}B
+/@manualfeed{statusdict /manualfeed true put}B /@copies{/#copies X}B
+/FMat[1 0 0 -1 0 0]N /FBB[0 0 0 0]N /nn 0 N /IE 0 N /ctr 0 N /df-tail{
+/nn 8 dict N nn begin /FontType 3 N /FontMatrix fntrx N /FontBBox FBB N
+string /base X array /BitMaps X /BuildChar{CharBuilder}N /Encoding IE N
+end dup{/foo setfont}2 array copy cvx N load 0 nn put /ctr 0 N[}B /df{
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+/base get 2 index get S /BitMaps get S get /ch-data X pop /ctr 0 N ch-dx
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+setcachedevice ch-width ch-height true[1 0 0 -1 -.1 ch-xoff sub ch-yoff
+.1 sub]/id ch-image N /rw ch-width 7 add 8 idiv string N /rc 0 N /gp 0 N
+/cp 0 N{rc 0 ne{rc 1 sub /rc X rw}{G}ifelse}imagemask restore}B /G{{id
+gp get /gp gp 1 add N dup 18 mod S 18 idiv pl S get exec}loop}B /adv{cp
+add /cp X}B /chg{rw cp id gp 4 index getinterval putinterval dup gp add
+/gp X adv}B /nd{/cp 0 N rw exit}B /lsh{rw cp 2 copy get dup 0 eq{pop 1}{
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+adv}B /rsh{rw cp 2 copy get dup 0 eq{pop 128}{dup 255 eq{pop 127}{dup 2
+idiv S 128 and or}ifelse}ifelse put 1 adv}B /clr{rw cp 2 index string
+putinterval adv}B /set{rw cp fillstr 0 4 index getinterval putinterval
+adv}B /fillstr 18 string 0 1 17{2 copy 255 put pop}for N /pl[{adv 1 chg}
+{adv 1 chg nd}{1 add chg}{1 add chg nd}{adv lsh}{adv lsh nd}{adv rsh}{
+adv rsh nd}{1 add adv}{/rc X nd}{1 add set}{1 add clr}{adv 2 chg}{adv 2
+chg nd}{pop nd}]dup{bind pop}forall N /D{/cc X dup type /stringtype ne{]
+}if nn /base get cc ctr put nn /BitMaps get S ctr S sf 1 ne{dup dup
+length 1 sub dup 2 index S get sf div put}if put /ctr ctr 1 add N}B /I{
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+%%EndSetup
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+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/people/images.pl b/people/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/people/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/people/labels.pl b/people/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..5f5dc7297fc94558324916d689165ebff4e13b1a
--- /dev/null
+++ b/people/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{"cmv"} ="$URL/people.html"; 
+$external_labels{"agb"} ="$URL/people.html"; 
+$external_labels{"jph"} ="$URL/people.html"; 
+$external_labels{"wnb"} ="$URL/people.html"; 
+$external_labels{"hjv"} ="$URL/people.html"; 
+$external_labels{"jen"} ="$URL/people.html"; 
+
+1;
\ No newline at end of file
diff --git a/people/people.html b/people/people.html
new file mode 100644
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+<HEAD>
+<TITLE>Newstar Project Team</TITLE>
+</HEAD>
+<BODY><P>
+<P>
+<b>NFRA/ASTRON</b>
+<P>
+Stichting Astronomisch Onderzoek in Nederland <BR>Netherlands Foundation for Reasearch in Astronomy <BR>P.O. Box 2 <BR>NL-7990 AA Dwingeloo <BR>Phone: +31 521 595100
+<P>
+<UL><LI>   General eMail account: <b> 
+        <a href="mailto:newstar@nfra.nl">newstar@nfra.nl</a> 
+        </b>
+<P>
+<LI>   Jan Noordam      Project Manager        <A NAME=jen><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> <i>JEN</i> 
+        (eMail: 
+         
+                <a href="mailto:noordam@nfra.nl">noordam@nfra.nl</a> 
+        ) 
+         
+                <IMG ALIGN=RIGHT SRC=../src/doc/bin/jen.gif> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br>
+<P>
+<LI>   Ger de Bruyn     Project Scientist      <A NAME=agb><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> <i>AGB</i> 
+        (eMail: 
+         
+                <a href="mailto:ger@nfra.nl"> ger@nfra.nl</a> 
+        ) 
+         
+                <IMG ALIGN=RIGHT SRC=../src/doc/bin/agb.gif> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br>
+<P>
+<LI>   Johan Hamaker                           <A NAME=jph><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> <i>JPH</i> 
+        (eMail: 
+         
+                <a href="mailto:hamaker@nfra.nl"> hamaker@nfra.nl</a> 
+        ) 
+         
+                <IMG ALIGN=RIGHT SRC=../src/doc/bin/jph.gif> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br>
+<P>
+<LI>   Henk Vosmeijer                          <A NAME=hjv><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> <i>HjV</i> 
+        (eMail: 
+         
+                <a href="mailto:vosmeijer@nfra.nl"> vosmeijer@nfra.nl</a> 
+        ) 
+         
+                <IMG ALIGN=RIGHT SRC=../src/doc/bin/hjv.gif> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br>
+<P>
+<LI>   Marco de Vos                            <A NAME=cmv><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> <i>CMV</i> 
+        (eMail: 
+         
+                <a href="mailto:devoscm@nfra.nl"> devoscm@nfra.nl</a> 
+        ) 
+         
+                <IMG ALIGN=RIGHT SRC=../src/doc/bin/cmv.gif> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br>
+<P>
+<LI>   Wim Brouw                               <A NAME=wnb><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> <i>WNB</i> 
+        (eMail: 
+         
+                <a href="mailto:wbrouw@atnf.csiro.au"> wbrouw@atnf.csiro.au</a> 
+        ) 
+         
+                <IMG ALIGN=RIGHT SRC=../src/doc/bin/wnb.gif> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br> 
+                <br>
+<P>
+</UL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+2995 y(4)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/plate_measure/_11313_tex2html_wrap202.png b/plate_measure/_11313_tex2html_wrap202.png
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new file mode 100644
index 0000000000000000000000000000000000000000..0abe966af01ba75382d3c9566d76f3ada1004c00
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+++ b/plate_measure/_11313_tex2html_wrap202.xbm
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+#define noname_height 11
+static char noname_bits[] = {
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new file mode 100644
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--- /dev/null
+++ b/plate_measure/_11313_tex2html_wrap204.xbm
@@ -0,0 +1,5 @@
+#define noname_width 13
+#define noname_height 8
+static char noname_bits[] = {
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+ 0x02};
diff --git a/plate_measure/images.pl b/plate_measure/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..d5705b1939bc576ac69722f6b5dbe84b03676d97
--- /dev/null
+++ b/plate_measure/images.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$;html_special_mark_gt;70^circ${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11313_tex2html_wrap202.xbm">'; 
+$key = q/{}$rightarrow${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11313_tex2html_wrap204.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/plate_measure/labels.pl b/plate_measure/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..5fa70bf23300b0cc5dd7cb47b7d1a963fe2dfdb4
--- /dev/null
+++ b/plate_measure/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/plate_measure.html"; 
+$external_labels{".pos"} ="$URL/plate_measure.html"; 
+$external_labels{".login"} ="$URL/plate_measure.html"; 
+$external_labels{".solve"} ="$URL/plate_measure.html"; 
+$external_labels{".diff"} ="$URL/plate_measure.html"; 
+$external_labels{".run"} ="$URL/plate_measure.html"; 
+
+1;
\ No newline at end of file
diff --git a/plate_measure/plate_measure.html b/plate_measure/plate_measure.html
new file mode 100644
index 0000000000000000000000000000000000000000..935aba75ad7ae28db6dcf55cc8db19f8cad45cb6
--- /dev/null
+++ b/plate_measure/plate_measure.html
@@ -0,0 +1,165 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Dwingeloo Plate Measuring Machine</b>
+<P>
+A <i>NEWSTAR </i> Guide to Determining Positions Using the Dwingeloo Plate Measuring Machine.
+<P>
+<i>Original by James Albinson, July 1983 <BR>Version 3, updated by Richard Strom, October 1992</i>
+<P>
+<i>For Problems, questions, complaints, suggestions on use and operation: See Richard Strom, alternatively Ger der Bruyn. <BR>In case of mechanical/electrical failures: See Jean Casse</i>.
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0001000000000000000> <b>Introduction</b></A></H1>
+<P>
+This document is based on previous versions by Seth Shostak and Bob Hanisch, and gives a simple procedure for measuring the positions of objects from the PSS prints or KPNO plates.  The general procedure is as follows:  
+<BR>(1) identify standard stars from an overlay of the region of interest,  
+<BR>(2) measure the positions of a number of standard stars and the desired objects,  
+<BR>(3) solve for the plate constants and the positions of the desired objects. A guide to these procedures is given below.
+<P>
+<A NAME=.login><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000> <b>Logging in</b></A></H1>
+<P>
+Turn on the terminal next to the measuring machine and the yellow Interloop interface to which it should be connected. (If the interface is off, there will be no response from the terminal. If the terminal is disconnected from the interface, you will have to ask for help to connect it up.) If you get the server prompt (`Server &gt;'), connect to the RZMVX4 computer (`c' should be enough) and log in under `measure', password: meas$$92
+<P>
+You now need to type the following command: assign user1: qd2:
+<P>
+You're now ready to run the OVERLAY program.
+<P>
+<A NAME=.run><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>Running the OVERLAY program</b></A></H1>
+<P>
+Type: exe overlay
+<P>
+The program will ask for a right ascension and declination; these refer to the field center you're interested in.  For example, if you want to find star positions around a galaxy, type the position of the galaxy.
+<P>
+An example:  
+<BR>RA_MAPCENTRE(RA of map_centrein h,m,s): 4,2,35.000  
+<BR>DEC_MAPCENTRE(DEC of map_centrein d,m,s): 69,40,42.00  
+<BR>For negative declinations simply prefix the declination degrees with a minus sign.
+<P>
+OVERLAY will produce some output on the lineprinter and an overlay plot on the QMS printer/plotter. It may be desirable to make the plot on a transparent sheet; in that case special Xerox transparent overhead sheets can be loaded in the QMS printer (check with other users first, and only load as many sheets as you need). Take the plot and identify your standard stars. If the plot was made on paper, you can circle the stellar positions on a plastic sheet using a marking pen that can be obtained from the secretaries. It is also helpful to label the stars with the same numbers that appear on the OVERLAY plot, as you will have to enter these numbers when measuring the positions. On the other hand, you may not want to write too much stuff on the plastic sheet as this may obliterate objects that you want to measure. Since it is not possible to measure any more than 30 standard stars, be sure that you select standard stars with numbers between 1 and 30. (OVERLAY numbers the stars in order of increasing distance from the field center.)
+<P>
+Special note for very northerly fields (dec <IMG ALIGN=BOTTOM ALT="" SRC="_11313_tex2html_wrap202.png">): For very northerly fields it is more convenient to make the overlays with a Schmidt projection rather than a linear projection (which is the default).  To do this type in the command @schmidt. This will produce plots with the Schmidt projection for all subsequent runs of OVERLAY.  To go back to a linear projection, simply type the command @linear.
+<P>
+Special note for measuring several fields: You should complete your measurements for each field before proceeding to the next field. The reason for this is that the program which solves for the plate constants and object positions uses the standard star positions from the most recent run of OVERLAY.
+<P>
+<A NAME=.pos><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000> <b>Measuring positions</b></A></H1>
+<P>
+Preliminaries. Turn on the plate illumination light. The switch is on top of the green box behind the measuring machine. Turn on the Television camera and monitor screen. The switch for this is the leftmost of the three rotary switches on the front of the monitor. Make sure that the lowest of the 7 channel knobs on the right-hand edge of the monitor is selected. After a few seconds the monitor should show an image. The brightness and contrast knobs are the other two rotary knobs on the front of the monitor. Adjust to suit. The focus knob is below and to the right of the eyepiece, facing the front of the machine. Adjust as necessary.
+<P>
+Place the ``sandwich&quot; of PSS print and plastic overlay between the glass plates of the measuring machine.  The orientation is not important.  Adjust the measuring machine so that the axes are set at the center of their travel (x-axis at 10.0, y-axis at 9.0). Then release the gray clamps, center the microscope over your field, and retighten the clamps.
+<P>
+Turn on the interface (white rocker switch on right) and make sure the mode switch is set to `TERMINAL'.  Turn on the two Sony Magnescale digital readouts and the illuminating lamp, if you haven't already (switch is on the little green box). Adjust the lamp for good illumination, and use the knurled knob to focus the image through the microscope (if no TV).  Push the `START/READ' switch on the interface.
+<P>
+Start up the measuring machine program by typing: exe measure
+<P>
+The program asks you if you want a new file. To start measuring a new field, answer this question with `y'. To continue measuring on a field still in position on the measuring machine, answer with `n'.
+<P>
+Set the mode switch on the interface chassis to `TRANSMIT'. Measure your standard stars (in any order) as follows:  
+<OL><LI> Center the standard star in the crosshairs.  
+<LI> Set the thumbswitches on the interface to the number of the standard star from the OVERLAY plot (i.e., a number between 01 and 30).  
+<LI> Push the `START/READ' switch.  This sends the x-y coordinates of the star to the computer, and you should also see them dispayed on the terminal.  
+</OL>
+<P>
+Repeat steps 1-3 for each standard star you want to measure (10 to 15 stars are usually sufficient).  Since there is no backlash in the digital readout, it is not necessary to repeat your measurements or to approach each star from the same direction.
+<P>
+If you have a large number of radio sources to identify and would like to have approximate x-y positions around which to look for optical identifications, skip from here to <A HREF="#.diff">section</A>.
+<P>
+Measure the ``unknown'' objects (stars, galaxies, or whatever) in the same manner, but set the thumbswitches to numbers between 31 and 98, incrementing the count by one for each object you measure. You may, of course, measure the objects in any order you find convenient. The x-y positions will continue to be displayed on the terminal, but the object number will be the thumbswitch setting minus 30.
+<P>
+When you have finished all the positions you want, set the thumbswitches to 99 and push the `START/READ' switch. This terminates the program. <b>Be sure to set the mode switch back to `TERMINAL'.</b>
+<P>
+<A NAME=.solve><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000> <b>Solving for plate constants and positions</b></A></H1>
+<P>
+Start up the program by typing: exe solve
+<P>
+The program asks you for some information about the plate:  
+<BR>- PLATE_TYPE: Type a carriage return if you used a PSS print, or the appropriate code for a KPNO plate.  
+<BR>- FIELDNAME: Type a name (up to 8 characters) of this field.  
+<BR>- TRANSFORM_CODE: Type `1' (x-y <IMG ALIGN=BOTTOM ALT="" SRC="_11313_tex2html_wrap204.png"> alpha,delta)  
+<BR>- PLATE_CENTER(hms,dms): Type the right ascension and declination of the field center in the format shown. These coordinates can be found in the little box in the upper left corner of each PSS print; put a comma between hms dms.
+<P>
+The program now goes on to solve for the plate constants. You have the opportunity to delete certain stars from the solution of plate constants if you have reason to believe that their measured positions are in error.  Assuming that they are all okay, however, just type `return' in response to this question.
+<P>
+- CORRECT_STAND?Type either 'Y' or `return'.
+<P>
+The program now solves for the coordinates of the unknown objects. When the program finishes, you have the option to send the results to be printed on the lineprinter:
+<P>
+- OUTPUT? The default is Y (yes), so type a `return'.  Finally, you may have the positions you've measured added to the standard star positions as secondary standards:
+<P>
+- SECONDARY_STAND?Typically the response is `no' (the default is yes).  You may now pick up your output downstairs from the lineprinter.
+<P>
+If your plate solution looks dubious, i.e., one or more stars have large errors, you can rerun SOLVE and delete these stars from the solution.  Run SOLVE again, and answer the questions concerning the type of plate and field name again.  Hereafter you want to use the same data as before.  SOLVE remembers all of the information from the previous run, and uses this information if you simply answer all of the questions with `return'.  So, answer the questions with `return's until you are asked:
+<P>
+- EXCLUDE_STAND: Type in the numbers in the specified format, and then continue as before to produce a new plate solution.
+<P>
+<A NAME=.diff><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0006000000000000000> <b>A different approach to making source identifications</b></A></H1>
+<P>
+If you have a large number of radio sources you want to try to identify, you could spend an eternity measuring candidate objects unless you know where on the plate to look.  It is possible to use SOLVE to get x-y positions for given radio source positions (in right ascension and declination epoch 1950), and these x-y positions can then be used as guides in measuring candidate objects.
+<P>
+To make use of this option, you must measure some standard star positions in the field of interest as <A HREF="#.pos">previously described</A>. Rather than measuring any unknown objects at this time, however, terminate MEASURE (set thumbswitches to 99 and push the `START/READ' switch) and run SOLVE (see  
+<A HREF="#.solve">section</A>). You will need to run SOLVE twice, first to check that your standard stars have been measured accurately (check the rms fit and the individual errors; if one or two stars are bad delete them from the fit the next time around), and second to convert given alphas and deltas (i.e. your radio source positions) to x-y coordinates.
+<P>
+Now run SOLVE a second time.  When the program asks you for the type of transformation (TRANSFORM_CODE), type a `2', i.e., transform (alpha,delta) <IMG ALIGN=BOTTOM ALT="" SRC="_11313_tex2html_wrap204.png"> (x,y). The program will then ask you to enter the coordinates of your source positions. You should type all of the alphas and deltas in the given format, (put a blank between alpha delta as opposed to a comma), and terminate your input with a blank line (i.e. an extra `return'). The rest of the program is then run in the same way as described previously in section  
+.
+<P>
+The output from SOLVE will now contain a list of x-y coordinates for your source positions.  You can use these to set the measuring machine to the appropriate position, and then measure candidate objects in the vicinity.  To do this, run MEASURE as described in steps III.a-d. However, when you are asked:
+<P>
+- NEWFILE? type a `no' (i.e., use the Old file).  The program then asks you how many objects were measured in the previous run of the program (it should be able to keep count itself, but this is a very stupid program):
+<P>
+- OLD_OBJECTS?Type in the number of objects previously measured.  This is <i>not</i> the highest numbered standard star, but rather simply the total number of objects measured.  At this point you can measure the positions of candidate objects just as in step III.f.  It is not necessary to measure any standard star positions again (i.e., skip step ...), as your unknown object x-y positions are simply being appended to your previous measurements.
+<P>
+When you have finished, please do not forget to logout; just type `lo' on the terminal. Turn off all the bits of the measuring machine and put the green cover over the camera and table. Put any PSS prints carefully back in their folders, and replace them at the right place in the cabinet.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/plotter/plotter__plot_format.html b/plotter/plotter__plot_format.html
new file mode 100644
index 0000000000000000000000000000000000000000..6aa4510a036d63fbc75af91d39c7d6a1af224f29
--- /dev/null
+++ b/plotter/plotter__plot_format.html
@@ -0,0 +1,18 @@
+<TITLE>Description of PLOT_FORMAT (PLOTTER)</TITLE>
+<H1>Description of general keyword PLOT_FORMAT</H1>
+
+<DT><EM>Prompt:</EM> A&lt;n&gt;-format of plot 0, 1, 2, 3, 4
+<DT><EM>Default:</EM> 4 /ASK.
+<DT><EM>Expected input:</EM> Character(1).<P>
+ Select format for (Encapsulated) PostScript plots: 
+	0 = A0 
+	1 = A1 
+	2 = A2 
+	3 = A3 
+	4 = A4 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../plotter/plotter_comm.html">List of general keywords</A> for PLOTTER
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/plotter/plotter__plotter.html b/plotter/plotter__plotter.html
new file mode 100644
index 0000000000000000000000000000000000000000..ed52d46861338864df6ca360de8a540547a406a5
--- /dev/null
+++ b/plotter/plotter__plotter.html
@@ -0,0 +1,31 @@
+<TITLE>Description of PLOTTER (PLOTTER)</TITLE>
+<H1>Description of general keyword PLOTTER</H1>
+
+<DT><EM>Prompt:</EM> plotter to use X11;  QMS, QMSP;  PL, PP, EL, EP;|-REGIS, FREGIS;  BIT1, BIT2, BIT3
+<DT><EM>Expected input:</EM> Character(8).<P>
+ Select device/mode for plotting: <P>
+    Xwindows: 
+	X11     X11 terminal 
+		The display used is given by (NGEN-) keyword DISPLAY 
+		and/or the environment variable DISPLAY <P>
+    PostScript printer: 
+	QMS     QMS laser printer in landscape orientation 
+	QMSP    QMS laser printer in portrait orientation <P>
+    PostScript files:: 
+	PL      Postscript file in landscape mode 
+	PP      PostScript file in portrait mode 
+	EL      Encapsulated Postscript file in landscape mode 
+	EP      Encapsulated Postscript file in portrait mode <P>
+    Miscellaneous graphics: 
+	REGIS   graphics VT terminal 
+	FREGIS  (*) REGIS to file <P>
+    Bitmap graphics: 
+	BIT1    (*) bitmap for 100 dpi 
+	BIT2    (*) bitmap for 200 dpi 
+	BIT3    (*) bitmap for 300 bpi 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../plotter/plotter_comm.html">List of general keywords</A> for PLOTTER
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/plotter_comm/plotter_comm.html b/plotter_comm/plotter_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..69e7a5346e8197a4ba3b3e69c8313d95ed57f4c6
--- /dev/null
+++ b/plotter_comm/plotter_comm.html
@@ -0,0 +1,17 @@
+<TITLE>Index of general keywords from PLOTTER</TITLE>
+<H1>Description of general keywords (PLOTTER)</H1>
+
+<UL>
+<LI> <A HREF="../plotter/plotter__plotter.html">
+  PLOTTER</A>
+  plotter to use X11;  QMS, QMSP;  PL, PP, EL, EP;|-REGIS, FREGIS;  BIT1, BIT2, BIT3
+<LI> <A HREF="../plotter/plotter__plot_format.html">
+  PLOT_FORMAT</A>
+  A&lt;n&gt;-format of plot 0, 1, 2, 3, 4
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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+b(of)i(the)g(individu)o(al)e(parameters)917 b(1)62 548
+y Fe(2.1)56 b(References)16 b(to)d(public)h(in)o(terfaces)31
+b(.)20 b(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)
+f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)71
+b(1)62 606 y(2.2)56 b(P)o(arameter)13 b(PLOTTER)g(.)20
+b(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h
+(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)
+f(.)g(.)71 b(1)62 664 y(2.3)56 b(P)o(arameter)13 b(PLOT)p
+492 664 13 2 v 16 w(F)o(ORMA)m(T)30 b(.)20 b(.)g(.)h(.)f(.)g(.)g(.)h(.)
+f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)g(.)h(.)f(.)g(.)h(.)f
+(.)g(.)g(.)h(.)f(.)g(.)h(.)f(.)g(.)71 b(2)0 942 y Fg(1)89
+b(Ov)n(erview)0 1056 y Fe(This)10 b(do)q(cumen)o(t)f(con)o(tains)g(an)h
+(o)o(v)o(erview)f(of)g(the)i(public)e(parameter)g(group)h(PLOTTER,)f
+(\(part)h(of)s(\))g(whic)o(h)f(is)h(included)0 1106 y(in)j(sev)o(eral)i
+Fd(NEWST)m(AR)e Fe(programs.)118 1178 y(sho)o(w)118 1251
+y(The)h(do)q(cumen)o(t)f(describ)q(es)j(the)e(individual)d(parameters)j
+(in)f(alphab)q(etical)g(order.)18 b(This)c(description)g(cen)o(ters)0
+1301 y(on)e(the)h(Help)f(texts,)h(whic)o(h)f(ha)o(v)o(e)g(b)q(een)i
+(designed)f(to)f(guide)g(the)g(user)i(to)e(the)h(prop)q(er)g(c)o(hoice)
+f(at)h(eac)o(h)f(junction,)g(ev)o(en)0 1351 y(if)h(his)h(kno)o(wledge)f
+(of)h(the)g(o)o(v)o(erall)f(w)o(orkings)g(of)h(the)g(program)e(is)i
+(only)f(sup)q(er\014cial.)118 1424 y(Please)18 b(note)g(that)f(the)h
+(generic)h(prompt)d(and)h(help)h(texts)g(de\014ned)g(for)f(these)i
+(parameters)f(are)f(frequen)o(tly)0 1474 y(sup)q(erseded)h(in)c(the)i
+(actual)e(applications)g(b)o(y)h(alternativ)o(e)f(texts)i(that)f(are)h
+(more)d(appropriate)i(to)g(the)h(situation)e(at)0 1523
+y(hand.)20 b(Unfortunately)m(,)14 b(the)i(presen)o(t)g(arc)o(hitecture)
+g(of)f Fd(NEWST)m(AR)f Fe(precludes)i(the)g(inclusion)e(of)g(suc)o(h)h
+(texts)h(in)e(the)0 1573 y(do)q(cumen)o(tation)d(system,)h(so)h(the)g
+(only)e(opp)q(ortunit)o(y)i(to)f(read)h(that)f(information)e(is)i
+(during)g(program)f(execution)i(\(in)0 1623 y(y)o(our)h(terminal)e
+(windo)o(w!\).)0 1782 y Fg(2)89 b(Descriptions)23 b(of)f(the)g(indivi)q
+(dual)k(parameters)0 1905 y Fc(2.1)74 b(References)17
+b(to)i(public)f(in)n(terfaces)0 2013 y(2.2)74 b(P)n(arameter)18
+b(PLOTTER)0 2112 y Fh(Pr)n(ompt:)g Fe(plotter)c(to)g(use)h(\()p
+Fh(may)g(vary)g(p)n(er)f(applic)n(ation)p Fe(\))0 2162
+y Fh(Exp)n(e)n(cte)n(d)h(input:)k Fe(Character)c(*8:)i(1)d(v)n(alue)157
+2232 y Fb(Select)j(device/mod)o(e)g(for)h(plotting:)78
+2304 y(Xwindows:)157 2350 y(X11)97 b(X11)18 b(terminal)314
+2396 y(The)g(display)f(used)h(is)h(given)f(by)h(\(NGEN-\))e(keyword)f
+(DISPLAY)314 2441 y(and/or)h(the)i(environm)o(ent)d(variable)g(DISPLAY)
+78 2513 y(PostScript)g(printer:)157 2559 y(QMS)97 b(QMS)18
+b(laser)g(printer)f(in)i(landscape)d(orientati)o(on)157
+2605 y(QMSP)77 b(QMS)18 b(laser)g(printer)f(in)i(portrait)d(orientatio)
+o(n)78 2677 y(PostScript)g(files::)157 2723 y(PL)117
+b(Postscrip)o(t)17 b(file)h(in)g(landscape)f(mode)157
+2768 y(PP)117 b(PostScrip)o(t)17 b(file)h(in)g(portrait)f(mode)157
+2814 y(EL)117 b(Encapsula)o(ted)16 b(Postscrip)o(t)h(file)h(in)g
+(landscape)f(mode)157 2860 y(EP)117 b(Encapsula)o(ted)16
+b(Postscrip)o(t)h(file)h(in)g(portrait)f(mode)935 2995
+y Fe(1)p eop
+%%Page: 2 2
+2 1 bop 78 0 a Fb(Miscellaneo)o(us)16 b(graphics:)157
+46 y(REGIS)57 b(graphics)16 b(VT)j(terminal)157 92 y(FREGIS)37
+b(\(*\))18 b(REGIS)g(to)h(file)78 171 y(Bitmap)f(graphics:)157
+216 y(BIT1)77 b(\(*\))18 b(bitmap)g(for)g(100)g(dpi)157
+262 y(BIT2)77 b(\(*\))18 b(bitmap)g(for)g(200)g(dpi)157
+308 y(BIT3)77 b(\(*\))18 b(bitmap)g(for)g(300)g(bpi)0
+465 y Fc(2.3)74 b(P)n(arameter)18 b(PLOT)p 578 465 17
+2 v 20 w(F)n(ORMA)-5 b(T)0 567 y Fh(Pr)n(ompt:)18 b Fe(A)p
+Fa(<)p Fe(n)p Fa(>)p Fe(-format)13 b(of)g(plot)g(\()p
+Fh(may)i(vary)g(p)n(er)g(applic)n(ation)p Fe(\))0 617
+y Fh(Exp)n(e)n(cte)n(d)g(input:)k Fe(Character)c(*1:)i(1)d(v)n(alue)157
+691 y Fb(Select)j(format)h(for)g(\(Encapsul)o(ate)o(d\))e(PostScript)g
+(plots:)157 737 y(0)j(=)g(A0)157 783 y(1)g(=)g(A1)157
+828 y(2)g(=)g(A2)157 874 y(3)g(=)g(A3)157 920 y(4)g(=)g(A4)935
+2995 y Fe(2)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/plotter_public_intfc/_12327_tex2html_wrap179.png b/plotter_public_intfc/_12327_tex2html_wrap179.png
new file mode 100644
index 0000000000000000000000000000000000000000..b9595289c5c2a9bf084a8543d7a8440fb4cd0876
Binary files /dev/null and b/plotter_public_intfc/_12327_tex2html_wrap179.png differ
diff --git a/plotter_public_intfc/_12327_tex2html_wrap179.xbm b/plotter_public_intfc/_12327_tex2html_wrap179.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..357f3a9a8f20ce616316aee6afe509b7e67f2961
--- /dev/null
+++ b/plotter_public_intfc/_12327_tex2html_wrap179.xbm
@@ -0,0 +1,5 @@
+#define noname_width 24
+#define noname_height 9
+static char noname_bits[] = {
+ 0x80,0x01,0x00,0xe0,0x00,0x00,0x38,0x80,0x7f,0x0e,0x80,0xcd,0x03,0x00,0xff,
+ 0x0f,0x80,0x0d,0x3c,0xc0,0x8c,0xf0,0x80,0x7f,0xc0,0x01,0x00};
diff --git a/plotter_public_intfc/images.pl b/plotter_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..7efff9290561cb73bc56d2bfd0add39bd081fbaf
--- /dev/null
+++ b/plotter_public_intfc/images.pl
@@ -0,0 +1,7 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$;html_special_mark_lt;${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12327_tex2html_wrap179.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/plotter_public_intfc/labels.pl b/plotter_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..af8c13f8f6be85c513a0d4ec9ba13978a86a8ebe
--- /dev/null
+++ b/plotter_public_intfc/labels.pl
@@ -0,0 +1,10 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/plotter_public_intfc.html"; 
+$external_labels{".plot.format"} ="$URL/plotter_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/plotter_public_intfc.html"; 
+$external_labels{".plotter"} ="$URL/plotter_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/plotter_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/plotter_public_intfc/plotter_public_intfc.html b/plotter_public_intfc/plotter_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..55136f2979beae670b731a75f965ab56516704fc
--- /dev/null
+++ b/plotter_public_intfc/plotter_public_intfc.html
@@ -0,0 +1,137 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group PLOTTER</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=plotter_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=plotter_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=plotter_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=plotter_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=plotter_public_intfc.html#SECTION0003200000000000000>  <b>Parameter PLOTTER</b></A>
+<LI> <A NAME=tex2html6 HREF=plotter_public_intfc.html#SECTION0003300000000000000>  <b>Parameter PLOT_FORMAT</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group PLOTTER, (part of) which is included in several <i>NEWSTAR </i> programs. 
+show
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.plotter><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter PLOTTER</b></A></H2>
+<P>
+  <em>Prompt:</em> plotter to use (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *8:  1 value
+<P>
+    <PRE>
+        Select device/mode for plotting:
+</PRE>
+<P>
+  <PRE>
+    Xwindows:
+        X11     X11 terminal
+                The display used is given by (NGEN-) keyword DISPLAY
+                and/or the environment variable DISPLAY
+</PRE>
+<P>
+  <PRE>
+    PostScript printer:
+        QMS     QMS laser printer in landscape orientation
+        QMSP    QMS laser printer in portrait orientation
+</PRE>
+<P>
+  <PRE>
+    PostScript files::
+        PL      Postscript file in landscape mode
+        PP      PostScript file in portrait mode
+        EL      Encapsulated Postscript file in landscape mode
+        EP      Encapsulated Postscript file in portrait mode
+</PRE>
+<P>
+  <PRE>
+    Miscellaneous graphics:
+        REGIS   graphics VT terminal
+        FREGIS  (*) REGIS to file
+</PRE>
+<P>
+  <PRE>
+    Bitmap graphics:
+        BIT1    (*) bitmap for 100 dpi
+        BIT2    (*) bitmap for 200 dpi
+        BIT3    (*) bitmap for 300 bpi
+</PRE>
+<P>
+<A NAME=.plot.format><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter PLOT_FORMAT</b></A></H2>
+<P>
+<em>Prompt:</em> A<IMG ALIGN=BOTTOM ALT="" SRC="_12327_tex2html_wrap179.png">n&gt;-format of plot (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *1:  1 value
+<P>
+  <PRE>
+        Select format for (Encapsulated) PostScript plots:
+        0 = A0
+        1 = A1
+        2 = A2
+        3 = A3
+        4 = A4
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/ppd_buffer.txt b/ppd_buffer.txt
new file mode 100644
index 0000000000000000000000000000000000000000..0911b64813ab5d032c5abddabed43bc105256ca7
--- /dev/null
+++ b/ppd_buffer.txt
@@ -0,0 +1,41 @@
+Aanpassen van de grootte van de ppd help-text buffer
+----------------------------------------------------
+
+(bijdrage van H.J. Vosmeijer/J.P. Hamaker, 940829)
+
+
+Als het compileren van een .pin/.psc/.pef file stuk loopt op een te kleine
+werk-buffer in sys_bldppd, moeten zowel deze buffer als een daarmee
+corresponderende buffer in de Newstar executables worden vergroot. Dit veresit
+de volgende wijzigingen in files in $n_src/dwarf, gevolgd door een gepaste
+reeks 'nsh build's
+
+
+Om de werk-buffer in cpl_2.def te vergroten moet het volgende
+gebeuren (b.v. van 5000  naar 10000 bytes):
+
+In cpl_2.def:
+  1. verander 5000 in 10000 in parameter (cpl__wrklmax = 5000)
+
+  2. verander 5000 in 10000 in parameter (cpl_wrkbuf = 421)  !&5000 !#C
+
+  3. hoog alle adressen op met 5000 (=(nieuw-oud)=(10000-5000)) voor de
+     variabelen die  NA  CPL_WRKBUF  en  VOOR  CPL__LENGTH  komen.
+     Dit zijn dus de waarden na het = teken)
+
+  4. pas CPL__LENGTH aan (=(CPL_ERRNTOT+3)/4)
+
+  5. verander 5000 in 10000 in CHARACTER*5000 CPL$WRKBUF
+
+  6. hoog alle waarden op met 5000 (=(nieuw-oud)=(10000-5000)) voor de
+     variabelen die  NA  CPL$WRKBUF  komen.
+
+In onderstaande files in genoemde regels 5000 in 10000 veranderen:
+   cplblock.for:   CHARACTER*5000  CPL$WRKBUF
+   cplread.for:    CHARACTER       KEYWORD*80, VALUE*5000
+   bpdbuild.for:   CHARACTER       VALUE*5000
+   bpdstore.for:   CHARACTER       STRING*5000, NAME*16
+   ppdhelp.fsc:    CHARACTER       WORK*5000, WORK2*80, LINE*80
+   ppdprompt.for:  CHARACTER       WORK*5000, PROGSTRM*80, KEYWORD*16
+
+
diff --git a/psc_guide.txt b/psc_guide.txt
new file mode 100644
index 0000000000000000000000000000000000000000..9d668a575afe8627f4f00a0aa5d635dc29f62484
--- /dev/null
+++ b/psc_guide.txt
@@ -0,0 +1,360 @@
+Style guide for parameter definition files
+------------------------------------------
+
+History:
+ 941110 contributed by JPH
+ 941117 Style recommendation 7.
+ 941212 Revise the latter following changes in cplvallist.for, ppdopstr.for.
+
+
+Summary
+=======
+
+	This document contains guidelines for writing .psc/.pef parameter
+definition files. A few implementation notes are added as an Appendix. The
+following subjects are addressed:
+
+	a. Definition of parameter properties
+
+	b. Definition of default values
+
+	c. Prompt formatting
+
+	d. Insertion of hypertext references
+
+
+Related documents
+=================
+
+	The reader is assumed to have some knowledge of LaTeX and the way it is
+used for Newstar documentation. The latter is described in the Newstar document
+"Guide for writing and maintaining Newstar documents".
+
+
+Definition of parameter properties
+==================================
+
+	A large number of properties can be defined for each parameter. I
+discuss only a few.
+
+	- ATTRIBUTES=<attr>[,<attr>]...
+
+	  . LOOP: WNDPAR returns the special status DWC_ENDOFLOOP when no more
+parameter values are available. The calling program may detect this status as a
+signal for some special action. When LOOP is not specified, the value(s)
+specified is/are simply re-used.
+
+	  . NULL_VALUES: It is allowed to enter 0 values, either by default or
+by the user. A null value is represented by an empty string: "". For a null
+reply, WNDPAR returns <number of values>=0.
+
+	  . WILD_CARDS: A wildcard, *, is allowed as default or reply. For a
+wildcard, WNDPAR returns <number of values>=-1.
+
+In a proper implementation, the latter two attributes should be defined only
+where appropriate. In Newstar, they are declared almost everywhere and
+consequently programs must make special checks in many places for illegitimate
+null and wildcard values.
+
+	This situation is clearly unsatisfactory, but systematic rectification
+is not worth the effort and risk of mistakes. Some efforts in this direction
+have been made but are being discontinued.
+
+
+Definition of parameter defaults
+================================
+
+	Defaults in a prompt can be defined in a number of ways. The DWARF
+design postulated that the interface presented to the user should be defined as
+much as possible in the .psc file; the
+
+	- DEFAULTS=<values>
+
+clause in a keyword description serves this purpose. As an alternative, dynamic
+defaulting can be used.
+
+	Newstar largely ignores this philosophy, by defining most defaults
+through the dynamic mechanism, even when the value is a constant. In some cases
+both .psc and dynamic defaults are provided, - in which case the latter will
+take precedence.
+
+	This situation is clearly unsatisfactory, but systematic rectification
+is not worth the effort and risk of mistakes. Some efforts in this direction
+have been made but are being discontinued.
+
+
+Prompt and options string formatting
+====================================
+
+	A Newstar prompt is composed of
+
+		<keyword> -
+		<prompt text>
+		(<options list>)
+		=<default>:
+
+The complete prompt is concatenated from these components and then formatted
+into one or more lines on the terminal.
+
+	As of november 1994, the formatting routine has been modified to allow
+the programmer more control over the form in which the prompt is displayed,
+through the use of some special punctuation:
+
+	- The prompt string may be terminated in a '|' to put the options
+string on a new line.
+
+	- The options string may contain the characters ' ,;|/[]' to format it:
+
+	  . The '|' can be used to split the string over multiple lines; when
+appended at the and of the list, it signals that the <default> must be put on a
+new line of its own.
+
+	  . ';' and ' ' can be used to group options in functionally related
+subsets;
+
+	  . '/' can be used to group options that are alternatives, e.g.
+BAND/NOBAND.
+
+	  . '[]' can be used to indicate options that one would only use in
+exceptional situations;
+
+	  . '(:)' can be used to insert comments (this may not work, it has not
+been tested).
+
+
+Long and short lines
+--------------------
+
+	Within Newstar a need exists for text files to be formatted as one line
+per full paragraph in some application, and in other uses for the same files to
+be formatted in lines that fit a terminal screen. The conversions can be made
+automatically, provided a few guidelines are heeded: See item 7 of the Style
+Recommendations below.
+
+
+Style recommendations
+---------------------
+
+	1. The '|' character will signal a line break and therefore cannot be
+used otherwise (e.g. as an 'OR' symbol).
+
+	2. If the prompt, options, and default strings combined leave enough
+room for a reply on the same line, donot insert any newlines.
+
+	3. If the options string must be divided over more than one line, then
+put the entire options string on lines of its own (i.e. terminate both the
+prompt and options strings in a '|');
+
+	4. Use blanks and semicolons to visually group the options, and use the
+same grouping in the help text. Insert newlines only between groups, and put a
+semicolon before such a newline.
+
+	5. Remember that the options string will be shown enclosed in
+parentheses. Therefore donot terminate it in a semicolon. (If it ends in a '|',
+that character will be shifted behind the closing parenthesis.)
+
+	6. Format the OPTION string in the way you want it to appear in the
+prompt, remembering that the prompting routine will indent each new line by 4
+blanks: (So donot insert additional blanks in your .psc file!)
+
+	OPTIONS=-
+QUIT; COPY,CCOPY,LINE; ZERO,MANUAL,INIT,RENORM;| -
+EXT,REF, IREF,FAR, IFR,MIFR, SHIFT,CLK; DX,DY,DZ, POLE,FREQ
+
+	7. Make sure the product of the number of options and the LENGTH for
+character parameters is less than 512. (All options are extended by CPL_VALLIST
+to LENGTH characters and concatenated in a local buffer defined by
+PPD_OPSTR_PUT.)
+
+	8. Newstar's automatic line-formatting mechanism may concatenate
+consecutive short lines into a longer one. It does, however, avoid improper
+joining of lines by assuming that the following input line types either start a
+new output line or terminate the current output line or both:
+
+	- a line starting in whitespace, '-' or a '!' comment character: new
+	  output line;
+
+	- a blank line or a line consisting of a '.' only: copy literally;
+
+	- a line containing an in-line comment or a double quote: terminate
+	  output line.
+
+Similarly, a line ending in a hyphen (the DWARF 'to be continued' mark)
+terminates the current output.
+
+
+
+TaTeX/Hypertext conversion of the Help texts
+============================================
+
+	The command 'ndoc Key' translates the files
+
+		<xxx>.psc resp. <xxx>.pef
+
+into LaTeX files
+
+		$n_doc/intfc/<xxx>_private_intfc.tef
+	  resp. $n_doc/intfc/<xxx>_public_intfc.tef
+
+It subsequently calls ndoc Cook to process a corresponding .tex file to produce
+the hypertext document.
+
+	(NOTE: This is a change w.r.t. the previous situation, in which only
+the hypertext translation was available, consisting of one separate small .html
+file per keyword. The logistics for the _intfc.tex/tef files is now entirely
+identical to that for the other .tex documents, which is advantageous in many
+ways.)
+
+
+Cross references
+----------------
+
+	To fully exploit the symmetry between LaTeX sources and the .tef files
+provision is made for cross-references in the latter. These take the form of
+LaTeX \textref commands on comment lines in the .psc/.pef file, e.g.
+
+	! {\em see also the}\textref{DWARF}{<file name>} interface description}
+
+Conversely, references to Help texts can be made both from other Help texts and
+LaTeX documents. For this purpose, ndoc Key generates a label for each help
+text:
+
+	keyword <XXX>_<YYY>_<ZZZ> --> label .<xxx>.<yyy>.<zzz>
+
+
+Appendix: Prompt formatting
+===========================
+
+	The DWARF susbsytem of NEWSTAR is responsible for displaying prompt
+information on the terminal and checking the user's reply. As inherited, the
+formatting of the prompts was very clumsy, making them difficult to read,
+particularly in those frequent cases where a large number of options must be
+chosen from.
+
+	It has proved possible by some very simple changes to give the maker of
+the .psc file, - that defines the prompt and options strings -, a great deal of
+control over the way a prompt is formatted. This is made possible by the fact
+that
+
+	a. Prompt and options strings are copied litterally from the .psc file
+to the binary .ppd file that an executable program reads.
+
+	b. Parsing of the options string relies on a string parameter that
+defines which characters delimit inidividual options in the options string. By
+extending the former string we may allow other characters than ',' to be used
+as delimiters.
+
+	c. The prompt is composed by essentially a simple concatenation of the
+prompt, options and default strings and then breaking it into lines for output
+on the terminal. It is easy to change the line-breaking algorithm to break
+lines at a predefined delimiter character; the vertical bar '|' was chosen for
+this purpose.
+
+	It has later been found that there are other DWARF routines that assume
+that a comma is the only delimiter, such as CPL_VALLIST. These seem to work
+correctly, provided only that the parameter's LENGTH is defined large enough
+(cf. Style recommendation number 7 above.). This can be safely done since this
+attribute is only used to allocate buffer space.
+
+
+Implementation in the prompt and reply paths
+--------------------------------------------
+
+	A schematic of the prompt and reply paths is shown in the following
+diagram:
+
+|GP_INP
+|  calls GP_INP_GET
+|
+|       GP_INP_GET
+|       | calls PPD_PROMPT
+|       |
+|       |       PPD_PROMPT
+|       |         calls PPD_PRSTR_GET to get <prompt string>
+|       |         calls PPD_OPSTR_GET to get <options string>
+|       |         returns with
+|       | PROMPT = <prompt string> (<options string> )'
+|       | appends '=<default string>' to PROMPT
+|       | calls DWC_INPUT with PROMPT
+|       |
+|       |       |DWC_INPUT
+|       |       | calls GEN_INPUT
+|       |       |
+|       |       |       |GEN_INPUT
+|       |       |       | formats prompt and outputs line by line
+									prompt
+******************************************************************************
+									reply
+
+									prompt
+******************************************************************************
+									reply
+|       |       |       | reads answer
+|       |       |       | detects DWC_EOFCTRLZ
+|       |       |       | returns
+|       |       |
+|       |       | returns
+|       |
+|       |  does some checks on ANSWER
+|       |  reprompts for some errors
+|
+| calls GP_INP_PARSE
+| ...
+| calls GP_INP_DECODE
+|
+|       GP_INP_DECODE
+|       | calls PV_BLK_DECODE
+|       | calls PPD_CHECK
+|       |
+|       |       PPD_CDHECK
+|       |       | if options defined:
+|       |       |   calls PPD_OPSTR_MATCH
+|       |       |
+|       |       |       PPD_OPSTR_MATCH
+|       |       |       | calls STR_MATCH_L
+|       |       |       |
+|       |       |       |       STR_MATCH_L
+|       |       |       |       |  returns <match number>
+|       |       |       |
+|       |       |       | loop <match number> times
+|       |       |       |   calls STR_SKIP_U (DELIM=',;|[]',...)
+|       |       |       |
+|       |       |       |       STR_SKIP_U
+|       |       |       |       |       skips up to character in argt DELIM
+|       |       |       |
+|       |       |       | end loop
+|       |       |       | calls STR_SKIP_W
+|       |       |       |
+|       |       |       |       STR_SKIP_W
+|       |       |       |       |       skips whitespace
+|       |       |       |
+|       |       |       | calls STR_COPY_U (DELIM='.;|[]',...)
+|       |       |       |
+|       |       |       |       STR_COPY_U
+|       |       |       |       |       copies up to character in argt DELIM
+|       |       |       |
+|       |       |       |returns full OPTION
+|       |       |
+|       |       |end if
+|       |       |...
+|       |
+|       |...
+| |...
+
+
+	In the prompt path GP_INP_GET and PPD_PROMPT concatenate the keyword,
+prompt, options and default strings in string PROMPT. These strings are taken
+litterally from the .PPD file or WNDPOH without any processing except for the
+insertion of a few punctuation marks to delineate the four components. All
+punctuation marks in the strings are preserved.
+
+	GEN_INPUT formats PROMPT into lines for the terminal. It interprets one
+or more vertical bars '|' as a newline and does not autonomously generate any
+additional newlines. Any lines after the first are indented by 4 spaces; apart
+from this, the formatting is entirely controlled by the bar characters in the
+strings as defined in the .psc file. No checks are made on the lengths of the
+lines being output.
+
+	The reply path uses the options string to check the reply and must
+therefore recognise all punctuation characters. This is realised extremely
+simply by including them in the DELIM argument so STR_SKIP_U and STR_COPY_U
diff --git a/psctest.txt b/psctest.txt
new file mode 100644
index 0000000000000000000000000000000000000000..3f5ad6b78d3f9c12bbc1a7c587ef3d6ecad921f6
--- /dev/null
+++ b/psctest.txt
@@ -0,0 +1,82 @@
+
+
+psctest.csh
+===========
+
+	Options to:
+
+	- Create a .pst file by running program under manual control.
+
+	- Create reference numbers on the parameter lines.
+
+	- Run program under control of a .pst file:
+	  = Including backtrack paths
+	  = Including on-line help requests at first appearance of each
+	    parameter.
+	  = Using only a certain range of parameter lines
+	  = In /ASK mode including hidden parameters
+
+
+
+.pst file
+=========
+
+	Consists of:
+
+	- Preamble: a csh script, ending in the line 'exit'. This script is
+executed by psctest.csh to set up initial conditions (i.e. verify accessibility
+of input files, remove left-over output files etc.).
+
+	- Parameter input: Lines of the form
+
+		<blanks>[*]<blanks><KEYWORD> = <value> ! <number>
+
+The lines are indented corresponding to the 'level' of the parameter in its
+local context. The asterix is positioned at the level of a preceding parameter
+that is the target for a backtrack request.
+
+	- Comment lines starting in a '!'.
+
+
+	The simplest way to generate an initial .pst file is through
+
+		psctest -m <program>
+
+The file may then be manually edited to e.g.
+
+	- insert the initialising script;
+
+	- remove spurious parts (e.g. backtracks accidentally made in the manual
+	   run);
+
+	- change improper backtrack targets to what they should be (Of course,
+	   corresponding changes must be made in the program code!).
+
+After a change in the parameter lines, they may be renumbered through
+
+		psctest -n.
+
+
+Special cases
+=============
+
+Unconditional backtracking
+--------------------------
+
+	To be realised by listing the parameters through which the backtrack is
+made with '#' input, at the proper indentation (i.e. indents for a backtrack
+chain decrease downward). Do not include '*' backtrack marks!
+
+
+Repetition loop
+---------------
+
+	Occurs e.g. in NSCAN LOAD, NMAP MAKE. Append indices in [] to the
+parameter name to show the cycle number. Continue increasing indentation
+throughout the loop.
+
+
+Hidden parameters
+-----------------
+
+	To be indented at the same level as the subsequent visible parameter.
diff --git a/qube.txt b/qube.txt
new file mode 100644
index 0000000000000000000000000000000000000000..e6a427d215fc65e17dc4fbc9c28d5cde7e878d25
--- /dev/null
+++ b/qube.txt
@@ -0,0 +1,226 @@
+QUBES: Software to make SCN-file UV-data available in various sort orders
+-------------------------------------------------------------------------
+History:
+	Contributed by WNB, 940810
+	WNB 940812: add interferometer errors
+
+
+Summary (JPH 940810)
+
+	This note documents software created by WNB during his 1994 visit at NFRA as infrastructure for the program NFILTER.)
+
+
+1. Introduction
+
+To be able to read a one-directional data vector from the Scan data in
+any of the possible coordinate direction, a number of NSCQ.. routines
+are available, replacing in essence NSCSCR and NMOMU4 and their
+initialisers.
+The possible directions are: frequency(f), ha(t), interferometer(i). No
+possibilty to go in the direction of Mosaic fields has been built in,
+mainly because different mosaic fields have no identical ha's: the
+4-dimensional structure (mosaic,f,t,i) is not a regular hypercube.
+The structure chosen assumes that the dataset to be considered
+consists of a series of 3-d cubes (f,t,i) at different mosaic points.
+In principle extension to a series of (mosaic,f,i) cubes at different
+ha's would be feasable.
+A field in the above is a set of observations at the same position on
+the sky, with identical (number of) frequencies, interferometers and
+hour angles. Note: the actual check on the number of hour angles is
+not extensive, to limit the sorting problems, but with actual WSRT
+observations this should not be a problem.
+An example of the actual use is given in NFIUVL.for, which at the
+moment is a simple test program, not an actual UVLIN.
+
+2. Routines
+
+To write a program using the NSCQ routines, the basic structure of the
+program is identical to programs using NSCSCR, i.e. scans in the
+i-direction. The user parameters used by the NSCQ routines are the
+same: Node, Sets and, possibly, Loops. Other selection parameters can
+be used in the same way as in other programs, and model data has to be
+initialised in the same way as well (i.e. NMODAX, NMOMUI and NMOMSC/L
+have to be used before the actual data loops can start).
+
+
+To set the field a (short) description of the standard program
+structure as it is now (*=optional):
+
+while WNDXLN			do all specified loops(*)
+  NMOMSL			calculate scan model(*)
+  while NSCSTL			do all sectors
+    NSCSIF			get interferometer table(*)
+    NSCMBL			get baseline table(*)
+    NCARRT			get redundant baseline(*)
+    NMORDH			get model parameters(*)
+    NMOMST			calculate some model parameters(*)
+    for i=ha-range		go through (selected) ha scans
+      NSCSCR			get corrected scan data
+      NMOMUV			calculate UV coordinates for scan (*)
+      NMOMU4			calculate model for scan(*)
+      action			including e.g. NSCSWI
+    end
+  end
+end
+
+The structure to go through data in different order is comparable:
+
+while WNDXLN			do all specified loops(*)
+  NMOMSL			calculate scan model(*)
+  NSCQOP			prepare SETs for reading
+  while NSCQFN			get next field in 4-d structure (and 
+					coordinate tables) and select
+					coordinate order
+    NSCMBL			get baseline table(*)
+    NCARRT			get redundant baselines (*)
+    
+    for i=first selected coordinate
+      for j=second selected coordinate
+        NSCQSR			read selected (pseudo-)scan along 3rd coord
+        				and model, if selected in QFN
+        action			including e.g. NSCQWA/M
+      end
+    end
+  end
+  NSCQCL			close Qube control area
+end
+
+routines to calculate e.g. UV-coordinates etc for the pseudo scans are
+easily added if necessary. 
+
+
+3. Description interface
+
+
+- NSCQOP_L(	QUA_J:O,			Qube control area ptr
+		FCA_J:I,		 	(Scan) file control area
+		SETS_J(0:SOF__N-1,0:*):I,	SETs selected by user
+		LPOFF_J(0:SOF__N-1)		Current Loop offsets
+		INFO_J(QINFO__L:QINFO__H):O	Info about 4-d qube
+	)
+
+QOP analyses the SETs (using also the loop info (LPOFF) and Scan file
+(FCA), and makes a sorted list of all Sector pointers. It also
+reserves buffers for later use.
+The QUA is a pointer to the control area to be used in all subsequent
+Q calls. 
+The INFO array returns the following information (parameters in
+CBITS_DEF):
+	INFO(QINFO_FLD)		number of different fields
+	INFO(QINFO_F)		max. number of frequencies found in all fields
+	INFO(QINFO_T)		max. # ha
+	INFO(QINFO_I)		max. # ifrs
+
+Note: the system works fastest if field selection is done by the Loop
+structure.
+
+
+- NSCQCL_L(	QUA_J:IO,			Qube control area ptr
+		FCA_J:I,			Scan file control area
+		SETS_J(0:SOF__N-1,0:*):I	SETs selected by user
+	)
+
+QCL frees all the buffers and temporary files used
+
+
+- NSCQFN_L(	QUA_J:I,			Qube control area ptr
+		FCA_J:I,			Scan file control area
+		ORDER_J:I,			Order of data reading
+		STH_B(0:STH__L-1):O,		A Sector header
+		INFO_J(QINFO__L:QINFO__H):O,	Info about 4-d qube
+		PINFO_J(QINFO__L:QINFO__H):O	Pointer to Info about 4-d qube
+	)
+
+QFN selects the next field for processing (or is .false. if no more).
+It uses the QUA and FCA, and the ORDER specified. The ORDER can be:
+		QUB_FTI [+QUB_M] [+QUB_OUT]
+		    TFI
+		    TIF
+		    ITF
+		    FIT
+		    IFT
+The ..I uses no sorting file, the I.. may use a large sorting file.
+The coding is: I=interferometer, F=frequency, T=ha. The last code
+specifies the direction of the 'scan' produced (i.e. FTI is the
+'normal' order, TIF produces a scan along the frequency axis); the 1st
+code specifies the highest loop direction the user wants to use. Note:
+you can loop in a different order than specified, but this will be
+rather inefficient in general.
+The _M modifier (e.g. QUB_TIF+QUB_M) will in addition to the data also
+generate the model data in the same 'scan' direction.
+The _OUT modifier will prepare and enable the writing of
+interferometer errors.
+
+The STH returned is one of the STHs of the field. I.e., the
+coordinates, number of interferometers etc will be correct, but time,
+frequency, ha and data depended on these will be random. It can,
+however, be used in routines like NSCMBL.
+
+The INFO returned is identical to that for QOP, but now the actual
+field number(1..), and axis lengths for this field are returned.
+
+The PINFO (at QINFO_T, QINFO_I, QINFO_F) returns pointers to tables
+with the actual coordinates along the axes. These values can be
+addressed as:
+	A_I(PINFO(QINFO_I)+n_i)		interferometer codes
+	A_E(PINFO(QINFO_T)+n_t)		ha values
+	A_D(PINFO(QINFO_F)+n_f)		frequencies
+with n=0,INFO(QINFO_x)-1
+
+
+- NSCQFR_L(	QUA_J:I,			Qube control area ptr
+		FCA_J:I				Scan file control area
+	)
+
+QFR resets the field search to the start of the field list
+
+
+- NSCQSR_L(	QUA_J:I,			Qube control area ptr
+		FCA_J:I,			Scan file area
+		AX1_J:I,			1st axis to read
+		AX2_J:I,			2nd axis to read
+		CAP_J:I,			apply bits
+		CDAP_J:I,			de-apply bits
+		PWGT_J:O,			pointer to scan weights
+		PDAT_J:O,			pointer to scan data
+		PMOD_J:O,			pointer to scan model
+		POUT_J:O,			pointer to area to put
+						ifr errors
+	)
+
+QSR reads a (pseudo-)scan along the 3rd axis selected in QFN at the
+position specified by AX1 and AX2 (axis types determined in QFN). I.e.
+with QUB_TIF and AX1,AX2=300,2 a frequency scan will be produced for
+the second interferometer in the interferometer table at the 300th ha
+point (values for the axes can be 0..INFO(corresponding)-1).
+
+The data is returned by a pointer to an array. These arrays have
+dimensions (0:3,0:length scan-1). Note: the index order is different
+from that returned by NSCSCR and NMOCIX, for obvious reasons.
+If n_p is the polarisation (0..3) wanted and n_d the data point
+(0..INFO()-1),the data can be accessed by:
+	A_E(PWGT+4*n_d+n_p)
+	A_X(PDAT+4*n_d+n_p)
+	A_X(PMOD+4*n_d+n_p)
+Interferometer error data (if QUB_OUT included in QFN) can be put into
+the array pointed to by POUT, and accessed by:
+	A_X(POUT+4*n_d+n_p)
+
+Note: the PMOD has only a valid value if QUB_M was used in QFN
+Note: the model data are already converted to XYX format
+
+
+- NSCQWA_L(	QUA_J:I,			Qube control area ptr
+  NSCQWM_L	FCA_J:I,			Scan file area
+		AX1_J:I,			1st axis to write
+		AX2_J:I,			2nd axis to write
+		CAP_J:I,			apply bits
+		CDAP_J:I			de-apply bits
+	)
+
+QWA will write the additive interferometer errors set (in pseudo-scan
+order in the array POUT obtained from QSR) to the scan data file.
+QWM the multiplicative interferometer errors.
+
+
+wnb/940812
diff --git a/rcp_batch_processing.ps b/rcp_batch_processing.ps
new file mode 100644
index 0000000000000000000000000000000000000000..9b7624fbc3700cac43fbdcd3b24becbb6181ede5
--- /dev/null
+++ b/rcp_batch_processing.ps
@@ -0,0 +1,368 @@
+%!PS-Adobe-2.0
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+%%Title: rcp_batch_processing_tmp.dvi
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+/bos{/SS save N}B /eos{SS restore}B end
+
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diff --git a/rcp_batch_processing/images.pl b/rcp_batch_processing/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_batch_processing/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_batch_processing/labels.pl b/rcp_batch_processing/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..aa7dd01a495336c9ed8d313634f26ba622caa616
--- /dev/null
+++ b/rcp_batch_processing/labels.pl
@@ -0,0 +1,12 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/rcp_batch_processing.html"; 
+$external_labels{".scope"} ="$URL/rcp_batch_processing.html"; 
+$external_labels{".detail.load"} ="$URL/rcp_batch_processing.html"; 
+$external_labels{".summary"} ="$URL/rcp_batch_processing.html"; 
+$external_labels{".contents"} ="$URL/rcp_batch_processing.html"; 
+$external_labels{".detail.layout"} ="$URL/rcp_batch_processing.html"; 
+$external_labels{".detail"} ="$URL/rcp_batch_processing.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_batch_processing/rcp_batch_processing.html b/rcp_batch_processing/rcp_batch_processing.html
new file mode 100644
index 0000000000000000000000000000000000000000..c16760b5f7897388039ff98bfbb3e2106150871c
--- /dev/null
+++ b/rcp_batch_processing/rcp_batch_processing.html
@@ -0,0 +1,95 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Simple Batch Processing</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_batch_processing.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_batch_processing.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_batch_processing.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_batch_processing.html#SECTION0004000000000000000> <b>Summary of the recipe</b></A>
+<LI> <A NAME=tex2html5 HREF=rcp_batch_processing.html#SECTION0005000000000000000> <b>More details for some of the steps</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=rcp_batch_processing.html#SECTION0005100000000000000> <b>Load your data</b></A>
+<LI> <A NAME=tex2html7 HREF=rcp_batch_processing.html#SECTION0005200000000000000> <b>Inspect the data file layout</b></A>
+</UL>
+</UL>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+...........
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe</b></A></H1>
+<P>
+The following is a step-by-step summary of the processing recipe. For some of these steps, more detail is provided below.
+<P>
+<OL><LI> <b>Load your data:</b>  from tape or optical disk (NSCAN, option ....). See also Recipe ``Reading data in Dwingeloo''. 
+<LI> <b>Inspect the data file layout:</b> (NSCAN, option ...). 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+</OL>
+<P>
+<A NAME=.detail><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>More details for some of the steps</b></A></H1>
+<P>
+<A NAME=.detail.load><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005100000000000000> <b>Load your data</b></A></H2>
+<P>
+<A NAME=.detail.layout><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000> <b>Inspect the data file layout</b></A></H2>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_circ_polarisation.ps b/rcp_circ_polarisation.ps
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+++ b/rcp_circ_polarisation.ps
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diff --git a/rcp_circ_polarisation/images.pl b/rcp_circ_polarisation/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_circ_polarisation/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_circ_polarisation/labels.pl b/rcp_circ_polarisation/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..87d396019da8e7775cafc4d4aeb24c06b56c52d9
--- /dev/null
+++ b/rcp_circ_polarisation/labels.pl
@@ -0,0 +1,10 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/rcp_circ_polarisation.html"; 
+$external_labels{".scope"} ="$URL/rcp_circ_polarisation.html"; 
+$external_labels{".summary"} ="$URL/rcp_circ_polarisation.html"; 
+$external_labels{".contents"} ="$URL/rcp_circ_polarisation.html"; 
+$external_labels{".detail"} ="$URL/rcp_circ_polarisation.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_circ_polarisation/rcp_circ_polarisation.html b/rcp_circ_polarisation/rcp_circ_polarisation.html
new file mode 100644
index 0000000000000000000000000000000000000000..440c65d4ded84fa618f5bfc005e77e3bc30487a2
--- /dev/null
+++ b/rcp_circ_polarisation/rcp_circ_polarisation.html
@@ -0,0 +1,87 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Circular Polarisation</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_circ_polarisation.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_circ_polarisation.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_circ_polarisation.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_circ_polarisation.html#SECTION0004000000000000000> <b>Summary of the recipe</b></A>
+<LI> <A NAME=tex2html5 HREF=rcp_circ_polarisation.html#SECTION0005000000000000000> <b>More details for some of the steps</b></A>
+</UL>
+Author: R.G. Strom
+<P>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+...........
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe</b></A></H1>
+<P>
+The following is a step-by-step summary of the processing recipe. For some of these steps, more detail is provided below.
+<P>
+<OL><LI> <b>Load your data:</b>  from tape or optical disk (NSCAN, option ....). See also Recipe ``Reading data in Dwingeloo''. 
+<LI> <b>Inspect the data file layout:</b> (NSCAN, option ...). 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+</OL>
+<P>
+<A NAME=.detail><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>More details for some of the steps</b></A></H1>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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diff --git a/rcp_continuum_21cm/images.pl b/rcp_continuum_21cm/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_continuum_21cm/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_continuum_21cm/labels.pl b/rcp_continuum_21cm/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..837eeb2b9429d22fe977a9468678177814f218b4
--- /dev/null
+++ b/rcp_continuum_21cm/labels.pl
@@ -0,0 +1,14 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".scope"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".detail.load"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".summary"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".6cm"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".contents"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".49/92cm"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".detail.layout"} ="$URL/rcp_continuum_21cm.html"; 
+$external_labels{".detail"} ="$URL/rcp_continuum_21cm.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_continuum_21cm/rcp_continuum_21cm.html b/rcp_continuum_21cm/rcp_continuum_21cm.html
new file mode 100644
index 0000000000000000000000000000000000000000..419d80249d746d999fb33c3bda9e5083a4e309d4
--- /dev/null
+++ b/rcp_continuum_21cm/rcp_continuum_21cm.html
@@ -0,0 +1,109 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Continuum measurements at 21 cm</b>  
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_continuum_21cm.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_continuum_21cm.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_continuum_21cm.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_continuum_21cm.html#SECTION0004000000000000000> <b>Summary of the recipe for 21cm</b></A>
+<LI> <A NAME=tex2html5 HREF=rcp_continuum_21cm.html#SECTION0005000000000000000> <b>More details for some of the steps</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=rcp_continuum_21cm.html#SECTION0005100000000000000> <b>Load your data</b></A>
+<LI> <A NAME=tex2html7 HREF=rcp_continuum_21cm.html#SECTION0005200000000000000> <b>Inspect the data file layout</b></A>
+</UL> 
+<LI> <A NAME=tex2html8 HREF=rcp_continuum_21cm.html#SECTION0006000000000000000> <b>Processing 6cm continuum data</b></A>
+<LI> <A NAME=tex2html9 HREF=rcp_continuum_21cm.html#SECTION0007000000000000000> <b>Processing 49/92cm continuum data</b></A>
+</UL>
+Author: A.G. de Bruyn
+<P>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+21 cm
+<P>
+6 cm
+<P>
+49/92 cm ...........
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe for 21cm</b></A></H1>
+<P>
+The following is a step-by-step summary of the processing recipe. For some of these steps, more detail is provided below.
+<P>
+<OL><LI> <b>Load your data:</b> from tape or optical disk (NSCAN, option ....). See also Recipe ``Reading data in Dwingeloo''.  
+<LI> <b>Inspect the data file layout:</b> (NSCAN, option ...).  
+<LI> <b>... :</b>  
+<LI> <b>... :</b>  
+<LI> <b>... :</b>  
+<LI> <b>... :</b>  
+</OL>
+<P>
+<A NAME=.detail><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000> <b>More details for some of the steps</b></A></H1>
+<P>
+<A NAME=.detail.load><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005100000000000000> <b>Load your data</b></A></H2>
+<P>
+<A NAME=.detail.layout><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005200000000000000> <b>Inspect the data file layout</b></A></H2>
+<P>
+<A NAME=.6cm><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0006000000000000000> <b>Processing 6cm continuum data</b></A></H1>
+<P>
+<A NAME=.49/92cm><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0007000000000000000> <b>Processing 49/92cm continuum data</b></A></H1>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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diff --git a/rcp_dynamic_range/images.pl b/rcp_dynamic_range/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_dynamic_range/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_dynamic_range/labels.pl b/rcp_dynamic_range/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..2fa7173618def2d80ba608c42775ed91eef9b76b
--- /dev/null
+++ b/rcp_dynamic_range/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_dynamic_range.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_dynamic_range/rcp_dynamic_range.html b/rcp_dynamic_range/rcp_dynamic_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..f5dd65f13e163e5d2f867c24fe3a9910e3d10ed2
--- /dev/null
+++ b/rcp_dynamic_range/rcp_dynamic_range.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: High Dynamic Range</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_dynamic_range.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_external_calibrators.ps b/rcp_external_calibrators.ps
new file mode 100644
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--- /dev/null
+++ b/rcp_external_calibrators.ps
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diff --git a/rcp_external_calibrators/images.pl b/rcp_external_calibrators/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_external_calibrators/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_external_calibrators/labels.pl b/rcp_external_calibrators/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..3c592f0dc353b14456a8e327d3ad247bf075125d
--- /dev/null
+++ b/rcp_external_calibrators/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_external_calibrators.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_external_calibrators/rcp_external_calibrators.html b/rcp_external_calibrators/rcp_external_calibrators.html
new file mode 100644
index 0000000000000000000000000000000000000000..bab77d38b0513d2f0572327dee8c859c8f955bb8
--- /dev/null
+++ b/rcp_external_calibrators/rcp_external_calibrators.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
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+ <b>Processing recipe: External Calibrators</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_external_calibrators.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
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+newstar@nfra.nl
diff --git a/rcp_line_21cm.ps b/rcp_line_21cm.ps
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+b(a)h(new)g(image)e(cub)r(e)h(with)g(sources)h(subtracted.)0
+2647 y Fc(No)o(w)14 b(y)o(ou)f(pro)q(ceed)i(with)f(step)h(6,)e(but)h
+(subtract)h(the)g(list)e(of)g(sources)j(found)d(in)h(the)g(previous)h
+(step.)935 2995 y(5)p eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/rcp_line_21cm/images.pl b/rcp_line_21cm/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_line_21cm/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_line_21cm/labels.pl b/rcp_line_21cm/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..f711b2e3708ff82b70e05aa3e777d7203c09be6e
--- /dev/null
+++ b/rcp_line_21cm/labels.pl
@@ -0,0 +1,27 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".remain.newcube"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".detail.passband"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".contents"} ="$URL/rcp_line_21cm.html"; 
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+$external_labels{".detail.load"} ="$URL/rcp_line_21cm.html"; 
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+$external_labels{".remain.flag"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".detail.inspcalvis"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".intro"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".detail.makecube"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".summary"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".remain.sourcepar"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".detail.transcal"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".scope"} ="$URL/rcp_line_21cm.html"; 
+$external_labels{".detail.cubecorr"} ="$URL/rcp_line_21cm.html"; 
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+$external_labels{".detail.subcont"} ="$URL/rcp_line_21cm.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_line_21cm/rcp_line_21cm.html b/rcp_line_21cm/rcp_line_21cm.html
new file mode 100644
index 0000000000000000000000000000000000000000..b4d209916bdcd689cf91fee98301e1c458ceeec3
--- /dev/null
+++ b/rcp_line_21cm/rcp_line_21cm.html
@@ -0,0 +1,212 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: 21cm line observations</b>  
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_line_21cm.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_line_21cm.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_line_21cm.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_line_21cm.html#SECTION0004000000000000000> <b>Summary of the recipe</b></A>
+<LI> <A NAME=tex2html5 HREF=rcp_line_21cm.html#SECTION0005000000000000000> <b>More details for some of the steps</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=rcp_line_21cm.html#SECTION0005100000000000000> <b>Load your data</b></A>
+<LI> <A NAME=tex2html7 HREF=rcp_line_21cm.html#SECTION0005200000000000000> <b>Inspect the file layout and flag/clip bad points</b></A>
+<LI> <A NAME=tex2html8 HREF=rcp_line_21cm.html#SECTION0005300000000000000> <b>Determine the instrumental gains/phases across the passband</b></A>
+<LI> <A NAME=tex2html9 HREF=rcp_line_21cm.html#SECTION0005400000000000000> <b>Plot the calibration results</b></A>
+<LI> <A NAME=tex2html10 HREF=rcp_line_21cm.html#SECTION0005500000000000000> <b>Transfer the gains/phases from the calibrator(s)</b></A>
+<LI> <A NAME=tex2html11 HREF=rcp_line_21cm.html#SECTION0005600000000000000> <b>Make a cube of images</b></A>
+<LI> <A NAME=tex2html12 HREF=rcp_line_21cm.html#SECTION0005700000000000000> <b>Visual inspection of images</b></A>
+<LI> <A NAME=tex2html13 HREF=rcp_line_21cm.html#SECTION0005800000000000000> <b>Subtract the continuum form the line channels</b></A>
+<LI> <A NAME=tex2html14 HREF=rcp_line_21cm.html#SECTION0005900000000000000> <b>Make a cube of the corrected visibilities</b></A>
+<LI> <A NAME=tex2html15 HREF=rcp_line_21cm.html#SECTION00051000000000000000> <b>Visual inspection of (calibrated) visibilities</b></A>
+<LI> <A NAME=tex2html16 HREF=rcp_line_21cm.html#SECTION00051100000000000000> <b>Make contour plots of images</b></A>
+<LI> <A NAME=tex2html17 HREF=rcp_line_21cm.html#SECTION00051200000000000000> <b>Transfer images to AIPS or GIPSY</b></A>
+</UL> 
+<LI> <A NAME=tex2html18 HREF=rcp_line_21cm.html#SECTION0006000000000000000> <b>Dealing with remaining imperfections</b></A>
+<UL> 
+<LI> <A NAME=tex2html19 HREF=rcp_line_21cm.html#SECTION0006100000000000000> <b>Further flagging of bad data.</b></A>
+<LI> <A NAME=tex2html20 HREF=rcp_line_21cm.html#SECTION0006200000000000000> <b>Make a new image cube.</b></A>
+<LI> <A NAME=tex2html21 HREF=rcp_line_21cm.html#SECTION0006300000000000000> <b>Finding and updating discrete source parameters.</b></A>
+<LI> <A NAME=tex2html22 HREF=rcp_line_21cm.html#SECTION0006400000000000000> <b>Make a new image cube with sources subtracted.</b></A>
+</UL>
+</UL>
+Author: A.G. de Bruyn
+<P>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+This recipe deals with the reduction of a 21cm line dataset. It describes the calibration of the (complex) passbands using one or more calibrators, the flagging of bad data and the production of an image cube. It shows you how to display this image cube in a movie-like fashion using GIDS. The recipe also includes a description of how to visually identify groups of bad datapoints (e.g. bad interferometers or bad channels) and flag/clip those data. If the field is littered with bright continuum sources at the edge of the field, or when you are working with a relatively wide band, the subtraction of the continuum in the image plane will produce undesirable chromatic effects (the continuum emission itself will go away but not their frequency- scaled sidelobe and grating-lobe responses). A simple procedure to remove the continuum in such cases will be given.
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+This recipe describes the series of steps to go through when you want to calibrate a WSRT 21cm line observation. It assumes that the S/N in the data is rather low and that selfcalibration is not required. It also assumes that you do not have to clean the final images.
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe</b></A></H1>
+<P>
+The following is a step-by-step summary of the processing recipe. For some of these steps, more detail is provided below.
+<P>
+<OL><LI> <b>Load your data:</b> from tape or optical disk (NSCAN). See also Recipe 005.  
+<LI> <b>Inspect the data file layout:</b> (NSCAN)  
+<LI> <b>Determine complex passbands:</b> from a calibrator (NCALIB)  
+<LI> <b>Inspect the calibration quality:</b> (NPLOT)  
+<LI> <b>Transfer the calibration corrections:</b> (NCALIB)  
+<LI> <b>Make a preliminary cube of images:</b> (NMAP)  
+<LI> <b>Inspect the image cube:</b> (NGIDS)  
+<LI> <b>Subtract the continuum:</b> (NMAP)  
+<LI> <b>Make a cube of (calibrated) visibilities:</b> (NMAP)  
+<LI> <b>Inspect the UV-data cube:</b> (NGIDS)  
+<LI> <b>Plot your images:</b> (NPLOT)  
+<LI> <b>Transfer your images to GIPSY or AIPS:</b> for further analysis.  
+<LI> <b>Dealing with remaining imperfections:</b> If there are bad groups of datapoints or if the continuum has not been removed satisfactorily the following additional steps may be required:  
+  <UL><LI> <b>Flag bad groups of data:</b> (NSCAN)  
+  <LI> <b>Make a new image cube:</b> (NMAP)  
+  <LI> <b>Find and Update source parameters:</b>  
+  of discrete continuum sources(NMODEL)  
+  <LI> <b>Make a new image cube:</b>  
+  with discrete sources subtracted (NMAP)  
+  </UL> Then proceed with step 7 and iterate if necessary.  
+</OL>
+<P>
+<A NAME=.detail><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000> <b>More details for some of the steps</b></A></H1>
+<P>
+<A NAME=.detail.load><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005100000000000000> <b>Load your data</b></A></H2>
+<P>
+Log in on the computer on which you want to read in the data. At present this is either the microVAX (RZMVX4) or the Alliant. You load data with the program NSCAN, option LOAD. Before you load your data you must know with what time resolution you want to read in the data, and which channels you wish to process. If your object is confined to a small region (say less than 10 arcmin) it may be sufficient to use 120 seconds averaging. If you wish to synthesize bigger fields I recommend using 60 seconds averaging, in order to avoid too much tangential smearing. If the data were Hanning tapered in Westerbork reading in every other channel may speed up the processing by a factor of two. Hence for a 32 channel observation you could answer at the channel question: &quot;2 to 28 by 2&quot;. Reading in the continuum channel (channel 0) is generally not necessary; it contains continuum data with contaminating line emission. It is also advised to read in the calibrator data into the same scanfile. If you do this in the second jobstep the data will be assigned the next highest 'group index'.
+<P>
+<A NAME=.detail.inspdata><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005200000000000000> <b>Inspect the file layout and flag/clip bad points</b></A></H2>
+<P>
+To find out how the data in the file is organized, and how you can access certain subsets of it, it is suggested to move 'up and down' within the program NSCAN. There are five levels of actions to choose, all of which work on different parts of the dataset. The layout of the file, or the function of the five-digit 'index' that points to the various observations, channels etc. is particularly important to memorize. To avoid that obviously bad points (e.g. correlator spikes) ruin the calibration solution you may wish to flag ('delete') any points with a value higher than a certain limit.  Usually the occurrence of correlator spikes is noted on the information you receive from Westerbork/Dwingeloo. Flagging is done on a point-by-point basis using the amplitude of the visibility. Be careful when you use this option if you have no information on the amplitude range which is normal. Preliminary clipping of calibrator data is generally not necessary. During program execution it will inform you at which hourangles interferometers have been clipped.  The cutoff value for the object data can of course be much lower. When visibility samples have been clipped they will be ignored in all programs. You can also undo any clipping; you do this by first typing &quot;undelete&quot; at the question where the type of flagging criterion is selected (HA, AN, RN, IFR, CLIP ...).
+<P>
+<A NAME=.detail.passband><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005300000000000000> <b>Determine the instrumental gains/phases across the passband</b></A></H2>
+<P>
+Run the (self-)calibration program NCALIB (option redundancy) for the calibrator source(s). In order to do this you need a 'model' for the calibrator field containing the fluxes and positions of the calibrator source and any (strong) surrounding sources (see Recipe 013: Using external calibrators). Depending on observing frequency and source there could be anywhere between one and many hundreds of sources in the model file. Upon execution the complex gains are determined, and stored, per telescope/polarisation for each time interval and channel.
+<P>
+<A NAME=.detail.plotcal><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005400000000000000> <b>Plot the calibration results</b></A></H2>
+<P>
+In order to decide which calibrator(s) to use, or which part of the calibration observation, you must inspect the quality of the output from the calibartor NCALIB run. Both the printed LOG from the previous step and/or a plot of the telescope complex gains and the residuals from the (self-) calibration solution are helpful to make up your mind. The program NPLOT (options 'telescope' and 'residuals') does the plotting. In general it suffices to plot one channel, somehwere in the middle of the band, to judge the quality of the gains (called amplitude) and phases for the various telescopes. Phase and gain slopes across the passband are usually the same, to first order, for all telescopes. Phase drifts at 21cm are typically a few degrees of phase over a 12 hour period; gain drifts  
+should generally be less than a few occasionally be larger. Consult the printout which contains summary information for each channel. If there are no instrumental problems the gain and phase errors should be equal to the thermal noise values (see Appendix ....).
+<P>
+<A NAME=.detail.transcal><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005500000000000000> <b>Transfer the gains/phases from the calibrator(s)</b></A></H2>
+<P>
+The corrections from the calibrator(s) are averaged over all available (non- flagged) hourangle scans and stored in each scan of the object scanfile. If your calibrator observations have equal length, and no scans have been flagged, the resulting value is just the mean of the individual calibrator averages. There is no provision to weight for the S/N ratio or the amplitude of the calibrator. This means that the transferred gains/phases are representative for a point in time halfway the time of the calibrator observations. This would be a good assumption for gain/phase drifts that go linear with time. For galactic 21cm line observations you will have calibrators observed at frequencies lower and higher (usually by about 1 MHz) than the frequency of your object. Usually these are scheduled before and after the time of observation of your object but this is not essential. If the calibrator observations have equal length then the averaged gain/phase would be appropriate for a frequency halfway the calibrator frequencies as if there is a linear gain/phase drift with frequency. If your object frequency is not halfway in frequency between the frequencies of the calibrators and you want to store gains/phases in your object file that refer to the frequency of your object, on the assumption that the gains/phase vary linearly with frequency, than you may play around with the length of the respective calibrator observations. This can be done using the NSCAN program (option DELETE, suboption HA (delete).
+<P>
+<A NAME=.detail.makecube><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005600000000000000> <b>Make a cube of images</b></A></H2>
+<P>
+Assuming that you do not want to selfcalibrate the object data (which for line observations is usually the case) you can now proceed to make an image cube. When making images you want to delete any obviously bad baselines. Because you do not yet know whether such bad baselines exist you might as well proceed with making your first series of images. It is possible to exclude visibilities that have an amplitude higher than a certain value. This clipping is not permanent, but only for the execution of NMAP. If the images look good, then all participating baselines are probably good. In an observations with 32 frequency channels, channel 1,29,30 and 31 are usually of poor quality so one would make maps of channels 2 through 28 only. Note that the 3d digit in the index of the 
+.WMP cube will always start counting at 0 and continues through 26. That is, channel 2 is really designated 0.0.0 and channel 28 is 0.0.26.
+<P>
+<A NAME=.detail.visinsp><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005700000000000000> <b>Visual inspection of images</b></A></H2>
+<P>
+Making final, good quality, images is generally an iterative procedure where you work in both the image plane and the UV-plane. This procedure is fastest if you can load the cubes directly into the memory of your display (e.g. X- terminal or workstation). GIDS, the Gipsy Image Display System, is a very useful program to do this. Currently it only runs on the Sun If you want to analyse the images in detail, using programs in GIPSY or AIPS) you will have to make FITS-images first. This can also be done using NMAP (option w16fits or w32fits) but is not shown here. Before you can run GIDS (via dwe NGIDS) you have to switch to an X-terminal (in Dwingeloo we have four HP X-terminals) or one of the two colour displays on the SUN (IPX's).
+<P>
+<A NAME=.detail.subcont><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005800000000000000> <b>Subtract the continuum form the line channels</b></A></H2>
+<P>
+After inspecting the cube of line images you can decide which channels to use for the continuum. Use the option FIDDLE (suboption SUM) to create an averaged continuum image. Then use the option ADD to add the continuum channels with weight -1 to each line image to create continuum-free line channels.
+<P>
+<A NAME=.detail.cubecorr><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005900000000000000> <b>Make a cube of the corrected visibilities</b></A></H2>
+<P>
+If the continuum-free line images look fine you are finished. However, there may be problems at some low level caused by interference, correlator errors or telescope/interferometer errors. Problems at certain position angles in the images correspond to certain hourangles and could be due to short-lived interference. An error pattern in the images, which is centered on the field centre (fringe-stopping centre) and not on strong continuum sources, shows that we are dealing with an additive, rather than multiplicative, error suggests that we are dealing with (DC-) offsets in the backend. To find out which baselines are causing the damage you can make a cube of the (calibrated) visibilities before they are gridded and transformed. You should use the option BASHA instead of UV in NMAP to generate such a cube. Answers to the questions on FFT and map size should be the defaults that are suggested. The best way to pick up low-level problems in the data (e.g. small offsets) is to create outputs for the real (COS) and imaginary (SIN) data. Working with the amplitudes and phases is generally only useful if you want to identify problems of a multiplicative nature and when the signal is well above the noise per visibility point.
+<P>
+<A NAME=.detail.inspcalvis><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION00051000000000000000> <b>Visual inspection of (calibrated) visibilities</b></A></H2>
+<P>
+The cube of UV-data has a different size than that of the images. With samples of 240 sec there are about 180 points in the horizontal direction and 152 points in the vertical direction (4 x 38). By choosing an 18m baseline increment when making the cube you will get the various baselines well separated and makes it easier to count on the screen which baselines are bad. The shortest baseline (9A=72m) is at the bottom of the 'image'. You can now proceed to make a new series of images where baseline 5B should be thrown out. Then you can define the 'continuum' channels and run NMAP to calculate an average continuum channel. This is not shown here because you may want to do this all in GIPSY or AIPS using FITS images. For the purpose of the demonstration this was done in Dwingeloo and the final 'continuum corrected' cube shows images of channels 7 though 23. These images were 512 x 512 in size and covered an area of 0.6 degrees.
+<P>
+<A NAME=.detail.contour><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION00051100000000000000> <b>Make contour plots of images</b></A></H2>
+<P>
+Use the program NPLOT, option MAP to make contour plots of images. There is a variety of output devices. In Dwingeloo you could first send a plot to a (graphics-) terminal  (option REGIS) to check the contourvalues that you would like to plot. When you are satisfied you can, by using the 'loop' option, send a series of plots to the QMS plotter in either portrait (QMSP) or landscape (QMS) mode. The former gives you, for square plotareas, somewhat more space to plot in, if at least you want to restrict yourself to a single A4 sheet. Dealing with the size question will take some experience. The default size of 1,1 will give you a plot of at most 5 inch. This is the case if the number of grid points is a power of two (32, 64, 128 etc). When using a size greater than 1,1 on a power-of-two image area in landscape mode the plot will not fit on one sheet and you have to use scissors and tape. On the portrait mode you can actually increase the size to 1.4,1.4 before it needs more than a single A4 sheet.
+<P>
+<A NAME=.detail.transcube><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION00051200000000000000> <b>Transfer images to AIPS or GIPSY</b></A></H2>
+<P>
+You can use the FITS write option in NMAP to generate 2 byte or 4 byte integer images in FITS format for further analysis in AIPS or GIPSY.
+<P>
+<A NAME=.remain><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0006000000000000000> <b>Dealing with remaining imperfections</b></A></H1>
+<P>
+If the inspection of the continuum subtracted image cube shows imperfections due to bad data or poor continuum subtraction you have to continue the reduction a bit further.
+<P>
+<A NAME=.remain.flag><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0006100000000000000> <b>Further flagging of bad data.</b></A></H2>
+<P>
+If the inspection of the visibility cube using NGIDS has indicated that there are errors in certain hour-angles or baselines you can flag these using the delete option in NSCAN. If there are only bad baselines you can also decide to exclude these baselines when preparing the specifications for a new NMAP. That is, you do not have to actively delete them.
+<P>
+<A NAME=.remain.newcube><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0006200000000000000> <b>Make a new image cube.</b></A></H2>
+<P>
+If the new image cube shows, after subtracting some averaged continuum image, residual (chromatic) grating rings due to strong sources at the edge of the field you need to subtract these sources in the original UV-data.
+<P>
+<A NAME=.remain.sourcepar><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0006300000000000000> <b>Finding and updating discrete source parameters.</b></A></H2>
+<P>
+In order to determine the flux densities and positions of these sources you search the continuum image using the FIND option in NMODEL. To improve the estimates of flux and coordinates you can use the UPDATE option in NMODEL. A single update, using only the UV-data with coninuum emission, usually suffices. 
+ The update algorithm will only work for discrete (point) sources. If there are extended sources with residual grating lobes you need to use NCLEAN (option Beam) to decompose that source into a number of delta- functions. The final list of components (updated discrete sources and clean- components) can be merged into one model file.
+<P>
+<A NAME=.remain.subtr><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0006400000000000000> <b>Make a new image cube with sources subtracted.</b></A></H2>
+<P>
+Now you proceed with step 6, but subtract the list of sources found in the previous step.
+<P>
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+</BODY> </HTML> 
+<HR>
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+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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new file mode 100644
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+++ b/rcp_linear_polarisation.ps
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+(degrees\))i(ha)o(v)o(e)f(to)f(b)q(e)h(en)o(tered)h(in)e(an)h(ASCI)q(I)
+g(\014le)f(\(see)i(the)0 332 y(description)i(in)f(NCALIB,)g(option)g(F)
+-5 b(ARAD)o(A)m(Y)17 b(under)h(SET)p 1018 332 13 2 v
+15 w(OPTION\),)g(and)f(the)h(correction)g(is)f(applied)g(using)0
+382 y(F)-5 b(ARAD)o(A)m(Y.)14 b(Note)i(that)f(the)g(HAs)h(do)f(not)g
+(ha)o(v)o(e)g(to)g(b)q(e)g(hourly)m(,)f(or)h(ev)o(en)h(regularly)f
+(spaced:)21 b(at)15 b(nigh)o(t)f(there)j(ma)o(y)0 432
+y(b)q(e)e(little)e(c)o(hange)h(in)f(the)i(F)m(arada)o(y)e(rotation,)f
+(and)i(a)g(single)f(correction)i(migh)o(t)d(su\016ce.)0
+573 y Fa(4.6)56 b(Correct)18 b(for)h(primary)d(b)r(eam)h(instrumen)n
+(tal)g(p)r(olarization)0 675 y Ff(The)12 b(instrumen)o(tal)f(p)q
+(olarization)g(determined)h(from)e(a)h(calibrator)h(is,)f(strictly)i
+(sp)q(eaking,)e(only)h(correct)h(for)f(a)f(source)0 725
+y(at)18 b(the)h(b)q(eam)e(cen)o(ter,)k(though)d(at)g(most)f
+(frequencies)j(the)f(v)n(ariation)e(within)h(the)g(half-p)q(o)o(w)o(er)
+g(primary)f(b)q(eam)g(is)0 774 y(small.)g(F)m(or)c(p)q(olarization)g
+(mapping)f(o)o(v)o(er)i(large)g(\014elds,)h(there)g(is)f(a)g(separate)h
+(correction)h(for)d(o\013-axis)h(instrumen)o(tal)0 824
+y(p)q(olarization)f(\(NCALIB:)h(NMODEL)g(-)g(BEAM\).)0
+965 y Fa(4.7)56 b(Ho)n(w)19 b(do)g(I)f(kno)n(w)i(that)e(m)n(y)g(data)h
+(are)f(correct?)25 b({)18 b(additional)g(hin)n(ts.)0
+1067 y Ff(Errors;)d(some)e(error)h(patterns;)h(e\013ect)h(of)d(source)i
+(exten)o(t.)118 1142 y(Ionospheric)g(e\013ects)h(and)d(the)i(I)f(map.)
