This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 278411226220546688,2461136.6640,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 278411226220546688 20260406.1640 11.05CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6640,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1640 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2071902,2461136.6640,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2071902 20260406.1640 13.78CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2110062,2461136.6640,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2110062 20260406.1640 12.39CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2112172,2461136.6640,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2112172 20260406.1640 12.16CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0438578+573332,2461136.6640,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0438578+573332 20260406.1640 11.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2131605,2461136.6640,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2131605 20260406.1640 12.05CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 03745-01205,2461136.6640,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 03745-01205 20260406.1640 12.29CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 278767571062765056,2461136.6640,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 278767571062765056 20260406.1640 12.56CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045206.63+583804.6,2461136.6640,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045206.63+583804.6 20260406.1640 13.20CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0420475+623457,2461136.6640,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0420475+623457 20260406.1640 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J067.0614+58.5138,2461136.6640,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J067.0614+58.5138 20260406.1640 13.47CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0416176+623335,2461136.6640,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0416176+623335 20260406.1640 13.48CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6640,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1640 14.07CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045050.81+645248.1,2461136.6640,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045050.81+645248.1 20260406.1640 10.68CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045356.18+582712.9,2461136.6640,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045356.18+582712.9 20260406.1640 10.56CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IX Cam,2461136.6640,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IX Cam 20260406.1640 11.86CV 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: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461136.66428737 06.04.2026 03:56:24.429 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 17252
Objects passed selection criteria: 17200
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 13946
Average stars matched: 12975.5 (93.041 %)
Memory usage VmPeak: 120348 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 23:11:35 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: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461136.66428737 06.04.2026 03:56:24.429 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 156
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 55 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): 118491
Objects passed selection criteria: 118181
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 92428
Average stars matched: 85930.2 (92.9699 %)
Memory usage VmPeak: 1941480 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 23:14:47 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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: 2461136.66365306
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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
Saving wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits to local_wcs_cache/
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
Saving wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits to local_wcs_cache/
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits'
wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:34.967 +62:00:35.66
Angular distance between the image centers 0.0184 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:37.500 +62:01:08.06
Angular distance between the image centers 0.0284 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 05:08:34.967 +62:00:35.66
Second-epoch second image center 05:08:37.500 +62:01:08.06
Angular distance between the image centers 0.01027 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/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.zAj1Vj7nll
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.UGFYDtMmht
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits &> /tmp/tmp.K4udbtGEvK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits &> /tmp/tmp.vUopn5Xl0E
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
The reference image (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat) found
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 18409 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 57.0231 to 95.6672 deg, Dec +55.2649 to +67.4913 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 57.0231 to 95.6672 deg, Dec 55.2649 to 67.4913 deg
Loaded 14048 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): 8129 out of 8891 total matches.
Matched with Tycho-2 8891 out of 18409 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955063
a=0.000000 b=1.000000 c=22.955063
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
2.0 pix Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
2.8 pix fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
2.8 pix fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Limiting magnitude estimates:
15.5 mag. Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.5 mag. Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
14.9 mag. fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
14.9 mag. fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zAj1Vj7nll (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1604, passed=18409
Got 18409 stars (including 16782 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 18409 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18199 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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.UGFYDtMmht (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1596, passed=18487
Got 18487 stars (including 16865 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 18487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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.K4udbtGEvK (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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1326, passed=14134
Got 14134 stars (including 12798 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 14134 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 13829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 13830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 13830 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.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.vUopn5Xl0E (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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1321, passed=14096
Got 14096 stars (including 12767 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 14096 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13690 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 13691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
Saving fully-calibrated image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits'
Preparing the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20943.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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
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Considering the candidate 20943_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 20943_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21714_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 21714_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:19:45.91 +64:26:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22076_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 22076_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:07:24.01 +57:49:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22509_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 22509_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:54:44.15 +64:34:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22558_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 22558_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:51:30.44 +63:46:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23197_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 23197_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:19:51.96 +63:15:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23225_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 23225_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:46:31.18 +59:02:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 3.711 278888478685529344 071.62898343868 +59.04530986913 10.5768 9.0846 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23236_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 23236_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:37:20.52 +60:18:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.415 471514944413587712 069.33496681214 +60.30745778249 11.7362 10.6924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23355_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 23355_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:35:38.06 +61:31:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.099 286130656838348032 083.90920343069 +61.52338113506 12.2138 11.3873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20623_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 20623_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:52:02.24 +57:44:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 3.058 277794125316317312 073.00903283012 +57.74130481410 11.0135 9.5551 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10918_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 10918_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:35:18.30 +62:16:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20048_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 20048_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:40:17.35 +59:35:07.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 18s
Prepared the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:24:58.50 +57:13:41.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Creating symlink local_wcs_cache/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits exists and is non-empty
wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:34.967 +62:00:35.66
Angular distance between the image centers 0.0184 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:37.500 +62:01:08.06
Angular distance between the image centers 0.0284 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 05:08:34.967 +62:00:35.66
Second-epoch second image center 05:08:37.500 +62:01:08.06
Angular distance between the image centers 0.01027 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/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.7pQxI96LaZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.7dca2xYnrD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits &> /tmp/tmp.Uxe49X8eEx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits &> /tmp/tmp.lpvBUrGLPH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
The reference image (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat) found
'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 131449 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 56.9471 to 95.6842 deg, Dec +55.1951 to +67.5012 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 56.9471 to 95.6842 deg, Dec 55.1951 to 67.5012 deg
Loaded 14165 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): 6817 out of 9000 total matches.
