This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.2796* 13 10 53.66 +18 32 35.5 11.3 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.7796,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.2796 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:10:53.66 +18:32:35.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.2796* 13 01 01.07 +17 51 17.8 13.9 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.7796,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.2796 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:01:01.07 +17:51:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.2796* 12 42 38.11 +20 21 47.8 12.5 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.7796,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.2796 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:42:38.11 +20:21:47.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.2796* 12 55 55.54 +24 03 49.4 13.9 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.7796,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.2796 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:55:55.54 +24:03:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.2796* 13 09 53.56 +23 25 41.0 14.4 U Com 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J13095360+2325410,2461119.7796,14.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J13095360+2325410 20260320.2796 14.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:09:53.56 +23:25:41.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20_00sec_-14_90C_LIGHT_0291_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20_00sec_-15_00C_LIGHT_0395_fits__*pix.png resample_wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20_00sec_-14_90C_LIGHT_0290_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.86784662 11.02.2026 08:49:31.948 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
First image: 2461082.86784662 11.02.2026 08:49:31.948 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Last image: 2461119.77985631 20.03.2026 06:42:49.585 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4699
Objects passed selection criteria: 4697
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4400
Average stars matched: 4152.75 (94.3807 %)
Memory usage VmPeak: 111228 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 02:56:01 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.86784662 11.02.2026 08:49:31.948 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
First image: 2461082.86784662 11.02.2026 08:49:31.948 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Last image: 2461119.77985631 20.03.2026 06:42:49.585 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 47
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 24416
Objects passed selection criteria: 24346
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 23477.2
Average stars matched: 22215.5 (94.6256 %)
Memory usage VmPeak: 128368 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 02:56:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat to cache
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461119.77925953
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits exists and is non-empty
Saving wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits to local_wcs_cache/
'wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits' -> 'local_wcs_cache/wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits'
wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits exists and is non-empty
Saving wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits to local_wcs_cache/
'wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits' -> 'local_wcs_cache/wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits'
wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits exists and is non-empty
Saving wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits to local_wcs_cache/
'wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits' -> 'local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits'
wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits exists and is non-empty
Saving wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits to local_wcs_cache/
'wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits' -> 'local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:55:24.859 +22:00:05.43
Second-epoch image center 12:55:23.107 +21:59:43.68
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:55:24.859 +22:00:05.43
Second-epoch image center 12:55:20.373 +21:59:59.66
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:55:23.107 +21:59:43.68
Second-epoch second image center 12:55:20.373 +21:59:59.66
Angular distance between the image centers 0.01146 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits &> /tmp/tmp.H5zjVKAmVK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits &> /tmp/tmp.s0mU9XAzjb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits &> /tmp/tmp.osOMZFT3rB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits &> /tmp/tmp.84wyc7YFaa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits and wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits and wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
Found non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits and wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
The reference image (wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits) and catalog (wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat) found
'wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 2966 out of 4958 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.863034
a=0.000000 b=1.000000 c=22.863034
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
2.2 pix Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
2.4 pix fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
2.4 pix fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Limiting magnitude estimates:
15.3 mag. Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
15.3 mag. Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
15.3 mag. fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
15.3 mag. fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.H5zjVKAmVK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits' -> 'wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=4958
Got 4958 stars (including 4564 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
util/solve_plate_with_UCAC5 got 4958 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits -region wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.s0mU9XAzjb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits' -> 'wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=380, passed=4905
Got 4905 stars (including 4521 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat
util/solve_plate_with_UCAC5 got 4905 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits -region wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.osOMZFT3rB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, passed=5694
Got 5694 stars (including 5325 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat
util/solve_plate_with_UCAC5 got 5694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits -region wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.84wyc7YFaa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=378, passed=5668
Got 5668 stars (including 5283 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat
util/solve_plate_with_UCAC5 got 5668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits -region wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits'
Saving fully-calibrated image wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits'
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits'
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits'