+118 1216 y(What)g(can)g(b)q(e)g(done)g(if)f(a)h(p)q(olarization)f(com)o
+(bination)e(is)j(missing?)118 1291 y(Etc.)935 2995 y(4)p
+eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap195.png b/rcp_linear_polarisation/_11796_tex2html_wrap195.png
new file mode 100644
index 0000000000000000000000000000000000000000..674f1e64a5f8d71d3dba70ce071a9d99417663d9
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap195.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap195.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap195.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..18428f43cc3e881ced346d3e163831275e15d464
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap195.xbm
@@ -0,0 +1,6 @@
+#define noname_width 19
+#define noname_height 11
+static char noname_bits[] = {
+ 0x0c,0x86,0x03,0x36,0x9b,0x02,0x33,0xd9,0x06,0xa3,0xd1,0x06,0xa3,0x91,0x03,
+ 0xb2,0x11,0x00,0xbe,0x11,0x00,0xb0,0x11,0x00,0x36,0x19,0x00,0x1a,0x1b,0x00,
+ 0x0c,0x0e,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap197.png b/rcp_linear_polarisation/_11796_tex2html_wrap197.png
new file mode 100644
index 0000000000000000000000000000000000000000..0c414433e1cc7c6b2977a0d4d94412df25286b05
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap197.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap197.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap197.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3eab27ea7cfac4ce354393c2aeb4e06a799a5ad6
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap197.xbm
@@ -0,0 +1,31 @@
+#define noname_width 110
+#define noname_height 29
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0xe0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x78,0x00,0x00,0xe0,0x83,0xf0,0x3d,0xdf,0x03,
+ 0x00,0xf0,0xb8,0xc7,0x09,0x30,0x00,0x00,0x00,0xc0,0xc0,0x18,0x8c,0x01,0x00,
+ 0x60,0x30,0x83,0x19,0x18,0x00,0x00,0x00,0x40,0xc0,0x04,0x4c,0x00,0x08,0xc0,
+ 0x08,0x46,0x10,0x18,0x00,0x00,0x00,0x60,0xc0,0x03,0x3c,0x00,0x08,0xc0,0x0c,
+ 0x66,0x30,0x18,0xf0,0x1f,0x00,0x60,0x80,0x03,0x38,0x00,0x08,0xc0,0x07,0x3e,
+ 0x30,0x18,0xf8,0x1f,0x00,0x60,0x80,0x01,0x18,0x00,0x08,0x80,0x03,0x1c,0x30,
+ 0x0c,0x00,0x00,0xf0,0x67,0xc0,0x03,0x3c,0xc0,0xff,0x80,0x01,0x0c,0x30,0x0c,
+ 0x00,0x00,0x00,0x60,0x60,0x03,0x36,0x00,0x08,0x80,0x01,0x0c,0x30,0x0c,0xf8,
+ 0x1f,0x00,0x60,0x30,0x06,0x63,0x00,0x08,0x80,0x00,0x04,0x30,0x1f,0x00,0x00,
+ 0x00,0x60,0x3c,0xcf,0xf3,0x00,0x08,0xe0,0x01,0x0f,0x30,0x00,0x00,0x00,0xc0,
+ 0x40,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x10,0x00,0x00,0x00,0x60,0xc3,
+ 0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x70,0xc3,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x70,0x82,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x02,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0xf0,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap199.png b/rcp_linear_polarisation/_11796_tex2html_wrap199.png
new file mode 100644
index 0000000000000000000000000000000000000000..2a8ecf27df162773bdae711a4027f01e7135610a
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap199.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap199.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap199.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..9e4a47556b71de2ac924dbf00717b0074d46b224
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap199.xbm
@@ -0,0 +1,31 @@
+#define noname_width 112
+#define noname_height 29
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x08,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0xf0,0x01,0x00,0x00,0x1f,0xe4,0x71,0x8f,0x03,
+ 0x00,0xc0,0xf7,0x7c,0x2f,0x18,0x03,0x00,0x00,0x00,0xc6,0x60,0x06,0x03,0x00,
+ 0x00,0x63,0x30,0x66,0x0c,0x03,0x00,0x00,0x00,0x82,0x11,0x8c,0x00,0x00,0x00,
+ 0x13,0x30,0x41,0x06,0x03,0x00,0x00,0x00,0x83,0x19,0xcc,0x00,0x00,0x00,0x0f,
+ 0xf0,0xc0,0x06,0x83,0xff,0x00,0x00,0x83,0x0f,0x7c,0x00,0x00,0x00,0x0e,0xe0,
+ 0xc0,0x07,0xc3,0xff,0x00,0x00,0x03,0x07,0x38,0x00,0x00,0x00,0x06,0x60,0xc0,
+ 0x03,0x03,0x00,0x80,0x3f,0x03,0x03,0x18,0x80,0xff,0x00,0x0f,0xf0,0xc0,0x83,
+ 0x01,0x00,0x00,0x00,0x03,0x03,0x18,0x00,0x00,0x80,0x0d,0xd8,0xc0,0xfe,0xc1,
+ 0xff,0x00,0x00,0x03,0x01,0x08,0x00,0x00,0xc0,0x18,0x8c,0xc1,0xee,0x01,0x00,
+ 0x00,0x00,0xc3,0x03,0x1e,0x00,0x00,0xf0,0x3c,0xcf,0xc3,0x38,0x01,0x00,0x00,
+ 0x06,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0xe0,0x01,0x00,0x00,0x1b,
+ 0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0xe0,0x00,0x00,0x80,0x1b,0x06,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x80,0x13,0x0c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x16,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x13,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x1f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap201.png b/rcp_linear_polarisation/_11796_tex2html_wrap201.png
new file mode 100644
index 0000000000000000000000000000000000000000..09a3926e5a6879c85e809e19f90ab371d1fc9f9c
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap201.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap201.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap201.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4767fce35f3da132d84dbab152a805016aeae79f
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap201.xbm
@@ -0,0 +1,31 @@
+#define noname_width 112
+#define noname_height 29
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x80,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x02,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x04,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x10,0xcf,0x01,0x00,0x80,0x0f,0xf2,0x38,0xbe,0x07,
+ 0x00,0xc0,0xf7,0x8f,0x23,0x86,0x00,0x00,0x00,0x00,0x63,0x30,0x18,0x03,0x00,
+ 0x00,0x63,0x06,0x63,0xc6,0x00,0x00,0x00,0x00,0xc1,0x08,0x98,0x00,0x00,0x00,
+ 0x13,0x8c,0x40,0x42,0x00,0x00,0x00,0x80,0xc1,0x0c,0x78,0x00,0x00,0x00,0x0f,
+ 0xcc,0xc0,0x43,0xc0,0x7f,0x00,0x80,0xc1,0x07,0x70,0x00,0x00,0x00,0x0e,0x7c,
+ 0xc0,0x43,0xe0,0x7f,0x00,0x80,0x81,0x03,0x30,0x00,0x00,0x00,0x06,0x38,0xc0,
+ 0x63,0x00,0x00,0xc0,0x9f,0x81,0x01,0x78,0x80,0xff,0x00,0x0f,0x18,0xc0,0x21,
+ 0x00,0x00,0x00,0x80,0x81,0x01,0x6c,0x00,0x00,0x80,0x0d,0x18,0xc0,0x31,0xe0,
+ 0x7f,0x00,0x80,0x81,0x00,0xc6,0x00,0x00,0xc0,0x18,0x08,0xc0,0x1b,0x00,0x00,
+ 0x00,0x80,0xe1,0x81,0xe7,0x01,0x00,0xf0,0x3c,0x1e,0xc0,0x0e,0x00,0x00,0x00,
+ 0x03,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x80,0x0d,
+ 0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0xc0,0x0d,0x03,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0xc0,0x09,0x06,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0b,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x09,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0xc0,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap203.png b/rcp_linear_polarisation/_11796_tex2html_wrap203.png
new file mode 100644
index 0000000000000000000000000000000000000000..9c0399e68dcfc34c90dcbebfb3ac906dbbb26f9e
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap203.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap203.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap203.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..6143f0f9aded98db485478e10a0a2114965e0987
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap203.xbm
@@ -0,0 +1,34 @@
+#define noname_width 123
+#define noname_height 29
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x38,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x3c,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x38,0x40,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x00,0xcf,0x03,0x00,0x00,0x00,0x38,
+ 0x20,0xbe,0x7f,0x1c,0x00,0x00,0x8f,0xe3,0x7b,0x01,0x82,0x01,0x00,0x00,0x00,
+ 0x00,0x30,0x18,0x33,0x18,0x00,0x00,0x06,0x83,0x31,0x03,0xc2,0x00,0x00,0x00,
+ 0x00,0x00,0x10,0x98,0x60,0x04,0x80,0x00,0x8c,0x80,0x09,0x02,0x46,0x00,0x00,
+ 0x00,0x00,0x00,0x18,0x78,0x60,0x06,0x80,0x00,0xcc,0x80,0x07,0x06,0x66,0x80,
+ 0xff,0x00,0x00,0x00,0x18,0x70,0xe0,0x03,0x80,0x00,0x7c,0x00,0x07,0x06,0x26,
+ 0xc0,0xff,0x00,0x00,0x00,0x18,0x30,0xc0,0x01,0x80,0x00,0x38,0x00,0x03,0x06,
+ 0x16,0x00,0x00,0xc0,0x7f,0xfe,0x18,0x78,0xc0,0x00,0xfc,0x0f,0x18,0x80,0x07,
+ 0x06,0x1e,0x00,0x00,0x00,0x00,0x00,0x18,0x6c,0xc0,0x00,0x80,0x00,0x18,0xc0,
+ 0x06,0x06,0x0e,0xc0,0xff,0x00,0x00,0x00,0x18,0xc6,0x40,0x00,0x80,0x00,0x08,
+ 0x60,0x0c,0x06,0x04,0x00,0x00,0x00,0x00,0x00,0x98,0xe7,0xf1,0x00,0x80,0x00,
+ 0x1e,0x78,0x1e,0x06,0x04,0x00,0x00,0x00,0x00,0x18,0x10,0x00,0x00,0x00,0x80,
+ 0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x00,0x6c,0x30,0x00,0x00,0x00,
+ 0x80,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x6e,0x30,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x4e,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x58,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x4c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x7e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap205.png b/rcp_linear_polarisation/_11796_tex2html_wrap205.png
new file mode 100644
index 0000000000000000000000000000000000000000..5dbe700e869fdb3c28b55915e0e86c790ec12de2
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap205.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap205.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap205.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..4349f592929f813262d9342e28997b3856c782f7
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap205.xbm
@@ -0,0 +1,10 @@
+#define noname_width 53
+#define noname_height 15
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0xfc,0xff,0x1f,0x08,0x00,0x00,0x00,0x06,0x00,0x01,0x0c,
+ 0x00,0x00,0x00,0x06,0xc0,0x01,0x00,0x00,0x00,0x00,0x03,0x00,0x01,0x00,0x00,
+ 0x00,0x00,0x03,0x00,0x01,0x0e,0xfc,0x07,0x80,0x01,0x00,0x01,0x0f,0xfe,0x07,
+ 0x80,0x01,0x00,0x01,0x06,0x00,0x00,0xc3,0xf0,0x1f,0x01,0x06,0x00,0x80,0xc7,
+ 0x00,0x00,0x01,0x0e,0xfe,0x07,0x66,0x00,0x00,0x01,0x0e,0x00,0x00,0x66,0x00,
+ 0xc0,0x07,0x00,0x00,0x00,0x3c,0x00,0x00,0x00,0x00,0x00,0x00,0x3c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap207.png b/rcp_linear_polarisation/_11796_tex2html_wrap207.png
new file mode 100644
index 0000000000000000000000000000000000000000..0b9c0ac1dfb90d230d198444907a7e08a619f8ce
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap207.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap207.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap207.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ea657c4f23fcbd844dc719014a2a7f8ba8fff6ff
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap207.xbm
@@ -0,0 +1,6 @@
+#define noname_width 19
+#define noname_height 11
+static char noname_bits[] = {
+ 0x10,0x99,0x03,0x18,0x8f,0x02,0x18,0xc1,0x06,0x1c,0xc1,0x06,0x16,0x8f,0x03,
+ 0x12,0x19,0x00,0x13,0x18,0x00,0xff,0x19,0x00,0x90,0x19,0x00,0x7c,0x1f,0x00,
+ 0x00,0x06,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap209.png b/rcp_linear_polarisation/_11796_tex2html_wrap209.png
new file mode 100644
index 0000000000000000000000000000000000000000..84ceb7c104eef9f3d2a620483b0e611023b28cb0
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap209.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap209.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap209.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3566e6376ccc9c31769576c0830ee27a1699dae0
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap209.xbm
@@ -0,0 +1,5 @@
+#define noname_width 20
+#define noname_height 10
+static char noname_bits[] = {
+ 0x20,0x00,0x00,0x20,0x20,0x0c,0x20,0x60,0x06,0x20,0xc0,0x03,0xff,0x83,0x01,
+ 0x20,0xc0,0x03,0x20,0x60,0x06,0x20,0x20,0x0c,0x20,0x00,0x00,0x20,0x00,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap211.png b/rcp_linear_polarisation/_11796_tex2html_wrap211.png
new file mode 100644
index 0000000000000000000000000000000000000000..0576c20c12fcd5d5001ce1d36b35e3bb5909eb19
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap211.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap211.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap211.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..74927b96d2de4fe8432c53daad071153022f36ac
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap211.xbm
@@ -0,0 +1,5 @@
+#define noname_width 10
+#define noname_height 13
+static char noname_bits[] = {
+ 0xf0,0x01,0x18,0x03,0x0c,0x03,0x06,0x03,0x06,0x03,0x07,0x03,0x03,0x03,0x83,
+ 0x01,0xfe,0x01,0xee,0x01,0x38,0x01,0xe0,0x01,0xe0,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap213.png b/rcp_linear_polarisation/_11796_tex2html_wrap213.png
new file mode 100644
index 0000000000000000000000000000000000000000..f9839e8e3c0e01cb6ccac10b68b5a4ce886d62d6
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap213.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap213.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap213.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ab0708cc56fac0adaeb999195b93286a59c3f5db
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap213.xbm
@@ -0,0 +1,9 @@
+#define noname_width 46
+#define noname_height 13
+static char noname_bits[] = {
+ 0x78,0x00,0x00,0x00,0x00,0x1f,0x30,0x00,0x00,0x00,0x80,0x31,0x18,0x10,0x80,
+ 0x00,0xc0,0x30,0x18,0x70,0x80,0x03,0x60,0x30,0x18,0xc0,0x01,0x0e,0x60,0x30,
+ 0x18,0x00,0x07,0x38,0x70,0x30,0x0c,0x00,0x1c,0xe0,0x30,0x30,0x0c,0x00,0x0e,
+ 0x70,0x30,0x18,0x0c,0x80,0x03,0x1c,0xe0,0x1f,0x1f,0xe0,0x00,0x07,0xe0,0x1e,
+ 0x00,0x30,0x80,0x01,0x80,0x13,0x00,0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,
+ 0x00,0x00,0x0e};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap215.png b/rcp_linear_polarisation/_11796_tex2html_wrap215.png
new file mode 100644
index 0000000000000000000000000000000000000000..daa6c3fbec75b133abe594d5dce82930033f7713
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap215.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap215.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap215.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2981e93716eff389a199213b640df919e9e109f7
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap215.xbm
@@ -0,0 +1,5 @@
+#define noname_width 9
+#define noname_height 11
+static char noname_bits[] = {
+ 0xcf,0x01,0x86,0x00,0xc6,0x00,0x42,0x00,0x43,0x00,0x43,0x00,0x63,0x00,0x21,
+ 0x00,0x31,0x00,0x1b,0x00,0x0e,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap217.png b/rcp_linear_polarisation/_11796_tex2html_wrap217.png
new file mode 100644
index 0000000000000000000000000000000000000000..03aed7004396bcd4d4031e79e8f88a20b9f9be6b
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap217.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap217.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap217.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..79b47dcc5782585edf493cc4f8d538e2b0ee9d06
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap217.xbm
@@ -0,0 +1,5 @@
+#define noname_width 10
+#define noname_height 11
+static char noname_bits[] = {
+ 0xcf,0x03,0x82,0x01,0xc2,0x00,0x46,0x00,0x66,0x00,0x26,0x00,0x16,0x00,0x1e,
+ 0x00,0x0e,0x00,0x04,0x00,0x04,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap221.png b/rcp_linear_polarisation/_11796_tex2html_wrap221.png
new file mode 100644
index 0000000000000000000000000000000000000000..1d2393b4294340cf55fe83c80ec76e21927f4dab
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap221.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap221.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap221.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5476362bce5ea44b42effb9997d9afef16a0f3ff
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap221.xbm
@@ -0,0 +1,11 @@
+#define noname_width 77
+#define noname_height 11
+static char noname_bits[] = {
+ 0xcf,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x1c,0x82,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x60,0x08,0xc2,0x00,0xc0,0x00,0x00,0x00,0x0c,0x00,0x60,0x0c,
+ 0x46,0x00,0x70,0x00,0x00,0x00,0x07,0x00,0x20,0x04,0x66,0x00,0x1c,0xc0,0x3f,
+ 0xc0,0x01,0xfc,0x33,0x04,0x26,0x00,0x07,0xc0,0x66,0x70,0x00,0x6c,0x36,0x04,
+ 0x16,0x80,0x01,0x80,0x7f,0x18,0x00,0xf8,0x37,0x06,0x1e,0x80,0x07,0xc0,0x06,
+ 0x78,0x00,0x6c,0x10,0x02,0x0e,0x00,0x1e,0x60,0x46,0xe0,0x01,0x66,0x14,0x03,
+ 0x04,0x00,0x78,0xc0,0x3f,0x80,0x07,0xfc,0xb3,0x01,0x04,0x00,0xe0,0x00,0x00,
+ 0x00,0x0e,0x00,0xe0,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap223.png b/rcp_linear_polarisation/_11796_tex2html_wrap223.png
new file mode 100644
index 0000000000000000000000000000000000000000..791d6e2035eb22eb32c00178bd43d582ec02d79c
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap223.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap223.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap223.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..ba6ff63879662a4f47ad979848fdfde03d402ada
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap223.xbm
@@ -0,0 +1,7 @@
+#define noname_width 39
+#define noname_height 10
+static char noname_bits[] = {
+ 0x7c,0x0f,0x00,0xe0,0x71,0x30,0x06,0x00,0xc0,0x60,0x30,0x01,0x00,0x80,0x11,
+ 0xf0,0x00,0x00,0x80,0x19,0xe0,0x00,0x00,0x80,0x0f,0x60,0x00,0x00,0x00,0x07,
+ 0xf0,0x00,0xfe,0x03,0x03,0xd8,0x00,0x00,0x00,0x03,0x8c,0x01,0x00,0x00,0x01,
+ 0xcf,0x03,0x00,0xc0,0x03};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap225.png b/rcp_linear_polarisation/_11796_tex2html_wrap225.png
new file mode 100644
index 0000000000000000000000000000000000000000..19c9ad678fe4d61855301bbe9c6f56672547c3c4
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap225.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap225.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap225.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..467c8d7e90ff65c392dd4586cb025216749d23c1
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap225.xbm
@@ -0,0 +1,9 @@
+#define noname_width 44
+#define noname_height 13
+static char noname_bits[] = {
+ 0xf0,0x01,0x3c,0x07,0x3c,0x0f,0x18,0x03,0x18,0x02,0x08,0x06,0x0c,0x03,0x18,
+ 0x03,0x08,0x03,0x06,0x03,0x08,0x01,0x18,0x01,0x06,0x03,0x0c,0x01,0x98,0x01,
+ 0x07,0x03,0x0c,0x01,0x98,0x00,0x03,0x03,0x8c,0x01,0x58,0x00,0x83,0x01,0x84,
+ 0x00,0x78,0x00,0xfe,0x31,0xc4,0x30,0x38,0x00,0xee,0x31,0x6c,0x30,0x10,0x00,
+ 0x38,0x21,0x38,0x20,0x10,0x00,0xe0,0x21,0x00,0x20,0x00,0x00,0xe0,0x10,0x00,
+ 0x10,0x00,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap227.png b/rcp_linear_polarisation/_11796_tex2html_wrap227.png
new file mode 100644
index 0000000000000000000000000000000000000000..3a6dde2e167d1706be0781bd7766480607339e97
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap227.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap227.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap227.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0ee97a53aa20e2b72a28205156f6e20b06938901
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap227.xbm
@@ -0,0 +1,10 @@
+#define noname_width 57
+#define noname_height 13
+static char noname_bits[] = {
+ 0x78,0x00,0x3e,0x00,0xcf,0x81,0xe7,0x01,0x30,0x00,0x63,0x00,0x86,0x00,0xc1,
+ 0x00,0x18,0x80,0x61,0x00,0xc6,0x00,0x61,0x00,0x18,0xc0,0x60,0x00,0x42,0x00,
+ 0x23,0x00,0x18,0xc0,0x60,0x00,0x43,0x00,0x33,0x00,0x18,0xe0,0x60,0x00,0x43,
+ 0x00,0x13,0x00,0x0c,0x60,0x60,0x00,0x63,0x00,0x0b,0x00,0x0c,0x60,0x30,0x00,
+ 0x21,0x00,0x0f,0x00,0x0c,0xc3,0x3f,0x06,0x31,0x06,0x07,0x00,0x1f,0xc3,0x3d,
+ 0x06,0x1b,0x06,0x02,0x00,0x00,0x02,0x27,0x04,0x0e,0x04,0x02,0x00,0x00,0x02,
+ 0x3c,0x04,0x00,0x04,0x00,0x00,0x00,0x01,0x1c,0x02,0x00,0x02,0x00,0x00};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap229.png b/rcp_linear_polarisation/_11796_tex2html_wrap229.png
new file mode 100644
index 0000000000000000000000000000000000000000..273cf4f8f062a2787fbf4b7d3fba250dc4404acb
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap229.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap229.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap229.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..b7d7180e479dc6553c07ddf123ffbacf1ac02ae9
--- /dev/null
+++ b/rcp_linear_polarisation/_11796_tex2html_wrap229.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 10
+static char noname_bits[] = {
+ 0x78,0x30,0x18,0x18,0x18,0x18,0x0c,0x0c,0x0c,0x1f};
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap231.png b/rcp_linear_polarisation/_11796_tex2html_wrap231.png
new file mode 100644
index 0000000000000000000000000000000000000000..345046f8a9a5646b02edbd75fc912a02b9b440c5
Binary files /dev/null and b/rcp_linear_polarisation/_11796_tex2html_wrap231.png differ
diff --git a/rcp_linear_polarisation/_11796_tex2html_wrap231.xbm b/rcp_linear_polarisation/_11796_tex2html_wrap231.xbm
new file mode 100644
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+#define noname_height 13
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new file mode 100644
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+#define noname_width 86
+#define noname_height 12
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new file mode 100644
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+#define noname_width 19
+#define noname_height 11
+static char noname_bits[] = {
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diff --git a/rcp_linear_polarisation/images.pl b/rcp_linear_polarisation/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..07be3116a1721888abb88c03ff0cc74f9119764a
--- /dev/null
+++ b/rcp_linear_polarisation/images.pl
@@ -0,0 +1,47 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$30^circ${}/;
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+$key = q/{}$X-Y${}/;
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+$key = q/{}$Q${}/;
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+$key = q/{}$45^circ${}/;
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+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap221.xbm">'; 
+$key = q/{}$$Q=<<114>>1over2<<114>>(YY-XX)$${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap199.xbm">'; 
+$key = q/{}$$V=-<<116>>iover2<<116>>(XY+YX)$${}/;
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+$key = q/{}$+times${}/;
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+$key = q/{}$Q,U,oriV${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap231.xbm">'; 
+
+1;
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diff --git a/rcp_linear_polarisation/labels.pl b/rcp_linear_polarisation/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..c4ac6b0806e6d89708b3db87f641da930fd6675d
--- /dev/null
+++ b/rcp_linear_polarisation/labels.pl
@@ -0,0 +1,12 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".hints"} ="$URL/rcp_linear_polarisation.html"; 
+$external_labels{".intro"} ="$URL/rcp_linear_polarisation.html"; 
+$external_labels{".scope"} ="$URL/rcp_linear_polarisation.html"; 
+$external_labels{".beam"} ="$URL/rcp_linear_polarisation.html"; 
+$external_labels{".summary"} ="$URL/rcp_linear_polarisation.html"; 
+$external_labels{".contents"} ="$URL/rcp_linear_polarisation.html"; 
+$external_labels{".detail"} ="$URL/rcp_linear_polarisation.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_linear_polarisation/rcp_linear_polarisation.html b/rcp_linear_polarisation/rcp_linear_polarisation.html
new file mode 100644
index 0000000000000000000000000000000000000000..c2d4ecf21a0c05cd7bea71e9e6210fd7fef32ae9
--- /dev/null
+++ b/rcp_linear_polarisation/rcp_linear_polarisation.html
@@ -0,0 +1,127 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Linear Polarisation</b>
+<P>
+Author: R.G. Strom
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_linear_polarisation.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_linear_polarisation.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_linear_polarisation.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_linear_polarisation.html#SECTION0004000000000000000> <b>Summary of the recipe</b></A>
+<LI> <A NAME=tex2html5 HREF=rcp_linear_polarisation.html#SECTION0005000000000000000> <b>More details for some of the steps</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=rcp_linear_polarisation.html#SECTION0005100000000000000> <b>Determine the instrumental polarization</b></A>
+<LI> <A NAME=tex2html7 HREF=rcp_linear_polarisation.html#SECTION0005200000000000000> <b>Correct for primary beam instrumental polarization</b></A>
+<LI> <A NAME=tex2html8 HREF=rcp_linear_polarisation.html#SECTION0005300000000000000> <b>How do I know that my data are correct? - additional hints.</b></A>
+</UL>
+</UL>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+For obtaining polarization maps from standard continuum observations (all four dipole combinations must be present). See also the description of the program NCALIB, part 3.
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+In a normal WSRT continuum observation, four dipole combinations (XX, XY, etc.) are measured for each fixed-movable (numbered-lettered telescope) baseline. Since mid-1983, the standard configuration is for the X-dipoles in all telescopes to be set parallel (hence the Y-dipoles are also). A polarization code is recorded for each observation, which gives the X-dipole position angle in the fixed and movable telescopes, in steps of <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap207.png">. The usual setting for the X-dipoles is <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap195.png"> (i.e., directed toward increasing RA), which gives a polarization code of 22. This results in the following definition of the Stokes parameters: <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap197.png"> <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap199.png"> <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap201.png"> <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap203.png"> (where <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap205.png">). In the remainder of this description it will be assumed that the observation being corrected has code 22, and of course that all four dipole combinations have good data.
+<P>
+<em>Most continuum observations made before mid-1983 were done with the dipoles in the movable telescopes rotated by <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap207.png"> to the fixed ones, usually with polarization code 21 [or in any event with the digits differing by an odd number]. For analyzing such observations, the user should consult with the WSRT User Service in Dwingeloo. From time to time, calibration sources are still observed in code 21 [generally indicated by `<IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap209.png">' appended to the source name]. In almost all line observations, only one or two of the dipole combinations (XX, YY) are measured; they are of course unsuitable for determining source polarization.</em>
+<P>
+The determination of the (observed) Stokes <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap211.png"> depends, as shown by the first two equations above, upon how well the gains of the XX and YY channels can be ascertained (since usually, <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap213.png">). For the <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap215.png"> and <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap217.png"> determinations, the critical parameters are the dipole setting or orthogonality, and the ellipticity. Moreover, since <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap217.png"> is usually small (i.e., <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap221.png">) its determination will also depend upon the quality of the XY and YX gains. The other parameter required to correct the XY and YX combinations is the <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap223.png"> phase difference. The correction is usually small (since it should have been determined and applied online in Westerbork) and has to be determined from an observation of a polarized source, or a special `crossed' (code 21) calibration source measurement. Finally, it may be necessary to correct for Faraday rotation in the ionosphere (this is usually only necessary at 49 and 92 cm), and for variations in the instrumental polarization if there is significant emission beyond the central part of the primary beam.
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe</b></A></H1>
+<P>
+The following is a step-by-step summary of the processing recipe. For some of these steps, more detail is provided below.
+<P>
+<OL><LI> <b>Load your data:</b> from tape or optical disk (NSCAN, option LOAD) See also Recipe ``Reading data in Dwingeloo''. 
+<LI> <b>Inspect the data file layout:</b> (NSCAN, option SHOW) 
+<LI> <b>Determine the instrumental gain and phase corrections for a strong calibrator with known polarisation:</b> (NCALIB, option REDUN.) 
+<LI> <b>Determine or set the instrumental polarization corrections for an unpolarised calibrator:</b> (NCALIB, option POLAR.) 
+<LI> <b>Map and inspect Stokes <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap225.png"> for the calibrator (optional):</b> (NMAP, followed by NPLOT or NGIDS.) 
+<LI> <b>Copy (or set by hand) the instrumental polarization corrections for the observed field:</b> (NCALIB, option POLAR COPY.) 
+<LI> <b>Determine, and apply if necessary, the correction for ionospheric Faraday rotation (optional, usually only necessary at 49/92 cm):</b> (NCALIB, option SET FARADAY.) 
+<LI> <b>Map and inspect <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap227.png"> images of field:</b> (NMAP, followed by NPLOT or NGIDS) 
+<LI> <b>Primary beam correction for each Stokes parameter (may only be necessary if source extends over large fraction of primary beam):</b> (NCALIB, options BEAM_FACTORS(for Stokes <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap229.png">) and INPOL* (where * = <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap231.png"> for the other three Stokes parameters).) 
+<LI> <b>Map the final corrected image in all Stokes parameters:</b> (NMAP) 
+</OL>
+<P>
+<A NAME=.detail><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>More details for some of the steps</b></A></H1>
+<P>
+<H2><A NAME=SECTION0005100000000000000> <b>Determine the instrumental polarization</b></A></H2>
+<P>
+Before determining the instrumental polarization using a calibrator, redundancy and selfcal solutions must be applied (use SELFCAL and ALIGN in the NCALIB option REDUN). This will also provide a useful check of the data quality. Note that at 92 cm (and in some cases 49 cm) there are background sources which may have to be included in the model used for ALIGN. Having run the ALIGN solution, NCALIB can be used to calculate the instrumental polarization (POLAR_OPTION: CALC) and examine the result (POLAR_OPTION: SHOW). Under normal conditions, the orthogonalities and positions of most dipoles should be under <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap233.png">, 
+and the ellipticities generally under 1%. Large values (more than a few 
+degrees or percent) probably indicate an instrumental problem (bad data) and require further investigation. Run a solution on a different calibrator as a check. Deviant points can be changed by hand (POLAR_OPTION: EDIT). Tables of instrumental polarization are also generated from time to time in Westerbork, and the values can be entered by hand (POLAR_OPTION: SET), or used to cross-check the solution from NCALIB. 
+As a check on the instrumental polarization thus generated, it may be useful to make a map of an unpolarized calibrator if one has been observed for a few hours or more during the same period (a shorter observation could also be used, but the map might prove difficult to interpret). Make sure that SELFCAL and ALIGN corrections have been successfully applied, and then look at the Q, U and V maps (made with NMAP). Ideally, they should be zero; the residual as a fraction of the flux density is an indication of the error which will be present in the polarization map of your observation. (If your source is very extended, however, the polarization error pattern generated by a point source may be misleading). 
+Finally, we have to determine (or at least check) the <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap223.png"> phase difference. This is best done using a linearly polarized calibrator (strictly speaking, a source with strong U signal). The method assumes that V is much smaller than U (since <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap237.png">, a nonnegligible V affects the <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap223.png"> phase), which is usually the case. The correction can be calculated (VZERO_OPTION: CALC, ASK, etc.) and applied to the data in several ways. Usually, the XY and YX phase zeroes have been determined and applied on-line to sufficient accuracy for most polarization maps, so the correction should be a few degrees or so. However, there have been instances where the difference was as much as <IMG ALIGN=BOTTOM ALT="" SRC="_11796_tex2html_wrap241.png">, so it is advisable to check. If various frequency channels are used, the phase difference should be calculated for each one separately, as the correction is usually frequency dependent.
+<P>
+<A NAME=.beam><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005200000000000000> <b>Correct for primary beam instrumental polarization</b></A></H2>
+<P>
+The instrumental polarization determined from a calibrator is, strictly speaking, only correct for a source at the beam center, though at most frequencies the variation within the half-power primary beam is small. For polarization mapping over large fields, there is a separate correction for off-axis instrumental polarization (NCALIB: NMODEL - BEAM).
+<P>
+<A NAME=.hints><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005300000000000000> <b>How do I know that my data are correct? - additional hints.</b></A></H2>
+<P>
+Errors; some error patterns; effect of source extent.
+<P>
+Ionospheric effects and the I map.
+<P>
+What can be done if a polarization combination is missing?
+<P>
+Etc.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
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+<P>.
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+<P>.
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+<P>.
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+<P>.
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+<P>.
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+<P>.
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+<P>.
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+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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new file mode 100644
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+#define noname_height 11
+static char noname_bits[] = {
+ 0x0c,0x60,0x00,0x02,0x00,0x00,0x46,0x06,0x08,0x00,0x00,0x0e,0x30,0x00,0x00,
+ 0x30,0x18,0x36,0xb0,0x81,0x03,0x00,0x00,0xcf,0x03,0x0e,0x00,0x00,0x1b,0xd8,
+ 0x00,0x00,0xd8,0x6c,0x32,0x90,0x01,0x02,0x00,0x80,0x4d,0x00,0x08,0x00,0x00,
+ 0x11,0xc8,0x00,0x00,0xdc,0x64,0x23,0x18,0x01,0x02,0x00,0x80,0x40,0x00,0x08,
+ 0x00,0x00,0x1b,0x8c,0x00,0x00,0x9c,0x46,0x23,0x18,0x01,0x02,0x00,0xc0,0xc7,
+ 0x03,0x08,0x00,0x00,0x0f,0x8c,0x00,0x00,0xc0,0x46,0x23,0x18,0x01,0x02,0x00,
+ 0xc0,0x4c,0x06,0x08,0x00,0x00,0x1f,0x8c,0x00,0x00,0xc0,0x46,0x23,0x18,0x01,
+ 0x02,0xfe,0xc3,0x08,0x06,0x08,0xfc,0x07,0x1d,0x8c,0xe0,0x3f,0x60,0x46,0x23,
+ 0x18,0x01,0x02,0x00,0xc0,0x68,0x06,0x08,0x00,0x80,0x11,0x8c,0x00,0x00,0xb0,
+ 0x46,0x32,0x93,0x19,0x02,0x00,0x80,0x6c,0x66,0x08,0x00,0x80,0x91,0xc9,0x00,
+ 0x00,0x98,0x64,0x36,0xb3,0x99,0x0f,0x00,0x80,0xcd,0x67,0x3e,0x00,0x00,0x9b,
+ 0xd9,0x00,0x00,0xfc,0x6c,0x1c,0xe0,0x00,0x00,0x00,0x00,0x87,0x01,0x00,0x00,
+ 0x00,0x0e,0x70,0x00,0x00,0x00,0x38};
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap233.png b/rcp_mosaic_21cm/_12039_tex2html_wrap233.png
new file mode 100644
index 0000000000000000000000000000000000000000..42a7a538f893e18a5c30194c63e42e1aa517d618
Binary files /dev/null and b/rcp_mosaic_21cm/_12039_tex2html_wrap233.png differ
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap233.xbm b/rcp_mosaic_21cm/_12039_tex2html_wrap233.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..455c5dba7371a8a6572767ce0f6a33ea6943010f
--- /dev/null
+++ b/rcp_mosaic_21cm/_12039_tex2html_wrap233.xbm
@@ -0,0 +1,9 @@
+#define noname_width 63
+#define noname_height 11
+static char noname_bits[] = {
+ 0x04,0x83,0x01,0x01,0x40,0x30,0x18,0x10,0x87,0xcd,0x86,0x01,0x70,0xd8,0x6c,
+ 0x18,0x84,0xec,0x86,0x01,0x40,0xc8,0x6e,0x18,0xc4,0xe8,0xc4,0x01,0x40,0x8c,
+ 0x4e,0x1c,0xc4,0x08,0x66,0xf1,0x43,0x8c,0x60,0x16,0xc4,0x08,0x26,0xd1,0x43,
+ 0x8c,0x60,0x12,0xc4,0x08,0x33,0xc1,0x40,0x8c,0x30,0x13,0xc4,0x88,0xf5,0x47,
+ 0x40,0x8c,0x58,0x7f,0x84,0xcc,0x04,0x79,0x43,0xc8,0x4c,0x10,0x9f,0xed,0xc7,
+ 0xff,0xf1,0xd9,0x7e,0x7c,0x00,0x07,0x00,0x00,0x00,0x70,0x00,0x00};
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap237.png b/rcp_mosaic_21cm/_12039_tex2html_wrap237.png
new file mode 100644
index 0000000000000000000000000000000000000000..991d4670e4185d10352c526690f40f773fcf1bce
Binary files /dev/null and b/rcp_mosaic_21cm/_12039_tex2html_wrap237.png differ
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap237.xbm b/rcp_mosaic_21cm/_12039_tex2html_wrap237.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d5ff2d5dd0e4114e04aef156f36df1f6e603d45d
--- /dev/null
+++ b/rcp_mosaic_21cm/_12039_tex2html_wrap237.xbm
@@ -0,0 +1,5 @@
+#define noname_width 14
+#define noname_height 12
+static char noname_bits[] = {
+ 0xf0,0x01,0x88,0x01,0x8c,0x01,0x8c,0x00,0x3c,0x00,0x78,0x06,0xc0,0x04,0xc2,
+ 0x1e,0x42,0x16,0x67,0x12,0x1d,0x3a,0x00,0x1b};
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap241.png b/rcp_mosaic_21cm/_12039_tex2html_wrap241.png
new file mode 100644
index 0000000000000000000000000000000000000000..d1765405ab7e224f7d68efad93e971528b4bd37f
Binary files /dev/null and b/rcp_mosaic_21cm/_12039_tex2html_wrap241.png differ
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap241.xbm b/rcp_mosaic_21cm/_12039_tex2html_wrap241.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0dd6247f41174ad4bd1918a3c0f073fba37750ed
--- /dev/null
+++ b/rcp_mosaic_21cm/_12039_tex2html_wrap241.xbm
@@ -0,0 +1,8 @@
+#define noname_width 44
+#define noname_height 12
+static char noname_bits[] = {
+ 0xf0,0x01,0x00,0x00,0x00,0x00,0x88,0x01,0x00,0x00,0x00,0x00,0x8c,0x01,0x00,
+ 0x18,0x00,0x00,0x8c,0x00,0x00,0x0e,0x00,0x00,0x3c,0x00,0x80,0x03,0xf8,0x07,
+ 0x78,0x06,0xe0,0x00,0xd8,0x0c,0xc0,0x04,0x30,0x00,0xf0,0x0f,0xc2,0x1e,0xf0,
+ 0x00,0xd8,0x00,0x42,0x16,0xc0,0x03,0xcc,0x08,0x67,0x12,0x00,0x0f,0xf8,0x07,
+ 0x1d,0x3a,0x00,0x1c,0x00,0x00,0x00,0x1b,0x00,0x00,0x00,0x00};
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap245.png b/rcp_mosaic_21cm/_12039_tex2html_wrap245.png
new file mode 100644
index 0000000000000000000000000000000000000000..699d34951f3ee0253498a272d2861c7c8946cd63
Binary files /dev/null and b/rcp_mosaic_21cm/_12039_tex2html_wrap245.png differ
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap245.xbm b/rcp_mosaic_21cm/_12039_tex2html_wrap245.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d1dcd0887eef5378e5236f3111e031c865239380
--- /dev/null
+++ b/rcp_mosaic_21cm/_12039_tex2html_wrap245.xbm
@@ -0,0 +1,8 @@
+#define noname_width 54
+#define noname_height 10
+static char noname_bits[] = {
+ 0x84,0x03,0x0c,0x00,0x84,0x03,0x0c,0x87,0x02,0x36,0x00,0x87,0x02,0x36,0xc4,
+ 0x06,0x37,0x00,0xc4,0x06,0x37,0xc4,0x06,0x27,0x00,0xc4,0x06,0x27,0x84,0x03,
+ 0x30,0x3f,0x84,0x03,0x30,0x04,0x00,0x30,0x3d,0x04,0x00,0x30,0x04,0x00,0x18,
+ 0x0c,0x04,0x00,0x18,0x04,0x00,0x2c,0x04,0x04,0x00,0x2c,0x04,0x60,0xa6,0x37,
+ 0x04,0x60,0x26,0x1f,0x60,0xbf,0x1f,0x1f,0x60,0x3f};
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap247.png b/rcp_mosaic_21cm/_12039_tex2html_wrap247.png
new file mode 100644
index 0000000000000000000000000000000000000000..d1765405ab7e224f7d68efad93e971528b4bd37f
Binary files /dev/null and b/rcp_mosaic_21cm/_12039_tex2html_wrap247.png differ
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap247.xbm b/rcp_mosaic_21cm/_12039_tex2html_wrap247.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..0dd6247f41174ad4bd1918a3c0f073fba37750ed
--- /dev/null
+++ b/rcp_mosaic_21cm/_12039_tex2html_wrap247.xbm
@@ -0,0 +1,8 @@
+#define noname_width 44
+#define noname_height 12
+static char noname_bits[] = {
+ 0xf0,0x01,0x00,0x00,0x00,0x00,0x88,0x01,0x00,0x00,0x00,0x00,0x8c,0x01,0x00,
+ 0x18,0x00,0x00,0x8c,0x00,0x00,0x0e,0x00,0x00,0x3c,0x00,0x80,0x03,0xf8,0x07,
+ 0x78,0x06,0xe0,0x00,0xd8,0x0c,0xc0,0x04,0x30,0x00,0xf0,0x0f,0xc2,0x1e,0xf0,
+ 0x00,0xd8,0x00,0x42,0x16,0xc0,0x03,0xcc,0x08,0x67,0x12,0x00,0x0f,0xf8,0x07,
+ 0x1d,0x3a,0x00,0x1c,0x00,0x00,0x00,0x1b,0x00,0x00,0x00,0x00};
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap249.png b/rcp_mosaic_21cm/_12039_tex2html_wrap249.png
new file mode 100644
index 0000000000000000000000000000000000000000..7617a83bd5cea3b13c97069bf40469baa8fea519
Binary files /dev/null and b/rcp_mosaic_21cm/_12039_tex2html_wrap249.png differ
diff --git a/rcp_mosaic_21cm/_12039_tex2html_wrap249.xbm b/rcp_mosaic_21cm/_12039_tex2html_wrap249.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2d045148a7c4a43fbfc2248f6be08cbe8d2d958b
--- /dev/null
+++ b/rcp_mosaic_21cm/_12039_tex2html_wrap249.xbm
@@ -0,0 +1,6 @@
+#define noname_width 29
+#define noname_height 11
+static char noname_bits[] = {
+ 0x00,0x00,0x03,0x00,0x00,0x80,0x0d,0x00,0x01,0xc0,0x0d,0x00,0x07,0xc0,0x09,
+ 0x00,0x1c,0x00,0x8c,0x1f,0x70,0x00,0xcc,0x06,0xc0,0x01,0x66,0x06,0xe0,0x00,
+ 0x6b,0x06,0x38,0x80,0x69,0x06,0x0e,0xc0,0xcf,0x03,0x03,0x00,0x00,0x00};
diff --git a/rcp_mosaic_21cm/images.pl b/rcp_mosaic_21cm/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..51042a06755d06bdc9b3dd9a12dfd64698a8d1b0
--- /dev/null
+++ b/rcp_mosaic_21cm/images.pl
@@ -0,0 +1,19 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$S_<<137>>h<<137>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap237.xbm">'; 
+$key = q/{}$1^circ.2x1^circ.2${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap245.xbm">'; 
+$key = q/{}$S_<<145>>h<<145>>;html_special_mark_lt;${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap241.xbm">'; 
+$key = q/{}$S_<<155>>h<<155>>;html_special_mark_lt;${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap247.xbm">'; 
+$key = q/{}$$0.0.1-65.1-8.0-20$${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap231.xbm">'; 
+$key = q/{}$1024x1024${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap233.xbm">'; 
+$key = q/{}$;html_special_mark_gt;2sigma${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap249.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/rcp_mosaic_21cm/labels.pl b/rcp_mosaic_21cm/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..d2801cdced7a7e4f847ad0334c6fdc8a08d8f4de
--- /dev/null
+++ b/rcp_mosaic_21cm/labels.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/rcp_mosaic_21cm.html"; 
+$external_labels{".scope"} ="$URL/rcp_mosaic_21cm.html"; 
+$external_labels{".summary"} ="$URL/rcp_mosaic_21cm.html"; 
+$external_labels{".contents"} ="$URL/rcp_mosaic_21cm.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_mosaic_21cm/rcp_mosaic_21cm.html b/rcp_mosaic_21cm/rcp_mosaic_21cm.html
new file mode 100644
index 0000000000000000000000000000000000000000..83ac4d0de098c575a3f9f5730c773b2a6045f80f
--- /dev/null
+++ b/rcp_mosaic_21cm/rcp_mosaic_21cm.html
@@ -0,0 +1,155 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Mosaicing at 21 cm</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_mosaic_21cm.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_mosaic_21cm.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_mosaic_21cm.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_mosaic_21cm.html#SECTION0004000000000000000> <b>Summary of the recipe</b></A>
+</UL>
+Author: T. Ghosh
+<P>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+This recipe suggests a way for making a 21-cm continuum mosaic map. In this example, a particular field was chosen where there were many previously-known radio sources within the region to be mapped. Hence, we knew that there was sufficient flux-density for almost all of the pointing centres to allow  us to run <i>selfcal</i>. If the user is not sure of having enough SNR for this, a modified version can be used.  Hence, consider this recipe as just a starting point, and <i>add salt to your taste</i>.
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+In the mosaic mode of observation, during one 12-hour period the telescopes, along with the fringe-stopping and the delay-tracking centres, cycle through a grid of pointings a number of times. In Fig 003.1, we used a 13 x 5 grid of these so called, <i>pointing centres</i>. There were about 21 cuts (or spokes), each containing two scans of 10-s duration for each pointing centre. The total 40-MHz bandwidth at 21 cm is usually divided into eight 5-MHz channels (although these are not contiguous). Hence, the data file had the following set indices (see also Ch 3.):  <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap231.png">
+<P>
+For a particular pointing centre, the reduction methodology is very much the same as that in Recipe 004. <b>However, all the maps are to be made using a common reference point (NMAP-option REFERENCE)</b>. Usually, for a large number of pointing centres, book-keeping etc. could be quite difficult. Here, all the advantages of the Automatic Batch Processing facility (ABP, Appendix D) can be very easily exploited. In the  following section we detail all the steps, indicating the pre-ABP, the ABP, and the post ABP stages, Stage I, II and III respectively, that were used to generate the map in Fig 003.1. These three stages also coincide with the <em>calibration using a different source</em>, the <em>Selfcal-Model formation loop for all the pointing centres</em>, and the <em>mosaicing</em> stages.
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe</b></A></H1>
+<P>
+<b>STAGE I:</b>
+<P>
+<OL><LI> <b>Load your data:</b> Source data from tape or optical disk (NSCAN). See also Recipe ``Reading data in Dwingeloo''. Also read the data from observations of a calibration source, (e.g. 3C147 in the case of Fig 003.1) made just before or after the <em>source field</em>. 
+<LI> <b>Inspect the data file and flag bad points mentioned on the WSRT green sheet :</b> (NSCAN, option SHOW etc). 
+<LI> <b>Calculate antenna-based phase and gain correction factors for the Calibrator data:</b> (NCALIB, option REDUNDANCY, suboption SELFCAL, using a model file obtained from AGB ) 
+<LI> <b>Copy the corrections to the source data:</b> (NCALIB, option SET, suboption COPY) 
+</OL>
+<P>
+<b>STAGE II:</b>
+<P>
+This stage could be batch processed (APPENDIX D). In the following, we first write a name for each task, which briefly describes the function of the step too. Within the bracket, we mention the programme to be used, and comment on a few important input parameters. Depending upon the flux density of the strongest source in the map of a particular pointing centre, the Stage is stopped at various <b>Exit points</b>.
+<P>
+For each pointing centre:
+<P>
+<OL><LI> <b>Raw:</b> (NMAP, make a <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap233.png"> pixel raw map of real size <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap245.png"> ) 
+<LI> <b>Find1:</b> (NMODEL, find model components down to a suitable limit e.g. 6 w.u. here) 
+</OL>
+<P>
+<b>Exit point 1:</b> If the flux density of the strongest component, <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap237.png"> is less than limit 1 (12 w.u., here) - STOP - Proceed to next pointing centre.
+<P>
+<OL><LI> <b>Upd1:</b> (NMODEL, Update the model list, delete sources weaker than a certain limit after updating, e.g. 6 w.u) 
+<LI> <b>Upd2:</b> (NMODEL, Second iteration of the above) 
+<LI> <b>Self1:</b> (NCALIB, self-calibrate ONLY the PHASE of the data using model, Upd2) 
+<LI> <b>Sub1:</b> (NMAP, make <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap245.png"> map after subtracting model, Upd2) 
+</OL>
+<P>
+<b>Exit point 2:</b> If <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap241.png">  limit 2 (20 w.u. here) - STOP - Proceed to next pointing centre.
+<P>
+<OL><LI> <b>Find2:</b> (NMODEL, find model components from map, Sub1 down to a suitable limit e.g. 5 w.u. here and add to the model, Upd2) 
+<LI> <b>Upd3:</b> (NMODEL, update the model list, Find2 and  delete sources weaker than a certain limit e.g. 5 w.u here) 
+<LI> <b>Upd4:</b> (NMODEL, second iteration of the above) 
+<LI> <b>Self2:</b> (NCALIB, self-calibrate the data using model, Upd4) 
+<LI> <b>Del1:</b> (NSCAN, delete scans with selfcal-amplitude and/or phase noise <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap249.png">) 
+<LI> <b>Sub2:</b> (NMAP, make <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap245.png">  map after subtracting model, Upd4) 
+</OL>
+<P>
+<b>Exit point 3:</b> If <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap247.png">  limit 3 (40 w.u. here) - STOP - Proceed to next pointing centre.
+<P>
+<OL><LI> <b>Find3:</b> (NMODEL, find model components from map, Sub2 down to a suitable limit e.g. 2.5 w.u. here and add to the model, Upd4) 
+<LI> <b>Upd5:</b> (NMODEL, update the model list, Find3 and delete soucres weaker than a certain limit e.g. 2.5 w.u here) 
+<LI> <b>Upd6:</b> (NMODEL, second iteration of the above) 
+<LI> <b>Self3:</b> (NCALIB, self-calibrate the data using model, Upd6) 
+<LI> <b>Del2:</b> (NSCAN, delete scans with selfcal-amplitude and/or phase noise <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap249.png">) 
+<LI> <b>Sub3:</b> (NMAP, make <IMG ALIGN=BOTTOM ALT="" SRC="_12039_tex2html_wrap245.png"> map after subtracting model, Upd6) 
+</OL>
+<P>
+<b>End of stage II</b>
+<P>
+At this point, for all the pointing centres, one should have a good model list, and a residual map. The common model components in the overlapping region can be checked for positional agreement. These can be cross-checked against any source within the region whose accurate position is known from the literature. Usually, agreements within 1 arcsec was achieved at this stage, which was already 1/10 th of the synthesised beam.
+<P>
+Depending upon the quality of the maps, they can be grouped into four classes.
+<P>
+<b>A.</b> Good maps, where noise is already at the theoretical limit, though there may still be residual sources, and their grating rings and sidelobes.
+<P>
+<b>B.</b> Maps containing grating rings from sources beyond the mapped region.
+<P>
+<b>C.</b> Maps with bad scans.
+<P>
+<b>D.</b> Maps with amplitude or/and Phase calibration problems.
+<P>
+For Class B maps, make larger low-resolution maps and try to include the strong (offending) source in the model list, and then start again at the beginning of Stage I (retaining the 'outside sources', though).
+<P>
+For Class C maps, search out the bad data (no easy-solution, sorry), delete it, and start again.
+<P>
+For Class D maps, there may be spurious sources in the model-list. Plot them, (NPLOT) and try to locate suspects, delete these, and continue (refer to sec..... if this doesn't help).
+<P>
+<b>STAGE III:</b>
+<P>
+Once all the maps are of Class A-quality, do the following:
+<P>
+<OL><LI> <b>Mkbeam :</b> (NMAP. Make beams for all the pointing centres) 
+<LI> <b>Clean :</b> (NCLEAN, option UVC. Clean the entire map with the number of components = 100, Gain = 0.1 and a Cycle-Depth value of 0.35) 
+<LI> <b>Restore :</b> (NCLEAN, option UREST. Restore both the model and the clean components) 
+<LI> <b>Extract :</b> (NMAP, option FIDDLE, suboption EXTRACT. Write out a smaller section of this map into one set index of a common map file that will be the input for the MOSAIC combination, here, inner 700 x 700 pixels of each pointing centre were used) 
+<LI> <b>Mosaic :</b> (NMAP, option FIDDLE, suboption MOSC. This part of the programme corrects the input maps for primary beam attenuation and then averages them with proper weightage) 
+<LI> <b>Ready to serve:</b> (NPLOT, NGIDS, write out FITS image and take it to AIPS ..... use the garnish of your choice) 
+</OL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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diff --git a/rcp_mosaic_92cm/images.pl b/rcp_mosaic_92cm/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_mosaic_92cm/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_mosaic_92cm/labels.pl b/rcp_mosaic_92cm/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..c86986be914aa71a23c6e20496b46081c304fc8a
--- /dev/null
+++ b/rcp_mosaic_92cm/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_mosaic_92cm.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_mosaic_92cm/rcp_mosaic_92cm.html b/rcp_mosaic_92cm/rcp_mosaic_92cm.html
new file mode 100644
index 0000000000000000000000000000000000000000..f6edd85dbba4ac43f756721b6be5387e17239383
--- /dev/null
+++ b/rcp_mosaic_92cm/rcp_mosaic_92cm.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Mosaicing at 92 cm</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_mosaic_92cm.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_old_data.ps b/rcp_old_data.ps
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+++ b/rcp_old_data.ps
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diff --git a/rcp_old_data/images.pl b/rcp_old_data/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_old_data/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_old_data/labels.pl b/rcp_old_data/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..bb4b757aaed8dbe6299723872f5f826e7eb95f96
--- /dev/null
+++ b/rcp_old_data/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_old_data.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_old_data/rcp_old_data.html b/rcp_old_data/rcp_old_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..f5854cf16a7119ddf5b0f6b6044350a2fc9d3ce7
--- /dev/null
+++ b/rcp_old_data/rcp_old_data.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Old WSRT data (1979-1984)</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_old_data.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
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+newstar@nfra.nl
diff --git a/rcp_pulsar_imaging.ps b/rcp_pulsar_imaging.ps
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--- /dev/null
+++ b/rcp_pulsar_imaging.ps
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diff --git a/rcp_pulsar_imaging/images.pl b/rcp_pulsar_imaging/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_pulsar_imaging/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_pulsar_imaging/labels.pl b/rcp_pulsar_imaging/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..74c4d1de4e6c9413dc272da66ac75696af008fa9
--- /dev/null
+++ b/rcp_pulsar_imaging/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_pulsar_imaging.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_pulsar_imaging/rcp_pulsar_imaging.html b/rcp_pulsar_imaging/rcp_pulsar_imaging.html
new file mode 100644
index 0000000000000000000000000000000000000000..589e58dbaa80ca4c0c9dbd154202438da9afe4dc
--- /dev/null
+++ b/rcp_pulsar_imaging/rcp_pulsar_imaging.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Pulsar Imaging</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_pulsar_imaging.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_read_data.ps b/rcp_read_data.ps
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diff --git a/rcp_read_data/images.pl b/rcp_read_data/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_read_data/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_read_data/labels.pl b/rcp_read_data/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..a7acb178162696ae8965087744c8fa38954e0a28
--- /dev/null
+++ b/rcp_read_data/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/rcp_read_data.html"; 
+$external_labels{".scope"} ="$URL/rcp_read_data.html"; 
+$external_labels{".detail.x"} ="$URL/rcp_read_data.html"; 
+$external_labels{".summary"} ="$URL/rcp_read_data.html"; 
+$external_labels{".contents"} ="$URL/rcp_read_data.html"; 
+$external_labels{".detail"} ="$URL/rcp_read_data.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_read_data/rcp_read_data.html b/rcp_read_data/rcp_read_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..cb95dffe9487f355b0bdd893496b8b18f50fb616
--- /dev/null
+++ b/rcp_read_data/rcp_read_data.html
@@ -0,0 +1,91 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Reading WSRT Data (in Dwingeloo)</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_read_data.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=rcp_read_data.html#SECTION0002000000000000000> <b>Scope of the recipe</b></A>
+<LI> <A NAME=tex2html3 HREF=rcp_read_data.html#SECTION0003000000000000000> <b>Introduction and background</b></A>
+<LI> <A NAME=tex2html4 HREF=rcp_read_data.html#SECTION0004000000000000000> <b>Summary of the recipe</b></A>
+<LI> <A NAME=tex2html5 HREF=rcp_read_data.html#SECTION0005000000000000000> <b>More details for some of the steps</b></A>
+<UL> 
+<LI> <A NAME=tex2html6 HREF=rcp_read_data.html#SECTION0005100000000000000> <b>..</b></A>
+</UL>
+</UL>
+Author: A.R. Foley
+<P>
+<A NAME=.scope><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000> <b>Scope of the recipe</b></A></H1>
+<P>
+...........
+<P>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000> <b>Introduction and background</b></A></H1>
+<P>
+<A NAME=.summary><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000> <b>Summary of the recipe</b></A></H1>
+<P>
+The following is a step-by-step summary of the processing recipe. For some of these steps, more detail is provided below.
+<P>
+<OL><LI> <b>... :</b> 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+<LI> <b>... :</b> 
+</OL>
+<P>
+<A NAME=.detail><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000> <b>More details for some of the steps</b></A></H1>
+<P>
+<A NAME=.detail.x><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0005100000000000000> <b>..</b></A></H2>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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diff --git a/rcp_simulated_data/images.pl b/rcp_simulated_data/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_simulated_data/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_simulated_data/labels.pl b/rcp_simulated_data/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..11c5bd23d35955aad6934f88e0194364cf5581ec
--- /dev/null
+++ b/rcp_simulated_data/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_simulated_data.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_simulated_data/rcp_simulated_data.html b/rcp_simulated_data/rcp_simulated_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..5b365e378dc1c2533f52a750bc1b1ee44bfbbc7d
--- /dev/null
+++ b/rcp_simulated_data/rcp_simulated_data.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Simulated UV Data</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_simulated_data.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_spectral_dr.ps b/rcp_spectral_dr.ps
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--- /dev/null
+++ b/rcp_spectral_dr.ps
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diff --git a/rcp_spectral_dr/images.pl b/rcp_spectral_dr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_spectral_dr/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_spectral_dr/labels.pl b/rcp_spectral_dr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..663706d31c7300f50c558798c3a080a4a3bf668c
--- /dev/null
+++ b/rcp_spectral_dr/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_spectral_dr.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_spectral_dr/rcp_spectral_dr.html b/rcp_spectral_dr/rcp_spectral_dr.html
new file mode 100644
index 0000000000000000000000000000000000000000..073d0396e87fda36578c965851d35072a08d287a
--- /dev/null
+++ b/rcp_spectral_dr/rcp_spectral_dr.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: High Spectral Dynamic Range</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_spectral_dr.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_uvfits_output.ps b/rcp_uvfits_output.ps
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--- /dev/null
+++ b/rcp_uvfits_output.ps
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+++ b/rcp_uvfits_output/images.pl
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+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_uvfits_output/labels.pl b/rcp_uvfits_output/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..94adf9389a1cf35bfea89f7534e818024b1650f3
--- /dev/null
+++ b/rcp_uvfits_output/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_uvfits_output.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_uvfits_output/rcp_uvfits_output.html b/rcp_uvfits_output/rcp_uvfits_output.html
new file mode 100644
index 0000000000000000000000000000000000000000..11b701ce0c60592e89fd9083b845f50cc17dd5e0
--- /dev/null
+++ b/rcp_uvfits_output/rcp_uvfits_output.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Generating UVFITS tapes for AIPS</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_uvfits_output.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_variability.ps b/rcp_variability.ps
new file mode 100644
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--- /dev/null
+++ b/rcp_variability.ps
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diff --git a/rcp_variability/images.pl b/rcp_variability/images.pl
new file mode 100644
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--- /dev/null
+++ b/rcp_variability/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_variability/labels.pl b/rcp_variability/labels.pl
new file mode 100644
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--- /dev/null
+++ b/rcp_variability/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_variability.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_variability/rcp_variability.html b/rcp_variability/rcp_variability.html
new file mode 100644
index 0000000000000000000000000000000000000000..75a4012ee06253b832d50d72538e60e5fe4562b0
--- /dev/null
+++ b/rcp_variability/rcp_variability.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Variability</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_variability.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/rcp_very_old_data.ps b/rcp_very_old_data.ps
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+(chapter)f(-)f(June)i(13,)f(1997)0 59 y Fb(Pro)r(cessing)22
+b(recip)r(e:)30 b(Old)23 b(WSR)-6 b(T)23 b(data)g(\(1971-1979\))0
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diff --git a/rcp_very_old_data/images.pl b/rcp_very_old_data/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/rcp_very_old_data/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/rcp_very_old_data/labels.pl b/rcp_very_old_data/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..033405fbfad5198162e79dc86a342db2000b5791
--- /dev/null
+++ b/rcp_very_old_data/labels.pl
@@ -0,0 +1,6 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".contents"} ="$URL/rcp_very_old_data.html"; 
+
+1;
\ No newline at end of file
diff --git a/rcp_very_old_data/rcp_very_old_data.html b/rcp_very_old_data/rcp_very_old_data.html
new file mode 100644
index 0000000000000000000000000000000000000000..c9607c7c95f17e6217c36910e89d8d2608432dad
--- /dev/null
+++ b/rcp_very_old_data/rcp_very_old_data.html
@@ -0,0 +1,57 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Processing recipe: Old WSRT data (1971-1979)</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=rcp_very_old_data.html#SECTION0001000000000000000>Contents</A>
+</UL>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/readme.txt b/readme.txt
new file mode 100755
index 0000000000000000000000000000000000000000..ba67d0ac7695cb96a64f7f8d3db76e0b1ef2d211
--- /dev/null
+++ b/readme.txt
@@ -0,0 +1,83 @@
+Updated December 4  1995
+Ger de Bruyn
+
+This directory contains MDL files for the primary and secondary WSRT
+flux density and position calibrators at the wavelengths of 6cm (4874
+MHZ), 21cm (1412 MHz), 49cm (608.8 MHz) and 92cm (325.125 MHz).
+
+The WSRT flux density scale is based on the Baars et al.  (Astron.
+Astrophys.  61, 104, 1977) scale values for the source 3C286.  3C286
+is not known to be variable to more than 1%.  The secondary
+calibrators 3C48 and 3C147 are, however, known to be variable, by
+about a few %, at wavelengths of 6 and 21 cm, and possibly also at
+longer wavelengths.  The values in the models may therefore have to be
+changed somewhat.  At 92cm we also have included models for 3C295 and
+3C345.  3C295 is a double radio source (4" separation) that CANNOT
+vary on human timescales (the source is tens of kpc in diameter) and
+will be used in the future to check the variability of all other
+calibrators.  At 6cm and 21cm 3C295 is strongly resolved across the
+array and is therefore less suitable as a calibrator.  The source
+3C345 is polarized (about 3% at 92cm) and can be used to check any
+phase-difference between the X and Y dipoles. In the future we hope to
+make regular observations at 92cm of either this source or other
+polarized calibrators (e.g. 3C303).
+
+At frequencies different from the normal ones the values will have to
+be changed according to the spectral index of the source.  Especially
+for 21cm line observations at large heliocentric velocities the
+correction may be several % and should not be neglected.  The values
+for the spectral index (spectral index = dlog(S)/dlog(freq) are:
+ at 6cm: 3C48 -0.95, 3C147 -0.91, 3C286 -0.62
+ at 21cm: 3C48 -0.84, 3C147 -0.70, 3C286 -0.45
+ at 92cm: 3C48 -0.68, 3C147 -0.62, 3C286 -0.34, 3C295 -0.60
+
+At 49 cm the band is so narrow that you will never have to worry about
+the spectral index.
+
+Especially the low-frequency models contain a varying numbers of
+background sources. The fluxdensities of these background sources
+obviously need to be adjusted for the frequency dependent primary
+beamwidth. You can do this using NMODEL, option FEDIT. This option
+will then ask you for a reference epoch (use B1950) and a SCN-file
+from which it gets the pointing centre of the calibrator observation.
+It then scales the background sources using a COS(cfr)**6 function
+(where c=0.0629, r is the radius in degrees and f is the frequency in
+MHz) which assumes that the primary beams scale with frequency. This
+is a good first order approximation.
+
+(The spectral indices at 92cm are only approximate. Most of the WSRT
+calibrators are socalled SSC sources which show a spectral turnover
+around 100-200 MHz).
+
+
+When doing bandpass calibration in line observations it is strongly
+advised to use a frequency INDEPENDENT value of the flux density. The
+models in this directory do not have a spectral index, so this will be
+the default when you use these models for calibration. The reference
+frequency in the header of the model is therefore not used.  (Note
+that if you would use a spectral index then each source in the
+synthesized field will adopt the spectral index of the calibrator and
+when you subtract images from two sides of the band then part of the
+source, and all its side/grating lobes, will remain in the image).
+
+However, it is possible to give the calibrator a spectral index using
+the EDIT command in NMODEL (first go to the MODIFY subgroup of
+keywords). (If you want to give all sources in the model the same
+spectral index you can use the FEDIT option).  This could be useful
+when you have data with the broadband 92cm DCB (which permits
+observations from 300 -390 MHz) and you want to determine real
+spectral indices for sources in your field. But if you wish to
+conduct bandwidth synthesis with the broadband 92cm system then again
+it is best to only change the models for the different primary beams
+but not for the intrinsic spectral index.
+
+
+If you have any questions about using the calibrator models I refer to
+NEWSTAR recipe #13 (to be written), or contact me (Ger de Bruyn,
+0521-595257, ger@nfra.nl)).
+
+
+
+
+
+
diff --git a/record_replay.ps b/record_replay.ps
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+b(batc)o(h)h(\014le)g(from)e(a)h(protot)o(yp)q(e.)19
+b(Whether)14 b(this)g(will)e(mak)o(e)g(a)i(friendlier)f(metho)q(d)g
+(than)h(the)g(presen)o(t)h(one)f(\(as)g(used)0 1228 y(in)f(WENSS)h(adn)
+g(WHISP\))g(remains)f(to)h(b)q(e)g(seen.)935 2995 y(3)p
+eop
+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/record_replay/images.pl b/record_replay/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/record_replay/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/record_replay/labels.pl b/record_replay/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..284da31b591052a6a298075c78d5bb61b58bae7e
--- /dev/null
+++ b/record_replay/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".intro"} ="$URL/record_replay.html"; 
+$external_labels{".renumber"} ="$URL/record_replay.html"; 
+$external_labels{".create"} ="$URL/record_replay.html"; 
+$external_labels{".batch"} ="$URL/record_replay.html"; 
+$external_labels{".contents"} ="$URL/record_replay.html"; 
+$external_labels{".replay"} ="$URL/record_replay.html"; 
+
+1;
\ No newline at end of file
diff --git a/record_replay/record_replay.html b/record_replay/record_replay.html
new file mode 100644
index 0000000000000000000000000000000000000000..5d6410990341c3759dbc3cd01feb8d82d06ad60c
--- /dev/null
+++ b/record_replay/record_replay.html
@@ -0,0 +1,162 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Capturing <i>NEWSTAR </i> program runs for repeated execution </b>
+<P>
+<P><em>Contributed by Johan Hamaker, November 1995  <P></em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=record_replay.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=record_replay.html#SECTION0002000000000000000>  <b>Introduction </b></A>
+<LI> <A NAME=tex2html3 HREF=record_replay.html#SECTION0003000000000000000>  <b>The batch recording method </b></A>
+<LI> <A NAME=tex2html4 HREF=record_replay.html#SECTION0004000000000000000>  <b>Creating a batch file </b></A>
+<LI> <A NAME=tex2html5 HREF=record_replay.html#SECTION0005000000000000000>  <b>Replaying a batch file </b></A>
+<LI> <A NAME=tex2html6 HREF=record_replay.html#SECTION0006000000000000000>  <b>Renumbering a batch file </b></A>
+</UL>
+<A NAME=.intro><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0002000000000000000>  <b>Introduction </b></A></H1>
+<P>
+        The <i>NEWSTAR </i> mechanism for repetitive execution programs with a minimum of user interaction is through the definition of default parameter values in a process symbol table.
+<P>
+        While attractive in concept, this approach is rather difficult to handle in practice for several reasons: 
+ <UL><LI>   There is a variety of mechanims involved and invoking the right one in each particular situation requires a thorough understanding of the entire parameter system.
+<P>
+<LI>   The symbol-table utilities dws[pecify] and dwv[iew] present the parameters in an arbitrary order, including (often a great number of) them that are irrelevant for the program run to be controlled.
+<P>
+<LI>   If a parameter is to be prompted for more than once during the program run, the successive values must be stored in the symbol table as successive value sets (separated by colons) for that parameter. 
+ </UL>  
+ These two effects combined make it difficult to keep track of the parameter set for a program run, in particular when a saved parameter set must be modified in detail to cover a slightly different situation. In practice, batch scripting has so far remained something of a black art mastered only by a few specialists.
+<P>
+<A NAME=.batch><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>The batch recording method </b></A></H1>
+<P>
+        The idea of the batch recording method is very simple: The parameter values from a manually executed program run are saved an ASCII file rather than the symbol table. They are recorded precisely in the order in which they are actually obtained and with the literal values as typed in by the user, as in the following simple example for NSCAN:
+<P>
+    <PRE>
+        OPTION = sh 
+          INPUT_SCN_NODE = ** 
+          INPUT_SCN_NODE = f 
+            FILE_ACTION = #  
+          INPUT_SCN_NODE = t 
+            FILE_ACTION = layout 
+            FILE_ACTION = ov 
+              OVERVIEW = obs 
+            FILE_ACTION = q 
+          INPUT_SCN_NODE =  
+        OPTION =  
+</PRE>
+<P>
+        For an identical re-execution of the program run, one may use this file as input. One may also edit it, however, to correct errors or instruct the program to prompt for those parameters that the user wants to control. For example, the above file could be edited to become:
+<P>
+    <PRE>
+        OPTION = SHOW  !    1  
+          INPUT_SCN_NODE = **  !    2 
+          INPUT_SCN_NODE = /ASK  !    3 
+            FILE_ACTION = LAYOUT  !    4 
+            FILE_ACTION = OVERVIEW  !    5 
+              OVERVIEW = OBS  !    6
+            FILE_ACTION = QUIT  !    7 
+          INPUT_SCN_NODE = ""  !    8 
+        OPTION = QUIT  !    9
+</PRE>
+<P>
+        There are several important advantages over the use of the symbol table:
+ <UL><LI>   The parameters appear in the batch file precisely in the order in which they will be used.
+<P>
+<LI>   Indentation may be used as shown above to represent the 'parameter hierarchy' and the way the program branches back after completion of a request, making it easy to follow the program's execution while reading the batch file.
+<P>
+<LI>   Comments may be appended to parameter values to facilitate the tracing of errors.
+ </UL>
+<P>
+        The method is implemented in three new commands:
+ <UL><LI>     dwrec &lt;program&gt;.&lt;ext&gt; to record a run of &lt;prorgam&gt; in a
+                file &lt;program&gt;.&lt;ext&gt;;
+<P>
+<LI>     dwrep &lt;program&gt;.&lt;ext&gt; to replay the file.
+<P>
+<LI>     dwren &lt;program&gt;.&lt;ext&gt; to [re]number the lines by appending a
+                comment to each line in the file, as shown above, for debugging
+                purposes
+ </UL>
+<P>
+<A NAME=.create><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0004000000000000000>  <b>Creating a batch file </b></A></H1>
+<P>
+        To create a batch file, use the command
+<P>
+  dwrec &lt;program&gt;.&lt;extension&gt;
+<P>
+The program will be excuted in the normal way, the only difference being that a batch file is created containing lines of the form
+<P>
+  &lt;paremeter&gt; = &lt;value&gt;  !  &lt;line number&gt;
+<P>
+        The user's replies are stored litterally; this is unlike in the <i>NEWSTAR </i> log files, where the value shown is the one actually used after interpretation of the user's reply by the parameter system.
+<P>
+        Parameters to be prompted for in later replays of the batch file must be given the value /ASK. This may be done by editing the file, but it is also possible to instruct the system to set thids special value at recording time, by appending the string !? to the reply. As an example, we show the complete run that would create the second example of the <A HREF="#.batch">preceding section</A>.
+<P>
+<em>put script here</em><A NAME=.replay><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0005000000000000000>  <b>Replaying a batch file </b></A></H1>
+<P>
+        The command to replay a batch file is
+<P>
+  dwrep &lt;program&gt;.&lt;extension&gt;
+<P>
+The program will run in nthe normal way, taking inputs from the batch file and prompting the user only where the value /ASK is specified.
+<P>
+<A NAME=.renumber><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H1><A NAME=SECTION0006000000000000000>  <b>Renumbering a batch file </b></A></H1>
+<P>
+        To renumber the lines, e.g. after manual addition of lines, use the command
+<P>
+  dwren &lt;program&gt;.&lt;extension&gt;
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/remote_tape.txt b/remote_tape.txt
new file mode 100644
index 0000000000000000000000000000000000000000..3956a7be5403d63f87c9d40047b662518ed70a31
--- /dev/null
+++ b/remote_tape.txt
@@ -0,0 +1,66 @@
+
+Transparent reading of the Optical Disks with Newstar
+-----------------------------------------------------
+
+It is now possible to access the optical disk units that are 
+connected to the VAX while working on a Unix machine.
+
+In Dwingeloo, the following tape-devices have been defined:
+
+   MAG4   //rzmvx4.astron.nl:1100/RZMVX4$MUA0  
+   MAG5   //rzmvx4.astron.nl:1101/RZMVX4$MUA1
+
+These devives allow you to read data from the units MUA0 and MUA1
+as if they were connected to your Unix machine.
+
+If you work on e.g. rzmws10 and you want to get data from MUA0,
+just run NSCAN and specify unit 4. 
+
+
+Note 1: Implementation
+ 
+   Transparent reading is implemented by a server on the VAX and
+   an extension of the tape-handling routines in Newstar.
+   The server on the VAX is USER5:[DEVOSCM.RMTD]RMTD.EXE
+   The server has to be started on two ports, this can be done
+   by including in the system-startup:
+
+      @user5:[devoscm.rmtd]rmtd_start.com  
+  
+   which will submit two jobs on RZMVX4_BATCH.
+
+   The names of the remote units have been defined in the startup file
+       $n_src/sys/newstar_nfra.csh
+
+   The routines changed for the implementation are $n_src/wng/wnftrw.cun 
+   and $n_src/wng/wnf???_x.cun. The code for the client side of the 
+   network is in wnftrw.cun. The changes in the other files are: (1) all
+   calls to open, close, read and write now go through a routine in 
+   wnftrw.cun and (2) all calls to routines wnftrw pass the MCA (not FCA)
+
+Note 2: Suggested testing
+
+   To test the reliability of the transparent tape-reading I suggest
+   the following. During the next week, all files read from Optical Disk
+   by the Reduction Group are read two times and then compared
+
+      1e. Unix: NSCAN LOAD UNIT=4 or 5 
+
+      2e. VAX:  NSCAN LOAD UNIT=4 or 5
+          Unix: ftp SCN-file
+                NSCAN CVX
+
+      3e. Unix: ~devoscm/tst.csh File1.SCN File2.SCN
+  
+   If the files have been loaded identically, no differences should appear.
+   The tst.csh procedure ignores differences of 1 unit in the data, since 
+   they can be produced by rounding errors during the time-averaging.
+
+   Any differences should be reported to Marco de Vos.
+
+   After testing some 10 SCN files, we are sure that no systematic errors 
+   take place. The remaining test is on reliability of the connection over
+   a longer period. This can be tested by using only the Unix version of 
+   Newstar to read data from the archive. After a month, we will have a 
+   good impression of the reliability. 
+
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new file mode 100644
index 0000000000000000000000000000000000000000..c98305c4bdf975c4a4a6db7daf807d9cdc78ddd0
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+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/scn_file/images.pl b/scn_file/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/scn_file/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/scn_file/labels.pl b/scn_file/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..30701481fd6214c963654bfed911d8024bd4ca72
--- /dev/null
+++ b/scn_file/labels.pl
@@ -0,0 +1,30 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".inspect"} ="$URL/scn_file.html"; 
+$external_labels{".model"} ="$URL/scn_file.html"; 
+$external_labels{".hierarchy"} ="$URL/scn_file.html"; 
+$external_labels{".edit"} ="$URL/scn_file.html"; 
+$external_labels{".apply"} ="$URL/scn_file.html"; 
+$external_labels{".contents"} ="$URL/scn_file.html"; 
+$external_labels{".polarisation"} ="$URL/scn_file.html"; 
+$external_labels{".delete"} ="$URL/scn_file.html"; 
+$external_labels{".operations"} ="$URL/scn_file.html"; 
+$external_labels{".reorganise"} ="$URL/scn_file.html"; 
+$external_labels{".gain.phase"} ="$URL/scn_file.html"; 
+$external_labels{".SCNSUM"} ="$URL/scn_file.html"; 
+$external_labels{".levels"} ="$URL/scn_file.html"; 
+$external_labels{".index.define"} ="$URL/scn_file.html"; 
+$external_labels{".SCNSUM.indices"} ="$URL/scn_file.html"; 
+$external_labels{".scn.hierarchy"} ="$URL/scn_file.html"; 
+$external_labels{".mosaic.sectors"} ="$URL/scn_file.html"; 
+$external_labels{".scn.indices"} ="$URL/scn_file.html"; 
+$external_labels{".corrections"} ="$URL/scn_file.html"; 
+$external_labels{".scan"} ="$URL/scn_file.html"; 
+$external_labels{".hypercube"} ="$URL/scn_file.html"; 
+$external_labels{".export"} ="$URL/scn_file.html"; 
+$external_labels{".sector"} ="$URL/scn_file.html"; 
+$external_labels{".scn.file"} ="$URL/scn_file.html"; 
+$external_labels{".creation"} ="$URL/scn_file.html"; 
+
+1;
\ No newline at end of file
diff --git a/scn_file/scn_file.html b/scn_file/scn_file.html
new file mode 100644
index 0000000000000000000000000000000000000000..31945f47f5f02e0926fde0451bad8ae9425ec053
--- /dev/null
+++ b/scn_file/scn_file.html
@@ -0,0 +1,350 @@
+<HEAD>
+<TITLE> The .SCN file </TITLE>
+</HEAD>
+<BODY><P>
+<P>
+<H1> The .SCN file </H1>
+<P><b></b><P>
+<b>Visibilities and associated data: The .SCN-file </b>
+<P>
+<P><em>Contributed by Johan Hamaker, November 1994  <P></em>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=scn_file.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=scn_file.html#SECTION0002000000000000000>  <b>Overview of .SCN file contents</b></A>
+<LI> <A NAME=tex2html3 HREF=scn_file.html#SECTION0003000000000000000>  <b>The visibility hypercube and its dimensions </b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=scn_file.html#SECTION0003100000000000000>  <b>.SCN-file hierarchy and indexing </b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=scn_file.html#SECTION0003110000000000000>  <b>The scan</b></A>
+<LI> <A NAME=tex2html6 HREF=scn_file.html#SECTION0003120000000000000>  <b>The sector</b></A>
+<LI> <A NAME=tex2html7 HREF=scn_file.html#SECTION0003130000000000000>  <b>The indexing levels </b></A>
+</UL> 
+<LI> <A NAME=tex2html8 HREF=scn_file.html#SECTION0003200000000000000>  <b>How index values are allocated</b></A>
+<LI> <A NAME=tex2html9 HREF=scn_file.html#SECTION0003300000000000000>  <b>The sector header </b></A>
+<LI> <A NAME=tex2html10 HREF=scn_file.html#SECTION0003400000000000000>  <b>The scan header </b></A>
+</UL> 
+<LI> <A NAME=tex2html11 HREF=scn_file.html#SECTION0004000000000000000>  <b>Operations on .SCN files in general</b></A>
+<UL> 
+<LI> <A NAME=tex2html12 HREF=scn_file.html#SECTION0004100000000000000>  <b>Creation </b></A>
+<LI> <A NAME=tex2html13 HREF=scn_file.html#SECTION0004200000000000000>  <b>Inspection </b></A>
+<UL> 
+<LI> <A NAME=tex2html14 HREF=scn_file.html#SECTION0004210000000000000>  <b>Editing </b></A>
+</UL> 
+<LI> <A NAME=tex2html15 HREF=scn_file.html#SECTION0004300000000000000>  <b>Export </b></A>
+<LI> <A NAME=tex2html16 HREF=scn_file.html#SECTION0004400000000000000>  <b>Reorganising sectors </b></A>
+<LI> <A NAME=tex2html17 HREF=scn_file.html#SECTION0004500000000000000>  <b>Deleting sectors </b></A>
+</UL> 
+<LI> <A NAME=tex2html18 HREF=scn_file.html#SECTION0005000000000000000>  <b>Operation on corrections in a .SCN file</b></A>
+<UL> 
+<LI> <A NAME=tex2html19 HREF=scn_file.html#SECTION0005100000000000000>  <b>Gain/phase corrections</b></A>
+<LI> <A NAME=tex2html20 HREF=scn_file.html#SECTION0005200000000000000>  <b>Polarisation corrections </b></A>
+<LI> <A NAME=tex2html21 HREF=scn_file.html#SECTION0005300000000000000>  <b>Controlling the application of corrections </b></A>
+</UL> 
+<LI> <A NAME=tex2html22 HREF=scn_file.html#SECTION0006000000000000000>  <b>Operations on model visibilities </b></A>
+</UL>
+<A NAME=.scn.file><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview of .SCN file contents</b></A></H1>
+<P>
+<A NAME=.SCNSUM><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P>
+        .SCN files hold all visibility data in <i>NEWSTAR </i>. The basic unit of data is the <em>scan</em>, an array of visibilities for one mosiac subfield, hour angle and frequency channel, with polarisation (XX, XY, ,YX, YY) and interferometer sequence number as its two dimensions. Series of scans that are contiguous in hour angle together form a <em>sector</em>. The organisation of the sectors in a .SCN file will be discussed <A HREF="#.SCNSUM.indices">below</A>.
+<P>
+        It is a fundamental tenet of <i>NEWSTAR </i> that visibility data are always stored as received from Westerbork. <em>Corrections</em> are stored separately as such, and only applied to the visibilities when the data are read in by a program. Thus, what changes during the history of a .SCN file is the correction tables, <em>not</em> the visibility data.
+<P>
+        An important mechanism for eliminating faulty data points is the use of <em>flags</em>. Since there are several different reasons for rejecting data, 8 different flag types are recognised. A <em>flag byte</em> is associated with each data point. Programs normally reject a data point if any one of these flags is set, but the user has the option ignore certain flag types.
+<P>
+        The <em>self-calibration</em> methods in <i>NEWSTAR </i> rely on comparing the observed visibility data with the visibilities of a <em>source model</em> to find the instrumental errors. To economise on the lengthy calculations necessary to generate the <em>model visibilities</em>, the latter may be saved in the .SCN file for reuse.
+<P>
+<A NAME=.hypercube><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000>  <b>The visibility hypercube and its dimensions </b></A></H1>
+<P>
+<A NAME=.scn.hierarchy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> The scan and sector structures in a .SCN-file with the indexing hierarchy in which they are embedded. 
+<A HREF="../fig/scn_hierarchy.ps"><STRONG>FIGURE</STRONG></A> 
+  <i><BR>See text for further explanation. </i>
+<P>
+        Visibilities in a synthesis observation are functions of a series of coordinate parameters. One may conceptually arrange them in a <em>hypercube</em> whose coordinate axes correspond to these parameters; alternatively, this hypercube may be visualised as a hierarchy in which each level corresponds to one of the parameters.
+<P>
+        The organisational model used in the .SCN file is a hyprid, in which the lowest levels form a compact array, which is embedded in a hierarchical <em>index structure</em> for the remaining levels. The order of the parameters in this arrangement is in principle quite arbitratry. <i>NEWSTAR </i>'s choice was motivated by considerations of efficiency in both storage space and sorting for the most important processes. The order is, from the bottom upwards:
+<P>
+ <UL><LI>   <em>Polarisation:</em> Each telescope contains 2 orthogonal dipoles named <em>X</em> and <em>Y</em>. Depending on the observing mode, there may be 4 (<em>XX, XY, YX, YY</em>), 2 (<em>XX, YY</em>) or 1 (<em>XX</em>) polarisation.
+<P>
+<LI>   <em>Interferometer:</em> The WSRT consisting of 14 telescopes, the number of interferometers formed between the elements can be 91 at most. Depending upon the availability of telescopes and the observing modes, the actual number (NIFR) is usually somewhat smaller. In the .SCN file, the interferometers are sorted in order of ascending baseline and assigned a sequence number from 0 to NIFR-1.
+<P>
+<LI>   <em>Hour Angle:</em> The hour angle for the middle of the integration interval to which the data pertain. Hour angles are referred to as such. The integration interval is a multiple of 10 UT seconds and is defined by the user when he reads in the data.
+<P>
+<LI>   <em>Frequency Channel:</em> For observations in several (NCHN) simultaneous frequency bands, these bands are numbered from 1 through NCHN. In a single observation, the bands are not necessarily equally wide and equidistant. By convention, the sum of all bands is called the <em>continuum channel</em> and assigned channel number 0.
+<P>
+<LI>   <em>Mosaic Subfield</em> or <em>Pointing Centre:</em> In a mosaic observation, subfields are repeatedly observed in a fixed sequence. The fields are assigned a sequence number starting at 0. By convention, field 0 is at the mosaic centre.
+<P>
+<LI>   <em>Observation:</em> An observation is a 'container' holding all the data that were read from a single WSRT observation <em>label</em> in a single run of NSCAN.load.
+<P>
+<LI>   <em>Group:</em> A group is likewise a container holding all observations loaded in a single NSCAN.load run.  
+ </UL>
+<P>
+        It is customary to loosely refer to the levels of this hierarchy as the <em>dimensions</em> of a six-dimensional <em>data (hyper)cube</em>. One should bear in mind, however, that the same 'dimension' may be of different magnitude in different 'sub-cubes' of this hypercube or, in other words, that the 'cube' is not regularly filled.
+<P>
+<A NAME=.hierarchy><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0003100000000000000>  <b>.SCN-file hierarchy and indexing </b></A></H2>
+<P>
+        An overview of the .SCN-file hierarchy is shown in  
+<A HREF=" #.scn.hierarchy">figure</A>. The levels correspond to those discussed  
+<A HREF="#.hypercube">above</A>. We shall discuss them from the bottom up.
+<P>
+        It is worth noting that the scan and sector headers combined contain all the information necessary to process the data. A sector may be divorced from the .SCN file without impairing its ability to be processed. The index blocks in the levels on top contain no 'scientific' information. Their only purpose is to organise the sectors.
+<P>
+<A NAME=.scan><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H3><A NAME=SECTION0003110000000000000>  <b>The scan</b></A></H3>
+<P>
+        The <em>scan</em> is the fundamental agggregate of data in a .SCN file. It is a two-dimensional array of visibilities for a single integration interval, with polarisation and interferometer as its dimensions.
+<P>
+        Associated with this block of data is a <em>scan header</em>. It contains descriptive data such as frequency and position parameters. In addition, it holds tables of those gain and phase corrections that may change from scan to scan, as well as data and correction statistics that are a measure of the data's quality. The contents are listed in the <A HREF="../src/nscan/sch.dsc"><b>definion file</b></A>.
