diff --git a/lsmtool/lsmtool.py b/bin/lsmtool
similarity index 98%
rename from lsmtool/lsmtool.py
rename to bin/lsmtool
index fef041cba35a71599c03cb1b409856315801d25f..2af2dc54acfea22a9c59612ab3476c8744b71e7b 100755
--- a/lsmtool/lsmtool.py
+++ b/bin/lsmtool
@@ -26,10 +26,9 @@ import sys
import os
import time
import logging
-import _version
-import _logging
+import lsmtool
+# from lsmtool import _version, _logging, skymodel
import lofar.parameterset
-import skymodel
if __name__=='__main__':
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diff --git a/docs/build/html/_sources/lsmtool.operations.txt b/docs/build/html/_sources/lsmtool.operations.txt
new file mode 100644
index 0000000000000000000000000000000000000000..d0997457149b8e3c2b8fd69cfa4dbaab27f6225f
--- /dev/null
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@@ -0,0 +1,102 @@
+lsmtool.operations package
+==========================
+
+Submodules
+----------
+
+lsmtool.operations.add module
+-----------------------------
+
+.. automodule:: lsmtool.operations.add
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.concatenate module
+-------------------------------------
+
+.. automodule:: lsmtool.operations.concatenate
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.group module
+-------------------------------
+
+.. automodule:: lsmtool.operations.group
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.merge module
+-------------------------------
+
+.. automodule:: lsmtool.operations.merge
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.move module
+------------------------------
+
+.. automodule:: lsmtool.operations.move
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.plot module
+------------------------------
+
+.. automodule:: lsmtool.operations.plot
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.remove module
+--------------------------------
+
+.. automodule:: lsmtool.operations.remove
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.select module
+--------------------------------
+
+.. automodule:: lsmtool.operations.select
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.setpatchpositions module
+-------------------------------------------
+
+.. automodule:: lsmtool.operations.setpatchpositions
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.transfer module
+----------------------------------
+
+.. automodule:: lsmtool.operations.transfer
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.ungroup module
+---------------------------------
+
+.. automodule:: lsmtool.operations.ungroup
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+
+Module contents
+---------------
+
+.. automodule:: lsmtool.operations
+ :members:
+ :undoc-members:
+ :show-inheritance:
diff --git a/doc/source/lsmtool.rst b/docs/build/html/_sources/lsmtool.txt
similarity index 100%
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diff --git a/docs/build/html/_sources/modules.txt b/docs/build/html/_sources/modules.txt
new file mode 100644
index 0000000000000000000000000000000000000000..70163ca4a8240831a17002576f0786b7b12a7df7
--- /dev/null
+++ b/docs/build/html/_sources/modules.txt
@@ -0,0 +1,7 @@
+lsmtool
+=======
+
+.. toctree::
+ :maxdepth: 4
+
+ lsmtool
diff --git a/docs/build/html/_sources/overview.txt b/docs/build/html/_sources/overview.txt
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@@ -0,0 +1,283 @@
+LSMTool: the LOFAR Local Sky Model Tool
+=======================================
+
+LSMTool is a Python package which allows for the manipulation of sky
+models in the ``makesourcedb`` format (understood by BBS and NDPPP).
+Note that LSMTool is still in beta. Please report bugs to
+drafferty@hs.uni-hamburg.de. To initialize your environment for LSMTool,
+users on CEP1 and CEP2 should run the following commands:
+
+::
+
+ use LofIm
+ source ~rafferty/init_lsmtool
+
+Note that the Pythonlibs LOFAR package includes an older version of
+astropy that conflicts with LSMTool and cannot be used in conjunction
+with it.
+
+Usage
+-----
+
+The command-line version of LSMTool can be run as follows:
+
+::
+
+ Usage: lsmtool.py <skymodel> <parset> [<beam MS>]
+ Options:
+ --version show program's version number and exit
+ -h, --help show this help message and exit
+ -q Quiet
+ -v Verbose
+
+The parset specifies the operations to perform and their parameters.
+These are described in the next sections.
+
+.. _operations_defined:
+
+Operations
+----------
+
+These are the operations that LSMTool can perform:
+
+SELECT
+ : Select sources by source or patch properties
+
+REMOVE
+ : Remove sources by source or patch properties
+
+TRANSFER
+ : Transfer a patch scheme from one sky model to another
+
+GROUP
+ : Group sources into patches
+
+UNGROUP
+ : Remove patches
+
+MOVE
+ : Move a source or patch position
+
+MERGE
+ : Merge two or more patches into one
+
+CONCATENATE
+ : Concatenate two sky models
+
+ADD
+ : Add a source
+
+SETPATCHPOSITIONS
+ : Calculate and set patch positions
+
+PLOT
+ : Plot a simple representation of the sky model
+
+Example parset
+--------------
+
+This is an example parset that filters on the flux, adds a source, and
+then groups the sources into patches:
+
+::
+
+ LSMTool.Steps = [selectbright, addsrc, grp, setpos]
+
+ # Select only sources above 1 mJy
+ LSMTool.Steps.selectbright.Operation = SELECT
+ LSMTool.Steps.selectbright.FilterExpression = I > 1.0 mJy
+
+ # Add a source
+ LSMTool.Steps.addsrc.Name = new_source
+ LSMTool.Steps.addsrc.Type = POINT
+ LSMTool.Steps.addsrc.Ra = 277.4232
+ LSMTool.Steps.addsrc.Dec = 48.3689
+ LSMTool.Steps.addsrc.I = 0.69
+
+ # Group using tessellation to a target flux of 50 Jy
+ LSMTool.Steps.grp.Operation = GROUP
+ LSMTool.Steps.grp.Algorithm = tessellate
+ LSMTool.Steps.grp.TargetFlux = 50.0 Jy
+ LSMTool.Steps.grp.Method = mid
+
+ # Set the patch positions to their midpoint and write final skymodel
+ LSMTool.Steps.setpos.Method = mid
+ LSMTool.Steps.setpos.Outfile = grouped.sky
+
+In the first line of this parset the step names are defined. In the next
+sections, the step parameters for every step are defined. Steps are
+applied sequentially, in the same order defined in the list of steps. A
+list of step-specific parameters is given in
+Table [lsmtool:tab:local\ :sub:`v`\ al].
+
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Var Name | Format | Example | Comment |
++====================+=================+================+===============================================================+
+| Operation | string | SELECT | An operation name (see :ref:`operations_defined`) |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| OutFile | string | out.sky | Name of output file |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **SELECT and REMOVE** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| FilterExpression | string | I > 10.0 Jy | Filter for selection |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Aggregate | bool | False | Filter by aggregated patch property |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| ApplyBeam | bool | True | If true, apparent fluxes will be used |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **TRANSFER** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| PatchFile | string | patches.sky | File with patches that will be transferred |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **GROUP** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Algorithm | string | tessellate | One of tessellate, cluster, single, every |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| TargetFlux | string | 10.0 Jy | Target total flux of patches (tessellate only) |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| NumClusters | int | 100 | Number of clusters (cluster only) |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| ApplyBeam | bool | True | If true, apparent fluxes will be used |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **UNGROUP** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **MOVE** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Name | string | src1 | Name of source or patch to move |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Position | list of floats | [12.3, 23.4] | RA and Dec in degrees to move to |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Shift | list of floats | [0.001, 0.0] | RA and Dec in degrees to shift by |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **MERGE** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Patches | list of strings | [bin1, bin2] | Patch names to merge |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Name | string | merged\_patch | Name of new merged patch |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **SETPATCHPOSITIONS** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Method | string | mid | Set patch positions to mid, mean, or wmean positions |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **CONCATENATE** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Skymodel2 | string | in2.sky | Name of sky model to concatenate |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| MatchBy | string | position | Identify duplicates by position or name |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Radius | string | 30 arcsec | Radius within which matches are identified |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Keep | string | all | If two sources match, keep: all, from1, or from2 |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **ADD** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Name | string | src1 | Name of source; required |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Type | string | POINT | Type; required |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Patch | string | new\_patch | Patch name; required if sky model has patches |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| RA | float or string | 12:45:30.4 | RA; required |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| Dec | float or string | +76.45.02.48 | Dec; required |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| I | float | 0.69 | Flux in Jy; required |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| AnyValidColumnName | | value | Any valid column name can be specified |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+| **PLOT** |
++--------------------+-----------------+----------------+---------------------------------------------------------------+
+
+Interactive use and scripting
+-----------------------------
+
+LSMTool can also be used interactively (in IPython, for example) or in
+Python scripts without the need for a parset. To use LSMTool in a Python
+script or interpreter, import it as follows:
+
+::
+
+ >>> import lsmtool
+
+A sky model can then be loaded with, e.g.:
+
+::
+
+ >>> LSM = lsmtool.load('skymodel.sky')
+
+All of the operations described in Section [lsmtool:operations] are
+available as methods of the resulting sky model object (with the same
+name as the corresponding operation). For example, the following
+commands with duplicate the steps done in the example parset given in
+Section [lsmtool:parset]:
+
+::
+
+ >>> LSM.select('I > 1.0 mJy')
+ >>> LSM.add({'Name':'new_source', 'Type':'POINT', 'Ra':277.4232, 'Dec':48.3689, 'I':0.69})
+ >>> LSM.group(algorithm='tesselate', targetFlux='10.0 Jy')
+ >>> LSM.setPatchPositions(method='mid')
+
+In many cases, the methods accept parameters with the same names as
+those used in a parset (see the full documentation for details). The sky
+model can then written to a new file with:
+
+::
+
+ >>> LSM.write('grouped.sky')
+
+Additionally, sky models can be written out as ds9 region files and kvis
+annotation files (as well as all the formats supported by the
+astropy.table package, such at VOTable, HDF5, and FITS):
+
+::
+
+ >>> LSM.write('outskymodel.reg', format='ds9')
+ >>> LSM.write('outskymodel.ann', format='kvis')
+ >>> LSM.write('outskymodel.fits', format='fits')
+ >>> LSM.write('outskymodel.hdf5', format='hdf5')
+ >>> LSM.write('outskymodel.vo', format='votable')
+
+In addition to the operations described above, a number of other methods
+are available:
+
+LSM.copy()
+ : Return a copy of the sky model object
+
+LSM.info()
+ : Print information about the sky model
+
+LSM.more()
+ : Print the sky model to the screen, using more-like controls
+
+LSM.getColNames()
+ : Returns a list of the column names in the sky model
+
+LSM.getColValues()
+ : Returns a numpy array of column values
+
+LSM.getRowIndex()
+ : Returns the row index or indices for a source or patch
+
+LSM.getRowValues()
+ : Returns a table or row for a source or patch
+
+LSM.getPatchPositions()
+ : Returns patch RA and Dec values
+
+LSM.getDefaltValues()
+ : Returns column default values
+
+LSM.getPatchSizes()
+ : Returns an array of patch sizes
+
+LSM.setColValues()
+ : Sets column values
+
+LSM.setRowValues()
+ : Sets row values
+
+LSM.setDefaultValues()
+ : Sets default column values
+
+For details on these methods, please see the full module documentation.
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@@ -0,0 +1,1431 @@
+<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Transitional//EN"
+ "http://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd">
+
+
+<html xmlns="http://www.w3.org/1999/xhtml">
+ <head>
+ <meta http-equiv="Content-Type" content="text/html; charset=utf-8" />
+
+ <title>LSMTool Module Documentation — LSMTool 1.0.0 documentation</title>
+
+ <link rel="stylesheet" href="_static/default.css" type="text/css" />
+ <link rel="stylesheet" href="_static/pygments.css" type="text/css" />
+
+ <script type="text/javascript">
+ var DOCUMENTATION_OPTIONS = {
+ URL_ROOT: './',
+ VERSION: '1.0.0',
+ COLLAPSE_INDEX: false,
+ FILE_SUFFIX: '.html',
+ HAS_SOURCE: true
+ };
+ </script>
+ <script type="text/javascript" src="_static/jquery.js"></script>
+ <script type="text/javascript" src="_static/underscore.js"></script>
+ <script type="text/javascript" src="_static/doctools.js"></script>
+ <script type="text/javascript" src="http://cdn.mathjax.org/mathjax/latest/MathJax.js?config=TeX-AMS-MML_HTMLorMML"></script>
+ <link rel="top" title="LSMTool 1.0.0 documentation" href="index.html" />
+ <link rel="prev" title="LSMTool: the LOFAR Local Sky Model Tool" href="overview.html" />
+ </head>
+ <body>
+ <div class="related">
+ <h3>Navigation</h3>
+ <ul>
+ <li class="right" style="margin-right: 10px">
+ <a href="genindex.html" title="General Index"
+ accesskey="I">index</a></li>
+ <li class="right" >
+ <a href="py-modindex.html" title="Python Module Index"
+ >modules</a> |</li>
+ <li class="right" >
+ <a href="overview.html" title="LSMTool: the LOFAR Local Sky Model Tool"
+ accesskey="P">previous</a> |</li>
+ <li><a href="index.html">LSMTool 1.0.0 documentation</a> »</li>
+ </ul>
+ </div>
+
+ <div class="document">
+ <div class="documentwrapper">
+ <div class="bodywrapper">
+ <div class="body">
+
+ <div class="section" id="lsmtool-module-documentation">
+<h1>LSMTool Module Documentation<a class="headerlink" href="#lsmtool-module-documentation" title="Permalink to this headline">¶</a></h1>
+<div class="toctree-wrapper compound">
+<ul class="simple">
+</ul>
+</div>
+<div class="section" id="module-lsmtool">
+<span id="lsmtool-module"></span><h2>lsmtool module<a class="headerlink" href="#module-lsmtool" title="Permalink to this headline">¶</a></h2>
+<p>The load() convenience function is used to load a sky model file into a
+SkyModel object.</p>
+<dl class="function">
+<dt id="lsmtool.load">
+<tt class="descclassname">lsmtool.</tt><tt class="descname">load</tt><big>(</big><em>fileName</em>, <em>beamMS=None</em><big>)</big><a class="headerlink" href="#lsmtool.load" title="Permalink to this definition">¶</a></dt>
+<dd><p>Loads a sky model from a file and returns a SkyModel object.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>fileName</strong> : str</p>
+<blockquote>
+<div><p>Input ASCII file from which the sky model is read. Must
+respect the makesourcedb format</p>
+</div></blockquote>
+<p><strong>beamMS</strong> : str, optional</p>
+<blockquote>
+<div><p>Measurement set from which the primary beam will be estimated. A
+column of attenuated Stokes I fluxes will be added to the table.</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first">SkyModel object</p>
+<blockquote class="last">
+<div><p>A SkyModel object that stores the sky model and provides methods for
+accessing it.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Load a sky model into a SkyModel object:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="kn">import</span> <span class="nn">lsmtool</span>
+<span class="gp">>>> </span><span class="n">s</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Load a sky model with a beam MS so that apparent fluxes will
+be available (in addition to intrinsic fluxes):</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">,</span> <span class="s">'SB100.MS'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations_lib">
+<span id="lsmtool-operations-lib-module"></span><h2>lsmtool.operations_lib module<a class="headerlink" href="#module-lsmtool.operations_lib" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations_lib.attenuate">
+<tt class="descclassname">lsmtool.operations_lib.</tt><tt class="descname">attenuate</tt><big>(</big><em>beamMS</em>, <em>fluxes</em>, <em>RADeg</em>, <em>DecDeg</em><big>)</big><a class="headerlink" href="#lsmtool.operations_lib.attenuate" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns flux attenuated by primary beam.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>beamMS</strong> : str</p>
+<blockquote>
+<div><p>Measurement set for which the beam model is made</p>
+</div></blockquote>
+<p><strong>fluxes</strong> : list</p>
+<blockquote>
+<div><p>List of fluxes to attenuate</p>
+</div></blockquote>
+<p><strong>RADeg</strong> : list</p>
+<blockquote>
+<div><p>List of RA values in degrees</p>
+</div></blockquote>
+<p><strong>DecDeg</strong> : list</p>
+<blockquote>
+<div><p>List of Dec values in degrees</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first last"><strong>attFluxes</strong> : numpy array</p>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations_lib.radec2xy">
+<tt class="descclassname">lsmtool.operations_lib.</tt><tt class="descname">radec2xy</tt><big>(</big><em>RA</em>, <em>Dec</em>, <em>refRA=None</em>, <em>refDec=None</em><big>)</big><a class="headerlink" href="#lsmtool.operations_lib.radec2xy" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns x, y for input ra, dec.</p>
+<p>Note that the reference RA and Dec must be the same in calls to both
+radec2xy() and xy2radec() if matched pairs of (x, y) <=> (RA, Dec) are
+desired.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>RA</strong> : list</p>
+<blockquote>
+<div><p>List of RA values in degrees</p>
+</div></blockquote>
+<p><strong>Dec</strong> : list</p>
+<blockquote>
+<div><p>List of Dec values in degrees</p>
+</div></blockquote>
+<p><strong>refRA</strong> : float, optional</p>
+<blockquote>
+<div><p>Reference RA in degrees.</p>
+</div></blockquote>
+<p><strong>refDec</strong> : float, optional</p>
+<blockquote>
+<div><p>Reference Dec in degrees</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first"><strong>x, y</strong> : list, list</p>
+<blockquote class="last">
+<div><p>Lists of x and y pixel values corresponding to the input RA and Dec
+values</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations_lib.xy2radec">
+<tt class="descclassname">lsmtool.operations_lib.</tt><tt class="descname">xy2radec</tt><big>(</big><em>x</em>, <em>y</em>, <em>refRA=0.0</em>, <em>refDec=0.0</em><big>)</big><a class="headerlink" href="#lsmtool.operations_lib.xy2radec" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns x, y for input ra, dec.</p>
+<p>Note that the reference RA and Dec must be the same in calls to both
+radec2xy() and xy2radec() if matched pairs of (x, y) <=> (RA, Dec) are
+desired.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>x</strong> : list</p>
+<blockquote>
+<div><p>List of x values in pixels</p>
+</div></blockquote>
+<p><strong>y</strong> : list</p>
+<blockquote>
+<div><p>List of y values in pixels</p>
+</div></blockquote>
+<p><strong>refRA</strong> : float, optional</p>
+<blockquote>
+<div><p>Reference RA in degrees</p>
+</div></blockquote>
+<p><strong>refDec</strong> : float, optional</p>
+<blockquote>
+<div><p>Reference Dec in degrees</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first"><strong>RA, Dec</strong> : list, list</p>
+<blockquote class="last">
+<div><p>Lists of RA and Dec values corresponding to the input x and y pixel
+values</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.skymodel">
+<span id="lsmtool-skymodel-module"></span><h2>lsmtool.skymodel module<a class="headerlink" href="#module-lsmtool.skymodel" title="Permalink to this headline">¶</a></h2>
+<dl class="class">
+<dt id="lsmtool.skymodel.SkyModel">
+<em class="property">class </em><tt class="descclassname">lsmtool.skymodel.</tt><tt class="descname">SkyModel</tt><big>(</big><em>fileName</em>, <em>beamMS=None</em>, <em>checkDup=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel" title="Permalink to this definition">¶</a></dt>
+<dd><p>Bases: <tt class="xref py py-class docutils literal"><span class="pre">object</span></tt></p>
+<p>Object that stores the sky model and provides methods for accessing it.</p>
+<p class="rubric">Methods</p>
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.add">
+<tt class="descname">add</tt><big>(</big><em>colNamesVals</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.add" title="Permalink to this definition">¶</a></dt>
+<dd><p>Add a source to the sky model.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>colNamesVals</strong> : dict</p>
+<blockquote class="last">
+<div><p>A dictionary that specifies the row values for the source to be added.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.concatenate">
+<tt class="descname">concatenate</tt><big>(</big><em>LSM2</em>, <em>matchBy='name'</em>, <em>radius=0.1</em>, <em>keep='all'</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.concatenate" title="Permalink to this definition">¶</a></dt>
+<dd><p>Concatenate two sky models.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>LSM2</strong> : SkyModel object</p>
+<blockquote>
+<div><p>Sky model to concatenate with the parent sky model</p>
+</div></blockquote>
+<p><strong>matchBy</strong> : str, optional</p>
+<blockquote>
+<div><p>Determines how duplicate sources are determined:
+- ‘name’ => duplicates are identified by name
+- ‘position’ => duplicates are identified by radius. Sources within the</p>
+<blockquote>
+<div><p>radius specified by the radius parameter are considered duplicates</p>
+</div></blockquote>
+</div></blockquote>
+<p><strong>radius</strong> : float, optional</p>
+<blockquote>
+<div><p>Radius in degrees for matching when matchBy=’position’</p>
+</div></blockquote>
+<p><strong>keep</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>Determines how duplicates are treated:
+- ‘all’ => all duplicates are kept; those with identical names are re-</p>
+<blockquote>
+<div><p>named</p>
+</div></blockquote>
+<ul class="simple">
+<li>‘from1’ => duplicates kept are those from sky model 1 (the parent)</li>
+<li>‘from2’ => duplicates kept are those from sky model 2 (LSM2)</li>
+</ul>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Concatenate two sky models, identifying duplicates by matching to the source
+names. When duplicates are found, keep the source from the parent sky model
+and discard the duplicate from second sky model (this might be useful when
+merging two gsm.py sky models that have some overlap):</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM2</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'gsm_sky2.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">concatenate</span><span class="p">(</span><span class="n">LSM2</span><span class="p">,</span> <span class="n">matchBy</span><span class="o">=</span><span class="s">'name'</span><span class="p">,</span> <span class="n">keep</span><span class="o">=</span><span class="s">'from1'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Concatenate two sky models, identifying duplicates by matching to the source
+positions within a radius of 10 arcsec. When duplicates are found, keep the
+source from the second sky model and discard the duplicate from the parent
+sky model (this might be useful when replacing parts of a low-resolution
+sky model with a high-resolution one):</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM2</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'high_res_sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">concatenate</span><span class="p">(</span><span class="n">LSM2</span><span class="p">,</span> <span class="n">matchBy</span><span class="o">=</span><span class="s">'position'</span><span class="p">,</span> <span class="n">radius</span><span class="o">=</span><span class="mf">10.0</span><span class="o">/</span><span class="mf">3600.0</span><span class="p">,</span>
+<span class="go"> keep='from2')</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.copy">
+<tt class="descname">copy</tt><big>(</big><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.copy" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns a copy of the sky model.</p>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getColNames">
+<tt class="descname">getColNames</tt><big>(</big><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getColNames" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns a list of all available column names.</p>
+<p class="rubric">Examples</p>
+<p>Get column names:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getColNames</span><span class="p">()</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getColValues">
+<tt class="descname">getColValues</tt><big>(</big><em>colName</em>, <em>units=None</em>, <em>aggregate=None</em>, <em>applyBeam=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getColValues" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns a numpy array of column values.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>colName</strong> : str</p>
+<blockquote>
+<div><p>Name of column</p>
+</div></blockquote>
+<p><strong>units</strong> : str, optional</p>
+<blockquote>
+<div><p>Output units (the values are converted as needed). By default, the
+units are those used by makesourcedb, with the exception of Ra and
+Dec which have default units of degrees.</p>
+</div></blockquote>
+<p><strong>aggregate</strong> : {‘sum’, ‘mean’, ‘wmean’, ‘min’, max’}, optional</p>
+<blockquote>
+<div><p>If set, the array returned will be of values aggregated
+over the patch members. The following aggregation functions are
+available:</p>
+<blockquote>
+<div><ul class="simple">
+<li>‘sum’: sum of patch values</li>
+<li>‘mean’: mean of patch values</li>
+<li>‘wmean’: Stokes I weighted mean of patch values</li>
+<li>‘min’: minimum of patch values</li>
+<li>‘max’: maximum of patch values</li>
+</ul>
+</div></blockquote>
+<p>Note that, in certain cases, certain aggregation functions will not
+produce meaningful results. For example, asking for the sum of
+the MajorAxis values per patch will not give a good indication of
+the size of the patch (to get the sizes, use the getPatchSizes()
+method). Additionally, applying the ‘mean’ or ‘wmean’ functions to
+the RA or Dec columns may give strange results near the poles or
+near RA = 0h. For aggregated RA and Dec values, use the
+getPatchPositions() method instead which projects the sources onto
+the image plane before aggregation.</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, fluxes will be attenuated by the beam. This attenuation
+also applies to fluxes used in aggregation functions.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Get Stokes I fluxes in Jy:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getColValues</span><span class="p">(</span><span class="s">'I'</span><span class="p">)</span>
+<span class="go">array([ 60.4892, 1.2413, 1.216 , ..., 1.12 , 1.25 , 1.16 ])</span>
+</pre></div>
+</div>
+<p>Get Stokes I fluxes in mJy:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getColValues</span><span class="p">(</span><span class="s">'I'</span><span class="p">,</span> <span class="n">units</span><span class="o">=</span><span class="s">'mJy'</span><span class="p">)</span>
+<span class="go">array([ 60489.2, 1241.3, 1216. , ..., 1120. , 1250. , 1160. ])</span>
+</pre></div>
+</div>
+<p>Get total Stokes I flux for the patches:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getColValues</span><span class="p">(</span><span class="s">'I'</span><span class="p">,</span> <span class="n">aggregate</span><span class="o">=</span><span class="s">'sum'</span><span class="p">)</span>
+<span class="go">array([ 61.7305, 1.216 , 3.9793, ..., 1.12 , 1.25 , 1.16 ])</span>
+</pre></div>
+</div>
+<p>Get flux-weighted average RA and Dec for the patches. As noted above, the
+getColValues() method is not appropriate for use with RA or Dec, so
+we must use getPatchPositions() instead:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">RA</span><span class="p">,</span> <span class="n">Dec</span> <span class="o">=</span> <span class="n">s</span><span class="o">.</span><span class="n">getPatchPositions</span><span class="p">(</span><span class="n">method</span><span class="o">=</span><span class="s">'wmean'</span><span class="p">,</span> <span class="n">asArray</span><span class="o">=</span><span class="bp">True</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getDefaltValues">
+<tt class="descname">getDefaltValues</tt><big>(</big><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getDefaltValues" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns dict of {colName:default} values for all columns with defaults.</p>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getPatchNames">
+<tt class="descname">getPatchNames</tt><big>(</big><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getPatchNames" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns array of all patch names in the sky model.</p>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getPatchPositions">
+<tt class="descname">getPatchPositions</tt><big>(</big><em>patchName=None</em>, <em>asArray=False</em>, <em>method=None</em>, <em>applyBeam=False</em>, <em>perPatchProjection=True</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getPatchPositions" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns arrays or a dict of patch positions (as {‘patchName’:(RA, Dec)}).</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>patchName</strong> : str or list, optional</p>
+<blockquote>
+<div><p>List of patch names for which the positions are desired</p>
+</div></blockquote>
+<p><strong>asArray</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, returns arrays of RA, Dec instead of a dict</p>
+</div></blockquote>
+<p><strong>method</strong> : None or str, optional</p>
+<blockquote>
+<div><p>This parameter specifies the method used to calculate the patch
+positions. If None, the current patch positions stored in the sky
+model, if any, will be returned.