Preparing the HTML report for the field Com-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20247.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20247_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
Preparing report for the candidate 20247_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20289_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 20289_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks
**** FOUND 12:54:32.13 +21:48:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20292_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 20292_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks
**** FOUND 12:34:50.66 +22:40:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20303_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 20303_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks
**** FOUND 12:36:51.61 +18:48:04.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Com-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:10:53.66 +18:32:35.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat to cache
SExtractor catalog cache: saved Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Creating symlink local_wcs_cache/wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
Creating symlink local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
Creating symlink local_wcs_cache/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits exists and is non-empty
wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits exists and is non-empty
wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits exists and is non-empty
wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:55:24.859 +22:00:05.43
Second-epoch image center 12:55:23.107 +21:59:43.68
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:55:24.859 +22:00:05.43
Second-epoch image center 12:55:20.373 +21:59:59.66
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 12:55:23.107 +21:59:43.68
Second-epoch second image center 12:55:20.373 +21:59:59.66
Angular distance between the image centers 0.01146 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits &> /tmp/tmp.qlSSRESTo5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits &> /tmp/tmp.GGgexcO3eb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits &> /tmp/tmp.KgsbByXDCp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits &> /tmp/tmp.cZeT13B2vX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits and wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits and wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
Found non-empty wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits and wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
The reference image (wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits) and catalog (wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat) found
'wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3023 out of 27072 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749064
a=0.000000 b=1.000000 c=22.749064
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
2.0 pix Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
2.3 pix fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
2.3 pix fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Limiting magnitude estimates:
15.5 mag. Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
15.4 mag. Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
15.5 mag. fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
15.5 mag. fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qlSSRESTo5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits' -> 'wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1034, passed=27063
Got 27063 stars (including 25975 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat
util/solve_plate_with_UCAC5 got 27063 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits -region wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GGgexcO3eb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits' -> 'wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WCS_IMAGE_NAME=wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WCS-calibrated image found: wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
Checking if the catalog wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits alredy exist and is non-empty...
Catalog wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat corresponding to the image wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
WCS catalog name: wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=992, passed=26674
Got 26674 stars (including 25634 good ones) from the SExtractor catalog wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat
util/solve_plate_with_UCAC5 got 26674 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits -region wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KgsbByXDCp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1100, passed=27371
Got 27371 stars (including 26243 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat
util/solve_plate_with_UCAC5 got 27371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits -region wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cZeT13B2vX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
WCS_IMAGE_NAME=wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
WCS-calibrated image found: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Checking if the catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat corresponding to the image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
WCS catalog name: wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1137, passed=27524
Got 27524 stars (including 26357 good ones) from the SExtractor catalog wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat
util/solve_plate_with_UCAC5 got 27524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits -region wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_Com-03-Q2b1x1_2026-02-11_02-49-31_20.00sec_-15.00C_LIGHT_0395.fits
Saving fully-calibrated image wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_Com-03-Q2b1x1_2026-02-11_02-50-24_20.00sec_-14.90C_LIGHT_0396.fits
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-41-58_20.00sec_-14.90C_LIGHT_0290.fits
Saving fully-calibrated image wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Com-03-Q2b1x1_015857_TTUQ2b1x1_17055_v4uuff7W/wcs_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291.fits
Preparing the HTML report for the field Com-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out31515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32032.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 31513_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 31513_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks
**** FOUND 12:28:16.16 +17:52:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31515_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
Preparing report for the candidate 31515_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31516_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 31516_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks
**** FOUND 13:14:33.95 +22:42:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31560_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 31560_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks
**** FOUND 13:10:53.65 +18:32:35.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 31622_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
Preparing report for the candidate 31622_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
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Considering the candidate 31763_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291
The candidate 31763_fd_Com-03-Q2b1x1_2026-03-20_01-42-49_20.00sec_-14.90C_LIGHT_0291 did not pass the final checks