+<P>
+<A NAME=.sector><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H3><A NAME=SECTION0003120000000000000>  <b>The sector</b></A></H3>
+<P>
+        A sequence of scans that is contiguous in hour angle is grouped together in a <em>sector</em>. The sector's contents are described in a <em>sector header</em>. Like the scan header, it contains descriptive data, corrections parameters that may be assumed to be constant for the time period covered by the sector and data/correction statistics for all the sector's scans combined. The contents are listed in the <A HREF="../src/nscan/sth.dsc"><b>definion file</b></A>.
+<P>
+<A NAME=.levels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<A NAME=.SCNSUM.indices><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H3><A NAME=SECTION0003130000000000000>  <b>The indexing levels </b></A></H3>
+<P>
+        The <A HREF="../file_indexing/file_indexing.html">index structure</A> in which the sectors are organised follows the levels listed <A HREF="#.hypercube">above</A>. The  
+&lt;sequence number&gt; is an extra index that allows one to have more than one sector for which the first four indices are identical. A complete  
+.SCN-sector designation reads:  
+ <DL COMPACT><DT>
+<DD> &lt;group&gt;.&lt;observation&gt;.&lt;field&gt;.&lt;channel&gt;.&lt;sequence number&gt;
+<P>
+ </DL>
+<P>
+<A NAME=.mosaic.sectors><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> Sectors in the uv plane. 
+<A HREF="../fig/mosaic_sectors.ps"><STRONG>FIGURE</STRONG></A> 
+ <i><BR>Left: For a standard observation the scans for a single observation and channel are contiguous and can be lumped together in a single sector. <BR>Right: In a mosaic observation the cuts for a given field are interleaved with cuts for other fields, so each cut is stored in a sector of its own. 
+<BR>The sector numbers shown are just by way of example. </i>
+<P>
+        One particularly important application of this possibility is in the organisation of the non-contiguous scans in a mosaic observation. In such an observation, the scans are not contiguous and therefore each 'hour-angle cut' forms a sector of its own (<A HREF=" #.mosaic.sectors">figure</A>).
+<P>
+<A NAME=.index.define><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0003200000000000000>  <b>How index values are allocated</b></A></H2>
+<P>
+<A NAME=.scn.indices><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> The allocation of the sector indices for a .SCN file. 
+<A HREF="../fig/scn_indices.ps"><STRONG>FIGURE</STRONG></A> 
+ <i><BR>- Every run of the NSCAN <em>LOAD</em> function creates a new <em>group</em>. 
+<BR>- Every (tape of optical-disk) label specified as input for such a run is stored in a new <em>observation</em>. 
+<BR>- The <em>field</em> and <em>channel</em> numbers are copied from the input. 
+<BR>- For a standard observation, the sequence number is 0. For a mosaic observation, the successive cuts for the same field and channel are given successive <em>sequence</em> numbers. </i>
+<P>
+        The method by which NSCAN allocates sector numbers is schematically shown in <A HREF=" #.scn.indices">figure</A>. The only control the user has is over the allocation of groups: Every NSCAN.load operation creates a new group, and the user defines which WSRT labels will be stored in that group.
+<P>
+<H2><A NAME=SECTION0003300000000000000>  <b>The sector header </b></A></H2>
+<P>
+        The sector header contains parametric data tha are constant throughout the sector. The most important groups are the following:  
+ <UL><LI>   Coordinates:  
+   <UL><LI>   right ascension (RA) and declination (DEC), both apparent and epoch;  
+  <LI>   start hour-angle (HAB) and increment between scans (HAI);  
+  <LI>   LSR frequency, frequency-channel number (CHN);  
+  <LI>   mosaic-subfield number (PTS);  
+  <LI>   telescope positions (RTP).  
+   </UL>
+<P>
+<LI>   Sector composition: Number of scans (SCN), number of  
+        polarisations (PLN), bandwidth (BAND), interferometer list  
+        (IFRP).
+<P>
+<LI>   Corrections: dipole errors.
+<P>
+<LI>   Noise statistics reported by the most recent  
+        <A HREF="../introduction/introduction.html#.selfcal">selfcal</A> extraction of corrections from  
+        the visibilities.
+<P>
+<LI>   Administrative information: length of a scan header plus data (SCNL).  
+ </UL>  For more details see the <A HREF="../src/nscan/sth.dsc">definition</A> file.
+<P>
+<H2><A NAME=SECTION0003400000000000000>  <b>The scan header </b></A></H2>
+<P>
+        The scan header contains the parametric data that apply specifically to one scan:  
+ <UL><LI>   Coordinate: Hour angle  
+<LI>   Corrections:  
+   <UL><LI>   Gain and phase corrections per  
+          <A HREF="../introduction/introduction.html#.SCNSUM">telescope</A>;  
+  <LI>   <A HREF="../introduction/introduction.html#.selfcal">global</A> corrections that may vary with  
+          hour angle: tropospheric and ionospheric refraction, extinction,  
+          Faraday rotation, clock;  
+   </UL>   
+<LI>   Noise statistics reported in the most recent  
+        <A HREF="../introduction/introduction.html#.selfcal">selfcal</A> extraction of corrections from  
+        the visibilities.  
+ </UL>  For more details see the <A HREF="../src/nscan/sch.dsc">definition</A> file.
+<P>
+<A NAME=.operations><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000>  <b>Operations on .SCN files in general</b></A></H1>
+<P>
+<A NAME=.creation><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004100000000000000>  <b>Creation </b></A></H2>
+<P>
+ <UL><LI>   From WSRT observations files: <A HREF="../nscan_descr/nscan_descr.html">NSCAN LOAD</A>.  
+<LI>   From ATCA (Australia Telescope Compact Array) files: NATNF  
+        LOAD.  
+<LI>   From old (R-series) SCN-files: <A HREF="../nscan_descr/nscan_descr.html">NSCAN FROM_OLD</A>.  
+<LI>   Simulated uv-data: NSIMUL.  
+ </UL>
+<P>
+<A NAME=.inspect><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004200000000000000>  <b>Inspection </b></A></H2>
+<P>
+Displays in tabular form:  
+ <UL><LI>   Summary of contents: <A HREF="../nscan_descr/nscan_descr.html">NSCAN SHOW</A>.  
+<LI>   Summary of one sector or scan header at a time: <A HREF="../nscan_descr/nscan_descr.html">NSCAN SHOW CONT           [CONT]</A>.  
+<LI>   Complete sector or scan header, one at a time: <A HREF="../nscan_descr/nscan_descr.html">NSCAN SHOW CONT           [CONT] SHOW</A>.  
+<LI>   Visibilities, weights, flags for one scan at a time: <A HREF="../nscan_descr/nscan_descr.html">NSCAN SHOW           CONT CONT DATA/WEIGHTS</A>.  
+<LI>   Telescope gain/phase corrections averaged over a range of scans:  
+        <A HREF="../ncalib_descr/ncalib_descr.html">NCALIB SHOW</A>  
+<LI>   Telescope dipole corrections averaged over a range of scans:  
+        <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR SHOW</A>  
+ </UL>
+<P>
+Graphic displays:  
+ <UL><LI>   Object or model visibilities vs. hour angle: NPLOT  
+        DATA/MODEL  
+<LI>   Object or model visibilities in the Cartesian UV plane:  
+        <A HREF="../nmap_descr/nmap_descr.html">NMAP..</A>  
+<LI>   Gain/phase corrections vs. hour angle: NPLOT  
+        TELESCOPE.  
+<LI>   Redundancy/Selfcal residuals: NPLOT RESIDUAL  
+ </UL>
+<P>
+        Additional possibilities for extracting. manipulating and displaying a variety of items from the .SCN file are available in  
+<A HREF="../ngcalc_descr/ngcalc_descr.html">NGCALC</A>.
+<P>
+<A NAME=.edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H3><A NAME=SECTION0004210000000000000>  <b>Editing </b></A></H3>
+<P>
+        Almost every value (observation parameters, corrections, etc) in the SCN-file headers may be edited manually through <A HREF="../nscan_descr/nscan_descr.html">NSCAN SHOW EDIT</A>. The effect of changing a value may range from trivial to catastrophic. If you run into a situation that you think can only be remedied by manual editing, you do better to contact the <A HREF="../people/people.html"><i>NEWSTAR </i> group</A> first.
+<P>
+<A NAME=.export><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004300000000000000>  <b>Export </b></A></H2>
+<P>
+ <UL><LI>   In UVFITS format (AIPS): <A HREF="../nscan_descr/nscan_descr.html">NSCAN UVFITS</A>  
+<LI>   Inspect a UVFITS file: <A HREF="../nscan_descr/nscan_descr.html">NSCAN PFITS</A>  
+ </UL>
+<P>
+<A NAME=.reorganise><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004400000000000000>  <b>Reorganising sectors </b></A></H2>
+<P>
+        You may want to reorganise the indexing of your sectors. This can be done to some extent through the <A HREF="../nscan_descr/nscan_descr.html">NSCAN REGROUP</A> function.
+<P>
+<A NAME=.delete><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004500000000000000>  <b>Deleting sectors </b></A></H2>
+<P>
+        The most important reason why one would want to delete sectors is to reclaim disk space. It would be fairly simple to provide a DELETE command that would make sectors invisible, but this would not free any space.
+<P>
+        An equivalent result can be achieved, however: Use  
+<A HREF="../ncopy_descr/ncopy_descr.html">NCOPY</A> to copy those sectors that you want to keep to a new .SCN file, then delete the old file.
+<P>
+.  
+<A NAME=.corrections><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000>  <b>Operation on corrections in a .SCN file</b></A></H1>
+<P>
+        Operations on corrections generally fall into either of two categories:  
+ <UL><LI>   Those that affect the gain/phase of individual dipole/interferometer  
+        hannels. This encompasses all corrections, except
+<P>
+<LI>   Those dealing with polarisation. These are 'special' in that they  
+        produce an effect of 'mixing' or 'crosstalk' between channels that would  
+        ideally be independent.  
+ </UL>
+<P>
+<A NAME=.gain.phase><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005100000000000000>  <b>Gain/phase corrections</b></A></H2>
+<P>
+ <UL><LI>   Zero, manual set: <A HREF="../ncalib_descr/ncalib_descr.html">NCALIB SET ZERO/MANUAL</A>  
+<LI>   Selfcal model fit: <A HREF="../ncalib_redun/ncalib_redun.html">NCALIB REDUN</A>  
+<LI>   Shift the reference value of telescope phases: <A HREF="../ncalib_redun/ncalib_redun.html">NCALIB           RENORM</A>  
+<LI>   Copy average corrections from one selection of scans to another one:  
+        <A HREF="../ncalib_descr/ncalib_descr.html">NCALIB SET COPY/CCOPY/LINE</A>  
+ </UL>
+<P>
+<A NAME=.polarisation><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005200000000000000>  <b>Polarisation corrections </b></A></H2>
+<P>
+Dipole errors:  
+ <UL><LI>   Zero, manual set: <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR ZERO/MANUAL</A>  
+<LI>   Estimation: <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR CALC</A>  
+<LI>   Copy average corrections from one selection of scans to another one:  
+        <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR COPY</A>  
+ </UL>   
+Phase-zero difference:  
+ <UL><LI>   Manual set: <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR VZERO MANUAL</A>  
+<LI>   Estimation: <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR VZERO CALC</A>  
+<LI>   Copy average corrections from one selection of scans to another one:  
+        <A HREF="../ncalib_polar/ncalib_polar.html">NCALIB POLAR VZERO COPY</A>  
+ </UL>
+<P>
+<A NAME=.apply><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0005300000000000000>  <b>Controlling the application of corrections </b></A></H2>
+<P>
+        Corrections are selectively applied to the visibilities whenever the data is read into memory to be processed. By default, all available corrections are selected. The user has the option to make his own selection. To this end, start your program with the /ASK switch:  
+ <DL COMPACT><DT>
+<DD>   dwe &lt;program&gt; /ASK
+<P>
+ </DL>  This will result in a long series of prompts. Simply type a &lt;CR&gt; to all, except those for the APPLY, DE_APPLY and FLAG parameters. More information can be found in the <A HREF="../introduction/introduction.html#.help">on-line help</A> texts.
+<P>
+        (We acknowledge that the appearance of many irrelevant prompts in this situation is unsatisfactory. We hope to correct this situation in the future.)
+<P>
+<A NAME=.model><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0006000000000000000>  <b>Operations on model visibilities </b></A></H1>
+<P>
+ <UL><LI>   Inserting/modifying the internal model: Use the <A HREF="../nmodel_handle/nmodel_handle.html">model           HANDLE</A> interface in NMODEL, NCALIB or NMAP.  
+<LI>   Deleting the indernal model: There is no operation to do this. See the  
+        <A HREF="../nmodel_handle/nmodel_handle.html">model HANDLE</A> document for a workaround.  
+ </UL>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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+%%For: jph@rzmws0 (johan hamaker)
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diff --git a/scnnode/scnnode__output_scn_node.html b/scnnode/scnnode__output_scn_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..7baae69b04cd36ad6c90e9072ad9bb972ec987aa
--- /dev/null
+++ b/scnnode/scnnode__output_scn_node.html
@@ -0,0 +1,18 @@
+<TITLE>Description of OUTPUT_SCN_NODE (SCNNODE)</TITLE>
+<H1>Description of general keyword OUTPUT_SCN_NODE</H1>
+
+<DT><EM>Prompt:</EM> Output .SCN file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the file name (no extension). <P>
+You may enter <P>
+	[&lt;directory&gt;/]** <P>
+to get a list of .SCN files in your current or another directory; then enter <P>
+	#&lt;n&gt; <P>
+to select the &lt;n&gt;'th file from that list. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnnode/scnnode_comm.html">List of general keywords</A> for SCNNODE
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnnode/scnnode__scn_node.html b/scnnode/scnnode__scn_node.html
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--- /dev/null
+++ b/scnnode/scnnode__scn_node.html
@@ -0,0 +1,34 @@
+<TITLE>Description of SCN_NODE (SCNNODE)</TITLE>
+<H1>Description of general keyword SCN_NODE</H1>
+
+<DT><EM>Prompt:</EM> .SCN file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+ Specify the file name (no extension). <P>
+You may enter <P>
+	[&lt;directory&gt;/]** <P>
+to get a list of .SCN files in your current or another directory; then enter <P>
+	#&lt;n&gt; <P>
+to select the &lt;n&gt;'th file from that list. 
+"! 
+!---------------------------------------------------------------------------- 
+!       Ref: 
+! 
+KEYWORD=INPUT_SCN_NODE 
+	DATA_TYP=C 
+	IO=I 
+	LENGTH=80 
+	SWITCHES=LOOP, NULL_VALUES, WILD_CARDS 
+	SEARCH=L, P 
+	PROMPT="Input .SCN file name  Specify the file name (no extension). <P>
+You may enter <P>
+	[&lt;directory&gt;/]** <P>
+to get a list of .SCN files in your current or another directory; then enter <P>
+	#&lt;n&gt; <P>
+to select the &lt;n&gt;'th file from that list. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnnode/scnnode_comm.html">List of general keywords</A> for SCNNODE
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnnode_comm/scnnode_comm.html b/scnnode_comm/scnnode_comm.html
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index 0000000000000000000000000000000000000000..f01325141eb961d926d2a268d04250caa125e90a
--- /dev/null
+++ b/scnnode_comm/scnnode_comm.html
@@ -0,0 +1,17 @@
+<TITLE>Index of general keywords from SCNNODE</TITLE>
+<H1>Description of general keywords (SCNNODE)</H1>
+
+<UL>
+<LI> <A HREF="../scnnode/scnnode__scn_node.html">
+  SCN_NODE</A>
+  .SCN file name
+<LI> <A HREF="../scnnode/scnnode__output_scn_node.html">
+  OUTPUT_SCN_NODE</A>
+  Output .SCN file name
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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+%%EOF
diff --git a/scnnode_public_intfc/images.pl b/scnnode_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/scnnode_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/scnnode_public_intfc/labels.pl b/scnnode_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..79858d4d47f6ed08d62dc709854c39962a101613
--- /dev/null
+++ b/scnnode_public_intfc/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".public"} ="$URL/scnnode_public_intfc.html"; 
+$external_labels{".input.scn.node"} ="$URL/scnnode_public_intfc.html"; 
+$external_labels{".output.scn.node"} ="$URL/scnnode_public_intfc.html"; 
+$external_labels{".scn.node"} ="$URL/scnnode_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/scnnode_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/scnnode_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/scnnode_public_intfc/scnnode_public_intfc.html b/scnnode_public_intfc/scnnode_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..1b049ce498e69e6b1aa9fad09be4aa5ffbf2e23b
--- /dev/null
+++ b/scnnode_public_intfc/scnnode_public_intfc.html
@@ -0,0 +1,158 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group SCNNODE</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=scnnode_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=scnnode_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=scnnode_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=scnnode_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=scnnode_public_intfc.html#SECTION0003200000000000000>  <b>Parameter INPUT_SCN_NODE</b></A>
+<LI> <A NAME=tex2html6 HREF=scnnode_public_intfc.html#SECTION0003300000000000000>  <b>Parameter OUTPUT_SCN_NODE</b></A>
+<LI> <A NAME=tex2html7 HREF=scnnode_public_intfc.html#SECTION0003400000000000000>  <b>Parameter SCN_NODE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group SCNNODE, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.input.scn.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter INPUT_SCN_NODE</b></A></H2>
+<P>
+  <em>Prompt:</em> Input .SCN file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+    <PRE>
+        Specify the file name (no extension).
+</PRE>
+<P>
+  <PRE>
+You may enter
+        [<directory>/]**
+</PRE>
+<P>
+  <PRE>
+to get a list of .SCN files in your current or another directory; then enter
+</PRE>
+<P>
+  <PRE>
+        #<n>
+</PRE>
+<P>
+  <PRE>
+to select the <n>'th file from that list.
+</PRE>
+<P>
+<A NAME=.output.scn.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter OUTPUT_SCN_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> Output .SCN file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the file name (no extension).
+</PRE>
+<P>
+  <PRE>
+You may enter
+        [<directory>/]**
+</PRE>
+<P>
+  <PRE>
+to get a list of .SCN files in your current or another directory; then enter
+</PRE>
+<P>
+  <PRE>
+        #<n>
+</PRE>
+<P>
+  <PRE>
+to select the <n>'th file from that list.
+</PRE>
+<P>
+<A NAME=.scn.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter SCN_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> .SCN file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+        Specify the file name (no extension).
+</PRE>
+<P>
+  <PRE>
+You may enter
+        [<directory>/]**
+</PRE>
+<P>
+  <PRE>
+to get a list of .SCN files in your current or another directory; then enter
+</PRE>
+<P>
+  <PRE>
+        #<n>
+</PRE>
+<P>
+  <PRE>
+to select the <n>'th file from that list.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/scnsets/scnsets__================.html b/scnsets/scnsets__================.html
new file mode 100644
index 0000000000000000000000000000000000000000..5860d2d0e9cd02fa1d0bf44162fbc8ae27e29cda
--- /dev/null
+++ b/scnsets/scnsets__================.html
@@ -0,0 +1,31 @@
+<TITLE>Description of ================ (SCNSETS)</TITLE>
+<H1>Description of general keyword ================</H1>
+
+<DT><EM>Prompt:</EM> OBS, ALTOBS, FLD, CHN, SCT Detail level for overview
+<DT><EM>Default:</EM> OBS.
+<DT><EM>Expected input:</EM> Character(10).<P>
+ Specify the level for the overview. <P>
+To get a quick overview of the entire file, use <P>
+	OBS     Shows a summary per observation (2nd index) listing the type of 
+		 observation, the fieldname, the sequence number ('Volgnummer'),  
+		 project number and UT date and time and the breakdown in 
+		 numbers of fields, channels and sectors and polarisations <P>
+To get more other details (frequency, bandwidth, HA range, number of scans and 
+number of interferometers),  use <P>
+	ALTOBS  for one line per observation 
+	FLD     for one line per field in all observations 
+	CHN     for one line per channel in all fields in all observations 
+	SCT     for one line per sector in all channels in all fields in all 
+		 observations <P>
+NOTE: Depending on what is in your file, the volume of output in the latter 
+three modes may be quite large. If you are not interested in the difference 
+(e.g. in hour angle) between sectors, do not use SCT; if you are not interested 
+in the differences (e.g. in frequency) between channels, do not use CHN. <P>
+There is presently no mechanism to select only specific groups or observations 
+for display. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__polarisation and.html b/scnsets/scnsets__polarisation and.html
new file mode 100644
index 0000000000000000000000000000000000000000..6afde861b58a5c58e7560e0c2c5aac7a650349b3
--- /dev/null
+++ b/scnsets/scnsets__polarisation and.html	
@@ -0,0 +1,64 @@
+<TITLE>Description of polarisation and (SCNSETS)</TITLE>
+<H1>Description of general keyword polarisation and</H1>
+
+<DT><EM>Prompt:</EM> Loop specifications: |-
+nr of cycles, index increment (grp.obs.fld.chn.seq) per cycle |
+<DT><EM>Default:</EM> "" /ASK.
+<DT><EM>Expected input:</EM> Character(32), 16 values.<P>
+ Quick reminders: =============== 
+
+<DT>   - L gives you a quick summary of the groups in your .SCN file 
+
+<DT>   - O gives you access to more detailed overviews in various levels of detail 
+
+<DT>   - #&lt;n&gt; is a synonym for the grp.obs.fld.chn.seq index that is sometimes 
+	convenient to use. # ('absolute') sector numbers are shown in most 
+	displays that show sector indices. 
+
+<DT>   - A loop is specified by the number of cycles and the index increment per 
+	cycle. Loops may be nested. <P>
+The loop concept in full: ======================== 
+	A loop specifies repeated execution of your operation. It is defined by 
+the number of cycles and the increment per cycle for the sector indices: <P>
+	&lt;n_cycle&gt;, &lt;grp_incr&gt;.&lt;obs_incr&gt;.&lt;fld_incr&gt;.&lt;chn_incr&gt;.&lt;seq_incr&gt; <P>
+Later you will define, through the SCN_SETS parameter, the sector set to be 
+processed in the first cycle. 
+   Example: 
+	SCN_LOOPS= 3, 0.0.2.1.0 
+	SCN_SETS= 2.*.0-2.3.0, 2.*.1. 
+   requests your operation to be executed three times, with sector sets 
+	2.*.0-2.3.0     (SCN_SETS value) 
+	2.*.2-4.4.0     (SCN_SETS + 1*increment) 
+	2.*.4-6.5.0     (SCN_SETS + 2*increment) <P>
+In the increment value, 0s and trailing dots may be omitted. Negative 
+increments are permitted. <P>
+Loops may be nested by giving more than one cycles-increment pair; in this case 
+the rightmost loop is executed inside the loop to its left. 
+   Example: 
+	SCN_LOOPS= 2, .1, 2, ..1 
+	SCN_SETS= 0.0.0.*.0 
+   results in your operation being performed on the following sequence of 
+   sectors: 
+	0.0.0.*.0 
+	0.0.1.*.0 
+	0.1.0.*.0 
+	0.1.1.*.0 <P>
+Some fine points: ================ 
+	Loops are a useful shorthand for specifying complicated repetitions of 
+the same operation on different sector sets. As the examples above demonstrate,  
+using SCN_LOOPS can save a lot of typing, in particular if the number of cycles 
+is large. <P>
+	Note that each cycle of a loop starts the requested operation anew. To 
+understand what this means, consider two ways to process all fields of a 
+16-field mosaic observation: <P>
+	SCN_LOOPS=&lt;no input&gt;                    SCN_LOOPS=16, ..1 
+	SCN_SETS=grp.obs.*                      SCN_SETS=grp.obs.0 <P>
+The left specification requests a single pass thorugh the operation using all 
+fields as input. The right specification requests 16 passes successively using 
+fields 0, 1, 2, ... as input. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__scn_channels.html b/scnsets/scnsets__scn_channels.html
new file mode 100644
index 0000000000000000000000000000000000000000..d84e5b89a4de73d672636cc851e5ca022a0a8e1b
--- /dev/null
+++ b/scnsets/scnsets__scn_channels.html
@@ -0,0 +1,28 @@
+<TITLE>Description of SCN_CHANNELS (SCNSETS)</TITLE>
+<H1>Description of general keyword SCN_CHANNELS</H1>
+
+<DT><EM>Prompt:</EM>  4th index: channels
+<DT><EM>Expected input:</EM> Character(32).<P>
+ Give the 'channel' index-range (chn) of a sector-Set 
+specification 
+							(grp.obs.fld.chn.seq). <P>
+The standard use of multiple channels in a .SCN file field is for the different 
+frequency channels or bands in an observation. Note that the index for the 
+first channel is 1; channel 0 is by definition the 'continuum' channel, i.e. 
+the sum of all the observed 'line' channels. <P>
+Possible answers ([]=optional): <P>
+	0               take the continuum channel 
+	n1              take channel nr n1 (n1=0, 1, 2, 3, ....) 
+	n1-n2[:n3]      loop over channels n1 through n2 [step n3] 
+	*               loop over all channels for the field (wildcard) 
+	n1-[*]          loop over all channels for the field,  
+			 starting with n1 [step n3] <P>
+NB: The associated SCN_LOOPS keyword allows even more looping over index 
+values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__scn_fields.html b/scnsets/scnsets__scn_fields.html
new file mode 100644
index 0000000000000000000000000000000000000000..2fbfb2d9ddf3da432e23625662bb4ac4c19b9a75
--- /dev/null
+++ b/scnsets/scnsets__scn_fields.html
@@ -0,0 +1,25 @@
+<TITLE>Description of SCN_FIELDS (SCNSETS)</TITLE>
+<H1>Description of general keyword SCN_FIELDS</H1>
+
+<DT><EM>Prompt:</EM>  3rd index: fields
+<DT><EM>Expected input:</EM> Character(32).<P>
+ Give the 'field' index-range (fld) of a sector-Set specification 
+							(grp.obs.fld.chn.seq) <P>
+The standard use of multiple fields in a .SCN file observation is for the 
+different pointing centres (fields) in a mosaic observation. <P>
+Possible answers ([]=optional): <P>
+	0               take first (or only) field 
+	n1              take field nr n1 (n1=0, 1, 2, 3, ....) 
+	n1-n2[:n3]      loop over fields n1 through n2 [step n3] 
+	*               loop over all fields in the observation (wildcard) 
+	n1-[*][:n3]     loop over all fields in the observation,  
+			 starting with n1 [step n3] <P>
+NB: The associated SCN_LOOPS keyword allows even more looping over index 
+values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__scn_groups.html b/scnsets/scnsets__scn_groups.html
new file mode 100644
index 0000000000000000000000000000000000000000..7ff65b5eaaac6f94ebfadfba51c6bf36e24085ac
--- /dev/null
+++ b/scnsets/scnsets__scn_groups.html
@@ -0,0 +1,25 @@
+<TITLE>Description of SCN_GROUPS (SCNSETS)</TITLE>
+<H1>Description of general keyword SCN_GROUPS</H1>
+
+<DT><EM>Prompt:</EM>  1st index: grp = groups
+<DT><EM>Expected input:</EM> Character(32).<P>
+ Give the 'group' index-range (grp) of a sector-set specification 
+							(grp.obs.fld.chn.seq) <P>
+An example of multiple groups in a .SCN file is one group for an observation 
+and another one for the associated calibrator observation(2). <P>
+Possible answers ([]=optional): <P>
+	0               take first (or only) group 
+	n1              take group nr n1 (n1=0, 1, 2, 3, ....) 
+	n1-n2[:n3]      loop over groups n1 through n2 [step n3] 
+	*               loop over all available groups (wildcard) 
+	n1-[*][:n3]     loop over all available groups,  
+			 starting with n1 [step n3] <P>
+NB: The associated SCN_LOOPS keyword allows even more looping over index 
+values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__scn_obss.html b/scnsets/scnsets__scn_obss.html
new file mode 100644
index 0000000000000000000000000000000000000000..04ac856d3f2d7e6374407fc9ccec597cf7f6f500
--- /dev/null
+++ b/scnsets/scnsets__scn_obss.html
@@ -0,0 +1,27 @@
+<TITLE>Description of SCN_OBSS (SCNSETS)</TITLE>
+<H1>Description of general keyword SCN_OBSS</H1>
+
+<DT><EM>Prompt:</EM>  2nd index: observations
+<DT><EM>Expected input:</EM> Character(32).<P>
+ Give the 'observation' index-range (obs) of a sector-Set 
+specification 
+							(grp.obs.fld.chn.seq) <P>
+Example of multiple observations in one ..SCN file group are: 
+	the parts of an interrupted 12h observation; 
+	observations of the same object, with different array configurations. <P>
+Possible answers ([]=optional): <P>
+	0               take first (or only) observation 
+	n1              take group nr n1 (n1=0, 1, 2, 3, ....) 
+	n1-n2[:n3]      loop over groups n1 through n2 [step n3] 
+	*               loop over all available observations (wildcard) 
+	n1-[*][:n3]     loop over all available observations,  
+			 starting with n1 [step n3] <P>
+NB: The associated SCN_LOOPS keyword allows even more looping over index 
+values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__scn_sectors.html b/scnsets/scnsets__scn_sectors.html
new file mode 100644
index 0000000000000000000000000000000000000000..7d1365eab790f1f6401f45d213a121938600d2ca
--- /dev/null
+++ b/scnsets/scnsets__scn_sectors.html
@@ -0,0 +1,31 @@
+<TITLE>Description of SCN_SECTORS (SCNSETS)</TITLE>
+<H1>Description of general keyword SCN_SECTORS</H1>
+
+<DT><EM>Prompt:</EM>  5th index: sectors
+<DT><EM>Expected input:</EM> Character(32).<P>
+ Give the 'sequence number' index-range (seq) of a sector-Set 
+specification 
+							(grp.obs.fld.chn.seq). <P>
+A standard use of multiple sectors for one .SCN file field and one frequency is 
+for the different hour-angle 'slices' in a mosaic observation. <P>
+Possible answers ([]=optional): <P>
+	0               take the first sector 
+	n1              take sector nr n1 (n1=0, 1, 2, 3, ....) 
+	n1-n2[:n3]      loop over sectors n1 through n2 [step n3] 
+	*               loop over all 
+			 (wildcard) 
+	n1-[*]          loop over all sectors for the field and channel,  
+			 starting with n1 [step n3] <P>
+NOTES: 
+	In a mosaic observation, the HOUR_ANGLE range parameter can be used to 
+select sectors. This is simpler but cruder: The same range applies to all 
+SCN_SETS and SCN_LOOPS specified. <P>
+	The associated SCN_LOOPS keyword allows even more looping over index 
+values. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets/scnsets__scn_sets.html b/scnsets/scnsets__scn_sets.html
new file mode 100644
index 0000000000000000000000000000000000000000..fe0404417758d79db458cf8bcb0e8bdff5bd7489
--- /dev/null
+++ b/scnsets/scnsets__scn_sets.html
@@ -0,0 +1,70 @@
+<TITLE>Description of SCN_SETS (SCNSETS)</TITLE>
+<H1>Description of general keyword SCN_SETS</H1>
+
+<DT><EM>Prompt:</EM> Sectors to process:  grp.obs.fld.chn.seq 
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+ Quick reminders: =============== 
+
+<DT>   - L gives you a quick summary of the groups in your .SCN file 
+
+<DT>   - O gives you access to more detailed overviews in various levels of detail 
+
+<DT>   - #&lt;n&gt; is a synonym for the grp.obs.fld.chn.seq index that is sometimes 
+	convenient to use. # ('absolute') sector numbers are shown in most 
+	displays that show sector indices. 
+
+<DT>   - @ or &gt; will prompt you for each of the 5 indices separately. Use this 
+	option if you are not yet comfortable with the sector-indexing system. 
+
+<DT>   - If you have requested looping (SCN_LOOPS parameter), the sectors you 
+	specify will be processed in the first loop cycle, and the indices 
+	incremented for each following cycle. 
+
+<DT>   - If you have second thoughts about looping, reply # or ctrl-D to backtrack. <P>
+Sector selection: ================ 
+	You may select SETS of sectors for processing by [ranges of] values for 
+the five indices. A range has the form &lt;start&gt;-[&lt;end&gt;][:&lt;step&gt;]. A wildcard '*' 
+means 'all'; *s and trailing dots may be omitted. 
+   Example 
+		. 3-7:2 . 4-:2 . 1-7 (blanks inserted for clarity only) 
+   meaning 
+	all grp (missing grp index is replaced by a '*') 
+	for each grp: obs=3 to 7 in steps of 2 (i.e. 3, 5 and 7) 
+	for each obs: all even fld starting at 4 
+	for each fld: chn=1 to 7; 
+	for each chn: all seq (omitted trailing seq index replaced by a '*') <P>
+ 
+Multiple SETS may be specified, separated by comma's: &lt;Set1&gt;, &lt;Set2&gt;, ... The 
+associated SCN_LOOPS keyword allows even more looping over index values. <P>
+Other keywords allow the user to select hour-angle range, polarisation and 
+interferometers within each SECTOR. <P>
+Explanation of sector indices: ============================= 
+	A .SCN file contains visibilities and associated data for one or more 
+objects. The basic unit of data is the SECTOR, which is a collection of SCANS 
+contiguous in hour angle for one sky position and one frequency. Sectors are 
+addressed through a SECTOR INDEX which is a string of five integers separated 
+by dots: 
+			grp.obs.fld.chn.seq <P>
+   The GROUP (grp) and OBSERVATION (obs) are basically administrative units for 
+    organising the data, e.g. per object. grp and obs number alocations have 
+    been determined by NSCAN when you read the data in. <P>
+   Mosaic observations contain multiple FIELDs (fld), numbered from 0 to n-1 in 
+    the sequence in which they were observed at the WSRT. A non-mosaic 
+    observation contains only field 0. <P>
+   Line and broadband continuum observations generally have several frequency 
+    CHANNELS (chn), also known as 'bands'. The channles are numbered from 1 to 
+    N. Channel 0 is by definition the 'continuum' channel, i.e. the sum of all 
+    'line' channels. <P>
+   In mosaic observations, the sector SEQUENCE (seq) number distinguishes the 
+    successive hour-angle 'sectors'. Other situations are conceivable where 
+    multiple sectors with the same grp.obs.fld.chn exist; it is then your 
+    responsibility to know what they represent. <P>
+Index values start at zero. (Remember that for the CHN index this is the 
+continuum channel.) <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../scnsets/scnsets_comm.html">List of general keywords</A> for SCNSETS
+<LI>Description of the <A HREF="../scn_descr/scn_descr.html">SCN file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/scnsets_comm/scnsets_comm.html b/scnsets_comm/scnsets_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..2b0d00c15bfab163d8243abc1e7f1837a65d1547
--- /dev/null
+++ b/scnsets_comm/scnsets_comm.html
@@ -0,0 +1,36 @@
+<TITLE>Index of general keywords from SCNSETS</TITLE>
+<H1>Description of general keywords (SCNSETS)</H1>
+
+<UL>
+<LI> <A HREF="../scnsets/scnsets__scn_sets.html">
+  SCN_SETS</A>
+  Sectors to process:  grp.obs.fld.chn.seq 
+<LI> <A HREF="../scnsets/scnsets__m of all.html">
+  m of all</A>
+  Loop specifications: |-
+nr of cycles, index increment (grp.obs.fld.chn.seq) per cycle |
+<LI> <A HREF="../scnsets/scnsets__overview.html">
+  OVERVIEW</A>
+  OBS, ALTOBS, FLD, CHN, SCT Detail level for overview
+<LI> <A HREF="../scnsets/scnsets__scn_groups.html">
+  SCN_GROUPS</A>
+   1st index: grp = groups
+<LI> <A HREF="../scnsets/scnsets__scn_obss.html">
+  SCN_OBSS</A>
+   2nd index: observations
+<LI> <A HREF="../scnsets/scnsets__scn_fields.html">
+  SCN_FIELDS</A>
+   3rd index: fields
+<LI> <A HREF="../scnsets/scnsets__scn_channels.html">
+  SCN_CHANNELS</A>
+   4th index: channels
+<LI> <A HREF="../scnsets/scnsets__scn_sectors.html">
+  SCN_SECTORS</A>
+   5th index: sectors
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group SCNSETS</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=scnsets_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=scnsets_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=scnsets_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=scnsets_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=scnsets_public_intfc.html#SECTION0003200000000000000>  <b>Parameter OVERVIEW</b></A>
+<LI> <A NAME=tex2html6 HREF=scnsets_public_intfc.html#SECTION0003300000000000000>  <b>Parameter SCN_CHANNELS</b></A>
+<LI> <A NAME=tex2html7 HREF=scnsets_public_intfc.html#SECTION0003400000000000000>  <b>Parameter SCN_FIELDS</b></A>
+<LI> <A NAME=tex2html8 HREF=scnsets_public_intfc.html#SECTION0003500000000000000>  <b>Parameter SCN_GROUPS</b></A>
+<LI> <A NAME=tex2html9 HREF=scnsets_public_intfc.html#SECTION0003600000000000000>  <b>Parameter SCN_LOOPS</b></A>
+<LI> <A NAME=tex2html10 HREF=scnsets_public_intfc.html#SECTION0003700000000000000>  <b>Parameter SCN_OBSS</b></A>
+<LI> <A NAME=tex2html11 HREF=scnsets_public_intfc.html#SECTION0003800000000000000>  <b>Parameter SCN_SECTORS</b></A>
+<LI> <A NAME=tex2html12 HREF=scnsets_public_intfc.html#SECTION0003900000000000000>  <b>Parameter SCN_SETS</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group SCNSETS, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.overview><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter OVERVIEW</b></A></H2>
+<P>
+  <em>Prompt:</em> Detail level for overview (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *10:  1 value
+<P>
+    <PRE>
+        Specify the level for the overview.
+</PRE>
+<P>
+  <PRE>
+To get a quick overview of the entire file, use
+</PRE>
+<P>
+  <PRE>
+        OBS     Shows a summary per observation (2nd index) listing the type of
+                 observation, the fieldname, the sequence number ('Volgnummer'),
+                 project number and UT date and time and the breakdown in
+                 numbers of fields, channels and sectors and polarisations
+</PRE>
+<P>
+  <PRE>
+To get more other details (frequency, bandwidth, HA range, number of scans and
+number of interferometers),  use
+</PRE>
+<P>
+  <PRE>
+        ALTOBS  for one line per observation
+        FLD     for one line per field in all observations
+        CHN     for one line per channel in all fields in all observations
+        SCT     for one line per sector in all channels in all fields in all
+                 observations
+</PRE>
+<P>
+  <PRE>
+NOTE: Depending on what is in your file, the volume of output in the latter
+three modes may be quite large. If you are not interested in the difference
+(e.g. in hour angle) between sectors, do not use SCT; if you are not interested
+in the differences (e.g. in frequency) between channels, do not use CHN.
+</PRE>
+<P>
+  <PRE>
+There is presently no mechanism to select only specific groups or observations
+for display.
+</PRE>
+<P>
+<A NAME=.scn.channels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter SCN_CHANNELS</b></A></H2>
+<P>
+<em>Prompt:</em>  4th index: channels (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the 'channel' index-range (chn) of a sector-Set
+specification
+                                                        (grp.obs.fld.chn.seq).
+</PRE>
+<P>
+  <PRE>
+The standard use of multiple channels in a .SCN file field is for the different
+frequency channels or bands in an observation. Note that the index for the
+first channel is 1; channel 0 is by definition the 'continuum' channel, i.e.
+the sum of all the observed 'line' channels.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take the continuum channel
+        n1              take channel nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over channels n1 through n2 [step n3]
+        *               loop over all channels for the field (wildcard)
+        n1-[*]          loop over all channels for the field,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+NB: The associated SCN_LOOPS keyword allows even more looping over index
+values.
+</PRE>
+<P>
+<A NAME=.scn.fields><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter SCN_FIELDS</b></A></H2>
+<P>
+<em>Prompt:</em>  3rd index: fields (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the 'field' index-range (fld) of a sector-Set specification
+                                                        (grp.obs.fld.chn.seq)
+</PRE>
+<P>
+  <PRE>
+The standard use of multiple fields in a .SCN file observation is for the
+different pointing centres (fields) in a mosaic observation.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) field
+        n1              take field nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over fields n1 through n2 [step n3]
+        *               loop over all fields in the observation (wildcard)
+        n1-[*][:n3]     loop over all fields in the observation,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+NB: The associated SCN_LOOPS keyword allows even more looping over index
+values.
+</PRE>
+<P>
+<A NAME=.scn.groups><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter SCN_GROUPS</b></A></H2>
+<P>
+<em>Prompt:</em>  1st index: grp  (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the 'group' index-range (grp) of a sector-set specification
+                                                        (grp.obs.fld.chn.seq)
+</PRE>
+<P>
+  <PRE>
+An example of multiple groups in a .SCN file is one group for an observation
+and another one for the associated calibrator observation(2).
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) group
+        n1              take group nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over groups n1 through n2 [step n3]
+        *               loop over all available groups (wildcard)
+        n1-[*][:n3]     loop over all available groups,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+NB: The associated SCN_LOOPS keyword allows even more looping over index
+values.
+</PRE>
+<P>
+<A NAME=.scn.loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter SCN_LOOPS</b></A></H2>
+<P>
+<em>Prompt:</em> Loop specifications: |- (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 to 16 values
+<P>
+  <PRE>
+        Quick reminders: ===============
+   - L gives you a quick summary of the groups in your .SCN file
+   - O gives you access to more detailed overviews in various levels of detail
+   - #<n> is a synonym for the grp.obs.fld.chn.seq index that is sometimes
+        convenient to use. # ('absolute') sector numbers are shown in most
+        displays that show sector indices.
+   - A loop is specified by the number of cycles and the index increment per
+        cycle. Loops may be nested.
+</PRE>
+<P>
+  <PRE>
+The loop concept in full: ========================
+        A loop specifies repeated execution of your operation. It is defined by
+the number of cycles and the increment per cycle for the sector indices:
+</PRE>
+<P>
+  <PRE>
+        <n_cycle>, <grp_incr>.<obs_incr>.<fld_incr>.<chn_incr>.<seq_incr>
+</PRE>
+<P>
+  <PRE>
+Later you will define, through the SCN_SETS parameter, the sector set to be
+processed in the first cycle.
+   Example:
+        SCN_LOOPS= 3, 0.0.2.1.0
+        SCN_SETS= 2.*.0-2.3.0, 2.*.1.
+   requests your operation to be executed three times, with sector sets
+        2.*.0-2.3.0     (SCN_SETS value)
+        2.*.2-4.4.0     (SCN_SETS + 1*increment)
+        2.*.4-6.5.0     (SCN_SETS + 2*increment)
+</PRE>
+<P>
+  <PRE>
+In the increment value, 0s and trailing dots may be omitted. Negative
+increments are permitted.
+</PRE>
+<P>
+  <PRE>
+Loops may be nested by giving more than one cycles-increment pair; in this case
+the rightmost loop is executed inside the loop to its left.
+   Example:
+        SCN_LOOPS= 2,.1, 2,..1
+        SCN_SETS= 0.0.0.*.0
+   results in your operation being performed on the following sequence of
+   sectors:
+        0.0.0.*.0
+        0.0.1.*.0
+        0.1.0.*.0
+        0.1.1.*.0
+</PRE>
+<P>
+  <PRE>
+Some fine points: ================
+        Loops are a useful shorthand for specifying complicated repetitions of
+the same operation on different sector sets. As the examples above demonstrate,
+using SCN_LOOPS can save a lot of typing, in particular if the number of cycles
+is large.
+        Note that each cycle of a loop starts the requested operation anew. To
+understand what this means, consider two ways to process all fields of a
+16-field mosaic observation:
+        SCN_LOOPS=<no input>                    SCN_LOOPS=16,..1
+        SCN_SETS=grp.obs.*                      SCN_SETS=grp.obs.0
+The left specification requests a single pass thorugh the operation using all
+fields as input. The right specification requests 16 passes successively using
+fields 0,1,2,... as input.
+</PRE>
+<P>
+<A NAME=.scn.obss><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter SCN_OBSS</b></A></H2>
+<P>
+<em>Prompt:</em>  2nd index: observations (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the 'observation' index-range (obs) of a sector-Set
+specification
+                                                        (grp.obs.fld.chn.seq)
+</PRE>
+<P>
+  <PRE>
+Example of multiple observations in one ..SCN file group are:
+        the parts of an interrupted 12h observation;
+        observations of the same object, with different array configurations.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) observation
+        n1              take group nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over groups n1 through n2 [step n3]
+        *               loop over all available observations (wildcard)
+        n1-[*][:n3]     loop over all available observations,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+NB: The associated SCN_LOOPS keyword allows even more looping over index
+values.
+</PRE>
+<P>
+<A NAME=.scn.sectors><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter SCN_SECTORS</b></A></H2>
+<P>
+<em>Prompt:</em>  5th index: sectors (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+        Give the 'sequence number' index-range (seq) of a sector-Set
+specification
+                                                        (grp.obs.fld.chn.seq).
+</PRE>
+<P>
+  <PRE>
+A standard use of multiple sectors for one .SCN file field and one frequency is
+for the different hour-angle 'slices' in a mosaic observation.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take the first sector
+        n1              take sector nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over sectors n1 through n2 [step n3]
+        *               loop over all
+                         (wildcard)
+        n1-[*]          loop over all sectors for the field and channel,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+NOTES:
+        In a mosaic observation, the HOUR_ANGLE range parameter can be used to
+select sectors. This is simpler but cruder: The same range applies to all
+SCN_SETS and SCN_LOOPS specified.
+</PRE>
+<P>
+  <PRE>
+        The associated SCN_LOOPS keyword allows even more looping over index
+values.
+</PRE>
+<P>
+<A NAME=.scn.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter SCN_SETS</b></A></H2>
+<P>
+<em>Prompt:</em> Sectors to process:  grp.obs.fld.chn.seq (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+        Quick reminders: ===============
+   - L gives you a quick summary of the groups in your .SCN file
+   - O gives you access to more detailed overviews in various levels of detail
+   - #<n> is a synonym for the grp.obs.fld.chn.seq index that is sometimes
+        convenient to use. # ('absolute') sector numbers are shown in most
+        displays that show sector indices.
+   -  or > will prompt you for each of the 5 indices separately. use this
+        option if you are not yet comfortable with the sector-indexing system.
+   - If you have requested looping (SCN_LOOPS parameter), the sectors you
+        specify will be processed in the first loop cycle, and the indices
+        incremented for each following cycle.
+   - If you have second thoughts about looping, reply # or ctrl-D to backtrack.
+</PRE>
+<P>
+  <PRE>
+Sector selection: ================
+        You may select SETS of sectors for processing by [ranges of] values for
+the five indices. A range has the form <start>-[<end>][:<step>]. A wildcard '*'
+means 'all'; *s and trailing dots may be omitted.
+   Example
+                . 3-7:2 . 4-:2 . 1-7 (blanks inserted for clarity only)
+   meaning
+        all grp (missing grp index is replaced by a '*')
+        for each grp: obs=3 to 7 in steps of 2 (i.e. 3, 5 and 7)
+        for each obs: all even fld starting at 4
+        for each fld: chn=1 to 7;
+        for each chn: all seq (omitted trailing seq index replaced by a '*')
+</PRE>
+<P>
+  <PRE>
+Multiple SETS may be specified, separated by comma's: <Set1>,<Set2>,... The
+associated SCN_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+  <PRE>
+Other keywords allow the user to select hour-angle range, polarisation and
+interferometers within each SECTOR.
+</PRE>
+<P>
+  <PRE>
+Explanation of sector indices: =============================
+        A .SCN file contains visibilities and associated data for one or more
+objects. The basic unit of data is the SECTOR, which is a collection of SCANS
+contiguous in hour angle for one sky position and one frequency. Sectors are
+addressed through a SECTOR INDEX which is a string of five integers separated
+by dots:
+                        grp.obs.fld.chn.seq
+</PRE>
+<P>
+  <PRE>
+   The GROUP (grp) and OBSERVATION (obs) are basically administrative units for
+    organising the data, e.g. per object. grp and obs number alocations have
+    been determined by NSCAN when you read the data in.
+</PRE>
+<P>
+  <PRE>
+   Mosaic observations contain multiple FIELDs (fld), numbered from 0 to n-1 in
+    the sequence in which they were observed at the WSRT. A non-mosaic
+    observation contains only field 0.
+</PRE>
+<P>
+  <PRE>
+   Line and broadband continuum observations generally have several frequency
+    CHANNELS (chn), also known as 'bands'. The channles are numbered from 1 to
+    N. Channel 0 is by definition the 'continuum' channel, i.e. the sum of all
+    'line' channels.
+</PRE>
+<P>
+  <PRE>
+   In mosaic observations, the sector SEQUENCE (seq) number distinguishes the
+    successive hour-angle 'sectors'. Other situations are conceivable where
+    multiple sectors with the same grp.obs.fld.chn exist; it is then your
+    responsibility to know what they represent.
+</PRE>
+<P>
+  <PRE>
+Index values start at zero. (Remember that for the CHN index this is the
+continuum channel.)
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/select/select__..html b/select/select__..html
new file mode 100644
index 0000000000000000000000000000000000000000..ea30248b43d906c54e639a1306f13cc3ed1d510b
--- /dev/null
+++ b/select/select__..html
@@ -0,0 +1,31 @@
+<TITLE>Description of . (SELECT)</TITLE>
+<H1>Description of general keyword .</H1>
+
+<DT><EM>Prompt:</EM> Changes to the telescope selection|
+<DT><EM>Expected input:</EM> Character(4), 20 values.<P>
+ Specify how you want to change the telescope selection. <P>
+The following codes are used to identify (groups of) telescopes: <P>
+	P       show the present selection table <P>
+   For the WSRT: 
+	0, 1, 2, 3, 4, 5, 6, 7, 8, 9, A, B, C, D: 
+		individual WSRT telescopes (case-insensitive) 
+	*       all telesopes 
+	F       all fixed telescopes = 0 through 9 
+	M       all movable telescopes = A through D 
+	Y       telescopes A and B 
+	Z       telescopes C and D <P>
+   Additional codes for the Australian Telecope Compact Array (ATCA): 
+	T       ATCA telescopes (8-D) 
+	U       the ATCA complement (0-7). <P>
+A telesope specification without a prefix or prefixed with a + sign is 
+SELECTED, a specification with a minus sign prefixed is ELIMINATED. Selection 
+and elimination are incremental. Up to 20 select/eliminate specifications may 
+be given, separated by comma's; they will be honored in the order in which you 
+give them. Prompting will continue until you stop replying. <P>
+Examples: -*, 3, +3, -8, *, -F, -U, T <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../select/select_comm.html">List of general keywords</A> for SELECT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/select/select__ha_range.html b/select/select__ha_range.html
new file mode 100644
index 0000000000000000000000000000000000000000..4d653bfe5ffd2a2edc793387692b5df4d85c6625
--- /dev/null
+++ b/select/select__ha_range.html
@@ -0,0 +1,12 @@
+<TITLE>Description of HA_RANGE (SELECT)</TITLE>
+<H1>Description of general keyword HA_RANGE</H1>
+
+<DT><EM>Prompt:</EM> HA range
+<DT><EM>Expected input:</EM> Real number in DEG, RAD, CIR, HMS, 2 values; min.value: -180.000000; max.value: 180.000000.<P>
+ Specify the hour-angle range to be selected <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../select/select_comm.html">List of general keywords</A> for SELECT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/select/select__select_ifrs.html b/select/select__select_ifrs.html
new file mode 100644
index 0000000000000000000000000000000000000000..3cb4550834646776f132be5c6fbd8e12e7680cb4
--- /dev/null
+++ b/select/select__select_ifrs.html
@@ -0,0 +1,46 @@
+<TITLE>Description of SELECT_IFRS (SELECT)</TITLE>
+<H1>Description of general keyword SELECT_IFRS</H1>
+
+<DT><EM>Prompt:</EM> Changes to the interferometer selection|
+<DT><EM>Expected input:</EM> Character(4), 40 values.<P>
+ Specify how you want to change the interferometer selection. <P>
+Interferometers are defined as combinations of two telescopes; an 
+interferometer may thus contain 1, 2 or 4 polarisations. <P>
+A combination of two different telescopes is called a CROSS[-correlating] 
+interferometer, a telescope combined with itself an AUTO[-correlating] 
+interferometer. At present, WSRT data contain only cross-interferometer data,  
+so selection/elimination of auto-interferometers is irrelevant. <P>
+The following codes are used to identify (groups of) telescopes: <P>
+	P       show the present selection table <P>
+   For the WSRT: 
+	0, 1, 2, 3, 4, 5, 6, 7, 8, 9, A, B, C, D: 
+		 individual WSRT telescopes (case-insensitive) 
+	*       all telescopes or all cross interferometers 
+	F       all fixed telescopes = 0 through 9 
+	M       all movable telescopes = A through D 
+	Y       telescopes A and B 
+	Z       telescopes C and D 
+	#       autocorrelation <P>
+   Additional codes for the Australian Telecope Compact Array (ATCA): 
+	T       ATCA telescopes (8-D) 
+	U       the ATCA complement (0-7). <P>
+An interferometer specification without a prefix or prefixed with a + sign is 
+SELECTED, a specification with a minus sign prefixed is ELIMINATED. Selection 
+and elimination are incremental. Up to 40 select/eliminate specifications may 
+be given, separated by comma's; they will be honored in the order in which you 
+give them. Prompting will continue until you stop replying. <P>
+The standard operation is on the cross-correlations. A telescope name followed 
+with a # indicates the auto-correlations. <P>
+Examples: 
+
+<DT>	-3F     eliminate combinations of 3 with other fixed telescopes 
+	FM, -9A  select all fixed-movable combinations (the WSRT's 40 'standard' 
+		 interferometers) except 9A 
+
+<DT>	-#, 33   eliminate all auto-interferometers, then re-select 33 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../select/select_comm.html">List of general keywords</A> for SELECT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/select/select__select_tels.html b/select/select__select_tels.html
new file mode 100644
index 0000000000000000000000000000000000000000..c6b4495ba6301a8ecf40eba322ae13332f924327
--- /dev/null
+++ b/select/select__select_tels.html
@@ -0,0 +1,31 @@
+<TITLE>Description of SELECT_TELS (SELECT)</TITLE>
+<H1>Description of general keyword SELECT_TELS</H1>
+
+<DT><EM>Prompt:</EM> Changes to the telescope selection|
+<DT><EM>Expected input:</EM> Character(4), 20 values.<P>
+ Specify how you want to change the telescope selection. <P>
+The following codes are used to identify (groups of) telescopes: <P>
+	P       show the present selection table <P>
+   For the WSRT: 
+	0, 1, 2, 3, 4, 5, 6, 7, 8, 9, A, B, C, D: 
+		individual WSRT telescopes (case-insensitive) 
+	*       all telesopes 
+	F       all fixed telescopes = 0 through 9 
+	M       all movable telescopes = A through D 
+	Y       telescopes A and B 
+	Z       telescopes C and D <P>
+   Additional codes for the Australian Telecope Compact Array (ATCA): 
+	T       ATCA telescopes (8-D) 
+	U       the ATCA complement (0-7). <P>
+A telesope specification without a prefix or prefixed with a + sign is 
+SELECTED, a specification with a minus sign prefixed is ELIMINATED. Selection 
+and elimination are incremental. Up to 20 select/eliminate specifications may 
+be given, separated by comma's; they will be honored in the order in which you 
+give them. Prompting will continue until you stop replying. <P>
+Examples: -*, 3, +3, -8, *, -F, -U, T <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../select/select_comm.html">List of general keywords</A> for SELECT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/select/select__select_xyx.html b/select/select__select_xyx.html
new file mode 100644
index 0000000000000000000000000000000000000000..5b0b64a315e2be5f0683951a63d9998a71f51f23
--- /dev/null
+++ b/select/select__select_xyx.html
@@ -0,0 +1,19 @@
+<TITLE>Description of SELECT_XYX (SELECT)</TITLE>
+<H1>Description of general keyword SELECT_XYX</H1>
+
+<DT><EM>Prompt:</EM> XYX, XY, Y, X, YX, YYX, XXY polarisations
+<DT><EM>Expected input:</EM> Character(4).<P>
+ Select the polarisation(s) to be used: <P>
+	XYX     all four combinations (XX, YX, YX, YY) 
+	XY      XX and YY 
+	X       XX only 
+	Y       YY only 
+	YX      XY and YX 
+	YYX     YX 
+	XXY     XY <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../select/select_comm.html">List of general keywords</A> for SELECT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/select_comm/select_comm.html b/select_comm/select_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..e6e103cda55442d318a7161ccc8a353f365359bf
--- /dev/null
+++ b/select_comm/select_comm.html
@@ -0,0 +1,23 @@
+<TITLE>Index of general keywords from SELECT</TITLE>
+<H1>Description of general keywords (SELECT)</H1>
+
+<UL>
+<LI> <A HREF="../select/select__select_xyx.html">
+  SELECT_XYX</A>
+  XYX, XY, Y, X, YX, YYX, XXY polarisations
+<LI> <A HREF="../select/select__ha_range.html">
+  HA_RANGE</A>
+  HA range
+<LI> <A HREF="../select/select__select_ifrs.html">
+  SELECT_IFRS</A>
+  Changes to the interferometer selection|
+<LI> <A HREF="../select/select__select_tels.html">
+  SELECT_TELS</A>
+  Changes to the telescope selection|
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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diff --git a/select_public_intfc/images.pl b/select_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/select_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
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+
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diff --git a/select_public_intfc/labels.pl b/select_public_intfc/labels.pl
new file mode 100644
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--- /dev/null
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+
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diff --git a/select_public_intfc/select_public_intfc.html b/select_public_intfc/select_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..9b30e1bb8579e22fd2650e36166905e5e48bd70f
--- /dev/null
+++ b/select_public_intfc/select_public_intfc.html
@@ -0,0 +1,223 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group SELECT</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=select_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=select_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=select_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=select_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=select_public_intfc.html#SECTION0003200000000000000>  <b>Parameter HA_RANGE</b></A>
+<LI> <A NAME=tex2html6 HREF=select_public_intfc.html#SECTION0003300000000000000>  <b>Parameter SELECT_IFRS</b></A>
+<LI> <A NAME=tex2html7 HREF=select_public_intfc.html#SECTION0003400000000000000>  <b>Parameter SELECT_TELS</b></A>
+<LI> <A NAME=tex2html8 HREF=select_public_intfc.html#SECTION0003500000000000000>  <b>Parameter SELECT_XYX</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group SELECT, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.ha.range><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter HA_RANGE</b></A></H2>
+<P>
+  <em>Prompt:</em> HA range (<em>may vary per application</em>)<BR><em>Expected input:</em> Real:  1 to 2 values
+<P>
+    <PRE>
+        Specify the hour-angle range to be selected
+</PRE>
+<P>
+<A NAME=.select.ifrs><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter SELECT_IFRS</b></A></H2>
+<P>
+<em>Prompt:</em> Changes to the interferometer selection| (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *4:  1 to 40 values
+<P>
+  <PRE>
+        Specify how you want to change the interferometer selection.
+</PRE>
+<P>
+  <PRE>
+Interferometers are defined as combinations of two telescopes; an
+interferometer may thus contain 1, 2 or 4 polarisations.
+</PRE>
+<P>
+  <PRE>
+A combination of two different telescopes is called a CROSS[-correlating]
+interferometer, a telescope combined with itself an AUTO[-correlating]
+interferometer. At present, WSRT data contain only cross-interferometer data,
+so selection/elimination of auto-interferometers is irrelevant.
+</PRE>
+<P>
+  <PRE>
+The following codes are used to identify (groups of) telescopes:
+</PRE>
+<P>
+  <PRE>
+        P       show the present selection table
+</PRE>
+<P>
+  <PRE>
+   For the WSRT:
+        0,1,2,3,4,5,6,7,8,9,A,B,C,D:
+                 individual WSRT telescopes (case-insensitive)
+        *       all telescopes or all cross interferometers
+        F       all fixed telescopes = 0 through 9
+        M       all movable telescopes = A through D
+        Y       telescopes A and B
+        Z       telescopes C and D
+        #       autocorrelation
+</PRE>
+<P>
+  <PRE>
+   Additional codes for the Australian Telecope Compact Array (ATCA):
+        T       ATCA telescopes (8-D)
+        U       the ATCA complement (0-7).
+</PRE>
+<P>
+  <PRE>
+An interferometer specification without a prefix or prefixed with a + sign is
+SELECTED, a specification with a minus sign prefixed is ELIMINATED. Selection
+and elimination are incremental. Up to 40 select/eliminate specifications may
+be given, separated by comma's; they will be honored in the order in which you
+give them. Prompting will continue until you stop replying.
+</PRE>
+<P>
+  <PRE>
+The standard operation is on the cross-correlations. A telescope name followed
+with a # indicates the auto-correlations.
+</PRE>
+<P>
+  <PRE>
+Examples:
+        -3F     eliminate combinations of 3 with other fixed telescopes
+        FM,-9A  select all fixed-movable combinations (the WSRT's 40 'standard'
+                 interferometers) except 9A
+        -#,33   eliminate all auto-interferometers, then re-select 33
+</PRE>
+<P>
+<A NAME=.select.tels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter SELECT_TELS</b></A></H2>
+<P>
+<em>Prompt:</em> Changes to the telescope selection| (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *4:  1 to 20 values
+<P>
+  <PRE>
+        Specify how you want to change the telescope selection.
+</PRE>
+<P>
+  <PRE>
+The following codes are used to identify (groups of) telescopes:
+</PRE>
+<P>
+  <PRE>
+        P       show the present selection table
+</PRE>
+<P>
+  <PRE>
+   For the WSRT:
+        0,1,2,3,4,5,6,7,8,9,A,B,C,D:
+                individual WSRT telescopes (case-insensitive)
+        *       all telesopes
+        F       all fixed telescopes = 0 through 9
+        M       all movable telescopes = A through D
+        Y       telescopes A and B
+        Z       telescopes C and D
+</PRE>
+<P>
+  <PRE>
+   Additional codes for the Australian Telecope Compact Array (ATCA):
+        T       ATCA telescopes (8-D)
+        U       the ATCA complement (0-7).
+</PRE>
+<P>
+  <PRE>
+A telesope specification without a prefix or prefixed with a + sign is
+SELECTED, a specification with a minus sign prefixed is ELIMINATED. Selection
+and elimination are incremental. Up to 20 select/eliminate specifications may
+be given, separated by comma's; they will be honored in the order in which you
+give them. Prompting will continue until you stop replying.
+</PRE>
+<P>
+  <PRE>
+Examples: -*,3,+3,-8,*,-F,-U,T
+</PRE>
+<P>
+<A NAME=.select.xyx><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter SELECT_XYX</b></A></H2>
+<P>
+<em>Prompt:</em> polarisations (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *4:  1 value
+<P>
+  <PRE>
+        Select the polarisation(s) to be used:
+</PRE>
+<P>
+  <PRE>
+        XYX     all four combinations (XX,YX,YX,YY)
+        XY      XX and YY
+        X       XX only
+        Y       YY only
+        YX      XY and YX
+        YYX     YX
+        XXY     XY
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
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diff --git a/selected_papers/images.pl b/selected_papers/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/selected_papers/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/selected_papers/labels.pl b/selected_papers/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..d35805c9867870f3893b1bcdf95871618e8f6160
--- /dev/null
+++ b/selected_papers/labels.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/selected_papers/selected_papers.html b/selected_papers/selected_papers.html
new file mode 100644
index 0000000000000000000000000000000000000000..d14a07a8a3e7a813727bc522967f9a68562f2245
--- /dev/null
+++ b/selected_papers/selected_papers.html
@@ -0,0 +1,55 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Selected papers</b>
+<P>
+There are some papers that are closely related to the material covered in this cookbook, and may therefore be interesting to the user. Copies of these papers are attached here. Others are mentioned in the bibliography of this Cookbook.