Matched with Tycho-2 9000 out of 131449 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.808691
a=0.000000 b=1.000000 c=22.808691
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 103 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
1.9 pix Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
2.6 pix fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
2.7 pix fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Limiting magnitude estimates:
15.6 mag. Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.6 mag. Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
15.0 mag. fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
15.0 mag. fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.7pQxI96LaZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=12667, passed=131418
Got 131418 stars (including 118531 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 131418 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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.7dca2xYnrD (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=12449, passed=130538
Got 130538 stars (including 117858 good ones) from the SExtractor catalog wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 130538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129188 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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.Uxe49X8eEx (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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=8812, passed=78039
Got 78039 stars (including 69154 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 78039 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 76212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 76212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 76211 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.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.lpvBUrGLPH (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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8771, passed=77634
Got 77634 stars (including 68785 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 77634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 75811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 75811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 75809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits -region wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Saving fully-calibrated image wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_Cam-09-Q2b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-55-29_20.00sec_-5.00C_LIGHT_0099.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.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_2026-04-05_CI_Cam-09-Q2b1x1_225711_TTUQ2b1x1_22727_sm6A8412/wcs_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100.fits
Preparing the HTML report for the field Cam-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out143593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out161802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out163157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out164881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out151233.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out109716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71135.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 32s
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: 12s
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Considering the candidate 151233_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151233_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:53:17.70 +64:45:03.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151236_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151236_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:19:11.70 +65:43:42.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)
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Considering the candidate 151239_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151239_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:57:11.83 +61:50:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 2.289 283347002633833088 089.29973803222 +61.83621096223 14.5409 13.9684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151248_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151248_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:27:22.88 +63:00:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 2.192 287218245635864832 081.84617240006 +63.01525289322 14.6216 14.0225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151262_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151262_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:30:24.68 +65:35:23.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151264_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151264_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:31:42.34 +63:09:58.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 151265_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151265_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:28:00.59 +58:12:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.551 470767212087798784 067.00255044075 +58.21017804693 13.4618 12.8691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151270_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151270_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:56:19.90 +61:29:53.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 151276_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151276_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:21:55.67 +58:37:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.044 470923892495009664 065.48276875636 +58.63171341496 13.0571 12.4578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151277_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151277_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:44.92 +58:57:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.155 281662963136837632 085.68737256227 +58.95555277619 14.3366 13.6516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151288_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151288_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:41:01.81 +65:42:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 151302_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151302_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:37:47.21 +62:12:09.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 151305_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151305_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:25:03.84 +58:23:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.234 470735738570374528 066.26574574381 +58.39687864632 13.0195 12.4392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151308_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151308_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:15.91 +61:21:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.651 283450288008424832 085.56664106139 +61.35504017084 13.3924 12.6169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151309_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 151309_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151313_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151313_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:23:45.15 +57:14:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.606 278452870223512064 065.93940786650 +57.23823302181 12.9364 12.3895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151319_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151319_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:33:02.17 +62:05:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151323_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151323_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:14:58.38 +63:06:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151326_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151326_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:29:38.23 +58:52:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.265 470801881063192832 067.40811862395 +58.87325254041 13.9715 13.3077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151330_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151330_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:22:24.46 +58:13:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.026 470711618033545856 065.60106220171 +58.21913481393 12.6461 11.9889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151334_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151334_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:46:06.99 +60:17:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151339_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151339_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:37:03.99 +57:35:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151340_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151340_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:43:41.95 +57:41:13.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151364_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151364_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:26:51.59 +57:47:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.891 278504886569358976 066.71336177625 +57.79163523194 12.1202 10.7696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151383_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 151383_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:28:48.93 +65:17:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152278_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 152278_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:06:21.13 +58:57:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 153926_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 153926_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:41:13.89 +58:04:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154754_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 154754_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:13:17.16 +62:42:02.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154883_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 154883_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:19:39.78 +58:06:53.