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Alexander Kutkin
apipeline
Commits
c7a66e8c
Commit
c7a66e8c
authored
Aug 9, 2021
by
Alexander Kutkin
Browse files
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fixed wrong mask file usage
parent
4abda057
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Changes
3
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3 changed files
cluster.py
+11
-9
11 additions, 9 deletions
cluster.py
imcal.py
+14
-13
14 additions, 13 deletions
imcal.py
imcal.yml
+5
-9
5 additions, 9 deletions
imcal.yml
with
30 additions
and
31 deletions
cluster.py
+
11
−
9
View file @
c7a66e8c
...
...
@@ -378,12 +378,6 @@ def auto_clustering(fig, ax, df, wcs, resid_data, pix_arcmin_scale, nbright,
small_resid
=
resid_data
[
py
-
boxsize
:
py
+
boxsize
,
px
-
boxsize
:
px
+
boxsize
]
ellipse_mean
,
ecc
,
amaj
,
numpix
=
ellipses_coh
(
small_resid
,
amin
=
20
,
amax
=
boxsize
-
1
,
dr
=
1.0
)
# print ellipse_mean, ecc, amaj, numpix
# if abs(ring_mean/resid_mean) > 1.7e5:
# if abs(ring_mean/small_resid_mean) > 1e4:
if
nclusters
==
'
auto
'
:
if
abs
(
ellipse_mean
/
rms
)
>
1.4
:
...
...
@@ -451,12 +445,20 @@ def auto_clustering(fig, ax, df, wcs, resid_data, pix_arcmin_scale, nbright,
return
final_clusters
# TODO
def
voronoy_clustering
():
"""
Use Voronoy clustering instead of fixed radius around sources
"""
pass
def
main
(
img
,
resid
,
model
,
auto
=
True
,
add_manual
=
False
,
nclusters
=
5
,
boxsize
=
250
,
nbright
=
80
,
cluster_radius
=
5
,
cluster_overlap
=
1.6
):
path
=
os
.
path
.
split
(
os
.
path
.
abspath
(
img
)
)
[
0
]
output
=
os
.
path
.
splitext
(
img
)[
0
]
+
'
-clustered.txt
'
imgbase
=
os
.
path
.
split
ext
(
img
)[
0
]
output
=
imgbase
+
'
-clustered.txt
'
df
=
pd
.
read_csv
(
model
,
skipinitialspace
=
True
)
df
[
'
ra
'
]
=
df
.
Ra
.
apply
(
ra2deg
)
...
...
@@ -491,7 +493,7 @@ def main(img, resid, model, auto=True, add_manual=False, nclusters=5, boxsize=25
if
clusters
:
write_df
(
df
,
clusters
,
output
=
output
)
fig
.
tight_layout
()
fig
.
savefig
(
path
+
'
/
clustering.png
'
)
fig
.
savefig
(
imgbase
+
'
-
clustering.png
'
)
return
output
...
...
This diff is collapsed.
Click to expand it.
imcal.py
+
14
−
13
View file @
c7a66e8c
...
...
@@ -326,13 +326,13 @@ def main(msin, outbase=None, cfgfile='imcal.yml'):
img1
=
outbase
+
'
_1
'
img2
=
outbase
+
'
_2
'
img3
=
outbase
+
'
_3
'
img_final
=
outbase
img_final
=
outbase
+
'
-dical
'
img_ddsub
=
outbase
+
'
-ddsub
'
img_ddcal
=
outbase
+
'
-ddcal
'
mask0
=
'
mask0.fits
'
mask1
=
'
mask1.fits
'
mask2
=
'
mask2.fits
'
mask0
=
outbase
+
'
-
mask0.fits
'
mask1
=
outbase
+
'
-
mask1.fits
'
mask2
=
outbase
+
'
-
mask2.fits
'
model1
=
outbase
+
'
_model1.sourcedb
'
model2
=
outbase
+
'
_model2.sourcedb
'
...
...