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
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+
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+newstar@nfra.nl
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+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/show_edit/_12943_tabular127.png b/show_edit/_12943_tabular127.png
new file mode 100644
index 0000000000000000000000000000000000000000..6a9e642e090686800b29687973803fa3cd925f5a
Binary files /dev/null and b/show_edit/_12943_tabular127.png differ
diff --git a/show_edit/_12943_tabular127.xbm b/show_edit/_12943_tabular127.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..658fc9da2c1770348ec5fe4faddc3d5394437818
--- /dev/null
+++ b/show_edit/_12943_tabular127.xbm
@@ -0,0 +1,547 @@
+#define noname_width 399
+#define noname_height 163
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x80,0x80,0x01,0x80,0x00,0x00,0x0c,0x00,
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+ 0xb8,0xf3,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x80,0x01,
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+ 0x22,0x1b,0x40,0x04,0x01,0x10,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
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+ 0x00,0x00,0x00,0x00,0x00,0x22,0x1b,0x40,0x04,0x01,0x10,0xc1,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x70,0xf3,0xf3,0xcf,0xff,0xe3,0xf9,0x80,0xef,0xee,0x79,0x00,0x0c,0x00,
+ 0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x22,0x1f,0x40,0x04,0x01,
+ 0x10,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x62,0x32,0x6d,0x62,0x32,0x8f,0x80,0xd9,
+ 0xc4,0xcc,0x00,0x0c,0x00,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x22,0x3b,0x40,0x04,0x01,0x10,0xc1,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x62,0xf2,0x6c,
+ 0x62,0xf2,0x8f,0x80,0xd1,0xc6,0xfc,0x00,0x0c,0x00,0x06,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x22,0x33,0x40,0x04,0x01,0x10,0xc1,0x00,0x00,0x00,
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+ 0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x3b,0xc0,0x06,0x01,
+ 0xb0,0xcd,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x63,0x12,0x4d,0x60,0x32,0x8e,0x80,0x99,
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+ 0xbe,0x1f,0xc0,0xc7,0x07,0xf0,0x79,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0xf7,0xf7,0xdf,
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+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x00,0x00,0x18,0x03,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0xf0,0x01,
+ 0x00,0x00,0x00,0x00,0x00};
diff --git a/show_edit/_12943_tabular144.png b/show_edit/_12943_tabular144.png
new file mode 100644
index 0000000000000000000000000000000000000000..92d4acf7ccffa2b1888321b85e69cf71f2768655
Binary files /dev/null and b/show_edit/_12943_tabular144.png differ
diff --git a/show_edit/_12943_tabular144.xbm b/show_edit/_12943_tabular144.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5cc68247a964c6d703d4cfe4a932eef11054e6d9
--- /dev/null
+++ b/show_edit/_12943_tabular144.xbm
@@ -0,0 +1,231 @@
+#define noname_width 452
+#define noname_height 60
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x77,0x00,0x1c,0x00,
+ 0x00,0x00,0x70,0x00,0x00,0x00,0x00,0x0c,0x00,0xe0,0xe0,0x00,0xc0,0x01,0x70,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x18,0x00,0x00,0x07,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x66,0x00,0x18,0x00,0x00,0x00,0x62,
+ 0x00,0x00,0x00,0x40,0x0c,0x00,0xc0,0xc0,0x00,0x80,0x01,0x78,0x00,0x00,0x00,
+ 0x00,0x21,0x00,0x08,0x18,0x00,0x10,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x63,0x00,0x00,0x00,
+ 0x60,0x00,0x00,0xc0,0xc0,0x00,0x80,0x01,0x18,0x00,0x00,0x00,0x80,0x31,0x00,
+ 0x08,0x00,0x00,0x18,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x63,0x00,0x00,0x00,0x60,0x00,0x00,
+ 0xc0,0xc0,0x00,0x80,0x01,0x18,0x00,0x00,0x00,0x80,0x31,0x00,0x08,0x00,0x00,
+ 0x18,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xfc,0x7f,0x66,
+ 0xf0,0xf9,0x7c,0xff,0x83,0xe7,0xe3,0x01,0xef,0xf7,0xee,0xf3,0xc0,0xc7,0x7c,
+ 0xbe,0x1d,0xbc,0xef,0xfb,0x1f,0xcf,0x7b,0x9e,0x0f,0xdc,0x0f,0x3c,0x3e,0x0f,
+ 0x7c,0xcf,0xff,0x78,0xe0,0xff,0xe7,0x0e,0x3c,0x1f,0x00,0x00,0x00,0x00,0x00,
+ 0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xd8,0x66,0x66,0x30,0x99,0x46,
+ 0xb6,0x01,0x63,0x32,0x83,0xd9,0x64,0xcc,0x9b,0xc1,0xcc,0x46,0xb3,0x07,0xd8,
+ 0xc8,0x33,0x33,0x9b,0x31,0xf3,0x08,0x98,0x09,0x18,0xa6,0x19,0x4c,0x9b,0x99,
+ 0xcd,0xc0,0xb6,0xcd,0x04,0x6c,0x13,0x00,0x00,0x00,0x00,0x00,0x3e,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xd8,0x63,0x66,0xf0,0x98,0xc6,0xf6,0x00,0x63,
+ 0xf2,0x83,0xdf,0x64,0xcc,0xf8,0xc1,0xc8,0xc6,0x83,0x03,0xd8,0xd8,0x30,0x33,
+ 0x9e,0x31,0xff,0x08,0x98,0x09,0x18,0xa6,0x1f,0x3c,0x9e,0x99,0xfd,0xc0,0x1e,
+ 0xcf,0x06,0x78,0x0f,0x00,0x00,0x00,0x00,0x00,0x2a,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xf0,0x63,0x66,0xf0,0x99,0xc6,0xfc,0x00,0x6b,0x32,0x80,0xc1,
+ 0x64,0xcd,0x18,0xc0,0xc8,0xc6,0x83,0x07,0xd8,0xd8,0x30,0x33,0x9b,0xb5,0xc3,
+ 0x08,0x98,0x09,0x58,0xa6,0x01,0x7c,0x9b,0x99,0x0d,0x80,0x9f,0x8d,0x03,0x6c,
+ 0x1f,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xb0,0x63,0x66,0x10,0x99,0x46,0xec,0x00,0x6b,0x32,0x82,0xd1,0x64,0xcd,0x18,
+ 0xc1,0xcc,0x46,0xa3,0x0f,0xd8,0xc8,0x30,0xb3,0xb9,0xb5,0xe3,0x08,0x98,0x09,
+ 0x58,0xa6,0x11,0xc4,0xb9,0x99,0x8d,0x80,0xdd,0x9c,0x03,0xe6,0x11,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0xf1,0xff,
+ 0xf0,0xfd,0x7d,0x4c,0x00,0xff,0xe7,0x01,0xef,0xef,0xff,0xf1,0xc0,0xe7,0x7d,
+ 0xde,0x1f,0xbc,0xef,0xf9,0x7f,0xbf,0xf7,0x9e,0x1f,0xfc,0x1f,0x78,0x7f,0x0f,
+ 0x7c,0xff,0xff,0x7b,0x80,0x89,0x1f,0x01,0xfc,0x1f,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xe0,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x0e,0x00,0x00,0x00,0xbc,0xfe,0x1f,0x1e,0xbe,0xef,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x0f,0x00,0x00,0x00,0xfe,0xfe,0x9f,0x7b,0xbe,0xef,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,
+ 0x00,0x00,0xc6,0x18,0xc6,0x61,0x1c,0xc7,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0xce,
+ 0x18,0xc6,0xe1,0x38,0x4f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xf7,0x7d,0xe0,0x01,0x7e,0xf8,0xc7,0xe0,
+ 0xb8,0x6f,0xc0,0xf7,0xfd,0xcf,0xff,0x78,0x7e,0x7c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x1b,0x79,0x60,0x03,0xfe,0xf8,0xc7,0xe0,0xf0,0x2f,0x60,
+ 0x1e,0x99,0x99,0x99,0xd9,0x4c,0x46,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x1b,0x1b,0xc0,0x03,0xf0,0x18,0xc6,0xe0,0xf0,0x3c,0x60,0x18,0x9b,0x99,
+ 0x99,0xf1,0x4c,0x46,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1b,0x1b,
+ 0x60,0x03,0xc2,0x18,0xc6,0xe1,0xf0,0x3c,0x60,0x18,0x9b,0x99,0x99,0xd9,0x4c,
+ 0x46,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1b,0x19,0x30,0x07,0xc6,
+ 0x18,0xc6,0x71,0x60,0x18,0x60,0x1c,0x99,0x99,0x99,0xcd,0x4d,0x46,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xf7,0x3d,0xe0,0x07,0x7e,0xfe,0x1f,0x3f,
+ 0x60,0x18,0xc0,0xf3,0xfd,0xff,0xff,0xfb,0xff,0xfc,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x60,0x77,0x00,0x1c,0x00,0x00,0x00,0x70,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0xc0,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x03,0xe0,0x0e,
+ 0x60,0x00,0x00,0x00,0x78,0xc0,0xc1,0x00,0x60,0x00,0x00,0x1c,0x00,0x70,0x70,
+ 0x00,0xe0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x66,
+ 0x00,0x18,0x00,0x00,0x00,0x62,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x20,0xe0,0x01,0x00,0x00,0x00,0x02,0x00,0xc0,0x03,0xc0,0x0c,0x40,0x00,0x04,
+ 0x00,0x6c,0x80,0x81,0x00,0x60,0x00,0x40,0x18,0x00,0x60,0x60,0x00,0xc0,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x66,0x00,0x18,0x00,
+ 0x00,0x00,0x63,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x60,0x00,
+ 0x00,0x00,0x00,0x03,0x00,0xc0,0x00,0xc0,0x0c,0x40,0x00,0x06,0x00,0x4c,0x80,
+ 0x81,0x00,0x00,0x00,0x60,0x18,0x00,0x60,0x60,0x00,0xc0,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x63,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x60,0x00,0x00,0x00,0x00,
+ 0x03,0x00,0xc0,0x00,0xc0,0x0c,0x40,0x00,0x06,0x00,0x0c,0x80,0x81,0x00,0x00,
+ 0x00,0x60,0x18,0x00,0x60,0x60,0x00,0xc0,0x00,0x1c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xfc,0x7f,0x66,0xf0,0xf9,0x7c,0xff,0x83,0xe7,0xe3,0x81,0x9f,
+ 0xe7,0x7f,0xbc,0x0f,0x3c,0x3f,0x3e,0xf0,0xbe,0xff,0x3f,0x9e,0xe7,0x83,0xef,
+ 0x81,0xc7,0x0c,0x7c,0x3c,0xcf,0x03,0x7e,0x9e,0xf9,0x7c,0x70,0x3f,0xf0,0xf8,
+ 0x3c,0xe0,0x63,0x3e,0xdf,0x0e,0x1c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xd8,0x66,0x66,0x30,0x99,0x46,0xb6,0x01,0x63,0x32,0x03,0x93,0xcd,0xcc,0xe6,
+ 0x09,0x6c,0x26,0x23,0x60,0x23,0x6f,0x66,0x36,0x63,0xc2,0xc8,0x80,0xcd,0x0c,
+ 0x46,0x6c,0xc6,0x06,0x4c,0xb3,0x8d,0x4c,0x60,0x26,0x60,0x98,0x66,0x60,0x66,
+ 0xa3,0xd9,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xd8,0x63,0x66,
+ 0xf0,0x98,0xc6,0xf6,0x00,0x63,0xf2,0x03,0x13,0xcf,0xcc,0xfe,0x07,0x78,0x26,
+ 0x23,0x60,0x63,0x63,0x66,0x3c,0xe3,0xc1,0xd8,0x00,0xcf,0x0c,0x46,0x78,0x86,
+ 0x07,0x4c,0xbf,0x8d,0x3c,0x60,0x26,0x60,0x98,0x7e,0x60,0x64,0xe3,0xc1,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x63,0x66,0xf0,0x99,0xc6,
+ 0xfc,0x00,0x6b,0x32,0x00,0x93,0xcd,0xcc,0x86,0x0f,0x6c,0x26,0x23,0x60,0x63,
+ 0x63,0x66,0x36,0xeb,0xc3,0xd8,0x80,0xcd,0x0c,0x46,0x6c,0xd6,0x06,0x4c,0x83,
+ 0x8d,0x7c,0x60,0x26,0x60,0x99,0x06,0x60,0x64,0xe3,0xc1,0x03,0x1c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xb0,0x63,0x66,0x10,0x99,0x46,0xec,0x00,0x6b,
+ 0x32,0x02,0xd3,0xdc,0xcc,0xc6,0x08,0xe6,0x26,0x23,0x60,0x23,0x63,0x66,0x73,
+ 0x2b,0xc2,0xc8,0xc0,0xdc,0x0c,0x46,0xe6,0x76,0x0e,0x4c,0xa3,0x8d,0x44,0x60,
+ 0x26,0x60,0x99,0x46,0x60,0x66,0xa3,0xd1,0x07,0x1c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0xf1,0xff,0xf0,0xfd,0x7d,0x4c,0x00,0xff,0xe7,0x81,0xbf,
+ 0xff,0xff,0xbd,0x0f,0xfc,0x7f,0x7e,0xf0,0xbe,0xf7,0xff,0x7e,0xef,0x83,0xef,
+ 0x81,0xff,0x1f,0xfc,0xfc,0xde,0x0f,0xee,0xde,0xfb,0x7d,0xf0,0x7f,0xe0,0xfd,
+ 0x3d,0xe0,0xf3,0x3e,0xef,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x77,0x00,0x1c,0x00,
+ 0x00,0x00,0x0e,0x00,0x00,0x00,0x00,0x60,0x00,0x0e,0x00,0x00,0x00,0x00,0x06,
+ 0x00,0x00,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x66,0x00,0x18,0x00,0x00,0x00,0x0f,
+ 0x00,0x00,0x00,0x10,0x60,0x00,0x0f,0x00,0x00,0x00,0x20,0x06,0x00,0x00,0x0f,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x30,
+ 0x00,0x00,0x00,0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x03,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x03,0x00,0x00,0x06,
+ 0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x78,0x00,0x00,0x00,0x00,0xf0,0x00,0x00,0x00,
+ 0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x03,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x03,0x00,0x80,0x07,0x00,0x00,0x00,
+ 0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x9c,0xff,0x8f,0xe7,0xef,0xc3,0xe1,0x00,0x00,0xfc,0x7f,0x66,
+ 0xf0,0xf9,0x7c,0xff,0x83,0xf7,0xfd,0xff,0xf1,0x3c,0x70,0xbf,0xe7,0xfb,0xff,
+ 0xe3,0x79,0xe7,0xfb,0x81,0xf7,0x7d,0xc0,0xf9,0xfb,0x79,0xfe,0x7c,0x1c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x87,0xbf,0x8d,0x6d,0x6f,0x07,0xe7,0x00,0x00,0xd8,0x66,0x66,0x30,0x99,0x46,
+ 0xb6,0x01,0x1b,0x79,0x33,0xb3,0x19,0x60,0x26,0x33,0xf2,0x66,0x66,0x33,0x36,
+ 0x32,0x01,0x1b,0x79,0x70,0xf8,0xb3,0xd9,0xf6,0xec,0x70,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0f,0xbf,0x8d,
+ 0x6f,0xfd,0x87,0x07,0x00,0x00,0xd8,0x63,0x66,0xf0,0x98,0xc6,0xf6,0x00,0x1b,
+ 0x1b,0x33,0xe3,0x19,0x60,0x26,0x33,0x36,0x66,0xc6,0x33,0x36,0x36,0x01,0x1b,
+ 0x1b,0xf0,0xf0,0xb3,0xf9,0xd6,0xfe,0x78,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x9c,0xbf,0xcd,0x6d,0xfd,0xc7,
+ 0x01,0x00,0x00,0xf0,0x63,0x66,0xf0,0x99,0xc6,0xfc,0x00,0x1b,0x1b,0x33,0xb3,
+ 0x59,0x60,0x26,0x33,0x36,0x66,0x66,0xb3,0x36,0x36,0x01,0x1b,0x1b,0xc0,0xf9,
+ 0xb3,0xdd,0xd6,0xfe,0x1c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0xbf,0xcd,0x6d,0x6d,0x76,0xe0,0x00,0x00,
+ 0xb0,0x63,0x66,0x10,0x99,0x46,0xec,0x00,0x1b,0x19,0x33,0x9b,0x5b,0x60,0x26,
+ 0x33,0x32,0x66,0x36,0xb7,0x36,0x32,0x01,0x1b,0x19,0x00,0xff,0xb3,0xdd,0xd6,
+ 0xcc,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xe0,0xff,0x9f,0xff,0xef,0x33,0xe0,0x00,0x00,0x30,0xf1,0xff,
+ 0xf0,0xfd,0x7d,0x4c,0x80,0xf7,0xbd,0xff,0xf7,0x7b,0xf0,0xff,0xe7,0x7b,0xff,
+ 0xef,0xf7,0xef,0xfb,0x83,0xf7,0x3d,0x00,0xfe,0xfb,0xfb,0xff,0x7c,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/show_edit/_12943_tabular152.png b/show_edit/_12943_tabular152.png
new file mode 100644
index 0000000000000000000000000000000000000000..c5b967b5f073b3651c9ed315679fd2ca3d136d62
Binary files /dev/null and b/show_edit/_12943_tabular152.png differ
diff --git a/show_edit/_12943_tabular152.xbm b/show_edit/_12943_tabular152.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..91750ca98d8d975851a36479fa3f0d5b15add1ff
--- /dev/null
+++ b/show_edit/_12943_tabular152.xbm
@@ -0,0 +1,360 @@
+#define noname_width 432
+#define noname_height 99
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0xe0,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x0e,0x00,
+ 0x80,0x01,0x38,0x00,0x70,0x00,0x00,0x8c,0x01,0x80,0x03,0x00,0x40,0x00,0xc0,
+ 0x01,0x00,0xe0,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,
+ 0x00,0x00,0x00,0x36,0x00,0x00,0x20,0x0c,0x00,0x00,0x01,0x3c,0x00,0x60,0x04,
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+ 0xff,0xf3,0x03,0x1f,0x03,0x00,0x78,0x7c,0x1e,0xf0,0xdd,0x3d,0x0f,0xfc,0xfb,
+ 0x3c,0xe0,0x7b,0xe0,0x81,0xef,0x7e,0x7e,0xf3,0x80,0x67,0xde,0xff,0x78,0xbf,
+ 0x07,0xcc,0xff,0x3e,0xe7,0xfb,0xc0,0x7d,0xf0,0x7c,0x3c,0xf0,0xdf,0x77,0x3f,
+ 0x3f,0x30,0xef,0xc7,0xff,0x7c,0xf3,0xc8,0x4c,0x66,0x66,0x02,0x33,0x03,0x00,
+ 0x30,0x4c,0x33,0x30,0x9b,0x98,0x19,0x4c,0xcb,0x66,0x30,0x32,0x60,0x83,0xc9,
+ 0x4c,0x13,0x9b,0xc1,0x6c,0xb3,0x99,0xcd,0x26,0x03,0x8c,0x6d,0x26,0x36,0x9b,
+ 0x80,0x4d,0x60,0x4c,0x66,0x30,0x8d,0x67,0xa6,0x09,0xb0,0xd9,0x64,0x62,0x4c,
+ 0xc3,0xd8,0x4c,0x66,0x66,0x02,0x23,0x00,0x00,0x30,0x4c,0x3f,0x30,0xda,0x98,
+ 0x1f,0x3c,0x6b,0x7e,0x30,0x36,0xc0,0x83,0xc7,0x4c,0x13,0xfb,0xc1,0x6f,0xbf,
+ 0x99,0xfd,0x26,0x03,0x8c,0x3d,0x26,0x36,0x98,0x80,0x3d,0x60,0x4c,0x7e,0xf0,
+ 0x8c,0x61,0xa6,0x09,0xb0,0xdf,0x64,0x62,0x4c,0xc3,0xd8,0x4c,0x66,0x66,0x02,
+ 0x23,0x00,0x00,0xb0,0x4c,0x03,0x30,0x72,0xd8,0x01,0x7c,0xb3,0x06,0x30,0x36,
+ 0x60,0x83,0xcf,0x4c,0x1e,0x1b,0xc0,0x60,0x83,0x99,0x0d,0x26,0x0b,0x0c,0x3f,
+ 0x26,0x36,0x98,0x80,0x7d,0x60,0x4d,0x06,0xf0,0xad,0x61,0x26,0x0f,0xb0,0xc1,
+ 0xc4,0x63,0x4d,0xe3,0xc8,0x6c,0x66,0x66,0x02,0x32,0x03,0x00,0xb0,0x4c,0x23,
+ 0x30,0x73,0xd8,0x11,0x44,0xb3,0x46,0x30,0x32,0x30,0x87,0xc8,0x4c,0x02,0x1b,
+ 0xc1,0x68,0xa3,0x99,0x8d,0x26,0x0b,0x0c,0x3b,0x26,0x36,0x9a,0x80,0x45,0x60,
+ 0x4d,0x46,0x10,0xad,0x61,0x26,0x01,0xb0,0xd1,0x44,0x60,0x4d,0x9e,0xef,0xfd,
+ 0xff,0xff,0x07,0x36,0x03,0x00,0xf0,0xfe,0x1e,0xf0,0x21,0x78,0x0f,0xfc,0xff,
+ 0x3c,0xe0,0x7b,0xe0,0x87,0xef,0xff,0xbe,0xf7,0x80,0xf7,0xde,0xff,0x7b,0x7f,
+ 0x0f,0x0c,0x13,0x7f,0xef,0xfd,0xc1,0x7f,0xe0,0xff,0x3c,0xf0,0xfd,0xf3,0x7f,
+ 0x1f,0x78,0xef,0xcf,0xe7,0xff,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x63,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x31,0x00,0x00,0x60,0x0c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x3c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x63,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x18,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x80,0x31,0x00,0x00,0x60,0x0c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x18,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1f,0x00,0x00,
+ 0xc0,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,0x00,0xc0,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x38,0x00,0x20,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x02,0x00,
+ 0x00,0x00,0x30,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x30,0x00,0x40,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x03,0x00,0x00,0x00,0x30,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xef,0xfb,0xc0,0x03,0xfc,0x8f,0xe7,0x7b,0xfc,0xc7,0xfb,0xe0,0xee,0xb1,
+ 0x9b,0xc7,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0xf2,0xc0,0x06,0xe6,
+ 0x89,0xcd,0xdb,0x66,0x63,0xf6,0xc0,0x64,0x33,0xd3,0xcc,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x36,0x36,0x80,0x07,0x86,0x09,0xcf,0xf0,0x06,0xe3,0x37,
+ 0xc0,0xc6,0x33,0xd3,0xcf,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x36,
+ 0xc0,0x06,0x86,0x89,0xcd,0xd8,0x06,0x6b,0x30,0x80,0x63,0x33,0xd3,0xc0,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x32,0x60,0x0e,0xc6,0xc9,0xdc,0xcc,
+ 0x47,0x6b,0x34,0x80,0x33,0x37,0xdb,0xc8,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xef,0x7b,0xc0,0x0f,0xfc,0x9f,0xff,0xf9,0x3d,0xcf,0x7b,0x00,0xe1,0x7f,
+ 0xbf,0xc7,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/show_edit/_12943_tex2html_wrap636.png b/show_edit/_12943_tex2html_wrap636.png
new file mode 100644
index 0000000000000000000000000000000000000000..eee8382ab30aacea79d9840bec39b9209823c74b
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap636.png differ
diff --git a/show_edit/_12943_tex2html_wrap636.xbm b/show_edit/_12943_tex2html_wrap636.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..53dd760651d68c894e110b4aa9dd62c070654add
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap636.xbm
@@ -0,0 +1,11 @@
+#define noname_width 36
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0xc1,0xe2,0x18,0x3e,0x08,0xc1,0xf3,0x19,0x3f,0x08,0xc1,0x91,0x03,0x33,0x08,
+ 0xc1,0xc0,0x83,0x31,0x08,0xc1,0xf0,0x83,0x31,0x08,0xc1,0x38,0x83,0x33,0x08,
+ 0xc1,0xb8,0x1b,0x3b,0x08,0xc1,0xf0,0x1b,0x3f,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap644.png b/show_edit/_12943_tex2html_wrap644.png
new file mode 100644
index 0000000000000000000000000000000000000000..d1c0cfd72f6c12eb214a3a7d444b4f29e741305b
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap644.png differ
diff --git a/show_edit/_12943_tex2html_wrap644.xbm b/show_edit/_12943_tex2html_wrap644.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f0cc194963bb834c681561934c09a5fcf849252e
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap644.xbm
@@ -0,0 +1,14 @@
+#define noname_width 50
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x30,0x03,0x3c,0x02,0x01,0x00,0x00,
+ 0x30,0x03,0x3e,0x02,0x01,0x00,0x00,0x30,0x03,0x06,0x02,0x01,0x00,0x00,0x30,
+ 0x03,0x06,0x02,0xc1,0xe2,0x18,0x3e,0x1f,0x1f,0x02,0xc1,0xf3,0x19,0x3f,0x3f,
+ 0x1f,0x02,0xc1,0x91,0x03,0x33,0x33,0x06,0x02,0xc1,0xc0,0x83,0x31,0x33,0x06,
+ 0x02,0xc1,0xf0,0x83,0x31,0x33,0x06,0x02,0xc1,0x38,0x83,0x33,0x33,0x06,0x02,
+ 0xc1,0xb8,0x1b,0x3b,0x33,0x06,0x02,0xc1,0xf0,0x1b,0x3f,0x33,0x06,0x02,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0x01};
diff --git a/show_edit/_12943_tex2html_wrap646.png b/show_edit/_12943_tex2html_wrap646.png
new file mode 100644
index 0000000000000000000000000000000000000000..b38e14ac2d1fd150b96e9fc60e6ac449b8fd5964
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap646.png differ
diff --git a/show_edit/_12943_tex2html_wrap646.xbm b/show_edit/_12943_tex2html_wrap646.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..259ae68bc7f6fe8b8ff51e3a90fdc3d393511555
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap646.xbm
@@ -0,0 +1,17 @@
+#define noname_width 66
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x03,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x01,0x00,0x00,0x30,0x03,0x3c,0x02,0x03,0x02,0x01,0x00,0x00,0x30,0x03,0xfe,
+ 0xc3,0x07,0x02,0x01,0x00,0x00,0x30,0x03,0xc6,0xc3,0x0c,0x02,0x01,0x00,0x00,
+ 0x30,0x03,0x06,0xc3,0x0c,0x02,0xc1,0xe2,0x18,0x3e,0x1f,0x1f,0x63,0x0c,0x02,
+ 0xc1,0xf3,0x19,0x3f,0x3f,0x1f,0x63,0x0c,0x02,0xc1,0x91,0x03,0x33,0x33,0x06,
+ 0x63,0x0c,0x02,0xc1,0xc0,0x83,0x31,0x33,0x06,0x63,0x0c,0x02,0xc1,0xf0,0x83,
+ 0x31,0x33,0x06,0x63,0x0c,0x02,0xc1,0x38,0x83,0x33,0x33,0x06,0xc3,0x0c,0x02,
+ 0xc1,0xb8,0x1b,0x3b,0x33,0x06,0xc3,0x0c,0x02,0xc1,0xf0,0x1b,0x3f,0x33,0xc6,
+ 0xcf,0x07,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap648.png b/show_edit/_12943_tex2html_wrap648.png
new file mode 100644
index 0000000000000000000000000000000000000000..92eeae146caa5cd642f6c9d5a8cdad4681035824
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap648.png differ
diff --git a/show_edit/_12943_tex2html_wrap648.xbm b/show_edit/_12943_tex2html_wrap648.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..877def0e9b074fdad7247f696385b0fcbb641c61
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap648.xbm
@@ -0,0 +1,12 @@
+#define noname_width 40
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x80,0x81,
+ 0x01,0x00,0x00,0x80,0x81,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xc1,0xe2,0x98,0xb1,0x81,0xc1,0xf3,0x99,0xbb,0x81,0xc1,0x91,0x03,0x9f,0x81,
+ 0xc1,0xc0,0x03,0x8e,0x81,0xc1,0xf0,0x03,0x8e,0x81,0xc1,0x38,0x03,0x9f,0x81,
+ 0xc1,0xb8,0x1b,0x9b,0x81,0xc1,0xf0,0x9b,0xb1,0x81,0x01,0x00,0x00,0x80,0x81,
+ 0x01,0x00,0x00,0xa0,0x81,0x01,0x00,0x00,0xe0,0x81,0x01,0x00,0x00,0xc0,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xff,0xff,0xff,0xff,0x7f};
diff --git a/show_edit/_12943_tex2html_wrap652.png b/show_edit/_12943_tex2html_wrap652.png
new file mode 100644
index 0000000000000000000000000000000000000000..ed185e29540fd5fd196880a9746957343a8407e1
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap652.png differ
diff --git a/show_edit/_12943_tex2html_wrap652.xbm b/show_edit/_12943_tex2html_wrap652.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1359049f8f233f5ce2ea370f5b354538056f2455
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap652.xbm
@@ -0,0 +1,6 @@
+#define noname_width 15
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0x3f,0x01,0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,
+ 0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,0x40,0x01,0x40,
+ 0x01,0x40,0xff,0x7f};
diff --git a/show_edit/_12943_tex2html_wrap666.png b/show_edit/_12943_tex2html_wrap666.png
new file mode 100644
index 0000000000000000000000000000000000000000..73b6f35d418e28ed15289285fda23be364232f3f
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap666.png differ
diff --git a/show_edit/_12943_tex2html_wrap666.xbm b/show_edit/_12943_tex2html_wrap666.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d7a915fe4c61a8115645720ff5a31f5c65d735a3
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap666.xbm
@@ -0,0 +1,18 @@
+#define noname_width 67
+#define noname_height 24
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0xc1,0x9f,0xff,0xf9,0x03,0x10,0x1c,0x00,0x04,0xc1,0xbf,0xff,0xf9,0x07,0x1e,
+ 0x3e,0x00,0x04,0xc1,0x30,0x18,0x18,0x06,0x1e,0x62,0x00,0x04,0xc1,0x30,0x18,
+ 0x18,0x06,0x18,0x63,0x00,0x04,0xc1,0x30,0x18,0x18,0x06,0x18,0x62,0x00,0x04,
+ 0xc1,0x3f,0x18,0x18,0x07,0x18,0x60,0x00,0x04,0xc1,0x1f,0x18,0xf8,0x03,0x18,
+ 0x70,0x00,0x04,0xc1,0x1c,0x18,0x18,0x00,0x18,0x38,0x00,0x04,0xc1,0x18,0x18,
+ 0x18,0x00,0x18,0x18,0x00,0x04,0xc1,0x38,0x18,0x18,0x00,0x18,0x0c,0x00,0x04,
+ 0xc1,0x30,0x18,0x18,0x30,0x18,0x06,0x00,0x04,0xc1,0x60,0x18,0x18,0x30,0x7e,
+ 0x7f,0x00,0x04,0x01,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x30,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/show_edit/_12943_tex2html_wrap668.png b/show_edit/_12943_tex2html_wrap668.png
new file mode 100644
index 0000000000000000000000000000000000000000..2580cc5c8a2d7bea3589bf97a5c5a93560570e65
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap668.png differ
diff --git a/show_edit/_12943_tex2html_wrap668.xbm b/show_edit/_12943_tex2html_wrap668.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..29d52c8bf1ef718c716ee3e66832357daed4b0a1
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap668.xbm
@@ -0,0 +1,36 @@
+#define noname_width 139
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x20,0x00,0x01,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x30,0x0e,0x03,0x18,0x07,0x00,0x10,0x00,0x70,
+ 0x00,0xc0,0x01,0x00,0x00,0x04,0x01,0x00,0x00,0x18,0x1f,0x06,0x98,0x0f,0x00,
+ 0x1e,0x00,0xf8,0x00,0xe0,0x03,0x00,0x0e,0x04,0x01,0x30,0x00,0x18,0x31,0x06,
+ 0x88,0x18,0x00,0x1e,0x00,0x88,0x01,0x60,0x06,0x00,0x0e,0x04,0x01,0x30,0x00,
+ 0x8c,0x31,0x0c,0xcc,0x18,0x00,0x18,0x00,0x8c,0x01,0x20,0x06,0x00,0x0f,0x04,
+ 0xc1,0xfa,0x7c,0x0c,0x31,0x0c,0x8c,0x18,0x00,0x18,0x00,0x88,0x01,0x00,0x06,
+ 0x00,0x0f,0x04,0xc1,0xfb,0xfc,0x0c,0x30,0x0c,0x04,0x18,0x00,0x18,0x00,0x80,
+ 0x01,0xc0,0x03,0x80,0x0d,0x04,0xc1,0x31,0xcc,0x0c,0x38,0x0c,0x06,0x1c,0x00,
+ 0x18,0x00,0xc0,0x01,0xc0,0x03,0x80,0x0d,0x04,0xc1,0x30,0xcc,0x0d,0x1c,0x0c,
+ 0x06,0x0e,0x00,0x18,0x00,0xe0,0x00,0x00,0x06,0xc0,0x0c,0x04,0xc1,0x30,0x8c,
+ 0x0d,0x0c,0x0c,0x02,0x06,0x00,0x18,0x00,0x60,0x00,0x00,0x06,0xc0,0x3f,0x04,
+ 0xc1,0x30,0xcc,0x0d,0x06,0x0c,0x02,0x03,0x00,0x18,0x00,0x30,0x00,0x10,0x06,
+ 0x00,0x0c,0x04,0xc1,0xb0,0xfc,0x0c,0x03,0x0c,0x83,0x81,0x01,0x18,0x06,0x18,
+ 0x18,0x30,0x66,0x00,0x0c,0x04,0xc1,0xf0,0xfc,0x8c,0x3f,0x0c,0xc1,0x9f,0x01,
+ 0x7e,0x06,0xfc,0x19,0xe0,0x67,0x00,0x0c,0x04,0x01,0x00,0x0c,0x0c,0x00,0x0c,
+ 0x01,0x00,0x01,0x00,0x04,0x00,0x10,0xc0,0x41,0x00,0x00,0x04,0x01,0x00,0x0c,
+ 0x18,0x00,0x86,0x01,0x80,0x01,0x00,0x06,0x00,0x18,0x00,0x60,0x00,0x00,0x04,
+ 0x01,0x00,0x0c,0x18,0x00,0x86,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x0c,0x30,0x00,0x83,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x20,0x00,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/show_edit/_12943_tex2html_wrap670.png b/show_edit/_12943_tex2html_wrap670.png
new file mode 100644
index 0000000000000000000000000000000000000000..baa61fcdf646ffcd2a65618785a151c005cd5d4a
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap670.png differ
diff --git a/show_edit/_12943_tex2html_wrap670.xbm b/show_edit/_12943_tex2html_wrap670.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..226a615054661f0c5adfb2b4e7a51692a76f018d
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap670.xbm
@@ -0,0 +1,13 @@
+#define noname_width 48
+#define noname_height 24
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0xc0,0x80,
+ 0x01,0x00,0x00,0x00,0xf0,0x81,0x01,0x30,0x00,0x00,0x30,0x83,0x01,0x30,0x00,
+ 0x00,0x30,0x83,0xc1,0xfa,0x7c,0x00,0x18,0x83,0xc1,0xfb,0xfc,0x00,0x18,0x83,
+ 0xc1,0x31,0xcc,0x00,0x18,0x83,0xc1,0x30,0xcc,0x01,0x18,0x83,0xc1,0x30,0x8c,
+ 0x01,0x18,0x83,0xc1,0x30,0xcc,0x01,0x30,0x83,0xc1,0xb0,0xfc,0x0c,0x30,0x83,
+ 0xc1,0xf0,0xfc,0x0c,0xf0,0x81,0x01,0x00,0x0c,0x08,0xc0,0x80,0x01,0x00,0x0c,
+ 0x0c,0x00,0x80,0x01,0x00,0x0c,0x00,0x00,0x80,0x01,0x00,0x0c,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x00,0x80,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/show_edit/_12943_tex2html_wrap672.png b/show_edit/_12943_tex2html_wrap672.png
new file mode 100644
index 0000000000000000000000000000000000000000..b58716d48ea7c2416e44eff5cf0991a9b9a3fbec
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap672.png differ
diff --git a/show_edit/_12943_tex2html_wrap672.xbm b/show_edit/_12943_tex2html_wrap672.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7502ad49eaefdb671e56270d9ae344cfb60a1241
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap672.xbm
@@ -0,0 +1,48 @@
+#define noname_width 193
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x20,0x00,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x30,0x0e,0x03,0x00,0x0e,0x0c,0x00,0x80,0x81,0xc1,0x01,0x00,
+ 0x00,0x00,0x0e,0x08,0xc0,0x00,0x00,0xc0,0x01,0x01,0x01,0x00,0x00,0x18,0x1f,
+ 0x06,0x00,0x1f,0x9f,0x3f,0xe0,0xe3,0xe3,0xf3,0x07,0x00,0x1c,0x1f,0x0f,0xf0,
+ 0xf9,0xf3,0xe3,0x01,0x01,0x01,0x30,0x00,0x18,0x31,0x06,0x00,0x31,0x33,0x30,
+ 0x60,0x66,0x66,0x06,0x06,0x00,0x1c,0x33,0x0f,0x30,0x03,0x33,0x70,0x00,0x01,
+ 0x01,0x30,0x00,0x8c,0x31,0x0c,0x80,0x31,0x33,0x38,0x70,0x66,0x26,0x06,0x07,
+ 0x00,0x1e,0x31,0x0c,0x38,0x83,0x33,0x30,0x00,0x01,0xc1,0xfa,0x7c,0x0c,0x31,
+ 0x0c,0x00,0x31,0x33,0x18,0x30,0x66,0x06,0x06,0x03,0x00,0x1e,0x30,0x0c,0x18,
+ 0x83,0x31,0xf8,0x01,0x01,0xc1,0xfb,0xfc,0x0c,0x30,0x0c,0x00,0x30,0x1f,0x0c,
+ 0x30,0xe6,0xc3,0x83,0x01,0x00,0x1b,0x1e,0x0c,0x18,0xc3,0xf0,0xf9,0x03,0x01,
+ 0xc1,0x31,0xcc,0x0c,0x38,0x0c,0x00,0x38,0x1f,0x0c,0x60,0xe6,0xc3,0x83,0x01,
+ 0x00,0x1b,0x1e,0x0c,0x30,0xc3,0xf0,0x3b,0x03,0x01,0xc1,0x30,0xcc,0x0d,0x1c,
+ 0x0c,0x00,0x1c,0x33,0x0c,0xe0,0x67,0x06,0x86,0x01,0x80,0x19,0x30,0x0c,0xf0,
+ 0xc3,0x30,0x1b,0x03,0x01,0xc1,0x30,0x8c,0x0d,0x0c,0x0c,0x00,0x8c,0x31,0x06,
+ 0xc0,0x37,0x06,0xc6,0x00,0x80,0x7f,0x30,0x0c,0xe0,0x63,0x00,0x1b,0x03,0x01,
+ 0xc1,0x30,0xcc,0x0d,0x06,0x0c,0x00,0x86,0x31,0x06,0x00,0x36,0x16,0xc6,0x00,
+ 0x00,0x98,0x30,0x0c,0x00,0x63,0x10,0x33,0x03,0x01,0xc1,0xb0,0xfc,0x0c,0x03,
+ 0x8c,0x01,0x03,0x33,0x06,0x23,0x63,0x36,0xc6,0x60,0x00,0x98,0x31,0x0c,0x93,
+ 0x61,0x18,0x33,0x03,0x01,0xc1,0xf0,0xfc,0x8c,0x3f,0x8c,0x81,0x3f,0x3f,0x06,
+ 0xe3,0xe3,0xe7,0xc7,0x60,0x00,0x18,0x3f,0x3f,0xf3,0x61,0xf0,0xf1,0x01,0x01,
+ 0x01,0x00,0x0c,0x0c,0x00,0x0c,0x01,0x00,0x0c,0x00,0xc0,0x80,0xc1,0x01,0x40,
+ 0x00,0x00,0x0e,0x00,0x60,0x00,0xe0,0xc0,0x00,0x01,0x01,0x00,0x0c,0x18,0x00,
+ 0x86,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x0c,0x18,0x00,0x06,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x0c,0x30,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x20,0x00,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01};
diff --git a/show_edit/_12943_tex2html_wrap674.png b/show_edit/_12943_tex2html_wrap674.png
new file mode 100644
index 0000000000000000000000000000000000000000..faaf3882388ce6577c279ec9fd833e46371df903
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap674.png differ
diff --git a/show_edit/_12943_tex2html_wrap674.xbm b/show_edit/_12943_tex2html_wrap674.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3680b125e37685db678b2ab002d4b63ab89f7f83
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap674.xbm
@@ -0,0 +1,16 @@
+#define noname_width 60
+#define noname_height 24
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0xc1,0x0c,0xc0,0x00,0x00,
+ 0x08,0x0e,0x08,0xc1,0x0c,0xc0,0x00,0x00,0x0f,0x1f,0x08,0xc1,0x00,0xc0,0x00,
+ 0x00,0x0f,0x31,0x08,0xc1,0x00,0xc0,0x00,0x00,0x8c,0x31,0x08,0xc1,0xec,0xc3,
+ 0x0c,0x00,0x0c,0x31,0x08,0xc1,0xec,0xc7,0x0e,0x00,0x0c,0x30,0x08,0xc1,0x6c,
+ 0xc6,0x07,0x00,0x0c,0x38,0x08,0xc1,0x6c,0xc6,0x03,0x00,0x0c,0x1c,0x08,0xc1,
+ 0x6c,0xc6,0x07,0x00,0x0c,0x0c,0x08,0xc1,0x6c,0xc6,0x06,0x00,0x0c,0x06,0x08,
+ 0xc1,0x6c,0xc6,0xce,0x00,0x0c,0x03,0x08,0xc1,0x6c,0xc6,0xdc,0x00,0xbf,0x3f,
+ 0x08,0x01,0x00,0x00,0x80,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap676.png b/show_edit/_12943_tex2html_wrap676.png
new file mode 100644
index 0000000000000000000000000000000000000000..ddeaf91bbbdd2367d805dafba8cd02462bc31cde
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap676.png differ
diff --git a/show_edit/_12943_tex2html_wrap676.xbm b/show_edit/_12943_tex2html_wrap676.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e8dee20978b0c8d32115edfd88a929d62b77fea6
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap676.xbm
@@ -0,0 +1,27 @@
+#define noname_width 98
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x03,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x02,0x10,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0xc1,0x0c,0xc0,0x00,0x83,0x30,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x02,0xc1,0x0c,0xc0,0x80,0xf1,0x60,0x00,0x00,0x00,0x00,0xc0,0x03,0x02,0xc1,
+ 0x00,0xc0,0x80,0xf1,0x60,0x00,0x00,0x00,0x00,0xc0,0x03,0x02,0xc1,0x00,0xc0,
+ 0xc0,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,0x03,0x02,0xc1,0xec,0xc3,0xcc,0xc0,
+ 0xc0,0x00,0x00,0x00,0x00,0x00,0x03,0x02,0xc1,0xec,0xc7,0xce,0xc0,0xc0,0x00,
+ 0x00,0x00,0x00,0x00,0x03,0x02,0xc1,0x6c,0xc6,0xc7,0xc0,0xc0,0xfc,0x9f,0xff,
+ 0x03,0x00,0x03,0x02,0xc1,0x6c,0xc6,0xc3,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,
+ 0x03,0x02,0xc1,0x6c,0xc6,0xc7,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,0x03,0x02,
+ 0xc1,0x6c,0xc6,0xc6,0xc0,0xc0,0xfc,0x9f,0xff,0x03,0x00,0x03,0x02,0xc1,0x6c,
+ 0xc6,0xce,0xc0,0xc0,0x00,0x00,0x00,0x30,0x00,0x03,0x02,0xc1,0x6c,0xc6,0xdc,
+ 0xf0,0xc3,0x00,0x00,0x00,0x30,0xc0,0x0f,0x02,0x01,0x00,0x00,0xc0,0x00,0xc0,
+ 0x00,0x00,0x00,0x20,0x00,0x00,0x02,0x01,0x00,0x00,0x80,0x01,0x60,0x00,0x00,
+ 0x00,0x30,0x00,0x00,0x02,0x01,0x00,0x00,0x80,0x01,0x60,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x03,0x30,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x02,0x01,0x00,0x00,0x00,0x02,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap680.png b/show_edit/_12943_tex2html_wrap680.png
new file mode 100644
index 0000000000000000000000000000000000000000..cdebbaa352d35561f7ba1efadbee4ba498746351
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap680.png differ
diff --git a/show_edit/_12943_tex2html_wrap680.xbm b/show_edit/_12943_tex2html_wrap680.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2b52bdda40d94c0ad090d810ea0079711b61b981
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap680.xbm
@@ -0,0 +1,7 @@
+#define noname_width 19
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0xff,0x07,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0xc1,0x18,0x04,
+ 0xc1,0x18,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,
+ 0xc1,0x18,0x04,0xc1,0x18,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,
+ 0x01,0x00,0x04,0xff,0xff,0x07};
diff --git a/show_edit/_12943_tex2html_wrap698.png b/show_edit/_12943_tex2html_wrap698.png
new file mode 100644
index 0000000000000000000000000000000000000000..e1b238ca993c36a479f80dab4cdc383379b59d62
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap698.png differ
diff --git a/show_edit/_12943_tex2html_wrap698.xbm b/show_edit/_12943_tex2html_wrap698.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..fa37d493ec9e1fb221cd9ad78bf35e9618240884
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap698.xbm
@@ -0,0 +1,11 @@
+#define noname_width 40
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x80,0x81,0x81,
+ 0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,
+ 0xc1,0x66,0xf0,0xf1,0x81,0xc1,0xff,0xf8,0xf9,0x81,0xc1,0xdd,0x99,0x99,0x81,
+ 0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x9d,0x9d,0x81,
+ 0xc1,0x8c,0xd9,0xd9,0x81,0xc1,0x8c,0xf9,0xf9,0x81,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xff,0xff,0xff,0xff,0x7f};
diff --git a/show_edit/_12943_tex2html_wrap700.png b/show_edit/_12943_tex2html_wrap700.png
new file mode 100644
index 0000000000000000000000000000000000000000..468b2e90f640926dcd5c1aaffe0476d0f3021253
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap700.png differ
diff --git a/show_edit/_12943_tex2html_wrap700.xbm b/show_edit/_12943_tex2html_wrap700.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..bba48f6f3a89d59912db72eea5e285f0b91fd3d6
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap700.xbm
@@ -0,0 +1,12 @@
+#define noname_width 37
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,0xc1,0x78,0x00,0x00,0x10,
+ 0xc1,0x7c,0x00,0x00,0x10,0x01,0x0c,0x00,0x00,0x10,0x01,0x0c,0x00,0x00,0x10,
+ 0xc1,0xbe,0xf5,0x61,0x10,0xc1,0xbe,0xf7,0x63,0x10,0xc1,0x8c,0x33,0x03,0x10,
+ 0xc1,0x8c,0x31,0x07,0x10,0xc1,0x8c,0x31,0x06,0x10,0xc1,0x8c,0x31,0x07,0x10,
+ 0xc1,0x8c,0xf1,0x63,0x10,0xc1,0x8c,0xf1,0x63,0x10,0x01,0x00,0x30,0x00,0x10,
+ 0x01,0x00,0x30,0x00,0x10,0x01,0x00,0x30,0x00,0x10,0x01,0x00,0x30,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0x1f};
diff --git a/show_edit/_12943_tex2html_wrap702.png b/show_edit/_12943_tex2html_wrap702.png
new file mode 100644
index 0000000000000000000000000000000000000000..10049a8814da47be3becbbb3b6d55802788d43d7
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap702.png differ
diff --git a/show_edit/_12943_tex2html_wrap702.xbm b/show_edit/_12943_tex2html_wrap702.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d6498696c82402c428d0c3cf28577a0fdb9b9394
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap702.xbm
@@ -0,0 +1,12 @@
+#define noname_width 33
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,0xc1,0x78,0x00,0x00,0x01,
+ 0xc1,0x7c,0x00,0x00,0x01,0x01,0x0c,0x00,0x00,0x01,0x01,0x0c,0x00,0x00,0x01,
+ 0xc1,0xbe,0xf5,0x01,0x01,0xc1,0xbe,0xf7,0x03,0x01,0xc1,0x8c,0x33,0x03,0x01,
+ 0xc1,0x8c,0x31,0x07,0x01,0xc1,0x8c,0x31,0x06,0x01,0xc1,0x8c,0x31,0x07,0x01,
+ 0xc1,0x8c,0xf1,0x03,0x01,0xc1,0x8c,0xf1,0x03,0x01,0x01,0x00,0x30,0x00,0x01,
+ 0x01,0x00,0x30,0x00,0x01,0x01,0x00,0x30,0x00,0x01,0x01,0x00,0x30,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,
+ 0xff,0xff,0xff,0xff,0x01};
diff --git a/show_edit/_12943_tex2html_wrap704.png b/show_edit/_12943_tex2html_wrap704.png
new file mode 100644
index 0000000000000000000000000000000000000000..ed185e29540fd5fd196880a9746957343a8407e1
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap704.png differ
diff --git a/show_edit/_12943_tex2html_wrap704.xbm b/show_edit/_12943_tex2html_wrap704.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1359049f8f233f5ce2ea370f5b354538056f2455
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap704.xbm
@@ -0,0 +1,6 @@
+#define noname_width 15
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0x3f,0x01,0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,
+ 0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,0x40,0x01,0x40,
+ 0x01,0x40,0xff,0x7f};
diff --git a/show_edit/_12943_tex2html_wrap706.png b/show_edit/_12943_tex2html_wrap706.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap706.png differ
diff --git a/show_edit/_12943_tex2html_wrap706.xbm b/show_edit/_12943_tex2html_wrap706.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap706.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap708.png b/show_edit/_12943_tex2html_wrap708.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap708.png differ
diff --git a/show_edit/_12943_tex2html_wrap708.xbm b/show_edit/_12943_tex2html_wrap708.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap708.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap732.png b/show_edit/_12943_tex2html_wrap732.png
new file mode 100644
index 0000000000000000000000000000000000000000..18226aff5dececf2d3b06a3d358f78dbf749143f
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap732.png differ
diff --git a/show_edit/_12943_tex2html_wrap732.xbm b/show_edit/_12943_tex2html_wrap732.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5d7096d62c9e7b20adc623354d762a799f5b73cd
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap732.xbm
@@ -0,0 +1,14 @@
+#define noname_width 41
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x00,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0xc2,0x00,0x01,0xc1,0x78,0x00,0xc3,0x00,0x01,0xc1,0x7c,0x00,
+ 0xf3,0x03,0x01,0x01,0x0c,0x00,0xf1,0x03,0x01,0x01,0x0c,0x80,0xe1,0x01,0x01,
+ 0xc1,0xbe,0x85,0xf1,0x03,0x01,0xc1,0xbe,0x87,0xd0,0x03,0x01,0xc1,0x8c,0xc3,
+ 0xc0,0x00,0x01,0xc1,0x8c,0xc1,0x00,0x00,0x01,0xc1,0x8c,0x41,0x00,0x00,0x01,
+ 0xc1,0x8c,0x41,0x00,0x00,0x01,0xc1,0x8c,0x61,0x00,0x00,0x01,0xc1,0x8c,0x21,
+ 0x00,0x00,0x01,0x01,0x00,0x20,0x00,0x00,0x01,0x01,0x00,0x30,0x00,0x00,0x01,
+ 0x01,0x00,0x10,0x00,0x00,0x01,0x01,0x00,0x10,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0x00};
diff --git a/show_edit/_12943_tex2html_wrap734.png b/show_edit/_12943_tex2html_wrap734.png
new file mode 100644
index 0000000000000000000000000000000000000000..0a020a64d74d59c66012b0e5d5e28a219b45853a
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap734.png differ
diff --git a/show_edit/_12943_tex2html_wrap734.xbm b/show_edit/_12943_tex2html_wrap734.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..c81b57b894554f965ee14cfc4e1c9846493cbd87
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap734.xbm
@@ -0,0 +1,8 @@
+#define noname_width 24
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0xc1,0x78,0x80,0xc1,0x7c,0x80,0x01,0x0c,0x80,0x01,0x0c,0x80,0xc1,0xbe,0x85,
+ 0xc1,0xbe,0x87,0xc1,0x8c,0x83,0xc1,0x8c,0x81,0xc1,0x8c,0x81,0xc1,0x8c,0x81,
+ 0xc1,0x8c,0x81,0xc1,0x8c,0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0x01,0x00,0x80,0xff,0xff,0xff};
diff --git a/show_edit/_12943_tex2html_wrap736.png b/show_edit/_12943_tex2html_wrap736.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap736.png differ
diff --git a/show_edit/_12943_tex2html_wrap736.xbm b/show_edit/_12943_tex2html_wrap736.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap736.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap738.png b/show_edit/_12943_tex2html_wrap738.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap738.png differ
diff --git a/show_edit/_12943_tex2html_wrap738.xbm b/show_edit/_12943_tex2html_wrap738.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap738.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap740.png b/show_edit/_12943_tex2html_wrap740.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d4a488f7c701d1e06dca54430ff6532f8c10879
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap740.png differ
diff --git a/show_edit/_12943_tex2html_wrap740.xbm b/show_edit/_12943_tex2html_wrap740.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..97ce9f71d9fb27d104241f40e48024be85d65895
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap740.xbm
@@ -0,0 +1,14 @@
+#define noname_width 45
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x80,0x00,0x08,0x10,0xc1,0x78,0xc0,0x00,0x18,0x10,0xc1,0x7c,0x60,
+ 0xf8,0x31,0x10,0x01,0x0c,0x60,0x18,0x30,0x10,0x01,0x0c,0x30,0x18,0x60,0x10,
+ 0xc1,0xbe,0x35,0x18,0x60,0x10,0xc1,0xbe,0x37,0xf8,0x60,0x10,0xc1,0x8c,0x33,
+ 0xf8,0x61,0x10,0xc1,0x8c,0x31,0x98,0x61,0x10,0xc1,0x8c,0x31,0x80,0x61,0x10,
+ 0xc1,0x8c,0x31,0x88,0x61,0x10,0xc1,0x8c,0x31,0x8c,0x61,0x10,0xc1,0x8c,0x31,
+ 0xf8,0x60,0x10,0x01,0x00,0x30,0x70,0x60,0x10,0x01,0x00,0x60,0x00,0x30,0x10,
+ 0x01,0x00,0x60,0x00,0x30,0x10,0x01,0x00,0xc0,0x00,0x18,0x10,0x01,0x00,0x80,
+ 0x00,0x08,0x10,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x00,0x10,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/show_edit/_12943_tex2html_wrap742.png b/show_edit/_12943_tex2html_wrap742.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap742.png differ
diff --git a/show_edit/_12943_tex2html_wrap742.xbm b/show_edit/_12943_tex2html_wrap742.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap742.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap744.png b/show_edit/_12943_tex2html_wrap744.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap744.png differ
diff --git a/show_edit/_12943_tex2html_wrap744.xbm b/show_edit/_12943_tex2html_wrap744.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap744.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap756.png b/show_edit/_12943_tex2html_wrap756.png
new file mode 100644
index 0000000000000000000000000000000000000000..3f795fd1310cea4934dc739560588f67a9b95291
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap756.png differ
diff --git a/show_edit/_12943_tex2html_wrap756.xbm b/show_edit/_12943_tex2html_wrap756.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..62424a5ac02bf56f805e639ad432c9cd6858bcc8
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap756.xbm
@@ -0,0 +1,17 @@
+#define noname_width 64
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xc1,0x0c,0xc0,0x00,0x00,
+ 0x00,0x3f,0x80,0xc1,0x0c,0xc0,0x00,0x00,0x80,0x3f,0x80,0xc1,0x00,0xc0,0x00,
+ 0x00,0x80,0x31,0x80,0xc1,0x00,0xc0,0x00,0x00,0x80,0x31,0x80,0xc1,0xec,0xc3,
+ 0xcc,0x0c,0xf7,0xf7,0x81,0xc1,0xec,0xc7,0xce,0x8c,0xff,0xf7,0x83,0xc1,0x6c,
+ 0xc6,0x07,0xc0,0x8d,0x31,0x83,0xc1,0x6c,0xc6,0x03,0xc0,0x8c,0x31,0x83,0xc1,
+ 0x6c,0xc6,0x07,0x80,0x8f,0x31,0x83,0xc1,0x6c,0xc6,0x06,0xc0,0x87,0x31,0x83,
+ 0xc1,0x6c,0xc6,0xce,0xcc,0x8f,0x31,0x83,0xc1,0x6c,0xc6,0xdc,0x8c,0x9f,0x31,
+ 0x83,0x01,0x00,0x00,0x00,0xc0,0x38,0x00,0x80,0x01,0x00,0x00,0x00,0xc0,0x30,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0xc0,0x1f,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x0f,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff};
diff --git a/show_edit/_12943_tex2html_wrap758.png b/show_edit/_12943_tex2html_wrap758.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap758.png differ
diff --git a/show_edit/_12943_tex2html_wrap758.xbm b/show_edit/_12943_tex2html_wrap758.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap758.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap760.png b/show_edit/_12943_tex2html_wrap760.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap760.png differ
diff --git a/show_edit/_12943_tex2html_wrap760.xbm b/show_edit/_12943_tex2html_wrap760.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap760.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap768.png b/show_edit/_12943_tex2html_wrap768.png
new file mode 100644
index 0000000000000000000000000000000000000000..5355db230b7fe62ec4ae61e248b907d939e9ac15
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap768.png differ
diff --git a/show_edit/_12943_tex2html_wrap768.xbm b/show_edit/_12943_tex2html_wrap768.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f64a3d2075f60ae2c5fa5c1b3e4f6a70db3788ce
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap768.xbm
@@ -0,0 +1,5 @@
+#define noname_width 15
+#define noname_height 14
+static char noname_bits[] = {
+ 0xf0,0x07,0x38,0x0e,0x0c,0x18,0x1e,0x3c,0x36,0x36,0x63,0x63,0xc3,0x61,0xc3,
+ 0x61,0x63,0x63,0x36,0x36,0x1e,0x3c,0x0c,0x18,0x38,0x0e,0xf0,0x07};
diff --git a/show_edit/_12943_tex2html_wrap778.png b/show_edit/_12943_tex2html_wrap778.png
new file mode 100644
index 0000000000000000000000000000000000000000..682b2a91b3f3127da55bef77d8eef0f3a6dfdb5d
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap778.png differ
diff --git a/show_edit/_12943_tex2html_wrap778.xbm b/show_edit/_12943_tex2html_wrap778.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..47d7f270a5e3ff1dfa59da8fe7fa2b02828f9b19
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap778.xbm
@@ -0,0 +1,14 @@
+#define noname_width 56
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x80,0x81,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x81,
+ 0x01,0x00,0x80,0xc1,0x66,0xf0,0xf1,0x31,0xf3,0x87,0xc1,0xff,0xf8,0xf9,0x31,
+ 0xf3,0x87,0xc1,0xdd,0x99,0x99,0x01,0x80,0x83,0xc1,0x8c,0x8d,0x8d,0x01,0x80,
+ 0x81,0xc1,0x8c,0x8d,0x8d,0x01,0xc0,0x81,0xc1,0x8c,0x9d,0x9d,0x01,0xe0,0x80,
+ 0xc1,0x8c,0xd9,0xd9,0x31,0x73,0x80,0xc1,0x8c,0xf9,0xf9,0x31,0xf3,0x87,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff};
diff --git a/show_edit/_12943_tex2html_wrap780.png b/show_edit/_12943_tex2html_wrap780.png
new file mode 100644
index 0000000000000000000000000000000000000000..e1b238ca993c36a479f80dab4cdc383379b59d62
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap780.png differ
diff --git a/show_edit/_12943_tex2html_wrap780.xbm b/show_edit/_12943_tex2html_wrap780.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..fa37d493ec9e1fb221cd9ad78bf35e9618240884
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap780.xbm
@@ -0,0 +1,11 @@
+#define noname_width 40
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x80,0x81,0x81,
+ 0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,
+ 0xc1,0x66,0xf0,0xf1,0x81,0xc1,0xff,0xf8,0xf9,0x81,0xc1,0xdd,0x99,0x99,0x81,
+ 0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x9d,0x9d,0x81,
+ 0xc1,0x8c,0xd9,0xd9,0x81,0xc1,0x8c,0xf9,0xf9,0x81,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xff,0xff,0xff,0xff,0x7f};
diff --git a/show_edit/_12943_tex2html_wrap782.png b/show_edit/_12943_tex2html_wrap782.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap782.png differ
diff --git a/show_edit/_12943_tex2html_wrap782.xbm b/show_edit/_12943_tex2html_wrap782.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap782.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap784.png b/show_edit/_12943_tex2html_wrap784.png
new file mode 100644
index 0000000000000000000000000000000000000000..9e43cfeb013558fb30201a36c97601448de002c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap784.png differ
diff --git a/show_edit/_12943_tex2html_wrap784.xbm b/show_edit/_12943_tex2html_wrap784.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d2a9d7834a13e3012fc9fc7c8c48164192b535a8
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap784.xbm
@@ -0,0 +1,11 @@
+#define noname_width 36
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0x81,0xc3,0xf1,0x31,0x08,0xc1,0xf7,0xf3,0x33,0x08,0x61,0x36,0x33,0x33,0x08,
+ 0xe1,0x1b,0x30,0x33,0x08,0xc1,0x1f,0x30,0x33,0x08,0x01,0x3e,0x30,0x33,0x08,
+ 0x61,0x76,0x33,0x33,0x08,0xe1,0xe7,0x33,0x33,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_12943_tex2html_wrap786.png b/show_edit/_12943_tex2html_wrap786.png
new file mode 100644
index 0000000000000000000000000000000000000000..9bd026647d2af88a4beca1872b70b709377d875c
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap786.png differ
diff --git a/show_edit/_12943_tex2html_wrap786.xbm b/show_edit/_12943_tex2html_wrap786.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..36a2bf7f4246d7126219ad3f07422e992608414f
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap786.xbm
@@ -0,0 +1,10 @@
+#define noname_width 40
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x81,0xc3,0xf1,0xf1,0x81,0xc1,0xf7,0xf3,0xf3,0x83,
+ 0x61,0x36,0x33,0x33,0x83,0xe1,0x1b,0x30,0x33,0x87,0xc1,0x1f,0x30,0x33,0x86,
+ 0x01,0x3e,0x30,0x33,0x87,0x61,0x76,0x33,0xf3,0x83,0xe1,0xe7,0x33,0xf3,0x83,
+ 0x01,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x30,0x80,
+ 0x01,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0xff,0xff,0xff,0xff,0xff};
diff --git a/show_edit/_12943_tex2html_wrap788.png b/show_edit/_12943_tex2html_wrap788.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap788.png differ
diff --git a/show_edit/_12943_tex2html_wrap788.xbm b/show_edit/_12943_tex2html_wrap788.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap788.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_12943_tex2html_wrap790.png b/show_edit/_12943_tex2html_wrap790.png
new file mode 100644
index 0000000000000000000000000000000000000000..bf03084f8686ed075d485a0936c27d89d0a7a420
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap790.png differ
diff --git a/show_edit/_12943_tex2html_wrap790.xbm b/show_edit/_12943_tex2html_wrap790.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..78f0c60e344659efdf06cf968aed421c312e1bfa
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap790.xbm
@@ -0,0 +1,18 @@
+#define noname_width 78
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x3f,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x01,0x40,0x00,0x00,0x70,0x00,0x00,0x00,0x0c,0x20,
+ 0x01,0x78,0xf8,0xf9,0xf9,0x00,0x00,0x00,0x0c,0x20,0x01,0x78,0x18,0x18,0x88,
+ 0x01,0x00,0x00,0x0c,0x20,0x01,0x60,0x18,0x18,0x8c,0x01,0x00,0x00,0x0c,0x20,
+ 0x01,0x60,0x18,0x18,0x88,0x99,0xe1,0x70,0x7c,0x20,0x01,0x60,0xf8,0xf8,0x80,
+ 0x99,0xf1,0xfd,0xfc,0x20,0x01,0x60,0xf8,0xf9,0xc1,0x01,0x98,0xcd,0xcc,0x20,
+ 0x01,0x60,0x98,0x99,0xe1,0x00,0xf8,0x06,0xcc,0x20,0x01,0x60,0x80,0x81,0x61,
+ 0x00,0xf0,0x07,0xcc,0x20,0x01,0x60,0x88,0x89,0x31,0x00,0x80,0x0f,0xcc,0x20,
+ 0xc1,0x60,0x8c,0x8d,0x19,0x98,0x99,0xdd,0xcc,0x20,0xc1,0xf8,0xf9,0xf8,0xfc,
+ 0x99,0xf9,0xf9,0xcc,0x20,0x01,0x00,0x70,0x70,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x3f};
diff --git a/show_edit/_12943_tex2html_wrap792.png b/show_edit/_12943_tex2html_wrap792.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_12943_tex2html_wrap792.png differ
diff --git a/show_edit/_12943_tex2html_wrap792.xbm b/show_edit/_12943_tex2html_wrap792.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_12943_tex2html_wrap792.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tabular148.png b/show_edit/_16745_tabular148.png
new file mode 100644
index 0000000000000000000000000000000000000000..92d4acf7ccffa2b1888321b85e69cf71f2768655
Binary files /dev/null and b/show_edit/_16745_tabular148.png differ
diff --git a/show_edit/_16745_tabular148.xbm b/show_edit/_16745_tabular148.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5cc68247a964c6d703d4cfe4a932eef11054e6d9
--- /dev/null
+++ b/show_edit/_16745_tabular148.xbm
@@ -0,0 +1,231 @@
+#define noname_width 452
+#define noname_height 60
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x77,0x00,0x1c,0x00,
+ 0x00,0x00,0x70,0x00,0x00,0x00,0x00,0x0c,0x00,0xe0,0xe0,0x00,0xc0,0x01,0x70,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x0c,0x18,0x00,0x00,0x07,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x66,0x00,0x18,0x00,0x00,0x00,0x62,
+ 0x00,0x00,0x00,0x40,0x0c,0x00,0xc0,0xc0,0x00,0x80,0x01,0x78,0x00,0x00,0x00,
+ 0x00,0x21,0x00,0x08,0x18,0x00,0x10,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x63,0x00,0x00,0x00,
+ 0x60,0x00,0x00,0xc0,0xc0,0x00,0x80,0x01,0x18,0x00,0x00,0x00,0x80,0x31,0x00,
+ 0x08,0x00,0x00,0x18,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x63,0x00,0x00,0x00,0x60,0x00,0x00,
+ 0xc0,0xc0,0x00,0x80,0x01,0x18,0x00,0x00,0x00,0x80,0x31,0x00,0x08,0x00,0x00,
+ 0x18,0x06,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xfc,0x7f,0x66,
+ 0xf0,0xf9,0x7c,0xff,0x83,0xe7,0xe3,0x01,0xef,0xf7,0xee,0xf3,0xc0,0xc7,0x7c,
+ 0xbe,0x1d,0xbc,0xef,0xfb,0x1f,0xcf,0x7b,0x9e,0x0f,0xdc,0x0f,0x3c,0x3e,0x0f,
+ 0x7c,0xcf,0xff,0x78,0xe0,0xff,0xe7,0x0e,0x3c,0x1f,0x00,0x00,0x00,0x00,0x00,
+ 0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xd8,0x66,0x66,0x30,0x99,0x46,
+ 0xb6,0x01,0x63,0x32,0x83,0xd9,0x64,0xcc,0x9b,0xc1,0xcc,0x46,0xb3,0x07,0xd8,
+ 0xc8,0x33,0x33,0x9b,0x31,0xf3,0x08,0x98,0x09,0x18,0xa6,0x19,0x4c,0x9b,0x99,
+ 0xcd,0xc0,0xb6,0xcd,0x04,0x6c,0x13,0x00,0x00,0x00,0x00,0x00,0x3e,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xd8,0x63,0x66,0xf0,0x98,0xc6,0xf6,0x00,0x63,
+ 0xf2,0x83,0xdf,0x64,0xcc,0xf8,0xc1,0xc8,0xc6,0x83,0x03,0xd8,0xd8,0x30,0x33,
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+ 0xf0,0x98,0xc6,0xf6,0x00,0x63,0xf2,0x03,0x13,0xcf,0xcc,0xfe,0x07,0x78,0x26,
+ 0x23,0x60,0x63,0x63,0x66,0x3c,0xe3,0xc1,0xd8,0x00,0xcf,0x0c,0x46,0x78,0x86,
+ 0x07,0x4c,0xbf,0x8d,0x3c,0x60,0x26,0x60,0x98,0x7e,0x60,0x64,0xe3,0xc1,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0x63,0x66,0xf0,0x99,0xc6,
+ 0xfc,0x00,0x6b,0x32,0x00,0x93,0xcd,0xcc,0x86,0x0f,0x6c,0x26,0x23,0x60,0x63,
+ 0x63,0x66,0x36,0xeb,0xc3,0xd8,0x80,0xcd,0x0c,0x46,0x6c,0xd6,0x06,0x4c,0x83,
+ 0x8d,0x7c,0x60,0x26,0x60,0x99,0x06,0x60,0x64,0xe3,0xc1,0x03,0x1c,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xb0,0x63,0x66,0x10,0x99,0x46,0xec,0x00,0x6b,
+ 0x32,0x02,0xd3,0xdc,0xcc,0xc6,0x08,0xe6,0x26,0x23,0x60,0x23,0x63,0x66,0x73,
+ 0x2b,0xc2,0xc8,0xc0,0xdc,0x0c,0x46,0xe6,0x76,0x0e,0x4c,0xa3,0x8d,0x44,0x60,
+ 0x26,0x60,0x99,0x46,0x60,0x66,0xa3,0xd1,0x07,0x1c,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x30,0xf1,0xff,0xf0,0xfd,0x7d,0x4c,0x00,0xff,0xe7,0x81,0xbf,
+ 0xff,0xff,0xbd,0x0f,0xfc,0x7f,0x7e,0xf0,0xbe,0xf7,0xff,0x7e,0xef,0x83,0xef,
+ 0x81,0xff,0x1f,0xfc,0xfc,0xde,0x0f,0xee,0xde,0xfb,0x7d,0xf0,0x7f,0xe0,0xfd,
+ 0x3d,0xe0,0xf3,0x3e,0xef,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x77,0x00,0x1c,0x00,
+ 0x00,0x00,0x0e,0x00,0x00,0x00,0x00,0x60,0x00,0x0e,0x00,0x00,0x00,0x00,0x06,
+ 0x00,0x00,0x0e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x66,0x00,0x18,0x00,0x00,0x00,0x0f,
+ 0x00,0x00,0x00,0x10,0x60,0x00,0x0f,0x00,0x00,0x00,0x20,0x06,0x00,0x00,0x0f,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x30,
+ 0x00,0x00,0x00,0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x18,0x00,0x00,0x03,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x03,0x00,0x00,0x06,
+ 0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x78,0x00,0x00,0x00,0x00,0xf0,0x00,0x00,0x00,
+ 0x00,0x00,0x66,0x00,0x18,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x18,0x00,0x00,
+ 0x03,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x03,0x00,0x80,0x07,0x00,0x00,0x00,
+ 0x00,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x9c,0xff,0x8f,0xe7,0xef,0xc3,0xe1,0x00,0x00,0xfc,0x7f,0x66,
+ 0xf0,0xf9,0x7c,0xff,0x83,0xf7,0xfd,0xff,0xf1,0x3c,0x70,0xbf,0xe7,0xfb,0xff,
+ 0xe3,0x79,0xe7,0xfb,0x81,0xf7,0x7d,0xc0,0xf9,0xfb,0x79,0xfe,0x7c,0x1c,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x87,0xbf,0x8d,0x6d,0x6f,0x07,0xe7,0x00,0x00,0xd8,0x66,0x66,0x30,0x99,0x46,
+ 0xb6,0x01,0x1b,0x79,0x33,0xb3,0x19,0x60,0x26,0x33,0xf2,0x66,0x66,0x33,0x36,
+ 0x32,0x01,0x1b,0x79,0x70,0xf8,0xb3,0xd9,0xf6,0xec,0x70,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x0f,0xbf,0x8d,
+ 0x6f,0xfd,0x87,0x07,0x00,0x00,0xd8,0x63,0x66,0xf0,0x98,0xc6,0xf6,0x00,0x1b,
+ 0x1b,0x33,0xe3,0x19,0x60,0x26,0x33,0x36,0x66,0xc6,0x33,0x36,0x36,0x01,0x1b,
+ 0x1b,0xf0,0xf0,0xb3,0xf9,0xd6,0xfe,0x78,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x9c,0xbf,0xcd,0x6d,0xfd,0xc7,
+ 0x01,0x00,0x00,0xf0,0x63,0x66,0xf0,0x99,0xc6,0xfc,0x00,0x1b,0x1b,0x33,0xb3,
+ 0x59,0x60,0x26,0x33,0x36,0x66,0x66,0xb3,0x36,0x36,0x01,0x1b,0x1b,0xc0,0xf9,
+ 0xb3,0xdd,0xd6,0xfe,0x1c,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xf0,0xbf,0xcd,0x6d,0x6d,0x76,0xe0,0x00,0x00,
+ 0xb0,0x63,0x66,0x10,0x99,0x46,0xec,0x00,0x1b,0x19,0x33,0x9b,0x5b,0x60,0x26,
+ 0x33,0x32,0x66,0x36,0xb7,0x36,0x32,0x01,0x1b,0x19,0x00,0xff,0xb3,0xdd,0xd6,
+ 0xcc,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xe0,0xff,0x9f,0xff,0xef,0x33,0xe0,0x00,0x00,0x30,0xf1,0xff,
+ 0xf0,0xfd,0x7d,0x4c,0x80,0xf7,0xbd,0xff,0xf7,0x7b,0xf0,0xff,0xe7,0x7b,0xff,
+ 0xef,0xf7,0xef,0xfb,0x83,0xf7,0x3d,0x00,0xfe,0xfb,0xfb,0xff,0x7c,0x03,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/show_edit/_16745_tabular156.png b/show_edit/_16745_tabular156.png
new file mode 100644
index 0000000000000000000000000000000000000000..c5b967b5f073b3651c9ed315679fd2ca3d136d62
Binary files /dev/null and b/show_edit/_16745_tabular156.png differ
diff --git a/show_edit/_16745_tabular156.xbm b/show_edit/_16745_tabular156.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..91750ca98d8d975851a36479fa3f0d5b15add1ff
--- /dev/null
+++ b/show_edit/_16745_tabular156.xbm
@@ -0,0 +1,360 @@
+#define noname_width 432
+#define noname_height 99
+static char noname_bits[] = {
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0xe0,0x00,0x00,0x00,0x00,0x0c,0x00,0x00,0x00,0x0e,0x00,
+ 0x80,0x01,0x38,0x00,0x70,0x00,0x00,0x8c,0x01,0x80,0x03,0x00,0x40,0x00,0xc0,
+ 0x01,0x00,0xe0,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,
+ 0x00,0x00,0x00,0x36,0x00,0x00,0x20,0x0c,0x00,0x00,0x01,0x3c,0x00,0x60,0x04,
+ 0x00,0x88,0x01,0x00,0x03,0x00,0x60,0x00,0x80,0x01,0x00,0xf0,0x00,0x00,0x00,
+ 0x00,0x42,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc0,0x00,0x00,0x00,0x00,0x37,0x00,0x00,
+ 0x30,0x0c,0x00,0x00,0x01,0x0c,0x00,0x60,0x06,0x00,0x08,0x00,0x00,0x03,0x00,
+ 0x60,0x00,0x80,0x01,0x00,0x30,0x00,0x00,0x00,0x00,0x43,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xc0,0x00,0x00,0x00,0x00,0x27,0x00,0x00,0x30,0x0c,0x00,0x00,0x01,0x0c,
+ 0x00,0x60,0x06,0x00,0x08,0x00,0x00,0x03,0x00,0x20,0x00,0x80,0x01,0x00,0x30,
+ 0x00,0x00,0x00,0x00,0x43,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xbe,0xcf,0x6e,0xff,0xf3,0x03,
+ 0x30,0x03,0x00,0x78,0x7c,0x1e,0xf0,0xf1,0xde,0x73,0x63,0x0f,0x80,0xcf,0xfd,
+ 0x1f,0xf3,0xdc,0x31,0x77,0x8f,0xdd,0x3c,0x78,0xbe,0xff,0x3f,0x9e,0xe7,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0xf3,0xc8,0x4c,0x66,0x66,0x02,0x30,0x03,0x00,0x30,0x4c,0x33,
+ 0x18,0x99,0xcd,0x66,0x62,0x06,0xc0,0x88,0x4d,0x33,0xb3,0x99,0x10,0x26,0x9b,
+ 0x99,0x66,0x30,0x23,0x6f,0x66,0x36,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xc3,0xd8,0x4c,
+ 0x66,0x66,0x02,0x18,0x00,0x00,0x30,0x4c,0x3f,0x18,0xf9,0x8d,0x67,0x62,0x06,
+ 0xc0,0x88,0x3d,0x23,0xe3,0xd9,0x10,0x36,0x9e,0x99,0x7e,0x30,0x63,0x63,0x66,
+ 0x3c,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0xc3,0xd8,0x4c,0x66,0x66,0x02,0x2c,0x00,0x00,
+ 0xb0,0x4c,0x03,0x18,0x19,0xcc,0x66,0x62,0x16,0xc0,0x88,0x7d,0x23,0xb3,0x71,
+ 0x18,0x1c,0x9b,0x99,0x06,0x30,0x63,0x63,0x66,0x36,0x0b,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0xe3,0xc8,0x6c,0x66,0x66,0x02,0x26,0x03,0x00,0xb0,0x4c,0x23,0x18,0x19,0x6d,
+ 0x6e,0x63,0x16,0xc0,0x88,0x45,0x33,0x9b,0x73,0x08,0x9c,0xb9,0xd9,0x46,0x30,
+ 0x23,0x63,0x66,0x73,0x0b,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x9e,0xef,0xfd,0xff,0xff,0x07,
+ 0x3f,0x03,0x00,0xf0,0xfe,0x1e,0xf0,0xf3,0xde,0xef,0xf7,0x1e,0x80,0xdf,0x7f,
+ 0x9f,0xf7,0x23,0x0c,0x08,0xff,0xfb,0x3d,0x78,0xbe,0xf7,0xff,0x7e,0x0f,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x20,0x0c,0x00,0x00,
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+ 0xc0,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x00,0x00,0x00,0xc0,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x38,0x00,0x20,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x1e,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x02,0x00,
+ 0x00,0x00,0x30,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x30,0x00,0x40,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x06,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x03,0x00,0x00,0x00,0x30,0x00,0xc0,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xef,0xfb,0xc0,0x03,0xfc,0x8f,0xe7,0x7b,0xfc,0xc7,0xfb,0xe0,0xee,0xb1,
+ 0x9b,0xc7,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0xf2,0xc0,0x06,0xe6,
+ 0x89,0xcd,0xdb,0x66,0x63,0xf6,0xc0,0x64,0x33,0xd3,0xcc,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x36,0x36,0x80,0x07,0x86,0x09,0xcf,0xf0,0x06,0xe3,0x37,
+ 0xc0,0xc6,0x33,0xd3,0xcf,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x36,
+ 0xc0,0x06,0x86,0x89,0xcd,0xd8,0x06,0x6b,0x30,0x80,0x63,0x33,0xd3,0xc0,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x32,0x60,0x0e,0xc6,0xc9,0xdc,0xcc,
+ 0x47,0x6b,0x34,0x80,0x33,0x37,0xdb,0xc8,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0xef,0x7b,0xc0,0x0f,0xfc,0x9f,0xff,0xf9,0x3d,0xcf,0x7b,0x00,0xe1,0x7f,
+ 0xbf,0xc7,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x40,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x30,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/show_edit/_16745_tex2html_wrap645.png b/show_edit/_16745_tex2html_wrap645.png
new file mode 100644
index 0000000000000000000000000000000000000000..eee8382ab30aacea79d9840bec39b9209823c74b
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap645.png differ
diff --git a/show_edit/_16745_tex2html_wrap645.xbm b/show_edit/_16745_tex2html_wrap645.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..53dd760651d68c894e110b4aa9dd62c070654add
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap645.xbm
@@ -0,0 +1,11 @@
+#define noname_width 36
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0xc1,0xe2,0x18,0x3e,0x08,0xc1,0xf3,0x19,0x3f,0x08,0xc1,0x91,0x03,0x33,0x08,
+ 0xc1,0xc0,0x83,0x31,0x08,0xc1,0xf0,0x83,0x31,0x08,0xc1,0x38,0x83,0x33,0x08,
+ 0xc1,0xb8,0x1b,0x3b,0x08,0xc1,0xf0,0x1b,0x3f,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap653.png b/show_edit/_16745_tex2html_wrap653.png
new file mode 100644
index 0000000000000000000000000000000000000000..d1c0cfd72f6c12eb214a3a7d444b4f29e741305b
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap653.png differ
diff --git a/show_edit/_16745_tex2html_wrap653.xbm b/show_edit/_16745_tex2html_wrap653.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..f0cc194963bb834c681561934c09a5fcf849252e
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap653.xbm
@@ -0,0 +1,14 @@
+#define noname_width 50
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x30,0x03,0x3c,0x02,0x01,0x00,0x00,
+ 0x30,0x03,0x3e,0x02,0x01,0x00,0x00,0x30,0x03,0x06,0x02,0x01,0x00,0x00,0x30,
+ 0x03,0x06,0x02,0xc1,0xe2,0x18,0x3e,0x1f,0x1f,0x02,0xc1,0xf3,0x19,0x3f,0x3f,
+ 0x1f,0x02,0xc1,0x91,0x03,0x33,0x33,0x06,0x02,0xc1,0xc0,0x83,0x31,0x33,0x06,
+ 0x02,0xc1,0xf0,0x83,0x31,0x33,0x06,0x02,0xc1,0x38,0x83,0x33,0x33,0x06,0x02,
+ 0xc1,0xb8,0x1b,0x3b,0x33,0x06,0x02,0xc1,0xf0,0x1b,0x3f,0x33,0x06,0x02,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x02,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0x01};
diff --git a/show_edit/_16745_tex2html_wrap655.png b/show_edit/_16745_tex2html_wrap655.png
new file mode 100644
index 0000000000000000000000000000000000000000..b38e14ac2d1fd150b96e9fc60e6ac449b8fd5964
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap655.png differ
diff --git a/show_edit/_16745_tex2html_wrap655.xbm b/show_edit/_16745_tex2html_wrap655.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..259ae68bc7f6fe8b8ff51e3a90fdc3d393511555
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap655.xbm
@@ -0,0 +1,17 @@
+#define noname_width 66
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x03,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x01,0x00,0x00,0x30,0x03,0x3c,0x02,0x03,0x02,0x01,0x00,0x00,0x30,0x03,0xfe,
+ 0xc3,0x07,0x02,0x01,0x00,0x00,0x30,0x03,0xc6,0xc3,0x0c,0x02,0x01,0x00,0x00,
+ 0x30,0x03,0x06,0xc3,0x0c,0x02,0xc1,0xe2,0x18,0x3e,0x1f,0x1f,0x63,0x0c,0x02,
+ 0xc1,0xf3,0x19,0x3f,0x3f,0x1f,0x63,0x0c,0x02,0xc1,0x91,0x03,0x33,0x33,0x06,
+ 0x63,0x0c,0x02,0xc1,0xc0,0x83,0x31,0x33,0x06,0x63,0x0c,0x02,0xc1,0xf0,0x83,
+ 0x31,0x33,0x06,0x63,0x0c,0x02,0xc1,0x38,0x83,0x33,0x33,0x06,0xc3,0x0c,0x02,
+ 0xc1,0xb8,0x1b,0x3b,0x33,0x06,0xc3,0x0c,0x02,0xc1,0xf0,0x1b,0x3f,0x33,0xc6,
+ 0xcf,0x07,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap657.png b/show_edit/_16745_tex2html_wrap657.png
new file mode 100644
index 0000000000000000000000000000000000000000..92eeae146caa5cd642f6c9d5a8cdad4681035824
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap657.png differ
diff --git a/show_edit/_16745_tex2html_wrap657.xbm b/show_edit/_16745_tex2html_wrap657.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..877def0e9b074fdad7247f696385b0fcbb641c61
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap657.xbm
@@ -0,0 +1,12 @@
+#define noname_width 40
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x80,0x81,
+ 0x01,0x00,0x00,0x80,0x81,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xc1,0xe2,0x98,0xb1,0x81,0xc1,0xf3,0x99,0xbb,0x81,0xc1,0x91,0x03,0x9f,0x81,
+ 0xc1,0xc0,0x03,0x8e,0x81,0xc1,0xf0,0x03,0x8e,0x81,0xc1,0x38,0x03,0x9f,0x81,
+ 0xc1,0xb8,0x1b,0x9b,0x81,0xc1,0xf0,0x9b,0xb1,0x81,0x01,0x00,0x00,0x80,0x81,
+ 0x01,0x00,0x00,0xa0,0x81,0x01,0x00,0x00,0xe0,0x81,0x01,0x00,0x00,0xc0,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xff,0xff,0xff,0xff,0x7f};
diff --git a/show_edit/_16745_tex2html_wrap661.png b/show_edit/_16745_tex2html_wrap661.png
new file mode 100644
index 0000000000000000000000000000000000000000..ed185e29540fd5fd196880a9746957343a8407e1
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap661.png differ
diff --git a/show_edit/_16745_tex2html_wrap661.xbm b/show_edit/_16745_tex2html_wrap661.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1359049f8f233f5ce2ea370f5b354538056f2455
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap661.xbm
@@ -0,0 +1,6 @@
+#define noname_width 15
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0x3f,0x01,0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,
+ 0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,0x40,0x01,0x40,
+ 0x01,0x40,0xff,0x7f};
diff --git a/show_edit/_16745_tex2html_wrap675.png b/show_edit/_16745_tex2html_wrap675.png
new file mode 100644
index 0000000000000000000000000000000000000000..73b6f35d418e28ed15289285fda23be364232f3f
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap675.png differ
diff --git a/show_edit/_16745_tex2html_wrap675.xbm b/show_edit/_16745_tex2html_wrap675.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d7a915fe4c61a8115645720ff5a31f5c65d735a3
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap675.xbm
@@ -0,0 +1,18 @@
+#define noname_width 67
+#define noname_height 24
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0xc1,0x9f,0xff,0xf9,0x03,0x10,0x1c,0x00,0x04,0xc1,0xbf,0xff,0xf9,0x07,0x1e,
+ 0x3e,0x00,0x04,0xc1,0x30,0x18,0x18,0x06,0x1e,0x62,0x00,0x04,0xc1,0x30,0x18,
+ 0x18,0x06,0x18,0x63,0x00,0x04,0xc1,0x30,0x18,0x18,0x06,0x18,0x62,0x00,0x04,
+ 0xc1,0x3f,0x18,0x18,0x07,0x18,0x60,0x00,0x04,0xc1,0x1f,0x18,0xf8,0x03,0x18,
+ 0x70,0x00,0x04,0xc1,0x1c,0x18,0x18,0x00,0x18,0x38,0x00,0x04,0xc1,0x18,0x18,
+ 0x18,0x00,0x18,0x18,0x00,0x04,0xc1,0x38,0x18,0x18,0x00,0x18,0x0c,0x00,0x04,
+ 0xc1,0x30,0x18,0x18,0x30,0x18,0x06,0x00,0x04,0xc1,0x60,0x18,0x18,0x30,0x7e,
+ 0x7f,0x00,0x04,0x01,0x00,0x00,0x00,0x20,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x30,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/show_edit/_16745_tex2html_wrap677.png b/show_edit/_16745_tex2html_wrap677.png
new file mode 100644
index 0000000000000000000000000000000000000000..2580cc5c8a2d7bea3589bf97a5c5a93560570e65
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap677.png differ
diff --git a/show_edit/_16745_tex2html_wrap677.xbm b/show_edit/_16745_tex2html_wrap677.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..29d52c8bf1ef718c716ee3e66832357daed4b0a1
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap677.xbm
@@ -0,0 +1,36 @@
+#define noname_width 139
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0x07,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x20,0x00,0x01,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x00,0x30,0x0e,0x03,0x18,0x07,0x00,0x10,0x00,0x70,
+ 0x00,0xc0,0x01,0x00,0x00,0x04,0x01,0x00,0x00,0x18,0x1f,0x06,0x98,0x0f,0x00,
+ 0x1e,0x00,0xf8,0x00,0xe0,0x03,0x00,0x0e,0x04,0x01,0x30,0x00,0x18,0x31,0x06,
+ 0x88,0x18,0x00,0x1e,0x00,0x88,0x01,0x60,0x06,0x00,0x0e,0x04,0x01,0x30,0x00,
+ 0x8c,0x31,0x0c,0xcc,0x18,0x00,0x18,0x00,0x8c,0x01,0x20,0x06,0x00,0x0f,0x04,
+ 0xc1,0xfa,0x7c,0x0c,0x31,0x0c,0x8c,0x18,0x00,0x18,0x00,0x88,0x01,0x00,0x06,
+ 0x00,0x0f,0x04,0xc1,0xfb,0xfc,0x0c,0x30,0x0c,0x04,0x18,0x00,0x18,0x00,0x80,
+ 0x01,0xc0,0x03,0x80,0x0d,0x04,0xc1,0x31,0xcc,0x0c,0x38,0x0c,0x06,0x1c,0x00,
+ 0x18,0x00,0xc0,0x01,0xc0,0x03,0x80,0x0d,0x04,0xc1,0x30,0xcc,0x0d,0x1c,0x0c,
+ 0x06,0x0e,0x00,0x18,0x00,0xe0,0x00,0x00,0x06,0xc0,0x0c,0x04,0xc1,0x30,0x8c,
+ 0x0d,0x0c,0x0c,0x02,0x06,0x00,0x18,0x00,0x60,0x00,0x00,0x06,0xc0,0x3f,0x04,
+ 0xc1,0x30,0xcc,0x0d,0x06,0x0c,0x02,0x03,0x00,0x18,0x00,0x30,0x00,0x10,0x06,
+ 0x00,0x0c,0x04,0xc1,0xb0,0xfc,0x0c,0x03,0x0c,0x83,0x81,0x01,0x18,0x06,0x18,
+ 0x18,0x30,0x66,0x00,0x0c,0x04,0xc1,0xf0,0xfc,0x8c,0x3f,0x0c,0xc1,0x9f,0x01,
+ 0x7e,0x06,0xfc,0x19,0xe0,0x67,0x00,0x0c,0x04,0x01,0x00,0x0c,0x0c,0x00,0x0c,
+ 0x01,0x00,0x01,0x00,0x04,0x00,0x10,0xc0,0x41,0x00,0x00,0x04,0x01,0x00,0x0c,
+ 0x18,0x00,0x86,0x01,0x80,0x01,0x00,0x06,0x00,0x18,0x00,0x60,0x00,0x00,0x04,
+ 0x01,0x00,0x0c,0x18,0x00,0x86,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0x01,0x00,0x0c,0x30,0x00,0x83,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x20,0x00,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x04,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x04,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x07};
diff --git a/show_edit/_16745_tex2html_wrap679.png b/show_edit/_16745_tex2html_wrap679.png
new file mode 100644
index 0000000000000000000000000000000000000000..baa61fcdf646ffcd2a65618785a151c005cd5d4a
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap679.png differ
diff --git a/show_edit/_16745_tex2html_wrap679.xbm b/show_edit/_16745_tex2html_wrap679.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..226a615054661f0c5adfb2b4e7a51692a76f018d
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap679.xbm
@@ -0,0 +1,13 @@
+#define noname_width 48
+#define noname_height 24
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0xc0,0x80,
+ 0x01,0x00,0x00,0x00,0xf0,0x81,0x01,0x30,0x00,0x00,0x30,0x83,0x01,0x30,0x00,
+ 0x00,0x30,0x83,0xc1,0xfa,0x7c,0x00,0x18,0x83,0xc1,0xfb,0xfc,0x00,0x18,0x83,
+ 0xc1,0x31,0xcc,0x00,0x18,0x83,0xc1,0x30,0xcc,0x01,0x18,0x83,0xc1,0x30,0x8c,
+ 0x01,0x18,0x83,0xc1,0x30,0xcc,0x01,0x30,0x83,0xc1,0xb0,0xfc,0x0c,0x30,0x83,
+ 0xc1,0xf0,0xfc,0x0c,0xf0,0x81,0x01,0x00,0x0c,0x08,0xc0,0x80,0x01,0x00,0x0c,
+ 0x0c,0x00,0x80,0x01,0x00,0x0c,0x00,0x00,0x80,0x01,0x00,0x0c,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,
+ 0x00,0x00,0x80,0xff,0xff,0xff,0xff,0xff,0xff};
diff --git a/show_edit/_16745_tex2html_wrap681.png b/show_edit/_16745_tex2html_wrap681.png
new file mode 100644
index 0000000000000000000000000000000000000000..b58716d48ea7c2416e44eff5cf0991a9b9a3fbec
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap681.png differ
diff --git a/show_edit/_16745_tex2html_wrap681.xbm b/show_edit/_16745_tex2html_wrap681.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..7502ad49eaefdb671e56270d9ae344cfb60a1241
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap681.xbm
@@ -0,0 +1,48 @@
+#define noname_width 193
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x20,0x00,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x30,0x0e,0x03,0x00,0x0e,0x0c,0x00,0x80,0x81,0xc1,0x01,0x00,
+ 0x00,0x00,0x0e,0x08,0xc0,0x00,0x00,0xc0,0x01,0x01,0x01,0x00,0x00,0x18,0x1f,
+ 0x06,0x00,0x1f,0x9f,0x3f,0xe0,0xe3,0xe3,0xf3,0x07,0x00,0x1c,0x1f,0x0f,0xf0,
+ 0xf9,0xf3,0xe3,0x01,0x01,0x01,0x30,0x00,0x18,0x31,0x06,0x00,0x31,0x33,0x30,
+ 0x60,0x66,0x66,0x06,0x06,0x00,0x1c,0x33,0x0f,0x30,0x03,0x33,0x70,0x00,0x01,
+ 0x01,0x30,0x00,0x8c,0x31,0x0c,0x80,0x31,0x33,0x38,0x70,0x66,0x26,0x06,0x07,
+ 0x00,0x1e,0x31,0x0c,0x38,0x83,0x33,0x30,0x00,0x01,0xc1,0xfa,0x7c,0x0c,0x31,
+ 0x0c,0x00,0x31,0x33,0x18,0x30,0x66,0x06,0x06,0x03,0x00,0x1e,0x30,0x0c,0x18,
+ 0x83,0x31,0xf8,0x01,0x01,0xc1,0xfb,0xfc,0x0c,0x30,0x0c,0x00,0x30,0x1f,0x0c,
+ 0x30,0xe6,0xc3,0x83,0x01,0x00,0x1b,0x1e,0x0c,0x18,0xc3,0xf0,0xf9,0x03,0x01,
+ 0xc1,0x31,0xcc,0x0c,0x38,0x0c,0x00,0x38,0x1f,0x0c,0x60,0xe6,0xc3,0x83,0x01,
+ 0x00,0x1b,0x1e,0x0c,0x30,0xc3,0xf0,0x3b,0x03,0x01,0xc1,0x30,0xcc,0x0d,0x1c,
+ 0x0c,0x00,0x1c,0x33,0x0c,0xe0,0x67,0x06,0x86,0x01,0x80,0x19,0x30,0x0c,0xf0,
+ 0xc3,0x30,0x1b,0x03,0x01,0xc1,0x30,0x8c,0x0d,0x0c,0x0c,0x00,0x8c,0x31,0x06,
+ 0xc0,0x37,0x06,0xc6,0x00,0x80,0x7f,0x30,0x0c,0xe0,0x63,0x00,0x1b,0x03,0x01,
+ 0xc1,0x30,0xcc,0x0d,0x06,0x0c,0x00,0x86,0x31,0x06,0x00,0x36,0x16,0xc6,0x00,
+ 0x00,0x98,0x30,0x0c,0x00,0x63,0x10,0x33,0x03,0x01,0xc1,0xb0,0xfc,0x0c,0x03,
+ 0x8c,0x01,0x03,0x33,0x06,0x23,0x63,0x36,0xc6,0x60,0x00,0x98,0x31,0x0c,0x93,
+ 0x61,0x18,0x33,0x03,0x01,0xc1,0xf0,0xfc,0x8c,0x3f,0x8c,0x81,0x3f,0x3f,0x06,
+ 0xe3,0xe3,0xe7,0xc7,0x60,0x00,0x18,0x3f,0x3f,0xf3,0x61,0xf0,0xf1,0x01,0x01,
+ 0x01,0x00,0x0c,0x0c,0x00,0x0c,0x01,0x00,0x0c,0x00,0xc0,0x80,0xc1,0x01,0x40,
+ 0x00,0x00,0x0e,0x00,0x60,0x00,0xe0,0xc0,0x00,0x01,0x01,0x00,0x0c,0x18,0x00,
+ 0x86,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x60,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x0c,0x18,0x00,0x06,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x0c,0x30,0x00,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x20,0x00,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01};
diff --git a/show_edit/_16745_tex2html_wrap683.png b/show_edit/_16745_tex2html_wrap683.png
new file mode 100644
index 0000000000000000000000000000000000000000..faaf3882388ce6577c279ec9fd833e46371df903
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap683.png differ
diff --git a/show_edit/_16745_tex2html_wrap683.xbm b/show_edit/_16745_tex2html_wrap683.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..3680b125e37685db678b2ab002d4b63ab89f7f83
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap683.xbm
@@ -0,0 +1,16 @@
+#define noname_width 60
+#define noname_height 24
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0xc1,0x0c,0xc0,0x00,0x00,
+ 0x08,0x0e,0x08,0xc1,0x0c,0xc0,0x00,0x00,0x0f,0x1f,0x08,0xc1,0x00,0xc0,0x00,
+ 0x00,0x0f,0x31,0x08,0xc1,0x00,0xc0,0x00,0x00,0x8c,0x31,0x08,0xc1,0xec,0xc3,
+ 0x0c,0x00,0x0c,0x31,0x08,0xc1,0xec,0xc7,0x0e,0x00,0x0c,0x30,0x08,0xc1,0x6c,
+ 0xc6,0x07,0x00,0x0c,0x38,0x08,0xc1,0x6c,0xc6,0x03,0x00,0x0c,0x1c,0x08,0xc1,
+ 0x6c,0xc6,0x07,0x00,0x0c,0x0c,0x08,0xc1,0x6c,0xc6,0x06,0x00,0x0c,0x06,0x08,
+ 0xc1,0x6c,0xc6,0xce,0x00,0x0c,0x03,0x08,0xc1,0x6c,0xc6,0xdc,0x00,0xbf,0x3f,
+ 0x08,0x01,0x00,0x00,0x80,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0xc0,0x00,0x00,
+ 0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap685.png b/show_edit/_16745_tex2html_wrap685.png
new file mode 100644
index 0000000000000000000000000000000000000000..ddeaf91bbbdd2367d805dafba8cd02462bc31cde
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap685.png differ
diff --git a/show_edit/_16745_tex2html_wrap685.xbm b/show_edit/_16745_tex2html_wrap685.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..e8dee20978b0c8d32115edfd88a929d62b77fea6
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap685.xbm
@@ -0,0 +1,27 @@
+#define noname_width 98
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x03,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x02,0x10,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0xc1,0x0c,0xc0,0x00,0x83,0x30,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x02,0xc1,0x0c,0xc0,0x80,0xf1,0x60,0x00,0x00,0x00,0x00,0xc0,0x03,0x02,0xc1,
+ 0x00,0xc0,0x80,0xf1,0x60,0x00,0x00,0x00,0x00,0xc0,0x03,0x02,0xc1,0x00,0xc0,
+ 0xc0,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,0x03,0x02,0xc1,0xec,0xc3,0xcc,0xc0,
+ 0xc0,0x00,0x00,0x00,0x00,0x00,0x03,0x02,0xc1,0xec,0xc7,0xce,0xc0,0xc0,0x00,
+ 0x00,0x00,0x00,0x00,0x03,0x02,0xc1,0x6c,0xc6,0xc7,0xc0,0xc0,0xfc,0x9f,0xff,
+ 0x03,0x00,0x03,0x02,0xc1,0x6c,0xc6,0xc3,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,
+ 0x03,0x02,0xc1,0x6c,0xc6,0xc7,0xc0,0xc0,0x00,0x00,0x00,0x00,0x00,0x03,0x02,
+ 0xc1,0x6c,0xc6,0xc6,0xc0,0xc0,0xfc,0x9f,0xff,0x03,0x00,0x03,0x02,0xc1,0x6c,
+ 0xc6,0xce,0xc0,0xc0,0x00,0x00,0x00,0x30,0x00,0x03,0x02,0xc1,0x6c,0xc6,0xdc,
+ 0xf0,0xc3,0x00,0x00,0x00,0x30,0xc0,0x0f,0x02,0x01,0x00,0x00,0xc0,0x00,0xc0,
+ 0x00,0x00,0x00,0x20,0x00,0x00,0x02,0x01,0x00,0x00,0x80,0x01,0x60,0x00,0x00,
+ 0x00,0x30,0x00,0x00,0x02,0x01,0x00,0x00,0x80,0x01,0x60,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x03,0x30,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x02,0x01,0x00,0x00,0x00,0x02,0x10,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap689.png b/show_edit/_16745_tex2html_wrap689.png
new file mode 100644
index 0000000000000000000000000000000000000000..cdebbaa352d35561f7ba1efadbee4ba498746351
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap689.png differ
diff --git a/show_edit/_16745_tex2html_wrap689.xbm b/show_edit/_16745_tex2html_wrap689.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2b52bdda40d94c0ad090d810ea0079711b61b981
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap689.xbm
@@ -0,0 +1,7 @@
+#define noname_width 19
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0xff,0x07,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0xc1,0x18,0x04,
+ 0xc1,0x18,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,
+ 0xc1,0x18,0x04,0xc1,0x18,0x04,0x01,0x00,0x04,0x01,0x00,0x04,0x01,0x00,0x04,
+ 0x01,0x00,0x04,0xff,0xff,0x07};
diff --git a/show_edit/_16745_tex2html_wrap707.png b/show_edit/_16745_tex2html_wrap707.png
new file mode 100644
index 0000000000000000000000000000000000000000..e1b238ca993c36a479f80dab4cdc383379b59d62
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap707.png differ
diff --git a/show_edit/_16745_tex2html_wrap707.xbm b/show_edit/_16745_tex2html_wrap707.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..fa37d493ec9e1fb221cd9ad78bf35e9618240884
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap707.xbm
@@ -0,0 +1,11 @@
+#define noname_width 40
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x80,0x81,0x81,
+ 0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,
+ 0xc1,0x66,0xf0,0xf1,0x81,0xc1,0xff,0xf8,0xf9,0x81,0xc1,0xdd,0x99,0x99,0x81,
+ 0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x9d,0x9d,0x81,
+ 0xc1,0x8c,0xd9,0xd9,0x81,0xc1,0x8c,0xf9,0xf9,0x81,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xff,0xff,0xff,0xff,0x7f};
diff --git a/show_edit/_16745_tex2html_wrap709.png b/show_edit/_16745_tex2html_wrap709.png
new file mode 100644
index 0000000000000000000000000000000000000000..468b2e90f640926dcd5c1aaffe0476d0f3021253
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap709.png differ
diff --git a/show_edit/_16745_tex2html_wrap709.xbm b/show_edit/_16745_tex2html_wrap709.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..bba48f6f3a89d59912db72eea5e285f0b91fd3d6
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap709.xbm
@@ -0,0 +1,12 @@
+#define noname_width 37
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,0xc1,0x78,0x00,0x00,0x10,
+ 0xc1,0x7c,0x00,0x00,0x10,0x01,0x0c,0x00,0x00,0x10,0x01,0x0c,0x00,0x00,0x10,
+ 0xc1,0xbe,0xf5,0x61,0x10,0xc1,0xbe,0xf7,0x63,0x10,0xc1,0x8c,0x33,0x03,0x10,
+ 0xc1,0x8c,0x31,0x07,0x10,0xc1,0x8c,0x31,0x06,0x10,0xc1,0x8c,0x31,0x07,0x10,
+ 0xc1,0x8c,0xf1,0x63,0x10,0xc1,0x8c,0xf1,0x63,0x10,0x01,0x00,0x30,0x00,0x10,
+ 0x01,0x00,0x30,0x00,0x10,0x01,0x00,0x30,0x00,0x10,0x01,0x00,0x30,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x10,
+ 0xff,0xff,0xff,0xff,0x1f};
diff --git a/show_edit/_16745_tex2html_wrap711.png b/show_edit/_16745_tex2html_wrap711.png
new file mode 100644
index 0000000000000000000000000000000000000000..10049a8814da47be3becbbb3b6d55802788d43d7
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap711.png differ
diff --git a/show_edit/_16745_tex2html_wrap711.xbm b/show_edit/_16745_tex2html_wrap711.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d6498696c82402c428d0c3cf28577a0fdb9b9394
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap711.xbm
@@ -0,0 +1,12 @@
+#define noname_width 33
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x01,0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,0xc1,0x78,0x00,0x00,0x01,
+ 0xc1,0x7c,0x00,0x00,0x01,0x01,0x0c,0x00,0x00,0x01,0x01,0x0c,0x00,0x00,0x01,
+ 0xc1,0xbe,0xf5,0x01,0x01,0xc1,0xbe,0xf7,0x03,0x01,0xc1,0x8c,0x33,0x03,0x01,
+ 0xc1,0x8c,0x31,0x07,0x01,0xc1,0x8c,0x31,0x06,0x01,0xc1,0x8c,0x31,0x07,0x01,
+ 0xc1,0x8c,0xf1,0x03,0x01,0xc1,0x8c,0xf1,0x03,0x01,0x01,0x00,0x30,0x00,0x01,
+ 0x01,0x00,0x30,0x00,0x01,0x01,0x00,0x30,0x00,0x01,0x01,0x00,0x30,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x01,
+ 0xff,0xff,0xff,0xff,0x01};
diff --git a/show_edit/_16745_tex2html_wrap713.png b/show_edit/_16745_tex2html_wrap713.png
new file mode 100644
index 0000000000000000000000000000000000000000..ed185e29540fd5fd196880a9746957343a8407e1
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap713.png differ
diff --git a/show_edit/_16745_tex2html_wrap713.xbm b/show_edit/_16745_tex2html_wrap713.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..1359049f8f233f5ce2ea370f5b354538056f2455
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap713.xbm
@@ -0,0 +1,6 @@
+#define noname_width 15
+#define noname_height 17
+static char noname_bits[] = {
+ 0xff,0x3f,0x01,0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,
+ 0x40,0x01,0x40,0x01,0x40,0xc1,0x40,0xc1,0x40,0x01,0x40,0x01,0x40,0x01,0x40,
+ 0x01,0x40,0xff,0x7f};
diff --git a/show_edit/_16745_tex2html_wrap715.png b/show_edit/_16745_tex2html_wrap715.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap715.png differ
diff --git a/show_edit/_16745_tex2html_wrap715.xbm b/show_edit/_16745_tex2html_wrap715.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap715.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap717.png b/show_edit/_16745_tex2html_wrap717.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap717.png differ
diff --git a/show_edit/_16745_tex2html_wrap717.xbm b/show_edit/_16745_tex2html_wrap717.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap717.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap741.png b/show_edit/_16745_tex2html_wrap741.png
new file mode 100644
index 0000000000000000000000000000000000000000..18226aff5dececf2d3b06a3d358f78dbf749143f
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap741.png differ
diff --git a/show_edit/_16745_tex2html_wrap741.xbm b/show_edit/_16745_tex2html_wrap741.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..5d7096d62c9e7b20adc623354d762a799f5b73cd
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap741.xbm
@@ -0,0 +1,14 @@
+#define noname_width 41
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x00,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0xc2,0x00,0x01,0xc1,0x78,0x00,0xc3,0x00,0x01,0xc1,0x7c,0x00,
+ 0xf3,0x03,0x01,0x01,0x0c,0x00,0xf1,0x03,0x01,0x01,0x0c,0x80,0xe1,0x01,0x01,
+ 0xc1,0xbe,0x85,0xf1,0x03,0x01,0xc1,0xbe,0x87,0xd0,0x03,0x01,0xc1,0x8c,0xc3,
+ 0xc0,0x00,0x01,0xc1,0x8c,0xc1,0x00,0x00,0x01,0xc1,0x8c,0x41,0x00,0x00,0x01,
+ 0xc1,0x8c,0x41,0x00,0x00,0x01,0xc1,0x8c,0x61,0x00,0x00,0x01,0xc1,0x8c,0x21,
+ 0x00,0x00,0x01,0x01,0x00,0x20,0x00,0x00,0x01,0x01,0x00,0x30,0x00,0x00,0x01,
+ 0x01,0x00,0x10,0x00,0x00,0x01,0x01,0x00,0x10,0x00,0x00,0x01,0x01,0x00,0x00,
+ 0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,0x01,0x00,0x00,0x00,0x00,0x01,
+ 0x01,0x00,0x00,0x00,0x00,0x01,0xff,0xff,0xff,0xff,0xff,0x00};
diff --git a/show_edit/_16745_tex2html_wrap743.png b/show_edit/_16745_tex2html_wrap743.png
new file mode 100644
index 0000000000000000000000000000000000000000..0a020a64d74d59c66012b0e5d5e28a219b45853a
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap743.png differ
diff --git a/show_edit/_16745_tex2html_wrap743.xbm b/show_edit/_16745_tex2html_wrap743.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..c81b57b894554f965ee14cfc4e1c9846493cbd87
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap743.xbm
@@ -0,0 +1,8 @@
+#define noname_width 24
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0xc1,0x78,0x80,0xc1,0x7c,0x80,0x01,0x0c,0x80,0x01,0x0c,0x80,0xc1,0xbe,0x85,
+ 0xc1,0xbe,0x87,0xc1,0x8c,0x83,0xc1,0x8c,0x81,0xc1,0x8c,0x81,0xc1,0x8c,0x81,
+ 0xc1,0x8c,0x81,0xc1,0x8c,0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0x01,0x00,0x80,0xff,0xff,0xff};
diff --git a/show_edit/_16745_tex2html_wrap745.png b/show_edit/_16745_tex2html_wrap745.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap745.png differ
diff --git a/show_edit/_16745_tex2html_wrap745.xbm b/show_edit/_16745_tex2html_wrap745.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap745.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap747.png b/show_edit/_16745_tex2html_wrap747.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap747.png differ
diff --git a/show_edit/_16745_tex2html_wrap747.xbm b/show_edit/_16745_tex2html_wrap747.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap747.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap749.png b/show_edit/_16745_tex2html_wrap749.png
new file mode 100644
index 0000000000000000000000000000000000000000..4d4a488f7c701d1e06dca54430ff6532f8c10879
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap749.png differ
diff --git a/show_edit/_16745_tex2html_wrap749.xbm b/show_edit/_16745_tex2html_wrap749.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..97ce9f71d9fb27d104241f40e48024be85d65895
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap749.xbm
@@ -0,0 +1,14 @@
+#define noname_width 45
+#define noname_height 27
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x1f,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,
+ 0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x80,0x00,0x08,0x10,0xc1,0x78,0xc0,0x00,0x18,0x10,0xc1,0x7c,0x60,
+ 0xf8,0x31,0x10,0x01,0x0c,0x60,0x18,0x30,0x10,0x01,0x0c,0x30,0x18,0x60,0x10,
+ 0xc1,0xbe,0x35,0x18,0x60,0x10,0xc1,0xbe,0x37,0xf8,0x60,0x10,0xc1,0x8c,0x33,
+ 0xf8,0x61,0x10,0xc1,0x8c,0x31,0x98,0x61,0x10,0xc1,0x8c,0x31,0x80,0x61,0x10,
+ 0xc1,0x8c,0x31,0x88,0x61,0x10,0xc1,0x8c,0x31,0x8c,0x61,0x10,0xc1,0x8c,0x31,
+ 0xf8,0x60,0x10,0x01,0x00,0x30,0x70,0x60,0x10,0x01,0x00,0x60,0x00,0x30,0x10,
+ 0x01,0x00,0x60,0x00,0x30,0x10,0x01,0x00,0xc0,0x00,0x18,0x10,0x01,0x00,0x80,
+ 0x00,0x08,0x10,0x01,0x00,0x00,0x00,0x00,0x10,0x01,0x00,0x00,0x00,0x00,0x10,
+ 0x01,0x00,0x00,0x00,0x00,0x10,0xff,0xff,0xff,0xff,0xff,0x1f};
diff --git a/show_edit/_16745_tex2html_wrap751.png b/show_edit/_16745_tex2html_wrap751.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap751.png differ
diff --git a/show_edit/_16745_tex2html_wrap751.xbm b/show_edit/_16745_tex2html_wrap751.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap751.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap753.png b/show_edit/_16745_tex2html_wrap753.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap753.png differ
diff --git a/show_edit/_16745_tex2html_wrap753.xbm b/show_edit/_16745_tex2html_wrap753.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap753.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap765.png b/show_edit/_16745_tex2html_wrap765.png
new file mode 100644
index 0000000000000000000000000000000000000000..3f795fd1310cea4934dc739560588f67a9b95291
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap765.png differ
diff --git a/show_edit/_16745_tex2html_wrap765.xbm b/show_edit/_16745_tex2html_wrap765.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..62424a5ac02bf56f805e639ad432c9cd6858bcc8
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap765.xbm
@@ -0,0 +1,17 @@
+#define noname_width 64
+#define noname_height 25
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xc1,0x0c,0xc0,0x00,0x00,
+ 0x00,0x3f,0x80,0xc1,0x0c,0xc0,0x00,0x00,0x80,0x3f,0x80,0xc1,0x00,0xc0,0x00,
+ 0x00,0x80,0x31,0x80,0xc1,0x00,0xc0,0x00,0x00,0x80,0x31,0x80,0xc1,0xec,0xc3,
+ 0xcc,0x0c,0xf7,0xf7,0x81,0xc1,0xec,0xc7,0xce,0x8c,0xff,0xf7,0x83,0xc1,0x6c,
+ 0xc6,0x07,0xc0,0x8d,0x31,0x83,0xc1,0x6c,0xc6,0x03,0xc0,0x8c,0x31,0x83,0xc1,
+ 0x6c,0xc6,0x07,0x80,0x8f,0x31,0x83,0xc1,0x6c,0xc6,0x06,0xc0,0x87,0x31,0x83,
+ 0xc1,0x6c,0xc6,0xce,0xcc,0x8f,0x31,0x83,0xc1,0x6c,0xc6,0xdc,0x8c,0x9f,0x31,
+ 0x83,0x01,0x00,0x00,0x00,0xc0,0x38,0x00,0x80,0x01,0x00,0x00,0x00,0xc0,0x30,
+ 0x00,0x80,0x01,0x00,0x00,0x00,0xc0,0x1f,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x0f,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff};
diff --git a/show_edit/_16745_tex2html_wrap767.png b/show_edit/_16745_tex2html_wrap767.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap767.png differ
diff --git a/show_edit/_16745_tex2html_wrap767.xbm b/show_edit/_16745_tex2html_wrap767.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap767.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap769.png b/show_edit/_16745_tex2html_wrap769.png
new file mode 100644
index 0000000000000000000000000000000000000000..dd186f99c9d18db5a701f709b4b9f415f01f46c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap769.png differ
diff --git a/show_edit/_16745_tex2html_wrap769.xbm b/show_edit/_16745_tex2html_wrap769.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a57b5faa9403585cf73408fb0b991ce0b0a6e5c8
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap769.xbm
@@ -0,0 +1,12 @@
+#define noname_width 52
+#define noname_height 19
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,
+ 0x80,0xcf,0x07,0x00,0x08,0x01,0x00,0xe0,0xcc,0x0c,0x00,0x08,0x01,0x00,0x66,
+ 0xc0,0xd8,0x00,0x08,0x01,0x80,0x73,0xc0,0x9c,0x03,0x08,0x01,0xe0,0x30,0xc0,
+ 0x0f,0x0e,0x08,0x01,0x38,0x30,0xc0,0x06,0x38,0x08,0x01,0x38,0x60,0xc0,0x0e,
+ 0x38,0x08,0x01,0xe0,0xe0,0xcc,0x0c,0x0e,0x08,0x01,0x80,0xc3,0xcf,0x98,0x03,
+ 0x08,0x01,0x00,0x06,0x00,0xc0,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x00,0x00,0x08,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap787.png b/show_edit/_16745_tex2html_wrap787.png
new file mode 100644
index 0000000000000000000000000000000000000000..682b2a91b3f3127da55bef77d8eef0f3a6dfdb5d
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap787.png differ
diff --git a/show_edit/_16745_tex2html_wrap787.xbm b/show_edit/_16745_tex2html_wrap787.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..47d7f270a5e3ff1dfa59da8fe7fa2b02828f9b19
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap787.xbm
@@ -0,0 +1,14 @@
+#define noname_width 56
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x80,0x81,0x01,0x00,0x80,0x01,0x00,0x80,
+ 0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x81,0x01,0x00,0x80,0x01,0x00,0x80,0x81,
+ 0x01,0x00,0x80,0xc1,0x66,0xf0,0xf1,0x31,0xf3,0x87,0xc1,0xff,0xf8,0xf9,0x31,
+ 0xf3,0x87,0xc1,0xdd,0x99,0x99,0x01,0x80,0x83,0xc1,0x8c,0x8d,0x8d,0x01,0x80,
+ 0x81,0xc1,0x8c,0x8d,0x8d,0x01,0xc0,0x81,0xc1,0x8c,0x9d,0x9d,0x01,0xe0,0x80,
+ 0xc1,0x8c,0xd9,0xd9,0x31,0x73,0x80,0xc1,0x8c,0xf9,0xf9,0x31,0xf3,0x87,0x01,
+ 0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,
+ 0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,0x80,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff};
diff --git a/show_edit/_16745_tex2html_wrap789.png b/show_edit/_16745_tex2html_wrap789.png
new file mode 100644
index 0000000000000000000000000000000000000000..e1b238ca993c36a479f80dab4cdc383379b59d62
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap789.png differ
diff --git a/show_edit/_16745_tex2html_wrap789.xbm b/show_edit/_16745_tex2html_wrap789.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..fa37d493ec9e1fb221cd9ad78bf35e9618240884
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap789.xbm
@@ -0,0 +1,11 @@
+#define noname_width 40
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x7f,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x80,0x81,0x81,
+ 0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,0x01,0x00,0x80,0x81,0x81,
+ 0xc1,0x66,0xf0,0xf1,0x81,0xc1,0xff,0xf8,0xf9,0x81,0xc1,0xdd,0x99,0x99,0x81,
+ 0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x8d,0x8d,0x81,0xc1,0x8c,0x9d,0x9d,0x81,
+ 0xc1,0x8c,0xd9,0xd9,0x81,0xc1,0x8c,0xf9,0xf9,0x81,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0xff,0xff,0xff,0xff,0x7f};
diff --git a/show_edit/_16745_tex2html_wrap791.png b/show_edit/_16745_tex2html_wrap791.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap791.png differ
diff --git a/show_edit/_16745_tex2html_wrap791.xbm b/show_edit/_16745_tex2html_wrap791.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap791.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap793.png b/show_edit/_16745_tex2html_wrap793.png
new file mode 100644
index 0000000000000000000000000000000000000000..9e43cfeb013558fb30201a36c97601448de002c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap793.png differ
diff --git a/show_edit/_16745_tex2html_wrap793.xbm b/show_edit/_16745_tex2html_wrap793.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..d2a9d7834a13e3012fc9fc7c8c48164192b535a8
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap793.xbm
@@ -0,0 +1,11 @@
+#define noname_width 36
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0x0f,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,0x01,0x00,0x00,0x30,0x08,
+ 0x81,0xc3,0xf1,0x31,0x08,0xc1,0xf7,0xf3,0x33,0x08,0x61,0x36,0x33,0x33,0x08,
+ 0xe1,0x1b,0x30,0x33,0x08,0xc1,0x1f,0x30,0x33,0x08,0x01,0x3e,0x30,0x33,0x08,
+ 0x61,0x76,0x33,0x33,0x08,0xe1,0xe7,0x33,0x33,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x08,
+ 0xff,0xff,0xff,0xff,0x0f};
diff --git a/show_edit/_16745_tex2html_wrap795.png b/show_edit/_16745_tex2html_wrap795.png
new file mode 100644
index 0000000000000000000000000000000000000000..9bd026647d2af88a4beca1872b70b709377d875c
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap795.png differ
diff --git a/show_edit/_16745_tex2html_wrap795.xbm b/show_edit/_16745_tex2html_wrap795.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..36a2bf7f4246d7126219ad3f07422e992608414f
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap795.xbm
@@ -0,0 +1,10 @@
+#define noname_width 40
+#define noname_height 20
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0x81,0xc3,0xf1,0xf1,0x81,0xc1,0xf7,0xf3,0xf3,0x83,
+ 0x61,0x36,0x33,0x33,0x83,0xe1,0x1b,0x30,0x33,0x87,0xc1,0x1f,0x30,0x33,0x86,
+ 0x01,0x3e,0x30,0x33,0x87,0x61,0x76,0x33,0xf3,0x83,0xe1,0xe7,0x33,0xf3,0x83,
+ 0x01,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x30,0x80,
+ 0x01,0x00,0x00,0x30,0x80,0x01,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x80,
+ 0x01,0x00,0x00,0x00,0x80,0xff,0xff,0xff,0xff,0xff};
diff --git a/show_edit/_16745_tex2html_wrap797.png b/show_edit/_16745_tex2html_wrap797.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap797.png differ
diff --git a/show_edit/_16745_tex2html_wrap797.xbm b/show_edit/_16745_tex2html_wrap797.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap797.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/_16745_tex2html_wrap799.png b/show_edit/_16745_tex2html_wrap799.png
new file mode 100644
index 0000000000000000000000000000000000000000..bf03084f8686ed075d485a0936c27d89d0a7a420
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap799.png differ
diff --git a/show_edit/_16745_tex2html_wrap799.xbm b/show_edit/_16745_tex2html_wrap799.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..78f0c60e344659efdf06cf968aed421c312e1bfa
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap799.xbm
@@ -0,0 +1,18 @@
+#define noname_width 78
+#define noname_height 22
+static char noname_bits[] = {
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x3f,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x01,0x40,0x00,0x00,0x70,0x00,0x00,0x00,0x0c,0x20,
+ 0x01,0x78,0xf8,0xf9,0xf9,0x00,0x00,0x00,0x0c,0x20,0x01,0x78,0x18,0x18,0x88,
+ 0x01,0x00,0x00,0x0c,0x20,0x01,0x60,0x18,0x18,0x8c,0x01,0x00,0x00,0x0c,0x20,
+ 0x01,0x60,0x18,0x18,0x88,0x99,0xe1,0x70,0x7c,0x20,0x01,0x60,0xf8,0xf8,0x80,
+ 0x99,0xf1,0xfd,0xfc,0x20,0x01,0x60,0xf8,0xf9,0xc1,0x01,0x98,0xcd,0xcc,0x20,
+ 0x01,0x60,0x98,0x99,0xe1,0x00,0xf8,0x06,0xcc,0x20,0x01,0x60,0x80,0x81,0x61,
+ 0x00,0xf0,0x07,0xcc,0x20,0x01,0x60,0x88,0x89,0x31,0x00,0x80,0x0f,0xcc,0x20,
+ 0xc1,0x60,0x8c,0x8d,0x19,0x98,0x99,0xdd,0xcc,0x20,0xc1,0xf8,0xf9,0xf8,0xfc,
+ 0x99,0xf9,0xf9,0xcc,0x20,0x01,0x00,0x70,0x70,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x20,0x01,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0x3f};
diff --git a/show_edit/_16745_tex2html_wrap801.png b/show_edit/_16745_tex2html_wrap801.png
new file mode 100644
index 0000000000000000000000000000000000000000..14085184830fc570ef3014c3415df718f2a820c0
Binary files /dev/null and b/show_edit/_16745_tex2html_wrap801.png differ
diff --git a/show_edit/_16745_tex2html_wrap801.xbm b/show_edit/_16745_tex2html_wrap801.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..8fe35282cc3857f2fe187bdea2d6f9c48d749d63
--- /dev/null
+++ b/show_edit/_16745_tex2html_wrap801.xbm
@@ -0,0 +1,8 @@
+#define noname_width 18
+#define noname_height 23
+static char noname_bits[] = {
+ 0xff,0xff,0x03,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x03,0x02,0x01,0x03,0x02,0xc1,0x0f,0x02,0xc1,0x0f,0x02,0x81,0x07,0x02,
+ 0xc1,0x0f,0x02,0x41,0x0f,0x02,0x01,0x03,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,0x01,0x00,0x02,
+ 0x01,0x00,0x02,0x01,0x00,0x02,0xff,0xff,0x03};
diff --git a/show_edit/images.pl b/show_edit/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..774d07ed3c9e24b70a579a82ebf3af018b6fba28
--- /dev/null
+++ b/show_edit/images.pl
@@ -0,0 +1,161 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}fbox<<494>>largesfifrp:<<494>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap709.xbm">'; 
+$key = q/{}fbox<<436>>largesfrtp(2)2,1,2,3,4<<436>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap677.xbm">'; 
+$key = q/{}fbox<<450>>largesflink(1)==,1<<450>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap676.xbm">'; 
+$key = q/{}fbox<<397>>largesfra:d<<397>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap645.xbm">'; 
+$key = q/{}fbox<<399>>largesfra:dhf<<399>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap644.xbm">'; 
+$key = q/{}fbox<<410>>largesfra:dhf10<<410>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap655.xbm">'; 
+$key = q/{tabular}<<128>>lll<<128>>;html_special_mark_amp;<verb_mark>2;html_special_mark_amp;unsignedbyte,I,J;html_special_mark_amp;<verb_mark>3;html_special_mark_amp;signedsame;html_special_mark_amp;<verb_mark>4;html_special_mark_amp;hexadecimalsame;html_special_mark_amp;<verb_mark>5;html_special_mark_amp;octalsame;html_special_mark_amp;<verb_mark>6;html_special_mark_amp;;html_special_mark_lt;n;html_special_mark_gt;characters;html_special_mark_amp;<verb_mark>7;html_special_mark_amp;real;html_special_mark_amp;<verb_mark>8;html_special_mark_amp;doubleprecision;html_special_mark_amp;<verb_mark>9;html_special_mark_amp;complex;html_special_mark_amp;<verb_mark>10;html_special_mark_amp;Angle,hh:mm:ss,dd.mm.ssfor;html_special_mark_amp;;html_special_mark_amp;Fractions,radians,degrees{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tabular127.xbm">'; 
+$key = q/{}fbox<<569>>largesflink::gfh<<569>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap765.xbm">'; 
+$key = q/{tabular}<<157>>lll<<157>>;html_special_mark_amp;column2:;html_special_mark_amp;thedefaulthtmladdnormallink<<426>><<424>>displayvalueformat<<424>><<426>><<425>>#.show.in.format<<425>>;html_special_mark_amp;column3:;html_special_mark_amp;thebyteoffsetofthefieldintheblock;html_special_mark_amp;column4:;html_special_mark_amp;thenumberofelementsinthefield;html_special_mark_amp;column5:;html_special_mark_amp;***??***;html_special_mark_amp;column6:;html_special_mark_amp;thebytesizeofasingleelement(whichisthestringlength;html_special_mark_amp;;html_special_mark_amp;foracharactervalue){tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tabular156.xbm">'; 
+$key = q/{}fbox<<590>>largesfmdd<<590>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap780.xbm">'; 
+$key = q/{}fbox<<538>>largesf~<<539>>smallsf<<718>><<718>>$<$<<719>><<719>>CR<<720>><<720>>$>$<<721>><<721>><<539>><<538>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap738.xbm">'; 
+$key = q/{}fbox<<633>>largesf.1552::sch<<633>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap799.xbm">'; 
+$key = q/{}fbox<<579>>largesf~<<580>>smallsf<<761>><<761>>$<$<<762>><<762>>CR<<763>><<763>>$>$<<764>><<764>><<580>><<579>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap769.xbm">'; 
+$key = q/{}fbox<<623>>largesfscnp<<623>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap795.xbm">'; 
+$key = q/{}fbox<<615>>largesfscnl<<615>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap793.xbm">'; 
+$key = q/{}fbox<<528>>largesfifr<<528>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap734.xbm">'; 
+$key = q/{}fbox<<511>>largesf~<<512>>smallsf<<694>><<694>>$<$<<695>><<695>>CR<<696>><<696>>$>$<<697>><<697>><<512>><<511>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap708.xbm">'; 
+$key = q/{}fbox<<427>>largesfrtp(2)2,1,2,3,4<<427>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap668.xbm">'; 
+$key = q/{}fbox<<415>>largesfra:xj<<415>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap657.xbm">'; 
+$key = q/{}fbox<<520>>largesfifr*<<520>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap732.xbm">'; 
+$key = q/{}fbox<<579>>largesfmdd::z<<579>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap778.xbm">'; 
+$key = q/{}fbox<<470>>largesf::<<470>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap689.xbm">'; 
+$key = q/{}fbox<<565>>largesf*<<565>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap758.xbm">'; 
+$key = q/{}fbox<<549>>largesf*<<549>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap742.xbm">'; 
+$key = q/{}fbox<<563>>largesf~<<564>>smallsf<<737>><<737>>$<$<<738>><<738>>CR<<739>><<739>>$>$<<740>><<740>><<564>><<563>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap753.xbm">'; 
+$key = q/{}fbox<<486>>largesfmdd<<486>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap707.xbm">'; 
+$key = q/{}fbox<<459>>largesflink(1)==,1<<459>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap685.xbm">'; 
+$key = q/{}fbox<<604>>largesf*<<604>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap791.xbm">'; 
+$key = q/{}fbox<<574>>largesf*<<574>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap767.xbm">'; 
+$key = q/{}fbox<<558>>largesf*<<558>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap751.xbm">'; 
+$key = q/{}fbox<<507>>largesf:<<507>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap713.xbm">'; 
+$key = q/{}fbox<<588>>largesfmdd::z<<588>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap787.xbm">'; 
+$key = q/{}fbox<<547>>largesf~<<548>>smallsf<<727>><<727>>$<$<<728>><<728>>CR<<729>><<729>>$>$<<730>><<730>><<548>><<547>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap747.xbm">'; 
+$key = q/{}fbox<<405>>largesfra:dhf<<405>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap653.xbm">'; 
+$key = q/{}fbox<<570>>largesf~<<571>>smallsf<<752>><<752>>$<$<<753>><<753>>CR<<754>><<754>>$>$<<755>><<755>><<571>><<570>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap760.xbm">'; 
+$key = q/{}fbox<<414>>largesf:<<414>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap652.xbm">'; 
+$key = q/{}fbox<<599>>largesfmdd<<599>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap789.xbm">'; 
+$key = q/{}fbox<<520>>largesf~<<521>>smallsf<<703>><<703>>$<$<<704>><<704>>CR<<705>><<705>>$>$<<706>><<706>><<521>><<520>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap717.xbm">'; 
+$key = q/{}fbox<<606>>largesfscnl<<606>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap784.xbm">'; 
+$key = q/{}fbox<<614>>largesfscnp<<614>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap786.xbm">'; 
+$key = q/{}fbox<<423>>largesf:<<423>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap661.xbm">'; 
+$key = q/{}fbox<<422>>largesfRTP,12<<422>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap666.xbm">'; 
+$key = q/{}fbox<<499>>largesfifrp<<499>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap711.xbm">'; 
+$key = q/{}fbox<<624>>largesf.1552::sch<<624>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap790.xbm">'; 
+$key = q/{}fbox<<506>>largesf*<<506>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap706.xbm">'; 
+$key = q/{}fbox<<632>>largesf*<<632>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap792.xbm">'; 
+$key = q/{}fbox<<537>>largesfifr<<537>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap743.xbm">'; 
+$key = q/{}fbox<<409>>largesfra:xj<<409>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap648.xbm">'; 
+$key = q/{}fbox<<454>>largesflink,12<<454>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap683.xbm">'; 
+$key = q/{}fbox<<641>>largesf*<<641>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap801.xbm">'; 
+$key = q/{}fbox<<435>>largesfrtp,0<<435>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap670.xbm">'; 
+$key = q/{}fbox<<595>>largesf*<<595>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap782.xbm">'; 
+$key = q/{}fbox<<515>>largesf*<<515>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap715.xbm">'; 
+$key = q/{}fbox<<391>>largesfra:d<<391>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap636.xbm">'; 
+$key = q/{}fbox<<404>>largesfra:dhf10<<404>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap646.xbm">'; 
+$key = q/{}fbox<<544>>largesfifr(5)<<544>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap740.xbm">'; 
+$key = q/{}fbox<<560>>largesflink::gfh<<560>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap756.xbm">'; 
+$key = q/{}fbox<<431>>largesfRTP,12<<431>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap675.xbm">'; 
+$key = q/{}fbox<<498>>largesf:<<498>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap704.xbm">'; 
+$key = q/{}fbox<<485>>largesfifrp:<<485>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap700.xbm">'; 
+$key = q/{}fbox<<445>>largesflink,12<<445>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap674.xbm">'; 
+$key = q/{tabular}<<145>>lll<<145>>;html_special_mark_amp;<verb_mark>12;html_special_mark_amp;willshowtheentireblockformattedinthesamewayas;html_special_mark_amp;;html_special_mark_amp;fora<<146>>bfSHOW<<146>>command;html_special_mark_amp;<verb_mark>13;html_special_mark_amp;willshowthenamesandformatsofalldatafieldsintheblock;html_special_mark_amp;<verb_mark>14;html_special_mark_amp;willshowformatinformationfor<verb_mark>15{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tabular144.xbm">'; 
+$key = q/{}fbox<<533>>largesf*<<533>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap736.xbm">'; 
+$key = q/{}fbox<<619>>largesf*<<619>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap788.xbm">'; 
+$key = q/{}fbox<<529>>largesfifr*<<529>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap741.xbm">'; 
+$key = q/{tabular}<<149>>lll<<149>>;html_special_mark_amp;<verb_mark>16;html_special_mark_amp;willshowtheentireblockformattedinthesamewayas;html_special_mark_amp;;html_special_mark_amp;fora<<150>>bfSHOW<<150>>command;html_special_mark_amp;<verb_mark>17;html_special_mark_amp;willshowthenamesandformatsofalldatafieldsintheblock;html_special_mark_amp;<verb_mark>18;html_special_mark_amp;willshowformatinformationfor<verb_mark>19{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tabular148.xbm">'; 
+$key = q/{}fbox<<628>>largesf*<<628>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap797.xbm">'; 
+$key = q/{}fbox<<542>>largesf*<<542>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap745.xbm">'; 
+$key = q/{}$bigotimes${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.xbm">'; 
+$key = q/{}fbox<<553>>largesfifr(5)<<553>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap749.xbm">'; 
+$key = q/{}fbox<<449>>largesfrtp(2),287.9837,431.9756<<449>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap681.xbm">'; 
+$key = q/{}fbox<<477>>largesfmdd<<477>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap698.xbm">'; 
+$key = q/{}fbox<<554>>largesf~<<555>>smallsf<<728>><<728>>$<$<<729>><<729>>CR<<730>><<730>>$>$<<731>><<731>><<555>><<554>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap744.xbm">'; 
+$key = q/{}fbox<<440>>largesfrtp(2),287.9837,431.9756<<440>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap672.xbm">'; 
+$key = q/{}fbox<<444>>largesfrtp,0<<444>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap679.xbm">'; 
+$key = q/{}fbox<<461>>largesf::<<461>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap680.xbm">'; 
+$key = q/{}fbox<<490>>largesfifrp<<490>>{}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap702.xbm">'; 
+$key = q/{tabular}<<153>>lll<<153>>;html_special_mark_amp;column2:;html_special_mark_amp;thedefaulthtmladdnormallink<<417>><<415>>displayvalueformat<<415>><<417>><<416>>#.show.in.format<<416>>;html_special_mark_amp;column3:;html_special_mark_amp;thebyteoffsetofthefieldintheblock;html_special_mark_amp;column4:;html_special_mark_amp;thenumberofelementsinthefield;html_special_mark_amp;column5:;html_special_mark_amp;***??***;html_special_mark_amp;column6:;html_special_mark_amp;thebytesizeofasingleelement(whichisthestringlength;html_special_mark_amp;;html_special_mark_amp;foracharactervalue){tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_12943_tabular152.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/show_edit/labels.pl b/show_edit/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..bb0d335186856a31c9b7d51d5701a1d85c208f06
--- /dev/null
+++ b/show_edit/labels.pl
@@ -0,0 +1,12 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".data.arrays"} ="$URL/show_edit.html"; 
+$external_labels{".pointers"} ="$URL/show_edit.html"; 
+$external_labels{".show.meta"} ="$URL/show_edit.html"; 
+$external_labels{".edit"} ="$URL/show_edit.html"; 
+$external_labels{".show.format"} ="$URL/show_edit.html"; 
+$external_labels{".contents"} ="$URL/show_edit.html"; 
+$external_labels{".abs.rel.address"} ="$URL/show_edit.html"; 
+
+1;
\ No newline at end of file
diff --git a/show_edit/show_edit.html b/show_edit/show_edit.html
new file mode 100644
index 0000000000000000000000000000000000000000..806c5d3139acb7f9d4f43969750611184e2c7874
--- /dev/null
+++ b/show_edit/show_edit.html
@@ -0,0 +1,649 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>SHOWing and EDITing data-file contents in <i>NEWSTAR </i></b>  
+<BR><BR><i>Contributed by Wim Brouw, December 1993 <BR>Revised/adapted by Johan Hamaker, June 1994 </i>
+<P>
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=show_edit.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=show_edit.html#SECTION0002000000000000000>  <b>Introduction</b></A>
+<LI> <A NAME=tex2html3 HREF=show_edit.html#SECTION0003000000000000000> <b>SHOW and EDIT</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=show_edit.html#SECTION0003100000000000000>  <b>Displaying data values in different formats </b></A>
+<LI> <A NAME=tex2html5 HREF=show_edit.html#SECTION0003200000000000000>  <b>Displaying parts of arrays</b></A>
+<LI> <A NAME=tex2html6 HREF=show_edit.html#SECTION0003300000000000000>  <b>Displaying information about data fields</b></A>
+</UL> 
+<LI> <A NAME=tex2html7 HREF=show_edit.html#SECTION0004000000000000000>  <b>Modifying data values </b></A>
+<LI> <A NAME=tex2html8 HREF=show_edit.html#SECTION0005000000000000000>  <b>Secondary blocks and substructures</b></A>
+<UL> 
+<LI> <A NAME=tex2html9 HREF=show_edit.html#SECTION0005100000000000000>  <b>Navigating secondary blocks</b></A>
+<LI> <A NAME=tex2html10 HREF=show_edit.html#SECTION0005200000000000000>  <b>Displaying/editing a substructure</b></A>
+</UL> 
+<LI> <A NAME=tex2html11 HREF=show_edit.html#SECTION0006000000000000000>  <b>Advanced options</b></A>
+<UL> 
+<LI> <A NAME=tex2html12 HREF=show_edit.html#SECTION0006100000000000000>  <b>Linked lists</b></A>
+<LI> <A NAME=tex2html13 HREF=show_edit.html#SECTION0006200000000000000>  <b>Data arrays</b></A>
+<LI> <A NAME=tex2html14 HREF=show_edit.html#SECTION0006300000000000000>  <b>Absolute and relative file addresses</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Introduction</b></A></H1>
+<P>
+        The programs NSCAN, NFLAG, NMAP and NGCALC have a SHOW option, with an EDIT sub-option.  This EDIT sub-option can be used to examine and change any field in the SCN, WMP and NGF files.  