+- ‘mid’ => calculate the midpoint of the patch
+- ‘mean’ => calculate the mean RA and Dec of the patch
+- ‘wmean’ => calculate the flux-weighted mean RA and Dec of the patch
+- None => current patch positions are returned
+Note that the mid, mean, and wmean positions are calculated from TAN-
+projected values.</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, fluxes used as weights will be attenuated by the beam.</p>
+</div></blockquote>
+<p><strong>perPatchProjection</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, a different projection center is used per patch. If False,
+a single projection center is used for all patches.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Get the current patch positions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getPatchPositions</span><span class="p">()</span>
+<span class="go">{'bin0': [<Angle 91.77565208333331 deg>, <Angle 41.57834805555555 deg>],</span>
+<span class="go"> 'bin1': [<Angle 91.59991874999997 deg>, <Angle 41.90387583333333 deg>],</span>
+<span class="go"> 'bin2': [<Angle 90.83773333333332 deg>, <Angle 42.189861944444445 deg>],</span>
+</pre></div>
+</div>
+<p>Get them as RA and Dec arrays in degrees:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getPatchPositions</span><span class="p">(</span><span class="n">asArray</span><span class="o">=</span><span class="bp">True</span><span class="p">)</span>
+<span class="go">(array([ 91.77565208, 91.59991875, 90.83773333]),</span>
+<span class="go"> array([ 41.57834806, 41.90387583, 42.18986194]))</span>
+</pre></div>
+</div>
+<p>Calculate the flux-weighted mean positions of each patch:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getPatchPositions</span><span class="p">(</span><span class="n">method</span><span class="o">=</span><span class="s">'wmean'</span><span class="p">,</span> <span class="n">asArray</span><span class="o">=</span><span class="bp">True</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getPatchSizes">
+<tt class="descname">getPatchSizes</tt><big>(</big><em>units=None</em>, <em>weight=False</em>, <em>applyBeam=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getPatchSizes" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns array of patch sizes.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>units</strong> : str, optional</p>
+<blockquote>
+<div><p>Units for returned sizes (e.g., ‘arcsec’, ‘degree’)</p>
+</div></blockquote>
+<p><strong>weight</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, weight the source positions inside the patch by flux</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True and weight is True, attenuate the fluxes used for weighting
+by the beam</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getRowIndex">
+<tt class="descname">getRowIndex</tt><big>(</big><em>rowName</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getRowIndex" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns index or indices for specified source or patch as a list.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>rowName</strong> : str</p>
+<blockquote class="last">
+<div><p>Name of the source or patch</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Get row index for the source ‘src1’:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">getRowIndex</span><span class="p">(</span><span class="s">'src1'</span><span class="p">)</span>
+<span class="go">[0]</span>
+</pre></div>
+</div>
+<p>Get row indices for the patch ‘bin1’ and verify the patch name:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">ind</span> <span class="o">=</span> <span class="n">s</span><span class="o">.</span><span class="n">getRowIndex</span><span class="p">(</span><span class="s">'bin1'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="k">print</span><span class="p">(</span><span class="n">s</span><span class="o">.</span><span class="n">getPatchNames</span><span class="p">()[</span><span class="n">ind</span><span class="p">])</span>
+<span class="go">['bin1' 'bin1']</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.getRowValues">
+<tt class="descname">getRowValues</tt><big>(</big><em>rowName</em>, <em>colName=None</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.getRowValues" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns an astropy table or table row for specified source or patch.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>rowName</strong> : str</p>
+<blockquote>
+<div><p>Name of the source or patch</p>
+</div></blockquote>
+<p><strong>colName</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>Column name. If given, returns row values for specified
+column only.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Get row values for the source ‘src1’:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">r</span> <span class="o">=</span> <span class="n">s</span><span class="o">.</span><span class="n">getRowValues</span><span class="p">(</span><span class="s">'src1'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Sum over the fluxes of sources in the ‘bin1’ patch:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">rows</span> <span class="o">=</span> <span class="n">s</span><span class="o">.</span><span class="n">getRowValues</span><span class="p">(</span><span class="s">'bin1'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">tot</span> <span class="o">=</span> <span class="mf">0.0</span>
+<span class="gp">>>> </span><span class="k">for</span> <span class="n">r</span> <span class="ow">in</span> <span class="n">rows</span><span class="p">:</span> <span class="n">tot</span> <span class="o">+=</span> <span class="n">r</span><span class="p">[</span><span class="s">'I'</span><span class="p">]</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.group">
+<tt class="descname">group</tt><big>(</big><em>algorithm</em>, <em>targetFlux=None</em>, <em>numClusters=100</em>, <em>applyBeam=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.group" title="Permalink to this definition">¶</a></dt>
+<dd><p>Groups sources into patches.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>LSM</strong> : SkyModel object</p>
+<blockquote>
+<div><p>Input sky model.</p>
+</div></blockquote>
+<p><strong>algorithm</strong> : str</p>
+<blockquote>
+<div><p>Algorithm to use for grouping:
+- ‘single’ => all sources are grouped into a single patch
+- ‘every’ => every source gets a separate patch
+- ‘cluster’ => SAGECAL clustering algorithm that groups sources into</p>
+<blockquote>
+<div><p>specified number of clusters (specified by the numClusters parameter).</p>
+</div></blockquote>
+<ul>
+<li><dl class="first docutils">
+<dt>‘tessellate’ => group into tiles whose total flux approximates</dt>
+<dd><p class="first last">the target flux (specified by the targetFlux parameter).</p>
+</dd>
+</dl>
+</li>
+<li><dl class="first docutils">
+<dt>the filename of a mask image => group by masked regions (where mask =</dt>
+<dd><p class="first last">True). Source outside of masked regions are given patches of their
+own.</p>
+</dd>
+</dl>
+</li>
+</ul>
+</div></blockquote>
+<p><strong>targetFlux</strong> : str or float, optional</p>
+<blockquote>
+<div><p>Target flux for tessellation (the total flux of each tile will be close
+to this value). The target flux can be specified as either a float in Jy
+or as a string with units (e.g., ‘25.0 mJy’).</p>
+</div></blockquote>
+<p><strong>numClusters</strong> : int, optional</p>
+<blockquote>
+<div><p>Number of clusters for clustering. Sources are grouped around the
+numClusters brightest sources.</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, fluxes will be attenuated by the beam.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Tesselate the sky model into patches with approximately 30 Jy total
+flux:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">group</span><span class="p">(</span><span class="s">'tessellate'</span><span class="p">,</span> <span class="n">targetFlux</span><span class="o">=</span><span class="mf">30.0</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.info">
+<tt class="descname">info</tt><big>(</big><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.info" title="Permalink to this definition">¶</a></dt>
+<dd><p>Prints information about the sky model.</p>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.merge">
+<tt class="descname">merge</tt><big>(</big><em>patches</em>, <em>name=None</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.merge" title="Permalink to this definition">¶</a></dt>
+<dd><p>Merge two or more patches together.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>patches</strong> : list of str</p>
+<blockquote>
+<div><p>List of patches to merge</p>
+</div></blockquote>
+<p><strong>name</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>Name of resulting merged patch</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Merge three patches into one:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">merge</span><span class="p">([</span><span class="s">'bin0'</span><span class="p">,</span> <span class="s">'bin1'</span><span class="p">,</span> <span class="s">'bin2'</span><span class="p">],</span> <span class="s">'binmerged'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.more">
+<tt class="descname">more</tt><big>(</big><em>colName=None</em>, <em>patchName=None</em>, <em>sourceName=None</em>, <em>sortBy=None</em>, <em>lowToHigh=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.more" title="Permalink to this definition">¶</a></dt>
+<dd><p>Prints the sky model table to the screen with more-like commands.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>colName</strong> : str, list of str, optional</p>
+<blockquote>
+<div><p>Name of column or columns to print. If None, all columns are printed</p>
+</div></blockquote>
+<p><strong>patchName</strong> : str, list of str, optional</p>
+<blockquote>
+<div><p>If given, returns column values for specified patch or patches only</p>
+</div></blockquote>
+<p><strong>sourceName</strong> : str, list of str, optional</p>
+<blockquote>
+<div><p>If given, returns column value for specified source or sources only</p>
+</div></blockquote>
+<p><strong>sortBy</strong> : str or list of str, optional</p>
+<blockquote>
+<div><p>Name of columns to sort on. If None, no sorting is done. If
+a list is given, sorting is done on the columns in the order given</p>
+</div></blockquote>
+<p><strong>lowToHigh</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, sort values from low to high instead of high to low</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Print the entire model:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">more</span><span class="p">()</span>
+</pre></div>
+</div>
+<p>Print only the ‘Name’ and ‘I’ columns for the ‘bin0’ patch:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">more</span><span class="p">([</span><span class="s">'Name'</span><span class="p">,</span> <span class="s">'I'</span><span class="p">],</span> <span class="s">'bin0'</span><span class="p">,</span> <span class="n">sortBy</span><span class="o">=</span><span class="p">[</span><span class="s">'I'</span><span class="p">])</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.move">
+<tt class="descname">move</tt><big>(</big><em>name</em>, <em>position=None</em>, <em>shift=None</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.move" title="Permalink to this definition">¶</a></dt>
+<dd><p>Move or shift a source.</p>
+<p>If both a position and a shift are specified, the source is moved to the
+new position and then shifted.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>name</strong> : str</p>
+<blockquote>
+<div><p>Source name.</p>
+</div></blockquote>
+<p><strong>position</strong> : list, optional</p>
+<blockquote>
+<div><p>A list specifying a new position as [RA, Dec] in either makesourcedb
+format (e.g., [‘12:23:43.21’, ‘+22.34.21.2’]) or in degrees (e.g.,
+[123.2312, 23.3422]).</p>
+</div></blockquote>
+<p><strong>shift</strong> : list, optional</p>
+<blockquote class="last">
+<div><p>A list specifying the shift as [RAShift, DecShift] in
+in degrees (e.g., [0.02312, 0.00342]).</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Move source ‘1609.6+6556’ to a new position:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">move</span><span class="p">(</span><span class="s">'1609.6+6556'</span><span class="p">,</span> <span class="n">position</span><span class="o">=</span><span class="p">[</span><span class="s">'16:10:00'</span><span class="p">,</span> <span class="s">'+65.57.00'</span><span class="p">])</span>
+</pre></div>
+</div>
+<p>Shift the source by 10 arcsec in Dec:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">move</span><span class="p">(</span><span class="s">'1609.6+6556'</span><span class="p">,</span> <span class="n">shift</span><span class="o">=</span><span class="p">[</span><span class="mf">0.0</span><span class="p">,</span> <span class="mf">10.0</span><span class="o">/</span><span class="mf">3600.0</span><span class="p">])</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.plot">
+<tt class="descname">plot</tt><big>(</big><em>fileName=None</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.plot" title="Permalink to this definition">¶</a></dt>
+<dd><p>Shows a simple plot of the sky model.</p>
+<p>The circles in the plot are scaled with flux. If the sky model is grouped
+into patches, sources are colored by patch and the patch positions are
+indicated with stars.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>fileName</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>If given, the plot is saved to a file instead of displayed.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.remove">
+<tt class="descname">remove</tt><big>(</big><em>filterExpression</em>, <em>aggregate=None</em>, <em>applyBeam=None</em>, <em>useRegEx=False</em>, <em>force=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.remove" title="Permalink to this definition">¶</a></dt>
+<dd><p>Filters the sky model, removing all sources that meet the given expression.</p>
+<p>After filtering, the sky model contains only those sources for which the
+given filter expression is false.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>filterExpression</strong> : str or dict</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>A string specifying the filter expression in the form:</dt>
+<dd><p class="first last">‘<property> <operator> <value> [<units>]’</p>
+</dd>
+</dl>
+<p>(e.g., ‘I <= 10.5 Jy’). These elements can also be given as a
+dictionary in the form:</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>{‘filterProp’:property, ‘filterOper’:operator,</dt>
+<dd><p class="first last">‘filterVal’:value, ‘filterUnits’:units}</p>
+</dd>
+</dl>
+</div></blockquote>
+<dl class="docutils">
+<dt>or as a list:</dt>
+<dd><p class="first last">[property, operator, value, value]</p>
+</dd>
+</dl>
+<p>The property to filter on must be a valid column name or the filename
+of a mask image.</p>
+<p>Supported operators are:
+- !=
+- <=
+- >=
+- >
+- <
+- = (or ‘==’)</p>
+<p>Units are optional and must be specified as required by astropy.units.</p>
+</div></blockquote>
+<p><strong>aggregate</strong> : str, optional</p>
+<blockquote>
+<div><p>If set, the array returned will be of values aggregated
+over the patch members. The following aggregation functions are
+available:
+- ‘sum’: sum of patch values
+- ‘mean’: mean of patch values
+- ‘wmean’: Stokes I weighted mean of patch values
+- ‘min’: minimum of patch values
+- ‘max’: maximum of patch values
+- True: only valid when the filter indices are specified directly as
+a numpy array. If True, filtering is done on patches instead of
+sources.</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, apparent fluxes will be used.</p>
+</div></blockquote>
+<p><strong>useRegEx</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, string matching will use regular expression matching. If
+False, string matching uses Unix filename matching.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Filter on column ‘I’ (Stokes I flux). This filter will remove all sources
+with Stokes I flux greater than 1.5 Jy:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">remove</span><span class="p">(</span><span class="s">'I > 1.5 Jy'</span><span class="p">)</span>
+<span class="go">INFO: Removed 1102 sources.</span>
+</pre></div>
+</div>
+<p>If the sky model has patches and the filter is desired per patch, use
+<tt class="docutils literal"><span class="pre">aggregate</span> <span class="pre">=</span> <span class="pre">function</span></tt>. For example, to select on the sum of the patch
+fluxes:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">remove</span><span class="p">(</span><span class="s">'I > 1.5 Jy'</span><span class="p">,</span> <span class="n">aggregate</span><span class="o">=</span><span class="s">'sum'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Filter on source names, removing those that match “src*_1?”:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">remove</span><span class="p">(</span><span class="s">'Name == src*_1?'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Use a CASA clean mask image to remove sources that lie in masked regions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">remove</span><span class="p">(</span><span class="s">'clean_mask.mask == True'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.select">
+<tt class="descname">select</tt><big>(</big><em>filterExpression</em>, <em>aggregate=None</em>, <em>applyBeam=False</em>, <em>useRegEx=False</em>, <em>force=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.select" title="Permalink to this definition">¶</a></dt>
+<dd><p>Filters the sky model, keeping all sources that meet the given expression.</p>
+<p>After filtering, the sky model contains only those sources for which the
+given filter expression is true.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>filterExpression</strong> : str or dict</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>The filter expression specified as:</dt>
+<dd><ul class="first last simple">
+<li>a string of <tt class="docutils literal"><span class="pre">'<property></span> <span class="pre"><operator></span> <span class="pre"><value></span> <span class="pre">[<units>]'</span></tt></li>
+<li>a list of <tt class="docutils literal"><span class="pre">[property,</span> <span class="pre">operator,</span> <span class="pre">value,</span> <span class="pre">unit]</span></tt></li>
+</ul>
+</dd>
+</dl>
+<p>The property to filter on must be a valid column name or the filename
+of a mask image.</p>
+<dl class="docutils">
+<dt>Supported operators are:</dt>
+<dd><ul class="first last simple">
+<li>!=</li>
+<li><=</li>
+<li>>=</li>
+<li>></li>
+<li><</li>
+<li>= (or ‘==’)</li>
+</ul>
+</dd>
+</dl>
+<p>Units are optional and must be specified as required by astropy.units.</p>
+</div></blockquote>
+<p><strong>aggregate</strong> : str, optional</p>
+<blockquote>
+<div><p>If set, the array returned will be of values aggregated
+over the patch members. The following aggregation functions are
+available:</p>
+<blockquote>
+<div><ul class="simple">
+<li>‘sum’: sum of patch values</li>
+<li>‘mean’: mean of patch values</li>
+<li>‘wmean’: Stokes I weighted mean of patch values</li>
+<li>‘min’: minimum of patch values</li>
+<li>‘max’: maximum of patch values</li>
+<li>True: only valid when the filter indices are specify directly as a numpy array. If True, filtering is done on patches instead of sources.</li>
+</ul>
+</div></blockquote>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, apparent fluxes will be used.</p>
+</div></blockquote>
+<p><strong>useRegEx</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, string matching will use regular expression matching. If
+False, string matching uses Unix filename matching.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Filter on column ‘I’ (Stokes I flux). This filter will select all sources
+with Stokes I flux greater than 1.5 Jy:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">select</span><span class="p">(</span><span class="s">'I > 1.5 Jy'</span><span class="p">)</span>
+<span class="go">INFO: Kept 1102 sources.</span>
+</pre></div>
+</div>
+<p>If the sky model has patches and the filter is desired per patch, use
+<tt class="docutils literal"><span class="pre">aggregate</span> <span class="pre">=</span> <span class="pre">function</span></tt>. For example, to select on the sum of the patch
+fluxes:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">select</span><span class="p">(</span><span class="s">'I > 1.5 Jy'</span><span class="p">,</span> <span class="n">aggregate</span><span class="o">=</span><span class="s">'sum'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Filter on source names, keeping those that match “src*_1?”:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">select</span><span class="p">(</span><span class="s">'Name == src*_1?'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Use a CASA clean mask image to keep sources that lie in masked regions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">filter</span><span class="p">(</span><span class="s">'clean_mask.mask == True'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.setColValues">
+<tt class="descname">setColValues</tt><big>(</big><em>colName</em>, <em>values</em>, <em>mask=None</em>, <em>index=None</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.setColValues" title="Permalink to this definition">¶</a></dt>
+<dd><p>Sets column values.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>colName</strong> : str</p>
+<blockquote>
+<div><p>Name of column. If not already present in the table, a new column
+will be created.</p>
+</div></blockquote>
+<p><strong>values</strong> : list, numpy array, or dict</p>
+<blockquote>
+<div><p>Array of values or dict of {sourceName:value} pairs. If list or
+array, the length must match the number of rows in the table. If
+dict, missing values will be masked unless already present. Values
+are assumed to be in units required by makesourcedb.</p>
+</div></blockquote>
+<p><strong>mask</strong> : list or array of bools, optional</p>
+<blockquote>
+<div><p>If values is a list or array, a mask can be specified (True means
+the value is masked).</p>
+</div></blockquote>
+<p><strong>index</strong> : int, optional</p>
+<blockquote class="last">
+<div><p>Index that specifies the column position in the table, if column is
+not already present in the table</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Set Stokes I fluxes:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setColValues</span><span class="p">(</span><span class="s">'I'</span><span class="p">,</span> <span class="p">[</span><span class="mf">1.0</span><span class="p">,</span> <span class="mf">1.1</span><span class="p">,</span> <span class="mf">1.2</span><span class="p">,</span> <span class="mf">0.0</span><span class="p">,</span> <span class="mf">1.3</span><span class="p">],</span> <span class="n">mask</span><span class="o">=</span><span class="p">[</span><span class="bp">False</span><span class="p">,</span>
+<span class="go"> False, False, True, False])</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.setDefaltValues">
+<tt class="descname">setDefaltValues</tt><big>(</big><em>colDict</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.setDefaltValues" title="Permalink to this definition">¶</a></dt>
+<dd><p>Sets default column values.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>colDict</strong> : dict</p>
+<blockquote class="last">
+<div><p>Dict specifying column names and default values as
+{‘colName’:value} where the value is in the units accepted by
+makesourcedb (e.g., Hz for ReferenceFrequency).</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Set new default value for ReferenceFrequency:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setDefaultValues</span><span class="p">({</span><span class="s">'ReferenceFrequency'</span><span class="p">:</span> <span class="mf">140e6</span><span class="p">})</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.setPatchPositions">
+<tt class="descname">setPatchPositions</tt><big>(</big><em>patchDict=None</em>, <em>method='mid'</em>, <em>applyBeam=False</em>, <em>perPatchProjection=True</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.setPatchPositions" title="Permalink to this definition">¶</a></dt>
+<dd><p>Sets the patch positions.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>patchDict</strong> : dict</p>
+<blockquote>
+<div><p>Dict specifying patch names and positions as {‘patchName’:[RA, Dec]}
+where both RA and Dec are degrees J2000 or in makesourcedb format.</p>
+</div></blockquote>
+<p><strong>method</strong> : None or str, optional</p>
+<blockquote>
+<div><p>If no patchDict is given, this parameter specifies the method used
+to set the patch positions:
+- ‘mid’ => the position is set to the midpoint of the patch
+- ‘mean’ => the positions is set to the mean RA and Dec of the patch
+- ‘wmean’ => the position is set to the flux-weighted mean RA and
+Dec of the patch
+- ‘zero’ => set all positions to [0.0, 0.0]</p>
+<p>Note that the mid, mean, and wmean positions are calculated from TAN-
+projected values.</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, fluxes used as weights will be attenuated by the beam.</p>
+</div></blockquote>
+<p><strong>perPatchProjection</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, a different projection center is used per patch. If False,
+a single projection center is used for all patches.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Set all patch positions to their (projected) midpoints:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setPatchPositions</span><span class="p">()</span>
+</pre></div>
+</div>
+<p>Set all patch positions to their (projected) flux-weighted mean
+positions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setPatchPositions</span><span class="p">(</span><span class="n">method</span><span class="o">=</span><span class="s">'wmean'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Set new position for the ‘bin0’ patch only:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setPatchPositions</span><span class="p">({</span><span class="s">'bin0'</span><span class="p">:</span> <span class="p">[</span><span class="mf">123.231</span><span class="p">,</span> <span class="mf">23.4321</span><span class="p">]})</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.setRowValues">
+<tt class="descname">setRowValues</tt><big>(</big><em>values</em>, <em>mask=None</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.setRowValues" title="Permalink to this definition">¶</a></dt>
+<dd><p>Sets values for a single row.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>values</strong> : list, numpy array, or dict</p>
+<blockquote>
+<div><p>Array of values or dict of {colName:value} pairs. If list or
+array, the length must match the number and order of the columns in
+the table. If dict, missing values will be masked unless already
+present.</p>
+</div></blockquote>
+<p><strong>mask</strong> : list or array of bools, optional</p>
+<blockquote class="last">
+<div><p>If values is a list or array, a mask can be specified (True means
+the value is masked).</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Set row values for the source ‘src1’:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setRowValues</span><span class="p">({</span><span class="s">'Name'</span><span class="p">:</span><span class="s">'src1'</span><span class="p">,</span> <span class="s">'Ra'</span><span class="p">:</span><span class="mf">213.123</span><span class="p">,</span> <span class="s">'Dec'</span><span class="p">:</span><span class="mf">23.1232</span><span class="p">,</span>
+<span class="go"> 'I':23.2, 'Type':'POINT'}</span>
+</pre></div>
+</div>
+<p>The RA and Dec values can be in degrees (as above) or in makesourcedb
+format. E.g.:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setRowValues</span><span class="p">({</span><span class="s">'Name'</span><span class="p">:</span><span class="s">'src1'</span><span class="p">,</span> <span class="s">'Ra'</span><span class="p">:</span><span class="s">'12:22:21.1'</span><span class="p">,</span>
+<span class="go"> 'Dec':'+14.46.31.5', 'I':23.2, 'Type':'POINT'}</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.transfer">
+<tt class="descname">transfer</tt><big>(</big><em>patchFile</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.transfer" title="Permalink to this definition">¶</a></dt>
+<dd><p>Transfer patches from the input sky model.</p>
+<p>Sources with the same name as those in patchFile will be grouped into
+the patches defined in patchFile. Sources that do not appear in patchFile
+will be placed into separate patches (one per source). Patch positions are
+not transferred.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>patchFile</strong> : str</p>