@@ -364,45 +364,46 @@ def main(msin, outbase=None, cfgfile='imcal.yml'):
threshold
=
img_max
/
cfg
[
'
clean0
'
][
'
max_over_thresh
'
]
wsclean
(
ms_split
,
outname
=
img0
,
automask
=
None
,
save_source_list
=
False
,
multifreq
=
False
,
mgain
=
None
,
kwstring
=
f
'
-threshold
{
threshold
}
'
)
if
not
os
.
path
.
exists
(
'
mask0.fits
'
)
:
create_mask
(
img0
+
'
-image.fits
'
,
img0
+
'
-residual.fits
'
,
clipval
=
20
,
outname
=
'
mask0.fits
'
)
create_mask
(
img0
+
'
-image.fits
'
,
img0
+
'
-residual.fits
'
,
clipval
=
20
,
outname
=
mask0
)
# clean1
if
not
os
.
path
.
exists
(
img1
+
'
-image.fits
'
)
and
(
not
os
.
path
.
exists
(
img1
+
'
-MFS-image.fits
'
)):
wsclean
(
ms_split
,
outname
=
img1
,
**
cfg
[
'
clean1
'
])
# fast shallow clean
wsclean
(
ms_split
,
fitsmask
=
mask0
,
outname
=
img1
,
**
cfg
[
'
clean1
'
])
# fast shallow clean
if
not
os
.
path
.
exists
(
model1
):
makesourcedb
(
img1
+
'
-sources.txt
'
,
out
=
model1
)
# dical1
if
not
os
.
path
.
exists
(
dical1
):
dical1
=
dical
(
ms_split
,
model1
,
msout
=
dical1
,
h5out
=
h5_1
,
**
cfg
[
'
dical1
'
])
view_sols
(
h5_1
,
outname
=
'
dical1
'
)
# clean2
if
(
not
os
.
path
.
exists
(
img2
+
'
-image.fits
'
))
and
(
not
os
.
path
.
exists
(
img2
+
'
-MFS-image.fits
'
)):
wsclean
(
dical1
,
outname
=
img2
,
**
cfg
[
'
clean2
'
])
create_mask
(
img2
+
'
-image.fits
'
,
img2
+
'
-residual.fits
'
,
clipval
=
7
,
outname
=
'
mask1
.fits
'
)
wsclean
(
dical1
,
fitsmask
=
mask0
,
outname
=
img2
,
**
cfg
[
'
clean2
'
])
create_mask
(
img2
+
'
-image.fits
'
,
img2
+
'
-residual.fits
'
,
clipval
=
7
,
outname
=
mask1
)
if
not
os
.
path
.
exists
(
model2
):
makesourcedb
(
img2
+
'
-sources.txt
'
,
out
=
model2
)
# dical2
if
not
os
.
path
.
exists
(
dical2
):
dical2
=
dical
(
dical1
,
model2
,
msout
=
dical2
,
h5out
=
h5_2
,
**
cfg
[
'
dical2
'
])
view_sols
(
h5_2
,
outname
=
'
dical2
'
)
# clean3
if
(
not
os
.
path
.
exists
(
img3
+
'
-image.fits
'
))
and
(
not
os
.
path
.
exists
(
img3
+
'
-MFS-image.fits
'
)):
wsclean
(
dical2
,
outname
=
img3
,
**
cfg
[
'
clean3
'
])
create_mask
(
img3
+
'
-image.fits
'
,
img3
+
'
-residual.fits
'
,
clipval
=
5
,
outname
=
'
mask2
.fits
'
)
wsclean
(
dical2
,
fitsmask
=
mask1
,
outname
=
img3
,
**
cfg
[
'
clean3
'
])
create_mask
(
img3
+
'
-image.fits
'
,
img3
+
'
-residual.fits
'
,
clipval
=
5
,
outname
=
mask2
)
if
not
os
.
path
.
exists
(
model3
):
makesourcedb
(
img3
+
'
-sources.txt
'
,
out
=
model3
)
# dical3
if
not
os
.
path
.
exists
(
dical3
):
dical3
=
dical
(
dical2
,
model3
,
msout
=
dical3
,
h5out
=
h5_3
,
**
cfg
[
'
dical3
'
])
view_sols
(
h5_3
,
outname
=
'
dical3
'
)
# clean4
if
(
not
os
.
path
.
exists
(
img_final
+
'
-image.fits
'
))
and
(
not
os
.
path
.
exists
(
img_final
+
'
-MFS-image.fits
'
)):
wsclean
(
dical3
,
outname
=
img_final
,
**
cfg
[
'
clean4
'
])
wsclean
(
dical3
,
fitsmask
=
mask2
,
outname
=
img_final
,
**
cfg
[
'
clean4
'
])
# Cluster
...