+        The EDIT option can show and/or edit the contents of <i>NEWSTAR </i> files. All values ('fields'), with the exception of values determining the structure of the file, may be edited individually (or in groups) by hand.  This is laborious, <em>but at least it is possible!</em>  
+        The different files contain a variety of blocks (e.g.  STH - sector header; MPH - map header).  In addition to manipulating these fields, <i>NEWSTAR </i> programs know how to present their names and values in an intelligible form to the user, and conversely how to interpret the user's editing instructions.  
+        After starting EDIT, the message:  
+        **** Editing STH **** (or MPH or ....)
+<P>
+will appear, indicating the actual block available for editing at this instant.
+<P>
+<H1><A NAME=SECTION0003000000000000000> <b>SHOW and EDIT</b></A></H1>
+<P>
+        <b>SHOW</b> gives a formatted display of the contents of the entire &quot;current&quot; block (i.e.  the block currently accessed through a navigating command such as <b>CONTINUE</b> or <b>NEXT</b>.  To display individual fields in the block one uses the <b>EDIT</b> option.  Once in edit mode, one may both display and modify fileds.  
+        The <i>display</i> commands for an individual field consist of the field name, optionally followed by a colon and qualifying information.  The various types of qualifier will be discussed below.  A display command becomes an <b>EDIT</b> command when followed by a comma plus one or more new values.  
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap645.png"> 
+  <PRE> 
+ RA             0.06725881318561733
+</PRE>
+<P>
+Note that <A HREF="#.pointers">pointer values</A> can not be shown this
+way.
+<P>
+<A NAME=.show.format><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>Displaying data values in different formats </b></A></H2>
+<P>
+        Appending a format specifier to the colon overrides the default format
+in which a value is displayed.  Some of the possible formats are:
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tabular127.png"><P>
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap653.png"> 
+  <PRE> 
+ RA                        01:36:51
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap655.png"> 
+  <PRE> 
+ RA                   01:36:51.1615
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap657.png"> 
+  <PRE> 
+ RA                        3fb137d4 
+</PRE>
+<P>
+        The full list of available formats, including fieldsize indicators,
+exists only in the form of a table in the program source file
+wnctxt_x.for.
+<P>
+<H2><A NAME=SECTION0003200000000000000>  <b>Displaying parts of arrays</b></A></H2>
+<P>
+        Elements of array fields can be selected by appending the start index
+and the number of elements to the field name, as follows: 
+        - &lt;name&gt;[(&lt;offset&gt;)][,/&lt;number&gt;] 
+will show the value of &lt;name&gt;.  If an offset is given for a
+multi-valued &lt;name&gt;, the display will start at this value; if
+/&lt;number&gt; is given, only that many values will be shown. 
+Examples are given <A HREF="#.edit">below</A>.  Remember that <b>indices start at
+0!</b>.
+<P>
+<A NAME=.show.meta><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003300000000000000>  <b>Displaying information about data fields</b></A></H2>
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_16745_tabular148.png"><P>
+<P>
+Examples:
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap661.png"> 
+  <PRE> 
+ Known names: 
+              LINK,      XJ, , ;     0,     2,     1,     4
+              LEN,       SI, , ;     8,     1,     1,     2
+              VER,       SI, , ;    10,     1,     1,     2
+              FIELD,     AL, , ;    28,     1,     0,    12
+                         .
+                         .
+
+              RA,   DAF12.7, , ;    40,     1,     0,     8
+              DEC,  DAF12.7, , ;    48,     1,     0,     8
+              RTP,    E12.4, , ;   124,    14,     0,     4
+              NIFR,      SJ, , ;   180,     1,     1,     4
+              IFRP,      XJ, ,   P:IFRT;   184,     1,     1,     4
+              NFD,       SJ, , ;   188,     1,     1,     4
+              FDP,       XJ, ,    P:FDW;   192,     1,     1,     4
+              NOH,       SJ, , ;   196,     1,     1,     4
+                        .
+                        .
+
+</PRE>
+<P>
+The entries in this table are:
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_16745_tabular156.png"><P>
+<P>
+<A NAME=.edit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0004000000000000000>  <b>Modifying data values </b></A></H1>
+<P>
+        Most values in a data file can be edited.  The field descriptors
+outlined above for <b>SHOW</b> are also valid for <b>EDIT</b>.  Edit commands are
+charaterised by the presence of a <b>comma</b> following the field descriptor:
+<P>
+&lt;name&gt;[&lt;(offset)&gt;][&lt;/number&gt;], &lt;value&gt; [,&lt;value&gt;...]
+<P>
+will change the value(s) at the given field. Examples:
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE> 
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap675.png"> 
+  <PRE> 
+ RTP          12.0000     143.9919     287.9837     431.9756     575.9674
+             719.9592     863.9511    1007.9429    1151.9348    1295.9266
+            1367.9257    1439.9176    2663.8491    2735.8452
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap677.png">
+<P>
+		<i>Note that names are not case-sensitive!</i>  
+  <PRE> 
+ RTP           1.0000       2.0000
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap679.png"> 
+  <PRE> 
+ RTP           0.0000     143.9919       1.0000       2.0000     575.9674
+             719.9592     863.9511    1007.9429    1151.9348    1295.9266
+            1367.9257    1439.9176    2663.8491    2735.8452
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap681.png"> 
+  <PRE> 
+ RTP         287.9837     431.9756     575.9674     719.9592     863.9511
+            1007.9429    1151.9348    1295.9266    1367.9257    1439.9176
+            2663.8491    2735.8452
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap683.png"> 
+  <PRE> Edit of field LINK not allowed 
+ LINK        0007ec60     00000098 
+</PRE>
+<P>
+        The last example demonstrates that certain fields cannot be changed
+because the integrity of the file depends on them.  This restriction may be
+overridden by appending '<b>==</b>' to the field descriptor:
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap685.png"> 
+  <PRE> 
+ LINK        00000001
+</PRE>
+<P>
+        The value given is interpreted with the default format descriptor
+displayed by the <A HREF="#.show.meta">name command</A>).  A different format can
+be used by giving a 
+<A HREF="#.show.format">format specifier</A>.
+<P>
+        For integers, the radix specifiers <tt>%X</tt> (hexadecimal), <tt>%D</tt>(decimal) and <tt>%O</tt> (octal) can also be used.  Values given as
+<P>
+        hh:[[mm][:[ss][.ttt]] or <BR>dd.[mm].[ss][.ttt]]
+<P>
+will be translated to degrees and saved in the appropriate F, 
+R or D format;
+<P>
+<A NAME=.pointers><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0005000000000000000>  <b>Secondary blocks and substructures</b></A></H1>
+<P>
+        The header blocks directly accessible through <b>SHOW/EDIT</b> contain
+pointers to other blocks.  When their value is listed, :P is appended,
+meaning that the value is the address of a block on disk in the corresponding
+format format.
+<P>
+        Certain fields in a block are arrays not of single values but of
+sub-blocks of some type; an example are the interferometer entries in the OHW
+block.  When such a field is listed, :S is appended, meaning that this
+is an array of subblocks.
+<P>
+        All secondary-block and substructure types known to the system 
+(i.e.  not only those associated with the current block) are displayed by the
+<b>::</b> command:
+<P>
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap689.png"> 
+  <PRE> 
+ Known P: types: STH, FDW, OHW, SCW, SHW, FDX, GFH, IFRT, MDH, MDD, SGH, MDL,
+SCH 
+        IFRC, B, I, J, E, D, X, Y, S:SET, S:SRC, S:BCOR, S:MOZP, S:IFR, IFH
+</PRE>
+<P>
+		<i>: indicates a sub-structure. The use of the data types <em>B,
+I</em> etc. is explained <A HREF="#.data.arrays">elsewhere</A>. </i>
+<P>
+<H2><A NAME=SECTION0005100000000000000>  <b>Navigating secondary blocks</b></A></H2>
+<P>
+        Specifying the name of a pointer will steer the editing process to the
+block pointed at: 
+  <PRE> 
+ *** Editing STH *** 
+</PRE> 
+  <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap707.png"> 
+  <PRE> 
+ *** Editing STH *** 
+</PRE>
+<P>
+		<i>So nothing happened: There is no MDD block attached to this STH
+block.</i>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap709.png"> 
+  <PRE> 
+ Edit data: IFRP, XJ, , P:IFRT; 184, 1, 1, 4 
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap711.png"> 
+  <PRE> 
+ *** Editing IFRT *** 
+</PRE>
+<P>
+		<i>This time we succeeded!</i>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap713.png"> 
+  <PRE> 
+ Known names: 
+              IFR,       XI, , ;     0,    88,     0,     2
+</PRE>
+<P>
+		<i>The IFR block is just an array of hex integers</i>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap715.png"> 
+  <PRE> 
+ IFR             0a09         0b0a         0d0c         0b09         0100 
+                 0201         0302         0403         0504         0605
+                   .
+                   .
+
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap717.png"> 
+  <PRE> 
+ *** Editing STH *** 
+</PRE>
+<P>
+		<i>A null reply returns us to the parent block</i>
+<P>
+<H2><A NAME=SECTION0005200000000000000>  <b>Displaying/editing a substructure</b></A></H2>
+<P>
+        An array of substructures can be shown in its entirety by: 
+        &lt;name&gt;* 
+Example: 
+    <PRE> 
+ *** Editing SHW *** 
+</PRE> 
+ <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap741.png"> 
+  <PRE> 
+ INFNR          16667      WTEL               0      OTEL              13
+ RBAS            2736      NIH             2040
+
+ INFNR          16665      WTEL               0      OTEL              12
+ RBAS            2664      NIH             2047
+                 .
+                 .
+
+ *** Editing SHW *** 
+</PRE>
+<P>
+		<i>Note that the current block is still SHW.</i>
+<P>
+A single sub-structure can be shown and edited by:
+<P>
+        &lt;name&gt;[(&lt;index&gt;)]
+<P>
+Example:
+<P>
+    <PRE> 
+ *** Editing SHW *** 
+</PRE> 
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap743.png"> 
+  <PRE> 
+ *** Editing S:IFR *** 
+</PRE>  
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap745.png"> 
+  <PRE> 
+ INFNR          16667      WTEL               0      OTEL              13
+ RBAS            2736      NIH             9120
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap747.png"> 
+  <PRE> 
+ *** Editing SHW *** 
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap749.png"> 
+  <PRE> 
+ *** Editing S:IFR *** 
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap751.png"> 
+  <PRE> 
+ INFNR          17689      WTEL               2      OTEL              12
+ RBAS            2376      NIH             9465
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap753.png"> 
+  <PRE> 
+ *** Editing SHW *** 
+</PRE>
+<P>
+<H1><A NAME=SECTION0006000000000000000>  <b>Advanced options</b></A></H1>
+<P>
+        The options described here are available for system programmers. 
+They assume a proper understanding of the architecture of Newstar data files
+and of the mechanisms (.dsc and .def files) through which it is defined.  No
+attempt will be made here to help the reader on these points... 
+        The syntax of the advanced options is less intuitively clear than what
+has been described above and its expressive power is limited. 
+In using it, the user will have to feel his way around, but he can safely do so
+as long as he doesnot rashly attempt to change any values.
+<P>
+<H2><A NAME=SECTION0006100000000000000>  <b>Linked lists</b></A></H2>
+<P>
+        Link pointers in linked lists are similar to other pointers, except
+that the type of the target block is not known a priori.  It must therefore be
+specified: 
+        &lt;name&gt;[(&lt;index&gt;)]::&lt;target block type&gt; 
+For example:
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap765.png"> 
+  <PRE> 
+ *** Editing GFH *** 
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap767.png"> 
+  <PRE> 
+ ID              .SCN      LEN              512      VER                1
+ CDAT     21-Sep-1993      CTIM           17:23      RDAT     13-Jun-1994 
+ RTIM           16:16      RCNT              50      NAME           A271A
+ DATTP              7
+ LINK        00006550     00500e08 
+ ALHD        00006550     00500e08 
+ NLINK              4      ALLEN              4
+ LINKG       00000200     008069c8 :P 
+ LHD         00000200     008069c8 :P 
+ NLINKG             2      LLEN               2      IDMDL              0
+ ID1                0      ID2                0      USER               0
+
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap769.png">
+<P>
+		<i>Return to STH</i>  
+  <PRE> 
+ *** Editing STH *** 
+</PRE>
+<P>
+<A NAME=.data.arrays><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006200000000000000>  <b>Data arrays</b></A></H2>
+<P>
+        Some pointers point to &quot;naked&quot; arrays of data structures.  An example
+is MDD in the STH which points to the array of complex model visibilities:
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap787.png">
+<P>
+		<i>We try to display the array in complex format ...</i>  
+  <PRE> 
+ MDD         006179c8     00000000 :P 
+</PRE>
+<P>
+		<i>but the system does not understand us!</i>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap789.png"> 
+  <PRE> 
+ *** Editing MDD *** 
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap791.png"> 
+  <PRE> 
+ MDD                -540.55+72.69I                0.00+0.00I
+                        0.00+0.00I                0.00+0.00I
+                    -540.50+72.76I                0.00+0.00I
+                        0.00+0.00I                0.00+0.00I
+                        .
+                        .
+
+</PRE>
+<P>
+		<i>This works, but it is not clear how we could select specific elements
+for display.</i>
+<P>
+        There are also data arrays whose address is defined implicitly by the
+fact that they contiguously follow a header block.  An example is the
+scan-visibilities block headed by the SCN header.  To access such data in the
+absence of a pointer, one must use a 
+<A HREF="#.abs.rel.address">byte offset</A>. 
+For this we need the length of the header, which we can easily find.  The
+technique is demonstrated below is a somewhat different context, <i>viz.</i>
+that of finding an SCH which is not directly pointed at.
+<P>
+    <PRE> 
+ *** Editing STH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap793.png"> 
+  <PRE> 
+ SCNL            1552
+</PRE>
+<P>
+		<i><BR>This is the length of an SCH plus the data.</i>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap795.png"> 
+  <PRE> 
+ *** Editing SCH *** 
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap797.png"> 
+  <PRE> 
+ HA       -90.1250124 deg  MAX         1294.000 W.U. SCAL        0.000000 
+ REDNS          0.000        0.000        0.000        0.000 W.U.
+                .
+                .
+
+</PRE>
+<P>
+    <BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap799.png">
+<P>
+		<i>Move to the next SCH. We can use multiples of SCNL to get to any of
+the SCHs.</i>  
+  <PRE> 
+ *** Editing SCH *** 
+</PRE>  
+<BR><IMG ALIGN=BOTTOM ALT="" SRC="_12943_tex2html_wrap768.png"> <b>EDIT</b> 
+ (Edit: name [(offset)][/length][:format] , val [, ...]) 
+ = "": 
+ <IMG ALIGN=BOTTOM ALT="" SRC="_16745_tex2html_wrap801.png"> 
+  <PRE> 
+ HA       -89.8743278 deg  MAX         1349.000 W.U. SCAL        0.000000 
+ REDNS          0.000        0.000        0.000        0.000 W.U.
+ ALGNS          0.000        0.000        0.000        0.000 W.U.
+                .
+                .
+
+</PRE>
+<P>
+<A NAME=.abs.rel.address><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0006300000000000000>  <b>Absolute and relative file addresses</b></A></H2>
+<P>
+        Absolute <em>file addresses</em> (i.e.  byte offsets in the file) can be
+used instead of field names.
+<P>
+        Relative addresses are byte offset relative to the start of the current
+block.  They are specified in the form
+<P>
+        .&lt;offset&gt;
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/spefu_type_categ.txt b/spefu_type_categ.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6c32b3447afb2353a2a4b13530a14f0863b1a434
--- /dev/null
+++ b/spefu_type_categ.txt
@@ -0,0 +1,65 @@
+List of codes in the OHW-fields SPEFU, TYPE, CATEG
+--------------------------------------------------
+	(original Dutch source unknown,
+	 translated litterally into English by JPH, 940621)
+
+History: 
+	JPH 940914      Format corrections
+
+
+	The OH (Observation Header) of an observation file on a WSRT tape is
+copied literally into a OHW block asspociated with one or more Sectors in a
+.SCN file. It contains several fields describing the natiure of the
+observation. The meaning of the ASCII that may occur in these fields is
+tabulated below.
+
+ SPEFU=   Meaning
+ ------   -------
+  PT     Pointing observation
+  HO     Holog observation
+  OF     Offset observation
+  VL     VLBI observation
+  MO     Mosaiking observation
+  PD     Pulsar observation (DCB)
+  DF     Delay offset observation (DCB)
+  LO     LO sweep observation
+  FS     FS frequency switching observation
+  SD     Switched dipole observation
+  NO     No special observation
+
+
+
+
+ TYPE
+ 1st char Meaning               2nd char Meaning
+ -------- -------               -------- -------
+ C       Other                  A        Supplememt to N,M,P or F
+ F       Frequency switch.      B        Baseline  (for C)
+ M       Mosaicking             C        Gain/phase (for C)
+ N       Norm. astr.            D        Dipole switch (for C)
+ P       Pulsar                 E        Extinction  (for C)
+ V       VLBI                   F        Phase only (for C)
+				G        Gain only (for C)
+				H        Holog (for C)
+				L        LO-delay (for C)
+				M        Monitoring (for N)
+				N        New (for N,M,P of F)
+				O        Redo (for N,M,P of F)
+				P        Parallax (for N of C)
+				Q        Offset (for C)
+				R        Pointing (for C)
+				S        System temp. (for C)
+				T        General Test (for C)
+				U        Universal (for C)
+				V        Videoband   (for C)
+				W        Delay (for C)
+
+
+
+ CATEG=         Meaning
+ ------         -------
+  I             Instrumental, including all calibrations
+  N             Astronomy: Nearby galaxies
+  S             Astronomy: Solar System
+  G             Astronomy: Galactic Object
+  E             Galactic astronomy not covered by N
diff --git a/src/doc/bin/agb.gif b/src/doc/bin/agb.gif
new file mode 100644
index 0000000000000000000000000000000000000000..050b197580dadc2959cf26e63dad6ce6841c836c
Binary files /dev/null and b/src/doc/bin/agb.gif differ
diff --git a/src/doc/bin/alpha_32_64.ps b/src/doc/bin/alpha_32_64.ps
new file mode 100644
index 0000000000000000000000000000000000000000..2bf5744eecaf88be5ece89196abdd21ed55b86ff
--- /dev/null
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@@ -0,0 +1,1403 @@
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+50.8 0 32 ( \(32 bits\) is aligned on a  4 byte boundary.  On MIPS systems,) W
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+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
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diff --git a/src/doc/txt/batch.txt b/src/doc/txt/batch.txt
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+From To:vdhulst Wed Jul 28 16:51:16 1993
+Date: Wed, 28 Jul 93 16:51:16 METDST
+To: vdhulst, kgb
+Subject: Over keywords en symbols
+Cc: noordam@nfra.nl
+Status: RO
+
+Fm: Marco de Vos
+To: Thijs van der Hulst en Kor Begeman
+
+Betreft:
+Batch processing in Newstar
+---------------------------
+
+Waarde heren,
+
+Ik heb wat details van DWARF opgespoord ten behoeve van automatische 
+processing. Hieronder volgt een voorlopig overzicht. Een aantal zaken 
+staat al in het Cookbook: Program Descriptions, Common.
+
+
+1e. DWARF Keywords, streams
+---------------------------
+
+Een gebruiker heeft invloed op de werking van een Newstar programma via
+de DWARF user-interface. Alle grootheden/parameters die een gebruiker
+in principe kan specificeren corresponderen met keywords, die een 
+waarde hebben. Die waarde kan op een aantal niveaus bepaald worden:
+
+   1e. Interne of program defaults:
+         De programmeur heeft een default waarde meegegeven bij de
+         definitie van het keyword (in de zgn. PIN-file). In een 
+         (beperkt) aantal gevallen staat er geen default in de PIN-file
+         maar geeft het programma zelf een default mee.
+
+   2e. Externe defaults:
+         De gebruiker heeft, buiten het programma om, een waarde 
+         gegeven aan het keyword door een DWARF symbool te definieren
+         (met dwspecify, met dwrestore, of door het programma eerder 
+         te gebruiken met de /SAVE switch)
+
+Voor een aantal algemene keywords wordt de externe default op twee 
+plaatsten gezocht: eerst in een tabel met defaults voor het programma
+(de "local" external default), als daar geen waarde staat in de algemene
+tabel (de external default van "NGEN").
+
+   3e. Het programma prompt de gebruiker voor het keyword en krijgt 
+       een waarde via toetsenbord of input-file. 
+
+Normaliter gaan de antwoorden die de user geeft op keyword prompts verloren
+wanneer het programma wordt verlaten. Er zijn twee manieren om een keyword
+te bewaren (alsof het met dwspecify was gegeven):
+
+   - Voor alle keywords de waarde bewaren: start programma met 
+         dwe <programma> /SAVE
+
+   - Voor individuele keywords de waarde bewaren: geef na de prompt
+         waarde /SAVE [/[NO]ASK]    (zie ook onder 3e)
+
+
+Op elk niveau kan een qualifier (switch) /ASK of /NOASK worden meegegeven.
+Deze bepaalt of de gebruiker voor het keyword geprompt wordt of niet
+(het opgeven van /[NO]ASK bij een prompt heeft alleen zin als ook de 
+/SAVE switch gegeven wordt).
+
+
+Met de /SAVE optie en dwspecify (= dws) kunnen vaste defaults voor een 
+programma worden gezet. Omdat het meestal wenselijk is verschillende 
+sets van defaults te gebruiken voor verschillende procedures kan een 
+programma in verschillende "streams" (wat was dat andere woord ook al 
+weer?) gestart worden. Elke "stream" heeft een eigen set defaults.
+
+Het commando om een programma te starten in een bepaalde "stream" is
+
+   dwe <programma>$<streamname>
+
+bv
+   dwe nscan$1
+   dwe nmap$standard
+   dwe nplot             default: stream 1
+
+Wanneer een keyword geen default heeft in de opgegeven stream wordt 
+een default in stream 0 gezocht, is daar ook niets dan blijft alleen
+de default van de PIN file over. Voor NGEN keywords wordt steeds zowel
+in de stream voor het programma als in de stream voor NGEN gezocht.
+
+ 
+
+2e. DWARF Symbols
+-----------------
+
+DWARF slaat externe defaults op als symbolen. Alle symbolen staan 
+fysiek in de file $DWARF_SYMBOLS (meestal ~/SYMBOL_DIR/SYMBOL.$$).
+
+Een DWARF keyword correspondeert met een symbool 
+
+     <Programma>$<Stream>_<Keyword>
+
+De waarde van het symbool is de character string die als default 
+gebruikt zal worden bij user-input, eventueel met de qualifier /ASK 
+of /NOASK er achter.
+
+Wanneer achter de waarde <space>/ASK staat, vervangt de waarde de default 
+van het programma, maar wordt de user toch geprompt voor het keyword.
+
+Wanneer achter de waarde <space>/NOASK staat, of wanneer er helemaal geen 
+qualifier staat, dan wordt de user niet meer voor het keyword geprompt.
+
+
+Naast deze keyword symbolen kunnen ook algemene symbolen gezet worden,
+die in antwoorden op prompts gebruikt kunnen worden, bv PI = 3.1415,
+NATUURLIJK = YES en zo voorts.
+
+
+De volgende utilities zijn beschikbaar om symbolen te manipuleren:
+
+
+ dwlet [symbol=value]  [/LOG[=long|short] [/NOLOG]   (= dwl)
+
+   Geef een waarde aan algemene symbolen. Kan niet gebruikt worden
+   om DWARF keywords te wijzigen.
+
+   Als er geen symbol=value wordt meegegeven wordt de standard input 
+   gelezen voor regels met "symbol=value", om te stoppen: lege regel 
+   of # of ^D.
+
+ dwspecify program[$stream] [/MENU] [/NOMENU]        (= dws)
+
+   Default stream is 1, default mode is /NOMENU.
+
+   Hiermee worden externe defautls voor DWARF keywords opgegeven.
+   Met /menu wordt voor elk keyword geprompt met de huidige 
+   (externe of interne) default, alleen wijzigingen worden in 
+   een symbool gezet. Met /nomenu worden van de standard input 
+   regels keyword=value gelezen.
+
+ dwclear [program[$stream]keyword,... [/CONFIRM] ...  (= dwc)
+
+   Verwijdert de definitie van de keywords, wildcards zijn toegestaan,
+   erg handig is bijvoorbeeld: dwclear nscan$*_*, om helemaal schoon
+   te beginnen.
+
+ dwsave  [program[$stream]keyword,... [/OUTPUT=file] [/CONFIRM] ... 
+
+   Default file is dwarfsave.sav, default extensie is sav
+
+   Schrijft de keywords en hun waarde in de genoemde (ASCII) file, 
+   wildcards zijn toegestaan. Default is *$*_*
+
+ dwrestore file [/CONFIRM] [/OVERWRITE]
+
+   Leest regels keyword=value van de genoemde file en definieert de
+   corresponderende symbolen.
+ 
+ dwview symbol,... [/EXTERN] [/GENERAL] [/INPUT=file] (=dwv)
+
+   Laat de waarde van symbolen zien:
+
+     Zonder /GENERAL en /INPUT:   
+       Symbols moeten de vorm [[program]$stream_]keyword hebben,
+       wildcards toegestaan. Laat zowel interne als externe defaults
+       zien, als /EXTERN alleen de externe (zowel "local" als "NGEN").
+
+     Met /INPUT:
+       Leest als dwrestore van de genoemde file, laat keywords zien      
+       die matchen met de genoemde symbols.
+
+     Met /GENERAL:   (optie gemaakt 28/07/93)
+       Symbols mag zowel DWARF keywords als algemene symbols bevatten,
+       wildcards toegestaan (bv: dwv /g *).
+       Voor keywords: alleen externde defaults worden getoond.
+       Als er precies een symbool is opgegeven is de uitvoer de 
+       waarde van dat symbool, anders regels symbol=value.
+
+
+Een typische manier om standard streams te gebruiken is dus:
+
+  dwe nscan$abc /save [/norun]       of   dws nscan$abc /menu
+  dwe nplot$abc /save [/norun]       
+
+  dwsave *$abc /output=abc
+
+Tenslotte commentaar invoegen in abc.sav, eventueel nog wat keywords 
+van de /ask switch voorzien.
+
+Dan bij gebruik:
+
+   dwrestore abc /override
+
+   dwe nscan$abc
+   dwe nplot$abc
+
+
+
+
+
+
+3e. Antwoorden op prompts
+-------------------------
+
+Het programma bepaalt (via de PIN file) wat voor antwoorden geldig zijn
+(character strings, numeric values). Binnen de grenzen van die geldigheid
+kunnen de volgende constructies worden opgegeven:
+
+   ?                     Geef online help
+
+   # of ^D               Exit (meestal: vraag vorige keyword)
+
+   ""                    Empty answer (meestal: by-pass option)
+ 
+   *                     Wildcard (meestal: take all)
+
+   ... ! Comment         Alles na een uitroepteken is commentaar
+
+   ...'Symbol'...        Het symbol wordt vertaald voor alle verdere 
+                           processing
+
+   (1=2)*4               Rekenkundige expressies worden uitgewerkt
+                           (alleen voor numerieke waarden, dus wel voor
+                            INPUT_LABELS, niet voor LOOPS)
+
+   99 TO 120 BY 2        Reeksen worden gegeven als begin TO eind BY stap
+                           (alleen voor numerieke waarden, dus wel voor
+                            INPUT_LABELS, niet voor LOOPS)
+
+   ... /SAVE [/[NO]ASK]  Bewaar deze waarde na afloop van het programma in
+                           een DWARF symbol. De qualifier /ASK of /NOASK
+                           wordt in het symbool bewaard (geen qualifier
+                           betekent in praktijk: /NOASK)
+
+   value1; value2; ...   Geef een reeks waardes op, de volgende keer dat
+                           het keyword wordt gevraagd neemt het programma
+                           de eerstvolgende waarde
+
+   value1,value2         Geef een vector op, alle waardes worden meteen
+                           naar het programma doorgegeven
+
+   /ASK=keyword          Wanneer het programma het opgegeven keyword 
+                           nodig heeft krijgt de gebruiker een prompt;
+ 			   als deze qualifier gegeven is wordt het 
+                           huidige keyword nog een keer gevraagd.
+
+
+
+Nota Bene: er is geen snelle manier om hidden keywords te zetten als
+           het programma al draait. Met dws is dat wel mogelijk.
+
+
+
+4e. Scripts en batch processing
+-----------------------------------------------
+
+Er zijn twee manieren om Newstar (of eigenlijk: DWARF) in batch mode
+te gebruiken. De simpelste manier lijkt me via shell scripts, waarin 
+keywords worden gelezen met dwrestore en vervolgens de nodige programma's
+worden gedraaid. 
+
+Er is (voor WENSS) een "Batch package" ontworpen om de interactie met
+de keyword files te vereenvoudigen. Voor zover ik kan zien is de enige
+functie het overnemen van de dwrestore en het zetten van /ASK achter
+een aantal keywords. Dit weegt denk ik niet op tegen de extra moeite om
+voor elk programma een "batch versie" te maken. Ik zal hier nog wat 
+beter naar kijken. Je hoort er nog van.
+ 
+
+5e. Voorstel voor wijzigingen en uitbreidingen
+----------------------------------------------
+
+De volgende wijzigingen in het huidige systeem lijken me wenselijk:
+
+  - Alternatieve specificatie voor streams omdat $ een Unix special 
+    character is. Ik stel voor om voor stream specificaties zowel
+    een $ als een . toe te staan (bv dwe nscan.test of dwe nscan$test).
+
+  - Van keywords die als symbol gedefinieerd zijn met /NOASK moet tijdens
+    de uitvoering van het programma het keyword en de waarde worden 
+    afgedrukt.
+
+
+Een "conditionele" batch processing kan vrij makkelijk worden gerealiseerd
+door de Newstar programma's bepaalde interne waarden in een (algemeen) 
+symbol te laten zetten. Die waarden kunnen dan in het shell script worden
+opgevraagd en getest. Bv: bij NSCAN kan het aantal Channels in symbol
+NCHAN worden gezet, in het shell script kan dan een test worden gedaan
+
+   if (`dwv /General nchan` == 128) then ...
+
+of de waarde kan in een shell variabele worden gezet
+
+   set channels=`dwv /g nchan`
+
+of de waarde kan worden toegekend aan een keyword voor een ander programma
+
+   dws nmap\$1 /NOMENU <_EOD_
+LOOPS='NCHAN',...1
+#
+_EOD_
+
+
+Wanneer jullie doorgeven op welke parameters je wilt testen is het een 
+kleine moeite die waarden in een symbol te zetten. Wanneer je een 
+programma met /SAVE draait zijn alle antwoorden van de user in elk
+geval beschikbaar in symbolen, dus daar kun je ook op testen.
+
+
+----------
+
+Tot zover maar weer even. Ik maak hier nog een fatsoenlijk (Engels) document
+van, maar hiermee kunnen jullie denk ik wel even vooruit.
+
+Hartelijk groeten,
+
+Marco.
+
+
+
+--
+
+
+ +--------------------------------------------------------------------------+
+ | NFRA/St. ASTRON      | eMail:  devoscm@astro.rug.nl         /  cccccccc  |
+ | P.O. Box 2           |  or:    devoscm@nfra.nl            /   c m   m  c |
+ | NL-7900 AA Dwingeloo |                                  /    c m m m  c  |
+ |                      | ---------------------------------+  c  m   m  c   |
+ | Phone: +31 5219 7244  \  "If you reinvent the wheel,    |   v      v     |
+ | Fax:   +31 5219 7332   \  make sure yours will look     |    v   v       |
+ | Telex: 42043 rzm nl     | different..."                 |      v         |
+ +--------------------------------------------------------------------------+
+
+
+
diff --git a/src/doc/txt/bug_reports.txt b/src/doc/txt/bug_reports.txt
new file mode 100644
index 0000000000000000000000000000000000000000..0c65ed83723cb931125d341f93cfdd905f4af602
--- /dev/null
+++ b/src/doc/txt/bug_reports.txt
@@ -0,0 +1,434 @@
+Newstar Bug reporting procedure
+-------------------------------
+
+     bug_reports.txt  14/06/93 v1.0 CMV
+     bug_reports.txt  06/09/93 v1.2 CMV
+     JPH 940621	Add list of contents. Include bug_report.2 (=sec. 6.1)
+
+
+INHOUD
+======
+1. Inleiding
+2. Procedure
+3. Revisions en Releases
+4. Functionality Requests
+5. Implementatie: nbug
+6. Prioriteitsstelling
+6.1 Update on priorities
+7. Slotopmerkingen
+
+
+1. Inleiding
+------------
+
+Zolang een programmapakket door een beperkte groep gebruikt wordt, is
+er weinig noodzaak voor al te veel formele procedures. Naarmate het 
+pakket door een grotere groep, met een grotere geografische verspreiding
+wordt gebruikt werkt een aantal informele overlegcircuits niet meer en 
+moet er een aantal afspraken over tijdschema's en rapportage gemaakt worden.
+
+Die afspraken moeten het volgende garanderen:
+
+  1e. Gebruikers weten welke versie van het pakket voor hen draait,
+      en wat de (voornaamste) eigenschappen van die versie zijn.
+
+  2e. Gebruikers die een "bug" rapporteren worden regelmatig op de 
+      hoogte gehouden van de afhandeling van die bug.
+
+  3e. Programmeurs weten aan welke programma's gewerkt wordt.
+
+  4e. Er is een duidelijke prioriteitstelling voor de verschillende
+      onderhouds- en ontwikkelingstaken, waardoor niet onevenredig
+      veel tijd wordt besteed aan minder belangrijke klussen.
+
+  5e. Er zijn duidelijke overleg momenten, waardoor er doorlopend 
+      een optimale werkverdeling is.
+
+  6e. Er is een rapportage procedure, waardoor ervaring bij debugging 
+      voor het nageslacht bewaard blijft.
+
+Voor wat betreft Newstar zijn de meeste van die punten nu (informeel) 
+geregeld. Dit rapport probeert het geheel te structureren, uitgaande 
+van de afhandeling van bugs. Aangezien in mijn optiek missende
+functionaliteit ook een bug is (het jeukt net zo erg...) geldt het 
+verhaal in hoofdlijnen ook voor functionality requests.
+
+
+
+2. Procedure
+------------
+
+Afhandeling van een bug doorloopt de volgende fasen (tussen haakjes de
+status die na deze fase aan de fout wordt toegekend, zie sectie 5):
+
+ 1e. Ontvangst                                      (Received)
+ 2e. Prioriteitsstelling, toewijzing                (Assigned)
+ 3e. Bevestiging naar gebruiker                     (Confirmed)
+
+Tussen 1e. en 3e. mag hooguit twee dagen verstijken. De bevestiging kan 
+ook inhouden: dit heeft lage prioriteit, we houden u op de hoogte. Een 
+bevestiging kan ook plaatsvinden voor prioriteitsstelling.
+
+ 4e. Reproductie van de fout
+
+Als 4e. problemen geeft, wordt teruggekoppeld naar de gebruiker:
+architectuur/site specifieke problemen, kan gebruiker reproduceren?
+Wanneer dit onderdeel meer dan een dag in beslag neemt, moet de 
+prioriteitstelling opnieuw worden bekeken.
+
+ 5e. Analyse van de fout                            (Analysed)
+
+Hier wordt de set van modules/bestanden waar de fout in kan zitten 
+afgebakend: tracen van de fout, controleren van asynchrone effecten etc.
+Wanneer dit onderdeel meer dan een dag in beslag neemt, moet de 
+prioriteitstelling opnieuw worden bekeken. Afhankelijk van de locatie
+van de fout kan de bug worden doorgeschoven naar een andere programmeur
+(bv omdat die de modules geschreven of recent gewijzigd heeft).
+
+  6e. Formuleren van een oplossing of omleiding
+
+Wanneer dit onderdeel meer dan een week in beslag neemt, moet de
+prioriteitstelling opnieuw bekeken worden. Ook moet de gebruiker 
+een bericht krijgen dat de zaak wel eens wat langer kon duren.
+
+  7e. Implementeren van de oplossing of omleiding   (Solved)
+
+Als het implementeren van de geformuleerde oplossing langer dan een week
+duurt, moeten we terug naar 6e.
+
+  8e. Validatie van de oplossing of omleiding       (Tested)
+
+Eventueel worden de wijzigingen gecontroleerd door de oorspronkelijke
+auteur van de modules.
+De gebruiker wordt verzocht op zijn site een test te draaien met de
+gewijzigde modules (evt ftp van executable naar user systeem op die site).
+
+  9e. Afwikkeling van de fout                       (Released)
+
+De wijzigingen worden in de NFRA Master geupdate, inclusief wijzigingen
+van de documentatie.
+De gebruiker die de bug gemeld had, wordt op de hoogte gesteld,
+de master op zijn site wordt bijgewerkt. 
+Andere sites ontvangen een melding van de wijzigingen, en worden 
+eventueel bijgewerkt.
+
+
+3. Revisions en releases
+------------------------
+
+Bij wijzigingen in Newstar kunnen we twee gevallen onderscheiden:
+  - de wijziging heeft een minimale invloed op het gebruik van de 
+    programma's (afgezien van het ontbreken van crashes etc.); 
+    kleine toevoegingen in functionaliteit vallen hier ook onder
+  - de wijziging heeft invloed op het gebruik van de programma's
+    (veranderde keywords, noodzaak om SCN files te converteren etc)
+ 
+In het eerste geval spreken we van een revision van Newstar. Bij een 
+revision is het niet nodig dat elke gebruiker een melding van
+dit heuglijke feit ontvangt. Ook is het niet nodig dat alle sites
+een revision onmiddelijke ontvangen. Het exporteren van een revision
+gebeurt door een beperkt aantal bestanden over te zenden (via een
+revision groupfile: update retrieve .....grp)
+
+In het tweede geval spreken we van een release van Newstar.
+Een release wordt expliciet aangekondigd aan alle gebruikers (evt via
+locale Newstar managers). Een release wordt ge\"exporteerd naar alle
+sites. Voor een release wordt het volledige Master systeem van de site
+gecontroleerd: update retrieve all)
+
+
+4. Functionality requests
+-------------------------
+
+Voor functionality requests geldt in principe hetzelfde als voor bug,
+met dien verstande dat het reproduceren van de fout vervalt, en dat de
+overige stappen een langere tijdschaal hebben. 
+
+
+5. Implementatie: nbug
+----------------------
+
+In de NFRA Master staat een subdirectory $n_src/doc/bug waarin voor 
+elke bug een bestand wordt bijgehouden. Deze bestanden (project files)
+kunnen met de Hypertext browser worden bekeken via een aantal indexen. 
+Onderlinge verbindingen zijn mogelijk.
+
+Onafhankelijk van de manier waaop de bug binnenkomt (eMail, formulier AGB,
+telefonisch, wandelgangen) wordt een project file gemaakt. Als de bug 
+elektronisch gerapporteerd werd, kan het betreffende bestand aan de
+project file gekoppeld worden, anders moet de essentiele informatie 
+worden ingevoerd. 
+
+Wanneer nieuwe informatie beschikbaar komt (na toewijzing, bevestiging,
+oplossing etc) wordt die toegevoegd aan de project file, eventueel met 
+een gekoppeld tekstbestand.
+
+De bug-reports worden bijgehouden middels de utility "nbug", die een 
+hele reeks opties heeft. De meeste opties corresponderen met de diverse
+stadia die een bug in zijn carriere kan doorlopen.
+
+  add          Invoeren nieuwe bug (kent nummer toe, vraagt details)
+  confirm      Ontvangstbevestiging
+  priority     Prioriteitstelling (vraagt priority en assignment)
+  suspend      Wordt tijdelijk niet aan gewerkt (behoudt prioriteit)
+
+  analysed     Fout is gevonden
+  solved       Fout is opgelost
+  tested       Oplossing is getest
+
+  released     Nieuwe software is vrijgegeven (priority wordt -1)
+
+  feedback     Bevestiging van contact met melder
+  status       Vraagt status op van bepaalde bug (kan beter via hypertext)
+ 
+
+Bovenstaande opties vragen allemaal om een associated file en een
+comment, en geven de optie om de project file te editen (emacs of $EDITOR).
+Ze voeren ook automatisch een index commando uit. Indices kunnen op
+ieder moment gemaakt worden met de index optie:
+
+  index        Maakt de standard indexen voor de hypertext
+                 - Alle bugs op volgorde van nummer
+                 - Alle bugs op volgorde van prioriteit
+                 - Alle actieve bugs op volgorde van prioriteit
+
+Naast indices voor on-line toegang zijn (geprinte) lijsten vooralsnog
+van groot belang. De volgende lijsten kunnen met de ndoc optie "list"
+worden gemaakt:
+
+  list        Maakt lijsten voor printout
+    full        Alle bugs op volgorde van nummer
+    priority    Alle bugs op volgorde van prioriteit
+    active      Alle actieve bugs op volgorde van prioriteit
+    late        Alle "vertraagde" bugs, dat is: 
+                  - ontvangen en niet binnen twee dagen bevestigd 
+                  - niet suspended en geen feedback binnen twee weken 
+                  - suspended of released en geen feedback binnen twee dagen
+
+    user        Alle bugs van een bepaalde user (Pietje Puk etc)
+    programmer  Alle bugs van een bepaalde programmeur (HjV, WNB, ...)
+
+
+In de lijsten (en indices) verschijnt de bug als volgt:
+
+ID   Pr.ty Origin              Worker Status   Action/Feedback  Description
+------------------------------------------------------------------------------
+
+0024    10 verheijen           None   Confirmed  930806/930823  Gridding in ..
+0023   200 verheijen           CMV    Confirmed  930806/930823  NGIDS locks ..
+:
+0020     0 verheijen           None   Confirmed  930806/930823  NGIDS much t..
+0019   300 verheijen, WHISP    CMV    Confirmed  930806/930823  NGIDS flaggi..
+:
+
+De volgende bestanden zijn van belang voor nbug:
+ 
+   $n_src/doc/bug/n????.prj           Project file
+   $n_src/doc/bug/detail/n????.*      Alle overige documenten
+
+   $n_src/doc/bug/nbug.txt           "Home Page" met links naar indices
+   $n_src/doc/bug/nbug.idx            Index op nummer
+   $n_src/doc/bug/npriority.idx       Index op priority   
+   $n_src/doc/bug/nactive.idx         Index op priority voor actieve bugs
+   
+Al deze bestanden zijn normale ASCII file die naar believe kunnen worden
+bijgewerkt voor veranderingen die niet door nbug worden ondersteund.
+
+
+6. Prioriteitsstelling
+----------------------
+
+De voorlopige strategie voor de prioriteiten is als volgt:
+ 
+  - Prioriteiten lopen van 0 tot 900
+  - De honderdtallen doen dienst als grove prioriteitsklassen
+    Bugs uit 900-999 worden in principe het eerst aangepakt
+  - De tientallen doen dienst als een globaal werkschema binnen de
+    prioriteitsklassen. Bugs uit 990-999 worden in principe eerder
+    aangepakt dan bugs uit 980-989
+  - De eenheden zijn een kunstmatig middel om een bug omhoog te kunnen
+    schuiven zonder alle overige project files te moeten wijzigen.
+    Als een bug met prioriteit 700 zeer urgent wordt, urgenter dan 
+    bestaande bugs met prioriteit 980, dan wordt de prioriteit gewijzigd
+    naar 981.
+
+  - Een tijdslimiet of schatting kan als commentaar bij de prioriteit-
+    stelling worden gegeven.
+
+Een definitief systeem zal worden vastgesteld op basis van ervaringen met
+het huidige voorstel.
+
+
+6.1 Update on the priority system:
+---------------------------------
+
+There are now five priority classes:
+
+ 100      -   Critical bugs, that make it impossible to use vital programs
+ 200      -   Urgent requests or bugs
+ 300      -   Desirable things
+ 400/500  -   Pro memori
+
+The priority scheme does not show any timeslicing, but is complemented 
+in this respect by the Project Plan.
+
+The header tag Class has been added to distinguish between Bugs
+and Requests, the tag Category shows the program (e.g. NSCAN, NPLOT) 
+with which the Bug/Request is mainly concerned.
+
+
+7. Slotopmerkingen
+------------------
+
+Het moge duidelijk zijn dat een dergelijk systeem niet beperkt is tot 
+gebruik binnen Newstar. Met een aantal triviale wijzigingen in nbug
+is het mogelijk voor een willekeurig software project een dergelijke 
+rapportage op te zetten.
+
+Ook is deze strategie in principe bruikbaar voor alle processen waarbij 
+een "checklist" van status veranderingen moet worden bijgehouden. 
+Desgewenst kan de volgorde van veranderingen worden vastgelegd. 
+
+We kunnen nbug vergelijken met andere bug-reporting systemen (zoals bv het 
+GNATS systeem van GNU). Deze systemen hebben een grotere nadruk op 
+automatische interactie/responsies via electronische mail. De on-line 
+toegankelijkheid is kleiner dan bij nbug, evenals de centrale rapportage 
+mogelijkheden. Desgewenst kan meer eMail interactie worden ingebouwd in
+nbug. Dit lijkt me in de huidige situatie (waar verreweg de meeste 
+klachten verbaal worden ingediend) nauwelijks de moeite.
+
+
+ 
+  
+
+Appendix A: Casus
+-----------------
+
+> _nbug add_
+Creating bug-report project file with id-number 0036
+Enter name of file with associated eMail: _~devoscm/tmp_
+Enter origin [Pietje Puk]: __
+Enter email address [Unknown]: _puk@rux.timboektoe.edu_
+Enter subject [Unknown]: _Cannot make poststam images anymore_
+Any comments: _Seems the same old problem again_
+
+Please confirm the bug within two days and set a priority as soon 
+as possible. Indices for the bug-database will be updated.
+
+Edit the project file (y,n)? [n] _n_
+0036     0 Pietje Puk   None   Received   930909/000000
+     Cannot make poststamp images anymore
+Updating indices...
+
+After I called him back, I type...
+
+> _nbug confirm 36_
+0036     0 Pietje Puk   None   Received   930909/000000
+     Cannot make poststamp images anymore
+Any comments: _Called back, Mr. Puk seems quite upset about this_
+Associated file (may be -bugid or detail/...): __
+Edit the project file (y,n)? [n] __
+0036     0 Pietje Puk   None   Confirmed  930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+Then JEN decides this is quite important...
+
+> _nbug priority_
+Enter bug-id: _36_
+0036     0 Pietje Puk   None   Confirmed  930909/930909
+     Cannot make poststamp images anymore
+Enter (new) priority: _900_
+Assign job to: _HjV_
+Any comments: _Must be solved with a week_
+Associated file (may be -bugid or detail/...): __
+Edit the project file (y,n)? [n] __
+0036  1000 Pietje Puk   HjV    Assigned   930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+So it is analysed immediately...
+
+> _nbug analy 36_
+0036  1000 Pietje Puk   HjV    Assigned   930909/930909
+     Cannot make poststamp images anymore
+Any comments: _Missing check on array bounds in NPLSTM_
+Associated file (may be -bugid or detail/...): _test.log_
+
+Edit the project file (y,n)? [n] __
+0036  1000 Pietje Puk   HjV    Analysed   930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+And when Dr. Puk calls me occasionally...
+
+> _nbug feedback 36_
+0036  1000 Pietje Puk   HjV    Analysed   930909/930909
+     Cannot make poststamp images anymore
+Any comments: _Pietje called again, told him Henk found it_
+Associated file (may be -bugid or detail/...): __
+Edit the project file (y,n)? [n] __
+0036  1000 Pietje Puk   HjV    Analysed   930909/930909
+     Cannot make poststamp images anymore
+Updating indices...
+
+Etc.
+
+Appendix B: Format of project file and indices
+----------------------------------------------
+
+n0036.prj:
+------------------------------------------------------------
+ <TITLE>Newstar Bug Report # 0036</TITLE>
+
+ <H1>Newstar Bug Report # 0036 </H1>
+
+ <DT><STRONG>Origin:</STRONG>           Pietje Puk
+ <DT><STRONG>Address:</STRONG>          puk@rux.timboektoe.edu
+ <DT><STRONG>Subject:</STRONG>          Cannot make poststamp images anymore
+ <DT><STRONG>Status:</STRONG>           Analysed
+ <DT><STRONG>Priority:</STRONG>         1000
+ <DT><STRONG>Worker:</STRONG>           <A HREF=../html/people.html#HjV>HjV</A>
+ <DT><STRONG>Last action:</STRONG>      930909
+ <DT><STRONG>Last feedback:</STRONG>    930909
+
+ <P>
+ <H2>Detailed description</H2>
+
+ <P>
+ <H2>History</H2>
+
+ <DT>930909 18:05 - <STRONG>Received</STRONG> by Marco de Vos
+ <DD>Seems the same old problem again 
+ (<A HREF=detail/n0036.1>detail</A>)
+ <DT>930909 18:07 - <STRONG>Confirmed</STRONG> by Marco de Vos
+ <DD>Called back, Mr. Puk seems quite upset about this
+ <DT>930909 18:07 - <STRONG>Assigned (HjV, priority 1000)</STRONG> by Jan Noordam
+ <DD>Must be solved with a week
+ <DT>930909 18:08 - <STRONG>Analysed</STRONG> by Henk Vosmeijer
+ <DD>Missing check on array bounds in NPLSTM
+ (<A HREF=detail/n0036.2>detail</A>)
+ <DT>930909 18:09 - <STRONG>Feedback</STRONG> by Marco de Vos
+ <DD>Pietje called again, told him Henk found it
+------------------------------------------------------------
+
+
+nbug.idx:
+------------------------------------------------------------
+ <TITLE>Newstar Bug Index: all keys</TITLE>
+ <H1>Index of all bugs sorted on ID number</H1>
+
+ <P>
+ <LI> For an index sorted on priority, click <A HREF=npriority.idx>here</A>
+ <LI> For an index of active items only, click <A HREF=nactive.idx>here</A>
+ <P>
+
+ <TT><DT>BugID Pr.ty - Subject
+ <DD><STRONG>Status...</STRONG> - Action/Feedback 
+ (<EM>Origin</EM> - Worked on)</TT><P>
+
+ <TT><DT><A HREF=n0001.prj>0001</A>: +0000 </TT> - Lines in NPLOT to ...
+ <TT><DT><A HREF=n0002.prj>0002</A>: +0000 </TT> - Programs stay sile...
+
+------------------------------------------------------------
+
diff --git a/src/doc/txt/calibr_models.txt b/src/doc/txt/calibr_models.txt
new file mode 100644
index 0000000000000000000000000000000000000000..55773e795b16efd0583214c39a77ae58b2cdbbe1
--- /dev/null
+++ b/src/doc/txt/calibr_models.txt
@@ -0,0 +1,79 @@
+From Ger@NFRA.NL Mon Dec  4 16:34:33 1995
+Date: Mon, 04 Dec 1995 16:34:07 +0100 (MET)
+From: Ger@NFRA.NL (Ger de Bruyn)
+Subject: models at 92cm
+To: foley@NFRA.NL (Tony Foley)
+To: henk@NFRA.NL (Henk Vosmeijer)
+To: jph@NFRA.NL (Johan Hamaker)
+To: noordam@NFRA.NL (Jan Noordam)
+X-Envelope-To: hjv@RZMWS0.NFRA.NL, jph@RZMWS0.NFRA.NL, noordam@RZMWS0.NFRA.NL
+Mime-Version: 1.0
+X-Mailer: ELM [version 2.4 PL23]
+Content-Type: text/plain; charset=US-ASCII
+Content-Transfer-Encoding: 7bit
+Content-Length: 2446
+Status: RO
+X-Lines: 61
+
+Beste mensen,
+
+Op /user4/92calib staan 5 modellen voor 325 MHz
+van 5 in Westerbork gebruikte calibrators (3C48, 147,
+286, 295 en 345)
+
+Ze bevatten ruim honderd componenten, voldoende voor een
+nauwkeurige zelfcalibratie.
+
+Bedenk echter het volgende:
+
+1) Ze gelden voor 325 MHz en als je ze in NCALIB
+wilt gebruiken op andere banden van het
+breedband 92cm systeem moet de BEAM optie aangezet
+worden. Dat corrigeert dan in eerste orde (met behulp
+van  een (cos**6(cfr) functie) voor de veranderende primaire
+bundel (met c=0.0629 dat nu geldt voor alle
+frequenties beneden 500 MHz). Echter op de laagste frequenties
+is de bundel waarschijnlijk breder dan een simpele
+frequentie schaling. Daar moet dan dus een nieuwe 
+coefficient voor worden bepaald alsmede een nieuw frequentie
+interval waarvoor die constante geldt voor worden gecreeerd.
+
+2) De calibratie bronnen zijn in werkelijkheid natuurlijk minder sterk
+op de hogere frequenties. Maar om redenen uitgelegd in een
+README help file in dezelfde directory wordt daar NIET voor
+gecorrigeerd !! Daar moeten de astronomen zelf voor corrigeren
+met behulp van de spectrale indices van die bronnen.
+
+
+3) De bron 3C345 mag niet als flux calibrator gebruikt worden omdat
+hij in fluxdichtheid varieert. Deze bron wordt slechts zo af en toe
+gemeten om dat hij gepolariseerd is waardoor met behulp van het Stokes
+U signaal het phase verschil van de XX en YY kanalen gecontroleerd
+kan worden onder de aanname dat V=0 (VZERO optie in NCALIB-polar)
+Deze bron heeft ook een RM van ongeveer 15-20 rad/m**2 waardoor de
+Stokes Q en U percentages afhangen van frequentie.
+Deze percentages staan dus ook niet in het model.
+Ze zijn trouwens afhankelijk van de ionosferische Faraday draaiiing
+die niet nauwkeurig bekend is.
+
+4) Voor de bron 3C303 (die ook i.v.m. met zijn hoge lineaire
+polarisatie wordt waargeneomen, net als 3C345) 
+wacht ik nog steeds op een aantal metingen 
+waaruit ik een goede kaart kan maken waaruit een model te halen is.
+Verder geldt voor deze bron hetzelfde als voor 3C345 behalve dat hij
+niet verandert in flux dichtheid.
+
+Henk: Kun jij deze modellen neerzetten op de plaats waar NEWSTAR
+zijn default modellen weghaalt.
+
+Als er vragen zijn dan hoor ik het wel.
+
+Ger
+-- 
+
+A.G. de Bruyn  (Ger)           | Internet:   ger@nfra.nl
+NFRA                           | 
+Postbus 2                      | Phone: (31)-521-595257
+7990 AA Dwingeloo              | Fax:   (31)-521-597332 
+The Netherlands
+
diff --git a/src/doc/txt/control_c.txt b/src/doc/txt/control_c.txt
new file mode 100644
index 0000000000000000000000000000000000000000..8f09648f448cff2d8b7f88fdf36c6a44826e8168
--- /dev/null
+++ b/src/doc/txt/control_c.txt
@@ -0,0 +1,38 @@
+Trapping control-C in Newstar programs -------------------------------------- 
+
+        (contributed by JPH 941005, gleaned from wndpar_x.fun, wngex.for) 
+
+
+
+
+        INCLUDE WXH_DEF ... 
+        XHCC(0)=1                       ! inhibit ... 
+        XHCC(0)=0                       ! clear 
+        IF (XHCC(1) .NE.0) THEN         ! was a control-C caught? 
+          XHCC(1)=0 
+          <action, typically CALL WNGEX> 
+        ENDIF 
+
+        This code has been used to create module WNGCC with entry points 
+
+                WNGCCD          disable control-C 
+                WNGCCE          enable control-C 
+                LOGICAL WNGCCC  check and reset 'control-c seen' status
+
+and several other entry points to check, count and reset the number of
+interrupts seen. 
+
+
+        The implementation is in entry point WNGEX0 in wngex.for. This routine
+is declared the handler for signal SIGINT by wngsxh.fsc. Its action is very
+simple: 
+
+        if xhcc(0) !=0 
+                xhcc(1)+=1 
+        else 
+                fall through to WNGEX 
+
+        endif 
+
+
+
diff --git a/src/doc/txt/copyright.txt b/src/doc/txt/copyright.txt
new file mode 100644
index 0000000000000000000000000000000000000000..8209468683845cd0fe3f8831c8a83f27369ed409
--- /dev/null
+++ b/src/doc/txt/copyright.txt
@@ -0,0 +1,157 @@
+NEWSTAR - Copyright Notice
+--------------------------
+
+    COPYRIGHT (c) 1991, 1994
+      by the Netherlands Foundation for Research in Astronomy
+
+    NFRA/St. ASTRON
+    P.O. Box 2
+    7990 AA Dwingeloo 
+    The Netherlands 
+
+
+     The information in this document is subject to change without
+     notice and should not be construed as a commitment by the NFRA.
+
+     The NFRA assumes no responsibility  for the use or reliability 
+     of the Newstar package and software exported together with it.
+
+     Permission to use, copy, and distribute Newstar software and its
+     documentation for any purpose is hereby granted, provided that
+     this copyright notice appears in all copies.
+
+     Permission to modify the software is granted, but not the right
+     to distribute the modified code. Modifications are to be distributed
+     exclusively through the Newstar Master Installation at the NFRA.
+     Please send any modifications to the Newstar manager who may 
+     include them in the Master Installation for further distribution.
+
+     Requests for copies of the Master Installation, for assistance with
+     the installation and for support of an unmodified version of the
+     Master Installation can be directed to the Newstar manager, who
+     can be reached by electronic mail as  newstar@nfra.nl  or through
+     the Newstar User Feedback System (refer to the documentation for
+     details). 
+
+
+     The Gipsy program gids and the giplib-library are distributed 
+     with Newstar. Gipsy is copyrighted by the Kapteyn Astronomical
+     Institute, University of Groningen. The original copyright notice 
+     for the Gipsy software is included at the end of this document.
+
+     A binary version of the Mosaic hypertext browser, developed at 
+     the NCSA (Illinois) is distributed with Newstar. The original
+     copyright notice for Mosaic is included at the end of this document.
+
+     Newstar includes a modified version of the X11-driver originally
+     developed for the PGPLOT package by Tim Pearson (Caltech). 
+
+
+
+COPYRIGHT Release 3.5
+
+                  Groningen Image Processing SYstem (GIPSY)
+
+                    COPYRIGHT (c) 1978, 1984, 1992, 1993, 1994
+
+                    Kapteyn Astronomical Institute,
+                    University of Groningen
+                    P.O. Box 800
+                    9700 AV Groningen
+                    The Netherlands
+
+
+     The information in this document is subject to change without
+     notice and should not be construed as a commitment by the Kapteyn
+     Astronomical Institute.
+
+     The Kapteyn Astronomical Institute assumes no responsibility  for
+     the use or reliability of its software.
+
+     Permission to use, copy, and distribute GIPSY software and its
+     documentation for any purpose is hereby granted, provided that
+     this copyright notice appears in all copies.
+
+     Permission to modify the software is granted, but not the right
+     to distribute the modified code. Modifications are to be distributed
+     via the GIPSY source server, which is currently kapteyn.astro.rug.nl.
+     You can send your modifications to the GIPSY manager, who will take
+     care of the distribution.
+
+     Permission to install modified or new code directly can be obtained
+     from the GIPSY Manager. The E-Mail address of the GIPSY Manager
+     is listed in $gip_sys/manager.mgr.
+
+     Reports of software failures will only be considered when you have
+     an automatic update of GIPSY sources installed at your site. See
+     $gip_sys/README.
+
+
+Everything not already copyrighted by CERN is copyrighted by NCSA
+(including the contents of the libhtmlw, libnet, libXmx, and src
+directories, but not including the contents of libdtm, which is
+entirely public domain).
+
+The official NCSA Mosaic copyright statement follows.
+
+/****************************************************************************
+ * NCSA Mosaic for the X Window System                                      *
+ * Software Development Group                                               *
+ * National Center for Supercomputing Applications                          *
+ * University of Illinois at Urbana-Champaign                               *
+ * 605 E. Springfield, Champaign IL 61820                                   *
+ * mosaic@ncsa.uiuc.edu                                                     *
+ *                                                                          *
+ * Copyright (C) 1993, Board of Trustees of the University of Illinois      *
+ *                                                                          *
+ * NCSA Mosaic software, both binary and source (hereafter, Software) is    *
+ * copyrighted by The Board of Trustees of the University of Illinois       *
+ * (UI), and ownership remains with the UI.                                 *
+ *                                                                          *
+ * The UI grants you (hereafter, Licensee) a license to use the Software    *
+ * for academic, research and internal business purposes only, without a    *
+ * fee.  Licensee may distribute the binary and source code (if released)   *
+ * to third parties provided that the copyright notice and this statement   *
+ * appears on all copies and that no charge is associated with such         *
+ * copies.                                                                  *
+ *                                                                          *
+ * Licensee may make derivative works.  However, if Licensee distributes    *
+ * any derivative work based on or derived from the Software, then          *
+ * Licensee will (1) notify NCSA regarding its distribution of the          *
+ * derivative work, and (2) clearly notify users that such derivative       *
+ * work is a modified version and not the original NCSA Mosaic              *
+ * distributed by the UI.                                                   *
+ *                                                                          *
+ * Any Licensee wishing to make commercial use of the Software should       *
+ * contact the UI, c/o NCSA, to negotiate an appropriate license for such   *
+ * commercial use.  Commercial use includes (1) integration of all or       *
+ * part of the source code into a product for sale or license by or on      *
+ * behalf of Licensee to third parties, or (2) distribution of the binary   *
+ * code or source code to third parties that need it to utilize a           *
+ * commercial product sold or licensed by or on behalf of Licensee.         *
+ *                                                                          *
+ * UI MAKES NO REPRESENTATIONS ABOUT THE SUITABILITY OF THIS SOFTWARE FOR   *
+ * ANY PURPOSE.  IT IS PROVIDED "AS IS" WITHOUT EXPRESS OR IMPLIED          *
+ * WARRANTY.  THE UI SHALL NOT BE LIABLE FOR ANY DAMAGES SUFFERED BY THE    *
+ * USERS OF THIS SOFTWARE.                                                  *
+ *                                                                          *
+ * By using or copying this Software, Licensee agrees to abide by the       *
+ * copyright law and all other applicable laws of the U.S. including, but   *
+ * not limited to, export control laws, and the terms of this license.      *
+ * UI shall have the right to terminate this license immediately by         *
+ * written notice upon Licensee's breach of, or non-compliance with, any    *
+ * of its terms.  Licensee may be held legally responsible for any          *
+ * copyright infringement that is caused or encouraged by Licensee's        *
+ * failure to abide by the terms of this license.                           *
+ *                                                                          *
+ * Comments and questions are welcome and can be sent to                    *
+ * mosaic-x@ncsa.uiuc.edu.                                                  *
+ ****************************************************************************/
+
+For more information on copyright and licensing issues, contact:
+
+Marc Andreessen 
+Software Development Group
+National Center for Supercomputing Applications
+605 E. Springfield, Champaign IL 61820
+marca@ncsa.uiuc.edu
diff --git a/src/doc/txt/debug_efficiently.txt b/src/doc/txt/debug_efficiently.txt
new file mode 100644
index 0000000000000000000000000000000000000000..9d6ad328325e8dbb362ede302dcae95ebf598ba2
--- /dev/null
+++ b/src/doc/txt/debug_efficiently.txt
@@ -0,0 +1,36 @@
+Efficient use of the dbx debugger on the SUNs
+---------------------------------------------
+
+(contributed by JPH 940919; based on research by CMV)
+
+
+	For the convenience of programmers who want to use dbx with Newstar
+programs, the objects in the Newstar libraries are routinely compiled with the
+-g option (Newstar nsh option 'build -d') which creates objects including the
+necessary symbolic information. When an executable is built with this same
+option, all this information is carried over, resulting in a .exe file in which
+all modules are accessible to dbx.
+
+	This is very convenient for a programmer who needs access not only to
+modules that he is modifying in his own shadow system but also to other
+unmodified modules in the master libraries; indeed, there is no need for him to
+copy master files to his shadow system for the mere purpose of recompiling them.
+	The disadvantage is that the .exe file carries a huge ballast of
+symbolic information (typically several hundred thousands of items) which take
+a long time (many minutes) to load at the expense of a more than unmodest
+consumption of machine resources.
+
+	CMV found the following simple procedure to load only those symbols
+that one actually needs:
+
+	> dbx
+	dbx> modules select <object_1>.o, <object_2>.o, ...
+	dbx> debug <$n_exe/<program>.exe
+	dbx> <set breakpoints or whatever>
+	dbx> run
+
+Should one discover in the subsequent debugging session that more modules are
+needed, then one may restart the above sequence without leaving dbx.