+<blockquote class="last">
+<div><p>Input sky model from which to transfer patches.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Transfer patches from one sky model to another and set their positions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">transfer</span><span class="p">(</span><span class="s">'master_sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">setPatchPositions</span><span class="p">(</span><span class="n">method</span><span class="o">=</span><span class="s">'mid'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.ungroup">
+<tt class="descname">ungroup</tt><big>(</big><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.ungroup" title="Permalink to this definition">¶</a></dt>
+<dd><p>Removes all patches from the sky model.</p>
+<p class="rubric">Examples</p>
+<p>Remove all patches:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">ungroup</span><span class="p">()</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="method">
+<dt id="lsmtool.skymodel.SkyModel.write">
+<tt class="descname">write</tt><big>(</big><em>fileName=None</em>, <em>format='makesourcedb'</em>, <em>clobber=False</em>, <em>sortBy=None</em>, <em>lowToHigh=False</em><big>)</big><a class="headerlink" href="#lsmtool.skymodel.SkyModel.write" title="Permalink to this definition">¶</a></dt>
+<dd><p>Writes the sky model to a file.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>filename</strong> : str</p>
+<blockquote>
+<div><p>Name of output file.</p>
+</div></blockquote>
+<p><strong>format: str, optional</strong></p>
+<blockquote>
+<div><dl class="docutils">
+<dt>Format of the output file. Allowed formats are:</dt>
+<dd><ul class="first last simple">
+<li>‘makesourcedb’ (BBS format)</li>
+<li>‘fits’</li>
+<li>‘votable’</li>
+<li>‘hdf5’</li>
+<li>‘ds9’</li>
+<li>‘kvis’</li>
+<li>plus all other formats supported by the astropy.table package</li>
+</ul>
+</dd>
+</dl>
+</div></blockquote>
+<p><strong>clobber</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, an existing file is overwritten.</p>
+</div></blockquote>
+<p><strong>sortBy</strong> : str or list of str, optional</p>
+<blockquote>
+<div><p>Name of columns to sort on. If None, no sorting is done. If
+a list is given, sorting is done on the columns in the order given</p>
+</div></blockquote>
+<p><strong>lowToHigh</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, sort values from low to high instead of high to low</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Write the model to a makesourcedb sky model file suitable for use with
+BBS:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'modsky.model'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Write to a fits catalog:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'sky.fits'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'fits'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Write to a ds9 region file:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">s</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'sky.reg'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'ds9'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+</dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.tableio">
+<span id="lsmtool-tableio-module"></span><h2>lsmtool.tableio module<a class="headerlink" href="#module-lsmtool.tableio" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.tableio.Dec2Angle">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">Dec2Angle</tt><big>(</big><em>Dec</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.Dec2Angle" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns Angle objects for input Dec values.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>Dec</strong> : str, float or list of str, float</p>
+<blockquote>
+<div><p>Values of Dec to convert. Can be strings in makesourcedb format or floats
+in degrees.</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first last"><strong>DecAngle</strong> : astropy.coordinates.Angle object</p>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.RA2Angle">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">RA2Angle</tt><big>(</big><em>RA</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.RA2Angle" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns Angle objects for input RA values.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>RA</strong> : str, float or list of str, float</p>
+<blockquote>
+<div><p>Values of RA to convert. Can be strings in makesourcedb format or floats
+in degrees.</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first last"><strong>RAAngle</strong> : astropy.coordinates.Angle object</p>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.ds9RegionWriter">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">ds9RegionWriter</tt><big>(</big><em>table</em>, <em>fileName</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.ds9RegionWriter" title="Permalink to this definition">¶</a></dt>
+<dd><p>Writes table to a ds9 region file.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>table</strong> : astropy.table.Table object</p>
+<blockquote>
+<div><p>Input sky model table</p>
+</div></blockquote>
+<p><strong>fileName</strong> : str</p>
+<blockquote class="last">
+<div><p>Output ASCII file to which the sky model is written.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.kvisAnnWriter">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">kvisAnnWriter</tt><big>(</big><em>table</em>, <em>fileName</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.kvisAnnWriter" title="Permalink to this definition">¶</a></dt>
+<dd><p>Writes table to a kvis annotation file.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>table</strong> : astropy.table.Table object</p>
+<blockquote>
+<div><p>Input sky model table</p>
+</div></blockquote>
+<p><strong>fileName</strong> : str</p>
+<blockquote class="last">
+<div><p>Output ASCII file to which the sky model is written.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.rowStr">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">rowStr</tt><big>(</big><em>row</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.rowStr" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns makesourcedb representation of a row.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>row</strong> : astropy.table.Row object</p>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first"><strong>line</strong> : str</p>
+<blockquote class="last">
+<div><p>Sting representing a row in a makesourcedb sky model file</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.skyModelIdentify">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">skyModelIdentify</tt><big>(</big><em>origin</em>, <em>*args</em>, <em>**kwargs</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.skyModelIdentify" title="Permalink to this definition">¶</a></dt>
+<dd><p>Identifies valid makesourcedb sky model files.</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.skyModelReader">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">skyModelReader</tt><big>(</big><em>fileName</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.skyModelReader" title="Permalink to this definition">¶</a></dt>
+<dd><p>Reads a makesourcedb sky model file into an astropy table.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>fileName</strong> : str</p>
+<blockquote>
+<div><p>Input ASCII file from which the sky model is read. Must
+respect the makesourcedb format</p>
+</div></blockquote>
+</td>
+</tr>
+<tr class="field-even field"><th class="field-name">Returns:</th><td class="field-body"><p class="first last"><strong>table</strong> : astropy.table.Table object</p>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.tableio.skyModelWriter">
+<tt class="descclassname">lsmtool.tableio.</tt><tt class="descname">skyModelWriter</tt><big>(</big><em>table</em>, <em>fileName</em><big>)</big><a class="headerlink" href="#lsmtool.tableio.skyModelWriter" title="Permalink to this definition">¶</a></dt>
+<dd><p>Writes table to a makesourcedb sky model file.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>fileName</strong> : str</p>
+<blockquote class="last">
+<div><p>Output ASCII file to which the sky model is written.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+</div>
+</div>
+
+
+ </div>
+ </div>
+ </div>
+ <div class="sphinxsidebar">
+ <div class="sphinxsidebarwrapper">
+ <h3><a href="index.html">Table Of Contents</a></h3>
+ <ul>
+<li><a class="reference internal" href="#">LSMTool Module Documentation</a><ul>
+<li><a class="reference internal" href="#module-lsmtool">lsmtool module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations_lib">lsmtool.operations_lib module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.skymodel">lsmtool.skymodel module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.tableio">lsmtool.tableio module</a></li>
+</ul>
+</li>
+</ul>
+
+ <h4>Previous topic</h4>
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+
+ <div class="section" id="lsmtool-operations-package">
+<h1>lsmtool.operations package<a class="headerlink" href="#lsmtool-operations-package" title="Permalink to this headline">¶</a></h1>
+<div class="section" id="submodules">
+<h2>Submodules<a class="headerlink" href="#submodules" title="Permalink to this headline">¶</a></h2>
+</div>
+<div class="section" id="module-lsmtool.operations.add">
+<span id="lsmtool-operations-add-module"></span><h2>lsmtool.operations.add module<a class="headerlink" href="#module-lsmtool.operations.add" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.add.add">
+<tt class="descclassname">lsmtool.operations.add.</tt><tt class="descname">add</tt><big>(</big><em>LSM</em>, <em>colNamesVals</em><big>)</big><a class="headerlink" href="#lsmtool.operations.add.add" title="Permalink to this definition">¶</a></dt>
+<dd><p>Add a source to the sky model.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>LSM</strong> : SkyModel object</p>
+<blockquote>
+<div><p>Input sky model.</p>
+</div></blockquote>
+<p><strong>colNamesVals</strong> : dict</p>
+<blockquote class="last">
+<div><p>A dictionary that specifies the row values for the source to be added.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.add.run">
+<tt class="descclassname">lsmtool.operations.add.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.add.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.concatenate">
+<span id="lsmtool-operations-concatenate-module"></span><h2>lsmtool.operations.concatenate module<a class="headerlink" href="#module-lsmtool.operations.concatenate" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.concatenate.concatenate">
+<tt class="descclassname">lsmtool.operations.concatenate.</tt><tt class="descname">concatenate</tt><big>(</big><em>LSM1</em>, <em>LSM2</em>, <em>matchBy='name'</em>, <em>radius=0.1</em>, <em>keep='all'</em><big>)</big><a class="headerlink" href="#lsmtool.operations.concatenate.concatenate" title="Permalink to this definition">¶</a></dt>
+<dd><p>Concatenate two sky models</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>LSM1</strong> : SkyModel object</p>
+<blockquote>
+<div><p>Parent sky model</p>
+</div></blockquote>
+<p><strong>LSM2</strong> : SkyModel object</p>
+<blockquote>
+<div><p>Sky model to concatenate with the parent sky model</p>
+</div></blockquote>
+<p><strong>matchBy</strong> : str, optional</p>
+<blockquote>
+<div><p>Determines how duplicate sources are determined:
+- ‘name’ => duplicates are identified by name
+- ‘position’ => duplicates are identified by radius. Sources within the</p>
+<blockquote>
+<div><p>radius specified by the radius parameter are considered duplicates</p>
+</div></blockquote>
+</div></blockquote>
+<p><strong>radius</strong> : float, optional</p>
+<blockquote>
+<div><p>Radius in degrees for matching when matchBy=’position’</p>
+</div></blockquote>
+<p><strong>keep</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>Determines how duplicates are treated:
+- ‘all’ => all duplicates are kept; those with identical names are re-</p>
+<blockquote>
+<div><p>named</p>
+</div></blockquote>
+<ul class="simple">
+<li>‘from1’ => duplicates kept are those from sky model 1 (LSM1)</li>
+<li>‘from2’ => duplicates kept are those from sky model 2 (LSM2)</li>
+</ul>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Concatenate two sky models, identifying duplicates by matching to the source
+names. When duplicates are found, keep the source from the parent sky model
+and discard the duplicate from second sky model (this might be useful when
+merging two sky models that have some overlap):</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM1</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky1.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM2</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky2.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">concatenate</span><span class="p">(</span><span class="n">LSM1</span><span class="p">,</span> <span class="n">LSM2</span><span class="p">,</span> <span class="n">matchBy</span><span class="o">=</span><span class="s">'name'</span><span class="p">,</span> <span class="n">keep</span><span class="o">=</span><span class="s">'from1'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Concatenate two sky models, identifying duplicates by matching to the source
+positions within a radius of 10 arcsec. When duplicates are found, keep the
+source from the second sky model and discard the duplicate from the parent
+sky model (this might be useful when replacing parts of a low-resolution
+sky model with a high-resolution one):</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM2</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'high_res_sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">concatenate</span><span class="p">(</span><span class="n">LSM1</span><span class="p">,</span> <span class="n">LSM2</span><span class="p">,</span> <span class="n">matchBy</span><span class="o">=</span><span class="s">'position'</span><span class="p">,</span> <span class="n">radius</span><span class="o">=</span><span class="mf">10.0</span><span class="o">/</span><span class="mf">3600.0</span><span class="p">,</span>
+<span class="go"> keep='from2')</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.concatenate.run">
+<tt class="descclassname">lsmtool.operations.concatenate.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.concatenate.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.group">
+<span id="lsmtool-operations-group-module"></span><h2>lsmtool.operations.group module<a class="headerlink" href="#module-lsmtool.operations.group" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.group.addEvery">
+<tt class="descclassname">lsmtool.operations.group.</tt><tt class="descname">addEvery</tt><big>(</big><em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.group.addEvery" title="Permalink to this definition">¶</a></dt>
+<dd><p>Add a Patch column with a different name for each source</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.group.addSingle">
+<tt class="descclassname">lsmtool.operations.group.</tt><tt class="descname">addSingle</tt><big>(</big><em>LSM</em>, <em>patchName</em><big>)</big><a class="headerlink" href="#lsmtool.operations.group.addSingle" title="Permalink to this definition">¶</a></dt>
+<dd><p>Add a Patch column with a single patch name</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.group.getPatchNamesFromMask">
+<tt class="descclassname">lsmtool.operations.group.</tt><tt class="descname">getPatchNamesFromMask</tt><big>(</big><em>mask</em>, <em>RARad</em>, <em>DecRad</em><big>)</big><a class="headerlink" href="#lsmtool.operations.group.getPatchNamesFromMask" title="Permalink to this definition">¶</a></dt>
+<dd><p>Returns an array of patch names for each (RA, Dec) pair in radians</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.group.group">
+<tt class="descclassname">lsmtool.operations.group.</tt><tt class="descname">group</tt><big>(</big><em>LSM</em>, <em>algorithm</em>, <em>targetFlux=None</em>, <em>numClusters=100</em>, <em>applyBeam=False</em><big>)</big><a class="headerlink" href="#lsmtool.operations.group.group" title="Permalink to this definition">¶</a></dt>
+<dd><p>Groups sources into patches</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>LSM</strong> : SkyModel object</p>
+<blockquote>
+<div><p>Input sky model.</p>
+</div></blockquote>
+<p><strong>algorithm</strong> : str</p>
+<blockquote>
+<div><p>Algorithm to use for grouping:
+- ‘single’ => all sources are grouped into a single patch
+- ‘every’ => every source gets a separate patch
+- ‘cluster’ => SAGECAL clustering algorithm that groups sources into</p>
+<blockquote>
+<div><p>specified number of clusters (specified by the numClusters parameter).</p>
+</div></blockquote>
+<ul>
+<li><dl class="first docutils">
+<dt>‘tessellate’ => group into tiles whose total flux approximates</dt>
+<dd><p class="first last">the target flux (specified by the targetFlux parameter).</p>
+</dd>
+</dl>
+</li>
+<li><dl class="first docutils">
+<dt>the filename of a mask image => group by masked regions (where mask =</dt>
+<dd><p class="first last">True). Source outside of masked regions are given patches of their
+own.</p>
+</dd>
+</dl>
+</li>
+</ul>
+</div></blockquote>
+<p><strong>targetFlux</strong> : str or float, optional</p>
+<blockquote>
+<div><p>Target flux for tessellation (the total flux of each tile will be close
+to this value). The target flux can be specified as either a float in Jy
+or as a string with units (e.g., ‘25.0 mJy’).</p>
+</div></blockquote>
+<p><strong>numClusters</strong> : int, optional</p>
+<blockquote>
+<div><p>Number of clusters for clustering. Sources are grouped around the
+numClusters brightest sources.</p>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, fluxes will be attenuated by the beam.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Tesselate the sky model into patches with approximately 30 Jy total
+flux:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">group</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'tessellate'</span><span class="p">,</span> <span class="n">targetFlux</span><span class="o">=</span><span class="mf">30.0</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.group.run">
+<tt class="descclassname">lsmtool.operations.group.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.group.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.merge">
+<span id="lsmtool-operations-merge-module"></span><h2>lsmtool.operations.merge module<a class="headerlink" href="#module-lsmtool.operations.merge" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.merge.merge">
+<tt class="descclassname">lsmtool.operations.merge.</tt><tt class="descname">merge</tt><big>(</big><em>LSM</em>, <em>patches</em>, <em>name=None</em><big>)</big><a class="headerlink" href="#lsmtool.operations.merge.merge" title="Permalink to this definition">¶</a></dt>
+<dd><p>Merge two or more patches together</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>patches</strong> : list of str</p>
+<blockquote>
+<div><p>List of patches to merge</p>
+</div></blockquote>
+<p><strong>name</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>Name of resulting merged patch</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Merge three patches into one:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">merge</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="p">[</span><span class="s">'bin0'</span><span class="p">,</span> <span class="s">'bin1'</span><span class="p">,</span> <span class="s">'bin2'</span><span class="p">],</span> <span class="s">'binmerged'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.merge.run">
+<tt class="descclassname">lsmtool.operations.merge.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.merge.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.move">
+<span id="lsmtool-operations-move-module"></span><h2>lsmtool.operations.move module<a class="headerlink" href="#module-lsmtool.operations.move" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.move.move">
+<tt class="descclassname">lsmtool.operations.move.</tt><tt class="descname">move</tt><big>(</big><em>LSM</em>, <em>name</em>, <em>position=None</em>, <em>shift=None</em><big>)</big><a class="headerlink" href="#lsmtool.operations.move.move" title="Permalink to this definition">¶</a></dt>
+<dd><p>Move or shift a source.</p>
+<p>If both a position and a shift are specified, the source is moved to the
+new position and then shifted.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>name</strong> : str</p>
+<blockquote>
+<div><p>Source name.</p>
+</div></blockquote>
+<p><strong>position</strong> : list, optional</p>
+<blockquote>
+<div><p>A list specifying a new position as [RA, Dec] in either makesourcedb
+format (e.g., [‘12:23:43.21’, ‘+22.34.21.2’]) or in degrees (e.g.,
+[123.2312, 23.3422]).</p>
+</div></blockquote>
+<p><strong>shift</strong> : list, optional</p>
+<blockquote class="last">
+<div><p>A list specifying the shift as [RAShift, DecShift] in
+in degrees (e.g., [0.02312, 0.00342]).</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Move source ‘1609.6+6556’ to a new position:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">move</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'1609.6+6556'</span><span class="p">,</span> <span class="n">position</span><span class="o">=</span><span class="p">[</span><span class="s">'16:10:00'</span><span class="p">,</span> <span class="s">'+65.57.00'</span><span class="p">])</span>
+</pre></div>
+</div>
+<p>Shift the source by 10 arcsec in Dec:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">move</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'1609.6+6556'</span><span class="p">,</span> <span class="n">shift</span><span class="o">=</span><span class="p">[</span><span class="mf">0.0</span><span class="p">,</span> <span class="mf">10.0</span><span class="o">/</span><span class="mf">3600.0</span><span class="p">])</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.move.run">
+<tt class="descclassname">lsmtool.operations.move.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.move.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.plot">
+<span id="lsmtool-operations-plot-module"></span><h2>lsmtool.operations.plot module<a class="headerlink" href="#module-lsmtool.operations.plot" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.plot.Dectickformatter">
+<tt class="descclassname">lsmtool.operations.plot.</tt><tt class="descname">Dectickformatter</tt><big>(</big><em>y</em>, <em>pos</em><big>)</big><a class="headerlink" href="#lsmtool.operations.plot.Dectickformatter" title="Permalink to this definition">¶</a></dt>
+<dd><p>Changes y tick labels from pixels to Dec in degrees</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.plot.RAtickformatter">
+<tt class="descclassname">lsmtool.operations.plot.</tt><tt class="descname">RAtickformatter</tt><big>(</big><em>x</em>, <em>pos</em><big>)</big><a class="headerlink" href="#lsmtool.operations.plot.RAtickformatter" title="Permalink to this definition">¶</a></dt>
+<dd><p>Changes x tick labels from pixels to RA in degrees</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.plot.formatCoord">
+<tt class="descclassname">lsmtool.operations.plot.</tt><tt class="descname">formatCoord</tt><big>(</big><em>x</em>, <em>y</em><big>)</big><a class="headerlink" href="#lsmtool.operations.plot.formatCoord" title="Permalink to this definition">¶</a></dt>
+<dd><p>Custom coordinate format</p>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.plot.plot">
+<tt class="descclassname">lsmtool.operations.plot.</tt><tt class="descname">plot</tt><big>(</big><em>LSM</em>, <em>fileName=None</em><big>)</big><a class="headerlink" href="#lsmtool.operations.plot.plot" title="Permalink to this definition">¶</a></dt>
+<dd><p>Shows a simple plot of the sky model.</p>
+<p>The circles in the plot are scaled with flux. If the sky model is grouped
+into patches, sources are colored by patch and the patch positions are
+indicated with stars.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>fileName</strong> : str, optional</p>
+<blockquote class="last">
+<div><p>If given, the plot is saved to a file instead of displayed.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.plot.run">
+<tt class="descclassname">lsmtool.operations.plot.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.plot.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.remove">
+<span id="lsmtool-operations-remove-module"></span><h2>lsmtool.operations.remove module<a class="headerlink" href="#module-lsmtool.operations.remove" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.remove.remove">
+<tt class="descclassname">lsmtool.operations.remove.</tt><tt class="descname">remove</tt><big>(</big><em>LSM</em>, <em>filterExpression</em>, <em>aggregate=None</em>, <em>applyBeam=None</em>, <em>useRegEx=False</em>, <em>force=False</em><big>)</big><a class="headerlink" href="#lsmtool.operations.remove.remove" title="Permalink to this definition">¶</a></dt>
+<dd><p>Filters the sky model, removing all sources that meet the given expression.</p>
+<p>After filtering, the sky model contains only those sources for which the
+given filter expression is false.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>filterExpression</strong> : str or dict</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>A string specifying the filter expression in the form:</dt>
+<dd><p class="first last">‘<property> <operator> <value> [<units>]’</p>
+</dd>
+</dl>
+<p>(e.g., ‘I <= 10.5 Jy’). These elements can also be given as a
+dictionary in the form:</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>{‘filterProp’:property, ‘filterOper’:operator,</dt>
+<dd><p class="first last">‘filterVal’:value, ‘filterUnits’:units}</p>
+</dd>
+</dl>
+</div></blockquote>
+<dl class="docutils">
+<dt>or as a list:</dt>
+<dd><p class="first last">[property, operator, value, value]</p>
+</dd>
+</dl>
+<p>The property to filter on must be a valid column name or the filename
+of a mask image.</p>
+<dl class="docutils">
+<dt>Supported operators are:</dt>
+<dd><ul class="first last simple">
+<li>!=</li>
+<li><=</li>
+<li>>=</li>
+<li>></li>
+<li><</li>
+<li>= (or ‘==’)</li>
+</ul>
+</dd>
+</dl>
+<p>Units are optional and must be specified as required by astropy.units.</p>
+</div></blockquote>
+<p><strong>aggregate</strong> : str, optional</p>
+<blockquote>
+<div><p>If set, the array returned will be of values aggregated
+over the patch members. The following aggregation functions are
+available:</p>
+<blockquote>
+<div><ul>
+<li><p class="first">‘sum’: sum of patch values</p>
+</li>
+<li><p class="first">‘mean’: mean of patch values</p>
+</li>
+<li><p class="first">‘wmean’: Stokes I weighted mean of patch values</p>
+</li>
+<li><p class="first">‘min’: minimum of patch values</p>
+</li>
+<li><p class="first">‘max’: maximum of patch values</p>
+</li>
+<li><dl class="first docutils">
+<dt>True: only valid when the filter indices are specified directly as</dt>
+<dd><p class="first last">a numpy array. If True, filtering is done on patches instead of
+sources.</p>
+</dd>
+</dl>
+</li>
+</ul>
+</div></blockquote>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, apparent fluxes will be used.</p>
+</div></blockquote>
+<p><strong>useRegEx</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, string matching will use regular expression matching. If
+False, string matching uses Unix filename matching.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Filter on column ‘I’ (Stokes I flux). This filter will remove all sources
+with Stokes I flux greater than 1.5 Jy:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">remove</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'I > 1.5 Jy'</span><span class="p">)</span>
+<span class="go">INFO: Removed 1102 sources.</span>
+</pre></div>
+</div>
+<p>If the sky model has patches and the filter is desired per patch, use
+<tt class="docutils literal"><span class="pre">aggregate</span> <span class="pre">=</span> <span class="pre">function</span></tt>. For example, to select on the sum of the patch
+fluxes:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">remove</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'I > 1.5 Jy'</span><span class="p">,</span> <span class="n">aggregate</span><span class="o">=</span><span class="s">'sum'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Filter on source names, removing those that match “src*_1?”:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">remove</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'Name == src*_1?'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Use a CASA clean mask image to remove sources that lie in masked regions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">remove</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'clean_mask.mask == True'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.remove.run">
