This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125748215871128448,2461150.6248,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3125748215871128448 20260420.1248 11.21CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112254596859130368,2461150.6248,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3112254596859130368 20260420.1248 11.04CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108445441905316864,2461150.6248,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3108445441905316864 20260420.1248 10.78CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112058540192896512,2461150.6248,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3112058540192896512 20260420.1248 10.43CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102552364516545792,2461150.6248,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3102552364516545792 20260420.1248 10.44CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111435838652515712,2461150.6248,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3111435838652515712 20260420.1248 10.55CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3058235418791990400,2461150.6248,9.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3058235418791990400 20260420.1248 9.03CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114280412673088640,2461150.6248,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3114280412673088640 20260420.1248 10.12CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17210,2461150.6248,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
NSV 17210 20260420.1248 9.77CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119852462723061120,2461150.6248,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3119852462723061120 20260420.1248 9.75CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.0773+01.7811,2461150.6248,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
ATO J102.0773+01.7811 20260420.1248 10.72CV 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
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112276892032630400,2461150.6248,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
Gaia DR3 3112276892032630400 20260420.1248 11.03CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0785 Mon,2461150.6248,10.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V0785 Mon 20260420.1248 10.64CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461150.6248,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
AG Mon 20260420.1248 10.12CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Mon,2461150.6248,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
BM Mon 20260420.1248 10.79CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Mon,2461150.6248,10.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
RR Mon 20260420.1248 10.45CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461150.62521381 20.04.2026 03:00:08.473 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 7 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): 33707
Objects passed selection criteria: 33386
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 19026.2
Average stars matched: 18385.8 (96.6336 %)
Memory usage VmPeak: 136940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 22:45:01 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461150.62521381 20.04.2026 03:00:08.473 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 61
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 35 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): 233476
Objects passed selection criteria: 232598
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 140615
Average stars matched: 134519 (95.6648 %)
Memory usage VmPeak: 2116720 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 22:52:37 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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: 2461150.62444708
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'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Image size: 941.5'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:23.990 -01:59:19.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:23.990 -01:59:19.33
Angular distance between the image centers 0.0811 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:21.346 -02:00:03.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:21.346 -02:00:03.47
Angular distance between the image centers 0.0906 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 06:51:23.990 -01:59:19.33
Second-epoch second image center 06:51:21.346 -02:00:03.47
Angular distance between the image centers 0.01648 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.COzsSQ01mP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.lBnNmCkE7L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits &> /tmp/tmp.EbmiLzJ2E4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits &> /tmp/tmp.uZtQL7vhux
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 deg
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
Tycho-2 catalog search boundaries: RA 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
11.2 mag. fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
11.1 mag. fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 9.2 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.COzsSQ01mP (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
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...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.lBnNmCkE7L (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EbmiLzJ2E4 (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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=76, passed=1830
Got 1830 stars (including 1748 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat
util/solve_plate_with_UCAC5 got 1830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 1773 with non-zero local correction accuracy
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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1777 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 907 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.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.uZtQL7vhux (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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=75, passed=1765
Got 1765 stars (including 1688 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat
util/solve_plate_with_UCAC5 got 1765 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 1716 with non-zero local correction accuracy
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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 1716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 1716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 908 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52507_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 52507_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:00:28.38 -00:31:36.5 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Image size: 941.5'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:23.990 -01:59:19.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:23.990 -01:59:19.33
Angular distance between the image centers 0.0811 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:21.346 -02:00:03.47 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:21.346 -02:00:03.47
Angular distance between the image centers 0.0906 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 06:51:23.990 -01:59:19.33
Second-epoch second image center 06:51:21.346 -02:00:03.47
Angular distance between the image centers 0.01648 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.VLqhc0pEZc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.vXurMQDFKn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits &> /tmp/tmp.DKdNk7WsD0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits &> /tmp/tmp.YW2kM62aVz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 deg
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
Tycho-2 catalog search boundaries: RA 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 59 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
1.8 pix fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
1.8 pix fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
11.1 mag. fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
11.2 mag. fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
All-image limiting magnitude estimate: 11.1 (SNR ) 10.9 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VLqhc0pEZc (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
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...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.vXurMQDFKn (6) ############
Parsing command line arguments...