+Breakpoints and the like remain valid, but the modules selected before must
+again be spelled out, - this is not nice but usually one needs only a few ...
+
diff --git a/src/doc/txt/doc_organisation.txt b/src/doc/txt/doc_organisation.txt
new file mode 100644
index 0000000000000000000000000000000000000000..4f37612030a1c841c912ceebdf8e8aa56c342538
--- /dev/null
+++ b/src/doc/txt/doc_organisation.txt
@@ -0,0 +1,776 @@
+The Organisation of Newstar documentation
+-----------------------------------------
+
+
+@(#) newdoc.txt  v1.6 08/09/93 CMV
+     newdoc.txt  v1.5 03/09/93 CMV
+     newdoc.txt  v1.4 05/08/93 CMV
+
+
+1. Introduction
+---------------
+
+
+This document defines the format and organisation of the Newstar 
+documentation. The next sections describe the way documentation can be 
+accessed, the way in which the documentation as a whole is organised and
+the way in which documentation should be formatted. This corresponds to the
+the point of view of a user, a Newstar site manager and a documentation 
+editor respectively. Appendices give detailed instructions for naming 
+conventions and editing.
+
+End-users who are just interested in using the documentation only
+need to read section 2, site managers and contributors should read
+the remaining sections as well.
+
+
+2. Accessebility
+----------------
+
+The Newstar user documentation is accessible in three forms:
+
+  1e. As on-line help from program prompts, either as "dumb-terminal"
+      text or through NCSA's xmosaic browser decribed below.
+
+  2e. By browsing the documentation using xmosaic or any other 
+      hypertext reader (e.g. the "dumb-terminal" reader for the
+      World Wide Web, developed at CERN)
+
+  3e. By reading the printed form of the documentation (the Newstar
+      Cookbook) either on paper or using an appropriate Postscript or
+      dvi viewer.
+
+
+The documentation is organised as a hypertext network, which means that
+various smaller pieces of information are connected by "links". This
+not only gives flexible index and glossary functions, but also allows for 
+a menu-like presentation of the on-line documentation (options 1e and
+2e). The pieces of information can also be put together in a single 
+large document, the Newstar Cookbook, where "links" show up as the
+usual references like "see also section 1.3".
+
+To access the on-line documentation, the user enters one or more
+questionmarks (?) in response to a prompt. If a single ? is entered,
+the help text will be shown on the terminal screen. If more than 
+one ? is entered, a separate window will be opened in which xmosaic 
+presents the requested information. If no window could be started,
+the help text will be given on the terminal. When an xmosaic window
+is open, all help text will be presented there, regardless of the
+number of questionmarks typed. The window remains active when the
+program quits, so the same window can be used by several programs 
+(so far only if run on the same host).  Xmosaic has been developed at 
+the NCSA and has many interesting options which fall outside the 
+scope of this document. 
+
+If the information is shown through xmosaic, the user can access the 
+remainder of the documentation though that browser. Certain words in 
+the text will appear underlined. The user can move the mouse on one
+of these words and click the left mouse button. Xmosaic will now display
+the information that is associated with the underlined word. This can 
+be a brief explanation of that word (glossary function) or a related 
+piece of documentation.
+
+Any help text explaining a prompt will have at least the following links
+appended to it (words within underscores will appear underlined):
+
+    More information:
+         _List of keywords_ for NSCAN
+         _The Newstar Cookbook_
+         Description of _program NSCAN_
+         Description of _common keywords_
+         The _DWARF User Interface_
+
+The list of keywords for any program will have the following list appended
+to it:
+
+    More information:
+         _The Newstar Cookbook_
+         Description of _program NSCAN_
+         Description of _common keywords_
+         
+Prompts related to specific file types will also contain links to
+documents revealing the secrets of such files.
+
+The hypertext network can also be accessed from outside a Newstar program
+by typing "nhyper" at the command line. This will present you a page
+with general information containing links to the table of contents of 
+the Newstar Cookbook and to some general help files (in particular the
+Newstar News file).
+
+
+3. Organisation
+---------------
+
+There are four different sources of information for the Newstar 
+documentation:
+
+  - Cookbook sections, which are LaTeX documents (with some restrictions
+    on the commands to be used, see below). They may contain ordinary
+    text, terminal scripts (created with help of "nscript", see below)
+    and may include postscript figures. These LaTeX files are translated
+    into the HTML format for inclusion in the hypertext network.
+
+    The LaTeX source files are all found in directory $n_src/doc/cook
+    The HTML versions are found in directory $n_src/doc/html
+ 
+
+  - Descriptive text (help-text) for program keywords, stored in 
+    so called PIN files (extensions .pin, .psc or .pef). The PIN files
+    are translated into LaTeX (for inclusion in the printed version
+    of the cookbook) and into HTML for inclusion in the hypertext
+    network. 
+
+    The PIN files are located in $n_src/nscan etc.
+    The LaTeX versions are found in directory $n_src/doc/cook
+    The HTML  versions are found in directory $n_src/doc/html
+
+
+  - Miscellaneous documents called Memo's, which are generally plain
+    ASCII files. For details on Newstar Memo's, refer to document
+    newmemo.txt
+
+    The NEWSTAR Memo's are found in directory $n_src/doc/memo
+
+  - Program source files can contain specially marked documentation
+    which can be extracted. The extracted documentation can be included
+    in the hypertext network.
+
+    Documentation from file abc.def is stored in $n_src/doc/extractabc.def
+
+
+  - Bugreports, with their present status and history, are a separate 
+    issue and are described in document bug_reports.txt.
+
+    Bugreports are found in directory $n_src/doc/bug
+
+
+Apart from these files there are:
+ 
+  - Files with LaTeX commands used to generated printed versions of the
+    cookbook or parts thereof. These files are found in $n_src/doc/cook
+    and have names cb_*.tex
+
+  - Index files for the hypertext network, generated automatically in
+    directory $n_src/doc/html
+
+
+Files are maintained though utility $n_src/sys/document.csh which uses 
+the program docaid.c ($n_exe/docaid.exe).
+
+There is a groupfile $n_src/doc/doc.grp listing files in or below $n_src/doc
+that have been created "by hand". A groupfile $n_src/doc/auto.grp will be
+updated together with the hypertext indices.
+
+Note: the files in directories keys and html are derived from files in 
+the source tree ($n_src). These files are updated automatically when 
+other files (e.g. ppd-files) are being compiled.
+This validates the principle that the source tree contains only all
+files needed for installation. The alternative would be to create a 
+directory in either the library or the executable tree for
+documentation. However, I think it is important that a full set of 
+documentation is available before installation. In my opinion this 
+outweights the violation of the source tree policy. It also makes
+it possible that, at least for the time being, files in the keys 
+and html directory are explicitly updated at NFRA. 
+
+
+An update of the documentation proceeds as follows:
+
+ "ndoc keys all"  Convert all pin, psc and pef files to LaTeX and html files
+ "ndoc extr all"  Extract documentation from files in $n_src/sys
+ "ndoc html all"  Convert all cookbook sections to html files
+ "ndoc index"     Make indices for the files in the html directory
+
+A shorthand for these commands is:  "ndoc full"
+
+Updating the documentation takes a few minutes and needs to be done at
+a single host only for all machines that share a filesystem.
+
+Other options of ndoc are:
+
+ "ndoc script"    Start the script utility (see Appendix C)
+ "ndoc print"     Print part of the Newstar Cookbook 
+ "ndoc hyper"     Start the hypertext browser at the Newstar Home Page
+ "ndoc memo"      Insert an external file into the Newstar Memo system
+
+The print command will ask you for a cookbook file to print. 
+
+
+4. Formatting 
+-------------
+
+Since a large amount of documentation is available already in 
+LaTeX, we choose to use LaTeX as our principle documentation 
+format. Although it is probably easier to convert an html document 
+to a LaTeX source than vice versa, this approach allows us to make 
+a fast start. To facilate translation we put some constrains on the
+infinite flexibility of LaTeX. These are given in the "style guide"
+found as Appendix A.
+
+Appendix A lists the "allowed" LaTeX commands, these are the commands
+that will be recognised by the LaTeX to HTML converter. Any other
+command will, for the time being, show up as ordinary text in the 
+xmosaic browser.
+
+The most important rules for writing documentation are the following:
+
+    1e. The basic element of Cookbook documentation is the section.
+        Each section should appear in a separate file.
+        It is well possible (and in fact preferable) to break
+        up sections in smaller units. 
+
+    2e. Figures, tables and other blocks containing large amounts 
+        of LaTeX commands not listed in Appendix A should be put in the
+        Cookbook by means of an \input or \include command. The embedding
+        commands (like \begin{figure} and \end{figure}) should also be
+        in that separate file. 
+
+        Such figures and tables will be converted to dvi or postscript 
+        files in the html directory.
+
+    3e. Terminal sessions can be included within cookbook sections.
+        However, for extended examples it is better to put them in a
+        separate file which is included by an \input or \include command.
+        This makes the hypertext more readable and facilates regeneration
+        if the programs change.
+
+        For a list of the LaTeX commands that will appear in terminal 
+        sessions, refer to Appendix A.
+ 
+        Refer to Appendix C for instructions on how to make 
+        terminal sessions using the  nscript command
+
+    4e. Within a section, the target of a hypertext link is marked 
+        through the \label command. See the naming conventions in 
+        Appendix B (eg. \label{nscan.descr.general}) 
+
+    5e. Within a section, a hypertext link is made though the \ref, \refn, 
+        \input and \include commands. The \input and \include commands
+        will translate to a lines: "See also: _Name of the include file_" 
+        in the browser. The \ref command will translate as follows:
+
+         ... This is explained in \ref{nscan.descr} where we see ...    ->
+         ... This is explained in _here_ where we see ...
+
+         ... This is explained in \ref{nscan.descr}{Chapter 4} ...    ->
+         ... This is explained in _Chapter 4_ ...
+
+        The last for will give a somewhat confusing output in the 
+        printed version.
+ 
+    6e. Within PIN files, links can also be made through the \ref command. 
+        In the "dumb-terminal" on-line help, these \ref commands show up 
+        as text and may at best serve as an entry in the printed version 
+        of the Cookbook.
+
+    7e. Filenames and labels should obey a strict naming scheme to 
+        allow for the proper files to be constructed. This naming 
+        scheme is given in Appendix B.
+
+
+5. Contributing to the Newstar documentation
+--------------------------------------------
+
+Contributions to the Newstar documentation are very welcome, in particular
+new recipes are appreciated. To contribute a recipe, put your text in a 
+file either as plain ASCII (with some indication as to sections etc) or
+using the LaTeX commands from Appendix A. Preferably you should use the 
+naming conventions from Appendix B. Send the files to me and we will put
+them in their proper place.
+
+
+    
+Appendix A:  Style Guide for the Newstar Cookbook
+----------
+
+The following conventions should be obeyed when writing LaTeX documents
+that should be converted to html using the docaid program:
+
+ - Only commands in the recognised subset (see below) may be used.
+
+ - The \begin{...} and \end{...} commands should be on a line of 
+   their own.
+
+ - To change font temporarily, use something like {\bf ...}, without
+   any space between the brace and \bf. Curently recognised fonts 
+   are:     \rm \bf \it \tt \tiny
+
+ - For verbatim text use either 
+
+      \begin{verbatim}
+      ...
+      \end{verbatim}
+
+   or {\tt ...} (with special characters escaped).
+   The commands used by nscript (\sline etc) use the latter strategy.
+
+ - The tabbing environment can be used inside documents with the
+   following restrictions. There should be a single definition line 
+   (with \= commands), which should follow the \begin{tabbing} line
+   without intervening empty/comment lines. The definition line will
+   not be copied to the hypertext, so use the \kill command.
+
+   Since tabbing in HTML is extremely poor, do not expect to much of 
+   presentation in xmosaic.
+
+ 
+The following subset of LaTeX commands is currently recognised by docaid.
+
+/*
+
+   Translation table for LaTeX to html
+   
+   Format: 
+
+     Column 1: name of the command (minimal match) without leading \
+     Column 2: length of command (all zero's, set by program)
+     Column 3: action routine
+                 NULL  No special action (just print replacement string)
+                _PUSH  Print closing tag for the replacement string when
+                        closing } is found
+                _SKIP  Skip any arghuments to the command
+                other  Special action, refer to code for details
+     Column 4: replacement string (or NULL if none)
+     
+    
+   Any LaTeX commands that do not start with a \ are handled separately,
+   however they are included in this table inside comments.
+
+*/
+     
+/*
+     The following lines correspond to definitions in cb_symbols.tex
+     Please update this list when cb_symbols.tex is changed
+*/
+   "cbdir",     0, NULL, "$n_src/doc/cook",
+   "NEWSTAR",   0, NULL, "<EM>NEWSTAR</EM>",
+   "Nseries",   0, NULL, "<EM>NEWSTAR</EM>",
+
+   "cVis",      0, NULL, "<EM>V</EM>",   
+   "pvis",      0, NULL, "<EM>Phi</EM>",
+   "avis",      0, NULL, "<EM>|V|</EM>",
+   "lavis",     0, NULL, "<EM>rho</EM>",
+
+   "cGain",     0, NULL, "<EM>G</EM>",
+   "cNoise",    0, NULL, "<EM>N</EM>",
+   "cCadd",     0, NULL, "<EM>C</EM>",
+
+   "perr",      0, NULL, "<EM>p</EM>",
+   "gerr",      0, NULL, "<EM>g</EM>",
+   "lerr",      0, NULL, "<EM>q</EM>",
+   "dang",      0, NULL, "<EM>phi</EM>",
+   "derr",      0, NULL, "<EM>Delta</EM>",
+   "eerr",      0, NULL, "<EM>Theta</EM>",
+
+   "Apol",      0, NULL, "<EM>epsilon</EM>",
+   "Bpol",      0, NULL, "<EM>eta</EM>",
+
+   "wgt",       0, NULL, "<EM>W</EM>",
+   "pwgt",      0, NULL, "<EM>W**p</EM>",
+   "lwgt",      0, NULL, "<EM>W**g</EM>",
+
+   "pzd",       0, NULL, "<EM>psi</EM>",
+
+   "farang",    0, NULL, "<EM>chi</EM>",
+
+/*
+   Here are the commands defined in cb_preamble.tex
+   Please update this list when cb_preamble.tex is changed
+*/
+  
+   "cbfile{",    0, _PUSH, "<TT>",
+   
+   "skeyword{",  0, _PUSH, "<DD><STRONG>",
+   "sprompt{",   0, _PUSH, "<EM>",
+   "sdefault{",  0, _PUSH, NULL,
+   "suser{",     0, _PUSH, " <KBD>",
+   "sline{",     0, _PUSH, "<DD><SAMP>",
+   "slong{",     0, _PUSH, "<DD><SAMP>",
+   "sskip",      0, NULL,  "<P>",
+   "scmd{",      0, _PUSH, "<DD>&gt; <KBD>",
+
+   "sinline{",  0, _PUSH, " . . . <EM>",
+   "scomment{", 0, _PUSH, "<EM><P>",
+
+   "setc",      0, NULL,  "<P>:<P>:<P>",   
+   "scr",       0, NULL,  "&lt;CR&gt;",
+   "gloshead{", 0, _PUSH, "<H2>",
+
+
+/*
+   Now follow the supported built-in LaTeX special characters
+
+   A tilde (~, smallspace) is replaced by an normal space character
+
+   Please mind that all commands below are prefixed by a backslash!
+*/
+
+   " ",          0, NULL, " ",
+   "$",          0, NULL, "$",
+   "#",          0, NULL, "#",
+   "&",          0, NULL, "&amp;",
+   "{",          0, NULL, "{",
+   "}",          0, NULL, "}",
+   "%",          0, NULL, "%",
+   "_",          0, NULL, "_",
+   "-",          0, NULL, NULL,
+   "\"o",        0, NULL, "&ouml;",
+   "wedge",      0, NULL, "^",
+
+   "arctan",     0, NULL, "<STRONG>arctan</STRONG>",
+   "ast",        0, NULL, "*",
+   "bigotimes",  0, NULL, "<STRONG>*</STRONG>",
+   "cdots",      0, NULL, "...",
+   "circ",       0, NULL, "o",
+   "copyright",  0, NULL, "(c)",
+   "delta",      0, NULL, "<EM>delta</EM>",
+   "div",        0, NULL, "-/-",
+   "equiv",      0, NULL, "==",
+   "exp",        0, NULL, "<STRONG>exp</STRONG>",
+   "gg",         0, NULL, "&gt;&gt;",
+   "infty",      0, NULL, "<STRONG>inf</STRONG>",
+   "lambda",     0, NULL, "<EM>lambda</EM>",
+   "ldots",      0, NULL, "...",
+   "log",        0, NULL, "<STRONG>log</STRONG>",
+   "over",       0, NULL, "/",
+   "phi",        0, NULL, "<EM>phi</EM>",
+   "pm",         0, NULL, "+/-",
+   "rightarrow", 0, NULL, "--&gt;",
+   "sigma",      0, NULL, "<EM>sigma</EM>",
+   "sqrt",       0, NULL, "<STRONG>sqrt</STRONG>",
+   "sum",        0, NULL, "<STRONG>SUM</STRONG>",
+   "theta",      0, NULL, "<EM>theta</EM>",
+   "times",      0, NULL, ".",
+   "vdots",      0, NULL, ":",
+
+/*
+   Line separating commands
+   
+   An empty line will also translate to a <P> tag
+*/
+   
+  "\\",                    0, NULL,         "<DD>", /* Trick to get newline */
+  "par",                   0, NULL,         "<P>",
+  "newpage",               0, NULL,         "<P>",
+  "vspace",                0, _SKIP,        "<P>",
+
+/*
+   Math modes
+   
+   $>$ and $<$ translate to the &gt; and &lt; entities,
+   any other $ .... $ construct is identical to \( ... \)
+   
+   $$ ... $$ constructs are identical to \[ ... \]
+*/
+                                                       /* Inline math mode  */
+  "(",                     0, NULL,         "  <EM> ",
+  ")",                     0, NULL,         " </EM> ",
+  "begin{math}",           0, NULL,         "  <EM> ",
+  "end{math}",             0, NULL,         " </EM> ",
+                                                      /* Display math mode */
+  "[",                     0, NULL,         "<P><EM>",
+  "]",                     0, NULL,         "</EM><P>",  
+  "begin{displaymath}",    0, NULL,         "<P><EM>",  
+  "end{displaymath}",      0, NULL,         "</EM><P>",  
+  "begin{equation}",       0, NULL,         "<P><EM>",  
+  "end{equation}",         0, NULL,         "</EM><P>",  
+  "begin{eqnarray}",       0, NULL,         "<P><EM>",  
+  "end{eqnarray}",         0, NULL,         "</EM><P>",  
+
+/*
+  Headings and references
+*/
+  "title{",                0, _PUSH,        "<H1>",
+  "chapter{",              0, _PUSH,        "<H1>",
+  "section{",              0, _PUSH,        "<H1>",
+  "subsection{",           0, _PUSH,        "<H2>",
+  "subsubsection{",        0, _PUSH,        "<H3>",
+
+  "label{",                0, _LABEL,       NULL,
+  "ref{",                  0, _ANCHOR,      NULL,
+  "pageref{",              0, _ANCHOR,      NULL,
+  "input{",                0, _ANCINP,      NULL,
+  "include{",              0, _ANCINP,      NULL,
+
+  "eqno{",                 0, _PUSH,        "<EM>",
+ 
+/*
+  Many things are just ignored
+*/
+  "tableofcontents",       0, NULL,         NULL,
+  "listoffigures",         0, NULL,         NULL,
+  "listoftable",           0, NULL,         NULL,
+  "makeindex",             0, NULL,         NULL,
+  "documentstyle",         0, _SKIP,        NULL,
+  "hskip",                 0, _SKIP,        NULL,
+  "hspace",                0, _SKIP,        NULL,
+  "hline",                 0, NULL,         NULL,
+  "maketitle",             0, NULL,         NULL,
+  "nonumber",              0, NULL,         NULL,
+  "pagestyle",             0, _SKIP,        NULL,
+  "pagenumbering",         0, _SKIP,        NULL,
+  "parbox",                0, _SKIP,        NULL,
+
+/*
+  Special handling for some environments
+*/  
+  "begin{thebibliography}",0, NULL,         "<H1>Bibliography</H1>\n",
+  "end{thebibliography}",  0, NULL,         "<P>",
+  "bibitem",               0, _LABBIB,      NULL,
+  "cite",                  0, _ANCBIB,      NULL,
+
+  "begin{tabbing}",        0, _TABBING,     NULL,
+  "end{tabbing}",          0, _TABBING,     "<P>",
+  ">",                     0, NULL,         " ",
+
+  "begin{figure",          0, _FIGURE,      NULL,
+  "end{figure",            0, _FIGURE,      "<P>",
+  "begin{tab",             0, _TABLE,       NULL,
+  "end{tab",               0, _TABLE,       "<P>",
+  "caption{",              0, _PUSH,        "<EM>",
+  
+  "begin{enumerate}",      0, NULL,         "<OL>",
+  "end{enumerate}",        0, NULL,         "</OL>",
+
+  "begin{itemize}",        0, NULL,         "<UL>",
+  "end{itemize}",          0, NULL,         "</UL>",
+  "item{",                 0, _PUSH,        "<LI> <STRONG>",
+  "itemitem{",             0, _PUSH,        "<LI> <STRONG>",
+  "item",                  0, NULL,         "<LI>",
+  "itemitem",              0, NULL,         "<LI>",
+  
+  "begin{verbatim}",       0, _VERBON,      "<PRE>",
+  "begin{verbatim*}",      0, _VERBON,      "<PRE>",
+  "end{verbatim}",         0, _VERBOF,      "</PRE>",
+
+/*
+  All other environments are just skipped.
+  Note: the order in the table is important here!
+*/    
+  "begin{",                0, _SKIP,        "<P>",
+  "end{",                  0, _SKIP,        "<P>",
+  "author{",               0, _SKIP,        NULL,
+
+  "end",                   0, NULL,         NULL,
+
+/*
+  Font selections. These are special case things, since the required
+  syntax for a temporary font change is:
+  
+    {\bf ... }
+    
+  etc, so we test on the {\ rather than on the \
+
+  "rm",                    0, _PUSH,        "<STRONG>",
+  "bf",                    0, _PUSH,        "<STRONG>",
+  "em",                    0, _PUSH,        "<EM>",
+  "it",                    0, _PUSH,        "<EM>",
+  "tt",                    0, _PUSH,        "<TT>",
+
+  Any isolated occurence of a font change is just ignored.
+  So you should use   \chapter{{\it Something fresh}} 
+  and not             \chapter{\it Something fresh}
+  
+*/
+  "tiny",                  0, NULL,         NULL,
+  "bf",                    0, NULL,         NULL,
+  "it",                    0, NULL,         NULL,
+  "rm",                    0, NULL,         NULL,
+  "tt",                    0, NULL,         NULL,
+  
+/*
+  The end of the table should be marked by a NULL command!
+*/
+  NULL,                    0, NULL,         NULL
+
+
+
+Appendix B:  Naming convention for Newstar Documentation
+-----------  
+
+***** ALL LABELS AND FILENAMES SHOULD BE IN LOWER CASE *****
+
+
+1e. Labels
+
+The following conventions should be used for the naming of labels 
+and references (commands \ref{...}, \pageref{...} \label{...}):
+
+  - The name of the label should consist of two or more elements 
+    separated by dots. The first two elements uniquely identify the
+    file to which the reference is made. As a consequence all labels 
+    in a file start with the same two elements. The remaining
+    elements serve as a reference within the file.
+
+  - The label corresponding to a file  a_b    is  a.b
+    A label within this file might be  a.b.c  or  a.b.c.d 
+
+    The label corresponding to a file  a_b_x    is  a.b_x
+    A label within this file might be  a.b_x.c  or  a.b_x.c.d_y-z 
+
+  - References to keywords should be made as follows: 
+
+     \ref{<name of pin/psc/pef file>.<name of keyword>}
+
+ *   In general the name of the pin/psc/pef file will be the name of
+ *   the program. For common keywords (including things like SCN_SETS)
+ *   the name of the PEF file should be used!
+
+
+  - Figures, tables, formulea and other pieces of "difficult" LaTeX 
+    will be included as GIF images, and should therefore be in separate
+    files. These files should have names fig_*.tex, tab_*.tex and 
+    eqn_*.tex. Normal labeling conventions apply to such files.
+
+For bibliographic references (commands \bibitem and \cite) the normal
+LaTeX conventions apply.
+
+
+2e. Filenames
+
+The cookbook is built based on the following tree (all filenames have
+extension .tex):
+                                                    Label
+  cookbook  (tittle page, table of contents)        cookbook
+   |
+   |
+   +-- ch_biblio                                    ch.biblio
+   |
+   +-- ch_general                                   ch.general
+   |    |
+   |    +-- gen_intro                               gen.intro
+   |    :
+   |
+   +-- ch_recipes                                   ch.recipes
+   |    |
+   |    +-- rcp_line_21cm                           rcp.line_21cm
+   |    +-- rcp_linear_polarisation                 rcp.linear_polarisation
+   |    :
+   |
+   +-- ch_files                                     ch.files
+   |    |
+   |    +-- files_descr                             files.descr
+   |    +-- scn_descr                               scn.descr
+   |    +-- mdl_descr                               mdl.descr
+   |    :
+   |
+   +-- ch_programs                                  ch.programs
+   |    |
+   |    +-- common_descr                            common.descr
+   |    +-- common_keys                             common.keys
+   |    |    |
+   |    |    + ngen_comm                            ngen.comm
+   |    |    :
+   |    |
+   |    +-- nscan_descr                             nscan.descr
+   |    +-- nscan_keys                              nscan.keys
+   |    |    |
+   |    |    + ngen_short                           ngen.short
+   |    |    :
+   |    |
+   |    +-- ncalib_descr                            ncalib.descr
+   |    +-- ncalib_redun                            ncalib.redun
+   |    +-- ncalib_polar                            ncalib.polar
+   |    +-- ncalib_keys                             ncalib.keys
+   |    |
+   |    :
+   |
+   +-- ch_appendices                                ch.appendices
+        |
+        + apx_wsrtfactsheet                         apx.wsrtfactsheet
+        + apx_arquery                               apx.arquery
+        :
+
+
+Files with keyword descriptions are generated automatically from the
+pin/psc/pef files:
+
+  - Each pin, psc and pef file is translated into a single LaTeX file
+    <name>_keys.tex (for pin/psc) or <name>_comm.tex (for pef). These 
+    files contain the full description of each keyword define in the
+    pin/psc/pef file. For pef files, a keyword summary is generated 
+    in file <name>_short.tex. An INCLUDE=NAME_PEF keyword in a psc file 
+    will be translated in a \include{name_short} and a \ref{name.comm}
+  
+  - Each pin, psc and pef file is translated into a html file with
+    links to files with information on the individual keywords.
+    The index file has name <name>_keys.html (for pin/psc) or 
+    <name>_comm.html (for pef). The files with keyword information are
+    named <name>_<keyword>.html
+
+Files with names fig_*.tex, tab_*.tex and eqn_*.tex will be included
+as GIF figures.
+
+
+Appendix C:  Creating scripts of terminal sessions
+-----------
+
+To create a script of a terminal session, the command
+
+   $n_src/sys/document.csh script [file]    
+
+should be used, this is conveniently aliased to "nscript".
+If no filename is given, you will be prompted for one.
+
+This command will start the script command. The user has to initialise
+Newstar by typing "$go" (this is not necessary if initialisation is done
+in the user's .cshrc file). The initialisation procedure (in 
+$n_src/sys/newstar_init.csh) notices that the script utility is used 
+and will switch the DWARF bell "on". The prmpt will be set to "script> ".
+You can execute all commands you like and then enter either "exit" or ^D. 
+The terminal session will now be transformed to a LaTeX file, which you 
+can edit at wish.
+
+The nscript command will ask you wether the terminal script should be
+"Latex'ed" and printed or displayed (using xdvi, which should be in 
+your path). Often, you will want to edit the file first and then
+view it. This is possible by typing:
+
+    nscript -p [file]
+
+When answering to system prompts, you can add comments by prefixing 
+them with a semicolon followed by a hash mark, e.g.:
+
+ script> dwe nscan   ;# First we start reading data from tape
+ script> ls -l ;      # This gives a directory listing
+
+If the hash is the first non-blank character on the line, the comment 
+will be on a line of it's own.
+ 
+ script> # To start newstar, just type the following commands:
+
+
+When answering to DWARF prompts, you can add comments by prefixing
+them with an exclamation mark, e.g.:
+
+ LEVELS = -20 -10 : 20 ! For this test, we use a single level
+ OPTION (blabla) = QUIT : ! No further processing needed!
+
+In the latter example, the second exclamation mark will just show up
+as an exclamation mark (of course), the "empty" user respons will 
+translate to "<CR>" in the output.
+
+
+   NB: In order to facilate the script command, the DWARF "bell" is 
+       now rung at the start of the prompt (used to be at the end).
+       The exclamation-mark comments turned out to be an existing DWARF
+       feature that had somewhat faded in the mist of times.
+
+The following LaTeX commands are used in translated terminal sessions;
+they are defined for LaTeX in $n_src/doc/cook/cb_preamble.tex:
+
+   \skeyword{ name of keyword }
+   \sprompt{  text of prompt  }
+   \sdefault{ default value   }
+   \suser{    user response   }
+
+   \sline{    line with terminal output }
+   \slong{    long line with terminal output }
+
+   \scmd{      respons of user to operating system prompt }
+
+   \sinline{  inline comment }
+   \scomment{ comment that is on a line of it's own }
+   \setc      % Vertical dots replacing terminal output
+   \scr       % Carriage Return in fixed width font
+
diff --git a/src/doc/txt/dwcalc.txt b/src/doc/txt/dwcalc.txt
new file mode 100644
index 0000000000000000000000000000000000000000..9dccc78319cb0089a052f3a7a0ea7d481154b43c
--- /dev/null
+++ b/src/doc/txt/dwcalc.txt
@@ -0,0 +1,276 @@
+The desk-calcutor program DWCALC
+--------------------------------
+
+HISTORY: 
+	 This file was originally written as a VAX/VMS HELP file. The program
+dwcalc was part of the DWARF infrastructure which has been merged into Newstar.
+This file has been taken over essentially as it was found.
+
+	8-oct-86        Ger van Diepen
+	JPH 940718      Update for Newstar
+	JPH 940918      Formatting for line-breaking algorithm
+
+
+DWCALC 
+======
+
+The program DWCALC is a handy desk-calculator, allowing the use of expressions
+(with units), symbols and formulae.  It is derived from the Dutch image
+processing system DWARF.  (Dwingeloo Westerbork Astronomical Reduction
+Facility). 
+
+ The program is started by the command 'dwcalc'.  Qualifiers can be used to
+control the program. If they are given  at the 'dwcalc' command-line, they
+serve as a global qualifier.  Global qualifiers can be overridden for each
+individual expression-line  by ending the line with the qualifiers, preceeded
+by at least one space  (to distinguish it from the division operator).
+
+ The input expressions are read from stdin.  The results are listed on stdout.
+Optionally (part of) input and output can be logged.  All input is converted to
+uppercase, therefore input is NOT case-sensitive.
+
+
+EXPRESSIONS 
+===========
+ After having started the program, the program asks you for an expression.  By
+giving a null-answer the program will be stopped.  Typing a question mark
+starts a help session.  Typing UNIT=? will show you the available units on
+printer or terminal.
+
+Expressions have the normal arithmetical format, using +,-,*,/,**  and
+parentheses. Blanks and unary signs are allowed.  However, note that / cannot
+be preceeded by a blank to distinguish  it from the qualifier-indicator.  The
+relational operators .NOT.,.EQ.,.NE.,.GT.,.GE.,.LE. and .LT.  are also allowed.
+ Also available are:    - some built-in functions (goniometric, etc.)    - unit
+specification and conversion    - special format for time or positions (using
+colons)    - symbol definition and substitution
+
+Integer numbers can be specified in octal or hexadecimal  format (use %O, %X,
+resp.). 
+
+
+FUNCTIONS 
+=========
+
+The following functions (similar to Fortran) can be used in expressions:
+
+	MIN     MAX     (1-10 arguments)
+	SIN     COS     TAN
+	ASIN    ACOS    ATAN     ATAN2
+	ABS     EXP     LOG     LOG10    SQRT
+	TRUNC   ROUND   MOD     SIGN
+
+Default unit for goniometric function is degrees, which can be overridden via
+the /UNIT-qualifier or by giving the unit in the  expression.
+
+The result of SIGN is:
+	-1  for negative values
+	 0  for zero
+	 1  for positive values
+
+Note that conversion to integer format implies rounding.
+
+
+UNITS 
+=====
+
+CALCULATE is able of converting from one unit to another.  It converts the
+units given in the expression to the unit given by  the /UNIT-qualifier. The
+units must belong to the same group (so  conversion from SEC to KM is
+impossible). 
+
+A unit can be given at several places:
+
+	- after a number           e.g. 10DEG
+	- after a subexpression    e.g. (10+3)deg
+	- after a symbol           e.g. PI RAD
+
+ Note that in the last case the blank is significant, else it is  optional.
+
+
+TIME_POSITION 
+-------------
+
+Times and positions can be given in HH:MM:SS (or DD:MM:SS) format using colons
+as separators. A unit may follow the value. Each part can be a floating number,
+which may exceed 60.
+
+The output can also be listed in that format by giving  /UNIT=HMS or /UNIT=DMS.
+
+This sexagesimal format allows for easy addition, subtraction and  conversion
+of times and positions.
+
+
+SYMBOLS 
+=======
+
+Symbols are very useful for storing results and for handling formulae. Both
+symbol substitution and definition is possible in DWCALC. DWCALC will always
+define global symbols. It is also possible to use predefined local or global
+symbols,  either numeric or alphanumeric.
+
+By defining a formula as a symbol, it is very easy to calculate the result of
+the formula for several values of its parameters. E.g.
+
+	$ VOLUME = "4/3*pi*r**3"
+	$ CALC
+	   Expression: r=3
+	   Expression: volume
+	   Expression: r=10
+	   Expression: volume
+
+
+DEFINITION 
+----------
+
+A symbol can be defined by using the constructS:
+
+	symbol_name = expression
+	symbol_name = "expression"
+
+In the first case the expression is evaluated and the result will be assigned
+to the symbol. In the second case the expression-text is assigned to the
+symbol, which is useful for defining formulae.
+
+Note that DCL uses the same procedure.
+
+SUBSTITUTION 
+------------
+
+Symbols can be substituted in an expression by giving its name enclosed in
+apostrophes or giving its name without  apostrophes.
+
+In the former case its value is substituted literally.  In the latter case its
+value is treated as a subexpression. E.g. if I=3+4 then
+
+	3*'i'   results in 3*3+4   = 13 and
+	3*i     results in 3*(3+4) = 21
+
+Note that nested substitution is possible. Circular substitution is detected by
+allowing a maximum of 25 substitutions.
+
+
+Examples 
+========
+
+Convert miles to kilometers
+
+	 $ dwcalc          10mile /unit=km
+
+If a whole series must be done it would be better to do:
+
+	 $ dwcalc/unit=km
+	    10mile
+	    8 mile
+	    (1.25+3.48)mile
+
+Convert right ascension from HH:MM:SS to degrees.
+
+	 $ dwcalc/unit=deg 9:23:48.329 hms
+
+Convert a time to seconds
+
+	 $ dwcalc/unit=sec 9:23:48.329 hr
+
+Do some time calculation
+
+	 $ dwcalc/unit=hms 10:34:48 + 2::45 - :34:56.89
+
+Calculate an expression and define the symbol ABC The result must be an integer
+
+	 $ dwcalc ABC = (2.34 * pi)+8*-cos(135+pi*28) /unit=deg
+
+Define a formula and calculate it for several parameters
+
+	 $ dwcalc
+	    VOLUME = "4/3*PI*R**3"
+	    R=2
+	    VOLUME
+	    R=10
+	    VOLUME
+
+Convert from hexadecimal to decimal
+
+	  %x1a2f
+
+Convert from decimal to hexadecimal
+
+	  2546 /rad=x
+
+/UNIT 
+=====
+
+This qualifier defines the default unit for the given values  and the unit in
+which the result will be expressed.  In this way it can be used for converting
+rom one unit to another.  Note however that conversion between different groups
+of units  is not allowed (e.g. seconds to meters is illegal).
+
+From DCL the available units can be shown via the command PRTUNIT.  From
+CALCULATE they can be shown via UNIT=?.
+
+Default is no units.
+
+
+/RADIX 
+======
+
+This qualifier defines in which radix the output will be listed. Possible
+values are:
+
+     D   decimal
+     O   octal
+     X   hexadecimal
+
+The default is D. O and X force TYPE=J if type is non-integer.
+
+
+/TYPE 
+=====
+
+This qualifier defines in which format the output will be listed. Note that all
+calculations are done in double precision and that  the program tests on
+integer overflow before conversion to an  integer format.  Possible values are:
+
+     B   signed byte
+     I   signed word       (integer*2)
+     J   signed longword   (integer*4)
+     L   logical
+     R   single precision  (real*4)
+     D   double precision  (real*8)
+
+The default is D.
+
+
+/STREAM 
+=======
+
+This qualifier is special to DWARF. It controls the stream of the application
+symbols. The stream-name will be inserted in a symbol-name, if that symbol-name
+ has the format "image_keyword".
+
+Default is no stream.
+
+
+/LIST 
+=====
+
+This qualifier controls if the results will be listed. Normally you will always
+list the result, but in command-files  it can be useful to negate this
+qualifier (i.e. /NOLIST).
+
+Default is list.
+
+
+/LOG 
+====
+
+This qualifier controls if the expressions and results will be written in the
+log-file CALCULATE.LOG (in the default directory). This log-file is written in
+such a way that it can be executed as a DCL command-file or can be used as
+input for the ARCHIVE-programs. This means that most lines will be flagged with
+an exclamation mark  (indicating comments), but symbol definitions are valid
+commands,  which can be executed. In this way users can calculate complex
+expressions and define the  results as symbols in a subprocess and execute the
+log-file in the  main process in order to obtain the results.
+
+Default is no logging.
diff --git a/src/doc/txt/memos.txt b/src/doc/txt/memos.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6fc76ebf4f0749ad7556c3bba1ad7c1bdc8c0983
--- /dev/null
+++ b/src/doc/txt/memos.txt
@@ -0,0 +1,145 @@
+The NEWSTAR memo system
+-----------------------
+
+This memo proposes a format for software memo series. 
+The vital element in this format is the Memo Header which gives
+all vital information. The various header elements are described 
+with their possible values,
+
+The only implementation currently available is for Newstar memo's. Some
+sample headers from this series are added.
+
+
+1. Function of memo's
+---------------------
+
+The function of a memo series is to document a design process and to 
+offer a convenient place where notes of various kinds can be dumped.
+
+In order to achieve this, it is essential that the header of each note
+clearly states what the purpose, subject and intended audience is.
+
+That way, it is sufficient to browse the headers of memo's in order
+to find information relevant to a certain person or problem
+
+
+2. Layout of memo headers
+-------------------------
+
+A memo header consists of the following fields, some of which are 
+required, others are optional:
+
+ * Name of memo series + index number                 [Required]
+
+   In fact the name of the memo series is a first order
+   selection of the intended audience. 
+   The serial number should be assigned on a central basis (preferably 
+   some automated procedure) and runs incrementally from 1.
+
+ * Subject                                            [Required]
+
+   The subject or description should be one line of highly descriptive
+   information. Since this line will show up in overview indices, 
+   it has to contain sufficient information to identify the scope
+   of the memo.
+
+ * Author                                             [Required]
+
+   This is just a textual identification. Preferably some database
+   with additional information on Memo authors should exist (including
+   up to date information on (eMail) addresses).
+
+ * Date                                               [Required]
+
+   This should be the date of issue of the original memo, for
+   updates see the next section
+
+ * Status                                             [Optional]
+
+   Possible values:  Info Proposal Design 
+
+   More than one value may be given, the list of possible values
+   may be extended
+
+   IF MISSING a status of Info should be assumed
+
+ * Action                                             [Optional]
+
+   Possible values:    Decision  Read  Feedback
+   Optional extension: "before <date>"
+
+   The action should be taken before the specified date, if no date
+   is given this is NOT equivalent to "as soon as possible" (in that
+   case a specific date should be given) but to "not necessary"
+
+   IF MISSING a status of Read should be assumed
+
+   
+ * To                                                 [Required]
+
+   The intended audience. This may be a specific name (e.g. Dr. P. Puk),
+   a generic name (WHISP Project Team) or The ... Memo Series
+
+ * Summary                                            [Required]
+
+   The full header including the summary should not exeed a single
+   page. Since Memo's are intended to be brief, no more than the
+   summary will be required in many cases.
+
+ * Replaces                                           [Optional]
+
+   Gives the numbers of the memo's that become obsolete by this one.
+
+ * Update on                                          [Optional]
+
+   Gives the numbers of the memo's are updated by this one.
+
+
+3. An example: the Newstar Memo Series
+--------------------------------------
+
+The Newstar memo series is part of the hypertext network of Newstar 
+documentation. The header layout in current practice does not follow
+the proposal in all details. 
+
+The body of the memo can be in any form (WP, ASCII text, Hypertext, LaTeX).
+In order enter the memo into the memo series, one enters the command
+
+    ndoc memo new [file]
+
+This will assign a unique number to the memo and create an empty memo
+header. You will be prompted for all header entries, and in addition 
+be asked for memo's, bug-reports and source files with which the memo 
+is concerned. These references appear as hypertext links in the on-line 
+version of the memo, and in normal text in the memo header.
+
+The specified file (which may be "none") will be moved into the directory
+with memo headers. The final header page will be presented for editing, 
+together with the associated file. This is the time to fill in the summary
+(which may be copied from the associated file).
+
+After completion, an index of all memo's will be automatically updated.
+
+
+4. Updates on existing memo's
+-----------------------------
+
+If a memo is updated, it is advised to enter the updates as a separate memo,
+indicating the differences only. If a modified text is stored, users are 
+forced to read through the entire memo and the preceding version to find 
+the differences. 
+
+Only if a memo has been changed substantially, so it is in fact better 
+to go through the whole text once more, a new memo can be created to 
+replace the original one.
+
+The header fields "Replaces" and "Update on" should be used to 
+indicate such cases.
+
+In the on-line implementation of the Newstar Memo Series, the headers
+of the updated/replaced memo's are modified to reflect this information
+as well. People keeping a paper copy can replace their header pages
+with the updates.
+
+
+
diff --git a/src/doc/txt/models_and_maps.txt b/src/doc/txt/models_and_maps.txt
new file mode 100644
index 0000000000000000000000000000000000000000..c4b4bd644dd816f2aa9185cd233dba4b269a8d14
--- /dev/null
+++ b/src/doc/txt/models_and_maps.txt
@@ -0,0 +1,89 @@
+How to apply models when making maps
+------------------------------------
+
+1e. Models and scanfiles
+------------------------
+
+Models can exist in two places:
+
+   1e. As a list of model parameters in a Model (MDL) file
+   2e. As a list of model parameters and complex uv-data points
+         in a Scan (SCN) file
+
+The model-list and the uv-model in a SCN file are always in accordance 
+with each other. 
+
+Models are update in the SCN files after a respons to the MODEL_ACTION 
+prompt. MODEL_ACTION is in fact: "What model is actually going to be used
+for processing and what model will finally end up in the SCN file?"
+
+The MODEL_ACTION question is asked in many cases:
+  1e. After the NMODEL option SAVE has been choosen
+  2e. After the NMAP option SUBTRACT has been choosen
+  3e. After the NCALIB option REDUNDANCY has been choosen
+  4e. After the NFLAG flagging operation ARESID has been choosen
+
+In all cases, the MODEL_ACTION is preceded by the MODEL_OPTION prompt.
+This allows you to create a temporary model list in memory by reading
+MDL files or by creating model components "by hand". The temporary model 
+list can be editied as well.
+
+The MODEL_ACTION determines what model is actually used in the 
+following processing AND what model is stored in the SCN file
+
+                         Used            Stored
+MERGE                  SCN ^ List       SCN ^ List
+ADD                    SCN + List       SCN + List
+NEW                      List             List
+TEMP                     List             SCN
+INCR                   SCN + List         SCN
+
+SCN:   Model currently present in the SCN file
+List:  Model currently in memory (constructed at MODEL_OPTION)
+ ^     Combination of two models, with common components occuring only
+         once in the final model
+ +     Addition of the two models, components occuring in both models
+         are added as well, so they get the double amplitude
+
+Obviously, options MERGE and NEW will be most commonly used.
+
+Apart from this choice, MODEL_ACTION lets you decide how the model should
+be calculated: should band smearing and time smearing be taken into account,
+should instrumental polarisation be taken into account.
+
+
+2. Subtracting models with NMAP
+-------------------------------
+
+There are two ways to subtract a model from uv-data before a map is made:
+
+  1e. In NMAP, answer SUBTRACT=YES
+
+      You will be asked for MODEL_OPTION to construct a temporary list,
+      and for MODEL_ACTION to determine what model is to be used.
+
+      This way you cannot use just the model that is present in the SCN file.
+
+      Also, you cannot use different models for different sets or different
+      SCN files (NMAP allows you to combine various SCN files, and to make 
+      several maps based on several groups etc)
+
+
+  2e. With NMAP, use DEAPPLY=MOD and SUBTRACT=NO
+
+      The uv-model in the SCN file(s) will be subtracted from the uv-data 
+      it corresponds to. The uv-model is considered a modification of the
+      visibilities corresponding to an empty sky. Deapplying this 
+      modification thus corresponds to subtraction of the uv-model.
+
+      This way, you can only use the model that is present in the SCN file.
+      This way, you can use different models for different groups in a SCN 
+      file, and different models for different SCN files.
+
+      However, you cannot add sources from another model, and you cannot
+      control the BAND/TIME/INPOL parameters (you should have done this when
+      you put the model in the SCN file).
+
+The same reasoning applies to NCALIB and NFLAG.
+
+
diff --git a/src/doc/txt/more_on_batch.txt b/src/doc/txt/more_on_batch.txt
new file mode 100644
index 0000000000000000000000000000000000000000..306b40f416cb11255f2113d065c7b1bf84fe5801
--- /dev/null
+++ b/src/doc/txt/more_on_batch.txt
@@ -0,0 +1,230 @@
+Fm: Marco de Vos (Newstar Project Team)
+To: Ulrich Schwarz & Paul Stoppelenburg
+
+Subject: 
+Hints for batchprocessing with Newstar
+--------------------------------------
+
+
+A. Layout for a batch-script
+----------------------------
+
+Batch-scripts always have the follwing layout:
+
+>>>>>>>>>>>>>>>>>>> Example follows below this line >>>>>>>>>>>
+#!/bin/csh -f
+#
+# Startup Newstar
+#
+source ~newstar/src/sys/newstar_rug.csh
+
+#
+# Maybe some identification
+#
+echo "Name of the script: $0"     # Prints the name of the file
+echo "Purpose: ....."             # Print the purpose of the file
+
+#
+# Clear all symbols
+#
+dwc '*$ch0'
+
+#
+# Define the symbols for this job
+#
+dws nmap\$ch0 /nomenu <<_EOD_
+OPTION=MAKE;QUIT ! The QUIT is for final exit
+LOOPS="";#       ! The # is in case we want to stop at the SCN_NODE prompt
+SCN_NODE=obs2; ""/ask    ! Just set the two defaults (/ASK)
+SCN_SETS=0.0.0.0.0
+HA_RANGE= -90,90
+SELECT_IFRS= -mm,-ff;""  ! The second answer should be ""
+... etc ...
+#
+_EOD_
+
+#
+#  Start the program
+#
+dwe nmap\$ch0
+
+#
+#  End
+#
+<<<<<<<<<<<<<<<< End of example <<<<<<<<<<<<<<<<<<<<<<<<<<<<<<
+
+
+There may be many different dws and dwe commands in a single file.
+
+In stead of typing  nmap\$0  you can also use  'nmap$0'  .
+
+
+
+
+B. Starting a batch-script
+--------------------------
+
+To start such a batch script, just type it's name, eg:
+
+  > nmap0.scr
+
+This may give a message like:     nmap0.scr: Permission denied.
+
+In that case you sould first type:
+
+  > chmod a+x nmap0.scr
+
+to change the mode ("protection") of the file such that All users 
+can eXecute it. You probably created the script from scratch with 
+an editor, so Unix treated it as an ordinary text file.
+
+
+
+C. Starting batch jobs in the background
+----------------------------------------
+
+To start a batch job in the background, leaving your terminal free
+for other work, just type the following:
+
+   > nmap0.scr >& output_file &
+
+All output that normally was shown on your screen will now end up in 
+the file named output_file (you can use any name you like).
+
+To check wether the job is finished you can try:
+
+   > more output_file           shows all of the "screen output"
+   > tail output_file           shows the last 20 lines or so
+   > ps lws | grep nmap0.scr    shows the status of the process (with
+                                 elapsed time etc.), no output means
+                                 the batch is finished
+
+There is a Newstar command which will execute a job in the background
+and send the output to you by mail when it finishes. Just type:
+
+   > nspawn nmap0.scr 
+
+The "screen output" will end up in  nmap0.scr.output. 
+The mail will be sent using elm with the command as subject.
+
+NOTA BENE: If you start a job in the background, all parameters should
+           be known in advance. So you should not use /ASK when specifying
+           parameters.
+
+
+
+D. How to set the keywords for a program
+----------------------------------------
+
+In a batch-script, you can set keywords in two different ways:
+
+1e. Use the dwspecify (dws) command:
+
+dws nmap\$ch0 /nomenu <<_EOD_
+OPTION=first_answer;second_answer;third_answer
+SCN_NODE=TEST;""
+#
+_EOD_
+
+The sequence of the keywords is not relevant.
+Each keyword should be set like: KEYWORD= value (not: nmap$ch0_keyword=value).
+You can only specify the keywords for one program (and one stream).
+
+You can enter the KEYWORD=value lines by hand, or edit the output
+from dwsave (remove the PROGRAM$Stream_ prefixes!)
+
+Alternatively you can extract keywords from a logfile:
+
+   >  grep '^>' NMAP.LOG | sed -e 's/^>//'  > output_file
+
+If this seems an interesting option, I will create a Newstar command
+for it (to save innocent Unix users all the '^>' things).
+
+
+2e. Use the dwrestore command:
+
+
+Typically, you will now do the following:
+
+ > dwe ncalib\$ch0 /norun/save
+ > dwe nmap\$ch0 /norun/save
+ > dwsave nmap\$ch0 /output=nmap0.keys
+
+Now you may want to edit nmap0.keys, which contains lines like:
+
+ NMAP$1_LOOPS=""";#"
+ NMAP$1_OPTION="MAKE;#"
+ NMAP$1_RUN="YES"
+ NMAP$1_SCN_NODE=""""
+
+In the batch script, you say:
+
+dwrestore nmap0.keys
+
+
+3e. Combine the use of dws and dwrestore
+
+
+Suppose we want to do a job repeatedly with the parameters saved above,
+but with only SCN_SETS differing from command to command. We may then
+combine dws and dwrestore as follows:
+
+
+#!bin/csh
+#!/bin/csh -f
+#
+# Startup Newstar
+#
+source ~newstar/src/sys/newstar_rug.csh
+
+#
+# Maybe some identification
+#
+echo "Name of the script: $0"     # Prints the name of the file
+echo "Purpose: ....."             # Print the purpose of the file
+
+#
+# Clear all symbols
+#
+dwc '*'
+
+#
+# Set up all "global" symbols for this job
+#
+dwrestore nmap0.keys
+
+#
+# Start a loop over the sets
+#
+foreach set ( 0 1 3 4 )
+
+#
+# Define SCN_SETS for ncalib
+#
+dws ncalib\$ch0 /nomenu <<_EOD_
+SCN_SETS=0.0.$set
+#
+_EOD_
+
+#
+# Run ncalib for this set
+#
+dwe ncalib\$ch0
+
+#
+# Define SCN_SETS for nmap
+#
+dws nmap\$ch0 /nomenu <<_EOD_
+SCN_SETS=0.0.$set
+#
+_EOD_
+
+#
+# Run ncalib for this set
+#
+dwe nmap\$ch0
+
+#
+# Next set
+#
+end 
diff --git a/src/doc/txt/ncalib_vzero.txt b/src/doc/txt/ncalib_vzero.txt
new file mode 100644
index 0000000000000000000000000000000000000000..d2b9347543be8855aea80f016bedc91690398e36
--- /dev/null
+++ b/src/doc/txt/ncalib_vzero.txt
@@ -0,0 +1,82 @@
+The VZERO algorithm	- JPH 960212
+
+Summary
+-------
+	Following a query by Jayaram Chengalur, this note provides an exegesis of W.N. Brouw's algorithm for determining the phase-zero-difference ('PZD') between the XX and YY interferometer subsets as implemeneted in the Newstar program NCALIB. The 180-degree ambiguity suggested by Chengalur appears indeed to exist; I suggest that a check could be implemented to insure selection of the  proper value for the PZD.
+				-------------
+
+
+Brouw's algorithm
+-----------------
+	I reproduce here the relevant lines of code from the program module NCAPVZ where the PZD is calculated:
+
+
+ 1	    DO I1=0,STHJ(STH_NIFR_J)-1			!ALL IFRS
+ 2	      IF (WGT(I1,1).GT.0 .AND. WGT(I1,2).GT.0 .AND. !XY/YX PRESENT
+ 3	1		ABS(DATC(I1,2)).NE.0) THEN	!SOME POWER
+ 4		CF=1					!COEFFICIENT
+ 5		CW=-DATC(I1,2)*DATC(I1,1)		!-YX.XY
+ 6		R0=ABS(CW)				!WEIGHT
+ 7		IF (R0.NE.0)
+ 8	1		CALL WNMLMN(MAR,LSQ_C_COMPLEX,CF,R0,
+ 9	1			(DATC(I1,2)-CONJG(DATC(I1,1)))/SQRT(CW))
+			.
+			solve 
+			.
+	IF (ABS(CSOL).NE.0) THEN
+10	  XYDIF=ATAN2(AIMAG(CSOL),REAL(CSOL))		!GET ANGLE
+	ELSE
+	  XYDIF=0
+	END IF
+11	CALL WNCTXT(F_TP,'A complex angle of !EC9.2\(!EC9.2) '//
+	1		'or !EAR9.2 degrees',
+	1		CSOL,CME,XYDIF)
+C
+
+	1: Process all interferometers, I1 = interferometer index
+	2: DATC = cpomplex visibility, WGT = weight; the first index is the 
+	   interferometer number, second index is 1 for XY, 2 for YX. Check 
+	   validity of data: if weight WGT equals 0, point has been deleted.	
+	3: This check seems to be redundant: If either XY or YX is 0, so will 
+	   be R0 in line 6 and consequently lines 8 and 9 will be skipped.
+	5: CW = -XY.YX
+	6: R0 = weight of this interferometer in the solution.
+	7: If the weight is 0, bypass lines 8 and 9 including the division by
+	   sqrt(CW).
+	8: Accumulate sum of (XY-YX*)/sqrt(-XY.YX) with weights |XY.YX|.
+	10: The result is a complex number, the weighted average of the 
+	   quantities of line 9 over all interferometers; its argument is the 
+	   phase difference we were after.
+	11: The test displaying this result is a bit sloppy!
+ 
+So the quantity that is averaged (line 8) is
+
+		P = sqrt(XY/YX) - sqrt(YX*/YX).sqrt(YX/XY)
+
+
+Interpretation
+--------------
+
+	I suggest the following interpretation:
+
+We seek to minimise |V| by multiplying X with a factor a.e^(i.phi), so
+
+		YX' = YX.a^2.e^(2i.phi)
+
+making
+
+		P' = sqrt(XY/YX) - a.e^(i.phi).sqrt(YX/XY)
+
+Setting P' = 0 gives us 
+
+		a.e^(i.phi) = sum[sqrt(XY/YX)] / sum[sqrt(YX/XY)]
+
+The amplitude factor a should be 1 after XX and YY Selfcal, and could be used for a consistency check. NCALIB implicity displays its value by printing out a.e^(i.phi) as a 'complex angle', but otherwise ignores it. 
+
+
+The PZD ambiguity
+-----------------
+ 
+	The 180-degree ambiguity in the VZERO determination noted by Chengalur is represented in the algorithm above by the sign ambiguity of the sqrt() function. 
+
+	It seems to me that whatever algorithm one uses, there is probably no way to avoid the appearance in one form or another of a factor 2 on the unknown phase phi. This means that one must check afterwards in some way that the algorithm selected the right value; for a calibrator there should be enough flux in a single scan to do this straightaway.  
diff --git a/src/doc/txt/ngcalc_lightcurve.txt b/src/doc/txt/ngcalc_lightcurve.txt
new file mode 100644
index 0000000000000000000000000000000000000000..a9e08acfe33de90ab86cf5f1616b96082ba049f6
--- /dev/null
+++ b/src/doc/txt/ngcalc_lightcurve.txt
@@ -0,0 +1,112 @@
+I,Q,U,V,p,angle lightcurves using NEWSTAR program NGCALC
+
+
+Ger de Bruyn 15-juni-1994
+
+The program NGCALC can extract 1-dimensional (Visibility data versus
+time/HA) data from a SCN-file. These can then be processed to yield
+lightcurves of all Stokes parameters for a range of baselines.
+
+A 'typical' run would go as follows:
+
+1) exe ngcalc/ask
+
+The /ask qualifier is only required if you wish to subtract the STORED
+selfcal MDL from the selfcal'ed visibility data.
+
+Input:
+ - the name of the NGF file you wish to create
+ - select option EXTRACT
+ - specify the name of the SCN-file
+ - select the SETS
+ - select the type of information you want to process (e.g. DATA)
+ - select the polarizations (specify XYX if you wish to form all
+   Stokes parameters)
+ - select the INTERFEROMETERS (e.g. FM)
+
+This is a slow program! It takes about 20 minutes CPU (on an HP710)
+for the extraction of 12 hours of data (720 scans of 1 minute) on 40
+baselines on one frequncy channel for each of the four XX,XY,YX,YY
+correlations. This then creates 40x4 files or 'plots' as they are called in
+the program.
+
+These plots will have a six-digit number containing information on the
+baselines, polarizations and frequency channel.
+
+2) Use the option MERGE to merge different HA-sections
+
+If the 12 hour observations was cut into more than one part, each
+HA-sector will get a separate file. You can then merge these two or
+more HA-slots into one file, where the appropriate HA information is
+preserved.
+
+You can use a double-loop here. One loop might run over polarization
+and one loop over baselines; e.g. 4,...1, 69,....1 if you had
+XX,XY,YX,YY and baselines from 9A (a 0 in the fifth digit) through 0D
+(a 68 in the fifth digit)
+
+
+3) Use option CALC, SHIFT to shift the visibilities to the source you
+wish to study
+
+Use the position (l,m in arcseconds) as given in your MODEL. You may
+(have to) use a loop again.
+
+
+4) Use the option MERGE to average all baselines you wish to use
+
+After the shift operation the source should be in the phase centre. This
+means that the source signal is contained in the COS part of the visibility.
+You can check, using the plotting facilities, whether indeed the SIN signal
+is consistent with noise around zero.
+
+You may wish to loop here over the fourth, polarization, index (e.g.
+4,...1)
+
+
+5) Use the COMBINE option to form Stokes I,Q,U and V
+
+Examples: 
+Q = (#0-#1)/2, where #0 is the YY file and #1 is the XX file.
+V = -0.5*imul(#0+#1) where #0 is the XY file and #1 is the YX file
+
+
+6) If required, smooth the data using option CALC, SMOOTH
+
+
+7) You can use the PLOT option at the various stages to see whether the
+results look as 'expected'
+
+8) Use option MON to dump the interesting files in an ASCII file for
+further processing with SUPERMONGO. The mongo file will contain as its first
+column the HA.
+
+  
+
+-----------------------------------------------------------
+N.B. There are a number of things to watch out for when using NGCALC
+
+1) Files can be addressed with the full six-digit index or with a # whichever
+you find more convenient. Note, however, that when using the #'s you can
+NOT use loops. 
+
+2) There is some logic to the index numbering system but it takes a while to
+get use to it. 
+
+3) When trying to form the polarization angle 0.5*atan(U/Q) you run into 
+the problem that this angle as calculated will be within the range -45 to
++45 degrees, while of course the true polarization angle is defined 
+within boundaries -90 and +90 degrees
+
+4) Unfortunately, the delete option does not yet work. If you have made a
+new file with erroneous specifications you would ideally like to
+throw it away because you might forget that it is unusable. 
+
+5) When using the loop system all the plotfiles that will be
+tried in the looping must be present.
+
+E.g. if you have 40 FM baselines in the NGF file they are numbered 0,2,8,9,....68
+with some numbers not occurring (This number is the order in which the
+baselines exist in the SCN file). Hence, if you wish to loop over baselines
+then you could say 69,....1 but then the program will stop after it has 
+done the first baseline, because baseline ....1 does not exist.
diff --git a/src/doc/txt/obscure_bugs.txt b/src/doc/txt/obscure_bugs.txt
new file mode 100644
index 0000000000000000000000000000000000000000..fb821540ca2edceb402d15d0710bc909b43d15f9
--- /dev/null
+++ b/src/doc/txt/obscure_bugs.txt
@@ -0,0 +1,26 @@
+obscure_bugs.txt
+
+A collection of obscure Newstar bugs and their antidotes
+--------------------------------------------------------
+
+	Like any system its size, Newstar is sensitive to programming errors
+that are eaily made. Some of these may result in very obscure behaviour that
+may be difficult to diagnose. This document is meant to formalise our
+collective knowledge in this area. Anyone who solves a problem of this type is
+invited to record his experience here so others after him may benefit from it.
+
+
+Symptom: When exiting, the program emits a series of messages
+-------
+	mv: <file name> is identical to <filename>
+
+Cause: The first argument in a WNCTXT call should be a bitmask (normally F_T or
+F_TP). Omitting it or putting something else in its place may cause this type
+of behaviour.
+(JPH 940909)
+
+
+Symptom: Program crashes with IOT 6 (?)
+-------
+Cause: Division by 0 (and probably other arithmetic exceptions)
+(JPH 940909)
diff --git a/src/doc/txt/ppd_buffer.txt b/src/doc/txt/ppd_buffer.txt
new file mode 100644
index 0000000000000000000000000000000000000000..0911b64813ab5d032c5abddabed43bc105256ca7
--- /dev/null
+++ b/src/doc/txt/ppd_buffer.txt
@@ -0,0 +1,41 @@
+Aanpassen van de grootte van de ppd help-text buffer
+----------------------------------------------------
+
+(bijdrage van H.J. Vosmeijer/J.P. Hamaker, 940829)
+
+
+Als het compileren van een .pin/.psc/.pef file stuk loopt op een te kleine
+werk-buffer in sys_bldppd, moeten zowel deze buffer als een daarmee
+corresponderende buffer in de Newstar executables worden vergroot. Dit veresit
+de volgende wijzigingen in files in $n_src/dwarf, gevolgd door een gepaste
+reeks 'nsh build's
+
+
+Om de werk-buffer in cpl_2.def te vergroten moet het volgende
+gebeuren (b.v. van 5000  naar 10000 bytes):
+
+In cpl_2.def:
+  1. verander 5000 in 10000 in parameter (cpl__wrklmax = 5000)
+
+  2. verander 5000 in 10000 in parameter (cpl_wrkbuf = 421)  !&5000 !#C
+
+  3. hoog alle adressen op met 5000 (=(nieuw-oud)=(10000-5000)) voor de
+     variabelen die  NA  CPL_WRKBUF  en  VOOR  CPL__LENGTH  komen.
+     Dit zijn dus de waarden na het = teken)
+
+  4. pas CPL__LENGTH aan (=(CPL_ERRNTOT+3)/4)
+
+  5. verander 5000 in 10000 in CHARACTER*5000 CPL$WRKBUF
+
+  6. hoog alle waarden op met 5000 (=(nieuw-oud)=(10000-5000)) voor de
+     variabelen die  NA  CPL$WRKBUF  komen.
+
+In onderstaande files in genoemde regels 5000 in 10000 veranderen:
+   cplblock.for:   CHARACTER*5000  CPL$WRKBUF
+   cplread.for:    CHARACTER       KEYWORD*80, VALUE*5000
+   bpdbuild.for:   CHARACTER       VALUE*5000
+   bpdstore.for:   CHARACTER       STRING*5000, NAME*16
+   ppdhelp.fsc:    CHARACTER       WORK*5000, WORK2*80, LINE*80
+   ppdprompt.for:  CHARACTER       WORK*5000, PROGSTRM*80, KEYWORD*16
+
+
diff --git a/src/doc/txt/psc_guide.txt b/src/doc/txt/psc_guide.txt
new file mode 100644
index 0000000000000000000000000000000000000000..9d668a575afe8627f4f00a0aa5d635dc29f62484
--- /dev/null
+++ b/src/doc/txt/psc_guide.txt
@@ -0,0 +1,360 @@
+Style guide for parameter definition files
+------------------------------------------
+
+History:
+ 941110 contributed by JPH
+ 941117 Style recommendation 7.
+ 941212 Revise the latter following changes in cplvallist.for, ppdopstr.for.
+
+
+Summary
+=======
+
+	This document contains guidelines for writing .psc/.pef parameter
+definition files. A few implementation notes are added as an Appendix. The
+following subjects are addressed:
+
+	a. Definition of parameter properties
+
+	b. Definition of default values
+
+	c. Prompt formatting
+
+	d. Insertion of hypertext references
+
+
+Related documents
+=================
+
+	The reader is assumed to have some knowledge of LaTeX and the way it is
+used for Newstar documentation. The latter is described in the Newstar document
+"Guide for writing and maintaining Newstar documents".
+
+
+Definition of parameter properties
+==================================
+
+	A large number of properties can be defined for each parameter. I
+discuss only a few.
+
+	- ATTRIBUTES=<attr>[,<attr>]...
+
+	  . LOOP: WNDPAR returns the special status DWC_ENDOFLOOP when no more
+parameter values are available. The calling program may detect this status as a
+signal for some special action. When LOOP is not specified, the value(s)
+specified is/are simply re-used.
+
+	  . NULL_VALUES: It is allowed to enter 0 values, either by default or
+by the user. A null value is represented by an empty string: "". For a null
+reply, WNDPAR returns <number of values>=0.
+
+	  . WILD_CARDS: A wildcard, *, is allowed as default or reply. For a
+wildcard, WNDPAR returns <number of values>=-1.
+
+In a proper implementation, the latter two attributes should be defined only
+where appropriate. In Newstar, they are declared almost everywhere and
+consequently programs must make special checks in many places for illegitimate
+null and wildcard values.
+
+	This situation is clearly unsatisfactory, but systematic rectification
+is not worth the effort and risk of mistakes. Some efforts in this direction
+have been made but are being discontinued.
+
+
+Definition of parameter defaults
+================================
+
+	Defaults in a prompt can be defined in a number of ways. The DWARF
+design postulated that the interface presented to the user should be defined as
+much as possible in the .psc file; the
+
+	- DEFAULTS=<values>
+
+clause in a keyword description serves this purpose. As an alternative, dynamic
+defaulting can be used.
+
+	Newstar largely ignores this philosophy, by defining most defaults
+through the dynamic mechanism, even when the value is a constant. In some cases
+both .psc and dynamic defaults are provided, - in which case the latter will
+take precedence.
+
+	This situation is clearly unsatisfactory, but systematic rectification
+is not worth the effort and risk of mistakes. Some efforts in this direction
+have been made but are being discontinued.
+
+
+Prompt and options string formatting
+====================================
+
+	A Newstar prompt is composed of
+
+		<keyword> -
+		<prompt text>
+		(<options list>)
+		=<default>:
+
+The complete prompt is concatenated from these components and then formatted
+into one or more lines on the terminal.
+
+	As of november 1994, the formatting routine has been modified to allow
+the programmer more control over the form in which the prompt is displayed,
+through the use of some special punctuation:
+
+	- The prompt string may be terminated in a '|' to put the options
+string on a new line.
+
+	- The options string may contain the characters ' ,;|/[]' to format it:
+
+	  . The '|' can be used to split the string over multiple lines; when
+appended at the and of the list, it signals that the <default> must be put on a
+new line of its own.
+
+	  . ';' and ' ' can be used to group options in functionally related
+subsets;
+
+	  . '/' can be used to group options that are alternatives, e.g.
+BAND/NOBAND.
+
+	  . '[]' can be used to indicate options that one would only use in
+exceptional situations;
+
+	  . '(:)' can be used to insert comments (this may not work, it has not
+been tested).
+
+
+Long and short lines
+--------------------
+
+	Within Newstar a need exists for text files to be formatted as one line
+per full paragraph in some application, and in other uses for the same files to
+be formatted in lines that fit a terminal screen. The conversions can be made
+automatically, provided a few guidelines are heeded: See item 7 of the Style
+Recommendations below.
+
+
+Style recommendations
+---------------------
+
+	1. The '|' character will signal a line break and therefore cannot be
+used otherwise (e.g. as an 'OR' symbol).
+
+	2. If the prompt, options, and default strings combined leave enough
+room for a reply on the same line, donot insert any newlines.
+
+	3. If the options string must be divided over more than one line, then
+put the entire options string on lines of its own (i.e. terminate both the
+prompt and options strings in a '|');
+
+	4. Use blanks and semicolons to visually group the options, and use the
+same grouping in the help text. Insert newlines only between groups, and put a
+semicolon before such a newline.
+
+	5. Remember that the options string will be shown enclosed in
+parentheses. Therefore donot terminate it in a semicolon. (If it ends in a '|',
+that character will be shifted behind the closing parenthesis.)
+
+	6. Format the OPTION string in the way you want it to appear in the
+prompt, remembering that the prompting routine will indent each new line by 4
+blanks: (So donot insert additional blanks in your .psc file!)
+
+	OPTIONS=-
+QUIT; COPY,CCOPY,LINE; ZERO,MANUAL,INIT,RENORM;| -
+EXT,REF, IREF,FAR, IFR,MIFR, SHIFT,CLK; DX,DY,DZ, POLE,FREQ
+
+	7. Make sure the product of the number of options and the LENGTH for
+character parameters is less than 512. (All options are extended by CPL_VALLIST
+to LENGTH characters and concatenated in a local buffer defined by
+PPD_OPSTR_PUT.)
+
+	8. Newstar's automatic line-formatting mechanism may concatenate
+consecutive short lines into a longer one. It does, however, avoid improper
+joining of lines by assuming that the following input line types either start a
+new output line or terminate the current output line or both:
+
+	- a line starting in whitespace, '-' or a '!' comment character: new
+	  output line;
+
+	- a blank line or a line consisting of a '.' only: copy literally;
+
+	- a line containing an in-line comment or a double quote: terminate
+	  output line.
+
+Similarly, a line ending in a hyphen (the DWARF 'to be continued' mark)
+terminates the current output.
+
+
+
+TaTeX/Hypertext conversion of the Help texts
+============================================
+
+	The command 'ndoc Key' translates the files
+
+		<xxx>.psc resp. <xxx>.pef
+
+into LaTeX files
+
+		$n_doc/intfc/<xxx>_private_intfc.tef
+	  resp. $n_doc/intfc/<xxx>_public_intfc.tef
+
+It subsequently calls ndoc Cook to process a corresponding .tex file to produce
+the hypertext document.
+
+	(NOTE: This is a change w.r.t. the previous situation, in which only
+the hypertext translation was available, consisting of one separate small .html
+file per keyword. The logistics for the _intfc.tex/tef files is now entirely
+identical to that for the other .tex documents, which is advantageous in many
+ways.)
+
+
+Cross references
+----------------
+
+	To fully exploit the symmetry between LaTeX sources and the .tef files
+provision is made for cross-references in the latter. These take the form of
+LaTeX \textref commands on comment lines in the .psc/.pef file, e.g.
+
+	! {\em see also the}\textref{DWARF}{<file name>} interface description}
+
+Conversely, references to Help texts can be made both from other Help texts and
+LaTeX documents. For this purpose, ndoc Key generates a label for each help
+text:
+
+	keyword <XXX>_<YYY>_<ZZZ> --> label .<xxx>.<yyy>.<zzz>
+
+
+Appendix: Prompt formatting
+===========================
+
+	The DWARF susbsytem of NEWSTAR is responsible for displaying prompt
+information on the terminal and checking the user's reply. As inherited, the
+formatting of the prompts was very clumsy, making them difficult to read,
+particularly in those frequent cases where a large number of options must be
+chosen from.
+
+	It has proved possible by some very simple changes to give the maker of
+the .psc file, - that defines the prompt and options strings -, a great deal of
+control over the way a prompt is formatted. This is made possible by the fact
+that
+
+	a. Prompt and options strings are copied litterally from the .psc file
+to the binary .ppd file that an executable program reads.
+
+	b. Parsing of the options string relies on a string parameter that
+defines which characters delimit inidividual options in the options string. By
+extending the former string we may allow other characters than ',' to be used
+as delimiters.
+
+	c. The prompt is composed by essentially a simple concatenation of the
+prompt, options and default strings and then breaking it into lines for output
+on the terminal. It is easy to change the line-breaking algorithm to break
+lines at a predefined delimiter character; the vertical bar '|' was chosen for
+this purpose.
+
+	It has later been found that there are other DWARF routines that assume
+that a comma is the only delimiter, such as CPL_VALLIST. These seem to work
+correctly, provided only that the parameter's LENGTH is defined large enough
+(cf. Style recommendation number 7 above.). This can be safely done since this
+attribute is only used to allocate buffer space.
+
+
+Implementation in the prompt and reply paths
+--------------------------------------------
+
+	A schematic of the prompt and reply paths is shown in the following
+diagram:
+
+|GP_INP
+|  calls GP_INP_GET
+|
+|       GP_INP_GET
+|       | calls PPD_PROMPT
+|       |
+|       |       PPD_PROMPT
+|       |         calls PPD_PRSTR_GET to get <prompt string>
+|       |         calls PPD_OPSTR_GET to get <options string>
+|       |         returns with
+|       | PROMPT = <prompt string> (<options string> )'
+|       | appends '=<default string>' to PROMPT
+|       | calls DWC_INPUT with PROMPT
+|       |
+|       |       |DWC_INPUT
+|       |       | calls GEN_INPUT
+|       |       |
+|       |       |       |GEN_INPUT
+|       |       |       | formats prompt and outputs line by line
+									prompt
+******************************************************************************
+									reply
+
+									prompt
+******************************************************************************
+									reply
+|       |       |       | reads answer
+|       |       |       | detects DWC_EOFCTRLZ
+|       |       |       | returns
+|       |       |
+|       |       | returns
+|       |
+|       |  does some checks on ANSWER
+|       |  reprompts for some errors
+|
+| calls GP_INP_PARSE
+| ...
+| calls GP_INP_DECODE
+|
+|       GP_INP_DECODE
+|       | calls PV_BLK_DECODE
+|       | calls PPD_CHECK
+|       |
+|       |       PPD_CDHECK
+|       |       | if options defined:
+|       |       |   calls PPD_OPSTR_MATCH
+|       |       |
+|       |       |       PPD_OPSTR_MATCH
+|       |       |       | calls STR_MATCH_L
+|       |       |       |
+|       |       |       |       STR_MATCH_L
+|       |       |       |       |  returns <match number>
+|       |       |       |
+|       |       |       | loop <match number> times
+|       |       |       |   calls STR_SKIP_U (DELIM=',;|[]',...)
+|       |       |       |
+|       |       |       |       STR_SKIP_U
+|       |       |       |       |       skips up to character in argt DELIM
+|       |       |       |
+|       |       |       | end loop
+|       |       |       | calls STR_SKIP_W
+|       |       |       |
+|       |       |       |       STR_SKIP_W
+|       |       |       |       |       skips whitespace
+|       |       |       |
+|       |       |       | calls STR_COPY_U (DELIM='.;|[]',...)
+|       |       |       |
+|       |       |       |       STR_COPY_U
+|       |       |       |       |       copies up to character in argt DELIM
+|       |       |       |
+|       |       |       |returns full OPTION
+|       |       |
+|       |       |end if
+|       |       |...
+|       |
+|       |...
+| |...
+
+
+	In the prompt path GP_INP_GET and PPD_PROMPT concatenate the keyword,
+prompt, options and default strings in string PROMPT. These strings are taken
+litterally from the .PPD file or WNDPOH without any processing except for the
+insertion of a few punctuation marks to delineate the four components. All
+punctuation marks in the strings are preserved.
+
+	GEN_INPUT formats PROMPT into lines for the terminal. It interprets one
+or more vertical bars '|' as a newline and does not autonomously generate any
+additional newlines. Any lines after the first are indented by 4 spaces; apart
+from this, the formatting is entirely controlled by the bar characters in the
+strings as defined in the .psc file. No checks are made on the lengths of the
+lines being output.
+
+	The reply path uses the options string to check the reply and must
+therefore recognise all punctuation characters. This is realised extremely
+simply by including them in the DELIM argument so STR_SKIP_U and STR_COPY_U
diff --git a/src/doc/txt/psctest.txt b/src/doc/txt/psctest.txt
new file mode 100644
index 0000000000000000000000000000000000000000..3f5ad6b78d3f9c12bbc1a7c587ef3d6ecad921f6
--- /dev/null
+++ b/src/doc/txt/psctest.txt
@@ -0,0 +1,82 @@
+
+
+psctest.csh
+===========
+
+	Options to:
+
+	- Create a .pst file by running program under manual control.
+
+	- Create reference numbers on the parameter lines.
+
+	- Run program under control of a .pst file:
+	  = Including backtrack paths
+	  = Including on-line help requests at first appearance of each
+	    parameter.
+	  = Using only a certain range of parameter lines
+	  = In /ASK mode including hidden parameters
+
+
+
+.pst file
+=========
+
+	Consists of:
+
+	- Preamble: a csh script, ending in the line 'exit'. This script is
+executed by psctest.csh to set up initial conditions (i.e. verify accessibility
+of input files, remove left-over output files etc.).
+
+	- Parameter input: Lines of the form
+
+		<blanks>[*]<blanks><KEYWORD> = <value> ! <number>
+
+The lines are indented corresponding to the 'level' of the parameter in its
+local context. The asterix is positioned at the level of a preceding parameter
+that is the target for a backtrack request.
+
+	- Comment lines starting in a '!'.
+
+
+	The simplest way to generate an initial .pst file is through
+
+		psctest -m <program>
+
+The file may then be manually edited to e.g.
+
+	- insert the initialising script;
+
+	- remove spurious parts (e.g. backtracks accidentally made in the manual
+	   run);
+
+	- change improper backtrack targets to what they should be (Of course,
+	   corresponding changes must be made in the program code!).
+
+After a change in the parameter lines, they may be renumbered through
+
+		psctest -n.
+
+
+Special cases
+=============
+
+Unconditional backtracking
+--------------------------
+
+	To be realised by listing the parameters through which the backtrack is
+made with '#' input, at the proper indentation (i.e. indents for a backtrack
+chain decrease downward). Do not include '*' backtrack marks!
+
+
+Repetition loop
+---------------
+
+	Occurs e.g. in NSCAN LOAD, NMAP MAKE. Append indices in [] to the
+parameter name to show the cycle number. Continue increasing indentation
+throughout the loop.
+
+
+Hidden parameters
+-----------------
+
+	To be indented at the same level as the subsequent visible parameter.
diff --git a/src/doc/txt/qube.txt b/src/doc/txt/qube.txt
new file mode 100644
index 0000000000000000000000000000000000000000..e6a427d215fc65e17dc4fbc9c28d5cde7e878d25
--- /dev/null
+++ b/src/doc/txt/qube.txt
@@ -0,0 +1,226 @@
+QUBES: Software to make SCN-file UV-data available in various sort orders
+-------------------------------------------------------------------------
+History:
+	Contributed by WNB, 940810
+	WNB 940812: add interferometer errors
+
+
+Summary (JPH 940810)
+
+	This note documents software created by WNB during his 1994 visit at NFRA as infrastructure for the program NFILTER.)
+
+
+1. Introduction
+
+To be able to read a one-directional data vector from the Scan data in
+any of the possible coordinate direction, a number of NSCQ.. routines
+are available, replacing in essence NSCSCR and NMOMU4 and their
+initialisers.
+The possible directions are: frequency(f), ha(t), interferometer(i). No
+possibilty to go in the direction of Mosaic fields has been built in,
+mainly because different mosaic fields have no identical ha's: the
+4-dimensional structure (mosaic,f,t,i) is not a regular hypercube.
+The structure chosen assumes that the dataset to be considered
+consists of a series of 3-d cubes (f,t,i) at different mosaic points.
+In principle extension to a series of (mosaic,f,i) cubes at different
+ha's would be feasable.
+A field in the above is a set of observations at the same position on
+the sky, with identical (number of) frequencies, interferometers and
+hour angles. Note: the actual check on the number of hour angles is
+not extensive, to limit the sorting problems, but with actual WSRT
+observations this should not be a problem.
+An example of the actual use is given in NFIUVL.for, which at the
+moment is a simple test program, not an actual UVLIN.
+
+2. Routines
+
+To write a program using the NSCQ routines, the basic structure of the
+program is identical to programs using NSCSCR, i.e. scans in the
+i-direction. The user parameters used by the NSCQ routines are the
+same: Node, Sets and, possibly, Loops. Other selection parameters can
+be used in the same way as in other programs, and model data has to be
+initialised in the same way as well (i.e. NMODAX, NMOMUI and NMOMSC/L
+have to be used before the actual data loops can start).
+
+
+To set the field a (short) description of the standard program
+structure as it is now (*=optional):
+
+while WNDXLN			do all specified loops(*)
+  NMOMSL			calculate scan model(*)
+  while NSCSTL			do all sectors
+    NSCSIF			get interferometer table(*)
+    NSCMBL			get baseline table(*)
+    NCARRT			get redundant baseline(*)
+    NMORDH			get model parameters(*)
+    NMOMST			calculate some model parameters(*)
+    for i=ha-range		go through (selected) ha scans
+      NSCSCR			get corrected scan data
+      NMOMUV			calculate UV coordinates for scan (*)
+      NMOMU4			calculate model for scan(*)
+      action			including e.g. NSCSWI
+    end
+  end
+end
+
+The structure to go through data in different order is comparable:
+
+while WNDXLN			do all specified loops(*)
+  NMOMSL			calculate scan model(*)
+  NSCQOP			prepare SETs for reading
+  while NSCQFN			get next field in 4-d structure (and 
+					coordinate tables) and select
+					coordinate order
+    NSCMBL			get baseline table(*)
+    NCARRT			get redundant baselines (*)
+    
+    for i=first selected coordinate
+      for j=second selected coordinate
+        NSCQSR			read selected (pseudo-)scan along 3rd coord
+        				and model, if selected in QFN
+        action			including e.g. NSCQWA/M
+      end
+    end
+  end
+  NSCQCL			close Qube control area
+end
+
+routines to calculate e.g. UV-coordinates etc for the pseudo scans are
+easily added if necessary. 
+
+
+3. Description interface
+
+
+- NSCQOP_L(	QUA_J:O,			Qube control area ptr
+		FCA_J:I,		 	(Scan) file control area
+		SETS_J(0:SOF__N-1,0:*):I,	SETs selected by user
+		LPOFF_J(0:SOF__N-1)		Current Loop offsets
+		INFO_J(QINFO__L:QINFO__H):O	Info about 4-d qube
+	)
+
+QOP analyses the SETs (using also the loop info (LPOFF) and Scan file
+(FCA), and makes a sorted list of all Sector pointers. It also
+reserves buffers for later use.
+The QUA is a pointer to the control area to be used in all subsequent
+Q calls. 
+The INFO array returns the following information (parameters in
+CBITS_DEF):
+	INFO(QINFO_FLD)		number of different fields
+	INFO(QINFO_F)		max. number of frequencies found in all fields
+	INFO(QINFO_T)		max. # ha
+	INFO(QINFO_I)		max. # ifrs
+
+Note: the system works fastest if field selection is done by the Loop
+structure.
+
+
+- NSCQCL_L(	QUA_J:IO,			Qube control area ptr
+		FCA_J:I,			Scan file control area
+		SETS_J(0:SOF__N-1,0:*):I	SETs selected by user
+	)
+
+QCL frees all the buffers and temporary files used
+
+
+- NSCQFN_L(	QUA_J:I,			Qube control area ptr
+		FCA_J:I,			Scan file control area
+		ORDER_J:I,			Order of data reading
+		STH_B(0:STH__L-1):O,		A Sector header
+		INFO_J(QINFO__L:QINFO__H):O,	Info about 4-d qube
+		PINFO_J(QINFO__L:QINFO__H):O	Pointer to Info about 4-d qube
+	)
+
+QFN selects the next field for processing (or is .false. if no more).
+It uses the QUA and FCA, and the ORDER specified. The ORDER can be:
+		QUB_FTI [+QUB_M] [+QUB_OUT]
+		    TFI
+		    TIF
+		    ITF
+		    FIT
+		    IFT
+The ..I uses no sorting file, the I.. may use a large sorting file.
+The coding is: I=interferometer, F=frequency, T=ha. The last code
+specifies the direction of the 'scan' produced (i.e. FTI is the
+'normal' order, TIF produces a scan along the frequency axis); the 1st
+code specifies the highest loop direction the user wants to use. Note:
+you can loop in a different order than specified, but this will be
+rather inefficient in general.
+The _M modifier (e.g. QUB_TIF+QUB_M) will in addition to the data also
+generate the model data in the same 'scan' direction.
+The _OUT modifier will prepare and enable the writing of
+interferometer errors.
+
+The STH returned is one of the STHs of the field. I.e., the
+coordinates, number of interferometers etc will be correct, but time,
+frequency, ha and data depended on these will be random. It can,
+however, be used in routines like NSCMBL.
+
+The INFO returned is identical to that for QOP, but now the actual
+field number(1..), and axis lengths for this field are returned.
+
+The PINFO (at QINFO_T, QINFO_I, QINFO_F) returns pointers to tables
+with the actual coordinates along the axes. These values can be
+addressed as:
+	A_I(PINFO(QINFO_I)+n_i)		interferometer codes
+	A_E(PINFO(QINFO_T)+n_t)		ha values
+	A_D(PINFO(QINFO_F)+n_f)		frequencies
+with n=0,INFO(QINFO_x)-1
+
+
+- NSCQFR_L(	QUA_J:I,			Qube control area ptr
+		FCA_J:I				Scan file control area
+	)
+
+QFR resets the field search to the start of the field list
+
+
+- NSCQSR_L(	QUA_J:I,			Qube control area ptr
+		FCA_J:I,			Scan file area
+		AX1_J:I,			1st axis to read
+		AX2_J:I,			2nd axis to read
+		CAP_J:I,			apply bits
+		CDAP_J:I,			de-apply bits
+		PWGT_J:O,			pointer to scan weights
+		PDAT_J:O,			pointer to scan data
+		PMOD_J:O,			pointer to scan model
+		POUT_J:O,			pointer to area to put
+						ifr errors
+	)
+
+QSR reads a (pseudo-)scan along the 3rd axis selected in QFN at the
+position specified by AX1 and AX2 (axis types determined in QFN). I.e.
+with QUB_TIF and AX1,AX2=300,2 a frequency scan will be produced for
+the second interferometer in the interferometer table at the 300th ha
+point (values for the axes can be 0..INFO(corresponding)-1).
+
+The data is returned by a pointer to an array. These arrays have
+dimensions (0:3,0:length scan-1). Note: the index order is different
+from that returned by NSCSCR and NMOCIX, for obvious reasons.
+If n_p is the polarisation (0..3) wanted and n_d the data point
+(0..INFO()-1),the data can be accessed by:
+	A_E(PWGT+4*n_d+n_p)
+	A_X(PDAT+4*n_d+n_p)
+	A_X(PMOD+4*n_d+n_p)
+Interferometer error data (if QUB_OUT included in QFN) can be put into
+the array pointed to by POUT, and accessed by:
+	A_X(POUT+4*n_d+n_p)
+
+Note: the PMOD has only a valid value if QUB_M was used in QFN
+Note: the model data are already converted to XYX format
+
+
+- NSCQWA_L(	QUA_J:I,			Qube control area ptr
+  NSCQWM_L	FCA_J:I,			Scan file area
+		AX1_J:I,			1st axis to write
+		AX2_J:I,			2nd axis to write
+		CAP_J:I,			apply bits
+		CDAP_J:I			de-apply bits
+	)
+
+QWA will write the additive interferometer errors set (in pseudo-scan
+order in the array POUT obtained from QSR) to the scan data file.
+QWM the multiplicative interferometer errors.
+
+
+wnb/940812
diff --git a/src/doc/txt/remote_tape.txt b/src/doc/txt/remote_tape.txt
new file mode 100644
index 0000000000000000000000000000000000000000..616c9b5763117c9a19bbafd2d45a2b4dfd1a867b
--- /dev/null
+++ b/src/doc/txt/remote_tape.txt
@@ -0,0 +1,66 @@
+
+Transparent reading of the Optical Disks with Newstar
+-----------------------------------------------------
+
+It is now possible to access the optical disk units that are 
+connected to the VAX while working on a Unix machine.
+
+In Dwingeloo, the following tape-devices have been defined:
+
+   MAG4   //rzmvx4.nfra.nl:1100/RZMVX4$MUA0  
+   MAG5   //rzmvx4.nfra.nl:1101/RZMVX4$MUA1
+
+These devives allow you to read data from the units MUA0 and MUA1
+as if they were connected to your Unix machine.
+
+If you work on e.g. rzmws10 and you want to get data from MUA0,
+just run NSCAN and specify unit 4. 