+<tt class="descclassname">lsmtool.operations.remove.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.remove.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.select">
+<span id="lsmtool-operations-select-module"></span><h2>lsmtool.operations.select module<a class="headerlink" href="#module-lsmtool.operations.select" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.select.run">
+<tt class="descclassname">lsmtool.operations.select.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.select.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.select.select">
+<tt class="descclassname">lsmtool.operations.select.</tt><tt class="descname">select</tt><big>(</big><em>LSM</em>, <em>filterExpression</em>, <em>aggregate=None</em>, <em>applyBeam=False</em>, <em>useRegEx=False</em>, <em>force=False</em><big>)</big><a class="headerlink" href="#lsmtool.operations.select.select" title="Permalink to this definition">¶</a></dt>
+<dd><p>Filters the sky model, keeping all sources that meet the given expression.</p>
+<p>After filtering, the sky model contains only those sources for which the
+given filter expression is true.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>filterExpression</strong> : str or dict</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>A string specifying the filter expression in the form:</dt>
+<dd><p class="first last">‘<property> <operator> <value> [<units>]’</p>
+</dd>
+</dl>
+<p>(e.g., ‘I <= 10.5 Jy’). These elements can also be given as a
+dictionary in the form:</p>
+<blockquote>
+<div><dl class="docutils">
+<dt>{‘filterProp’:property, ‘filterOper’:operator,</dt>
+<dd><p class="first last">‘filterVal’:value, ‘filterUnits’:units}</p>
+</dd>
+</dl>
+</div></blockquote>
+<dl class="docutils">
+<dt>or as a list:</dt>
+<dd><p class="first last">[property, operator, value, value]</p>
+</dd>
+</dl>
+<p>The property to filter on must be a valid column name or the filename
+of a mask image.</p>
+<dl class="docutils">
+<dt>Supported operators are:</dt>
+<dd><ul class="first last simple">
+<li>!=</li>
+<li><=</li>
+<li>>=</li>
+<li>></li>
+<li><</li>
+<li>= (or ‘==’)</li>
+</ul>
+</dd>
+</dl>
+<p>Units are optional and must be specified as required by astropy.units.</p>
+</div></blockquote>
+<p><strong>aggregate</strong> : str, optional</p>
+<blockquote>
+<div><p>If set, the array returned will be of values aggregated
+over the patch members. The following aggregation functions are
+available:</p>
+<blockquote>
+<div><ul>
+<li><p class="first">‘sum’: sum of patch values</p>
+</li>
+<li><p class="first">‘mean’: mean of patch values</p>
+</li>
+<li><p class="first">‘wmean’: Stokes I weighted mean of patch values</p>
+</li>
+<li><p class="first">‘min’: minimum of patch values</p>
+</li>
+<li><p class="first">‘max’: maximum of patch values</p>
+</li>
+<li><dl class="first docutils">
+<dt>True: only valid when the filter indices are specified directly as</dt>
+<dd><p class="first last">a numpy array. If True, filtering is done on patches instead of
+sources.</p>
+</dd>
+</dl>
+</li>
+</ul>
+</div></blockquote>
+</div></blockquote>
+<p><strong>applyBeam</strong> : bool, optional</p>
+<blockquote>
+<div><p>If True, apparent fluxes will be used.</p>
+</div></blockquote>
+<p><strong>useRegEx</strong> : bool, optional</p>
+<blockquote class="last">
+<div><p>If True, string matching will use regular expression matching. If
+False, string matching uses Unix filename matching.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Filter on column ‘I’ (Stokes I flux). This filter will select all sources
+with Stokes I flux greater than 1.5 Jy:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">select</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'I > 1.5 Jy'</span><span class="p">)</span>
+<span class="go">INFO: Kept 1102 sources.</span>
+</pre></div>
+</div>
+<p>If the sky model has patches and the filter is desired per patch, use
+<tt class="docutils literal"><span class="pre">aggregate</span> <span class="pre">=</span> <span class="pre">function</span></tt>. For example, to select on the sum of the patch
+fluxes:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">select</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'I > 1.5 Jy'</span><span class="p">,</span> <span class="n">aggregate</span><span class="o">=</span><span class="s">'sum'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Filter on source names, keeping those that match “src*_1?”:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">select</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'Name == src*_1?'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Use a CASA clean mask image to keep sources that lie in masked regions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="nb">filter</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'clean_mask.mask == True'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.setpatchpositions">
+<span id="lsmtool-operations-setpatchpositions-module"></span><h2>lsmtool.operations.setpatchpositions module<a class="headerlink" href="#module-lsmtool.operations.setpatchpositions" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.setpatchpositions.run">
+<tt class="descclassname">lsmtool.operations.setpatchpositions.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.setpatchpositions.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.transfer">
+<span id="lsmtool-operations-transfer-module"></span><h2>lsmtool.operations.transfer module<a class="headerlink" href="#module-lsmtool.operations.transfer" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.transfer.run">
+<tt class="descclassname">lsmtool.operations.transfer.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.transfer.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+<dl class="function">
+<dt id="lsmtool.operations.transfer.transfer">
+<tt class="descclassname">lsmtool.operations.transfer.</tt><tt class="descname">transfer</tt><big>(</big><em>LSM</em>, <em>patchFile</em><big>)</big><a class="headerlink" href="#lsmtool.operations.transfer.transfer" title="Permalink to this definition">¶</a></dt>
+<dd><p>Transfer patches from the input sky model.</p>
+<p>Sources with the same name as those in patchFile will be grouped into
+the patches defined in patchFile. Sources that do not appear in patchFile
+will be placed into separate patches (one per source). Patch positions are
+not transferred.</p>
+<table class="docutils field-list" frame="void" rules="none">
+<col class="field-name" />
+<col class="field-body" />
+<tbody valign="top">
+<tr class="field-odd field"><th class="field-name">Parameters:</th><td class="field-body"><p class="first"><strong>patchFile</strong> : str</p>
+<blockquote class="last">
+<div><p>Input sky model from which to transfer patches.</p>
+</div></blockquote>
+</td>
+</tr>
+</tbody>
+</table>
+<p class="rubric">Examples</p>
+<p>Transfer patches from one sky model to another and set their positions:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">transfer</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="s">'master_sky.model'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">setPatchPositions</span><span class="p">(</span><span class="n">LSM</span><span class="p">,</span> <span class="n">method</span><span class="o">=</span><span class="s">'mid'</span><span class="p">)</span>
+</pre></div>
+</div>
+</dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations.ungroup">
+<span id="lsmtool-operations-ungroup-module"></span><h2>lsmtool.operations.ungroup module<a class="headerlink" href="#module-lsmtool.operations.ungroup" title="Permalink to this headline">¶</a></h2>
+<dl class="function">
+<dt id="lsmtool.operations.ungroup.run">
+<tt class="descclassname">lsmtool.operations.ungroup.</tt><tt class="descname">run</tt><big>(</big><em>step</em>, <em>parset</em>, <em>LSM</em><big>)</big><a class="headerlink" href="#lsmtool.operations.ungroup.run" title="Permalink to this definition">¶</a></dt>
+<dd></dd></dl>
+
+</div>
+<div class="section" id="module-lsmtool.operations">
+<span id="module-contents"></span><h2>Module contents<a class="headerlink" href="#module-lsmtool.operations" title="Permalink to this headline">¶</a></h2>
+</div>
+</div>
+
+
+ </div>
+ </div>
+ </div>
+ <div class="sphinxsidebar">
+ <div class="sphinxsidebarwrapper">
+ <h3><a href="index.html">Table Of Contents</a></h3>
+ <ul>
+<li><a class="reference internal" href="#">lsmtool.operations package</a><ul>
+<li><a class="reference internal" href="#submodules">Submodules</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.add">lsmtool.operations.add module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.concatenate">lsmtool.operations.concatenate module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.group">lsmtool.operations.group module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.merge">lsmtool.operations.merge module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.move">lsmtool.operations.move module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.plot">lsmtool.operations.plot module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.remove">lsmtool.operations.remove module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.select">lsmtool.operations.select module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.setpatchpositions">lsmtool.operations.setpatchpositions module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.transfer">lsmtool.operations.transfer module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations.ungroup">lsmtool.operations.ungroup module</a></li>
+<li><a class="reference internal" href="#module-lsmtool.operations">Module contents</a></li>
+</ul>
+</li>
+</ul>
+
+ <h3>This Page</h3>
+ <ul class="this-page-menu">
+ <li><a href="_sources/lsmtool.operations.txt"
+ rel="nofollow">Show Source</a></li>
+ </ul>
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+<h1>lsmtool<a class="headerlink" href="#lsmtool" title="Permalink to this headline">¶</a></h1>
+<div class="toctree-wrapper compound">
+<ul>
+<li class="toctree-l1"><a class="reference internal" href="lsmtool.html">LSMTool Module Documentation</a><ul>
+<li class="toctree-l2"><a class="reference internal" href="lsmtool.html#subpackages">Subpackages</a><ul>
+<li class="toctree-l3"><a class="reference internal" href="lsmtool.operations.html">lsmtool.operations package</a><ul>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#submodules">Submodules</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.add">lsmtool.operations.add module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.concatenate">lsmtool.operations.concatenate module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.group">lsmtool.operations.group module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.merge">lsmtool.operations.merge module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.move">lsmtool.operations.move module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.plot">lsmtool.operations.plot module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.remove">lsmtool.operations.remove module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.select">lsmtool.operations.select module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.setpatchpositions">lsmtool.operations.setpatchpositions module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.transfer">lsmtool.operations.transfer module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations.ungroup">lsmtool.operations.ungroup module</a></li>
+<li class="toctree-l4"><a class="reference internal" href="lsmtool.operations.html#module-lsmtool.operations">Module contents</a></li>
+</ul>
+</li>
+</ul>
+</li>
+<li class="toctree-l2"><a class="reference internal" href="lsmtool.html#module-lsmtool.operations_lib">lsmtool.operations_lib module</a></li>
+<li class="toctree-l2"><a class="reference internal" href="lsmtool.html#module-lsmtool.skymodel">lsmtool.skymodel module</a></li>
+<li class="toctree-l2"><a class="reference internal" href="lsmtool.html#module-lsmtool.tableio">lsmtool.tableio module</a></li>
+<li class="toctree-l2"><a class="reference internal" href="lsmtool.html#module-lsmtool">Module contents</a></li>
+</ul>
+</li>
+</ul>
+</div>
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+ <input type="hidden" name="check_keywords" value="yes" />
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+ Enter search terms or a module, class or function name.
+ </p>
+</div>
+<script type="text/javascript">$('#searchbox').show(0);</script>
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+ </div>
+ <div class="clearer"></div>
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+ <div class="related">
+ <h3>Navigation</h3>
+ <ul>
+ <li class="right" style="margin-right: 10px">
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+ >modules</a> |</li>
+ <li><a href="index.html">LSMTool 1.0.0 documentation</a> »</li>
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diff --git a/doc/build/html/objects.inv b/docs/build/html/objects.inv
similarity index 100%
rename from doc/build/html/objects.inv
rename to docs/build/html/objects.inv
diff --git a/docs/build/html/overview.html b/docs/build/html/overview.html
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+++ b/docs/build/html/overview.html
@@ -0,0 +1,459 @@
+<!DOCTYPE html PUBLIC "-//W3C//DTD XHTML 1.0 Transitional//EN"
+ "http://www.w3.org/TR/xhtml1/DTD/xhtml1-transitional.dtd">
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+<html xmlns="http://www.w3.org/1999/xhtml">
+ <head>
+ <meta http-equiv="Content-Type" content="text/html; charset=utf-8" />
+
+ <title>LSMTool: the LOFAR Local Sky Model Tool — LSMTool 1.0.0 documentation</title>
+
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+ <div class="body">
+
+ <div class="section" id="lsmtool-the-lofar-local-sky-model-tool">
+<h1>LSMTool: the LOFAR Local Sky Model Tool<a class="headerlink" href="#lsmtool-the-lofar-local-sky-model-tool" title="Permalink to this headline">¶</a></h1>
+<p>LSMTool is a Python package which allows for the manipulation of sky
+models in the <tt class="docutils literal"><span class="pre">makesourcedb</span></tt> format (understood by BBS and NDPPP).
+Note that LSMTool is still in beta. Please report bugs to
+<a class="reference external" href="mailto:drafferty%40hs.uni-hamburg.de">drafferty<span>@</span>hs<span>.</span>uni-hamburg<span>.</span>de</a>. To initialize your environment for LSMTool,
+users on CEP1 and CEP2 should run the following commands:</p>
+<div class="highlight-python"><div class="highlight"><pre>use LofIm
+source ~rafferty/init_lsmtool
+</pre></div>
+</div>
+<p>Note that the Pythonlibs LOFAR package includes an older version of
+astropy that conflicts with LSMTool and cannot be used in conjunction
+with it.</p>
+<div class="section" id="usage">
+<h2>Usage<a class="headerlink" href="#usage" title="Permalink to this headline">¶</a></h2>
+<p>The command-line version of LSMTool can be run as follows:</p>
+<div class="highlight-python"><div class="highlight"><pre>Usage: lsmtool.py <skymodel> <parset> [<beam MS>]
+Options:
+ --version show program's version number and exit
+ -h, --help show this help message and exit
+ -q Quiet
+ -v Verbose
+</pre></div>
+</div>
+<p>The parset specifies the operations to perform and their parameters.
+These are described in the next sections.</p>
+</div>
+<div class="section" id="operations">
+<span id="operations-defined"></span><h2>Operations<a class="headerlink" href="#operations" title="Permalink to this headline">¶</a></h2>
+<p>These are the operations that LSMTool can perform:</p>
+<dl class="docutils">
+<dt>SELECT</dt>
+<dd>: Select sources by source or patch properties</dd>
+<dt>REMOVE</dt>
+<dd>: Remove sources by source or patch properties</dd>
+<dt>TRANSFER</dt>
+<dd>: Transfer a patch scheme from one sky model to another</dd>
+<dt>GROUP</dt>
+<dd>: Group sources into patches</dd>
+<dt>UNGROUP</dt>
+<dd>: Remove patches</dd>
+<dt>MOVE</dt>
+<dd>: Move a source or patch position</dd>
+<dt>MERGE</dt>
+<dd>: Merge two or more patches into one</dd>
+<dt>CONCATENATE</dt>
+<dd>: Concatenate two sky models</dd>
+<dt>ADD</dt>
+<dd>: Add a source</dd>
+<dt>SETPATCHPOSITIONS</dt>
+<dd>: Calculate and set patch positions</dd>
+<dt>PLOT</dt>
+<dd>: Plot a simple representation of the sky model</dd>
+</dl>
+</div>
+<div class="section" id="example-parset">
+<h2>Example parset<a class="headerlink" href="#example-parset" title="Permalink to this headline">¶</a></h2>
+<p>This is an example parset that filters on the flux, adds a source, and
+then groups the sources into patches:</p>
+<div class="highlight-python"><div class="highlight"><pre>LSMTool.Steps = [selectbright, addsrc, grp, setpos]
+
+# Select only sources above 1 mJy
+LSMTool.Steps.selectbright.Operation = SELECT
+LSMTool.Steps.selectbright.FilterExpression = I > 1.0 mJy
+
+# Add a source
+LSMTool.Steps.addsrc.Name = new_source
+LSMTool.Steps.addsrc.Type = POINT
+LSMTool.Steps.addsrc.Ra = 277.4232
+LSMTool.Steps.addsrc.Dec = 48.3689
+LSMTool.Steps.addsrc.I = 0.69
+
+# Group using tessellation to a target flux of 50 Jy
+LSMTool.Steps.grp.Operation = GROUP
+LSMTool.Steps.grp.Algorithm = tessellate
+LSMTool.Steps.grp.TargetFlux = 50.0 Jy
+LSMTool.Steps.grp.Method = mid
+
+# Set the patch positions to their midpoint and write final skymodel
+LSMTool.Steps.setpos.Method = mid
+LSMTool.Steps.setpos.Outfile = grouped.sky
+</pre></div>
+</div>
+<p>In the first line of this parset the step names are defined. In the next
+sections, the step parameters for every step are defined. Steps are
+applied sequentially, in the same order defined in the list of steps. A
+list of step-specific parameters is given in
+Table [lsmtool:tab:local<sub>v</sub>al].</p>
+<table border="1" class="docutils">
+<colgroup>
+<col width="17%" />
+<col width="15%" />
+<col width="14%" />
+<col width="54%" />
+</colgroup>
+<thead valign="bottom">
+<tr class="row-odd"><th class="head">Var Name</th>
+<th class="head">Format</th>
+<th class="head">Example</th>
+<th class="head">Comment</th>
+</tr>
+</thead>
+<tbody valign="top">
+<tr class="row-even"><td>Operation</td>
+<td>string</td>
+<td>SELECT</td>
+<td>An operation name (see <a class="reference internal" href="#operations-defined"><em>Operations</em></a>)</td>
+</tr>
+<tr class="row-odd"><td>OutFile</td>
+<td>string</td>
+<td>out.sky</td>
+<td>Name of output file</td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>SELECT and REMOVE</strong></td>
+</tr>
+<tr class="row-odd"><td>FilterExpression</td>
+<td>string</td>
+<td>I > 10.0 Jy</td>
+<td>Filter for selection</td>
+</tr>
+<tr class="row-even"><td>Aggregate</td>
+<td>bool</td>
+<td>False</td>
+<td>Filter by aggregated patch property</td>
+</tr>
+<tr class="row-odd"><td>ApplyBeam</td>
+<td>bool</td>
+<td>True</td>
+<td>If true, apparent fluxes will be used</td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>TRANSFER</strong></td>
+</tr>
+<tr class="row-odd"><td>PatchFile</td>
+<td>string</td>
+<td>patches.sky</td>
+<td>File with patches that will be transferred</td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>GROUP</strong></td>
+</tr>
+<tr class="row-odd"><td>Algorithm</td>
+<td>string</td>
+<td>tessellate</td>
+<td>One of tessellate, cluster, single, every</td>
+</tr>
+<tr class="row-even"><td>TargetFlux</td>
+<td>string</td>
+<td>10.0 Jy</td>
+<td>Target total flux of patches (tessellate only)</td>
+</tr>
+<tr class="row-odd"><td>NumClusters</td>
+<td>int</td>
+<td>100</td>
+<td>Number of clusters (cluster only)</td>
+</tr>
+<tr class="row-even"><td>ApplyBeam</td>
+<td>bool</td>
+<td>True</td>
+<td>If true, apparent fluxes will be used</td>
+</tr>
+<tr class="row-odd"><td colspan="4"><strong>UNGROUP</strong></td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>MOVE</strong></td>
+</tr>
+<tr class="row-odd"><td>Name</td>
+<td>string</td>
+<td>src1</td>
+<td>Name of source or patch to move</td>
+</tr>
+<tr class="row-even"><td>Position</td>
+<td>list of floats</td>
+<td>[12.3, 23.4]</td>
+<td>RA and Dec in degrees to move to</td>
+</tr>
+<tr class="row-odd"><td>Shift</td>
+<td>list of floats</td>
+<td>[0.001, 0.0]</td>
+<td>RA and Dec in degrees to shift by</td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>MERGE</strong></td>
+</tr>
+<tr class="row-odd"><td>Patches</td>
+<td>list of strings</td>
+<td>[bin1, bin2]</td>
+<td>Patch names to merge</td>
+</tr>
+<tr class="row-even"><td>Name</td>
+<td>string</td>
+<td>merged_patch</td>
+<td>Name of new merged patch</td>
+</tr>
+<tr class="row-odd"><td colspan="4"><strong>SETPATCHPOSITIONS</strong></td>
+</tr>
+<tr class="row-even"><td>Method</td>
+<td>string</td>
+<td>mid</td>
+<td>Set patch positions to mid, mean, or wmean positions</td>
+</tr>
+<tr class="row-odd"><td colspan="4"><strong>CONCATENATE</strong></td>
+</tr>
+<tr class="row-even"><td>Skymodel2</td>
+<td>string</td>
+<td>in2.sky</td>
+<td>Name of sky model to concatenate</td>
+</tr>
+<tr class="row-odd"><td>MatchBy</td>
+<td>string</td>
+<td>position</td>
+<td>Identify duplicates by position or name</td>
+</tr>
+<tr class="row-even"><td>Radius</td>
+<td>string</td>
+<td>30 arcsec</td>
+<td>Radius within which matches are identified</td>
+</tr>
+<tr class="row-odd"><td>Keep</td>
+<td>string</td>
+<td>all</td>
+<td>If two sources match, keep: all, from1, or from2</td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>ADD</strong></td>
+</tr>
+<tr class="row-odd"><td>Name</td>
+<td>string</td>
+<td>src1</td>
+<td>Name of source; required</td>
+</tr>
+<tr class="row-even"><td>Type</td>
+<td>string</td>
+<td>POINT</td>
+<td>Type; required</td>
+</tr>
+<tr class="row-odd"><td>Patch</td>
+<td>string</td>
+<td>new_patch</td>
+<td>Patch name; required if sky model has patches</td>
+</tr>
+<tr class="row-even"><td>RA</td>
+<td>float or string</td>
+<td>12:45:30.4</td>
+<td>RA; required</td>
+</tr>
+<tr class="row-odd"><td>Dec</td>
+<td>float or string</td>
+<td>+76.45.02.48</td>
+<td>Dec; required</td>
+</tr>
+<tr class="row-even"><td>I</td>
+<td>float</td>
+<td>0.69</td>
+<td>Flux in Jy; required</td>
+</tr>
+<tr class="row-odd"><td>AnyValidColumnName</td>
+<td> </td>
+<td>value</td>
+<td>Any valid column name can be specified</td>
+</tr>
+<tr class="row-even"><td colspan="4"><strong>PLOT</strong></td>
+</tr>
+</tbody>
+</table>
+</div>
+<div class="section" id="interactive-use-and-scripting">
+<h2>Interactive use and scripting<a class="headerlink" href="#interactive-use-and-scripting" title="Permalink to this headline">¶</a></h2>
+<p>LSMTool can also be used interactively (in IPython, for example) or in
+Python scripts without the need for a parset. To use LSMTool in a Python
+script or interpreter, import it as follows:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="kn">import</span> <span class="nn">lsmtool</span>
+</pre></div>
+</div>
+<p>A sky model can then be loaded with, e.g.:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span> <span class="o">=</span> <span class="n">lsmtool</span><span class="o">.</span><span class="n">load</span><span class="p">(</span><span class="s">'skymodel.sky'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>All of the operations described in Section [lsmtool:operations] are
+available as methods of the resulting sky model object (with the same
+name as the corresponding operation). For example, the following
+commands with duplicate the steps done in the example parset given in
+Section [lsmtool:parset]:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">select</span><span class="p">(</span><span class="s">'I > 1.0 mJy'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">add</span><span class="p">({</span><span class="s">'Name'</span><span class="p">:</span><span class="s">'new_source'</span><span class="p">,</span> <span class="s">'Type'</span><span class="p">:</span><span class="s">'POINT'</span><span class="p">,</span> <span class="s">'Ra'</span><span class="p">:</span><span class="mf">277.4232</span><span class="p">,</span> <span class="s">'Dec'</span><span class="p">:</span><span class="mf">48.3689</span><span class="p">,</span> <span class="s">'I'</span><span class="p">:</span><span class="mf">0.69</span><span class="p">})</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">group</span><span class="p">(</span><span class="n">algorithm</span><span class="o">=</span><span class="s">'tesselate'</span><span class="p">,</span> <span class="n">targetFlux</span><span class="o">=</span><span class="s">'10.0 Jy'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">setPatchPositions</span><span class="p">(</span><span class="n">method</span><span class="o">=</span><span class="s">'mid'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>In many cases, the methods accept parameters with the same names as
+those used in a parset (see the full documentation for details). The sky
+model can then written to a new file with:</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'grouped.sky'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>Additionally, sky models can be written out as ds9 region files and kvis
+annotation files (as well as all the formats supported by the
+astropy.table package, such at VOTable, HDF5, and FITS):</p>
+<div class="highlight-python"><div class="highlight"><pre><span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'outskymodel.reg'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'ds9'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'outskymodel.ann'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'kvis'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'outskymodel.fits'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'fits'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'outskymodel.hdf5'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'hdf5'</span><span class="p">)</span>
+<span class="gp">>>> </span><span class="n">LSM</span><span class="o">.</span><span class="n">write</span><span class="p">(</span><span class="s">'outskymodel.vo'</span><span class="p">,</span> <span class="n">format</span><span class="o">=</span><span class="s">'votable'</span><span class="p">)</span>
+</pre></div>
+</div>
+<p>In addition to the operations described above, a number of other methods
+are available:</p>
+<dl class="docutils">
+<dt>LSM.copy()</dt>
+<dd>: Return a copy of the sky model object</dd>
+<dt>LSM.info()</dt>
+<dd>: Print information about the sky model</dd>
+<dt>LSM.more()</dt>
+<dd>: Print the sky model to the screen, using more-like controls</dd>
+<dt>LSM.getColNames()</dt>
+<dd>: Returns a list of the column names in the sky model</dd>
+<dt>LSM.getColValues()</dt>
+<dd>: Returns a numpy array of column values</dd>
+<dt>LSM.getRowIndex()</dt>
+<dd>: Returns the row index or indices for a source or patch</dd>
+<dt>LSM.getRowValues()</dt>
+<dd>: Returns a table or row for a source or patch</dd>
+<dt>LSM.getPatchPositions()</dt>
+<dd>: Returns patch RA and Dec values</dd>
+<dt>LSM.getDefaltValues()</dt>
+<dd>: Returns column default values</dd>
+<dt>LSM.getPatchSizes()</dt>
+<dd>: Returns an array of patch sizes</dd>
+<dt>LSM.setColValues()</dt>
+<dd>: Sets column values</dd>
+<dt>LSM.setRowValues()</dt>
+<dd>: Sets row values</dd>
+<dt>LSM.setDefaultValues()</dt>
+<dd>: Sets default column values</dd>
+</dl>
+<p>For details on these methods, please see the full module documentation.</p>
+</div>
+</div>
+
+
+ </div>
+ </div>
+ </div>
+ <div class="sphinxsidebar">
+ <div class="sphinxsidebarwrapper">
+ <h3><a href="index.html">Table Of Contents</a></h3>
+ <ul>
+<li><a class="reference internal" href="#">LSMTool: the LOFAR Local Sky Model Tool</a><ul>
+<li><a class="reference internal" href="#usage">Usage</a></li>
+<li><a class="reference internal" href="#operations">Operations</a></li>
+<li><a class="reference internal" href="#example-parset">Example parset</a></li>
+<li><a class="reference internal" href="#interactive-use-and-scripting">Interactive use and scripting</a></li>
+</ul>
+</li>
+</ul>
+
+ <h4>Previous topic</h4>
+ <p class="topless"><a href="index.html"
+ title="previous chapter">Welcome to LSMTool’s documentation!</a></p>
+ <h4>Next topic</h4>
+ <p class="topless"><a href="lsmtool.html"
+ title="next chapter">LSMTool Module Documentation</a></p>
+ <h3>This Page</h3>
+ <ul class="this-page-menu">
+ <li><a href="_sources/overview.txt"
+ rel="nofollow">Show Source</a></li>
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+<div id="searchbox" style="display: none">
+ <h3>Quick search</h3>
+ <form class="search" action="search.html" method="get">
+ <input type="text" name="q" />
+ <input type="submit" value="Go" />
+ <input type="hidden" name="check_keywords" value="yes" />
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+ </form>
+ <p class="searchtip" style="font-size: 90%">
+ Enter search terms or a module, class or function name.