...
This diff is collapsed.
Click to expand it.
imcal.yml
+
5
−
9
View file @
c7a66e8c
...
...
@@ -24,7 +24,6 @@ clean1: # wsclean setup
mgain
:
0
automask
:
20
autothresh
:
5
fitsmask
:
'
mask0.fits'
multiscale
:
False
kwstring
:
'
-use-wgridder
-parallel-deconvolution
1400'
# use this for additional wsclean options, e.g. '-weight uniform -use-idg'
...
...
@@ -32,7 +31,7 @@ dical1: # DPPP setup for direction independent calibration
solint
:
20
mode
:
'
phaseonly'
uvlambdamin
:
500
# Ignore baselines / channels with UV < uvlambdamin wavelengths.
#
cal_nchan: 3
1
# number of chans with the same solutions
cal_nchan
:
3
0
# number of chans with the same solutions
clean2
:
imagesize
:
3072
...
...
@@ -40,7 +39,6 @@ clean2:
multifreq
:
8
automask
:
10
autothresh
:
5
fitsmask
:
'
mask0.fits'
multiscale
:
True
kwstring
:
'
-use-wgridder
-parallel-deconvolution
1400
-parallel-gridding
8
-deconvolution-channels
3'
...
...
@@ -48,7 +46,7 @@ dical2:
solint
:
1
mode
:
'
phaseonly'
uvlambdamin
:
500
# Ignore baselines / channels with UV < uvlambdamin wavelengths.
cal_nchan
:
3
1
# number of chans with the same solutions
cal_nchan
:
3
0
# number of chans with the same solutions
clean3
:
imagesize
:
3072
...
...
@@ -56,7 +54,6 @@ clean3:
multifreq
:
8
automask
:
7
autothresh
:
3.5
fitsmask
:
'
mask1.fits'
multiscale
:
True
kwstring
:
'
-use-wgridder
-parallel-deconvolution
1400
-parallel-gridding
8
-deconvolution-channels
3'
...
...
@@ -64,7 +61,7 @@ dical3:
solint
:
800
mode
:
'
diagonal'
uvlambdamin
:
500
# Ignore baselines / channels with UV < uvlambdamin wavelengths.
cal_nchan
:
3
1
# number of chans with the same solutions
cal_nchan
:
3
0
# number of chans with the same solutions
.
clean4
:
imagesize
:
3072
...
...
@@ -73,7 +70,6 @@ clean4:
automask
:
4.5
autothresh
:
0.5
multiscale
:
True
fitsmask
:
'
mask2.fits'
kwstring
:
'
-use-wgridder
-parallel-deconvolution
1400
-parallel-gridding
8
-deconvolution-channels
3
-weight
briggs
0.0'
####################### CLUSTERING #######################
...
...
@@ -88,9 +84,9 @@ cluster:
######################## DD CALIBRATION #######################
ddcal
:
# see DPPP/DDECal documentation
solint
:
120
# Solution interval in timesteps (1
~
30sec for Apertif).
solint
:
120
# Solution interval in timesteps (1
corresponds to
30
sec
onds
for Apertif).
mode
:
'
diagonal'
# Type of constraint to apply.
nfreq
:
15
# Number of channels in each channel block, for which the solution is assumed to be constant.
nfreq
:
30
# Number of channels in each channel block, for which the solution is assumed to be constant.
startchan
:
0
nchan
:
0
uvlambdamin
:
500
# Ignore baselines / channels with UV < uvlambdamin wavelengths.
...
...
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