+
+
+Note 1: Implementation
+ 
+   Transparent reading is implemented by a server on the VAX and
+   an extension of the tape-handling routines in Newstar.
+   The server on the VAX is USER5:[DEVOSCM.RMTD]RMTD.EXE
+   The server has to be started on two ports, this can be done
+   by including in the system-startup:
+
+      @user5:[devoscm.rmtd]rmtd_start.com  
+  
+   which will submit two jobs on RZMVX4_BATCH.
+
+   The names of the remote units have been defined in the startup file
+       $n_src/sys/newstar_nfra.csh
+
+   The routines changed for the implementation are $n_src/wng/wnftrw.cun 
+   and $n_src/wng/wnf???_x.cun. The code for the client side of the 
+   network is in wnftrw.cun. The changes in the other files are: (1) all
+   calls to open, close, read and write now go through a routine in 
+   wnftrw.cun and (2) all calls to routines wnftrw pass the MCA (not FCA)
+
+Note 2: Suggested testing
+
+   To test the reliability of the transparent tape-reading I suggest
+   the following. During the next week, all files read from Optical Disk
+   by the Reduction Group are read two times and then compared
+
+      1e. Unix: NSCAN LOAD UNIT=4 or 5 
+
+      2e. VAX:  NSCAN LOAD UNIT=4 or 5
+          Unix: ftp SCN-file
+                NSCAN CVX
+
+      3e. Unix: ~devoscm/tst.csh File1.SCN File2.SCN
+  
+   If the files have been loaded identically, no differences should appear.
+   The tst.csh procedure ignores differences of 1 unit in the data, since 
+   they can be produced by rounding errors during the time-averaging.
+
+   Any differences should be reported to Marco de Vos.
+
+   After testing some 10 SCN files, we are sure that no systematic errors 
+   take place. The remaining test is on reliability of the connection over
+   a longer period. This can be tested by using only the Unix version of 
+   Newstar to read data from the archive. After a month, we will have a 
+   good impression of the reliability. 
+
diff --git a/src/doc/txt/spefu_type_categ.txt b/src/doc/txt/spefu_type_categ.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6c32b3447afb2353a2a4b13530a14f0863b1a434
--- /dev/null
+++ b/src/doc/txt/spefu_type_categ.txt
@@ -0,0 +1,65 @@
+List of codes in the OHW-fields SPEFU, TYPE, CATEG
+--------------------------------------------------
+	(original Dutch source unknown,
+	 translated litterally into English by JPH, 940621)
+
+History: 
+	JPH 940914      Format corrections
+
+
+	The OH (Observation Header) of an observation file on a WSRT tape is
+copied literally into a OHW block asspociated with one or more Sectors in a
+.SCN file. It contains several fields describing the natiure of the
+observation. The meaning of the ASCII that may occur in these fields is
+tabulated below.
+
+ SPEFU=   Meaning
+ ------   -------
+  PT     Pointing observation
+  HO     Holog observation
+  OF     Offset observation
+  VL     VLBI observation
+  MO     Mosaiking observation
+  PD     Pulsar observation (DCB)
+  DF     Delay offset observation (DCB)
+  LO     LO sweep observation
+  FS     FS frequency switching observation
+  SD     Switched dipole observation
+  NO     No special observation
+
+
+
+
+ TYPE
+ 1st char Meaning               2nd char Meaning
+ -------- -------               -------- -------
+ C       Other                  A        Supplememt to N,M,P or F
+ F       Frequency switch.      B        Baseline  (for C)
+ M       Mosaicking             C        Gain/phase (for C)
+ N       Norm. astr.            D        Dipole switch (for C)
+ P       Pulsar                 E        Extinction  (for C)
+ V       VLBI                   F        Phase only (for C)
+				G        Gain only (for C)
+				H        Holog (for C)
+				L        LO-delay (for C)
+				M        Monitoring (for N)
+				N        New (for N,M,P of F)
+				O        Redo (for N,M,P of F)
+				P        Parallax (for N of C)
+				Q        Offset (for C)
+				R        Pointing (for C)
+				S        System temp. (for C)
+				T        General Test (for C)
+				U        Universal (for C)
+				V        Videoband   (for C)
+				W        Delay (for C)
+
+
+
+ CATEG=         Meaning
+ ------         -------
+  I             Instrumental, including all calibrations
+  N             Astronomy: Nearby galaxies
+  S             Astronomy: Solar System
+  G             Astronomy: Galactic Object
+  E             Galactic astronomy not covered by N
diff --git a/src/doc/txt/wndpoh.txt b/src/doc/txt/wndpoh.txt
new file mode 100644
index 0000000000000000000000000000000000000000..86995310d08edde2b6d58312f30e6e85dbd36add
--- /dev/null
+++ b/src/doc/txt/wndpoh.txt
@@ -0,0 +1,173 @@
+Dynamic tailoring of the Newstar program-parameter interface
+------------------------------------------------------------
+
+Contributed by Johan Hamaker, 940916
+
+
+Statement of the problem
+========================
+
+	The DWARF parameter interface and the way it is harnessed in the
+Newstar programs is plagued by several problems that confuse the user:
+
+	- many keywords are used in multiple places serving multiple, often
+quite different, functions ("keyword overloading");
+
+	- since DWARF allows only static definitions of keyword prompt, options
+and help text, the information provided to the user in a prompt is either too
+generic (in order to cover all functions for which the keyword is used) or
+confusing (when a keyword is re-used in a context that differs from the one it
+was designed for);
+
+	- the logic underlying the order in which prompts are presented is in
+many places different from a user's natural expectations.
+
+	Following the DWARF design philosophy a proper solution would be to
+split overloaded keywords into multiple ones; in addition the order of the
+prompts could be made more natural to the uninitiated user. Both of these
+options are unacceptable because of their pervasive impact on existing batch
+procedures.
+
+	In trying out various ways to patch the situation I noticed that the
+only information that a user can hardly avoid noticing is that provided in the
+prompts (and in the help texts if he consults these). Everything else is very
+easily overlooked.
+
+	The problem, then, is to provide prompts, options and help texts
+specific to each of the quite different contexts in which a keyword may be
+used, without resorting to changing the keywords themselves. In other words, we
+want a method enabling programs to set these prompt components dynamically. As
+a practical matter, the method should have a minimal impact on the existing
+programs.
+
+
+The new subroutine WNDPOH
+=========================
+
+	A new routine WNDPOH has been created that accepts dynamic Prompt,
+Options and Help strings. These will be used in the subsequent parameter prompt
+(directly through WNDPAR or indirectly through WNDNOD, NSCHAS etc.). The prompt
+and options strings replace those in the .ppd file; the help text may either be
+inserted in front of the .pps text or replace it.  Thus, the call sequence is
+simply
+
+		CALL WNDPOH (<prompt>, <options>, <help>)
+		CALL WNDPAR (...
+
+or
+
+		CALL WNDPOH (<prompt>, <options>, <help>)
+		CALL NSCHAS (...
+
+etc.
+There is no need to clear the strings later, this is done automatically once an
+answer from the user has been accepted.
+
+
+Details on the call arguments
+-----------------------------
+
+	The help text may contain newline directives in the WNCTXT format: !/.
+It is recommended to format help text in lines that will fit in single
+80-character Fortran lines and extend the quoted string over as many
+continuation lines as are necessary, e.g.
+
+	    CALL WNDPOH(
+	1'Target node to which to write corrections',' ',
+	3'SET COPY copies the average telescope corrections from 1 complete!/
+	3input sector to selected parts of any number of output sectors.')
+
+A help text ending in a line '#-' signals that the text OVERRIDES the .ppd help
+text rather than being prepended to it (so the .ppd text will not be shown).
+
+	The <prompt> and <options> strings are limited to 128 characters, the
+<help> text to 512 (or a few less). Blank arguments to WNDPOH are ignored, i.e.
+they leave the corresponding dynamic text unaltered.
+
+
+Where to program dynamic prompting
+----------------------------------
+
+	The following is a list (possibly still incomplete) of keywords and
+subroutine calls that may need dynamic prompting. A complete example of how I
+envisage the use of WNDPOH is in ncadat.for.
+
+	all <xxx>_NODE keywords (WNDNOD)
+
+	all <xxx>_SETS keywords (WNDST<x>)
+
+	all <xxx>_LOOPS keywords (WNDXLP) in those cases where the loop controls
+	  more than one ,xxx>_SETS stream
+
+	SELECT_XYX (NSCPL<x>) when used to select telescope rather than
+	  interferometer polarisations. In this case the dynamic options are
+	  'X,Y,XY', and the subsequent NSCPLS call must read
+		CALL NSCPLS(XY_P,<pol.mask>)
+	  where XY_P is defined in CBITS_DEF
+
+	SELECT_IFRS (NSCIF<x>), SELECT_TELS (NSCTL<x>) in those cases where it
+	  is not obvious to which stream (input or output) the selection
+	  pertains.
+
+
+Limitations
+===========
+
+	1. The dynamic information is not included in the hypertext display for
+the keyword, because the hypertext source file is a static derivate of the .psc
+or .pef file. For this reason the dynamic information is always shown on the
+terminal for all forms of on-line help requests.
+
+	2. As stated before, the method can not change the order in which
+prompts appear.
+
+	3. Since the dynamic texts are provided by the program, they are not
+available to dwspecify. I consider this a minor disadvantage since dwspecify is
+a primitive program in other ways as well. For interactively setting up
+parameter values dwexe/norun is a much better alternative that does have access
+to the dynamic texts.
+
+
+
+APPENDIX: Implementation
+========================
+
+	WNDPAR through GET_PARM calls on routines PPD_PRSTR_GET, PPD_OPSTR_GET
+and PPD_HSTR_GET to fetch the prompt, options and help strings from the .ppd
+file. To allow a program to modify e.g. the prompt dynamically, a new entry
+point PPD_PRSTR_LSET was created. It takes a prompt string as argument and
+stores it in an internal buffer. When PPD_PRSTR_GET is called later, it checks
+this buffer and if it finds anything there, uses it instead of the .ppd prompt.
+The same method is used to allow dynamic options and help texts; a dynamic help
+text may either override the static text or be inserted in front of it. A
+terminating line '#-' is inter[reted as an 'override' flag.
+
+	For the programmer's convenience, a single routine is available to set
+dynamic information pertaining to the subsequent direct or indirect (through
+another routine such as WNDSTA) WNDPAR call.
+
+	The dynamic information will be used in the prompt and any automatic
+repeat of it; it will then automatically be cleared.
+
+
+Automatic clearing
+==================
+
+	Subroutines like WNDNOD, WNDSTA, NSCIFS are called in various contexts,
+so the use of WNDPOH with them is desirable. Internally, these routines call
+WNDPAR and may do so repeatedly in case of an incorrect reply. For this reason
+WNDPAR can not automatically clear the dynamic strings.
+
+	The solution is for the calling subroutines to set an 'inhibit
+clearing' flag. WNDPAR will only clear the dynamic strings if this flag is
+clear. Any routine that sets the flag is responsible for clearing both the falg
+and the strings, through a call to WNDPOHC.
+
+	The flag must be accessible to several routines and must therefore
+reside in a COMMON block. At present the location A_J(0) defined by WNG_DEF is
+used because it was available. This solution is sound except that it is
+invisible outside the routines that use the flag; an unexpected conflict could
+arise later when someone decides that he may use this location for another
+purpose.
+
+
diff --git a/src/doc/txt/wntinc.txt b/src/doc/txt/wntinc.txt
new file mode 100644
index 0000000000000000000000000000000000000000..296f4526bdb649db5f0684978d28aa9fea1dff19
--- /dev/null
+++ b/src/doc/txt/wntinc.txt
@@ -0,0 +1,473 @@
+wntinc.txt      draft-5 930902/WNB
+
+
+The Newstar table compiler WNTINC
+---------------------------------
+
+
+
+1. Introduction
+
+WNTINC is a replacement for WNTAB. The major changes are based on
+comments/remarks made by JPH and MdV, and on deficiencies found by myself.
+It has been rewritten to make it more modular and to get rid of any
+non-described numerical codes.
+Main features:
+- calculation on local variables
+- multiple structure definitions
+- structure definitions inside DEFINE
+- structures in data statements
+- implicit array lengths
+- implicit string lengths
+- alignment possibilities
+- map/union options (not implemented in this version yet)
+- deletion of some unused options
+- complete C coverage
+- continuation lines
+
+An example of the use can be found in wnt.dsc
+
+
+2. Input structure
+
+The input file to WNTINC is a NAME.dsc file. The parameter to WNTINC is
+NAME, possibly modified by a directory indication. Whatever the case of
+NAME, it will be assumed to reference a lc NAME.dsc.
+All input lines will be converted to UC, unless enclosed in "". The output
+names will all be UC for Fortran and Unix parameters; lc for Unix variable
+names.
+Blanks in the following indicate 'white space' (i.e. in general spaces
+and/or tabs)
+
+NAME.dsc will consist of a number of lines. Each line consists of a (possibly
+empty) command part, followed by an optional comment part which should be
+preceded with an !. A line can be continued by having the last non-blank
+character in the command part to be a '\'.
+An empty line will be considered to be a comment line; a comment not
+starting at the beginning of the line will be considered to be a
+continuation of the previous line (whether '\' present or not. (This
+is to distinguish comments that should precede fields from comments that
+should follow fields)).
+
+Each command can be:
+- empty (i.e. comment line only)
+	can occur everywhere
+- the first non-blank character a '%': commands that steer the behaviour
+  of the compiling process
+	can occur everywhere
+- the first non-blank character a '.': commands that steer the data
+  interpretation process
+	can occur only in 'data-blocks'; except .DEFINE: can occur only
+	once outside a data-block; .STRUCTURE (.BEGIN) that can occur
+	inside and outside data-blocks and which define the start of
+	data-blocks; .PARAMETER that can occur everywhere
+- data command (starts always with a '-' (dummy name)) or alphabetic character
+
+
+3. Output files
+
+WNTINC produces the following output files (NAME is the input file name
+name, or set by the %NAME) (all filenames in lc):
+
+a. If .STRUCTURE type data blocks present:
+
+- NAME_o.def    Fortran include file containing parameters and/or comments
+		and/or 'structure-type' definitions
+- NAME_o.inc    C include file containing parameters and/or comments and/or
+		structure definitions
+- NAME_t.def    Fortran include file containing information for translating
+		data structures from one representation to another (using
+		WNTT* routines)
+- NAME_t.inc    C include file
+- NAME_e.def    Fortran include file containing information for formatted
+		printout and/or input of data structures
+- NAME_e.inc    C include file
+
+b. If a .DEFINE data block present, or if no .STRUCTURE and no .DEFINE type
+	present:
+
+- NAME.def      Fortran include file containing comments, parameters (if no
+		_o present) and/or common blocks and/or data definitions
+- NAME.inc      C include file containing the same
+- NAME_bd.for   Common block data-initialisation (if necessary)
+
+d. Always:
+
+NAME.LIS describing:
+- the input lines
+- the offset in and structure of common blocks and data structures.
+
+
+4. Comment lines
+
+
+Commment outside data blocks will be considered to be comments for the .dsc
+file only.
+Comments inside data blocks will form part of the program output. Lines
+starting with a ! will be output proceeding the data items following. Other
+comments will always follow the data items they follow.
+
+
+5. % commands
+
+%name commands steer the compiling process. Some action may be dependent on
+wether it is inside or outside data blocks. The following commands are
+recognized:
+
+%NAME=string            name of output files to be used.
+			Default: input file name
+%DATE=yymmdd            date of producing output
+			Default: today
+%USER=name              name of user
+			Default: login name
+%VERSION=num            Current version
+			Default: 1
+%SYSTEM=num             Current system
+			Default;1
+
+%%NAME                  will show currently defined name
+%%DATE                  .. date
+%%USER                  .. user
+%%VERSION               .. version
+%%SYSTEM                .. system
+
+If more than one of the above commands are encountered, the last will be
+used
+
+
+%[NO]LIST               list lines in log (e.g. to suppress include file
+listing)
+			Default: LIST
+%[NO]PRINT              list comments in output (not fully implemented)
+			Default: print
+%[NO]ALIGN              align data items on their lengths (complex data on
+			their constituant length; structure on the largest
+			element length included in the structure)
+
+The above act as switches
+
+%INSERT=string          include specified file
+%INCLUDE=string         include specified file
+			As a rule the string will be of the form NAME_DSF,
+			referencing an include file name.dsf
+
+The above are identical
+
+%COMMENT=string         include specified comment at begin of output file
+%REVISION=nam=yymmdd=string include specified comment as a revision
+%FORTRAN=string         include the Fortran statement (e.g. IMPLICIT NONE).
+			If outside data block: at begin of output; if inside:
+			at end of output
+%CC=string              include the C statement
+
+The above act additive
+
+%LOCAL=name=expr        specify a local variable name with a value expr.
+			The value of the name can be an integer value, or
+			a character string. If the expr can be evaluated to
+			an integer constant it will have an integer value,
+			else a character string value.
+			In most places were information has to be supplied it
+			can be supplied as:
+			- integer expression: containing known variable names,
+			  integer constants (), +-*/, +- unary
+			- character expression: single known name with a
+			  character value
+			- string (anything that cannot be interpreted as
+			  one of the above)
+			Note: an expression starting with a ( will be
+			deemed to have been ended at the belonging ). This
+			is for some formatting reason.
+			Note: / is only recognised if not preceded and or
+			followed by blanks. This is to recognize the /../
+			initialisation
+			Examples:
+			2.              is string "2."
+			01              is value 1 (and string "1" if
+appropiate)
+			(1)*2           is string "(1)*2"
+			+(1)*2          is value 2 ("2" string)
+
+%GLOBAL=name=expr       identical to the combination:
+			%LOCAL=name=expr
+			.PARAMETER
+				name    tp      /expr/
+			where tp is either J or C(length expr)
+
+
+6. . commands
+
+. commands define some aspects of the data commands present. Recognized:
+
+
+.END                    ends blocks starting with .STRUCTURE, .DEFINE, or
+			.MAP
+.DEFINE                 starts a 'define-block'
+			Can only occur once outside a data block (define-
+			or struct-block). The sub-type will initially be
+			data
+.STRUCTURE[=sname]      starts a structure block with name sname or NAME
+			can occur inside or outside a define-block. Many
+			structure blocks are allowed, but they may not be
+			nested (there references (see S:) may, of course,
+			be nested.
+			Each structure block should have a unique name
+			(i.e. only one unnamed allowed). The sub-type
+			will initially be data
+.BEGIN[=sname]          identical to .STRUCTURE (for historical reasons)
+
+The above define the type of current data block. It will define the output
+files produced, and which sub-types are allowed.
+
+
+.[OFFSET]=nexpr         will define a current offset
+			Only for structure-blocks; assumed to be in data-sub
+			For define-blocks allowed in common-sub
+.ALIGN=nexpr            Align offset on specified lengths (note the program
+			knows the defined local variables LB_B etc)
+			Allowed in common-sub en structure data-sub
+.MAP[=nexpr]            will start equivalence structures
+.UNION[=nexpr]          will start the next structure to be equivalent
+			The nexpr will serve as an id that can be used in
+			the WNT translation tables to get the proper
+			translation of the data; and is used to generate
+			a name for C. Definition ends at .END
+			Can only be used in structure-blocks at data-sub
+			Note: Not implemented yet, but its action can be
+			made by the equivalence = (except for the translation
+			choice option)
+.PARAMETER              Interprets following data lines as parameters
+.DATA                   Interprets following lines as data
+.COMMON[=cname]         Interprets following lines as to belong to common
+			cname_COM (or NAME_COM)
+			Only in define-block
+
+7. Data commands
+
+A data command describes a data-item. It consists of two mandatory fields
+separated by blanks, and an optional (obligatory for parameters and implied
+lengths) initialisation and an optional editing field (only allowed for
+structure data-sub).
+A full command is:
+
+	name[=rnam]     type    [/init, ..../] [<edit>]
+
+Name can be "-" to indicate a dummy name (to be used for filling) or a name
+starting with an alphabetic (including _$) character and having only
+alphanumeric characters (including _$).
+The name can be followed with an '=' followed by a reference name (not valid
+for parameter data). The data will be put at the same offset as the data at
+the reference name. Limitations:
+- rnam should immediately precede name in the same sub-block, i.e. all names
+	referencing the same rnam should be continuous after rnam
+- name should describe an entity not larger than the entity of rnam
+- if in ALIGN mode, the alignment of name should be of the same or lesser
+	value than that of rnam
+
+Type describes the data entity. It consists of a type indicator, optionally
+followed by an array definition.
+
+The indicator can be:
+	-  B  I1                byte
+	I  I2                   integer*2
+	J  I4                   integer*4
+	K                       long integer (for now identical to J)
+	E  R4                   real*4
+	D  R8                   real*8
+	X                       complex*8
+	Y                       complex*16
+	A                       double length ASCII
+	Cnexpr                  character*(nexpr)
+	C*                      character*(*) (length from initialisation
+				string; hence only allowed for parameters
+				and data in common-sub or define data-sub
+	S:name                  structure as defined by name
+	A:[([start][,inc])]     enumeration(add). If in a data-type mode in
+				define-block, it will generate a character
+				string array with an implied length from
+				the initialisation data, containing the
+				strings provided and a final ' ' string.
+				This variable can then be used in e.g.
+				WNCAFU to do a minimax search for its
+				occurrence. In addition (and in all other
+				cases only) it will produce a series of
+				parameters consisting of pre_txt with
+				values starting at start and incrementing
+				with inc, where the txt is the first three
+				(or less if not existing) characters of the
+				strings, and pre__N will be defined to give
+				the number of values+1; pre__I the increment
+				and pre__L and pre__H the lowest and highest
+				values. The pre__*
+				will also be available as local variables.
+				Default start, inc: 1
+				E.g.:
+				cb  E:          /structure,define,end/
+				will produce:
+				  CHARACTER*(10) CB__TXT(4)
+				    DATA CB__TXT/'STRUCTURE','DEFINE','END',' '/
+				  INTEGER CB_STR,CB_DEF,CB_END,CB__N,
+						CB__I,CB__H,CB__L
+				    PARAMETER(CB_STR=1,CB_DEF=2,CB_END=3,
+						CB__N=4,CB__I=1,CB__L=1,CB__H=3)
+	AR:[([start][,inc])]    as A:, but the parameter names will be *_pre
+	M:[([start][,fac])]     enumeration(mul). As A:, but multiplicative
+				rather than additive.
+				Default start, fac: 1, 2
+	MR:[([start][,fac])]    as M:, but *_pre parameters
+	N:[(val,...)]           enumeration(named). As A:, but values are
+				specified (up to number of array indices
+				allowed, currently 16).
+				Default val: 1,2,3,...
+				Note: No __H,__L and __I produced
+	NR:[(val,...)]          as N:, but *_pre parameters
+
+	[A|M|N][R][F][*]:[...]  as A: M: or N:, but Reversed name_ if R present,
+				full name (rather than 3 first characters)
+				if F present, no __ names and text if * present.
+
+
+
+
+Array specification:
+
+	(nexpr[:nexpr],....) The last index (i.e. the high-bound) can be
+specified as '*' to indicate an implied length to be deduced from the
+initialisation string (if this was allowed). All format types except
+A:, M: and N: can have an array index.
+
+
+Initialisation data:
+
+	/init, .../  each init can be an expression, or (nexpr)init. In the
+latter case the (nexpr) gives a repeat factor.
+If the format was character and the string contains blanks, ',' '/' or
+anything that can be but should not be interpreted as an expression (e.g.
+'02' which may not be converted to '2'), or is case sensitive, it should be
+enclosed in "".
+
+
+Edit data:
+
+	<format,code,units,special>
+
+Each field may be omitted, trailing ',' may be omitted.
+	format:         WNCTXT (WNCTXI) type format (e.g. AEF12.6)
+			Default: deduced from item
+	code:           0: editing of field allowed, >0: not allowed
+			Default: 0
+	units:          string specifying units (e.g. "deg")
+			Default: " "
+	special:        string to indicate something special defined by user
+			of edit data (e.g. if formatting types are not
+			sufficient, e.g. to type interferometer names)
+			Default: " "
+			The special field is used for S: fields, the default
+			will be "S:NAME". By definition the user can put
+			anything in it. The only definition I have now is:
+			"D:NAME" for a field containing a disk pointer to
+			to a structure NAME. The editing routine will be
+			extended to recognise these special codes.
+
+8. Program changes, omissions
+
+The following features are not fully implemented yet:
+
+- initialisation of structures (relatively easy, will do soon)
+- MAP/UNION: the = feature caters for everything except the run-time choice
+	of translation table. This last feature is probably dangerous anyway.
+	If the need arises, easily to implement.
+- C: I have only tested that the .inc files look ok, and are all accepted
+	by the C compilers.
+
+The following existing programs need changes:
+
+- ncomp/ndel.ssc: to change to WNTINC: done
+- no _m.mvx output: use existing ones by preserving them. If the f??.dsc files
+	change, the .mvx has to change. However, the DECalpha has a different
+	assembler from the VAX, and changes are necessary anyway in the
+	existing Macro programs (i.e. the I/O routines).
+	I have done the preservation, and will look at changing the Macro
+	programs to Fortran.
+- no .RECORD: it has been enhanced by the S: data item: scw.dsc and ohw.dsc
+	uses this: change done
+- output now _o.inc rather than -c.inc to get uniform naming: wnf I/O
+	routines have to change: done
+
+
+9. Detailed program output
+
+
+The output of the program consist of:
+- parameters
+- structure definitions
+- data definitions
+- common defintions
+- translation tables
+- edit tables
+
+- Parameters
+
+Parameters are output in Fortran as PARAMETER, with name and type as given.
+In C as #define NAME init-text
+Note: Maybe they should be given as:
+	#define NAME (cast) init-text   ?? comments please
+For A:, M:, N: type the following INTEGER PARAMETERs are produced:
+	NAME__N                 # of items in list +1 (==first available
+				element). Also available as local variable
+	NAME__L                 First value (not for N:)
+	NAME__H                 Last value (not for N:)
+	NAME__I                 Increment(A:) or factor(M:)
+	NAME_txt                For each non-empty init-txt (i.e. not ,, or ,/)
+				the first 3 char of the text (or less if
+				shorter text) are taken as txt.
+
+- Structure definitions
+
+Structure definitions are given in C as:
+	struct struct-name { type name [indices]; ,,,};
+All names in lc; indices in reversed order from Fortran.
+In Fortran each given name is combined with the struct-name sname to
+produce the following INTEGER PARAMETERs:
+	SNAME__L                Byte length of structure
+	SNAME__V                Version
+	SNAME__S                System
+In the edit output:
+	SNAME__EL               Length of edit arrays
+The above are also available as %LOCAL constants
+For historic reasons also available:
+	snameHDL
+	snameHDV
+	snameHDS
+	snameEDL
+For all structure elements:
+	SNAME_NAME_1            Byte offset from start of structure
+In addition for CHARACTER data:
+	SNAME_NAME_N            Length in characters
+for STRUCTURE data:
+	SNAME_NAME_N            Length in bytes
+for all if the offset from the beginning is an integer multiple of the unit
+size of the data type (e.g. LB_J=4 for INTEGER; structure length for structure):
+	SNAME_NAME_type         Offset in unit-length units from start
+				of structure. Types are the types as given
+				in the definition (C,J,E,Y,S etc)
+
+
+
+Automatic formatting of data structures
+---------------------------------------
+	(contributed 941010 by JPH,
+	 based on research and correspondence with WNB)
+
+
+	WNTINC copies the edit directives in <xxx>.DSC literally to <XXX>_E_DEF.
+The directives are not interpreted, so they may have any form; double quotes
+can be used to include blanks etc.".
+
+	They must fit, however, in elements of the CHARACTER array declared in
+the latter file. The declaration is written by WNTIOS through WNCTXT calls. On
+941010 the length has been increased fro 10 to 12 characters.
+
+	The directives are read and interpreted by NSCXXS. This routine imposes
+some formatting constraints and defaults of its own. See the comments in that
+file.
diff --git a/src/doc/txt/xmosaic_restart.txt b/src/doc/txt/xmosaic_restart.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6adc97a418cc72e412e0cdb63bcf2448e0e1831a
--- /dev/null
+++ b/src/doc/txt/xmosaic_restart.txt
@@ -0,0 +1,51 @@
+
+Xmosaic restart protocol
+========================
+
+	xmosaic is started by genaid.exe. genaid stores the pid of xmosaic in a
+file /tmp/xm-<display name>, where <display name> is derived from the
+environment variable DISPLAY by substituting a dot for each colon.
+
+	To access xmosaic from a parameter prompt in a Newstar program, PPDHELP
+call genmosaic.cun. The latter routine reads the file created by genaid to
+retrieve xmosaic's pid, <pid>. It then follows the protocol defined by xmosaic
+to access the appropriate help information in mosaic form:
+
+
+	1. Create a file /tmp/Mosaic.<pid>, containing the lines
+
+		goto
+		file://localhost/<directory>/file.html
+
+	2. Sending a SIGUSR1 signal to process <pid>.
+
+The latter signal causes xmosaic to opend the file /tmp/Mosaic.pid and act on
+its contents.
+
+
+Changes, early november 1994
+============================
+
+	Parameter .html files are now clustered in one .html file per .psc or
+.pef file. Finding the right target for display by mosaic requires some
+searching, which is done most easily in a .csh script:
+
+	set target = \
+	    `grep -l <Keyword> $n_hlp/intfc/<program>_private_intfc.psc`
+	if ($#target != 0) then
+	  set typ = 'private'
+	else
+	  set target = `grep -l <Keyword> $n_src/*/*.pef`
+	  if ($#target != 0) then
+	    set typ = 'public'
+	  else
+	    <emit error message>
+	endif
+	set label = `echo <keyword> sed -e 'y:A...Z_:a...z.:' `
+	echo 'goto' >! /tmp/Mosaic.<pid>
+	echo \
+"file://localhost$n_hlp/<pgm>_${typ}_intfc/<pgm>_${typ}_intfc.html#$target" \
+	  >> /tmp/Mosaic.<pid>
+	ln -s /tmp/Mosaic.<pid> /tmp/xmosaic.<pid>
+	kill -SIGUSR1 <pid>
+
diff --git a/src/nmap/mph.dsc b/src/nmap/mph.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..f1d42fe4ff5271c1d725b121ce8e1d16c956b525
--- /dev/null
+++ b/src/nmap/mph.dsc
@@ -0,0 +1,111 @@
+!+ MPH.DSC
+!  WNB 910219
+!
+!  Revisions:
+!
+%REVISION=CMV=940517="Add JOBP (pointer to job-summary)"
+%REVISION=WNB=931216="Add some edit formats"
+%REVISION=WNB=931015="Use SSH"
+%REVISION=WNB=930803="Text only"
+%REVISION=WNB=920828="Add VELC, VELR, FRQ0, FRQV, FRQC, INST"
+%REVISION=WNB=920818="Add VEL"
+%REVISION=WNB=910219="Original version"
+!
+!	Define Map Header block
+!
+%COMMENT="MPH.DSC defines the map header block"
+%COMMENT=" "
+!
+%VERSION=1					!VERSION
+%SYSTEM=1
+%USER=WNB
+%%DATE
+%%NAME
+!-
+.PARAMETER
+.BEGIN=MPH
+%INCLUDE=SSH_DSF				!STANDARD AREA
+	FNM	C12				!FIELD NAME
+	EPO	E		<E12.1>		!EPOCH (E.G. 1950.0)
+	RA	D		<DAF12.7>	!RIGHT ASCENSION (CIRCLES)
+	DEC	D		<DAF12.7>	!DECLINATION (CIRCLES)
+	FRQ	D		<D12.6>		!FREQUENCY (MHZ)
+	BDW	D		<D12.6>		!BANDWIDTH (MHZ)
+	RAO	D		<DAF12.7>	!OBSERVED RIGHT ASCENSION (CIR)
+	DECO	D		<DAF12.7>	!OBSERVED DECL. (CIRCLES)
+	FRQO	D		<D12.6>		!OBSERVED FREQ. (MHZ)
+	ODY	I				!OBSERVED DAY SINCE JAN 0
+	OYR	I				!OBSERVED YEAR OR 0 (E.G. 1985)
+	DCD	I				!DATA CODE:
+						! 2= I
+						! 4= J
+						! 5= E
+						! 8= D
+	PCD	I				!PROGRAM CODE:	0= NMAP
+	SRA	D		<DAF12.7,1>	!SEPARATION IN RA (CIRCLES)
+	SDEC	D		<DAF12.7,1>	!SEPARATION DEC (CIRCLES)
+	SFRQ	D		<D12.6>		!SEPARATION FREQ. (MHZ)
+	NRA	J		<,1>		!# OF POINTS IN RA
+	NDEC	J		<,1>		!# OF POINTS IN DEC
+	NFRQ	J		<,1>		!# OF POINTS IN FREQ.
+	ZRA	J				!CENTRE RA (1ST POINT=0)
+	ZDEC	J				!CENTRE DEC (1ST LINE=0)
+	ZFRQ	J				!CENTRE FREQUENCY (1ST MAP=0)
+	MXR	J				!POSITION MAX. IN RA
+	MXD	J				!POSITION MAX. IN DEC
+	MXF	J				!POSITION MAX. IN FREQUENCY
+	MNR	J				!POS. MIN. RA
+	MND	J				!POS. MIN. DEC
+	MNF	J				!POS. MIN. FREQ.
+	MAX	E		<E12.3>		!MAX. IN MAPS
+	MIN	E		<E12.3>		!MIN. IN MAPS
+	SHR	D		<DAF12.7>	!SHIFT IN RA (ADD, CIRCLES)
+	SHD	D		<DAF12.7>	!SHIFT IN DEC (ADD, CIRCLES)
+	SHF	D		<D12.6>		!SHIFT IN FREQ. (ADD, MHZ)
+	SUM	D		<D12.6>		!NORMALISING SUM
+	UNI	E		<E12.1>		!MULTIPLIER TO GET JY
+	UCM	C24				!USER COMMENT
+	NPT	J				!# OF INPUT DATA POINTS
+	TYP	C4				!MAP TYPE (MAP, AP, COV ETC)
+	POL	C2				!POL. TYPE (OR SO)
+	CD	I(0:7)				! 0: TAPER TYPE
+						! 1: CONVOLUTION TYPE
+						! 2: CORRECT FOR CONVOLUTION
+						! 3: CLIPPING DONE
+						! 4: SOURCE SUBTRACTION
+						! 5: DATA TYPE
+						! 6: UV COORDINATE TYPE
+						! 7: DE-BEAM COUNT
+	EPT	I				!MAP EPOCH USED:
+						! 0: APPARENT
+						! 1: AS SPECIFIED IN EPOCH
+	OEP	E		<E12.2>		!OBSERVATION EPOCH (EG 1985.78)
+	NOS	E		<E12.3>		!MAP NOISE (W.U.)
+	FRA	E		<EAF12.4>	!FIELD SIZE RA (CIRCLES)
+	FDEC 	E		<EAF12.4>	!FIELD SIZE DEC (CIRCLES)
+	FFRQ	E		<E12.3>		!FIELD SIZE FREQ (MHZ)
+	TEL	C8				!NAME OF TELESCOPE
+	FSR	J				!FFT SIZE RA
+	FSD	J				!FFT SIZE DEC
+	MDP	J		<XJ,1>		!MAP DATA POINTER
+	NBL	J				!# OF BASELINES IN MAP
+	NST	J				!# OF SETS IN MAP
+	VEL	E		<E12.1>		!VELOCITY IN M/S
+	VELC	J				!VELOCITY CODE:
+						! 0= CONTINUUM
+						! 1= HELIOCENTRIC RADIO
+						! 2= LSR RADIO
+						! 3= HELIOCENTRIC OPTICAL
+						! 4= LSR OPTICAL
+	VELR	E		<E12.4>		!VELOCITY AT REF. FREQ. (FRQC)
+	INST	J				!INSTRUMENT:
+						! 0= WSRT
+						! 1= ATCA
+	FRQ0	D		<D12.6>		!REST FREQUENCY FOR LINE (MHZ)
+	FRQV	D		<D12.6>		!REAL FREQUENCY FOR LINE (MHZ)
+	FRQC	D		<D12.6>		!CENTRE FREQUENCY FOR LINE (MHZ)
+	JOBP	J		<XJ,1>		!POINTER TO JOB SUMMARY LOG
+	JOBL	J		<XJ,1>		!LENGTH (IN BYTES) OF LOG
+	-	-(152)				!RESERVED
+.END
+!-
diff --git a/src/nscan/fdw.dsc b/src/nscan/fdw.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..af09ce1ec2dabe250ddf78b73e60c88e3fcc819c
--- /dev/null
+++ b/src/nscan/fdw.dsc
@@ -0,0 +1,76 @@
+!+ FDW.DSC
+!  WNB 900118
+!
+!  Revisions:
+!
+%REVISION=CMV=940414="Add historical notes"
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=WNB=900118="Tape vs 7, system 59"
+!
+!	Define WSRT FD block
+!
+%COMMENT="FDW.DSC defines the WSRT FD block"
+!
+!
+%VERSION=7					!VERSION
+%SYSTEM=59
+%USER=WNB
+%%DATE
+%%NAME
+!-
+.PARAMETER
+.BEGIN=FDW
+				! (*) means use with care, not repaired
+	CBI	I		!Unequal data block flag (32767)
+	CBT	C2		!Type identification: File Description (FD)
+	NFD	J		!Record number of this record
+	LFD	J		!Number of FD records in this group
+	NFDE	J		!First FD record number at end of dataset
+	SDAY	I		!Local U.T. day number
+				!  FVERS<5: ST
+	STIM	I		!Start U.T. time in units of 10 sec.
+				!  FVERS<5: ST
+				!  FVERS<3: units of minutes 
+	ETIM	I		!End U.T. time in units of 10 sec. (*)
+				!  ols<43: -32768
+	-	I		!Empty (Delete character)
+	FVERS	I		!Tape format version
+	LRCRD	I		!Record length in bytes
+	PHBLL	I		!Total number of records per block
+	NOBS	I		!Number of simultaneous observations
+	OLSYS	I		!Online program system nr. (*)
+				!  ols<46: reserved
+	-	-(0:1)
+	COH	C2		!'OH'
+	LOH	I		!Number of OH records per OH group
+	NOH	J		!First record number of first OH group
+	MOH	J		!Number of OH groups
+				!  FVERS<7: NOHE = recnr backup OH record
+	CSC	C2		!'SC'
+	LSC	I		!Number of SC records per SC group
+	NSC	J		!First record number of first SC group
+	MSC	J		!Number of SC groups
+	CSH	C2		!'SH'
+	LSH	I		!Number of SH records per SH group (*)
+				!  FVERS>6: Max length, SH's may differ
+	NSH	J		!First record number of first SH group
+	MSH	J		!Number of SH groups or number of sets
+	CIH	C2		!'IH'
+	LIH	I		!Number of IH records per IH group
+	NIH	J		!First record number of first IH group
+	MIH	J		!Total number of IH groups
+	CDB	C2		!'DB'
+	LDB	I		!1
+	NDB	J		!First record number of first DB group
+	MDB	J		!Total number of DB records
+	-	-(0:3)
+	NBL	J		!Total number of blocks within the dataset
+	VOLUME	C6		!Name of magnetic volume or tape
+	LABEL	C4		!Name of dataset or label
+	LENGTH	I		!Total length in feet of the dataset
+	REDDATE	J		!Civil date on which the dataset was made in
+				!the format YYDDD (Y : year, D : daynumber)
+	REDTIME	I		!Civil time in minutes on which the dataset was made
+	-	-(0:5)
+.END					!END DEFINITION
+!-
diff --git a/src/nscan/ihw.dsc b/src/nscan/ihw.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..0f8f5ab605381a07f234d00ee2c3466e1225d5c9
--- /dev/null
+++ b/src/nscan/ihw.dsc
@@ -0,0 +1,91 @@
+!+ IHW.DSC
+!  WNB 900118
+!
+!  Revisions:
+!
+!
+!	Define WSRT IH block
+!
+!
+!
+%VERSION=7					!VERSION
+%SYSTEM=59
+%USER=WNB
+%%DATE
+%%NAME
+%REVISION=CMV=940414="Add historical notes"
+%REVISION=WNB=900118="Tape vs 7, system 59"
+%COMMENT="FDW.DSC defines the WSRT IH block"
+!-
+.PARAMETER
+.BEGIN=IHW
+				! (*) means use with care, not repaired
+	CBI	I		!Unequal data block flag (32767)
+	CBT	C2		!Identification: Interferometer Header (IH)
+	NIH	J		!Record number of this record
+	LIH 	J		!Number of IH records in this group
+	IHLNK	J		!First record of the next IH group
+	SDAY	I		!Local U.T. day number
+				!  FVERS<5: ST
+	STIM	I		!Start U.T. time in units of 10 sec
+				!  FVERS<5: ST
+				!  FVERS<3: units of minutes 
+	BANDNR	I		!Frequentie bandnr. (*)
+				!  FVERS<6: Setnr.
+	INFNR	I		!Interferometer number of this infr. (*)
+				!  See SHW.DSC
+	WTEL	I		!West telescope indicator: 0-D is 0...13 (*)
+				!  See SHW.DSC
+	OTEL	I		!East telescope indicator: 0-D is 0...13 (*)
+				!  See SHW.DSC
+	BFREQ	J		!Set frequency (2**(-16) Mhz) (*)
+				!  FVERS<2: single float (E) 
+	DRT	E		!Baseline of the interferometer (M)
+	HAB	E		!Start hourangle, middle of the first
+				!integration time in U.T. sec
+				!  FVERS<5: in S.T. sec
+	HAE	E		!End hourangle, middle of the last
+				!integration time in U.T. sec
+				!  FVERS<5: in S.T. sec
+	DHA	E		!Hour angle increment (Integration time in U.T. sec)
+				!  FVERS<5: in S.T. sec
+	LD	I		!Number of data records in this group (*)
+				!  FVERS<6: in S.T. sec
+	NDATP	I		!Number of data points, inclusive NDELP
+	NDELP	I		!Number of deleted data points
+	NEXP	I		!Common exponential scaling factor
+				!  ols=42: should be 1
+	FSCAL	I		!Common multiplication scaling factor
+				!  ols=42: should be 1
+	OFFS	I		!Common offset scaling factor
+	NOISE	E		!Amplitude noise
+				!  FVERS<3: NOISE...MEPHA are empty
+	ACOS	E		!Average cosine
+	MECOS	E		!Mean error in average cosine
+	MACOS	I		!Maximal cosine
+	MICOS	I		!Minimal cosine
+	ASIN	E		!Average sine
+	MESIN	E		!Mean error in average sine
+	MASIN	I		!Maximal sine
+	MISIN	I		!Minimal sine
+	AAMP	E		!Average amplitude
+	MEAMP	E 		!Mean error in average amplitude
+	MAAMP	I		!Maximal amplitude
+	MIAMP	I		!Minimal amplitude
+	APHA	E		!Average phase
+	MEPHA	E		!Mean error in average phase
+	INCT	I		!Increment time in U.T. sec.
+				!  ols=52: float
+				!  FVERS<5: in S.T. sec.
+	DWELT	I		!Time per mosaicking pattern pos. per radial
+				!in sec. (=INCT if no mosaicking)
+				! ols<60: reserved
+	VOLGNR	J		!Observation number (*)
+				! FVERS<2: reserved
+	INTT	E		!Integration time in U.T sec.
+				! ols<53: reserved
+	DRADT	I		!Time between 2 successive radials of the same
+				!mosaicking pattern in sec (=INCT if no mos.)
+	-	-(0:5)		!	    -
+.END					!END DEFINITION
+!-
diff --git a/src/nscan/ohw.dsc b/src/nscan/ohw.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..641e2e5ac99321db5faf51a1fcef64eda80422d4
--- /dev/null
+++ b/src/nscan/ohw.dsc
@@ -0,0 +1,178 @@
+!+ OHW.DSC
+!  WNB 900118
+!
+!  Revisions:
+!
+%REVISION=JPH=970220="Add PATPO, PATFD"
+%REVISION=CMV=960228="Increased max. number of SETS"
+%REVISION=CMV=940829="Change max. number of SETS"
+%REVISION=CMV=940414="Add historical notes"
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=WNB=930803="Change .RECORD"
+%REVISION=WNB=920813="Add MSNP"
+%REVISION=WNB=911022="Add SPEFU"
+%REVISION=WNB=900118="Tape vs 7, system 59"
+!
+!
+!	Define WSRT OH block
+!
+!
+%COMMENT="OHW.DSC defines the WSRT OH block"
+!
+%VERSION=7					!VERSION
+%SYSTEM=59
+%USER=WNB
+%%DATE
+%%NAME
+!-
+%LOCAL=MAXSET=5000		!Maximum number of sets
+.PARAMETER
+	OHWSET	J	/MAXSET/
+!
+.STRUCTURE=SET			!Set definitions
+	BFREQ	J		!Set observing frequency (2**(-16).Mhz) (*)
+				!  FVERS<2: single float (E)
+	DATYP	C2		!Data type (IF, XX, XY, YX, or YY)
+	BANDNR	I		!Band number
+	NSH	J		!First record number of current set
+.END				!End SET definition
+.BEGIN=OHW
+				! (*) means use with care, not repaired
+	CBI	I		!Unequal data block flag (32767)
+	CBT	C2		!Type identificator: Observation Header (OH)
+	NOH	J		!Record number of this record
+	LOH	J		!Number of OH records in this group with 
+				!information (*)
+				!  FVERS<5: erroneous (always 54)
+	NOHN	J		!First OH record number of next group (last:-32768)
+	SDAY	I		!Local U.T. day number
+				!  FVERS<5: ST
+	STIM	I		!Start U.T. time in units of 10 sec.
+				!  FVERS<5: ST
+				!  FVERS<3: units of minutes 
+	ETIM	I		!End U.T. time in units of 10 sec.
+				!  ols<43: -32768
+	-	I		!Empty (Delete character)
+	NSC	I		!First record number of SC group
+	PROJECT	I		!Project number
+	FIELD	C12		!Fieldname
+	VOLGNR	J		!Observation number (yynnnnn)
+				!  FVERS<2: no year (yy) in number 
+				!  ols=57:  yyyy in stead of yy (00327..00586
+	STUURC	I		!Online peripherals control bits (*)
+				!  FVERS<3: line (1) or cont (0)
+	TYPE	C2		!Observation type
+	DATE	I(6)		!Epoche and civil start time of the observation
+	PRFLG	I		!Online program flags (*)
+				!  FVERS<3: reserved
+	OLSYS	I		!Online program system nr.
+				!  FVERS<3: reserved
+	JDAY	D	<D12.2>	!Time of the middle of the observation in julian days
+	BECEN	D	<D12.7>	!Time of the middle of the obs. in bessel centuries
+	JUCEN	D	<D12.7>	!Time of the middle of the obs. in julian centuries
+	FREQC	I		!Observing frequency code
+	CATEG	C2		!Astronomical type of observation
+	ALLOC	I 		!Program committee allocation code
+	REQUEST	C4		!Date of reception request from by tel. group
+	STATBG	J(0:1)		!Status BG corrections
+	STATBE	J(0:1)		!Status BE corrections
+	STATSE	J(0:1)		!Status SE corrections
+	POPER	I		!Period on pointing grid point 
+				!(Units 10 sec) (*)
+				!  FVERS<5: NOBSN
+	DXBIT	B(0:1)		!DXB control bit
+	APCS	B(0:1)		!DXB recycling instel code
+	RA1	D	<DAF12.7> !Right ascension fieldcentre of epoche
+	DEC1	D	<DAF12.7> !Declination fieldcentre of epoche
+	MODE	I		!Digital correlator mode
+	POLC	I 		!Dipole position code
+	BAND	E	<E12.6>	!Total bandwidth (DLB). Sum of all bands (DCB)
+	NTOT	I		!Total number of channels (*)
+				!  FVERS=(>?)6: 4096 for DCB
+	NFREQ	I		!Total number of frequency points or bands
+	SFREQ	I		!Spacing of the frequency points in
+				!units of 0.1 Khz (Only DLB)
+				!DCB --> CDCBD - Bitcode 
+				!Bit 0 - 7: Describing used bands (Band: 1 - 8)
+				!Bit 8 -15: Describing used bandwith (1 = 5 Mhz,
+				!0 = 10 Mhz)
+	NRPOL	I		!Number of polarization channels
+	NRINT	I		!Number of interferometers (*)
+				!  FVERS>=6: number of standard ifrs
+	TELWD	I(0:1)		!Receiver in use/not in use code
+	BSINT	I		!Basic intergration time of the backend (U.T.)
+				!  FVERS<5: S.T.
+				!  ols=52:  0.1 U.T. sec
+	CONFNR	J		!System configuration number
+	BECODE	C4		!DLB ,DCB ,DXB .
+				!  FVERS<6: reserved (always DLB)
+	RA0	D 	<DAF12.7> !Apparent right ascension field centre at middleof obs.
+	DEC0	D	<DAF12.7> !Apparent declination field centre at middle of obs.
+	FREQ	D	<D12.6> !Obs. freq. of middle of band for middle of
+				!observation (DLB) or primary fringe stopping
+				!Frequency (DCB).
+	HAST	D	<DAF12.7> !Hour angle middle of first 10 sec U.T. period
+	HAEND	D	<DAF12.7> !Hour angle middle of last 10 sec  U.T. period
+	LST	D	<DAF12.7> !Local sidereal time of middle of the observation
+				! PARALLAX...RDEC2 lots of changes FVERS<4 (*)
+	PARALAX	E	<EAF12.7> !Paralax for apparent observations (Epoche= 9)
+				!in circles
+	RRA1	E	<E12.8>	!Pointing offset or linear rate in R.A. 
+				!(Circles per juliaans day or degrees/U.T.day)
+	RDEC1	E	<E12.8>	!Pointing offset or linear rate in DECL.
+				!(Circles per juliaans day or degrees/U.T.day)
+	RRA2	E		!Pointing offset or quadratic rate in R.A.
+				!(Circles per juliaans day or degrees/U.T.day**2)
+	RDEC2	E		!Pointing offset or quadratic rate in DECL.
+				!(Circles per juliaans day or degrees/U.T.day**2)
+	VLCTY	E		!Velocity (Km/sec) in system given by velc
+				!(DCB - empty)
+	VELC	I		!Velocity reference system code (DCB - empty)
+				! INX...FDEC3 lots of changes FVERS<4
+	INX	I		!Telescope bits for pointing offset
+	DRA	E	<EAF12.7> !Pointing offset in RA  (Circles)
+	DDEC	E	<EAF12.7> !Pointing offset in DEC (Circles)
+	NPC	I		!Period on the centre (Units of 10 sec.)
+	NPS1	I		!Period on source 1   (Units of 10 sec.)
+	FDRA1	E	<EAF12.7> !Offset in RA  for source 1
+	FDEC1	E	<EAF12.7> !Offset in DEC for source 1
+	NPS2	I		!Period on source 2   (Units of 10 sec.)
+	-	-(0:1)		!            -
+	FDRA2	E	<EAF12.7> !Offset in RA  for source 2
+	FDEC2	E	<EAF12.7> !Offset in DEC for source 2
+	NPS3	I		!Period on source 3   (Units of 10 sec.)
+	-	-(0:1)		!            -
+	FDRA3	E	<EAF12.7> !Offset in RA  for source 3
+	FDEC3	E	<EAF12.7> !Offset in DEC for source 3
+	-	-(0:1)		!            -
+	SPEFU	C2		!Special observation type code
+				!  ols<61: reserved
+				!  VOLGNR 9100750..9101671: archive in EBCEDIC 
+	POST	J(0:13)		!Position telescopes in 2**(-16) M
+	TAPER	I		!Code of weighting function used for the
+				!Fourier transform to frequency (DCB - empty).
+	DEVC0	B(0:1)		!Device code bits (*)
+				!  ols<43: reserved
+	FREQ0	D	<D12.6>	!Rest freq. for line observations (Line) or
+				!observing freq. (DCB), 0 if FREQC<10
+				!  FVERS<6: reserved 
+	STOPAR	I		!Data in channel-fluxes (0) or in stokes-
+				!parameters (1). (Dwingeloo use)
+				!  ols<43: reserved
+	MSPAT	I		!Mosaicking pattern number (=0: no mosaicking)
+				!  ols<60: reserved
+	MPOSN	I		!Position in mosaicking pattern (0,1,...,N-1)
+				!  ols<60: reserved
+	MSNP	I		!Number of pos. in mosaick pattern (else 1)
+				!  ols<62: reserved
+	-	-(0:17)		! - to be filled in -
+	PATPO	I	<XI>	!Mask of telescopes that scan in position
+	PATFD	I	<XI>	!Mask of telesc. that scan in fringe-stop
+				! and delay position 
+	-	-(0:267)	!	            -
+	NRSTS	I		!Total number of sets
+	NRFRQ	I		!Total number of frequency points
+	LENT	I		!Number of bytes per entry in the following table
+	SET	S:SET(0:MAXSET)	!Set definitions
+.END					!END DEFINITION
+!-
diff --git a/src/nscan/sch.dsc b/src/nscan/sch.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..3a9715322112cb262301e7f47fdee1756fc14b75
--- /dev/null
+++ b/src/nscan/sch.dsc
@@ -0,0 +1,94 @@
+!+ SCH.DSC
+!  WNB 900304
+!
+!  Revisions:
+!
+%REVISION=JPH=961112="Complete JPH 941007"
+%REVISION=HjV=950511="Add AOTHUSED:
+%REVISION=JPH=941010="add pseudo units for various fields; P(deg) --> P(rad)"
+%REVISION=JPH=941007="split tables in X and Y parts, format for 6 per line"
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=WNB=930803="Use NSTAR.DSF"
+%REVISION=JPH=930616="Apply/deapply and FL_ bit masks to cbits.dsc; comments"
+%REVISION=WNB=930604="Add FL_, change BITS contents"
+%REVISION=WNB=930602="Add IREF, AIREF, CLKC, ACLKC; SCH_M_IREF, CLK"
+%REVISION=WNB=930602="Delete DOB, DEGEN"
+%REVISION=JPH=930128="Add apply/deapply mask bits"
+%REVISION=WNB=921217="Add PANG"
+%REVISION=WNB=900304="Original version SCH"
+!
+!	Define Scan Header block
+!
+%COMMENT="SCH.DSC defines the scan header block"
+%COMMENT=" "
+%COMMENT="REDNS, ALGNS, OTHNS must be in this order and adjacent"
+%COMMENT=" "
+!
+%VERSION=1				!VERSION
+%SYSTEM=1
+%USER=WNB
+%%DATE
+%%NAME
+!
+! Get global # of telescopes
+!
+%INCLUDE=NSTAR_DSF
+!
+!-
+.PARAMETER
+	SCHTEL	J	/NSTAR_TEL/		! # OF TELESCOPES
+!
+.BEGIN=SCH
+	HA	E		<EAF12.7,,"deg">! APP. HA (CIRCLES)
+	MAX	E		<E12.3,,"W.U.">	! COS/SIN MAX (W.U.)
+	SCAL	E		<E12.6>		! COS/SIN SCALE MULTIPLIER - 1
+	REDNS		E(0:1)	<+,," ">
+	REDNSX=REDNS	E(0:1)	<E12.3,,"W.U.">	!REDUNDANCY NOISE (W.U., G/P)
+	REDNSY		E(0:1)	<E12.3,,"W.U.">	!REDUNDANCY NOISE (W.U., G/P)
+	ALGNS		E(0:1)	<+,," ">
+	ALGNSX=ALGNS	E(0:1)	<E12.3,,"W.U.">	!ALIGN NOISE (W.U., G/P)
+	ALGNSY		E(0:1)	<E12.3,,"W.U.">	!ALIGN NOISE (W.U., G/P)
+	OTHNS		E(0:1)	<+,," ">
+	OTHNSX=OTHNS	E(0:1)	<E12.3,,"W.U.">	!OTHER NOISE (W.U., G/P)
+	OTHNSY		E(0:1)	<E12.3,,"W.U.">	!OTHER NOISE (W.U. G/P)
+	BITS	J		<XJ>		!GENERAL BITS (8-15: flag bits)
+	CLKC	E		<E12.6,,"s">	!CLOCK CORRECTION (sec)
+	ACLKC	E		<E12.6,,"s">	!APPL. CLOCK CORRECTION (sec)
+	IREF	E		<EAF12.2,,"deg/km"> 
+						!IONOS. REFRACT. (CIRCLES/km)
+	EXT	E		<E12.5,,"factr-1">	! EXTINCTION FACTOR -1
+	REFR	E		<E12.5,,"mu-1">	! REFRACTION (MU-1)
+	FARAD	E		<EAR12.2,,"deg"> !FARADAY ROTATION (RADIANS)
+ 	REDC		E(0:1,0:NSTAR_TEL-1) <+,," ">
+ 	REDCX=REDC	E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					 	! X REDUNDANCY CORRECTION
+ 	REDCY		E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					 	! Y REDUNDANCY CORRECTION
+	ALGC		E(0:1,0:NSTAR_TEL-1) <+,," ">
+	ALGCX=ALGC	E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					 	! X ALIGN CORRECTION (LOG)
+ 	ALGCY		E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					   	! Y ALIGN CORRECTION (LOG)
+	OTHC 		E(0:1,0:NSTAR_TEL-1) <+,," ">
+ 	OTHCX=OTHC 	E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					  	! X OTHER CORRECTION (LOG)
+ 	OTHCY		E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					 	! Y OTHER CORRECTION (LOG)
+	IFRAC	J		<XJ,1,,P:IFRC>	!POINTER TO ADD IFR CORRECTIONS
+	IFRMC	J		<XJ,1,,P:IFRC>	!POINTER TO MUL. IFR CORRNS
+	AEXT	E		<E12.5>		!APPLIED EXTINCTION FACTOR -1
+	AREFR	E		<E12.5>		!APPLIED REFRACTION (MU-1)
+	AFARAD	E		<E12.2>		!APPLIED FARADAY rotation
+	AOTHC		E(0:1,0:NSTAR_TEL-1) <+,," ">
+	AOTHCX=AOTHC	E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					 	! X APPLIED OTHER CORRECTION
+ 	AOTHCY		E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"ln G, P(rad)">
+					 	! Y APPLIED OTHER CORRECTION
+	AIFRAC	J		<XJ,1,,P:IFRC>	!PTR TO APPL. ADD IFR CORRN
+	AIFRMC	J		<XJ,1,,P:IFRC>	!PTR TO APPL. MUL IFR CORRN
+	PANG	E		<EAF12.2,,"deg"> !PARALL. ANGLE (CIRCLES)
+	AIREF	E		<EAF12.2,,"deg/km"> 
+						!APPLIED IONOSPH.. REFRCTN
+	AOTHUSED	J			!1 = AOTH DE-APPLIED
+.END						!END DEFINITION
+!-
diff --git a/src/nscan/scw.dsc b/src/nscan/scw.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..9ac3024c127d65d9220f1f0c7c5a48883e987c73
--- /dev/null
+++ b/src/nscan/scw.dsc
@@ -0,0 +1,234 @@
+!+ SCW.DSC
+!  WNB 900118
+!
+!  Revisions:
+!
+%REVISION=CMV=940414="Add historical notes"
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=WNB=930803="Change .RECORD"
+%REVISION=WNB=911022="Add mosaicking RA/DEC"
+%REVISION=WNB=900118="Tape vs 7, system 59"
+!
+!
+!	Define WSRT SC block
+!
+!
+%COMMENT="SCW.DSC defines the WSRT SC block"
+!
+%VERSION=7					!VERSION
+%SYSTEM=59
+%USER=WNB
+%%DATE
+%%NAME
+!-
+.PARAMETER
+.STRUCTURE=SRC			!Subtracted sources
+	SRAI	D	<DAF12.7> !Right ascension subtracted source  nr. I
+	SDECI	D	<DAF12.7> !Declination subtracted source nr. I
+	SFXXI	E	<E12.3>	!Intensity XX subtracted source nr. I
+	SFXYI	E	<E12.3>	!    "     XY	"	   "	 "
+	SFYXI	E	<E12.3>	!    "     YX	"	   "	 "
+	SFYYI	E	<E12.3>	!    "     YY	"	   "	 "
+.END
+.STRUCTURE=BCOR			!Band corrections
+	PZ	I(32)		!Phase correction band 1
+	DOFS	I(32)		!Delay offset band 1
+	-	-(0:127)	!		-
+	TSYS	E(32)	 	!System temperatures band 1
+	GAIN	E(32)	 	!Receiver gainfactors band 1
+	NOIS	E(32)	 	!Noise source temperatures band 1
+	GNCL	I(32)	 	!Amplitude correction methods band 1
+	-	-(0:255)	!		-
+.END
+.STRUCTURE=MOZP			!Mozaicking positions
+	RA0	J		!RA epoch position
+	DEC0	J		!DEC epoch position
+	RA1	J		!RA apparent
+	DEC1	J		!DEC apparent
+	SDEC	J		!sin(DEC1)
+	CDEC	J		!cos(DEC1)
+	MVNPA	J(0:2)		!Apparent position vector
+	MDVNPA	J(0:2)		!Differential apparent position vector
+	FREQ1	D	<D12.6>	!Apparent band centre frequency (MHz)
+				!  ols<62: reserved
+	-	-(0:7)
+.END
+.BEGIN=SCW
+				! (*) means use with care, not repaired
+	CBI	I		!Unequal data block flag (32767)
+	CBT	C2		!Type identificator: System Calibration (SC)
+	NSC	J		!Record number of this record
+	LSC	J		!Number of SC records
+	NSCN	J		!First SC record of next SC group (=-32768 for last)
+	SDAY	I		!Local U.T. day number
+				!  FVERS<5: ST
+	STIM	I		!Start U.T. time in units of 10 sec.
+				!  FVERS<5: ST
+				!  FVERS<3: units of minutes 
+	ETIM	I		!End U.T. time in units of 10 sec. (*)
+				!  ols<43: -32768
+	-	I 		!Empty (Delete character)
+	CFE	J		!Code front end
+	CIF	J 		!Code if part
+	CBE	J		!Code backend
+	CPC	J		!Code pheripheral computers
+	CMC	J		!Code main computer
+	LRED	I		!Reduction level (Dwingeloo red. code)
+	-	-(0:25)		!Reserved for Dwingeloo reduction
+	VOLUME	C6		!The volume name of the input
+	LABEL	C4		!The label or dataset name of the input
+	-	-(0:5)		!               -
+	FSYN	E		!Frequency synthesizer (Mhz)
+	LO2L	E		!Frequency local oscillator 2 for DLB (Mhz) (*)
+				!  FVERS<6: LO2
+	LO2C	E		!Frequency local oscillator 2 for DCB (Mhz) (*)
+				!  FVERS<6: LO3
+	VIDE0	E		!If to video mixing frequency (Mhz)
+	FF0	E		!Fringe stopping frequency offset (Mhz)
+	AFRATE	E		!Artificial fringe rate (Mhz) (*)
+				!  FVERS<6: reserved
+	DOFSIJ	I(0:27)		!Delay offsets in nano sec for if lines
+				!OX, OY,... to DX, DY. (*)
+				!  <04/09/80: in cm
+	PREC	D(3,3)	<D12.9>	!Precession matrix
+	NUTA	D(3,3)	<D12.9>	!Nutation matrix
+	ABER	D(3)	<D12.9>	!Aberration vector
+	VNPA	D(3)	<D12.9>	!Apparent position vector
+	DVNPA	D(3)	<D12.9>	!Differential apparent position vector (Circle/U.T.day)
+				!  FVERS<5: in S.T.
+	EQNOX	D	<D12.9>	!Equation of equinoxes
+	DEQNOX	D	<D12.9>	!Differential equation of equinoxes (Circle/U.T.day)
+				!  FVERS<5: in S.T.
+	EPS	D	<D12.9>	!True obliquity
+	DEPS	D	<D12.9>	!Nutation in obliquity
+	DPSI	D	<D12.9>	!Nutation in length
+	-	-(0:3)		!	-
+	GLAT	E	<EAF12.7> !Geocentric latitude (Circles)
+				!  ols<43: different field (never used)
+	WLAT	E	<EAF12.7> !Geographic latitude of the delay switching point
+	WLON	E	<EAF12.7> !Geographic longtitude used for the siderial clock point
+	CENTRE	E	<E12.4>	!Position of the delay switching point
+				!W.R.T. old coordinate system (= 3000)
+	PHI	E	<EAF12.7> !Rotation angle
+	FREQ	D	<D12.6>	!Fringe stopping frequency for middle observation
+	ONCLM	E	<E12.6>	!Total online clock correction for app coord moment
+	CSHAD	E(3)		!Telescope 'shadowing' coefficients
+	BL1	J		!Code broadband long term (phase)
+	BL2	J		!Code broadband long term (amplitude)
+	-	-(0:7)		!            -
+	BGS	J		!Code broadband short term
+	BGT	J		!Code telescope coefficients
+	-	-(0:7)		!	    -
+	BET	J		!Code if corrections
+	BED	J		!Code delay corrections
+	-	-(0:7)		!	    -
+	SEV	J		!Code video corrections
+	BF	J		!Code field dependent corrections
+	-	-(0:7)		!	    -
+				! GCODE...DPLE: FVERS<3: reserved
+	GCODE	I		!Main amplitude correction method (1-3)
+	-	-(0:1)		!	    -
+	GNCAL	B(0:27)		!Final ampl. correction method per IF -DLB- (Per byte)
+	TSYSI	E(0:27)	<E12.2>	!System temperatures (K)
+	RGAINI	E(0:27)	<E12.4>	!Receiver gain factors per IF
+	TNOISI	E(0:27)	<E12.2>	!Noise source temperature (K)  0X,0Y,...DY
+	JDCP	E		!Julian day for last known bih data
+	YEAR	I		!Civil year of JDCP
+	MONTH	I		!Civil month of JDCP
+	DAY	I		!Civil day of JDCP
+	-	-(0:1)		!	 -
+	CLCOFF	E		!Fixed clock offset
+	CLOCK	E		!Total online clock correction for JDCP moment
+	DCLOCK	E		!Differential clock correction
+	CUTST	D	<D12.9>	!(Length u.t.day / length s.t.day) -1
+				!  FVERS<5: reserved
+	-	-(0:11)		!	 -
+	POLEOFF	E		!Fixed declination of the baseline pole
+	POLE	E		!Total baseline pole correction for JDCP moment
+	DPLE	E		!Differential baseline pole correction
+	LO3C	E(8)		!DCB local oscillators band 1 to 8 (Mhz) (*)
+				!  FVERS<6: FB0..7
+	LO3G	E		!Average DCB local oscillator used for fringe (Mhz) (*)
+				!  FVERS<6: reserved
+	FCODE	I		!Code IF switches
+	DELTA	E(0:27)		!Real part dipole corr. factors (0X,0Y,...DY) in % (*)
+				!  ols<43: reserved
+				!  ols>46: different units
+	THETA	E(0:27)		!Imaginary part dipole corr. factors (0X,0Y,...DY) in % (*)
+				!  ols<43: reserved
+				!  ols>46: different units
+	FENRS	I(0:27)		!Front end nrs (0X,0Y,1X,...,DY) (*)
+				!  ols<57: reserved
+	-	-(0:3)		!-
+	FROFS	E		!RF frequency step size (System 49)
+	SYNF	I		!Synthesizer multiplication factor
+				!  ols<43: reserved
+	LODEL	I(0:27)		!Delay values of the lo-cables (Nsec)
+	FRO	D		!Observing freq. for IF phase zero values (Mhz)
+				!  ols<26: reserved
+	CCOR	E		!Offline clock correction (Dwingeloo use)
+	DPOLM	E		!Total baseline pole corr. for app. coord moment
+	CFREQ	E		!Offline frequency correction
+	CQI	I(0:13)		!Position corrections per tel. in Q direction
+				!(10**(-4) M)
+	CNI	I(0:13)		!Position corrections per tel. in N direction
+				!(10**(-4) M)
+	CPI	I(0:13)		!Position corrections per tel. in P direction
+				!(10**(-4) M)
+	AD0	E		!Average telescope axis difference (M)
+	CPSI	I(0:13)		!Polar axis correction per tel. (2**(-24) circles)
+	CPWI	I(0:13)		!Polar axis correction per tel. (2**(-24) circles)
+	PZIJ	I(0:27)		!If phase zero corrections for primary fringe
+				!(2**(-16) circles)
+				! C?X? FVERS<3: incorrect values
+	C2X2	E(4)		!4 coefficients for v. Vleck corr. 2x2 mode
+	C2X3	E(4)		! 	"	"	"    "    2x3  "
+	C2X4	E(4)		!	"	"	"    "    2x4  "
+	C4X3	E(4)		!	"	"	"    "    4x3  "
+	C4X4	E(4)		!	"	"	"    "    4x4  "
+	CFGJI	E(112)		!Coefficients for video band gain  corrections
+	CFFJI	E(112)		!Coefficients for video band phase corrections
+	TEMP	I		!Outside temperature (Degrees celcius)
+	BAR	I		!Air pressure (Mb)
+	HUM	I		!Humidity degree
+	-	-(0:1)		!            -
+	CMU1	E       	!Refraction coefficient dry air
+	H1	E		!Scale height dry air
+	CMU2	E     		!Refraction index water vapour
+	H2	E		!Scale height water vapour
+	CEXT	E		!Extinction coefficient
+				!  ols<43: reserved
+	RHA	E(24)		!Hour angle table (Circles)
+	CFRA	E(24)		!24 rotation angles (Circles)
+	CRIF	E(24)		!Refraction corrections (Circles)
+	-	-(0:279)	!	            -   
+	CMON	C64		!Monitoring information
+	-	-(0:19)		!	    -
+	NRPNCH	I		!Nr. of information fields in PNCHI (Max =4)
+	NRSUBT	I		!Nr. of subtracted sources (Max. is 9)
+	-	-(0:7)		!            -
+	PNCHI	C320		!General information fields
+	SRC	S:SRC(9)	!Subtracted sources
+	-	C4		!Gain/phase table name
+	TMP	J		!Table number (Code)
+	-	-(0:3)		!	 -
+				!  
+	LENTMP	I		!Nr. of records on disk necessary for this table.
+				!0 or 11 means 160 interf. (Only standard)
+				!27 means 420 interf. (Standard and non-standard)
+	-	-(0:1)		!	 -
+	PH0	E(0:159)	!	160 phase zero values, per interferometer
+				!in radians  (0XAX - 9YDY)
+	GN0	E(0:159)	!	160 gain factors, per interferometer 
+				!(0XAX - 9YDY)
+	PH10	E(0:259)	!	260 phase zero values, per interferometer
+				!in radians  (0X0X - DYDY) (Non-standard)
+	GN10	E(0:259)	!	260 gain factors, per interferometer 
+				!(0X0X - DYDY) (Non-standard)
+	-	-(0:463)	!	-
+	BCOR	S:BCOR(8)	!Band corrections
+				!  FVERS<6: reserved/not on tape
+	MOZP	S:MOZP(120)	!Mozaicking positions
+				!  FVERS<7: reserved/not on tape
+.END
+!-
diff --git a/src/nscan/shw.dsc b/src/nscan/shw.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..a4f69e8cd16a566011b7d833f76bbe333174431e
--- /dev/null
+++ b/src/nscan/shw.dsc
@@ -0,0 +1,67 @@
+!+ SHW.DSC
+!  WNB 900118
+!
+!  Revisions:
+!
+%REVISION=CMV=940414="Add historical notes"
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=WNB=930803="Change .RECORD"
+%REVISION=WNB=900118="Tape vs 7, system 59"
+!
+!	Define WSRT SH block
+!
+!
+!
+%VERSION=7					!VERSION
+%SYSTEM=59
+%USER=WNB
+%LOCAL=IFRLEN=12				!Length IFR subblock
+%%DATE
+%%NAME
+%COMMENT="SHW.DSC defines the WSRT SH block"
+!-
+.PARAMETER
+.STRUCTURE=IFR			!IFR table
+	INFNR	  I		!Interferometer number
+				!  FVERS<2: different codes
+	WTEL	  I		!West telescope indicator
+	OTEL	  I		!East telescope indicator
+	RBAS	  I		!Baseline rounded to nearest meter
+	NIH	  J		!Record # of IH block
+.END				!End IFR table
+.BEGIN=SHW
+				! (*) means use with care, not repaired
+	CBI	I		!Unequal data block flag (32767)
+	CBT	C2		!Identification: Set Header (SH)
+	NSH	J		!Record number of this record
+	LSH	J 		!Number of SH records with information
+				!  FVERS<5: always 5
+	MHLNK	J		!First record number of the next SH group
+	SDAY	I		!Local U.T. day number
+				!  FVERS<5: ST
+	STIM	I		!Start U.T. time in units of 10 sec
+				!  FVERS<5: ST
+				!  FVERS<3: units of minutes 
+	BANDNR	I		!Frequentie bandnr.
+				!  FVERS<6: set nr
+	-	I		!Empty (Delete character) (Internal use Dw'loo:SETNR)
+	BFREQ	J		!Set frequency (2**(-16) Mhz)
+				!  FVERS<2: single float (E)
+	SFREQ	I		!Spacing in frequency (DLB), bandwidth (DCB) (Mhz)
+	DATYP	C2		!Data type (IF, XX, XY, YX, or YY)
+	POLC	I		!Dipole position code
+	NRINT	I 		!Number of interferometers in the set (40,88 or 160)
+	PTS	J		!Total number of observed points in the set
+	WIDTH	E	<E12.6>	!Bandwidth (Mhz)
+				! ols<46: reserved
+	CORC0	B(0:1)		!Correctioncode: 
+				!   Bit 0 = 1 : IF phase correction applied
+				!   Bit 1 = 1 : IF gain correction applied
+				!   Zero      : IF correction not applied
+				! ols<43: reserved
+	-	-(0:109)	!	              -
+	NENT	I		!Number of entries in the index table (40,88 or 160)
+	LENT	I		!Entry length in bytes
+ 	IFR	S:IFR(0:159)	!IFR table
+.END					!END DEFINITION
+!-
diff --git a/src/nscan/sth.dsc b/src/nscan/sth.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..86f0d1922606c16d3874f86486dafdac132fd07b
--- /dev/null
+++ b/src/nscan/sth.dsc
@@ -0,0 +1,131 @@
+!+ STH.DSC
+!  WNB 900304
+!
+!  Revisions:
+!
+%REVISION=JPH=960605="Add DL, DM; RA edits PF i.s.o. AF" 
+%REVISION=JPH=941013="Split tables in X/Y parts; add many units"
+%REVISION=CMV=940420="Add IFP (no NVS necessary)"
+%REVISION=CMV=940224="Add STH_DSHFT (no NVS necessary)"
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=WNB=931130="Add ACORM"
+%REVISION=WNB=931015="Use SSH"
+%REVISION=WNB=930820="Add P: edit code"
+%REVISION=WNB=930819="Version 4: Add DIPC, new model data format"
+%REVISION=WNB=930803="Use NSTAR.DSF"
+%REVISION=WNB=920616="Add SHFT, ASHFT"
+%REVISION=WNB=920604="Change version/system to 3 for flagging, add FEXP"
+%REVISION=JPH=930224="Put comment in correct place"
+%REVISION=WNB=920828="Add VELR"
+%REVISION=WNB=920515="Add INST"
+%REVISION=WNB=910219="Make polarisation corrections correct length"
+%REVISION=WNB=900304="Original version SSH"
+!
+!	Define Set Header block
+!
+%COMMENT="STH.DSC defines the set header block"
+%COMMENT=" "
+%COMMENT="REDNS, ALGNS, OTHNS must be in this order and adjacent"
+%COMMENT=" "
+!
+%VERSION=4					!VERSION
+%SYSTEM=4
+%USER=WNB
+%%DATE
+%%NAME
+!
+! Get number of telescopes
+!
+%INCLUDE=NSTAR_DSF
+!-
+.PARAMETER
+	STHTEL	J	/NSTAR_TEL/		!# OF TELESCOPES
+	STHIFR	J	/NSTAR_TEL*(NSTAR_TEL+1)/2/ !MAX. # OF INTERFEROMETERS
+.BEGIN=STH
+%INCLUDE=SSH_DSF				! STANDARD AREA
+	BEC	I				! BACKEND CONFIGURATION
+	PTS	I				! POINTING SET #
+	VNR	J				! OBS # (=VOLG+CYCLUS*65536)
+	CHAN	I				! BAND NUMBER
+	PLN	I				! # OF POLARISATIONS
+	FIELD	C12				! FIELDNAME
+	RA	D		<DPF12.7,,"deg">! OBS RA (CIRCLES)
+	DEC	D		<DAF12.7,,"deg">! OBS DEC
+	RAE	D		<DPF12.7,,"deg">! EPOCH RA
+	DECE	D		<DAF12.7,,"deg">! EPOCH DEC
+	HAB	E		<EAF12.7,,"deg">! FIRST HA APP.
+	HAI	E		<EAF12.7,,"deg">! HA INCREMENT
+	SCN	J		<,1>		! # OF SCANS
+	OEP	E		<E12.2>		! OBS. EPOCH (E.G. 1980.12)
+	EPO	E		<E12.1>		! EPOCH (E.G. 2000.0)
+	-	E
+	FRQ	D		<D12.6,,"MHz">	! APP. FREQUENCY
+	FRQE	D		<D12.6,,"MHz">	!LSR FREQUENCY
+	BAND	E		<E12.6,,"MHz">	!BANDWIDTH (MHZ)
+	HAV	E		<EAF12.7,,"deg">	!AVERAGING HA (CIRCLES)
+	OBS	I(0:1)				!OBS. DAY/YEAR
+	RTP	E(0:NSTAR_TEL-1) <E12.4,,"m">	! TEL. POSITIONS
+	NIFR	J		<,1>		!# OF IFRS
+	IFRP	J		<XJ,1,,P:IFRT>	!POINTER TO IFR LIST
+	NFD	J		<,1>		!FD BLOCK
+	FDP	J		<XJ,1,,P:FDW>
+	NOH	J		<,1>		!LENGTH OH
+	OHP	J		<XJ,1,,P:OHW>	!POINTER TO OH
+	NSC	J		<,1>		!SC BLOCK
+	SCP	J		<XJ,1,,P:SCW>
+	NSH	J		<,1>		!SH BLOCK
+	SHP	J		<XJ,1,,P:SHW>
+	SCNP	J		<XJ,1,,P:SCH>	!POINTER TO SCAN AREA
+	SCNL	J		<,1>		!LENGTH OF SCAN
+	REDNS	E(0:1)		<E12.4,,"W.U.">	! X REDUNDANCY NOISE (G/P)
+	REDNSY	E(0:1)		<E12.4,,"W.U.">	! Y REDUNDANCY NOISE (G/P)
+	ALGNS	E(0:1)		<E12.4,,"W.U.">	! X ALIGN NOISE
+	ALGNSY	E(0:1)		<E12.4,,"W.U.">	! Y ALIGN NOISE
+	OTHNS	E(0:1)		<E12.4,,"W.U.">	! X OTHER NOISE
+	OTHNSY	E(0:1)		<E12.4,,"W.U.">	! Y OTHER NOISE
+	MDL	J(0:1)		<XJ,1,,P:MDH>	!POINTER TO MODEL LISTS
+	MDD	J(0:1)		<XJ,1,,P:MDD>	!POINTER TO MODEL DATA
+	PHI	E		<EAF12.1,,"deg">! PRECESSION ROT. ANGLE
+	POLC	E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"pos/ell: rad">
+						! X POL. CORRECTIONS
+	POLCY	E(0:1,0:NSTAR_TEL-1) <11$E10.4,,"pos/ell: rad">
+						! Y POL. CORRECTIONS
+						! (G/P=orient./ellipt., radians)
+	FRQ0	D		<D12.6,,"MHz">	! REST FREQUENCY FOR LINE
+	FRQV	D		<D12.6,,"MHz">	! REAL FREQUENCY FOR LINE
+	FRQC	D		<D12.6,,"MHz">	! CENTRE FREQUENCY FOR LINE
+	VEL	E		<E12.4,,"m/s">	!VELOCITY FOR LINE (M/S)
+	VELC	J				!VELOCITY CODE:
+						! 0= CONTINUUM
+						! 1=HELIOCENTRIC RADIO
+						! 2= LSR RADIO
+						! 3= HELIOCENTRIC OPTICAL
+						! 4= LSR OPTICAL
+	MJD	D		<D12.5>		!START MJD (DAYS)
+	UTST	D		<D12.5>		!CONVERSION UT/ST DAY LENGTH
+	INST	J				!INSTRUMENT:
+						! 0= WSRT
+						! 1= ATCA
+	VELR	E		<E12.4,,"m/s">	!VELOCITY AT REF. FREQ. (FRQC)
+	WFAC	E		<E12.4,,"1-factr">
+						! 1-FACTOR TO ABS. SCH WEIGHTS
+	SHFT	E(0:1)		<E12.4,,"arcsec"> ! DE-APPLY L-M SHIFT IN ARCSEC
+	ASHFT	E(0:1)		<E12.4,,"arcsec"> ! APPLY SHIFT (NOWHERE SET)
+	DIPC	J		<XJ>		!DIPOLE CODE: TEL # * 4 * CODE:
+						! 0     = 0 DEG (VERT) X DIPOLE
+						! 1,2,3 = 45, 90, 135 DEG
+						! STANDARD PARALLEL: 2 .........
+						! STANDARD CROSS:    2 .... 1111
+	ACORM	J				!AMPL. CORRECTION METHOD:
+						! 0 = STANDARD
+						! 1 = CORRELATION COEFF. GIVEN
+	DSHFT	E(0:1)		<E12.4,,"arcsec/day">
+						! DE-APPLY SHIFT rate
+						!  (L,M IN ARCSEC PER DAY)
+	IFHP	J		<XJ,1,,P:IFH>	!POINTER TO Tot.Power/IF area
+	IFHL	J		<,1>		!LENGTH  OF Tot.Power/IF-DATA
+	DLDM	E(0:1)		<EAR12.4,,"deg">! offsets of source in interfer-
+						!  ometric beam measurements
+	-	-(12)				!RESERVED
+.END
+!-
diff --git a/src/wng/gfh.dsc b/src/wng/gfh.dsc
new file mode 100644
index 0000000000000000000000000000000000000000..dd524909ce4abe536a75d3755e95651a01d60e33
--- /dev/null
+++ b/src/wng/gfh.dsc
@@ -0,0 +1,49 @@
+!+ GFH.DSC
+!  WNB 900131
+!
+!  Revisions:
+!
+%REVISION=WNB=931215="Add some edit formats"
+%REVISION=JPH=930903="Comments"
+%REVISION=WNB=930803="Include gfh_eqv.def"
+%REVISION=WNB=900131="Original version"
+!
+!	Define general DWARF-redundancy file header
+!
+%COMMENT="GFH.DSC defines the general file header redundancy files"
+%COMMENT=" "
+!
+%VERSION=1					!VERSION
+%SYSTEM=1
+%USER=WNB
+%%DATE
+%%NAME
+!-
+.PARAMETER
+.BEGIN=GFH
+	ID	C4	<,1>	!Type of block (e.g. .SCN)
+	LEN	J	<,1>	!Length header
+	VER	J	<,1>	!Version
+	CDAT	C11		!Creation date (dd-mmm-yyyy)
+	CTIM	C5		!Creation time (hh:mm)
+	RDAT	C11		!Revision date
+	RTIM	C5		!Revision time
+	RCNT	J		!Revison count
+	NAME	C80	<,1>	!Node name used
+	DATTP	B	<,1>	!Data type (1,2=VAX, 3=Alliant, 4=Convex)
+	-	-(0:22)		!Reserved
+	LINK	J(0:1)	<XJ,1>	!Link to data
+	  ALHD=LINK J(0:1)  <XJ,1> !absolute listhead
+	NLINK	J	<,1>	!Count linkage
+	  ALLEN=NLINK J <,1>	!absolute-list length
+	LINKG	J(0:1)	<XJ,1,,P:SGH> !Secondary link
+	  LHD=LINKG J(0:1) <XJ,1,,P:SGH> !(subgroup) listhead
+	NLINKG	J	<,1>	
+	  LLEN=NLINKG J <,1>	!(subgroup) list length
+	IDMDL	J	<,1>	!Model unique identification (not used)
+	ID1	J	<,1>	!Other id
+	ID2	J	<,1>	!Other id
+	USER	-		!Start user area
+.OFFSET=512			!Reserve with binary zeroes
+.END					!END DEFINITION
+!-
diff --git a/unit/unit__input_unit.html b/unit/unit__input_unit.html
new file mode 100644
index 0000000000000000000000000000000000000000..352985c48b2a745879c3f331afe03adc613dbce8
--- /dev/null
+++ b/unit/unit__input_unit.html
@@ -0,0 +1,32 @@
+<TITLE>Description of INPUT_UNIT (UNIT)</TITLE>
+<H1>Description of general keyword INPUT_UNIT</H1>
+
+<DT><EM>Prompt:</EM> 0, 1, 2, 3, 4, 5, 6, 7, 8, 9, D input 'tape' unit: number or 'D' for 'disk' |
+<DT><EM>Expected input:</EM> Character(1).<P>
+ Specify the input unit for your data: <P>
+	0, ..9    Tape/optical disk/DAT unit 
+	D        Disk <P>
+The correspondence between the unit numbers and the devices on your host 
+machine is defined by the environment variables MAG&lt;n&gt;. The list below shows 
+the values with which NEWSTAR is distributed, but your local installation may 
+be different, so you do wello to check with your local site manager <P>
+   classic 0.5-inch magtape: 
+	0        1600 bpi 
+	1        6250 bpi 
+	2         800 bpi <P>
+   optical disk, formatted as a magtape: 
+	4 
+	5 <P>
+   DAT, ExaByte or similar tape: 
+	6 
+	7 
+	8 
+	9 <P>
+You may enter '*' to get a list of unit numbers available for you, but this 
+will not tell you to what physical devices these correspond. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../unit/unit_comm.html">List of general keywords</A> for UNIT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/unit/unit__output_unit.html b/unit/unit__output_unit.html
new file mode 100644
index 0000000000000000000000000000000000000000..388a40827d2247dc6c6d3cfc7622ade844a1ab18
--- /dev/null
+++ b/unit/unit__output_unit.html
@@ -0,0 +1,32 @@
+<TITLE>Description of OUTPUT_UNIT (UNIT)</TITLE>
+<H1>Description of general keyword OUTPUT_UNIT</H1>
+
+<DT><EM>Prompt:</EM> output 'tape' unit: number or 'D' for 'disk' | 0, 1, 2, 3, 4, 5, 6, 7, 8, 9, D
+<DT><EM>Expected input:</EM> Character(1).<P>
+Specify the input unit for your data: <P>
+	0, ..9    Tape/optical disk/DAT unit 
+	D        Disk <P>
+The correspondence between the unit numbers and the devices on your host 
+machine is defined by the environment variables MAG&lt;n&gt;. The list below shows 
+the values with which NEWSTAR is distributed, but your local installation may 
+be different, so you do wello to check with your local site manager <P>
+   classic 0.5-inch magtape: 
+	0        1600 bpi 
+	1        6250 bpi 
+	2         800 bpi <P>
+   optical disk, formatted as a magtape: 
+	4 
+	5 <P>
+   DAT, ExaByte or similar tape: 
+	6 
+	7 
+	8 
+	9 <P>
+You may enter '*' to get a list of unit numbers available for you, but this 
+will not tell you to what physical devices these correspond. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../unit/unit_comm.html">List of general keywords</A> for UNIT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/unit/unit__output_volume.html b/unit/unit__output_volume.html
new file mode 100644
index 0000000000000000000000000000000000000000..c2c44c48bfccd70dc10cf652ed336325c957fcf3
--- /dev/null
+++ b/unit/unit__output_volume.html
@@ -0,0 +1,13 @@
+<TITLE>Description of OUTPUT_VOLUME (UNIT)</TITLE>
+<H1>Description of general keyword OUTPUT_VOLUME</H1>
+
+<DT><EM>Prompt:</EM> Output volume name
+<DT><EM>Expected input:</EM> Character(6).<P>
+Specify the full name for the output volume. <P>
+This name is used for the administration in MEDIAD <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../unit/unit_comm.html">List of general keywords</A> for UNIT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/unit/unit__overwrite.html b/unit/unit__overwrite.html
new file mode 100644
index 0000000000000000000000000000000000000000..d543920e1601cdc334eff0abfee511d6c522b58f
--- /dev/null
+++ b/unit/unit__overwrite.html
@@ -0,0 +1,14 @@
+<TITLE>Description of OVERWRITE (UNIT)</TITLE>
+<H1>Description of general keyword OVERWRITE</H1>
+
+<DT><EM>Prompt:</EM> Overwrite (YES/NO)
+<DT><EM>Default:</EM> YES /ASK.