+ </p>
+</div>
+<script type="text/javascript">$('#searchbox').show(0);</script>
+ </div>
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+ <div class="related">
+ <h3>Navigation</h3>
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+ <a href="genindex.html" title="General Index"
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+ Created using <a href="http://sphinx-doc.org/">Sphinx</a> 1.2.2.
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+</html>
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+\gdef\HyperFirstAtBeginDocument#1{#1}
+\providecommand\HyField@AuxAddToFields[1]{}
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+\@writefile{toc}{\select@language{english}}
+\@writefile{lof}{\select@language{english}}
+\@writefile{lot}{\select@language{english}}
+\newlabel{index::doc}{{}{1}{\relax }{section*.2}{}}
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+Scanning style file ./python.ist......done (6 attributes redefined, 0 ignored).
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+Transcript written in LSMTool.ilg.
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+\title{LSMTool Documentation}
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+\author{David Rafferty}
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+\expandafter\def\csname PYG@tok@mi\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.13,0.50,0.31}{##1}}}
+\expandafter\def\csname PYG@tok@kn\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.44,0.13}{##1}}}
+\expandafter\def\csname PYG@tok@o\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.40,0.40,0.40}{##1}}}
+\expandafter\def\csname PYG@tok@kr\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.44,0.13}{##1}}}
+\expandafter\def\csname PYG@tok@s\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.25,0.44,0.63}{##1}}}
+\expandafter\def\csname PYG@tok@kp\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.00,0.44,0.13}{##1}}}
+\expandafter\def\csname PYG@tok@w\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.73,0.73,0.73}{##1}}}
+\expandafter\def\csname PYG@tok@kt\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.56,0.13,0.00}{##1}}}
+\expandafter\def\csname PYG@tok@sc\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.25,0.44,0.63}{##1}}}
+\expandafter\def\csname PYG@tok@sb\endcsname{\def\PYG@tc##1{\textcolor[rgb]{0.25,0.44,0.63}{##1}}}
+\expandafter\def\csname PYG@tok@k\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.00,0.44,0.13}{##1}}}
+\expandafter\def\csname PYG@tok@se\endcsname{\let\PYG@bf=\textbf\def\PYG@tc##1{\textcolor[rgb]{0.25,0.44,0.63}{##1}}}
+\expandafter\def\csname PYG@tok@sd\endcsname{\let\PYG@it=\textit\def\PYG@tc##1{\textcolor[rgb]{0.25,0.44,0.63}{##1}}}
+
+\def\PYGZbs{\char`\\}
+\def\PYGZus{\char`\_}
+\def\PYGZob{\char`\{}
+\def\PYGZcb{\char`\}}
+\def\PYGZca{\char`\^}
+\def\PYGZam{\char`\&}
+\def\PYGZlt{\char`\<}
+\def\PYGZgt{\char`\>}
+\def\PYGZsh{\char`\#}
+\def\PYGZpc{\char`\%}
+\def\PYGZdl{\char`\$}
+\def\PYGZhy{\char`\-}
+\def\PYGZsq{\char`\'}
+\def\PYGZdq{\char`\"}
+\def\PYGZti{\char`\~}
+% for compatibility with earlier versions
+\def\PYGZat{@}
+\def\PYGZlb{[}
+\def\PYGZrb{]}
+\makeatother
+
+\begin{document}
+
+\maketitle
+\tableofcontents
+\phantomsection\label{index::doc}
+
+
+LSMTool is a Python package which allow the manipulation of sky models in the \code{makesourcedb} format understood by BBS. Note that LSMTool is still in beta. Please report bugs to \code{drafferty@hs.uni-hamburg.de}. To initialize your environment for LSMTool, users on CEP1 and CEP2 should run the following commands:
+
+\begin{Verbatim}[commandchars=\\\{\}]
+use LofIm
+source \PYGZti{}rafferty/init\PYGZus{}lsmtool
+\end{Verbatim}
+
+Note that the Pythonlibs LOFAR package includes an older version of astropy that conflicts with LSMTool and cannot be used in conjunction with it.
+
+
+\chapter{Indices and tables}
+\label{index:welcome-to-lsmtool-s-documentation}\label{index:indices-and-tables}\begin{itemize}
+\item {}
+\emph{genindex}
+
+\item {}
+\emph{modindex}
+
+\item {}
+\emph{search}
+
+\end{itemize}
+
+
+
+\renewcommand{\indexname}{Index}
+\printindex
+\end{document}
diff --git a/docs/build/latex/LSMTool.toc b/docs/build/latex/LSMTool.toc
new file mode 100644
index 0000000000000000000000000000000000000000..6d091978bed213ec5a250dea105579bad056fa75
--- /dev/null
+++ b/docs/build/latex/LSMTool.toc
@@ -0,0 +1,2 @@
+\select@language {english}
+\contentsline {chapter}{\numberline {1}Indices and tables}{3}{chapter.1}
diff --git a/docs/build/latex/Makefile b/docs/build/latex/Makefile
new file mode 100644
index 0000000000000000000000000000000000000000..6b87ad8814ccb4cbe23593049f8a909d38a1c9e3
--- /dev/null
+++ b/docs/build/latex/Makefile
@@ -0,0 +1,66 @@
+# Makefile for Sphinx LaTeX output
+
+ALLDOCS = $(basename $(wildcard *.tex))
+ALLPDF = $(addsuffix .pdf,$(ALLDOCS))
+ALLDVI = $(addsuffix .dvi,$(ALLDOCS))
+
+# Prefix for archive names
+ARCHIVEPRREFIX =
+# Additional LaTeX options
+LATEXOPTS =
+
+all: $(ALLPDF)
+all-pdf: $(ALLPDF)
+all-dvi: $(ALLDVI)
+all-ps: all-dvi
+ for f in *.dvi; do dvips $$f; done
+
+all-pdf-ja:
+ for f in *.pdf *.png *.gif *.jpg *.jpeg; do extractbb $$f; done
+ for f in *.tex; do platex -kanji=utf8 $(LATEXOPTS) $$f; done
+ for f in *.tex; do platex -kanji=utf8 $(LATEXOPTS) $$f; done
+ for f in *.tex; do platex -kanji=utf8 $(LATEXOPTS) $$f; done
+ -for f in *.idx; do mendex -U -f -d "`basename $$f .idx`.dic" -s python.ist $$f; done
+ for f in *.tex; do platex -kanji=utf8 $(LATEXOPTS) $$f; done
+ for f in *.tex; do platex -kanji=utf8 $(LATEXOPTS) $$f; done
+ for f in *.dvi; do dvipdfmx $$f; done
+
+zip: all-$(FMT)
+ mkdir $(ARCHIVEPREFIX)docs-$(FMT)
+ cp $(ALLPDF) $(ARCHIVEPREFIX)docs-$(FMT)
+ zip -q -r -9 $(ARCHIVEPREFIX)docs-$(FMT).zip $(ARCHIVEPREFIX)docs-$(FMT)
+ rm -r $(ARCHIVEPREFIX)docs-$(FMT)
+
+tar: all-$(FMT)
+ mkdir $(ARCHIVEPREFIX)docs-$(FMT)
+ cp $(ALLPDF) $(ARCHIVEPREFIX)docs-$(FMT)
+ tar cf $(ARCHIVEPREFIX)docs-$(FMT).tar $(ARCHIVEPREFIX)docs-$(FMT)
+ rm -r $(ARCHIVEPREFIX)docs-$(FMT)
+
+bz2: tar
+ bzip2 -9 -k $(ARCHIVEPREFIX)docs-$(FMT).tar
+
+# The number of LaTeX runs is quite conservative, but I don't expect it
+# to get run often, so the little extra time won't hurt.
+%.dvi: %.tex
+ latex $(LATEXOPTS) '$<'
+ latex $(LATEXOPTS) '$<'
+ latex $(LATEXOPTS) '$<'
+ -makeindex -s python.ist '$(basename $<).idx'
+ latex $(LATEXOPTS) '$<'
+ latex $(LATEXOPTS) '$<'
+
+%.pdf: %.tex
+ pdflatex $(LATEXOPTS) '$<'
+ pdflatex $(LATEXOPTS) '$<'
+ pdflatex $(LATEXOPTS) '$<'
+ -makeindex -s python.ist '$(basename $<).idx'
+ pdflatex $(LATEXOPTS) '$<'
+ pdflatex $(LATEXOPTS) '$<'
+
+clean:
+ rm -f *.dvi *.log *.ind *.aux *.toc *.syn *.idx *.out *.ilg *.pla
+
+.PHONY: all all-pdf all-dvi all-ps clean
+.PHONY: all-pdf-ja
+
diff --git a/docs/build/latex/fncychap.sty b/docs/build/latex/fncychap.sty
new file mode 100644
index 0000000000000000000000000000000000000000..9a56c04ed4223ce77e463eea87755151f5d4864c
--- /dev/null
+++ b/docs/build/latex/fncychap.sty
@@ -0,0 +1,683 @@
+%%% Copyright Ulf A. Lindgren
+%%%
+%%% Note Premission is granted to modify this file under
+%%% the condition that it is saved using another
+%%% file and package name.
+%%%
+%%% Revision 1.1 (1997)
+%%%
+%%% Jan. 8th Modified package name base date option
+%%% Jan. 22th Modified FmN and FmTi for error in book.cls
+%%% \MakeUppercase{#}->{\MakeUppercase#}
+%%% Apr. 6th Modified Lenny option to prevent undesired
+%%% skip of line.
+%%% Nov. 8th Fixed \@chapapp for AMS
+%%%
+%%% Revision 1.2 (1998)
+%%%
+%%% Feb. 11th Fixed appendix problem related to Bjarne
+%%% Aug. 11th Fixed problem related to 11pt and 12pt
+%%% suggested by Tomas Lundberg. THANKS!
+%%%
+%%% Revision 1.3 (2004)
+%%% Sep. 20th problem with frontmatter, mainmatter and
+%%% backmatter, pointed out by Lapo Mori
+%%%
+%%% Revision 1.31 (2004)
+%%% Sep. 21th problem with the Rejne definition streched text
+%%% caused ugly gaps in the vrule aligned with the title
+%%% text. Kindly pointed out to me by Hendri Adriaens
+%%%
+%%% Revision 1.32 (2005)
+%%% Jun. 23th compatibility problem with the KOMA class 'scrbook.cls'
+%%% a remedy is a redefinition of '\@schapter' in
+%%% line with that used in KOMA. The problem was pointed
+%%% out to me by Mikkel Holm Olsen
+%%%
+%%% Revision 1.33 (2005)
+%%% Aug. 9th misspelled ``TWELV'' corrected, the error was pointed
+%%% out to me by George Pearson
+%%%
+%%% Revision 1.34 (2007)
+%%% Added an alternative to Lenny provided by Peter
+%%% Osborne (2005-11-28)
+%%% Corrected front, main and back matter, based on input
+%%% from Bas van Gils (2006-04-24)
+%%% Jul. 30th Added Bjornstrup option provided by Jean-Marc
+%%% Francois (2007-01-05).
+%%% Reverted to \MakeUppercase{#} see rev 1.1, solved
+%%% problem with MakeUppercase and MakeLowercase pointed
+%%% out by Marco Feuerstein (2007-06-06)
+
+
+%%% Last modified Jul. 2007
+
+\NeedsTeXFormat{LaTeX2e}[1995/12/01]
+\ProvidesPackage{fncychap}
+ [2007/07/30 v1.34
+ LaTeX package (Revised chapters)]
+
+%%%% For conditional inclusion of color
+\newif\ifusecolor
+\usecolorfalse
+
+
+
+%%%% DEFINITION OF Chapapp variables
+\newcommand{\CNV}{\huge\bfseries}
+\newcommand{\ChNameVar}[1]{\renewcommand{\CNV}{#1}}
+
+
+%%%% DEFINITION OF TheChapter variables
+\newcommand{\CNoV}{\huge\bfseries}
+\newcommand{\ChNumVar}[1]{\renewcommand{\CNoV}{#1}}
+
+\newif\ifUCN
+\UCNfalse
+\newif\ifLCN
+\LCNfalse
+\def\ChNameLowerCase{\LCNtrue\UCNfalse}
+\def\ChNameUpperCase{\UCNtrue\LCNfalse}
+\def\ChNameAsIs{\UCNfalse\LCNfalse}
+
+%%%%% Fix for AMSBook 971008
+
+\@ifundefined{@chapapp}{\let\@chapapp\chaptername}{}
+
+
+%%%%% Fix for Bjarne and appendix 980211
+
+\newif\ifinapp
+\inappfalse
+\renewcommand\appendix{\par
+ \setcounter{chapter}{0}%
+ \setcounter{section}{0}%
+ \inapptrue%
+ \renewcommand\@chapapp{\appendixname}%
+ \renewcommand\thechapter{\@Alph\c@chapter}}
+
+%%%%% Fix for frontmatter, mainmatter, and backmatter 040920
+
+\@ifundefined{@mainmatter}{\newif\if@mainmatter \@mainmattertrue}{}
+
+%%%%%
+
+
+
+\newcommand{\FmN}[1]{%
+\ifUCN
+ {\MakeUppercase{#1}}\LCNfalse
+\else
+ \ifLCN
+ {\MakeLowercase{#1}}\UCNfalse
+ \else #1
+ \fi
+\fi}
+
+
+%%%% DEFINITION OF Title variables
+\newcommand{\CTV}{\Huge\bfseries}
+\newcommand{\ChTitleVar}[1]{\renewcommand{\CTV}{#1}}
+
+%%%% DEFINITION OF the basic rule width
+\newlength{\RW}
+\setlength{\RW}{1pt}
+\newcommand{\ChRuleWidth}[1]{\setlength{\RW}{#1}}
+
+\newif\ifUCT
+\UCTfalse
+\newif\ifLCT
+\LCTfalse
+\def\ChTitleLowerCase{\LCTtrue\UCTfalse}
+\def\ChTitleUpperCase{\UCTtrue\LCTfalse}
+\def\ChTitleAsIs{\UCTfalse\LCTfalse}
+\newcommand{\FmTi}[1]{%
+\ifUCT
+ {\MakeUppercase{#1}}\LCTfalse
+\else
+ \ifLCT
+ {\MakeLowercase{#1}}\UCTfalse
+ \else {#1}
+ \fi
+\fi}
+
+
+
+\newlength{\mylen}
+\newlength{\myhi}
+\newlength{\px}
+\newlength{\py}
+\newlength{\pyy}
+\newlength{\pxx}
+
+
+\def\mghrulefill#1{\leavevmode\leaders\hrule\@height #1\hfill\kern\z@}
+
+\newcommand{\DOCH}{%
+ \CNV\FmN{\@chapapp}\space \CNoV\thechapter
+ \par\nobreak
+ \vskip 20\p@
+ }
+\newcommand{\DOTI}[1]{%
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@
+ }
+\newcommand{\DOTIS}[1]{%
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@
+ }
+
+%%%%%% SONNY DEF
+
+\DeclareOption{Sonny}{%
+ \ChNameVar{\Large\sf}
+ \ChNumVar{\Huge}
+ \ChTitleVar{\Large\sf}
+ \ChRuleWidth{0.5pt}
+ \ChNameUpperCase
+ \renewcommand{\DOCH}{%
+ \raggedleft
+ \CNV\FmN{\@chapapp}\space \CNoV\thechapter
+ \par\nobreak
+ \vskip 40\p@}
+ \renewcommand{\DOTI}[1]{%
+ \CTV\raggedleft\mghrulefill{\RW}\par\nobreak
+ \vskip 5\p@
+ \CTV\FmTi{#1}\par\nobreak
+ \mghrulefill{\RW}\par\nobreak
+ \vskip 40\p@}
+ \renewcommand{\DOTIS}[1]{%
+ \CTV\raggedleft\mghrulefill{\RW}\par\nobreak
+ \vskip 5\p@
+ \CTV\FmTi{#1}\par\nobreak
+ \mghrulefill{\RW}\par\nobreak
+ \vskip 40\p@}
+}
+
+%%%%%% LENNY DEF
+
+\DeclareOption{Lenny}{%
+
+ \ChNameVar{\fontsize{14}{16}\usefont{OT1}{phv}{m}{n}\selectfont}
+ \ChNumVar{\fontsize{60}{62}\usefont{OT1}{ptm}{m}{n}\selectfont}
+ \ChTitleVar{\Huge\bfseries\rm}
+ \ChRuleWidth{1pt}
+ \renewcommand{\DOCH}{%
+ \settowidth{\px}{\CNV\FmN{\@chapapp}}
+ \addtolength{\px}{2pt}
+ \settoheight{\py}{\CNV\FmN{\@chapapp}}
+ \addtolength{\py}{1pt}
+
+ \settowidth{\mylen}{\CNV\FmN{\@chapapp}\space\CNoV\thechapter}
+ \addtolength{\mylen}{1pt}
+ \settowidth{\pxx}{\CNoV\thechapter}
+ \addtolength{\pxx}{-1pt}
+
+ \settoheight{\pyy}{\CNoV\thechapter}
+ \addtolength{\pyy}{-2pt}
+ \setlength{\myhi}{\pyy}
+ \addtolength{\myhi}{-1\py}
+ \par
+ \parbox[b]{\textwidth}{%
+ \rule[\py]{\RW}{\myhi}%
+ \hskip -\RW%
+ \rule[\pyy]{\px}{\RW}%
+ \hskip -\px%
+ \raggedright%
+ \CNV\FmN{\@chapapp}\space\CNoV\thechapter%
+ \hskip1pt%
+ \mghrulefill{\RW}%
+ \rule{\RW}{\pyy}\par\nobreak%
+ \vskip -\baselineskip%
+ \vskip -\pyy%
+ \hskip \mylen%
+ \mghrulefill{\RW}\par\nobreak%
+ \vskip \pyy}%
+ \vskip 20\p@}
+
+
+ \renewcommand{\DOTI}[1]{%
+ \raggedright
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@}
+
+ \renewcommand{\DOTIS}[1]{%
+ \raggedright
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@}
+ }
+
+%%%%%% Peter Osbornes' version of LENNY DEF
+
+\DeclareOption{PetersLenny}{%
+
+% five new lengths
+\newlength{\bl} % bottom left : orig \space
+\setlength{\bl}{6pt}
+\newcommand{\BL}[1]{\setlength{\bl}{#1}}
+\newlength{\br} % bottom right : orig 1pt
+\setlength{\br}{1pt}
+\newcommand{\BR}[1]{\setlength{\br}{#1}}
+\newlength{\tl} % top left : orig 2pt
+\setlength{\tl}{2pt}
+\newcommand{\TL}[1]{\setlength{\tl}{#1}}
+\newlength{\trr} % top right :orig 1pt
+\setlength{\trr}{1pt}
+\newcommand{\TR}[1]{\setlength{\trr}{#1}}
+\newlength{\blrule} % top right :orig 1pt
+\setlength{\trr}{0pt}
+\newcommand{\BLrule}[1]{\setlength{\blrule}{#1}}
+
+
+ \ChNameVar{\fontsize{14}{16}\usefont{OT1}{phv}{m}{n}\selectfont}
+ \ChNumVar{\fontsize{60}{62}\usefont{OT1}{ptm}{m}{n}\selectfont}
+ \ChTitleVar{\Huge\bfseries\rm}
+ \ChRuleWidth{1pt}
+\renewcommand{\DOCH}{%
+
+
+%%%%%%% tweaks for 1--9 and A--Z
+\ifcase\c@chapter\relax%
+\or\BL{-3pt}\TL{-4pt}\BR{0pt}\TR{-6pt}%1
+\or\BL{0pt}\TL{-4pt}\BR{2pt}\TR{-4pt}%2
+\or\BL{0pt}\TL{-4pt}\BR{2pt}\TR{-4pt}%3
+\or\BL{0pt}\TL{5pt}\BR{2pt}\TR{-4pt}%4
+\or\BL{0pt}\TL{3pt}\BR{2pt}\TR{-4pt}%5
+\or\BL{-1pt}\TL{0pt}\BR{2pt}\TR{-2pt}%6
+\or\BL{0pt}\TL{-3pt}\BR{2pt}\TR{-2pt}%7
+\or\BL{0pt}\TL{-3pt}\BR{2pt}\TR{-2pt}%8
+\or\BL{0pt}\TL{-3pt}\BR{-4pt}\TR{-2pt}%9
+\or\BL{-3pt}\TL{-3pt}\BR{2pt}\TR{-7pt}%10
+\or\BL{-6pt}\TL{-6pt}\BR{0pt}\TR{-9pt}%11
+\or\BL{-6pt}\TL{-6pt}\BR{2pt}\TR{-7pt}%12
+\or\BL{-5pt}\TL{-5pt}\BR{0pt}\TR{-9pt}%13
+\or\BL{-6pt}\TL{-6pt}\BR{0pt}\TR{-9pt}%14
+\or\BL{-3pt}\TL{-3pt}\BR{3pt}\TR{-6pt}%15
+\or\BL{-3pt}\TL{-3pt}\BR{3pt}\TR{-6pt}%16
+\or\BL{-5pt}\TL{-3pt}\BR{-8pt}\TR{-6pt}%17
+\or\BL{-5pt}\TL{-5pt}\BR{0pt}\TR{-9pt}%18
+\or\BL{-3pt}\TL{-3pt}\BR{-6pt}\TR{-9pt}%19
+\or\BL{0pt}\TL{0pt}\BR{0pt}\TR{-5pt}%20
+\fi
+
+\ifinapp\ifcase\c@chapter\relax%
+\or\BL{0pt}\TL{14pt}\BR{5pt}\TR{-19pt}%A
+\or\BL{0pt}\TL{-5pt}\BR{-3pt}\TR{-8pt}%B
+\or\BL{-3pt}\TL{-2pt}\BR{1pt}\TR{-6pt}\BLrule{0pt}%C
+\or\BL{0pt}\TL{-5pt}\BR{-3pt}\TR{-8pt}\BLrule{0pt}%D
+\or\BL{0pt}\TL{-5pt}\BR{2pt}\TR{-3pt}%E
+\or\BL{0pt}\TL{-5pt}\BR{-10pt}\TR{-1pt}%F
+\or\BL{-3pt}\TL{0pt}\BR{0pt}\TR{-7pt}%G
+\or\BL{0pt}\TL{-5pt}\BR{3pt}\TR{-1pt}%H
+\or\BL{0pt}\TL{-5pt}\BR{3pt}\TR{-1pt}%I
+\or\BL{2pt}\TL{0pt}\BR{-3pt}\TR{1pt}%J
+\or\BL{0pt}\TL{-5pt}\BR{3pt}\TR{-1pt}%K
+\or\BL{0pt}\TL{-5pt}\BR{2pt}\TR{-19pt}%L
+\or\BL{0pt}\TL{-5pt}\BR{3pt}\TR{-1pt}%M
+\or\BL{0pt}\TL{-5pt}\BR{-2pt}\TR{-1pt}%N
+\or\BL{-3pt}\TL{-2pt}\BR{-3pt}\TR{-11pt}%O
+\or\BL{0pt}\TL{-5pt}\BR{-9pt}\TR{-3pt}%P
+\or\BL{-3pt}\TL{-2pt}\BR{-3pt}\TR{-11pt}%Q
+\or\BL{0pt}\TL{-5pt}\BR{4pt}\TR{-8pt}%R
+\or\BL{-2pt}\TL{-2pt}\BR{-2pt}\TR{-7pt}%S
+\or\BL{-3pt}\TL{0pt}\BR{-5pt}\TR{4pt}\BLrule{8pt}%T
+\or\BL{-7pt}\TL{-11pt}\BR{-5pt}\TR{-7pt}\BLrule{0pt}%U
+\or\BL{-14pt}\TL{-5pt}\BR{-14pt}\TR{-1pt}\BLrule{14pt}%V
+\or\BL{-10pt}\TL{-9pt}\BR{-13pt}\TR{-3pt}\BLrule{7pt}%W
+\or\BL{0pt}\TL{-5pt}\BR{3pt}\TR{-1pt}\BLrule{0pt}%X
+\or\BL{-6pt}\TL{-4pt}\BR{-7pt}\TR{1pt}\BLrule{7pt}%Y
+\or\BL{0pt}\TL{-5pt}\BR{3pt}\TR{-1pt}\BLrule{0pt}%Z
+\fi\fi
+%%%%%%%
+ \settowidth{\px}{\CNV\FmN{\@chapapp}}
+ \addtolength{\px}{\tl} %MOD change 2pt to \tl
+ \settoheight{\py}{\CNV\FmN{\@chapapp}}
+ \addtolength{\py}{1pt}
+
+ \settowidth{\mylen}{\CNV\FmN{\@chapapp}\space\CNoV\thechapter}
+ \addtolength{\mylen}{\trr}% MOD change 1pt to \tr
+ \settowidth{\pxx}{\CNoV\thechapter}
+ \addtolength{\pxx}{-1pt}
+
+ \settoheight{\pyy}{\CNoV\thechapter}
+ \addtolength{\pyy}{-2pt}
+ \setlength{\myhi}{\pyy}
+ \addtolength{\myhi}{-1\py}
+ \par
+ \parbox[b]{\textwidth}{%
+ \rule[\py]{\RW}{\myhi}%
+ \hskip -\RW%
+ \rule[\pyy]{\px}{\RW}%
+ \hskip -\px%
+ \raggedright%
+ \CNV\FmN{\@chapapp}\rule{\blrule}{\RW}\hskip\bl\CNoV\thechapter%MOD
+% \CNV\FmN{\@chapapp}\space\CNoV\thechapter %ORIGINAL
+ \hskip\br% %MOD 1pt to \br
+ \mghrulefill{\RW}%
+ \rule{\RW}{\pyy}\par\nobreak%
+ \vskip -\baselineskip%
+ \vskip -\pyy%
+ \hskip \mylen%
+ \mghrulefill{\RW}\par\nobreak%
+ \vskip \pyy}%
+ \vskip 20\p@}
+
+
+ \renewcommand{\DOTI}[1]{%
+ \raggedright
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@}
+
+ \renewcommand{\DOTIS}[1]{%
+ \raggedright
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@}
+ }
+
+
+%
+
+
+%%%%%% BJORNSTRUP DEF
+
+\DeclareOption{Bjornstrup}{%
+ \usecolortrue
+ % pzc (Zapf Chancelery) is nice. ppl (Palatino) is cool too.