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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DKdNk7WsD0 (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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=565, passed=26594
Got 26594 stars (including 25988 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat
util/solve_plate_with_UCAC5 got 26594 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 25887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 25886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 25886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 907 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.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.YW2kM62aVz (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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=569, passed=26524
Got 26524 stars (including 25912 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat
util/solve_plate_with_UCAC5 got 26524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 25830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 25828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 25828 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_fd_Mon-02-Q1b1x1_2026-04-19_21-59-02_20.00sec_-4.90C_LIGHTs_0026.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.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_2026-04-19_CI_Mon-02-Q1b1x1_220109_TTUQ1b1x1_3249418_idK8oNda/wcs_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out288164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out121122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288855.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 117s
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: 9s
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Considering the candidate 288150_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288150_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288151_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288151_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288161_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288161_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288162_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288162_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288163_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288163_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288164_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288164_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:02.59 -04:31:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.92, MAG_FAINT_SEARCH_LIMIT=10.90)GAIADR2_OUTPUT=# 0.919 3103799215002782976 100.76064209246 -04.53229268374 10.4848 9.7149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288165_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288165_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:38:07.49 -01:28:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288167_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288167_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288168_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288168_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:10:07.90 +01:24:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288169_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288169_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:33:37.85 +01:56:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288172_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288172_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288352_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288352_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288364_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288364_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:54.49 +01:33:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288369_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288369_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288399_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288399_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288522_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288522_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:31.34 +01:47:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288667_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288667_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:40.17 -00:32:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.36, MAG_FAINT_SEARCH_LIMIT=11.34)GAIADR2_OUTPUT=# 0.692 3113219246514568576 102.66724852826 -00.54000569020 11.1991 10.5064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288675_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288675_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288814_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:13.14 +02:40:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288819_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 288819_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:51:37.22 +00:26:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 0.761 3113576308614129408 102.90501560737 +00.44942258340 11.7443 11.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288855_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288855_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 176200_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 176200_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 124121_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 124121_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:51:41.20 -02:24:09.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 127999_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 127999_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:49:16.40 -02:16:19.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 143246_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 143246_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:42.01 -01:45:23.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 114016_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 114016_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:58.88 -02:48:12.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154375_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 154375_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:48:19.05 -01:19:10.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160520_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 160520_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:24.61 -01:07:37.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 173456_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 173456_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:49.80 -00:32:32.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52620_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 52620_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:17.06 -05:10:25.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 152351_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 152351_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:52.80 -01:20:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 49468_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 49468_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:22.79 -05:18:58.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 121814_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 121814_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:38:20.43 -02:32:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 46808_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 46808_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:00:17.79 -05:21:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107626_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 107626_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:34:21.63 -03:04:27.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 198847_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 198847_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:41:05.44 +00:29:42.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75085_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 75085_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:54.66 -04:14:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 80991_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 80991_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:06.71 -03:54:52.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 157311_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 157311_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:33:37.98 -01:13:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 49685_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 49685_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:04:05.15 -05:19:26.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 41592_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 41592_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:56.26 -05:43:18.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 211049_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 211049_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:47:51.61 +02:24:40.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53553_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 53553_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:36:35.31 -05:12:42.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247718_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 247718_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:35:15.84 +00:53:23.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 209751_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 209751_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:29:14.82 +02:38:43.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 164997_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 164997_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:25:16.93 -00:56:51.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 149786_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 149786_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:26:39.55 -01:30:27.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75219_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 75219_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:10:13.53 -04:14:07.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82569_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 82569_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:10.66 -03:54:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 182305_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 182305_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:15.61 -00:16:35.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254067_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 254067_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:20.34 +02:54:29.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 174633_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 174633_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:51.54 -00:29:34.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 188270_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 188270_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:22:03.42 +00:10:37.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178647_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 178647_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:23.41 -00:18:07.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195635_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 195635_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:13.81 +00:17:55.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 63748_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027
The candidate 63748_fd_Mon-02-Q1b1x1_2026-04-19_22-00-08_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