+<DT><EM>Expected input:</EM> Logical.<P>
+Specify if one wants to overwrite the current label (YES) or not (NO). <P>
+BEWARE: All subsequent labels will also be overwritten. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../unit/unit_comm.html">List of general keywords</A> for UNIT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/unit/unit__unit.html b/unit/unit__unit.html
new file mode 100644
index 0000000000000000000000000000000000000000..46d602289a0e9e24221cff38a5539f31c6cb33f6
--- /dev/null
+++ b/unit/unit__unit.html
@@ -0,0 +1,32 @@
+<TITLE>Description of UNIT (UNIT)</TITLE>
+<H1>Description of general keyword UNIT</H1>
+
+<DT><EM>Prompt:</EM> 0, 1, 2, 3, 4, 5, 6, 7, 8, 9, D 'tape' unit: number or 'D' for 'disk' |
+<DT><EM>Expected input:</EM> Character(1).<P>
+ Specify the input unit for your data: <P>
+	0, ..9    Tape/optical disk/DAT unit 
+	D        Disk <P>
+The correspondence between the unit numbers and the devices on your host 
+machine is defined by the environment variables MAG&lt;n&gt;. The list below shows 
+the values with which NEWSTAR is distributed, but your local installation may 
+be different, so you do well to check with your local site manager <P>
+   classic 0.5-inch magtape: 
+	0        1600 bpi 
+	1        6250 bpi 
+	2         800 bpi <P>
+   optical disk, formatted as a magtape: 
+	4 
+	5 <P>
+   DAT, ExaByte or similar tape: 
+	6 
+	7 
+	8 
+	9 <P>
+You may enter '*' to get a list of unit numbers available for you, but this 
+will not tell you to what physical devices these correspond. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../unit/unit_comm.html">List of general keywords</A> for UNIT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/unit/unit__volume_type.html b/unit/unit__volume_type.html
new file mode 100644
index 0000000000000000000000000000000000000000..3f3ea7c43ae16d783abfb305c5e3b305c3cc4549
--- /dev/null
+++ b/unit/unit__volume_type.html
@@ -0,0 +1,18 @@
+<TITLE>Description of VOLUME_TYPE (UNIT)</TITLE>
+<H1>Description of general keyword VOLUME_TYPE</H1>
+
+<DT><EM>Prompt:</EM> Abbreviated medium type
+<DT><EM>Expected input:</EM> Character(4).<P>
+Specify the type for the output volume. <P>
+This name is used for the administration in MEDIAD <P>
+<DT><STRONG>	DOD</STRONG> - DEC Optical Disk 
+<DT><STRONG>	DAT</STRONG> - Digital Audio Tape 
+<DT><STRONG>	800</STRONG> - 9-track tape,  800 bpi 
+<DT><STRONG>	1600</STRONG> - 9-track tape, 1600 bpi 
+<DT><STRONG>	6250</STRONG> - 9-track tape, 6250 bpi <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../unit/unit_comm.html">List of general keywords</A> for UNIT
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/unit_comm/unit_comm.html b/unit_comm/unit_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..ba015208d77543204868552748a3d5c6169070b1
--- /dev/null
+++ b/unit_comm/unit_comm.html
@@ -0,0 +1,29 @@
+<TITLE>Index of general keywords from UNIT</TITLE>
+<H1>Description of general keywords (UNIT)</H1>
+
+<UL>
+<LI> <A HREF="../unit/unit__unit.html">
+  UNIT</A>
+  0, 1, 2, 3, 4, 5, 6, 7, 8, 9, D 'tape' unit: number or 'D' for 'disk' |
+<LI> <A HREF="../unit/unit__input_unit.html">
+  INPUT_UNIT</A>
+  0, 1, 2, 3, 4, 5, 6, 7, 8, 9, D input 'tape' unit: number or 'D' for 'disk' |
+<LI> <A HREF="../unit/unit__output_unit.html">
+  OUTPUT_UNIT</A>
+  output 'tape' unit: number or 'D' for 'disk' | 0, 1, 2, 3, 4, 5, 6, 7, 8, 9, D
+<LI> <A HREF="../unit/unit__output_volume.html">
+  OUTPUT_VOLUME</A>
+  Output volume name
+<LI> <A HREF="../unit/unit__volume_type.html">
+  VOLUME_TYPE</A>
+  Abbreviated medium type
+<LI> <A HREF="../unit/unit__overwrite.html">
+  OVERWRITE</A>
+  Overwrite (YES/NO)
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
diff --git a/unit_public_intfc.ps b/unit_public_intfc.ps
new file mode 100644
index 0000000000000000000000000000000000000000..1f34334b128a4ade591ed3b1fa4dd2ec7df85b17
--- /dev/null
+++ b/unit_public_intfc.ps
@@ -0,0 +1,611 @@
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+%%Pages: 3
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+%%EndComments
+%DVIPSCommandLine: dvips -o /newstar/master/hlp/unit_public_intfc.ps
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+
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+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group UNIT</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=unit_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=unit_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=unit_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=unit_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=unit_public_intfc.html#SECTION0003200000000000000>  <b>Parameter INPUT_UNIT</b></A>
+<LI> <A NAME=tex2html6 HREF=unit_public_intfc.html#SECTION0003300000000000000>  <b>Parameter OUTPUT_UNIT</b></A>
+<LI> <A NAME=tex2html7 HREF=unit_public_intfc.html#SECTION0003400000000000000>  <b>Parameter OUTPUT_VOLUME</b></A>
+<LI> <A NAME=tex2html8 HREF=unit_public_intfc.html#SECTION0003500000000000000>  <b>Parameter OVERWRITE</b></A>
+<LI> <A NAME=tex2html9 HREF=unit_public_intfc.html#SECTION0003600000000000000>  <b>Parameter UNIT</b></A>
+<LI> <A NAME=tex2html10 HREF=unit_public_intfc.html#SECTION0003700000000000000>  <b>Parameter VOLUME_TYPE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group UNIT, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.input.unit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter INPUT_UNIT</b></A></H2>
+<P>
+  <em>Prompt:</em> input 'tape' unit: number or 'D' for 'disk' | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *1:  1 value
+<P>
+    <PRE>
+        Specify the input unit for your data:
+</PRE>
+<P>
+  <PRE>
+        0,..9    Tape/optical disk/DAT unit
+        D        Disk
+</PRE>
+<P>
+  <PRE>
+The correspondence between the unit numbers and the devices on your host
+machine is defined by the environment variables MAG<n>. The list below shows
+the values with which NEWSTAR is distributed, but your local installation may
+be different, so you do wello to check with your local site manager
+</PRE>
+<P>
+  <PRE>
+   classic 0.5-inch magtape:
+        0        1600 bpi
+        1        6250 bpi
+        2         800 bpi
+</PRE>
+<P>
+  <PRE>
+   optical disk, formatted as a magtape:
+        4
+        5
+</PRE>
+<P>
+  <PRE>
+   DAT, ExaByte or similar tape:
+        6
+        7
+        8
+        9
+</PRE>
+<P>
+  <PRE>
+You may enter '*' to get a list of unit numbers available for you, but this
+will not tell you to what physical devices these correspond.
+</PRE>
+<P>
+<A NAME=.output.unit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter OUTPUT_UNIT</b></A></H2>
+<P>
+<em>Prompt:</em> output 'tape' unit: number or 'D' for 'disk' | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *1:  1 value
+<P>
+  <PRE>
+Specify the input unit for your data:
+</PRE>
+<P>
+  <PRE>
+        0,..9    Tape/optical disk/DAT unit
+        D        Disk
+</PRE>
+<P>
+  <PRE>
+The correspondence between the unit numbers and the devices on your host
+machine is defined by the environment variables MAG<n>. The list below shows
+the values with which NEWSTAR is distributed, but your local installation may
+be different, so you do wello to check with your local site manager
+</PRE>
+<P>
+  <PRE>
+   classic 0.5-inch magtape:
+        0        1600 bpi
+        1        6250 bpi
+        2         800 bpi
+</PRE>
+<P>
+  <PRE>
+   optical disk, formatted as a magtape:
+        4
+        5
+</PRE>
+<P>
+  <PRE>
+   DAT, ExaByte or similar tape:
+        6
+        7
+        8
+        9
+</PRE>
+<P>
+  <PRE>
+You may enter '*' to get a list of unit numbers available for you, but this
+will not tell you to what physical devices these correspond.
+</PRE>
+<P>
+<A NAME=.output.volume><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter OUTPUT_VOLUME</b></A></H2>
+<P>
+<em>Prompt:</em> Output volume name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *6:  1 value
+<P>
+  <PRE>
+Specify the full name for the output volume.
+</PRE>
+<P>
+  <PRE>
+This name is used for the administration in MEDIAD
+</PRE>
+<P>
+<A NAME=.overwrite><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter OVERWRITE</b></A></H2>
+<P>
+<em>Prompt:</em> Overwrite (YES/NO) (<em>may vary per application</em>)<BR><em>Expected input:</em> Yes/No:  1 value
+<P>
+  <PRE>
+Specify if one wants to overwrite the current label (YES) or not (NO).
+</PRE>
+<P>
+  <PRE>
+BEWARE: All subsequent labels will also be overwritten.
+</PRE>
+<P>
+<A NAME=.unit><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter UNIT</b></A></H2>
+<P>
+<em>Prompt:</em> 'tape' unit: number or 'D' for 'disk' | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *1:  1 value
+<P>
+  <PRE>
+        Specify the input unit for your data:
+</PRE>
+<P>
+  <PRE>
+        0,..9    Tape/optical disk/DAT unit
+        D        Disk
+</PRE>
+<P>
+  <PRE>
+The correspondence between the unit numbers and the devices on your host
+machine is defined by the environment variables MAG<n>. The list below shows
+the values with which NEWSTAR is distributed, but your local installation may
+be different, so you do well to check with your local site manager
+</PRE>
+<P>
+  <PRE>
+   classic 0.5-inch magtape:
+        0        1600 bpi
+        1        6250 bpi
+        2         800 bpi
+</PRE>
+<P>
+  <PRE>
+   optical disk, formatted as a magtape:
+        4
+        5
+</PRE>
+<P>
+  <PRE>
+   DAT, ExaByte or similar tape:
+        6
+        7
+        8
+        9
+</PRE>
+<P>
+  <PRE>
+You may enter '*' to get a list of unit numbers available for you, but this
+will not tell you to what physical devices these correspond.
+</PRE>
+<P>
+<A NAME=.volume.type><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter VOLUME_TYPE</b></A></H2>
+<P>
+<em>Prompt:</em> Abbreviated medium type (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *4:  1 value
+<P>
+  <PRE>
+Specify the type for the output volume.
+</PRE>
+<P>
+  <PRE>
+This name is used for the administration in MEDIAD
+</PRE>
+<P>
+  <PRE>
+        DOD     - DEC Optical Disk
+        DAT     - Digital Audio Tape
+        800     - 9-track tape,  800 bpi
+        1600    - 9-track tape, 1600 bpi
+        6250    - 9-track tape, 6250 bpi
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/wmp_descr.ps b/wmp_descr.ps
new file mode 100644
index 0000000000000000000000000000000000000000..50d812f66d0d82721215a0c23961dca40f909204
--- /dev/null
+++ b/wmp_descr.ps
@@ -0,0 +1,716 @@
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+ 0x33,0x63,0x62,0x26,0x30,0xdb,0xe6,0x09,0x30,0x26,0xb3,0x19,0x00,0x00,0x00,
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+ 0xfd,0x23,0xa6,0xdf,0x64,0xf8,0x81,0x89,0xc9,0xcc,0x8c,0x7e,0x03,0xec,0x31,
+ 0x63,0x62,0x26,0xf0,0xf3,0x86,0x09,0x30,0x36,0xa3,0x1f,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x23,
+ 0x06,0x00,0xc0,0xe4,0x0f,0x23,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x0f,
+ 0x23,0xa6,0xc1,0x64,0x18,0x80,0x89,0xc9,0xcc,0x8c,0x06,0x03,0xf8,0x31,0x6b,
+ 0x62,0x26,0x30,0xd8,0x86,0x09,0xb0,0x1c,0xa3,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x32,0x06,
+ 0x00,0xc0,0x24,0x8e,0x33,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x8e,0x33,
+ 0xb6,0xd1,0x64,0x1c,0x81,0x89,0xcd,0xcc,0xcc,0x46,0x03,0xd8,0x31,0x6b,0x62,
+ 0x26,0x30,0xce,0xc7,0x09,0xb0,0x1c,0xb3,0x11,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x36,0x06,0x00,
+ 0xe0,0xef,0x7b,0x3e,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0xe0,0x7b,0x3e,0x7e,
+ 0xef,0xcf,0xf3,0xc0,0x9f,0xff,0xff,0x7d,0xbc,0x07,0x98,0x78,0xff,0xf7,0x7f,
+ 0xe0,0xf9,0xfd,0x1f,0xf0,0x08,0x1f,0x0f,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x1c,0x02,0x00,0x00,
+ 0x00,0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x08,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,
+ 0x00,0x20,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x20,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x0f,0x03,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x03,0x00,0x00,0x00,0x00,
+ 0x70,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x70,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x87,0x07,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x80,0x01,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00};
diff --git a/wmp_descr/_13339_tex2html_wrap278.png b/wmp_descr/_13339_tex2html_wrap278.png
new file mode 100644
index 0000000000000000000000000000000000000000..2b5cb676792d18daf8d9863d4ed0eb99f5ab1183
Binary files /dev/null and b/wmp_descr/_13339_tex2html_wrap278.png differ
diff --git a/wmp_descr/_13339_tex2html_wrap278.xbm b/wmp_descr/_13339_tex2html_wrap278.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..201ffa9763aa9e7f4ab4aefe523c152224ea16eb
--- /dev/null
+++ b/wmp_descr/_13339_tex2html_wrap278.xbm
@@ -0,0 +1,4 @@
+#define noname_width 5
+#define noname_height 7
+static char noname_bits[] = {
+ 0x04,0x04,0x1f,0x0e,0x1f,0x15,0x04};
diff --git a/wmp_descr/images.pl b/wmp_descr/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..28e73384a11925d8c2d5739d0241caee915f85a9
--- /dev/null
+++ b/wmp_descr/images.pl
@@ -0,0 +1,9 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{tabular}<<113>>lll<<113>>1);html_special_mark_amp;group;html_special_mark_amp;spareindex2);html_special_mark_amp;field;html_special_mark_amp;pointingcentre(mosaicing)3);html_special_mark_amp;channel;html_special_mark_amp;frequencychannel,orDCBband4);html_special_mark_amp;polarisation;html_special_mark_amp;0=IorXX,1=QorXY,2=UorYX,3=VorYY5);html_special_mark_amp;type;html_special_mark_amp;0=map,1=ap,2=cov,3=real,4=imag,5=ampl,6=phase6);html_special_mark_amp;nseq;html_special_mark_amp;sequencenumberwithineachtype{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_13339_tabular112.xbm">'; 
+$key = q/{}$ast${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_13339_tex2html_wrap278.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/wmp_descr/labels.pl b/wmp_descr/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..2aa6171377c568d229f2e046dd7dc096265a3a11
--- /dev/null
+++ b/wmp_descr/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".file.layout"} ="$URL/wmp_descr.html"; 
+$external_labels{".header.items"} ="$URL/wmp_descr.html"; 
+$external_labels{".map.header"} ="$URL/wmp_descr.html"; 
+$external_labels{".data"} ="$URL/wmp_descr.html"; 
+$external_labels{".contents"} ="$URL/wmp_descr.html"; 
+$external_labels{".organ"} ="$URL/wmp_descr.html"; 
+
+1;
\ No newline at end of file
diff --git a/wmp_descr/wmp_descr.html b/wmp_descr/wmp_descr.html
new file mode 100644
index 0000000000000000000000000000000000000000..7c73e48f7bf6d950144ec8a8d0becb99cf104078
--- /dev/null
+++ b/wmp_descr/wmp_descr.html
@@ -0,0 +1,213 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>The WMP-file (image data)</b>  
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=wmp_descr.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=wmp_descr.html#SECTION0002000000000000000> <b>Organisation of the WMP file: Maps</b></A>
+<LI> <A NAME=tex2html3 HREF=wmp_descr.html#SECTION0003000000000000000> <b>File layout and file header</b></A>
+<LI> <A NAME=tex2html4 HREF=wmp_descr.html#SECTION0004000000000000000> <b>The Map header</b></A>
+<UL> 
+<LI> <A NAME=tex2html5 HREF=wmp_descr.html#SECTION0004100000000000000> <b>Explanation of items in the Map header</b></A>
+</UL> 
+<LI> <A NAME=tex2html6 HREF=wmp_descr.html#SECTION0005000000000000000> <b>The Map data</b></A>
+</UL>
+<A NAME=.organ><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0002000000000000000> <b>Organisation of the WMP file: Maps</b></A></H1>
+<P>
+        The <i>NEWSTAR </i> WMP file contains `image data', i.e.  a collection of 2-dimensional arrays of data.  The various `images' in a WMP file <i>are related in some way</i>, but do not have to have the same dimensions.  Examples are radio maps at various frequencies (line observations), polarisations, or pointing directions (mosaicking).  There may also be antenna patterns and various kinds of residual maps, or even rectangular arrays ov uv-data.
+<P>
+The basic unit in the WMP file is the Map (a 2-dimensional array of pixel values). It can be selected by the user by means of 6 integer indices:  
+<BR><BR><P><IMG ALIGN=BOTTOM ALT="" SRC="_13339_tabular112.png"><P>  
+<BR><BR>Indices may also be ranges of indices, or wildcards (<IMG ALIGN=BOTTOM ALT="" SRC="_13339_tex2html_wrap278.png">), as explained in more detail in the section `Overview of <i>NEWSTAR </i> files' in this Cookbook.  Note that the Map in the WMP-file plays the same role as the Set in the  SCN-file.
+<P>
+        All indices are just running numbers (<b>starting at 0!</b>), except `type' and `polarisation', which have fixed codes (see above).
+<P>
+        Neither the `field' nor the `channel' index nrs correspond with the `field' or `channel' nrs in the SCN-file.  The reason for this is that a map may be made from a <em>combination</em> of fields or channels.
+<P>
+        Usually, all Maps belong to the same `group' (0).  Therefore, the first index is called a `spare index' here.  However, any selection of Maps may be put into a new group in the same WMP file, using the NMAP option REGROUP.
+<P>
+        The 6th index allows for a sequence of Maps of a certain type, usually derived from each other.  Examples are residual Maps after  
+<A HREF="../nclean_descr/nclean_descr.html">CLEANing</A>, or the Maps that result from  
+<A HREF="../nmap_descr/nmap_descr.html#.fiddle">combining other Maps</A>.
+<P>
+<A NAME=.file.layout><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0003000000000000000> <b>File layout and file header</b></A></H1>
+<P>
+        A summary of the WMP-file contents and layout may be obtained by using the program NMAP, option SHOW:
+<P>
+****** Put new script here ******
+<P>
+This particular WMP-file actually contains the following (rather strange) collection of Maps:
+<P>
+		<BR><tt>g.f.c.p.t.n (#abs)</tt>
+<P>
+		<i>group.field.chan.pol.type.nseq</i>
+<P>
+		<BR><tt>0.0.0.0.2.0(#0) type COVE </tt>
+<P>
+		<i>uv-coverage for XY-map</i>
+<P>
+		<BR><tt>0.0.0.0.6.0(#1) type PHAS </tt>
+<P>
+		<i>map of XY phases</i>
+<P>
+		<BR><tt>0.0.0.0.0.0(#2) type MAP </tt>
+<P>
+		<i>XY-map</i>
+<P>
+		<BR><tt>0.0.0.0.1.0(#3) type AP </tt>
+<P>
+		<i>antenna pattern for XY-map</i>
+<P>
+		<BR><tt>0.0.0.1.6.0(#4) type PHAS </tt>
+<P>
+		<i>map of Q phases</i>
+<P>
+		<BR><tt>0.0.0.1.0.0(#5) type MAP </tt>
+<P>
+		<i>Q-map</i>
+<P>
+		<BR><tt>0.0.0.2.6.0(#6) type PHAS </tt>
+<P>
+		<i>map of V phases</i>
+<P>
+		<BR><tt>0.0.0.2.0.0(#7) type MAP </tt>
+<P>
+		<i>V-map</i>
+<P>
+		<BR><tt>0.0.0.3.6.0(#8) type PHAS </tt>
+<P>
+		<i>map of iV phases</i>
+<P>
+		<BR><tt>0.0.0.3.0.0(#9) type MAP </tt>
+<P>
+		<i>iV-map</i>
+<P>
+The 10 `datasets' (Maps) in this WMP-file belong to 1 `group' (1st index, =0).  The number in parentheses indicates the <em>absolute Map nr</em> within the file.
+<P>
+Note that the number of polarisations is not really 4, and that the number of types is not really 7.  Indicated are the highest index values present, plus one.
+<P>
+The WMP file header only contains book-keeping information that allows the program to find its way around:
+<P>
+****** Put new script here *****
+<P>
+<A NAME=.map.header><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0004000000000000000> <b>The Map header</b></A></H1>
+<P>
+Each Map in a WMP file contains a header with information, which can be inspected with the program <A HREF="../nmap_descr/nmap_descr.html#.show">NMAP, option SHOW</A>:
+<P>
+****** Put new script here *****
+<P>
+<A NAME=.header.items><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H2><A NAME=SECTION0004100000000000000> <b>Explanation of items in the Map header</b></A></H2>
+<P>
+<UL><LI>  LINK: Link (pointer) to other Maps  
+<LI>  LEN: Length of header block (bytes?)  
+<LI>  VER: Version nr of the header  
+<LI>  SETN: Abs Map (Set) nr, i.e. the one needed for direct reference  
+        (e.g. #setn)  
+<LI>  FNM: Field (pointing centre) name  
+<LI>  EPO: Epoch (e.g. 1950.0)  
+<LI>  RA: RA of field centre (degr)  
+<LI>  DEC: DEC of field centre (degr)  
+<LI>  FRQ: Central frequency (MHz)  
+<LI>  BDW: Bandwidth (MHz)  
+<LI>  RAO, DECO, FRQO: Observed RA (degr), DEC (degr), freq (MHz)  
+<LI>  ODY, OYR: Observed day (since January 0th) and year (since 1900)  
+<LI>  DCD: Data code (2=I, 4=J, 5=E, 8=D)  
+<LI>  PCD: Program code (0=NMAP)  
+<LI>  SRA, SDEC, SFRQ: Separation in RA (degr), DEC (degr) and freq (MHz)  
+<LI>  NRA, NDEC, NFRQ: Nr of points in RA, DEC and frequ  
+<LI>  ZRA, ZDEC, ZFRQ: Centre RA (1st point=0), DEC (1st line=0), frequ (1st map=0)  
+<LI>  MXR, MXD, MXF: Position max in RA, DEC, frequ  
+<LI>  MNR, MND, MNF: Position min in RA, DEC, frequ  
+<LI>  MAX, MIN: Max, min map value  
+<LI>  SHR, SHD, SHF: Shift in RA, DEC (add, degr?) or frequ (add, MHz)  
+<LI>  SUM: Normalising sum  
+<LI>  UNI: Multiplier to get Jy  
+<LI>  UCM: User comment  
+<LI>  NPT: Nr of input uv-data points  
+<LI>  TYP: Map type (MAP, AP, COV, PHAS etc)  
+<LI>  POL: Polarisation type (I,Q,U,V or XX,XY,YX,YY)  
+<LI>  CD: Codes (array of 8 integer switches, 0-7):  
+        taper type (0), convolution type (1),  
+        correct for convolution (2), clipping done (3),  
+        source subtraction (4), data type (5),  
+        uv coordinate type (6), de-beam count (7)  
+<LI>  EPT: Map epoch used (0=apparent, 1=as specified in EPO above)  
+<LI>  OEP: Observation epoch (e.g. 1985.78)  
+<LI>  NOS: Map rms noise (W.U.)  
+<LI>  FRA, FDEC, FFRQ: Field size in RA (degr), DEC (degr), frequ (MHz)  
+<LI>  TEL: Telescope name (e.g. WSRT)  
+<LI>  FSR, FSD: FFT size RA, DEC  
+<LI>  MDP: Map data pointer  
+<LI>  NBL: Nr of baselines that have contributed to the Map  
+<LI>  NST: Nr of uv-data sets that have contributed to the Map  
+<LI>  VEL: Velocity (m/s)  
+<LI>  VELC: Velocity code (0=continuum, 1=heliocentric radio, 2=LSR radio,  
+        3=heliocentric optical, 4=LSR optical)  
+<LI>  VELR: Velocity at reference frequ (FRQC)  
+<LI>  INST: Instrument code (0=WSRT, 1=ATCA)  
+<LI>  FRQ0, FRQV, FRQC: Rest, Real and Centre frequency for line (MHz)  
+</UL>
+<P>
+<A NAME=.data><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0005000000000000000> <b>The Map data</b></A></H1>
+<P>
+        The actual data in a Map can be displayed on the X-screen as a color map by using the program NGIDS, or as a contour or gray-scale plot with the program NPLOT.  However, its is also possible to inspect small areas of a WMP Map, or its statistics, with the program NMAP, option  SHOW:
+<P>
+****** Put new script here *****
+<P>
+Note that the `noise' option gives the rms of the pixel values in the selected area(s), while the `offset' option gives the rms with respect to their average value (offset). A histogram of pixel values is printed in the log-file (NMAP.LOG).
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/wmpnode/wmpnode__output_wmp_node.html b/wmpnode/wmpnode__output_wmp_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..84acb0bf0616d5e3e5a3ad54d41feea2d294b25d
--- /dev/null
+++ b/wmpnode/wmpnode__output_wmp_node.html
@@ -0,0 +1,15 @@
+<TITLE>Description of OUTPUT_WMP_NODE (WMPNODE)</TITLE>
+<H1>Description of general keyword OUTPUT_WMP_NODE</H1>
+
+<DT><EM>Prompt:</EM> Output .WMP file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (no extension). <P>
+You may enter '[&lt;directory&gt;/]**' to get a list of .WMP files in your current or 
+another directory; then enter '#&lt;n&gt;' to select the &lt;n&gt;th file from that list. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../wmpnode/wmpnode_comm.html">List of general keywords</A> for WMPNODE
+<LI>Description of the <A HREF="../wmp_descr/wmp_descr.html">WMP file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/wmpnode/wmpnode__wmp_node.html b/wmpnode/wmpnode__wmp_node.html
new file mode 100644
index 0000000000000000000000000000000000000000..ca0bb79ba967169a90ea53a447d55e78846501d1
--- /dev/null
+++ b/wmpnode/wmpnode__wmp_node.html
@@ -0,0 +1,29 @@
+<TITLE>Description of WMP_NODE (WMPNODE)</TITLE>
+<H1>Description of general keyword WMP_NODE</H1>
+
+<DT><EM>Prompt:</EM> .WMP file name
+<DT><EM>Expected input:</EM> Character(80).<P>
+Specify the file name (no extension). <P>
+You may enter '[&lt;directory&gt;/]**' to get a list of .WMP files in your current or 
+another directory; then enter '#&lt;n&gt;' to select the &lt;n&gt;th file from that list. 
+"! 
+!---------------------------------------------------------------------------- 
+!       Ref: 
+! 
+KEYWORD=INPUT_WMP_NODE 
+	DATA_TYP=C 
+	IO=I 
+	LENGTH=80 
+	SWITCHES=LOOP, NULL_VALUES, WILD_CARDS 
+	SEARCH=L, P 
+	PROMPT="Input .WMP file name  
+Specify the file name (no extension). <P>
+You may enter '[&lt;directory&gt;/]**' to get a list of .WMP files in your current or 
+another directory; then enter '#&lt;n&gt;' to select the &lt;n&gt;th file from that list. 
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../wmpnode/wmpnode_comm.html">List of general keywords</A> for WMPNODE
+<LI>Description of the <A HREF="../wmp_descr/wmp_descr.html">WMP file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/wmpnode_comm/wmpnode_comm.html b/wmpnode_comm/wmpnode_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..1eb6124cc22350d1488cc5b9914e23928dbe52d9
--- /dev/null
+++ b/wmpnode_comm/wmpnode_comm.html
@@ -0,0 +1,17 @@
+<TITLE>Index of general keywords from WMPNODE</TITLE>
+<H1>Description of general keywords (WMPNODE)</H1>
+
+<UL>
+<LI> <A HREF="../wmpnode/wmpnode__wmp_node.html">
+  WMP_NODE</A>
+  .WMP file name
+<LI> <A HREF="../wmpnode/wmpnode__output_wmp_node.html">
+  OUTPUT_WMP_NODE</A>
+  Output .WMP file name
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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diff --git a/wmpnode_public_intfc/images.pl b/wmpnode_public_intfc/images.pl
new file mode 100644
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--- /dev/null
+++ b/wmpnode_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/wmpnode_public_intfc/labels.pl b/wmpnode_public_intfc/labels.pl
new file mode 100644
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--- /dev/null
+++ b/wmpnode_public_intfc/labels.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".wmp.node"} ="$URL/wmpnode_public_intfc.html"; 
+$external_labels{".public"} ="$URL/wmpnode_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/wmpnode_public_intfc.html"; 
+$external_labels{".input.wmp.node"} ="$URL/wmpnode_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/wmpnode_public_intfc.html"; 
+$external_labels{".output.wmp.node"} ="$URL/wmpnode_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/wmpnode_public_intfc/wmpnode_public_intfc.html b/wmpnode_public_intfc/wmpnode_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..dc1e6b88996f133ff278cad403fd9f921d0fd4c1
--- /dev/null
+++ b/wmpnode_public_intfc/wmpnode_public_intfc.html
@@ -0,0 +1,122 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group WMPNODE</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=wmpnode_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=wmpnode_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=wmpnode_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=wmpnode_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=wmpnode_public_intfc.html#SECTION0003200000000000000>  <b>Parameter INPUT_WMP_NODE</b></A>
+<LI> <A NAME=tex2html6 HREF=wmpnode_public_intfc.html#SECTION0003300000000000000>  <b>Parameter OUTPUT_WMP_NODE</b></A>
+<LI> <A NAME=tex2html7 HREF=wmpnode_public_intfc.html#SECTION0003400000000000000>  <b>Parameter WMP_NODE</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group WMPNODE, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.input.wmp.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter INPUT_WMP_NODE</b></A></H2>
+<P>
+  <em>Prompt:</em> Input .WMP file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+    <PRE>
+Specify the file name (no extension).
+</PRE>
+<P>
+  <PRE>
+You may enter '[<directory>/]**' to get a list of .WMP files in your current or
+another directory; then enter '#<n>' to select the <n>th file from that list.
+</PRE>
+<P>
+<A NAME=.output.wmp.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter OUTPUT_WMP_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> Output .WMP file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the file name (no extension).
+</PRE>
+<P>
+  <PRE>
+You may enter '[<directory>/]**' to get a list of .WMP files in your current or
+another directory; then enter '#<n>' to select the <n>th file from that list.
+</PRE>
+<P>
+<A NAME=.wmp.node><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter WMP_NODE</b></A></H2>
+<P>
+<em>Prompt:</em> .WMP file name (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *80:  1 value
+<P>
+  <PRE>
+Specify the file name (no extension).
+</PRE>
+<P>
+  <PRE>
+You may enter '[<directory>/]**' to get a list of .WMP files in your current or
+another directory; then enter '#<n>' to select the <n>th file from that list.
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/wmpsets/wmpsets__wmp_sets.html b/wmpsets/wmpsets__wmp_sets.html
new file mode 100644
index 0000000000000000000000000000000000000000..afb74abcce9baab7238dde0cf995293cf2ececfd
--- /dev/null
+++ b/wmpsets/wmpsets__wmp_sets.html
@@ -0,0 +1,57 @@
+<TITLE>Description of WMP_SETS (WMPSETS)</TITLE>
+<H1>Description of general keyword WMP_SETS</H1>
+
+<DT><EM>Prompt:</EM> Images to process:  grp.fld.chn.pol.typ.seq |
+<DT><EM>Expected input:</EM> Character(32), 64 values.<P>
+	A NEWSTAR .WMP file contains maps and antenna patterns for one or more 
+objects. The basic unit of data is the two-dimensional IMAGE representing 
+either a MAP of a piece of sky or the synthesised ANTENNA PATTERN. Images are 
+addressed through an IMAGE INDEX which is a string of six integers separated by 
+dots: <P>
+			grp.fld.chn.pol.typ.seq <P>
+   A GROUP is basically an administrative unit, allowing the user to subdivide 
+    his data, e.g. per object. <P>
+   The FIELD and CHANNEL are the field and channel numbers of the observation(s) 
+    in the .SCN file from which the image was made. These numbers are defined by 
+    the way the observation was made and should be indentical for 
+    all observations involved (which could, e.g., be several 12-hour mosaic 
+    observations with different baseline sets.). <P>
+   POL is a code indicating the polarisation. The code distinguishes the 
+    four components of a full polarisation represntation: <P>
+		0, 1, 2, 3 =  XX.XY.YX.YY or 
+		0, 1, 2, 3 =  I, Q, U, V <P>
+    but it is your responsibility to remember which of the two representations 
+    applies. <P>
+   TYP codes the type of image: 0 for a map, 1 for an antenna pattern. <P>
+   The image SEQ uence number distinguishes images for which all five of 
+    the preceding indices are identical. It is used in particular to distinguish 
+    residual maps in a CLEAN sequence. It is your responsibility to know what 
+    the different SEQ values represent. <P>
+Index values start at zero. (Remember that for the CHN index 0 is the continuum 
+channel.) <P>
+You may select SETS of images for processing through [ranges of] values for the 
+five indices, e.g. <P>
+		2.3-5:2.*.1-7.* <P>
+The WILDCARD value '*' means 'all'. Each index may also be specified as a 
+RANGE: &lt;first&gt;-&lt;last&gt;[&lt;:increment&gt;]. Indices omitted are assumed to be '*',  
+i.e.  ....1.0  means *.*.*.*.1.0. For wildcards at the end the dots may also be 
+omitted, i.e. 1.0 means 1.0.*.*.*.* <P>
+The notation 3-5:2 stands for 'from 3 through 5 in steps of 2'. The step must 
+be positive; if it is omitted, it is taken to be 1 (as in '1-7' above). <P>
+Multiple image SETS may be specified, separated by comma's: &lt;Set1&gt;, &lt;Set2&gt;, ... 
+The associated WMP_LOOPS keyword allows even more looping over index values. <P>
+IF YOU WANT TO BE REMINDED OF WHAT IMAGES ARE IN YOUR FILE: 
+	Type O or L in response to this prompt to get an Overview or Layout 
+	of your .WMP file. <P>
+IF YOU DO NOT YET FEEL COMFORTABLE WITH THESE CONCEPTS MORE HELP IS PROVIDED: 
+	Type '@' or '&gt;' to be prompted for each of the 6 indices separately,  
+	with more specific explanation per index. <P>
+IF YOU GET BORED WITH 6-NUMBER INDICES: 
+	Absolute Cut nrs '#&lt;n&gt;' can be used as an alternative. <P>
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../wmpsets/wmpsets_comm.html">List of general keywords</A> for WMPSETS
+<LI>Description of the <A HREF="../wmp_descr/wmp_descr.html">WMP file format</A>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI>The <A HREF="../common_descr/common_descr.html">DWARF User Interface</A>
+</UL>
diff --git a/wmpsets_comm/wmpsets_comm.html b/wmpsets_comm/wmpsets_comm.html
new file mode 100644
index 0000000000000000000000000000000000000000..e779c06f09140b345c676761a7b808b0616db165
--- /dev/null
+++ b/wmpsets_comm/wmpsets_comm.html
@@ -0,0 +1,36 @@
+<TITLE>Index of general keywords from WMPSETS</TITLE>
+<H1>Description of general keywords (WMPSETS)</H1>
+
+<UL>
+<LI> <A HREF="../wmpsets/wmpsets__wmp_sets.html">
+  WMP_SETS</A>
+  Images to process:  grp.fld.chn.pol.typ.seq |
+<LI> <A HREF="../wmpsets/wmpsets__can be used as an alternative..html">
+  can be used as an alternative.</A>
+  Loop specifications: |-
+nr of cycles, index increment (grp.fld.chn.pol.typ.seq) per cycle |
+<LI> <A HREF="../wmpsets/wmpsets__wmp_groups.html">
+  WMP_GROUPS</A>
+  1st index: grp = groups
+<LI> <A HREF="../wmpsets/wmpsets__wmp_fields.html">
+  WMP_FIELDS</A>
+  2nd index: field(s)
+<LI> <A HREF="../wmpsets/wmpsets__wmp_channels.html">
+  WMP_CHANNELS</A>
+  3rd index: channel(s)
+<LI> <A HREF="../wmpsets/wmpsets__wmp_polars.html">
+  WMP_POLARS</A>
+  4th index: polarisation(s)
+<LI> <A HREF="../wmpsets/wmpsets__wmp_types.html">
+  WMP_TYPES</A>
+  5th index: typ = map (0) or antenna (1)
+<LI> <A HREF="../wmpsets/wmpsets__wmp_maps.html">
+  WMP_MAPS</A>
+  6th index: image sequence number(s)
+</UL>
+
+
+ <H3> More information: </H3> <UL>
+<LI><A HREF="../homepage.html">NEWSTAR Documentation Home page</A>
+<LI><A HREF="../hb_contents/hb_contents.html">The NEWSTAR Cookbook</A>
+</UL>
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+%%Trailer
+end
+userdict /end-hook known{end-hook}if
+%%EOF
diff --git a/wmpsets_public_intfc/images.pl b/wmpsets_public_intfc/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..9964356306f906e11b6eb6b3f6b74a29c859f62e
--- /dev/null
+++ b/wmpsets_public_intfc/images.pl
@@ -0,0 +1,5 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+
+1;
\ No newline at end of file
diff --git a/wmpsets_public_intfc/labels.pl b/wmpsets_public_intfc/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..37539f77a9e39e63eb095a682914e195e6334d2b
--- /dev/null
+++ b/wmpsets_public_intfc/labels.pl
@@ -0,0 +1,16 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".wmp.groups"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".public"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.maps"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.fields"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.types"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".descriptions"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.channels"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".contents"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.sets"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.polars"} ="$URL/wmpsets_public_intfc.html"; 
+$external_labels{".wmp.loops"} ="$URL/wmpsets_public_intfc.html"; 
+
+1;
\ No newline at end of file
diff --git a/wmpsets_public_intfc/wmpsets_public_intfc.html b/wmpsets_public_intfc/wmpsets_public_intfc.html
new file mode 100644
index 0000000000000000000000000000000000000000..67090ab8e47c9d8bcee3269117d6668d09c293ab
--- /dev/null
+++ b/wmpsets_public_intfc/wmpsets_public_intfc.html
@@ -0,0 +1,443 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>Public parameter group WMPSETS</b> 
+<A NAME=.contents><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<P><H2><A NAME=SECTION0001000000000000000>Contents</A></H2>
+<UL> 
+<LI> <A NAME=tex2html1 HREF=wmpsets_public_intfc.html#SECTION0001000000000000000>Contents</A>
+<LI> <A NAME=tex2html2 HREF=wmpsets_public_intfc.html#SECTION0002000000000000000>  <b>Overview</b></A>
+<LI> <A NAME=tex2html3 HREF=wmpsets_public_intfc.html#SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A>
+<UL> 
+<LI> <A NAME=tex2html4 HREF=wmpsets_public_intfc.html#SECTION0003100000000000000>  <b>References to public interfaces</b></A>
+<LI> <A NAME=tex2html5 HREF=wmpsets_public_intfc.html#SECTION0003200000000000000>  <b>Parameter WMP_CHANNELS</b></A>
+<LI> <A NAME=tex2html6 HREF=wmpsets_public_intfc.html#SECTION0003300000000000000>  <b>Parameter WMP_FIELDS</b></A>
+<LI> <A NAME=tex2html7 HREF=wmpsets_public_intfc.html#SECTION0003400000000000000>  <b>Parameter WMP_GROUPS</b></A>
+<LI> <A NAME=tex2html8 HREF=wmpsets_public_intfc.html#SECTION0003500000000000000>  <b>Parameter WMP_LOOPS</b></A>
+<LI> <A NAME=tex2html9 HREF=wmpsets_public_intfc.html#SECTION0003600000000000000>  <b>Parameter WMP_MAPS</b></A>
+<LI> <A NAME=tex2html10 HREF=wmpsets_public_intfc.html#SECTION0003700000000000000>  <b>Parameter WMP_POLARS</b></A>
+<LI> <A NAME=tex2html11 HREF=wmpsets_public_intfc.html#SECTION0003800000000000000>  <b>Parameter WMP_SETS</b></A>
+<LI> <A NAME=tex2html12 HREF=wmpsets_public_intfc.html#SECTION0003900000000000000>  <b>Parameter WMP_TYPES</b></A>
+</UL>
+</UL>
+<H1><A NAME=SECTION0002000000000000000>  <b>Overview</b></A></H1>
+<P>
+        This document contains an overview of the public parameter group WMPSETS, (part of) which is included in several <i>NEWSTAR </i> programs.
+<P>
+        The 
+document describes the individual parameters in alphabetical order. This description centers on the Help texts, which have been designed to guide the user to the proper choice at each junction, even if his knowledge of the overall workings of the program is only superficial.
+<P>
+        Please note that the generic prompt and help texts defined for these parameters are frequently superseded in the actual applications by alternative texts that are more appropriate to the situation at hand. Unfortunately, the present architecture of <i>NEWSTAR </i> precludes the inclusion of such texts in the documentation system, so the only opportunity to read that information is during program execution (in your terminal window!).
+<P>
+<A NAME=.descriptions><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H1><A NAME=SECTION0003000000000000000>  <b>Descriptions of the individual parameters</b></A></H1>
+<P>
+<A NAME=.public><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003100000000000000>  <b>References to public interfaces</b></A></H2>
+<P>
+<A NAME=.wmp.channels><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> 
+<H2><A NAME=SECTION0003200000000000000>  <b>Parameter WMP_CHANNELS</b></A></H2>
+<P>
+  <em>Prompt:</em> 3rd index: channel(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+    <PRE>
+Give the channel index-range CHN of an image-Set specification
+                                                (grp.fld.CHN.pol.typ.seq)
+</PRE>
+<P>
+  <PRE>
+Remember that channel 0 is the 'continuum' channel.
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take the continuum channel
+        n1              take channel nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over channels n1 through n2 [step n3]
+        *               loop over all channels for the field (wildcard)
+        n1-[*]          loop over all channels for the field,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated WMP_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.wmp.fields><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003300000000000000>  <b>Parameter WMP_FIELDS</b></A></H2>
+<P>
+<em>Prompt:</em> 2nd index: field(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the field index (range) FLD of an image-Set specification
+                                                (grp.FLD.chn.pol.typ.seq)
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) field
+        n1              take field nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over fields n1 through n2 [step n3]
+        *               loop over all fields in the observation (wildcard)
+        n1-[*][:n3]     loop over all fields in the observation,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated WMP_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.wmp.groups><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003400000000000000>  <b>Parameter WMP_GROUPS</b></A></H2>
+<P>
+<em>Prompt:</em> 1st index: grp  (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the group index (range) GRP of an image-Set specification
+                                                (GRP.fld.chn.pol.typ.seq)
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take first (or only) group
+        n1              take group nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over groups n1 through n2 [step n3]
+        *               loop over all available groups (wildcard)
+        n1-[*][:n3]     loop over all available groups,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated WMP_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.wmp.loops><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003500000000000000>  <b>Parameter WMP_LOOPS</b></A></H2>
+<P>
+<em>Prompt:</em> Loop specifications: |- (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 to 16 values
+<P>
+  <PRE>
+Using the WMP_LOOPS parameter in combination with your WMP_SETS soecification,
+you may specify repetitions of the operation you are currently defining,
+systematically incrementing the Group, Channel, etc. indices for each new cycle.
+</PRE>
+<P>
+  <PRE>
+This is done by specifying here pairs of values:
+</PRE>
+<P>
+  <PRE>
+        n1,incr1, n2,incr2, ...
+</PRE>
+<P>
+  <PRE>
+In each pair, the first value (n) indicates the number of times the loop has to
+execute; the second value (incr) indicates how the imaqge index is to be
+changed at the start of the successive loops.
+</PRE>
+<P>
+  <PRE>
+Example:
+        The specification WMP_SETS = grp.fld.1-2.* would select the combination
+of all images of frequency channels 1 and 2 for the field grp.fld. If you wish
+to process 32 sets of successive such pairs of frequency channels, you would
+have to type in all the successive WMP_SETS specifications:
+</PRE>
+<P>
+  <PRE>
+        grp.fld.1-2, grp.fld.3-4, ....., grp.fld.63-64
+</PRE>
+<P>
+  <PRE>
+Instead, you may specify WMP_LOOPS=32,0.0.2 and the first index only for
+WMP_SETS. This will cause the program to execute the present operation 32 times
+in a loop, starting with your WMP_SETS specification and then incrementing its
+indices by 0.0.2 for every iteration; this is equivalent to the above 32
+separate runs of the program.
+</PRE>
+<P>
+  <PRE>
+n must be > 0, and the increment can be any index string with simple positive
+or negative integers. An increment of 0 may be omitted, i.e. the increment
+specifications 0.0.3.0 and ..3 are equivalent.
+</PRE>
+<P>
+  <PRE>
+Loops may be nested (to a limiting depth of 8 levels). A following loop
+specification is executed inside the preceding one(s).
+</PRE>
+<P>
+  <PRE>
+Example of NESTED loops:
+        To run your program for 64 fields (fld index), for 10 odd channels (chn
+index) per field, starting at channel 7 and combining all polarisations (pol
+index) every time, specify:
+</PRE>
+<P>
+  <PRE>
+                WMP_LOOPS=64,.1, 10,..2
+                WMP_SETS=grp.0.7.* (initial set of images)
+</PRE>
+<P>
+  <PRE>
+The second loop is executed as an inner loop inside the first one, that is, for
+each mosaic subfield the channels are processed in a contiguous sequence.
+</PRE>
+<P>
+  <PRE>
+IF YOU WANT TO BE REMINDED OF WHAT IMAGES ARE IN YOUR FILE:
+        Type O or L in response to this prompt to get an Overview or Layout
+        of the file for which you need to specify the sets.
+</PRE>
+<P>
+<A NAME=.wmp.maps><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003600000000000000>  <b>Parameter WMP_MAPS</b></A></H2>
+<P>
+<em>Prompt:</em> 6th index: image sequence number(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the sequence-number index (range) SEQ of an image-Set specification
+                                                (grp.fld.chn.pol.typ.SEQ)
+</PRE>
+<P>
+  <PRE>
+Possible answers ([]=optional):
+</PRE>
+<P>
+  <PRE>
+        0               take the first image
+        n1              take image nr n1 (n1=0,1,2,3,....)
+        n1-n2[:n3]      loop over images n1 through n2 [step n3]
+        *               loop over all
+                         (wildcard)
+        n1-[*][:n3]     loop over all available ifrs|tels,
+                         starting with n1 [step n3]
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated WMP_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.wmp.polars><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003700000000000000>  <b>Parameter WMP_POLARS</b></A></H2>
+<P>
+<em>Prompt:</em> 4th index: polarisation(s) (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the polarisation index (range) POL of an image-Set specification
+                                                (grp.fld.chn.POL.typ.seq)
+</PRE>
+<P>
+  <PRE>
+        POL is a number indicating the polarisation. For interferometer data,
+pol=0,1,2,3 represents XX,XY,YX,YY. For telescope data, pol=0,1 represents X,Y.
+</PRE>
+<P>
+  <PRE>
+        This index is useful for defining loops (WMP_LOOPS parameter).
+Otherwise you may find the SELECT_XYX parameter more convenient.
+</PRE>
+<P>
+  <PRE>
+        If you prefer to use WMP_POLARS here, examples of reasonable answers
+are:
+                *       XX, XY, YX, YY
+                0-3:3   XX, YY
+                0       XX
+                3       YY
+</PRE>
+<P>
+  <PRE>
+Note:
+ The associated WMP_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+<A NAME=.wmp.sets><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003800000000000000>  <b>Parameter WMP_SETS</b></A></H2>
+<P>
+<em>Prompt:</em> Images to process:  grp.fld.chn.pol.typ.seq | (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 to 64 values
+<P>
+  <PRE>
+        A NEWSTAR .WMP file contains maps and antenna patterns for one or more
+objects. The basic unit of data is the two-dimensional IMAGE representing
+either a MAP of a piece of sky or the synthesised ANTENNA PATTERN. Images are
+addressed through an IMAGE INDEX which is a string of six integers separated by
+dots:
+</PRE>
+<P>
+  <PRE>
+                        grp.fld.chn.pol.typ.seq
+</PRE>
+<P>
+  <PRE>
+   A GROUP is basically an administrative unit, allowing the user to subdivide
+    his data, e.g. per object.
+</PRE>
+<P>
+  <PRE>
+   The FIELD and CHANNEL are the field and channel numbers of the observation(s)
+    in the .SCN file from which the image was made. These numbers are defined by
+    the way the observation was made and should be indentical for
+    all observations involved (which could, e.g., be several 12-hour mosaic
+    observations with different baseline sets.).
+</PRE>
+<P>
+  <PRE>
+   POL is a code indicating the polarisation. The code distinguishes the
+    four components of a full polarisation represntation:
+</PRE>
+<P>
+  <PRE>
+                0,1,2,3 =  XX.XY.YX.YY or
+                0,1,2,3 =  I,Q,U,V
+</PRE>
+<P>
+  <PRE>
+    but it is your responsibility to remember which of the two representations
+    applies.
+</PRE>
+<P>
+  <PRE>
+   TYP codes the type of image: 0 for a map, 1 for an antenna pattern.
+</PRE>
+<P>
+  <PRE>
+   The image SEQ uence number distinguishes images for which all five of
+    the preceding indices are identical. It is used in particular to distinguish
+    residual maps in a CLEAN sequence. It is your responsibility to know what
+    the different SEQ values represent.
+</PRE>
+<P>
+  <PRE>
+Index values start at zero. (Remember that for the CHN index 0 is the continuum
+channel.)
+</PRE>
+<P>
+  <PRE>
+You may select SETS of images for processing through [ranges of] values for the
+five indices, e.g.
+</PRE>
+<P>
+  <PRE>
+                2.3-5:2.*.1-7.*
+</PRE>
+<P>
+  <PRE>
+The WILDCARD value '*' means 'all'. Each index may also be specified as a
+RANGE: <first>-<last>[<:increment>]. Indices omitted are assumed to be '*',
+i.e.  ....1.0  means *.*.*.*.1.0. For wildcards at the end the dots may also be
+omitted, i.e. 1.0 means 1.0.*.*.*.*
+</PRE>
+<P>
+  <PRE>
+The notation 3-5:2 stands for 'from 3 through 5 in steps of 2'. The step must
+be positive; if it is omitted, it is taken to be 1 (as in '1-7' above).
+</PRE>
+<P>
+  <PRE>
+Multiple image SETS may be specified, separated by comma's: <Set1>,<Set2>,...
+The associated WMP_LOOPS keyword allows even more looping over index values.
+</PRE>
+<P>
+  <PRE>
+IF YOU WANT TO BE REMINDED OF WHAT IMAGES ARE IN YOUR FILE:
+        Type O or L in response to this prompt to get an Overview or Layout
+        of your .WMP file.
+</PRE>
+<P>
+  <PRE>
+IF YOU DO NOT YET FEEL COMFORTABLE WITH THESE CONCEPTS MORE HELP IS PROVIDED:
+        type '' or '>' to be prompted for each of the 6 indices separately,
+        with more specific explanation per index.
+</PRE>
+<P>
+  <PRE>
+IF YOU GET BORED WITH 6-NUMBER INDICES:
+        Absolute Cut nrs '#<n>' can be used as an alternative.
+</PRE>
+<P>
+<A NAME=.wmp.types><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>
+<H2><A NAME=SECTION0003900000000000000>  <b>Parameter WMP_TYPES</b></A></H2>
+<P>
+<em>Prompt:</em> 5th index: typ  (<em>may vary per application</em>)<BR><em>Expected input:</em> Character *32:  1 value
+<P>
+  <PRE>
+Give the type index (range) TYP of an image-Set specification
+                                                (grp.fld.chn.pol.TYP.seq)
+</PRE>
+<P>
+  <PRE>
+This index is most useful in loop specifications (parameter WMP_LOOPS).
+</PRE>
+<P>
+  <PRE>
+Possible answers:
+</PRE>
+<P>
+  <PRE>
+        0               maps only
+        1               antenna patterns only
+        0-1 or *        both maps and antenna patterns
+</PRE>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/wnb.gif b/wnb.gif
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diff --git a/wndpoh.txt b/wndpoh.txt
new file mode 100644
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+++ b/wndpoh.txt
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+Dynamic tailoring of the Newstar program-parameter interface
+------------------------------------------------------------
+
+Contributed by Johan Hamaker, 940916
+
+
+Statement of the problem
+========================
+
+	The DWARF parameter interface and the way it is harnessed in the
+Newstar programs is plagued by several problems that confuse the user:
+
+	- many keywords are used in multiple places serving multiple, often
+quite different, functions ("keyword overloading");
+
+	- since DWARF allows only static definitions of keyword prompt, options
+and help text, the information provided to the user in a prompt is either too
+generic (in order to cover all functions for which the keyword is used) or
+confusing (when a keyword is re-used in a context that differs from the one it
+was designed for);
+
+	- the logic underlying the order in which prompts are presented is in
+many places different from a user's natural expectations.
+
+	Following the DWARF design philosophy a proper solution would be to
+split overloaded keywords into multiple ones; in addition the order of the
+prompts could be made more natural to the uninitiated user. Both of these
+options are unacceptable because of their pervasive impact on existing batch
+procedures.
+
+	In trying out various ways to patch the situation I noticed that the
+only information that a user can hardly avoid noticing is that provided in the
+prompts (and in the help texts if he consults these). Everything else is very
+easily overlooked.
+
+	The problem, then, is to provide prompts, options and help texts
+specific to each of the quite different contexts in which a keyword may be
+used, without resorting to changing the keywords themselves. In other words, we
+want a method enabling programs to set these prompt components dynamically. As
+a practical matter, the method should have a minimal impact on the existing
+programs.
+
+
+The new subroutine WNDPOH
+=========================
+
+	A new routine WNDPOH has been created that accepts dynamic Prompt,
+Options and Help strings. These will be used in the subsequent parameter prompt
+(directly through WNDPAR or indirectly through WNDNOD, NSCHAS etc.). The prompt
+and options strings replace those in the .ppd file; the help text may either be
+inserted in front of the .pps text or replace it.  Thus, the call sequence is
+simply
+
+		CALL WNDPOH (<prompt>, <options>, <help>)
+		CALL WNDPAR (...
+
+or
+
+		CALL WNDPOH (<prompt>, <options>, <help>)
+		CALL NSCHAS (...
+
+etc.
+There is no need to clear the strings later, this is done automatically once an
+answer from the user has been accepted.
+
+
+Details on the call arguments
+-----------------------------
+
+	The help text may contain newline directives in the WNCTXT format: !/.
+It is recommended to format help text in lines that will fit in single
+80-character Fortran lines and extend the quoted string over as many
+continuation lines as are necessary, e.g.
+
+	    CALL WNDPOH(
+	1'Target node to which to write corrections',' ',
+	3'SET COPY copies the average telescope corrections from 1 complete!/
+	3input sector to selected parts of any number of output sectors.')
+
+A help text ending in a line '#-' signals that the text OVERRIDES the .ppd help
+text rather than being prepended to it (so the .ppd text will not be shown).
+
+	The <prompt> and <options> strings are limited to 128 characters, the
+<help> text to 512 (or a few less). Blank arguments to WNDPOH are ignored, i.e.
+they leave the corresponding dynamic text unaltered.
+
+
+Where to program dynamic prompting
+----------------------------------
+
+	The following is a list (possibly still incomplete) of keywords and
+subroutine calls that may need dynamic prompting. A complete example of how I
+envisage the use of WNDPOH is in ncadat.for.
+
+	all <xxx>_NODE keywords (WNDNOD)
+
+	all <xxx>_SETS keywords (WNDST<x>)
+
+	all <xxx>_LOOPS keywords (WNDXLP) in those cases where the loop controls
+	  more than one ,xxx>_SETS stream
+
+	SELECT_XYX (NSCPL<x>) when used to select telescope rather than
+	  interferometer polarisations. In this case the dynamic options are
+	  'X,Y,XY', and the subsequent NSCPLS call must read
+		CALL NSCPLS(XY_P,<pol.mask>)
+	  where XY_P is defined in CBITS_DEF
+
+	SELECT_IFRS (NSCIF<x>), SELECT_TELS (NSCTL<x>) in those cases where it
+	  is not obvious to which stream (input or output) the selection
+	  pertains.
+
+
+Limitations
+===========
+
+	1. The dynamic information is not included in the hypertext display for
+the keyword, because the hypertext source file is a static derivate of the .psc
+or .pef file. For this reason the dynamic information is always shown on the
+terminal for all forms of on-line help requests.
+
+	2. As stated before, the method can not change the order in which
+prompts appear.
+
+	3. Since the dynamic texts are provided by the program, they are not
+available to dwspecify. I consider this a minor disadvantage since dwspecify is
+a primitive program in other ways as well. For interactively setting up
+parameter values dwexe/norun is a much better alternative that does have access
+to the dynamic texts.
+
+
+
+APPENDIX: Implementation
+========================
+
+	WNDPAR through GET_PARM calls on routines PPD_PRSTR_GET, PPD_OPSTR_GET
+and PPD_HSTR_GET to fetch the prompt, options and help strings from the .ppd
+file. To allow a program to modify e.g. the prompt dynamically, a new entry
+point PPD_PRSTR_LSET was created. It takes a prompt string as argument and
+stores it in an internal buffer. When PPD_PRSTR_GET is called later, it checks
+this buffer and if it finds anything there, uses it instead of the .ppd prompt.
+The same method is used to allow dynamic options and help texts; a dynamic help
+text may either override the static text or be inserted in front of it. A
+terminating line '#-' is inter[reted as an 'override' flag.
+
+	For the programmer's convenience, a single routine is available to set
+dynamic information pertaining to the subsequent direct or indirect (through
+another routine such as WNDSTA) WNDPAR call.
+
+	The dynamic information will be used in the prompt and any automatic
+repeat of it; it will then automatically be cleared.
+
+
+Automatic clearing
+==================
+
+	Subroutines like WNDNOD, WNDSTA, NSCIFS are called in various contexts,
+so the use of WNDPOH with them is desirable. Internally, these routines call
+WNDPAR and may do so repeatedly in case of an incorrect reply. For this reason
+WNDPAR can not automatically clear the dynamic strings.
+
+	The solution is for the calling subroutines to set an 'inhibit
+clearing' flag. WNDPAR will only clear the dynamic strings if this flag is
+clear. Any routine that sets the flag is responsible for clearing both the falg
+and the strings, through a call to WNDPOHC.
+
+	The flag must be accessible to several routines and must therefore
+reside in a COMMON block. At present the location A_J(0) defined by WNG_DEF is
+used because it was available. This solution is sound except that it is
+invisible outside the routines that use the flag; an unexpected conflict could
+arise later when someone decides that he may use this location for another
+purpose.
+
+
diff --git a/wntinc.txt b/wntinc.txt
new file mode 100644
index 0000000000000000000000000000000000000000..e3d976b5ff5acb9565de658ef6766c5619659368
--- /dev/null
+++ b/wntinc.txt
@@ -0,0 +1,450 @@
+wntinc.txt	draft-5 930902/WNB
+
+
+
+1. Introduction
+
+WNTINC is a replacement for WNTAB. The major changes are based on
+comments/remarks made by JPH and MdV, and on deficiencies found by myself.
+It has been rewritten to make it more modular and to get rid of any
+non-described numerical codes.
+Main features:
+- calculation on local variables
+- multiple structure definitions
+- structure definitions inside DEFINE
+- structures in data statements
+- implicit array lengths
+- implicit string lengths
+- alignment possibilities
+- map/union options (not implemented in this version yet)
+- deletion of some unused options
+- complete C coverage
+- continuation lines
+
+An example of the use can be found in wnt.dsc
+
+
+2. Input structure
+
+The input file to WNTINC is a NAME.dsc file. The parameter to WNTINC is
+NAME, possibly modified by a directory indication. Whatever the case of
+NAME, it will be assumed to reference a lc NAME.dsc.
+All input lines will be converted to UC, unless enclosed in "". The output
+names will all be UC for Fortran and Unix parameters; lc for Unix variable
+names.
+Blanks in the following indicate 'white space' (i.e. in general spaces
+and/or tabs)
+
+NAME.dsc will consist of a number of lines. Each line consists of a (possibly
+empty) command part, followed by an optional comment part which should be
+preceded with an !. A line can be continued by having the last non-blank
+character in the command part to be a '\'.
+An empty line will be considered to be a comment line; a comment not
+starting at the beginning of the line will be considered to be a
+continuation of the previous line (whether '\' present or not. (This
+is to distinguish comments that should precede fields from comments that
+should follow fields)).
+
+Each command can be:
+- empty (i.e. comment line only)
+	can occur everywhere
+- the first non-blank character a '%': commands that steer the behaviour
+  of the compiling process
+	can occur everywhere
+- the first non-blank character a '.': commands that steer the data
+  interpretation process
+	can occur only in 'data-blocks'; except .DEFINE: can occur only
+	once outside a data-block; .STRUCTURE (.BEGIN) that can occur
+	inside and outside data-blocks and which define the start of
+	data-blocks; .PARAMETER that can occur everywhere
+- data command (starts always with a '-' (dummy name)) or alphabetic character
+
+
+3. Output files
+
+WNTINC produces the following output files (NAME is the input file name
+name, or set by the %NAME) (all filenames in lc):
+
+a. If .STRUCTURE type data blocks present:
+
+- NAME_o.def	Fortran include file containing parameters and/or comments
+		and/or 'structure-type' definitions
+- NAME_o.inc	C include file containing parameters and/or comments and/or
+		structure definitions
+- NAME_t.def	Fortran include file containing information for translating
+		data structures from one representation to another (using
+		WNTT* routines)
+- NAME_t.inc	C include file
+- NAME_e.def	Fortran include file containing information for formatted
+		printout and/or input of data structures
+- NAME_e.inc	C include file
+
+b. If a .DEFINE data block present, or if no .STRUCTURE and no .DEFINE type
+	present:
+
+- NAME.def	Fortran include file containing comments, parameters (if no
+		_o present) and/or common blocks and/or data definitions
+- NAME.inc	C include file containing the same
+- NAME_bd.for	Common block data-initialisation (if necessary)
+
+d. Always:
+
+NAME.LIS describing:
+- the input lines
+- the offset in and structure of common blocks and data structures.
+
+
+4. Comment lines
+
+
+Commment outside data blocks will be considered to be comments for the .dsc
+file only.
+Comments inside data blocks will form part of the program output. Lines
+starting with a ! will be output proceeding the data items following. Other
+comments will always follow the data items they follow.
+
+
+5. % commands
+
+%name commands steer the compiling process. Some action may be dependent on
+wether it is inside or outside data blocks. The following commands are
+recognized:
+
+%NAME=string		name of output files to be used.
+			Default: input file name
+%DATE=yymmdd		date of producing output
+			Default: today
+%USER=name		name of user 
+			Default: login name
+%VERSION=num		Current version
+			Default: 1
+%SYSTEM=num		Current system
+			Default;1
+
+%%NAME			will show currently defined name
+%%DATE			.. date
+%%USER			.. user
+%%VERSION		.. version
+%%SYSTEM		.. system
+
+If more than one of the above commands are encountered, the last will be
+used
+
+
+%[NO]LIST		list lines in log (e.g. to suppress include file listing)
+			Default: LIST
+%[NO]PRINT		list comments in output (not fully implemented)
+			Default: print
+%[NO]ALIGN		align data items on their lengths (complex data on
+			their constituant length; structure on the largest
+			element length included in the structure)
+
+The above act as switches
+
+%INSERT=string		include specified file
+%INCLUDE=string		include specified file
+			As a rule the string will be of the form NAME_DSF,
+			referencing an include file name.dsf
+
+The above are identical
+
+%COMMENT=string		include specified comment at begin of output file
+%REVISION=nam=yymmdd=string include specified comment as a revision
+%FORTRAN=string		include the Fortran statement (e.g. IMPLICIT NONE).
+			If outside data block: at begin of output; if inside:
+			at end of output
+%CC=string		include the C statement
+
+The above act additive
+
+%LOCAL=name=expr	specify a local variable name with a value expr.
+			The value of the name can be an integer value, or
+			a character string. If the expr can be evaluated to
+			an integer constant it will have an integer value,
+			else a character string value.
+			In most places were information has to be supplied it
+			can be supplied as:
+			- integer expression: containing known variable names,
+			  integer constants (), +-*/, +- unary
+			- character expression: single known name with a
+			  character value
+			- string (anything that cannot be interpreted as
+			  one of the above)
+			Note: an expression starting with a ( will be
+			deemed to have been ended at the belonging ). This
+			is for some formatting reason.
+			Note: / is only recognised if not preceded and or
+			followed by blanks. This is to recognize the /../
+			initialisation
+			Examples:
+			2.		is string "2."
+			01		is value 1 (and string "1" if appropiate)
+			(1)*2		is string "(1)*2"
+			+(1)*2		is value 2 ("2" string)
+
+%GLOBAL=name=expr	identical to the combination:
+			%LOCAL=name=expr
+			.PARAMETER
+				name	tp	/expr/
+			where tp is either J or C(length expr)			
+
+
+6. . commands
+
+. commands define some aspects of the data commands present. Recognized:
+
+
+.END			ends blocks starting with .STRUCTURE, .DEFINE, or
+			.MAP
+.DEFINE			starts a 'define-block' 
+			Can only occur once outside a data block (define-
+			or struct-block). The sub-type will initially be
+			data
+.STRUCTURE[=sname]	starts a structure block with name sname or NAME
+			can occur inside or outside a define-block. Many
+			structure blocks are allowed, but they may not be
+			nested (there references (see S:) may, of course,
+			be nested.
+			Each structure block should have a unique name
+			(i.e. only one unnamed allowed). The sub-type
+			will initially be data
+.BEGIN[=sname]		identical to .STRUCTURE (for historical reasons)
+
+The above define the type of current data block. It will define the output
+files produced, and which sub-types are allowed.
+
+
+.[OFFSET]=nexpr		will define a current offset
+			Only for structure-blocks; assumed to be in data-sub
+			For define-blocks allowed in common-sub
+.ALIGN=nexpr		Align offset on specified lengths (note the program
+			knows the defined local variables LB_B etc)
+			Allowed in common-sub en structure data-sub
+.MAP[=nexpr]		will start equivalence structures
+.UNION[=nexpr]		will start the next structure to be equivalent
+			The nexpr will serve as an id that can be used in
+			the WNT translation tables to get the proper
+			translation of the data; and is used to generate
+			a name for C. Definition ends at .END
+			Can only be used in structure-blocks at data-sub
+			Note: Not implemented yet, but its action can be
+			made by the equivalence = (except for the translation
+			choice option)
+.PARAMETER		Interprets following data lines as parameters
+.DATA			Interprets following lines as data
+.COMMON[=cname]		Interprets following lines as to belong to common
+			cname_COM (or NAME_COM)
+			Only in define-block
+
+7. Data commands
+
+A data command describes a data-item. It consists of two mandatory fields
+separated by blanks, and an optional (obligatory for parameters and implied
+lengths) initialisation and an optional editing field (only allowed for
+structure data-sub).
+A full command is:
+
+	name[=rnam]	type	[/init, ..../] [<edit>]
+
+Name can be "-" to indicate a dummy name (to be used for filling) or a name
+starting with an alphabetic (including _$) character and having only
+alphanumeric characters (including _$).
+The name can be followed with an '=' followed by a reference name (not valid
+for parameter data). The data will be put at the same offset as the data at
+the reference name. Limitations:
+- rnam should immediately precede name in the same sub-block, i.e. all names
+	referencing the same rnam should be continuous after rnam
+- name should describe an entity not larger than the entity of rnam
+- if in ALIGN mode, the alignment of name should be of the same or lesser
+	value than that of rnam
+
+Type describes the data entity. It consists of a type indicator, optionally
+followed by an array definition.
+
+The indicator can be:
+	-  B  I1		byte
+	I  I2			integer*2
+	J  I4			integer*4
+	K			long integer (for now identical to J)
+	E  R4			real*4
+	D  R8			real*8
+	X			complex*8
+	Y			complex*16
+	A			double length ASCII
+	Cnexpr			character*(nexpr)
+	C*			character*(*) (length from initialisation
+				string; hence only allowed for parameters
+				and data in common-sub or define data-sub
+	S:name			structure as defined by name
+	A:[([start][,inc])]	enumeration(add). If in a data-type mode in
+				define-block, it will generate a character
+				string array with an implied length from
+				the initialisation data, containing the
+				strings provided and a final ' ' string.
+				This variable can then be used in e.g.
+				WNCAFU to do a minimax search for its
+				occurrence. In addition (and in all other
+				cases only) it will produce a series of
+				parameters consisting of pre_txt with
+				values starting at start and incrementing
+				with inc, where the txt is the first three
+				(or less if not existing) characters of the
+				strings, and pre__N will be defined to give
+				the number of values+1; pre__I the increment
+				and pre__L and pre__H the lowest and highest
+				values. The pre__*
+				will also be available as local variables.
+				Default start, inc: 1
+				E.g.:
+				cb  E:		/structure,define,end/
+				will produce:
+				  CHARACTER*(10) CB__TXT(4)
+				    DATA CB__TXT/'STRUCTURE','DEFINE','END',' '/
+				  INTEGER CB_STR,CB_DEF,CB_END,CB__N,
+						CB__I,CB__H,CB__L
+				    PARAMETER(CB_STR=1,CB_DEF=2,CB_END=3,
+						CB__N=4,CB__I=1,CB__L=1,CB__H=3)
+	AR:[([start][,inc])]	as A:, but the parameter names will be *_pre
+	M:[([start][,fac])]	enumeration(mul). As A:, but multiplicative
+				rather than additive.
+				Default start, fac: 1, 2
+	MR:[([start][,fac])]	as M:, but *_pre parameters
+	N:[(val,...)]		enumeration(named). As A:, but values are
+				specified (up to number of array indices
+				allowed, currently 16).
+				Default val: 1,2,3,...
+				Note: No __H,__L and __I produced
+	NR:[(val,...)]		as N:, but *_pre parameters
+
+	[A|M|N][R][F][*]:[...]	as A: M: or N:, but Reversed name_ if R present,
+				full name (rather than 3 first characters)
+				if F present, no __ names and text if * present.
+
+
+
+
+Array specification:
+
+	(nexpr[:nexpr],....) The last index (i.e. the high-bound) can be
+specified as '*' to indicate an implied length to be deduced from the
+initialisation string (if this was allowed). All format types except
+A:, M: and N: can have an array index.
+
+
+Initialisation data:
+
+	/init, .../  each init can be an expression, or (nexpr)init. In the
+latter case the (nexpr) gives a repeat factor.
+If the format was character and the string contains blanks, ',' '/' or
+anything that can be but should not be interpreted as an expression (e.g.
+'02' which may not be converted to '2'), or is case sensitive, it should be
+enclosed in "".
+
+
+Edit data:
+
+	<format,code,units,special> 
+
+Each field may be omitted, trailing ',' may be omitted.
+	format:		WNCTXT (WNCTXI) type format (e.g. AEF12.6)
+			Default: deduced from item
+	code:		0: editing of field allowed, >0: not allowed
+			Default: 0
+	units:		string specifying units (e.g. "deg")
+			Default: " "
+	special:	string to indicate something special defined by user
+			of edit data (e.g. if formatting types are not
+			sufficient, e.g. to type interferometer names)
+			Default: " "
+			The special field is used for S: fields, the default
+			will be "S:NAME". By definition the user can put
+			anything in it. The only definition I have now is:
+			"D:NAME" for a field containing a disk pointer to
+			to a structure NAME. The editing routine will be
+			extended to recognise these special codes.
+
+8. Program changes, omissions
+
+The following features are not fully implemented yet:
+
+- initialisation of structures (relatively easy, will do soon)
+- MAP/UNION: the = feature caters for everything except the run-time choice
+	of translation table. This last feature is probably dangerous anyway.
+	If the need arises, easily to implement.
+- C: I have only tested that the .inc files look ok, and are all accepted
+	by the C compilers.
+
+The following existing programs need changes:
+
+- ncomp/ndel.ssc: to change to WNTINC: done
+- no _m.mvx output: use existing ones by preserving them. If the f??.dsc files
+	change, the .mvx has to change. However, the DECalpha has a different
+	assembler from the VAX, and changes are necessary anyway in the
+	existing Macro programs (i.e. the I/O routines).
+	I have done the preservation, and will look at changing the Macro
+	programs to Fortran.
+- no .RECORD: it has been enhanced by the S: data item: scw.dsc and ohw.dsc
+	uses this: change done
+- output now _o.inc rather than -c.inc to get uniform naming: wnf I/O
+	routines have to change: done
+
+
+9. Detailed program output
+
+
+The output of the program consist of:
+- parameters
+- structure definitions
+- data definitions
+- common defintions
+- translation tables
+- edit tables
+
+- Parameters
+
+Parameters are output in Fortran as PARAMETER, with name and type as given.
+In C as #define NAME init-text
+Note: Maybe they should be given as:
+	#define NAME (cast) init-text	?? comments please
+For A:, M:, N: type the following INTEGER PARAMETERs are produced:
+	NAME__N			# of items in list +1 (==first available
+				element). Also available as local variable
+	NAME__L			First value (not for N:)
+	NAME__H			Last value (not for N:)
+	NAME__I			Increment(A:) or factor(M:)
+	NAME_txt		For each non-empty init-txt (i.e. not ,, or ,/)
+				the first 3 char of the text (or less if
+				shorter text) are taken as txt.
+
+- Structure definitions
+
+Structure definitions are given in C as:
+	struct struct-name { type name [indices]; ,,,};
+All names in lc; indices in reversed order from Fortran.
+In Fortran each given name is combined with the struct-name sname to
+produce the following INTEGER PARAMETERs:
+	SNAME__L		Byte length of structure
+	SNAME__V		Version
+	SNAME__S		System
+In the edit output:
+	SNAME__EL		Length of edit arrays
+The above are also available as %LOCAL constants
+For historic reasons also available:
+	snameHDL
+	snameHDV
+	snameHDS
+	snameEDL
+For all structure elements:
+	SNAME_NAME_1		Byte offset from start of structure
+In addition for CHARACTER data:
+	SNAME_NAME_N		Length in characters
+for STRUCTURE data:
+	SNAME_NAME_N		Length in bytes
+for all if the offset from the beginning is an integer multiple of the unit
+size of the data type (e.g. LB_J=4 for INTEGER; structure length for structure):
+	SNAME_NAME_type		Offset in unit-length units from start
+				of structure. Types are the types as given
+				in the definition (C,J,E,Y,S etc)
+
+
+
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+ 0x00,0x08,0x00,0x00,0x80,0x11,0x8c,0x30,0x00,0x00,0x00,0x08,0x01,0xc0,0x0c,
+ 0x00,0x04,0x90,0x20,0x10,0x23,0x40,0x36,0x82,0x8d,0x00,0x02,0x80,0x40,0x8c,
+ 0x00,0x08,0x00,0x00,0x00,0xbe,0x11,0x00,0x00,0x00,0x08,0x00,0x00,0x80,0x11,
+ 0x8c,0x10,0x00,0x00,0x00,0x08,0x01,0xc0,0x08,0x00,0x04,0x98,0x30,0x18,0xa3,
+ 0x3f,0x36,0xc2,0x8c,0x00,0x02,0x80,0x40,0x8c,0x00,0x08,0x00,0x00,0x00,0xba,
+ 0x11,0x00,0x00,0x00,0x08,0x00,0x00,0x80,0x11,0x8c,0x18,0x00,0x00,0x00,0x08,
+ 0x01,0xc0,0x08,0x00,0x04,0xf8,0x33,0x18,0x23,0x60,0x36,0x62,0x8d,0x00,0x02,
+ 0x80,0x40,0x8c,0x00,0x08,0x00,0x00,0x00,0xa3,0x11,0x00,0x00,0x00,0x08,0x00,
+ 0x00,0x80,0x11,0x8c,0x18,0x00,0x00,0x00,0x08,0x01,0x80,0x0c,0x00,0x04,0x80,
+ 0x30,0x18,0x32,0x60,0x26,0x33,0xc9,0x00,0x02,0x80,0x40,0xc8,0x00,0x08,0x00,
+ 0x00,0x00,0x23,0x19,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x99,0xc9,0x18,0x00,
+ 0x00,0x00,0x08,0x01,0x80,0x0d,0x00,0x04,0xe0,0x33,0x18,0x36,0xc0,0x67,0xfb,
+ 0xd9,0x00,0x02,0xe0,0xf3,0xd9,0x00,0x08,0x00,0x00,0x00,0x36,0x1b,0x00,0x00,
+ 0x00,0x08,0x00,0x00,0x00,0x9b,0xd9,0x18,0x00,0x00,0x00,0x08,0x01,0x00,0x07,
+ 0x00,0x04,0x00,0x30,0x18,0x1c,0x80,0xc1,0x01,0x70,0x00,0x02,0x00,0x00,0x70,
+ 0x00,0x08,0x00,0x00,0x00,0x1c,0x0e,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x0e,
+ 0x70,0x18,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,
+ 0x01,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,
+ 0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x04,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x08,0x00,
+ 0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x08,0x01,0x00,0x00,0x00,0x04,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x00,0x02,0x00,0x00,0x00,0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,
+ 0x00,0x08,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x00,0x08,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,0xff,
+ 0xff,0xff,0xff,0xff,0xff,0x0f};
diff --git a/wsrt_fact_sheet/_13438_tex2html_wrap213.png b/wsrt_fact_sheet/_13438_tex2html_wrap213.png
new file mode 100644
index 0000000000000000000000000000000000000000..7824e292260eea7d3b760c36eef8c1ed2a69b8f3
Binary files /dev/null and b/wsrt_fact_sheet/_13438_tex2html_wrap213.png differ
diff --git a/wsrt_fact_sheet/_13438_tex2html_wrap213.xbm b/wsrt_fact_sheet/_13438_tex2html_wrap213.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..a31d7ecb8f2d05aebec6a4e03500fc208fd9b0e0
--- /dev/null
+++ b/wsrt_fact_sheet/_13438_tex2html_wrap213.xbm
@@ -0,0 +1,4 @@
+#define noname_width 7
+#define noname_height 7
+static char noname_bits[] = {
+ 0x61,0x33,0x1e,0x0c,0x1e,0x33,0x61};
diff --git a/wsrt_fact_sheet/_13438_tex2html_wrap215.png b/wsrt_fact_sheet/_13438_tex2html_wrap215.png
new file mode 100644
index 0000000000000000000000000000000000000000..4f92163ec5b5b6bd36db3f10045d2d3fad286037
Binary files /dev/null and b/wsrt_fact_sheet/_13438_tex2html_wrap215.png differ
diff --git a/wsrt_fact_sheet/_13438_tex2html_wrap215.xbm b/wsrt_fact_sheet/_13438_tex2html_wrap215.xbm
new file mode 100644
index 0000000000000000000000000000000000000000..2e3f6c8d5f7a83541e5b9a8b1ba97b1f007b9865
--- /dev/null
+++ b/wsrt_fact_sheet/_13438_tex2html_wrap215.xbm
@@ -0,0 +1,6 @@
+#define noname_width 23
+#define noname_height 14
+static char noname_bits[] = {
+ 0xfe,0x03,0x00,0x36,0x03,0x00,0x33,0x02,0x00,0x31,0x02,0x00,0x10,0x00,0x00,
+ 0x18,0x00,0x00,0x18,0x00,0x00,0x18,0x4c,0x62,0x08,0xee,0x72,0x3f,0x6e,0x72,
+ 0x00,0x4f,0x7b,0x00,0xcf,0x7b,0x00,0x60,0x01,0x00,0xe0,0x01};
diff --git a/wsrt_fact_sheet/images.pl b/wsrt_fact_sheet/images.pl
new file mode 100644
index 0000000000000000000000000000000000000000..a49c90ecdd7c25205f3a4c40f9383161278ac4d9
--- /dev/null
+++ b/wsrt_fact_sheet/images.pl
@@ -0,0 +1,11 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate image original text (scrambled) with physical files.
+
+$key = q/{}$T_<<115>>sys<<115>>${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_13438_tex2html_wrap215.xbm">'; 
+$key = q/{}$times${}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_13438_tex2html_wrap213.xbm">'; 
+$key = q/{tabular}<<198>>|c|r@<<118>>--<<118>>l|c|c|c|<<198>>hlinemulticolumn<<119>>1<<119>><<120>>|c|<<120>><<121>><<217>><<217>>$lambda$<<218>><<218>><<121>>;html_special_mark_amp;multicolumn<<122>>2<<122>><<123>>|c|<<123>><<124>>Frequ<<124>>;html_special_mark_amp;multicolumn<<125>>1<<125>><<126>>|c|<<126>><<199>><<219>><<219>>$T_<<127>>sys<<127>>$<<220>><<220>><<199>>;html_special_mark_amp;multicolumn<<128>>1<<128>><<129>>|c|<<129>><<130>>MaxBW<<130>>;html_special_mark_amp;multicolumn<<131>>1<<131>><<132>>|c|<<132>><<133>>Sensitivity<<133>>multicolumn<<134>>1<<134>><<135>>|c|<<135>><<136>>cm<<136>>;html_special_mark_amp;multicolumn<<137>>2<<137>><<138>>|c|<<138>><<139>>MHz<<139>>;html_special_mark_amp;multicolumn<<140>>1<<140>><<141>>|c|<<141>><<142>>K<<142>>;html_special_mark_amp;multicolumn<<143>>1<<143>><<144>>|c|<<144>><<145>>MHz<<145>>;html_special_mark_amp;multicolumn<<146>>1<<146>><<147>>|c|<<147>><<148>>mJy<<148>>hline92;html_special_mark_amp;320;html_special_mark_amp;330;html_special_mark_amp;130;html_special_mark_amp;5;html_special_mark_amp;0.549;html_special_mark_amp;607;html_special_mark_amp;610;html_special_mark_amp;110;html_special_mark_amp;2.5;html_special_mark_amp;0.621;html_special_mark_amp;1365;html_special_mark_amp;1425;html_special_mark_amp;60;html_special_mark_amp;60;html_special_mark_amp;0.0618;html_special_mark_amp;1590;html_special_mark_amp;1730;html_special_mark_amp;60;html_special_mark_amp;80;html_special_mark_amp;0.156;html_special_mark_amp;4770;html_special_mark_amp;5020;html_special_mark_amp;110;html_special_mark_amp;80;html_special_mark_amp;0.07hline{tabular}/;
+$cached_env_img{$key} ='<IMG ALIGN=BOTTOM ALT="" SRC="_13438_tabular117.xbm">'; 
+
+1;
\ No newline at end of file
diff --git a/wsrt_fact_sheet/labels.pl b/wsrt_fact_sheet/labels.pl
new file mode 100644
index 0000000000000000000000000000000000000000..4c2629388a842666ccf6f64fac417166e3c95645
--- /dev/null
+++ b/wsrt_fact_sheet/labels.pl
@@ -0,0 +1,7 @@
+# LaTeX2HTML 0.5.3 (Wed Jan 26 1994)
+# Associate symbolic labels with physical files.
+
+$external_labels{".wsrt.layout"} ="$URL/wsrt_fact_sheet.html"; 
+$external_labels{".sensitivity"} ="$URL/wsrt_fact_sheet.html"; 
+
+1;
\ No newline at end of file
diff --git a/wsrt_fact_sheet/wsrt_fact_sheet.html b/wsrt_fact_sheet/wsrt_fact_sheet.html
new file mode 100644
index 0000000000000000000000000000000000000000..96c29dbebc5df9c557e765693867642751445666
--- /dev/null
+++ b/wsrt_fact_sheet/wsrt_fact_sheet.html
@@ -0,0 +1,74 @@
+<HEAD>
+<TITLE>No Title</TITLE>
+</HEAD>
+<BODY><P>
+ <b>WSRT fact sheet</b>
+<P>
+<A NAME=.wsrt.layout><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A> The layout of the WSRT on its East-West baseline. 
+<A HREF="../fig/wsrt_layout.ps"><STRONG>FIGURE</STRONG></A> 
+ .]<i><BR>The WSRT array consists of 10 fixed and 2 pairs of movable telescopes, placed on a straight East-West line of about 3km length. Each telescope has a diameter of 25m, and a mesh-width of 8 mm.  The interval between the 10 fixed telescopes (labeled 0 through 9) is 144m. The movable pair AB is placed on a 300m railtrack immediately to the East of the fixed array; the second movable pair, CD sits on 150m of rail track 1.2 km away. 
+<BR>The positions of the <em>fixed telescopes</em> (0-9) are defined from West to East as 0(144)1296m.  The 4 <b>movable telescopes</b> (A,B and C,D) can be moved to increase the uv-coverage.  In the <em>standard configurations</em>, all four are moved together, so that their relative positions remains constant: AB=CD=72m, AC=BD=09=1296m, 0A=9C, 0B=9D. Thus, in the Standard Configuration, the only parameter needed to specify the array is the distance 9A: 
+<BR><BR>-       9A=36m: telescopes ABCD are placed at 1332, 1404, 2628, 2700 m <BR>-       9A=54m: telescopes ABCD are placed at 1350, 1422, 2646, 2718 m <BR>-       9A=72m: telescopes ABCD are placed at 1368, 1440, 2664, 2736 m <BR>-       9A=90m: telescopes ABCD are placed at 1386, 1458, 2682, 2754 m 
+<BR><BR>Regular covering of the uv-plane gives the lowest grating sidelobes.  This is achieved by placing the movable telescopes in such a way that the 12-hour concentric elliptic uv-tracks are regularly spaced, in the following way: 
+<BR><BR>-       1<IMG ALIGN=BOTTOM ALT="" SRC="_13438_tex2html_wrap213.png">12 hrs: 9A=72m, giving 72m intervals between uv-tracks. <BR>-       2<IMG ALIGN=BOTTOM ALT="" SRC="_13438_tex2html_wrap213.png">12 hrs: add 9A=36m, giving 36m intervals. <BR>-       4<IMG ALIGN=BOTTOM ALT="" SRC="_13438_tex2html_wrap213.png">12 hrs: add 9A=54 and =90m, giving 18m intervals (with the shortest 18m spacing missing). 
+<BR><BR>Smaller intervals between uv-tracks are better, since this causes the first grating ring to have a larger radius.  For intervals of 18m (smaller than the telescope diameter), the grating rings will be essentially outside the primary beam. </i>
+<P>
+        The redundant spacings in the regular WSRT array can be used for model-independent internal calibration.  The visibilities measured by two redundant interferometers (i.e.  with the same baseline length and orientation) must obviously be identical.  Thus, any differences between them must be caused by instrumental errors, including the effects of the Earth troposhere and ionosphere.
+<P>
+        Maximum redundancy occurs if 9A=72m in the standard configuration 
+<A HREF=" #.wsrt.layout">figure</A>: baselines 9A=AB=CD=72m, and 09=1B=AC=BD=1296m.  In this case, there is a `full redundancy solution' for both phase and gain, linking the errors of all 14 telescopes.  For other values of the distance 9A, there will still be a full solution for the telescope gain errors, but the phase solution will usually be split up into three independent groups: the fixed array (0-9), A/C and B/D.
+<P>
+<A NAME=.sensitivity><IMG ALIGN=MIDDLE SRC="../icons/invis_anchor.png"></A>  
+<H1><A NAME=SECTION0001000000000000000> <b>Sensitivity</b></A></H1>
+<P>
+The following tables gives WSRT interferometer system temperatures and sensitivities. The theoretical rms continuum sensitivity for 12 hrs observation is based on the given <IMG ALIGN=BOTTOM ALT="" SRC="_13438_tex2html_wrap215.png"> and maximum bandwidth.
+<P>
+<P><IMG ALIGN=BOTTOM ALT="" SRC="_13438_tabular117.png"><P>
+<P>
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+<P>.
+
+</BODY> </HTML> 
+<HR>
+
+</BODY>
+<P><ADDRESS>
+newstar@nfra.nl
diff --git a/xmosaic_restart.txt b/xmosaic_restart.txt
new file mode 100644
index 0000000000000000000000000000000000000000..6adc97a418cc72e412e0cdb63bcf2448e0e1831a
--- /dev/null
+++ b/xmosaic_restart.txt
@@ -0,0 +1,51 @@
+
+Xmosaic restart protocol
+========================
+
+	xmosaic is started by genaid.exe. genaid stores the pid of xmosaic in a
+file /tmp/xm-<display name>, where <display name> is derived from the
+environment variable DISPLAY by substituting a dot for each colon.
+
+	To access xmosaic from a parameter prompt in a Newstar program, PPDHELP
+call genmosaic.cun. The latter routine reads the file created by genaid to
+retrieve xmosaic's pid, <pid>. It then follows the protocol defined by xmosaic
+to access the appropriate help information in mosaic form:
+
+
+	1. Create a file /tmp/Mosaic.<pid>, containing the lines
+
+		goto
+		file://localhost/<directory>/file.html
+
+	2. Sending a SIGUSR1 signal to process <pid>.
+
+The latter signal causes xmosaic to opend the file /tmp/Mosaic.pid and act on
+its contents.
+
+
+Changes, early november 1994
+============================
+
+	Parameter .html files are now clustered in one .html file per .psc or
+.pef file. Finding the right target for display by mosaic requires some
+searching, which is done most easily in a .csh script:
+
+	set target = \
+	    `grep -l <Keyword> $n_hlp/intfc/<program>_private_intfc.psc`
+	if ($#target != 0) then
+	  set typ = 'private'
+	else
+	  set target = `grep -l <Keyword> $n_src/*/*.pef`
+	  if ($#target != 0) then
+	    set typ = 'public'
+	  else
+	    <emit error message>
+	endif
+	set label = `echo <keyword> sed -e 'y:A...Z_:a...z.:' `
+	echo 'goto' >! /tmp/Mosaic.<pid>
+	echo \
+"file://localhost$n_hlp/<pgm>_${typ}_intfc/<pgm>_${typ}_intfc.html#$target" \
+	  >> /tmp/Mosaic.<pid>
+	ln -s /tmp/Mosaic.<pid> /tmp/xmosaic.<pid>
+	kill -SIGUSR1 <pid>
+