+ \ChNumVar{\fontsize{76}{80}\usefont{OT1}{pzc}{m}{n}\selectfont}
+ \ChTitleVar{\raggedleft\Large\sffamily\bfseries}
+
+ \setlength{\myhi}{10pt} % Space between grey box border and text
+ \setlength{\mylen}{\textwidth}
+ \addtolength{\mylen}{-2\myhi}
+ \renewcommand{\DOCH}{%
+ \settowidth{\py}{\CNoV\thechapter}
+ \addtolength{\py}{-10pt} % Amount of space by which the
+% % number is shifted right
+ \fboxsep=0pt%
+ \colorbox[gray]{.85}{\rule{0pt}{40pt}\parbox[b]{\textwidth}{\hfill}}%
+ \kern-\py\raise20pt%
+ \hbox{\color[gray]{.5}\CNoV\thechapter}\\%
+ }
+
+ \renewcommand{\DOTI}[1]{%
+ \nointerlineskip\raggedright%
+ \fboxsep=\myhi%
+ \vskip-1ex%
+ \colorbox[gray]{.85}{\parbox[t]{\mylen}{\CTV\FmTi{#1}}}\par\nobreak%
+ \vskip 40\p@%
+ }
+
+ \renewcommand{\DOTIS}[1]{%
+ \fboxsep=0pt
+ \colorbox[gray]{.85}{\rule{0pt}{40pt}\parbox[b]{\textwidth}{\hfill}}\\%
+ \nointerlineskip\raggedright%
+ \fboxsep=\myhi%
+ \colorbox[gray]{.85}{\parbox[t]{\mylen}{\CTV\FmTi{#1}}}\par\nobreak%
+ \vskip 40\p@%
+ }
+}
+
+
+%%%%%%% GLENN DEF
+
+
+\DeclareOption{Glenn}{%
+ \ChNameVar{\bfseries\Large\sf}
+ \ChNumVar{\Huge}
+ \ChTitleVar{\bfseries\Large\rm}
+ \ChRuleWidth{1pt}
+ \ChNameUpperCase
+ \ChTitleUpperCase
+ \renewcommand{\DOCH}{%
+ \settoheight{\myhi}{\CTV\FmTi{Test}}
+ \setlength{\py}{\baselineskip}
+ \addtolength{\py}{\RW}
+ \addtolength{\py}{\myhi}
+ \setlength{\pyy}{\py}
+ \addtolength{\pyy}{-1\RW}
+
+ \raggedright
+ \CNV\FmN{\@chapapp}\space\CNoV\thechapter
+ \hskip 3pt\mghrulefill{\RW}\rule[-1\pyy]{2\RW}{\py}\par\nobreak}
+
+ \renewcommand{\DOTI}[1]{%
+ \addtolength{\pyy}{-4pt}
+ \settoheight{\myhi}{\CTV\FmTi{#1}}
+ \addtolength{\myhi}{\py}
+ \addtolength{\myhi}{-1\RW}
+ \vskip -1\pyy
+ \rule{2\RW}{\myhi}\mghrulefill{\RW}\hskip 2pt
+ \raggedleft\CTV\FmTi{#1}\par\nobreak
+ \vskip 80\p@}
+
+\newlength{\backskip}
+ \renewcommand{\DOTIS}[1]{%
+% \setlength{\py}{10pt}
+% \setlength{\pyy}{\py}
+% \addtolength{\pyy}{\RW}
+% \setlength{\myhi}{\baselineskip}
+% \addtolength{\myhi}{\pyy}
+% \mghrulefill{\RW}\rule[-1\py]{2\RW}{\pyy}\par\nobreak
+% \addtolength{}{}
+%\vskip -1\baselineskip
+% \rule{2\RW}{\myhi}\mghrulefill{\RW}\hskip 2pt
+% \raggedleft\CTV\FmTi{#1}\par\nobreak
+% \vskip 60\p@}
+%% Fix suggested by Tomas Lundberg
+ \setlength{\py}{25pt} % eller vad man vill
+ \setlength{\pyy}{\py}
+ \setlength{\backskip}{\py}
+ \addtolength{\backskip}{2pt}
+ \addtolength{\pyy}{\RW}
+ \setlength{\myhi}{\baselineskip}
+ \addtolength{\myhi}{\pyy}
+ \mghrulefill{\RW}\rule[-1\py]{2\RW}{\pyy}\par\nobreak
+ \vskip -1\backskip
+ \rule{2\RW}{\myhi}\mghrulefill{\RW}\hskip 3pt %
+ \raggedleft\CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@}
+ }
+
+%%%%%%% CONNY DEF
+
+\DeclareOption{Conny}{%
+ \ChNameUpperCase
+ \ChTitleUpperCase
+ \ChNameVar{\centering\Huge\rm\bfseries}
+ \ChNumVar{\Huge}
+ \ChTitleVar{\centering\Huge\rm}
+ \ChRuleWidth{2pt}
+
+ \renewcommand{\DOCH}{%
+ \mghrulefill{3\RW}\par\nobreak
+ \vskip -0.5\baselineskip
+ \mghrulefill{\RW}\par\nobreak
+ \CNV\FmN{\@chapapp}\space \CNoV\thechapter
+ \par\nobreak
+ \vskip -0.5\baselineskip
+ }
+ \renewcommand{\DOTI}[1]{%
+ \mghrulefill{\RW}\par\nobreak
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 60\p@
+ }
+ \renewcommand{\DOTIS}[1]{%
+ \mghrulefill{\RW}\par\nobreak
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 60\p@
+ }
+ }
+
+%%%%%%% REJNE DEF
+
+\DeclareOption{Rejne}{%
+
+ \ChNameUpperCase
+ \ChTitleUpperCase
+ \ChNameVar{\centering\Large\rm}
+ \ChNumVar{\Huge}
+ \ChTitleVar{\centering\Huge\rm}
+ \ChRuleWidth{1pt}
+ \renewcommand{\DOCH}{%
+ \settoheight{\py}{\CNoV\thechapter}
+ \parskip=0pt plus 1pt % Set parskip to default, just in case v1.31
+ \addtolength{\py}{-1pt}
+ \CNV\FmN{\@chapapp}\par\nobreak
+ \vskip 20\p@
+ \setlength{\myhi}{2\baselineskip}
+ \setlength{\px}{\myhi}
+ \addtolength{\px}{-1\RW}
+ \rule[-1\px]{\RW}{\myhi}\mghrulefill{\RW}\hskip
+ 10pt\raisebox{-0.5\py}{\CNoV\thechapter}\hskip 10pt\mghrulefill{\RW}\rule[-1\px]{\RW}{\myhi}\par\nobreak
+ \vskip -3\p@% Added -2pt vskip to correct for streched text v1.31
+ }
+ \renewcommand{\DOTI}[1]{%
+ \setlength{\mylen}{\textwidth}
+ \parskip=0pt plus 1pt % Set parskip to default, just in case v1.31
+ \addtolength{\mylen}{-2\RW}
+ {\vrule width\RW}\parbox{\mylen}{\CTV\FmTi{#1}}{\vrule width\RW}\par\nobreak%
+ \vskip -3pt\rule{\RW}{2\baselineskip}\mghrulefill{\RW}\rule{\RW}{2\baselineskip}%
+ \vskip 60\p@% Added -2pt in vskip to correct for streched text v1.31
+ }
+ \renewcommand{\DOTIS}[1]{%
+ \setlength{\py}{\fboxrule}
+ \setlength{\fboxrule}{\RW}
+ \setlength{\mylen}{\textwidth}
+ \addtolength{\mylen}{-2\RW}
+ \fbox{\parbox{\mylen}{\vskip 2\baselineskip\CTV\FmTi{#1}\par\nobreak\vskip \baselineskip}}
+ \setlength{\fboxrule}{\py}
+ \vskip 60\p@
+ }
+ }
+
+
+%%%%%%% BJARNE DEF
+
+\DeclareOption{Bjarne}{%
+ \ChNameUpperCase
+ \ChTitleUpperCase
+ \ChNameVar{\raggedleft\normalsize\rm}
+ \ChNumVar{\raggedleft \bfseries\Large}
+ \ChTitleVar{\raggedleft \Large\rm}
+ \ChRuleWidth{1pt}
+
+
+%% Note thechapter -> c@chapter fix appendix bug
+%% Fixed misspelled 12
+
+ \newcounter{AlphaCnt}
+ \newcounter{AlphaDecCnt}
+ \newcommand{\AlphaNo}{%
+ \ifcase\number\theAlphaCnt
+ \ifnum\c@chapter=0
+ ZERO\else{}\fi
+ \or ONE\or TWO\or THREE\or FOUR\or FIVE
+ \or SIX\or SEVEN\or EIGHT\or NINE\or TEN
+ \or ELEVEN\or TWELVE\or THIRTEEN\or FOURTEEN\or FIFTEEN
+ \or SIXTEEN\or SEVENTEEN\or EIGHTEEN\or NINETEEN\fi
+}
+
+ \newcommand{\AlphaDecNo}{%
+ \setcounter{AlphaDecCnt}{0}
+ \@whilenum\number\theAlphaCnt>0\do
+ {\addtocounter{AlphaCnt}{-10}
+ \addtocounter{AlphaDecCnt}{1}}
+ \ifnum\number\theAlphaCnt=0
+ \else
+ \addtocounter{AlphaDecCnt}{-1}
+ \addtocounter{AlphaCnt}{10}
+ \fi
+
+
+ \ifcase\number\theAlphaDecCnt\or TEN\or TWENTY\or THIRTY\or
+ FORTY\or FIFTY\or SIXTY\or SEVENTY\or EIGHTY\or NINETY\fi
+ }
+ \newcommand{\TheAlphaChapter}{%
+
+ \ifinapp
+ \thechapter
+ \else
+ \setcounter{AlphaCnt}{\c@chapter}
+ \ifnum\c@chapter<20
+ \AlphaNo
+ \else
+ \AlphaDecNo\AlphaNo
+ \fi
+ \fi
+ }
+ \renewcommand{\DOCH}{%
+ \mghrulefill{\RW}\par\nobreak
+ \CNV\FmN{\@chapapp}\par\nobreak
+ \CNoV\TheAlphaChapter\par\nobreak
+ \vskip -1\baselineskip\vskip 5pt\mghrulefill{\RW}\par\nobreak
+ \vskip 20\p@
+ }
+ \renewcommand{\DOTI}[1]{%
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@
+ }
+ \renewcommand{\DOTIS}[1]{%
+ \CTV\FmTi{#1}\par\nobreak
+ \vskip 40\p@
+ }
+}
+
+\DeclareOption*{%
+ \PackageWarning{fancychapter}{unknown style option}
+ }
+
+\ProcessOptions* \relax
+
+\ifusecolor
+ \RequirePackage{color}
+\fi
+\def\@makechapterhead#1{%
+ \vspace*{50\p@}%
+ {\parindent \z@ \raggedright \normalfont
+ \ifnum \c@secnumdepth >\m@ne
+ \if@mainmatter%%%%% Fix for frontmatter, mainmatter, and backmatter 040920
+ \DOCH
+ \fi
+ \fi
+ \interlinepenalty\@M
+ \if@mainmatter%%%%% Fix for frontmatter, mainmatter, and backmatter 060424
+ \DOTI{#1}%
+ \else%
+ \DOTIS{#1}%
+ \fi
+ }}
+
+
+%%% Begin: To avoid problem with scrbook.cls (fncychap version 1.32)
+
+%%OUT:
+%\def\@schapter#1{\if@twocolumn
+% \@topnewpage[\@makeschapterhead{#1}]%
+% \else
+% \@makeschapterhead{#1}%
+% \@afterheading
+% \fi}
+
+%%IN:
+\def\@schapter#1{%
+\if@twocolumn%
+ \@makeschapterhead{#1}%
+\else%
+ \@makeschapterhead{#1}%
+ \@afterheading%
+\fi}
+
+%%% End: To avoid problem with scrbook.cls (fncychap version 1.32)
+
+\def\@makeschapterhead#1{%
+ \vspace*{50\p@}%
+ {\parindent \z@ \raggedright
+ \normalfont
+ \interlinepenalty\@M
+ \DOTIS{#1}
+ \vskip 40\p@
+ }}
+
+\endinput
+
+
diff --git a/docs/build/latex/python.ist b/docs/build/latex/python.ist
new file mode 100644
index 0000000000000000000000000000000000000000..9ffa0f959f9e60e18c3a7f5fcd518a34964bf68c
--- /dev/null
+++ b/docs/build/latex/python.ist
@@ -0,0 +1,11 @@
+line_max 100
+headings_flag 1
+heading_prefix " \\bigletter "
+
+preamble "\\begin{theindex}
+\\def\\bigletter#1{{\\Large\\sffamily#1}\\nopagebreak\\vspace{1mm}}
+
+"
+
+symhead_positive "{Symbols}"
+numhead_positive "{Numbers}"
diff --git a/docs/build/latex/sphinx.sty b/docs/build/latex/sphinx.sty
new file mode 100644
index 0000000000000000000000000000000000000000..554845f8353214aa643a935ff32f7ed999cc1c8f
--- /dev/null
+++ b/docs/build/latex/sphinx.sty
@@ -0,0 +1,522 @@
+%
+% sphinx.sty
+%
+% Adapted from the old python.sty, mostly written by Fred Drake,
+% by Georg Brandl.
+%
+
+\NeedsTeXFormat{LaTeX2e}[1995/12/01]
+\ProvidesPackage{sphinx}[2010/01/15 LaTeX package (Sphinx markup)]
+
+\@ifclassloaded{memoir}{}{\RequirePackage{fancyhdr}}
+
+\RequirePackage{textcomp}
+\RequirePackage{fancybox}
+\RequirePackage{titlesec}
+\RequirePackage{tabulary}
+\RequirePackage{amsmath} % for \text
+\RequirePackage{makeidx}
+\RequirePackage{framed}
+\RequirePackage{ifthen}
+\RequirePackage{color}
+% For highlighted code.
+\RequirePackage{fancyvrb}
+% For table captions.
+\RequirePackage{threeparttable}
+% Handle footnotes in tables.
+\RequirePackage{footnote}
+\makesavenoteenv{tabulary}
+% For floating figures in the text.
+\RequirePackage{wrapfig}
+% Separate paragraphs by space by default.
+\RequirePackage{parskip}
+% For parsed-literal blocks.
+\RequirePackage{alltt}
+
+% Redefine these colors to your liking in the preamble.
+\definecolor{TitleColor}{rgb}{0.126,0.263,0.361}
+\definecolor{InnerLinkColor}{rgb}{0.208,0.374,0.486}
+\definecolor{OuterLinkColor}{rgb}{0.216,0.439,0.388}
+% Redefine these colors to something not white if you want to have colored
+% background and border for code examples.
+\definecolor{VerbatimColor}{rgb}{1,1,1}
+\definecolor{VerbatimBorderColor}{rgb}{1,1,1}
+
+% Uncomment these two lines to ignore the paper size and make the page
+% size more like a typical published manual.
+%\renewcommand{\paperheight}{9in}
+%\renewcommand{\paperwidth}{8.5in} % typical squarish manual
+%\renewcommand{\paperwidth}{7in} % O'Reilly ``Programmming Python''
+
+% use pdfoutput for pTeX and dvipdfmx
+\ifx\kanjiskip\undefined\else
+ \ifx\Gin@driver{dvipdfmx.def}\undefined\else
+ \newcount\pdfoutput\pdfoutput=0
+ \fi
+\fi
+
+% For graphicx, check if we are compiling under latex or pdflatex.
+\ifx\pdftexversion\undefined
+ \usepackage{graphicx}
+\else
+ \usepackage[pdftex]{graphicx}
+\fi
+
+% for PDF output, use colors and maximal compression
+\newif\ifsphinxpdfoutput\sphinxpdfoutputfalse
+\ifx\pdfoutput\undefined\else\ifcase\pdfoutput
+ \let\py@NormalColor\relax
+ \let\py@TitleColor\relax
+\else
+ \sphinxpdfoutputtrue
+ \input{pdfcolor}
+ \def\py@NormalColor{\color[rgb]{0.0,0.0,0.0}}
+ \def\py@TitleColor{\color{TitleColor}}
+ \pdfcompresslevel=9
+\fi\fi
+
+% XeLaTeX can do colors, too
+\ifx\XeTeXrevision\undefined\else
+ \def\py@NormalColor{\color[rgb]{0.0,0.0,0.0}}
+ \def\py@TitleColor{\color{TitleColor}}
+\fi
+
+% Increase printable page size (copied from fullpage.sty)
+\topmargin 0pt
+\advance \topmargin by -\headheight
+\advance \topmargin by -\headsep
+
+% attempt to work a little better for A4 users
+\textheight \paperheight
+\advance\textheight by -2in
+
+\oddsidemargin 0pt
+\evensidemargin 0pt
+%\evensidemargin -.25in % for ``manual size'' documents
+\marginparwidth 0.5in
+
+\textwidth \paperwidth
+\advance\textwidth by -2in
+
+
+% Style parameters and macros used by most documents here
+\raggedbottom
+\sloppy
+\hbadness = 5000 % don't print trivial gripes
+
+\pagestyle{empty} % start this way
+
+% Use this to set the font family for headers and other decor:
+\newcommand{\py@HeaderFamily}{\sffamily\bfseries}
+
+% Redefine the 'normal' header/footer style when using "fancyhdr" package:
+\@ifundefined{fancyhf}{}{
+ % Use \pagestyle{normal} as the primary pagestyle for text.
+ \fancypagestyle{normal}{
+ \fancyhf{}
+ \fancyfoot[LE,RO]{{\py@HeaderFamily\thepage}}
+ \fancyfoot[LO]{{\py@HeaderFamily\nouppercase{\rightmark}}}
+ \fancyfoot[RE]{{\py@HeaderFamily\nouppercase{\leftmark}}}
+ \fancyhead[LE,RO]{{\py@HeaderFamily \@title, \py@release}}
+ \renewcommand{\headrulewidth}{0.4pt}
+ \renewcommand{\footrulewidth}{0.4pt}
+ % define chaptermark with \@chappos when \@chappos is available for Japanese
+ \ifx\@chappos\undefined\else
+ \def\chaptermark##1{\markboth{\@chapapp\space\thechapter\space\@chappos\space ##1}{}}
+ \fi
+ }
+ % Update the plain style so we get the page number & footer line,
+ % but not a chapter or section title. This is to keep the first
+ % page of a chapter and the blank page between chapters `clean.'
+ \fancypagestyle{plain}{
+ \fancyhf{}
+ \fancyfoot[LE,RO]{{\py@HeaderFamily\thepage}}
+ \renewcommand{\headrulewidth}{0pt}
+ \renewcommand{\footrulewidth}{0.4pt}
+ }
+}
+
+% Some custom font markup commands.
+%
+\newcommand{\strong}[1]{{\textbf{#1}}}
+\newcommand{\code}[1]{\texttt{#1}}
+\newcommand{\bfcode}[1]{\code{\bfseries#1}}
+\newcommand{\email}[1]{\textsf{#1}}
+
+% Redefine the Verbatim environment to allow border and background colors.
+% The original environment is still used for verbatims within tables.
+\let\OriginalVerbatim=\Verbatim
+\let\endOriginalVerbatim=\endVerbatim
+
+% Play with vspace to be able to keep the indentation.
+\newlength\distancetoright
+\def\mycolorbox#1{%
+ \setlength\distancetoright{\linewidth}%
+ \advance\distancetoright -\@totalleftmargin %
+ \fcolorbox{VerbatimBorderColor}{VerbatimColor}{%
+ \begin{minipage}{\distancetoright}%
+ #1
+ \end{minipage}%
+ }%
+}
+\def\FrameCommand{\mycolorbox}
+
+\renewcommand{\Verbatim}[1][1]{%
+ % list starts new par, but we don't want it to be set apart vertically
+ \bgroup\parskip=0pt%
+ \smallskip%
+ % The list environement is needed to control perfectly the vertical
+ % space.
+ \list{}{%
+ \setlength\parskip{0pt}%
+ \setlength\itemsep{0ex}%
+ \setlength\topsep{0ex}%
+ \setlength\partopsep{0pt}%
+ \setlength\leftmargin{0pt}%
+ }%
+ \item\MakeFramed {\FrameRestore}%
+ \small%
+ \OriginalVerbatim[#1]%
+}
+\renewcommand{\endVerbatim}{%
+ \endOriginalVerbatim%
+ \endMakeFramed%
+ \endlist%
+ % close group to restore \parskip
+ \egroup%
+}
+
+
+% \moduleauthor{name}{email}
+\newcommand{\moduleauthor}[2]{}
+
+% \sectionauthor{name}{email}
+\newcommand{\sectionauthor}[2]{}
+
+% Augment the sectioning commands used to get our own font family in place,
+% and reset some internal data items:
+\titleformat{\section}{\Large\py@HeaderFamily}%
+ {\py@TitleColor\thesection}{0.5em}{\py@TitleColor}{\py@NormalColor}
+\titleformat{\subsection}{\large\py@HeaderFamily}%
+ {\py@TitleColor\thesubsection}{0.5em}{\py@TitleColor}{\py@NormalColor}
+\titleformat{\subsubsection}{\py@HeaderFamily}%
+ {\py@TitleColor\thesubsubsection}{0.5em}{\py@TitleColor}{\py@NormalColor}
+\titleformat{\paragraph}{\small\py@HeaderFamily}%
+ {\py@TitleColor}{0em}{\py@TitleColor}{\py@NormalColor}
+
+% {fulllineitems} is the main environment for object descriptions.
+%
+\newcommand{\py@itemnewline}[1]{%
+ \@tempdima\linewidth%
+ \advance\@tempdima \leftmargin\makebox[\@tempdima][l]{#1}%
+}
+
+\newenvironment{fulllineitems}{
+ \begin{list}{}{\labelwidth \leftmargin \labelsep 0pt
+ \rightmargin 0pt \topsep -\parskip \partopsep \parskip
+ \itemsep -\parsep
+ \let\makelabel=\py@itemnewline}
+}{\end{list}}
+
+% \optional is used for ``[, arg]``, i.e. desc_optional nodes.
+\newcommand{\optional}[1]{%
+ {\textnormal{\Large[}}{#1}\hspace{0.5mm}{\textnormal{\Large]}}}
+
+\newlength{\py@argswidth}
+\newcommand{\py@sigparams}[2]{%
+ \parbox[t]{\py@argswidth}{#1\code{)}#2}}
+\newcommand{\pysigline}[1]{\item[#1]\nopagebreak}
+\newcommand{\pysiglinewithargsret}[3]{%
+ \settowidth{\py@argswidth}{#1\code{(}}%
+ \addtolength{\py@argswidth}{-2\py@argswidth}%
+ \addtolength{\py@argswidth}{\linewidth}%
+ \item[#1\code{(}\py@sigparams{#2}{#3}]}
+
+% Production lists
+%
+\newenvironment{productionlist}{
+% \def\optional##1{{\Large[}##1{\Large]}}
+ \def\production##1##2{\\\code{##1}&::=&\code{##2}}
+ \def\productioncont##1{\\& &\code{##1}}
+ \parindent=2em
+ \indent
+ \setlength{\LTpre}{0pt}
+ \setlength{\LTpost}{0pt}
+ \begin{longtable}[l]{lcl}
+}{%
+ \end{longtable}
+}
+
+% Notices / Admonitions
+%
+\newlength{\py@noticelength}
+
+\newcommand{\py@heavybox}{
+ \setlength{\fboxrule}{1pt}
+ \setlength{\fboxsep}{6pt}
+ \setlength{\py@noticelength}{\linewidth}
+ \addtolength{\py@noticelength}{-2\fboxsep}
+ \addtolength{\py@noticelength}{-2\fboxrule}
+ %\setlength{\shadowsize}{3pt}
+ \noindent\Sbox
+ \minipage{\py@noticelength}
+}
+\newcommand{\py@endheavybox}{
+ \endminipage
+ \endSbox
+ \fbox{\TheSbox}
+}
+
+\newcommand{\py@lightbox}{{%
+ \setlength\parskip{0pt}\par
+ \noindent\rule[0ex]{\linewidth}{0.5pt}%
+ \par\noindent\vspace{-0.5ex}%
+ }}
+\newcommand{\py@endlightbox}{{%
+ \setlength{\parskip}{0pt}%
+ \par\noindent\rule[0.5ex]{\linewidth}{0.5pt}%
+ \par\vspace{-0.5ex}%
+ }}
+
+% Some are quite plain:
+\newcommand{\py@noticestart@note}{\py@lightbox}
+\newcommand{\py@noticeend@note}{\py@endlightbox}
+\newcommand{\py@noticestart@hint}{\py@lightbox}
+\newcommand{\py@noticeend@hint}{\py@endlightbox}
+\newcommand{\py@noticestart@important}{\py@lightbox}
+\newcommand{\py@noticeend@important}{\py@endlightbox}
+\newcommand{\py@noticestart@tip}{\py@lightbox}
+\newcommand{\py@noticeend@tip}{\py@endlightbox}
+
+% Others gets more visible distinction:
+\newcommand{\py@noticestart@warning}{\py@heavybox}
+\newcommand{\py@noticeend@warning}{\py@endheavybox}
+\newcommand{\py@noticestart@caution}{\py@heavybox}
+\newcommand{\py@noticeend@caution}{\py@endheavybox}
+\newcommand{\py@noticestart@attention}{\py@heavybox}
+\newcommand{\py@noticeend@attention}{\py@endheavybox}
+\newcommand{\py@noticestart@danger}{\py@heavybox}
+\newcommand{\py@noticeend@danger}{\py@endheavybox}
+\newcommand{\py@noticestart@error}{\py@heavybox}
+\newcommand{\py@noticeend@error}{\py@endheavybox}
+
+\newenvironment{notice}[2]{
+ \def\py@noticetype{#1}
+ \csname py@noticestart@#1\endcsname
+ \strong{#2}
+}{\csname py@noticeend@\py@noticetype\endcsname}
+
+% Allow the release number to be specified independently of the
+% \date{}. This allows the date to reflect the document's date and
+% release to specify the release that is documented.
+%
+\newcommand{\py@release}{}
+\newcommand{\version}{}
+\newcommand{\shortversion}{}
+\newcommand{\releaseinfo}{}
+\newcommand{\releasename}{Release}
+\newcommand{\release}[1]{%
+ \renewcommand{\py@release}{\releasename\space\version}%
+ \renewcommand{\version}{#1}}
+\newcommand{\setshortversion}[1]{%
+ \renewcommand{\shortversion}{#1}}
+\newcommand{\setreleaseinfo}[1]{%
+ \renewcommand{\releaseinfo}{#1}}
+
+% Allow specification of the author's address separately from the
+% author's name. This can be used to format them differently, which
+% is a good thing.
+%
+\newcommand{\py@authoraddress}{}
+\newcommand{\authoraddress}[1]{\renewcommand{\py@authoraddress}{#1}}
+
+% This sets up the fancy chapter headings that make the documents look
+% at least a little better than the usual LaTeX output.
+%
+\@ifundefined{ChTitleVar}{}{
+ \ChNameVar{\raggedleft\normalsize\py@HeaderFamily}
+ \ChNumVar{\raggedleft \bfseries\Large\py@HeaderFamily}
+ \ChTitleVar{\raggedleft \textrm{\Huge\py@HeaderFamily}}
+ % This creates chapter heads without the leading \vspace*{}:
+ \def\@makechapterhead#1{%
+ {\parindent \z@ \raggedright \normalfont
+ \ifnum \c@secnumdepth >\m@ne
+ \DOCH
+ \fi
+ \interlinepenalty\@M
+ \DOTI{#1}
+ }
+ }
+}
+
+% Redefine description environment so that it is usable inside fulllineitems.
+%
+\renewcommand{\description}{%
+ \list{}{\labelwidth\z@%
+ \itemindent-\leftmargin%
+ \labelsep5pt%
+ \let\makelabel=\descriptionlabel}}
+
+% Definition lists; requested by AMK for HOWTO documents. Probably useful
+% elsewhere as well, so keep in in the general style support.
+%
+\newenvironment{definitions}{%
+ \begin{description}%
+ \def\term##1{\item[##1]\mbox{}\\*[0mm]}
+}{%
+ \end{description}%
+}
+
+% Tell TeX about pathological hyphenation cases:
+\hyphenation{Base-HTTP-Re-quest-Hand-ler}
+
+
+% The following is stuff copied from docutils' latex writer.
+%
+\newcommand{\optionlistlabel}[1]{\bf #1 \hfill}
+\newenvironment{optionlist}[1]
+{\begin{list}{}
+ {\setlength{\labelwidth}{#1}
+ \setlength{\rightmargin}{1cm}
+ \setlength{\leftmargin}{\rightmargin}
+ \addtolength{\leftmargin}{\labelwidth}
+ \addtolength{\leftmargin}{\labelsep}
+ \renewcommand{\makelabel}{\optionlistlabel}}
+}{\end{list}}
+
+\newlength{\lineblockindentation}
+\setlength{\lineblockindentation}{2.5em}
+\newenvironment{lineblock}[1]
+{\begin{list}{}
+ {\setlength{\partopsep}{\parskip}
+ \addtolength{\partopsep}{\baselineskip}
+ \topsep0pt\itemsep0.15\baselineskip\parsep0pt
+ \leftmargin#1}
+ \raggedright}
+{\end{list}}
+
+% Redefine includgraphics for avoiding images larger than the screen size
+% If the size is not specified.
+\let\py@Oldincludegraphics\includegraphics
+
+\newbox\image@box%
+\newdimen\image@width%
+\renewcommand\includegraphics[2][\@empty]{%
+ \ifx#1\@empty%
+ \setbox\image@box=\hbox{\py@Oldincludegraphics{#2}}%
+ \image@width\wd\image@box%
+ \ifdim \image@width>\linewidth%
+ \setbox\image@box=\hbox{\py@Oldincludegraphics[width=\linewidth]{#2}}%
+ \box\image@box%
+ \else%
+ \py@Oldincludegraphics{#2}%
+ \fi%
+ \else%
+ \py@Oldincludegraphics[#1]{#2}%
+ \fi%
+}
+
+% to make pdf with correct encoded bookmarks in Japanese
+% this should precede the hyperref package
+\ifx\kanjiskip\undefined\else
+ \usepackage{atbegshi}
+ \ifx\ucs\undefined
+ \ifnum 42146=\euc"A4A2
+ \AtBeginShipoutFirst{\special{pdf:tounicode EUC-UCS2}}
+ \else
+ \AtBeginShipoutFirst{\special{pdf:tounicode 90ms-RKSJ-UCS2}}
+ \fi
+ \else
+ \AtBeginShipoutFirst{\special{pdf:tounicode UTF8-UCS2}}
+ \fi
+\fi
+
+% Include hyperref last.
+\RequirePackage[colorlinks,breaklinks,
+ linkcolor=InnerLinkColor,filecolor=OuterLinkColor,
+ menucolor=OuterLinkColor,urlcolor=OuterLinkColor,
+ citecolor=InnerLinkColor]{hyperref}
+% Fix anchor placement for figures with captions.
+% (Note: we don't use a package option here; instead, we give an explicit
+% \capstart for figures that actually have a caption.)
+\RequirePackage{hypcap}
+
+% From docutils.writers.latex2e
+\providecommand{\DUspan}[2]{%
+ {% group ("span") to limit the scope of styling commands
+ \@for\node@class@name:=#1\do{%
+ \ifcsname docutilsrole\node@class@name\endcsname%
+ \csname docutilsrole\node@class@name\endcsname%
+ \fi%
+ }%
+ {#2}% node content
+ }% close "span"
+}
+
+\providecommand*{\DUprovidelength}[2]{
+ \ifthenelse{\isundefined{#1}}{\newlength{#1}\setlength{#1}{#2}}{}
+}
+
+\DUprovidelength{\DUlineblockindent}{2.5em}
+\ifthenelse{\isundefined{\DUlineblock}}{
+ \newenvironment{DUlineblock}[1]{%
+ \list{}{\setlength{\partopsep}{\parskip}
+ \addtolength{\partopsep}{\baselineskip}
+ \setlength{\topsep}{0pt}
+ \setlength{\itemsep}{0.15\baselineskip}
+ \setlength{\parsep}{0pt}
+ \setlength{\leftmargin}{#1}}
+ \raggedright
+ }
+ {\endlist}
+}{}
+
+
+% From footmisc.sty: allows footnotes in titles
+\let\FN@sf@@footnote\footnote
+\def\footnote{\ifx\protect\@typeset@protect
+ \expandafter\FN@sf@@footnote
+ \else
+ \expandafter\FN@sf@gobble@opt
+ \fi
+}
+\edef\FN@sf@gobble@opt{\noexpand\protect
+ \expandafter\noexpand\csname FN@sf@gobble@opt \endcsname}
+\expandafter\def\csname FN@sf@gobble@opt \endcsname{%
+ \@ifnextchar[%]
+ \FN@sf@gobble@twobracket
+ \@gobble
+}
+\def\FN@sf@gobble@twobracket[#1]#2{}
+
+% adjust the margins for footer,
+% this works with the jsclasses only (Japanese standard document classes)
+\ifx\@jsc@uplatextrue\undefined\else
+ \hypersetup{setpagesize=false}
+ \setlength\footskip{2\baselineskip}
+ \addtolength{\textheight}{-2\baselineskip}
+\fi
+
+% fix the double index and bibliography on the table of contents
+% in jsclasses (Japanese standard document classes)
+\ifx\@jsc@uplatextrue\undefined\else
+ \renewcommand{\theindex}{
+ \cleardoublepage
+ \phantomsection
+ \py@OldTheindex
+ }
+ \renewcommand{\thebibliography}[1]{
+ \cleardoublepage
+ \phantomsection
+ \py@OldThebibliography{1}
+ }
+\fi
+
+% disable \@chappos in Appendix in pTeX
+\ifx\kanjiskip\undefined\else
+ \let\py@OldAppendix=\appendix
+ \renewcommand{\appendix}{
+ \py@OldAppendix
+ \gdef\@chappos{}
+ }
+\fi
diff --git a/docs/build/latex/sphinxhowto.cls b/docs/build/latex/sphinxhowto.cls
new file mode 100644
index 0000000000000000000000000000000000000000..26e63a7ee48f1d1955a54fc478d69a20bf4f1d2d
--- /dev/null
+++ b/docs/build/latex/sphinxhowto.cls
@@ -0,0 +1,104 @@
+%
+% sphinxhowto.cls for Sphinx (http://sphinx-doc.org/)
+%
+
+\NeedsTeXFormat{LaTeX2e}[1995/12/01]
+\ProvidesClass{sphinxhowto}[2009/06/02 Document class (Sphinx HOWTO)]
+
+% 'oneside' option overriding the 'twoside' default
+\newif\if@oneside
+\DeclareOption{oneside}{\@onesidetrue}
+% Pass remaining document options to the parent class.
+\DeclareOption*{\PassOptionsToClass{\CurrentOption}{\sphinxdocclass}}
+\ProcessOptions\relax
+
+% Default to two-side document
+\if@oneside
+% nothing to do (oneside is the default)
+\else
+\PassOptionsToClass{twoside}{\sphinxdocclass}
+\fi
+
+\LoadClass{\sphinxdocclass}
+
+% Set some sane defaults for section numbering depth and TOC depth. You can
+% reset these counters in your preamble.
+%
+\setcounter{secnumdepth}{2}
+
+% Change the title page to look a bit better, and fit in with the fncychap
+% ``Bjarne'' style a bit better.
+%
+\renewcommand{\maketitle}{
+ \rule{\textwidth}{1pt}
+ \ifsphinxpdfoutput
+ \begingroup
+ % These \defs are required to deal with multi-line authors; it
+ % changes \\ to ', ' (comma-space), making it pass muster for
+ % generating document info in the PDF file.
+ \def\\{, }
+ \def\and{and }
+ \pdfinfo{
+ /Author (\@author)
+ /Title (\@title)
+ }
+ \endgroup
+ \fi
+ \begin{flushright}
+ \sphinxlogo%
+ {\rm\Huge\py@HeaderFamily \@title} \par
+ {\em\large\py@HeaderFamily \py@release\releaseinfo} \par
+ \vspace{25pt}
+ {\Large\py@HeaderFamily
+ \begin{tabular}[t]{c}
+ \@author
+ \end{tabular}} \par
+ \vspace{25pt}
+ \@date \par
+ \py@authoraddress \par
+ \end{flushright}
+ \@thanks
+ \setcounter{footnote}{0}
+ \let\thanks\relax\let\maketitle\relax
+ %\gdef\@thanks{}\gdef\@author{}\gdef\@title{}
+}
+
+\let\py@OldTableofcontents=\tableofcontents
+\renewcommand{\tableofcontents}{
+ \begingroup
+ \parskip = 0mm
+ \py@OldTableofcontents
+ \endgroup
+ \rule{\textwidth}{1pt}
+ \vspace{12pt}
+}
+
+\@ifundefined{fancyhf}{
+ \pagestyle{plain}}{
+ \pagestyle{normal}} % start this way; change for
+\pagenumbering{arabic} % ToC & chapters
+
+\thispagestyle{empty}
+
+% Fix the bibliography environment to add an entry to the Table of
+% Contents.
+% For an article document class this environment is a section,
+% so no page break before it.
+\let\py@OldThebibliography=\thebibliography
+\renewcommand{\thebibliography}[1]{
+ \phantomsection
+ \py@OldThebibliography{1}
+ \addcontentsline{toc}{section}{\bibname}
+}
+
+% Same for the indices.
+% The memoir class already does this, so we don't duplicate it in that case.
+%
+\@ifclassloaded{memoir}{}{
+ \let\py@OldTheindex=\theindex
+ \renewcommand{\theindex}{
+ \phantomsection
+ \py@OldTheindex
+ \addcontentsline{toc}{section}{\indexname}
+ }
+}
diff --git a/docs/build/latex/sphinxmanual.cls b/docs/build/latex/sphinxmanual.cls
new file mode 100644
index 0000000000000000000000000000000000000000..a6b9b392859c2a6fee6af23d8232f9e3fdb5f32e
--- /dev/null
+++ b/docs/build/latex/sphinxmanual.cls
@@ -0,0 +1,148 @@
+%
+% sphinxmanual.cls for Sphinx (http://sphinx-doc.org/)
+%
+
+\NeedsTeXFormat{LaTeX2e}[1995/12/01]
+\ProvidesClass{sphinxmanual}[2009/06/02 Document class (Sphinx manual)]
+
+% chapters starting at odd pages (overridden by 'openany' document option)
+\PassOptionsToClass{openright}{\sphinxdocclass}
+
+% 'oneside' option overriding the 'twoside' default
+\newif\if@oneside
+\DeclareOption{oneside}{\@onesidetrue}
+% Pass remaining document options to the parent class.
+\DeclareOption*{\PassOptionsToClass{\CurrentOption}{\sphinxdocclass}}
+\ProcessOptions\relax
+
+% Defaults two-side document
+\if@oneside
+% nothing to do (oneside is the default)
+\else
+\PassOptionsToClass{twoside}{\sphinxdocclass}
+\fi
+
+\LoadClass{\sphinxdocclass}
+
+% Set some sane defaults for section numbering depth and TOC depth. You can
+% reset these counters in your preamble.
+%
+\setcounter{secnumdepth}{2}
+\setcounter{tocdepth}{1}
+
+% Change the title page to look a bit better, and fit in with the fncychap
+% ``Bjarne'' style a bit better.
+%
+\renewcommand{\maketitle}{%
+ \begin{titlepage}%
+ \let\footnotesize\small
+ \let\footnoterule\relax
+ \rule{\textwidth}{1pt}%
+ \ifsphinxpdfoutput
+ \begingroup
+ % These \defs are required to deal with multi-line authors; it
+ % changes \\ to ', ' (comma-space), making it pass muster for
+ % generating document info in the PDF file.
+ \def\\{, }
+ \def\and{and }
+ \pdfinfo{
+ /Author (\@author)
+ /Title (\@title)
+ }
+ \endgroup
+ \fi
+ \begin{flushright}%
+ \sphinxlogo%
+ {\rm\Huge\py@HeaderFamily \@title \par}%
+ {\em\LARGE\py@HeaderFamily \py@release\releaseinfo \par}
+ \vfill
+ {\LARGE\py@HeaderFamily
+ \begin{tabular}[t]{c}
+ \@author
+ \end{tabular}
+ \par}
+ \vfill\vfill
+ {\large
+ \@date \par
+ \vfill
+ \py@authoraddress \par
+ }%
+ \end{flushright}%\par
+ \@thanks
+ \end{titlepage}%
+ \cleardoublepage%
+ \setcounter{footnote}{0}%
+ \let\thanks\relax\let\maketitle\relax
+ %\gdef\@thanks{}\gdef\@author{}\gdef\@title{}
+}
+
+
+% Catch the end of the {abstract} environment, but here make sure the abstract
+% is followed by a blank page if the 'openright' option is used.
+%
+\let\py@OldEndAbstract=\endabstract
+\renewcommand{\endabstract}{
+ \if@openright
+ \ifodd\value{page}
+ \typeout{Adding blank page after the abstract.}
+ \vfil\pagebreak
+ \fi
+ \fi
+ \py@OldEndAbstract
+}
+
+% This wraps the \tableofcontents macro with all the magic to get the spacing
+% right and have the right number of pages if the 'openright' option has been
+% used. This eliminates a fair amount of crud in the individual document files.
+%
+\let\py@OldTableofcontents=\tableofcontents
+\renewcommand{\tableofcontents}{%
+ \pagenumbering{roman}%
+ \setcounter{page}{1}%
+ \pagebreak%
+ \pagestyle{plain}%
+ {%
+ \parskip = 0mm%
+ \py@OldTableofcontents%
+ \if@openright%
+ \ifodd\value{page}%
+ \typeout{Adding blank page after the table of contents.}%
+ \pagebreak\hspace{0pt}%
+ \fi%
+ \fi%
+ \cleardoublepage%
+ }%
+ \pagenumbering{arabic}%
+ \@ifundefined{fancyhf}{}{\pagestyle{normal}}%
+}
+\pagenumbering{alph}
+
+% This is needed to get the width of the section # area wide enough in the
+% library reference. Doing it here keeps it the same for all the manuals.
+%
+\renewcommand*\l@section{\@dottedtocline{1}{1.5em}{2.6em}}
+\renewcommand*\l@subsection{\@dottedtocline{2}{4.1em}{3.5em}}
+
+% Fix the bibliography environment to add an entry to the Table of
+% Contents.
+% For a report document class this environment is a chapter.
+\let\py@OldThebibliography=\thebibliography
+\renewcommand{\thebibliography}[1]{
+ \cleardoublepage
+ \phantomsection
+ \py@OldThebibliography{1}
+ \addcontentsline{toc}{chapter}{\bibname}
+}
+
+% Same for the indices.
+% The memoir class already does this, so we don't duplicate it in that case.
+%
+\@ifclassloaded{memoir}{}{
+ \let\py@OldTheindex=\theindex
+ \renewcommand{\theindex}{
+ \cleardoublepage
+ \phantomsection
+ \py@OldTheindex
+ \addcontentsline{toc}{chapter}{\indexname}
+ }
+}
diff --git a/docs/build/latex/tabulary.sty b/docs/build/latex/tabulary.sty
new file mode 100644
index 0000000000000000000000000000000000000000..7ea572c1213b369f51c32103149f18c32861b442
--- /dev/null
+++ b/docs/build/latex/tabulary.sty
@@ -0,0 +1,449 @@
+%%
+%% This is file `tabulary.sty',
+%% generated with the docstrip utility.
+%%
+%% The original source files were:
+%%
+%% tabulary.dtx (with options: `package')
+%% DRAFT VERSION
+%%
+%% File `tabulary.dtx'.
+%% Copyright (C) 1995 1996 2003 2008 David Carlisle
+%% This file may be distributed under the terms of the LPPL.
+%% See 00readme.txt for details.
+%%
+\NeedsTeXFormat{LaTeX2e}
+\ProvidesPackage{tabulary}
+ [2008/12/01 v0.9 tabulary package (DPC)]
+\RequirePackage{array}
+\catcode`\Z=14
+\DeclareOption{debugshow}{\catcode`\Z=9\relax}
+\ProcessOptions
+\def\arraybackslash{\let\\=\@arraycr}
+\def\@finalstrut#1{%
+ \unskip\ifhmode\nobreak\fi\vrule\@width\z@\@height\z@\@depth\dp#1}
+\newcount\TY@count
+\def\tabulary{%
+ \let\TY@final\tabular
+ \let\endTY@final\endtabular
+ \TY@tabular}
+\def\TY@tabular#1{%
+ \edef\TY@{\@currenvir}%
+ {\ifnum0=`}\fi
+ \@ovxx\TY@linewidth
+ \@ovyy\TY@tablewidth
+ \count@\z@
+ \@tempswatrue
+ \@whilesw\if@tempswa\fi{%
+ \advance\count@\@ne
+ \expandafter\ifx\csname TY@F\the\count@\endcsname\relax
+ \@tempswafalse
+ \else
+ \expandafter\let\csname TY@SF\the\count@\expandafter\endcsname
+ \csname TY@F\the\count@\endcsname
+ \global\expandafter\let\csname TY@F\the\count@\endcsname\relax
+ \expandafter\let\csname TY@S\the\count@\expandafter\endcsname
+ \csname TY@\the\count@\endcsname
+ \fi}%
+ \global\TY@count\@ne
+ \TY@width\xdef{0pt}%
+ \global\TY@tablewidth\z@
+ \global\TY@linewidth#1\relax
+Z\message{^^J^^JTable^^J%
+Z Target Width: \the\TY@linewidth^^J%
+Z \string\tabcolsep: \the\tabcolsep\space
+Z \string\arrayrulewidth: \the\arrayrulewidth\space
+Z \string\doublerulesep: \the\doublerulesep^^J%
+Z \string\tymin: \the\tymin\space
+Z \string\tymax: \the\tymax^^J}%
+ \let\@classz\TY@classz
+ \let\verb\TX@verb
+ \toks@{}\TY@get@body}
+\let\TY@@mkpream\@mkpream
+\def\TY@mkpream{%
+ \def\@addamp{%
+ \if@firstamp \@firstampfalse \else
+ \global\advance\TY@count\@ne
+ \edef\@preamble{\@preamble &}\fi
+ \TY@width\xdef{0pt}}%
+ \def\@acol{%
+ \TY@subwidth\col@sep
+ \@addtopreamble{\hskip\col@sep}}%
+ \let\@arrayrule\TY@arrayrule
+ \let\@classvi\TY@classvi
+ \def\@classv{\save@decl
+ \expandafter\NC@ecs\@nextchar\extracolsep{}\extracolsep\@@@
+ \sbox\z@{\d@llarbegin\@nextchar\d@llarend}%
+ \TY@subwidth{\wd\z@}%
+ \@addtopreamble{\d@llarbegin\the@toks\the\count@\relax\d@llarend}%
+ \prepnext@tok}%
+ \global\let\@mkpream\TY@@mkpream
+ \TY@@mkpream}
+\def\TY@arrayrule{%
+ \TY@subwidth\arrayrulewidth
+ \@addtopreamble \vline}
+\def\TY@classvi{\ifcase \@lastchclass
+ \@acol \or
+ \TY@subwidth\doublerulesep
+ \@addtopreamble{\hskip \doublerulesep}\or
+ \@acol \or
+ \@classvii
+ \fi}
+\def\TY@tab{%
+ \setbox\z@\hbox\bgroup
+ \let\[$\let\]$%
+ \let\equation$\let\endequation$%
+ \col@sep\tabcolsep
+ \let\d@llarbegin\begingroup\let\d@llarend\endgroup
+ \let\@mkpream\TY@mkpream
+ \def\multicolumn##1##2##3{\multispan##1\relax}%
+ \CT@start\TY@tabarray}
+\def\TY@tabarray{\@ifnextchar[{\TY@array}{\@array[t]}}
+\def\TY@array[#1]{\@array[t]}
+\def\TY@width#1{%
+ \expandafter#1\csname TY@\the\TY@count\endcsname}
+\def\TY@subwidth#1{%
+ \TY@width\dimen@
+ \advance\dimen@-#1\relax
+ \TY@width\xdef{\the\dimen@}%
+ \global\advance\TY@linewidth-#1\relax}
+\def\endtabulary{%
+ \gdef\@halignto{}%
+ \expandafter\TY@tab\the\toks@
+ \crcr\omit
+ {\xdef\TY@save@row{}%
+ \loop
+ \advance\TY@count\m@ne
+ \ifnum\TY@count>\z@
+ \xdef\TY@save@row{\TY@save@row&\omit}%
+ \repeat}\TY@save@row
+ \endarray\global\setbox1=\lastbox\setbox0=\vbox{\unvbox1
+ \unskip\global\setbox1=\lastbox}\egroup
+ \dimen@\TY@linewidth
+ \divide\dimen@\TY@count
+ \ifdim\dimen@<\tymin
+ \TY@warn{tymin too large (\the\tymin), resetting to \the\dimen@}%
+ \tymin\dimen@
+ \fi
+ \setbox\tw@=\hbox{\unhbox\@ne
+ \loop
+\@tempdima=\lastskip
+\ifdim\@tempdima>\z@
+Z \message{ecs=\the\@tempdima^^J}%
+ \global\advance\TY@linewidth-\@tempdima
+\fi
+ \unskip
+ \setbox\tw@=\lastbox
+ \ifhbox\tw@
+Z \message{Col \the\TY@count: Initial=\the\wd\tw@\space}%
+ \ifdim\wd\tw@>\tymax
+ \wd\tw@\tymax
+Z \message{> max\space}%
+Z \else
+Z \message{ \@spaces\space}%
+ \fi
+ \TY@width\dimen@
+Z \message{\the\dimen@\space}%
+ \advance\dimen@\wd\tw@
+Z \message{Final=\the\dimen@\space}%
+ \TY@width\xdef{\the\dimen@}%
+ \ifdim\dimen@<\tymin
+Z \message{< tymin}%
+ \global\advance\TY@linewidth-\dimen@
+ \expandafter\xdef\csname TY@F\the\TY@count\endcsname
+ {\the\dimen@}%
+ \else
+ \expandafter\ifx\csname TY@F\the\TY@count\endcsname\z@
+Z \message{***}%
+ \global\advance\TY@linewidth-\dimen@
+ \expandafter\xdef\csname TY@F\the\TY@count\endcsname
+ {\the\dimen@}%
+ \else
+Z \message{> tymin}%
+ \global\advance\TY@tablewidth\dimen@
+ \global\expandafter\let\csname TY@F\the\TY@count\endcsname
+ \maxdimen
+ \fi\fi
+ \advance\TY@count\m@ne
+ \repeat}%
+ \TY@checkmin
+ \TY@checkmin
+ \TY@checkmin
+ \TY@checkmin
+ \TY@count\z@
+ \let\TY@box\TY@box@v
+ {\expandafter\TY@final\the\toks@\endTY@final}%
+ \count@\z@
+ \@tempswatrue
+ \@whilesw\if@tempswa\fi{%
+ \advance\count@\@ne
+ \expandafter\ifx\csname TY@SF\the\count@\endcsname\relax
+ \@tempswafalse
+ \else
+ \global\expandafter\let\csname TY@F\the\count@\expandafter\endcsname
+ \csname TY@SF\the\count@\endcsname
+ \global\expandafter\let\csname TY@\the\count@\expandafter\endcsname
+ \csname TY@S\the\count@\endcsname
+ \fi}%
+ \TY@linewidth\@ovxx
+ \TY@tablewidth\@ovyy
+ \ifnum0=`{\fi}}
+\def\TY@checkmin{%
+ \let\TY@checkmin\relax
+\ifdim\TY@tablewidth>\z@
+ \Gscale@div\TY@ratio\TY@linewidth\TY@tablewidth
+ \ifdim\TY@tablewidth <\TY@linewidth
+ \def\TY@ratio{1}%
+ \fi
+\else
+ \TY@warn{No suitable columns!}%
+ \def\TY@ratio{1}%
+\fi
+\count@\z@
+Z \message{^^JLine Width: \the\TY@linewidth,
+Z Natural Width: \the\TY@tablewidth,
+Z Ratio: \TY@ratio^^J}%
+\@tempdima\z@
+\loop
+\ifnum\count@<\TY@count
+\advance\count@\@ne
+ \ifdim\csname TY@F\the\count@\endcsname>\tymin
+ \dimen@\csname TY@\the\count@\endcsname
+ \dimen@\TY@ratio\dimen@
+ \ifdim\dimen@<\tymin
+Z \message{Column \the\count@\space ->}%
+ \global\expandafter\let\csname TY@F\the\count@\endcsname\tymin
+ \global\advance\TY@linewidth-\tymin
+ \global\advance\TY@tablewidth-\csname TY@\the\count@\endcsname
+ \let\TY@checkmin\TY@@checkmin
+ \else
+ \expandafter\xdef\csname TY@F\the\count@\endcsname{\the\dimen@}%
+ \advance\@tempdima\csname TY@F\the\count@\endcsname
+ \fi
+ \fi
+Z \dimen@\csname TY@F\the\count@\endcsname\message{\the\dimen@, }%
+\repeat
+Z \message{^^JTotal:\the\@tempdima^^J}%
+}
+\let\TY@@checkmin\TY@checkmin
+\newdimen\TY@linewidth
+\def\tyformat{\everypar{{\nobreak\hskip\z@skip}}}
+\newdimen\tymin
+\tymin=10pt
+\newdimen\tymax
+\tymax=2\textwidth
+\def\@testpach{\@chclass
+ \ifnum \@lastchclass=6 \@ne \@chnum \@ne \else
+ \ifnum \@lastchclass=7 5 \else
+ \ifnum \@lastchclass=8 \tw@ \else
+ \ifnum \@lastchclass=9 \thr@@
+ \else \z@
+ \ifnum \@lastchclass = 10 \else
+ \edef\@nextchar{\expandafter\string\@nextchar}%
+ \@chnum
+ \if \@nextchar c\z@ \else
+ \if \@nextchar l\@ne \else
+ \if \@nextchar r\tw@ \else
+ \if \@nextchar C7 \else
+ \if \@nextchar L8 \else
+ \if \@nextchar R9 \else
+ \if \@nextchar J10 \else
+ \z@ \@chclass
+ \if\@nextchar |\@ne \else
+ \if \@nextchar !6 \else
+ \if \@nextchar @7 \else
+ \if \@nextchar <8 \else
+ \if \@nextchar >9 \else
+ 10
+ \@chnum
+ \if \@nextchar m\thr@@\else
+ \if \@nextchar p4 \else
+ \if \@nextchar b5 \else
+ \z@ \@chclass \z@ \@preamerr \z@ \fi \fi \fi \fi\fi \fi \fi\fi \fi
+ \fi \fi \fi \fi \fi \fi \fi \fi \fi \fi \fi}
+\def\TY@classz{%
+ \@classx
+ \@tempcnta\count@
+ \ifx\TY@box\TY@box@v
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+\newlabel{lsmtool:tab:local_val}{{1}{3}{Definition of variables in the LSMTool parset. \relax \relax }{table.caption.1}{}}
diff --git a/docs/lsmtool.log b/docs/lsmtool.log
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+)
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+\sf@bottom=\skip54
+)
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+LaTeX Warning: Unused global option(s):
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+
+(./lsmtool.aux)
+\openout1 = `lsmtool.aux'.
+
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+File: ot1txr.fd 2000/12/15 v3.1
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+(/usr/local/texlive/2012/texmf-dist/tex/generic/oberdiek/gettitlestring.sty
+Package: gettitlestring 2010/12/03 v1.4 Cleanup title references (HO)
+)
+\c@section@level=\count116
+)
+LaTeX Info: Redefining \ref on input line 24.
+LaTeX Info: Redefining \pageref on input line 24.
+LaTeX Info: Redefining \nameref on input line 24.
+(./lsmtool.out) (./lsmtool.out)
+\@outlinefile=\write3
+\openout3 = `lsmtool.out'.
+
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+[Loading MPS to PDF converter (version 2006.09.02).]
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+\MPnumerator=\count121
+\makeMPintoPDFobject=\count122
+\everyMPtoPDFconversion=\toks21
+) (/usr/local/texlive/2012/texmf-dist/tex/latex/oberdiek/epstopdf-base.sty
+Package: epstopdf-base 2010/02/09 v2.5 Base part for package epstopdf
+(/usr/local/texlive/2012/texmf-dist/tex/latex/oberdiek/grfext.sty
+Package: grfext 2010/08/19 v1.1 Manage graphics extensions (HO)
+)
+Package grfext Info: Graphics extension search list:
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+G,.JBIG2,.JB2,.eps]
+(grfext) \AppendGraphicsExtensions on input line 452.
+(/usr/local/texlive/2012/texmf-dist/tex/latex/latexconfig/epstopdf-sys.cfg
+File: epstopdf-sys.cfg 2010/07/13 v1.3 Configuration of (r)epstopdf for TeX Liv
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+))
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+
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+Overfull \hbox (53.86507pt too wide) in paragraph at lines 107--162
+ [][]
+ []
+
+
+Overfull \hbox (2.74364pt too wide) in paragraph at lines 182--182
+[]\OT1/txtt/m/n/10 >>> LSM.add({'Name':'new_source', 'Type':'POINT', 'Ra':277.4
+232, 'Dec':48.3689, 'I':0.69})[]
+ []
+
+[2] [3]
+Package atveryend Info: Empty hook `BeforeClearDocument' on input line 214.
+[4]
+Package atveryend Info: Empty hook `AfterLastShipout' on input line 214.
+(./lsmtool.aux)
+Package atveryend Info: Executing hook `AtVeryEndDocument' on input line 214.
+Package atveryend Info: Executing hook `AtEndAfterFileList' on input line 214.
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+(rerunfilecheck) Checksum: 62653F51F019715D3B957EE5CD75C0AB;328.
+Package atveryend Info: Empty hook `AtVeryVeryEnd' on input line 214.
+ )
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+ype1/urw/times/utmr8a.pfb>
+Output written on lsmtool.pdf (4 pages, 53399 bytes).
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+ 41 words of extra memory for PDF output out of 10000 (max. 10000000)
+
diff --git a/docs/lsmtool.out b/docs/lsmtool.out
new file mode 100644
index 0000000000000000000000000000000000000000..78b102561aebaf62d0bce1b632aa3fa698697d9e
--- /dev/null
+++ b/docs/lsmtool.out
@@ -0,0 +1,5 @@
+\BOOKMARK [1][-]{section.1}{LSMTool: the LOFAR Local Sky Model Tool}{}% 1
+\BOOKMARK [2][-]{subsection.1.1}{Usage}{section.1}% 2
+\BOOKMARK [2][-]{subsection.1.2}{Operations}{section.1}% 3
+\BOOKMARK [2][-]{subsection.1.3}{Example parset}{section.1}% 4
+\BOOKMARK [2][-]{subsection.1.4}{Interactive use and scripting}{section.1}% 5
diff --git a/doc/lsmtool.pdf b/docs/lsmtool.pdf
similarity index 100%
rename from doc/lsmtool.pdf
rename to docs/lsmtool.pdf
diff --git a/docs/lsmtool.synctex.gz b/docs/lsmtool.synctex.gz
new file mode 100644
index 0000000000000000000000000000000000000000..cdc84eda1db88024b82c824e48c6208dbc4bc835
Binary files /dev/null and b/docs/lsmtool.synctex.gz differ
diff --git a/doc/lsmtool.tex b/docs/lsmtool.tex
similarity index 100%
rename from doc/lsmtool.tex
rename to docs/lsmtool.tex
diff --git a/doc/source/.DS_Store b/docs/source/.DS_Store
similarity index 100%
rename from doc/source/.DS_Store
rename to docs/source/.DS_Store
diff --git a/doc/source/conf.py b/docs/source/conf.py
similarity index 100%
rename from doc/source/conf.py
rename to docs/source/conf.py
diff --git a/doc/source/index.rst b/docs/source/index.rst
similarity index 100%
rename from doc/source/index.rst
rename to docs/source/index.rst
diff --git a/docs/source/lsmtool.rst b/docs/source/lsmtool.rst
new file mode 100644
index 0000000000000000000000000000000000000000..6a572a1728c0728cfaab98a4bb1dd3c80d0525d7
--- /dev/null
+++ b/docs/source/lsmtool.rst
@@ -0,0 +1,39 @@
+LSMTool Module Documentation
+============================
+
+.. toctree::
+
+lsmtool module
+-------------------------------
+
+.. automodule:: lsmtool
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+
+lsmtool.operations_lib module
+-----------------------------
+
+.. automodule:: lsmtool.operations_lib
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.skymodel module
+-----------------------
+
+.. automodule:: lsmtool.skymodel
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.tableio module
+----------------------
+
+.. automodule:: lsmtool.tableio
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+
diff --git a/doc/source/overview.rst b/docs/source/overview.rst
similarity index 100%
rename from doc/source/overview.rst
rename to docs/source/overview.rst
diff --git a/docs/test/lsmtool.operations.rst b/docs/test/lsmtool.operations.rst
new file mode 100644
index 0000000000000000000000000000000000000000..d0997457149b8e3c2b8fd69cfa4dbaab27f6225f
--- /dev/null
+++ b/docs/test/lsmtool.operations.rst
@@ -0,0 +1,102 @@
+lsmtool.operations package
+==========================
+
+Submodules
+----------
+
+lsmtool.operations.add module
+-----------------------------
+
+.. automodule:: lsmtool.operations.add
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.concatenate module
+-------------------------------------
+
+.. automodule:: lsmtool.operations.concatenate
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.group module
+-------------------------------
+
+.. automodule:: lsmtool.operations.group
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.merge module
+-------------------------------
+
+.. automodule:: lsmtool.operations.merge
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.move module
+------------------------------
+
+.. automodule:: lsmtool.operations.move
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.plot module
+------------------------------
+
+.. automodule:: lsmtool.operations.plot
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.remove module
+--------------------------------
+
+.. automodule:: lsmtool.operations.remove
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.select module
+--------------------------------
+
+.. automodule:: lsmtool.operations.select
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.setpatchpositions module
+-------------------------------------------
+
+.. automodule:: lsmtool.operations.setpatchpositions
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.transfer module
+----------------------------------
+
+.. automodule:: lsmtool.operations.transfer
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations.ungroup module
+---------------------------------
+
+.. automodule:: lsmtool.operations.ungroup
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+
+Module contents
+---------------
+
+.. automodule:: lsmtool.operations
+ :members:
+ :undoc-members:
+ :show-inheritance:
diff --git a/docs/test/lsmtool.rst b/docs/test/lsmtool.rst
new file mode 100644
index 0000000000000000000000000000000000000000..65a688eb464a37f120b21184781427d0be68d55e
--- /dev/null
+++ b/docs/test/lsmtool.rst
@@ -0,0 +1,53 @@
+lsmtool package
+===============
+
+Subpackages
+-----------
+
+.. toctree::
+
+ lsmtool.operations
+
+Submodules
+----------
+
+lsmtool.lsmtool module
+----------------------
+
+.. automodule:: lsmtool.lsmtool
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.operations_lib module
+-----------------------------
+
+.. automodule:: lsmtool.operations_lib
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.skymodel module
+-----------------------
+
+.. automodule:: lsmtool.skymodel
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+lsmtool.tableio module
+----------------------
+
+.. automodule:: lsmtool.tableio
+ :members:
+ :undoc-members:
+ :show-inheritance:
+
+
+Module contents
+---------------
+
+.. automodule:: lsmtool
+ :members:
+ :undoc-members:
+ :show-inheritance:
diff --git a/docs/test/modules.rst b/docs/test/modules.rst
new file mode 100644
index 0000000000000000000000000000000000000000..70163ca4a8240831a17002576f0786b7b12a7df7
--- /dev/null
+++ b/docs/test/modules.rst
@@ -0,0 +1,7 @@
+lsmtool
+=======
+
+.. toctree::
+ :maxdepth: 4
+
+ lsmtool
diff --git a/lsmtool/skymodel.py b/lsmtool/skymodel.py
index f9ac7a387e7a6798b2bbec5df3222d69ac0700d1..63a59aacb645ddc90209fe23d21817b357eace07 100644
--- a/lsmtool/skymodel.py
+++ b/lsmtool/skymodel.py
@@ -845,7 +845,11 @@ class SkyModel(object):
import numpy as np
sourceNames = self.getColValues('Name')
- patchNames = self.getColValues('Patch')
+ if self.hasPatches:
+ patchNames = self.getColValues('Patch')
+ else:
+ patchNames = []
+
if rowName in sourceNames:
return self._getNameIndx(rowName)
elif rowName in patchNames:
diff --git a/runtests.py b/runtests.py
index f1081fe11678f3292dd04cd7c6d80881c92b0863..140b2a4b22824e856db55896fe02f4b1b4c58b93 100644
--- a/runtests.py
+++ b/runtests.py
@@ -1,6 +1,2979 @@
#! /usr/bin/env python
-import subprocess
+sources = """
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+N/r/XY5KpA==
+"""
+
+import sys
+import base64
+import zlib
+
+class DictImporter(object):
+ def __init__(self, sources):
+ self.sources = sources
+
+ def find_module(self, fullname, path=None):
+ if fullname == "argparse" and sys.version_info >= (2,7):
+ # we were generated with <python2.7 (which pulls in argparse)
+ # but we are running now on a stdlib which has it, so use that.
+ return None
+ if fullname in self.sources:
+ return self
+ if fullname + '.__init__' in self.sources:
+ return self
+ return None
+
+ def load_module(self, fullname):
+ # print "load_module:", fullname
+ from types import ModuleType
+ try:
+ s = self.sources[fullname]
+ is_pkg = False
+ except KeyError:
+ s = self.sources[fullname + '.__init__']
+ is_pkg = True
+
+ co = compile(s, fullname, 'exec')
+ module = sys.modules.setdefault(fullname, ModuleType(fullname))
+ module.__file__ = "%s/%s" % (__file__, fullname)
+ module.__loader__ = self
+ if is_pkg:
+ module.__path__ = [fullname]
+
+ do_exec(co, module.__dict__) # noqa
+ return sys.modules[fullname]
+
+ def get_source(self, name):
+ res = self.sources.get(name)
+ if res is None:
+ res = self.sources.get(name + '.__init__')
+ return res
if __name__ == "__main__":
- subprocess.call(['python', 'tests/validation.py'])
+ if sys.version_info >= (3, 0):
+ exec("def do_exec(co, loc): exec(co, loc)\n")
+ import pickle
+ sources = sources.encode("ascii") # ensure bytes
+ sources = pickle.loads(zlib.decompress(base64.decodebytes(sources)))
+ else:
+ import cPickle as pickle
+ exec("def do_exec(co, loc): exec co in loc\n")
+ sources = pickle.loads(zlib.decompress(base64.decodestring(sources)))
+
+ importer = DictImporter(sources)
+ sys.meta_path.insert(0, importer)
+
+ entry = "import pytest; raise SystemExit(pytest.cmdline.main())"
+ do_exec(entry, locals()) # noqa
diff --git a/setup.py b/setup.py
index 004a09221d85208d2914da7513c538816621faa0..064272c8efb2d72f81db22265d5df021eb32d7d9 100644
--- a/setup.py
+++ b/setup.py
@@ -1,7 +1,6 @@
from __future__ import print_function
from setuptools import setup, Command
import os
-
import lsmtool._version
@@ -11,6 +10,21 @@ if os.path.exists('README.md'):
with open('README.md') as f:
long_description=f.read()
+
+class PyTest(Command):
+ user_options = []
+ def initialize_options(self):
+ pass
+
+ def finalize_options(self):
+ pass
+
+ def run(self):
+ import sys,subprocess
+ errno = subprocess.call([sys.executable, 'runtests.py'])
+ raise SystemExit(errno)
+
+
setup(
name='lsmtool',
version=lsmtool._version.__version__,
@@ -29,7 +43,8 @@ setup(
'Topic :: Scientific/Engineering :: Astronomy',
'Topic :: Software Development :: Libraries :: Python Modules',
],
- install_requires=['numpy','astropy'],
- scripts = ['lsmtool/lsmtool.py'],
+ install_requires=['numpy','astropy >= 0.4'],
+ scripts = ['bin/lsmtool'],
packages=['lsmtool','lsmtool.operations'],
+ cmdclass = {'test': PyTest},
)
diff --git a/tests/test_lsmtool.py b/tests/test_lsmtool.py
new file mode 100644
index 0000000000000000000000000000000000000000..a281dae460ce30574c1f6b58669adbe9fdef0878
--- /dev/null
+++ b/tests/test_lsmtool.py
@@ -0,0 +1,39 @@
+#! /usr/bin/env python
+# Runs an example of each operation
+import lsmtool
+
+s = lsmtool.load('tests/no_patches.sky')
+
+print('Select individual sources with Stokes I fluxes above 1 Jy')
+s.select('I > 1.0 Jy')
+
+print('Transfer patches from patches.sky')
+s.transfer('tests/patches.sky')
+
+print('Remove patches with total fluxes below 2 Jy')
+s.remove('I < 2.0 Jy', aggregate='sum')
+
+print('Ungroup the skymodel')
+s.ungroup()
+
+print('Concatenate with concat.sky')
+s.concatenate('tests/concat.sky', matchBy = 'position', radius = '30 arcsec', keep = 'from2')
+
+print('Add a source')
+s.add({'Name': 'src1', 'Type': 'POINT', 'Ra': 277.4232, 'Dec': 48.3689, 'I': 0.69})
+
+print('Group using tessellation to a target flux of 50 Jy')
+s.group('tessellate', targetFlux = '50.0 Jy')
+
+print('Move patch Patch_1 to 16:04:16.2288, 58.03.06.912')
+s.move('Patch_1', position = ['16:04:16.2288', '58.03.06.912'])
+
+print('Merge patches Patch_0 and Patch_2')
+s.merge(['Patch_0', 'Patch_2'], name = 'merged_patch')
+
+print('Set patch positions to midpoint of patch and write final model to file')
+s.setPatchPositions(method='mid')
+s.write('tests/final.sky', clobber=True)
+
+print('Plot the sky model')
+s.plot('tests/plot.pdf')