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155943_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 155943_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:42:31.93 +61:17:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156050_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 156050_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:56:16.69 +63:17:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156259_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 156259_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:28:38.60 +64:17:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156723_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 156723_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:14:52.45 +63:07:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157011_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 157011_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:29:12.72 +62:41:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157590_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 157590_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:06:12.58 +61:09:37.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 157615_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 157615_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:44:20.85 +60:48:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157945_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 157945_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:50:58.78 +65:46:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158093_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 158093_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:38:02.03 +63:56:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158538_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 158538_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:29:13.99 +57:52:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158718_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 158718_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:48:38.71 +59:31:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158823_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 158823_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:34:41.79 +57:49:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159069_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159069_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:43:40.59 +58:53:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159253_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159253_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:30:51.08 +63:58:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159351_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159351_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:25:22.84 +59:49:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159355_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159355_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:46:08.09 +60:53:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159394_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159394_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:39:46.16 +59:27:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159400_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159400_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:05:09.34 +60:10:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159622_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159622_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:05:12.43 +64:37:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.801 479202699654073600 076.30197933634 +64.62368812301 11.9978 9.9496 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159818_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159818_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:32:11.97 +65:21:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159927_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 159927_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:18:44.82 +64:09:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.365 478225646132310400 079.68693537093 +64.16023145149 13.9852 13.3634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160230_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160230_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:31:13.86 +60:38:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.973 282950040278813952 082.80670141614 +60.64761510204 14.6984 14.0215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160231_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160231_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:49:35.68 +60:47:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 0.681 282435885451777920 087.39827924149 +60.79822484484 14.0783 13.3014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160361_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160361_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:44:08.10 +62:21:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.255 286556511435549824 086.03434670291 +62.35501747756 14.1350 13.5827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160371_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160371_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:34:11.39 +63:57:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160404_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160404_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:25:36.46 +59:49:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160578_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160578_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:22:25.98 +60:19:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160683_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160683_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:36:51.21 +59:40:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160779_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 160779_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:43:09.47 +59:48:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.109 282321158285337472 085.79007103985 +59.81503412695 14.2382 13.6690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161082_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161082_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:17:16.46 +59:28:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161318_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161318_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:15:18.02 +59:22:56.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 161555_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161555_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:03:24.23 +61:24:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161718_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161718_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:37:11.97 +59:25:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.476 281926055654255872 084.29949359423 +59.42438197020 14.3753 13.4366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161760_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161760_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:59:49.50 +61:42:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.809 282582945132128768 089.95661748356 +61.70938587164 14.5013 14.1479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161802_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161802_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:48:38.54 +58:18:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 4.064 278066872919684352 072.16003618210 +58.31465826966 12.8297 11.1776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 161814_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 161814_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:12:37.46 +61:30:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162415_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 162415_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:35:20.83 +62:53:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.480 286500505061494400 083.83672841844 +62.88638026232 14.8296 14.2940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162467_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 162467_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:34:51.43 +60:45:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.145 283030755602135424 083.71357006301 +60.75095258297 15.1194 14.4721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162722_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 162722_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:47:23.87 +57:49:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 4.888 277978156074866816 071.84857753227 +57.82217021116 12.6940 11.0764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 163157_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 163157_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:34:24.28 +61:40:28.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
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Considering the candidate 164881_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 164881_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:46:13.00 +62:09:17.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)
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Considering the candidate 165385_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 165385_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:40:16.26 +63:04:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.182 286518062887927680 085.06759000261 +63.07474072665 15.2293 14.5865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61241_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 61241_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 20974_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 20974_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
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Considering the candidate 44559_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 44559_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:40:17.38 +59:35:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23430_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 23430_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 28304_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 28304_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 103232_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 103232_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:33:39.45 +62:33:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19902_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 19902_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 17362_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 17362_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 114638_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 114638_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:54:44.19 +64:34:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100048_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 100048_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:24:46.67 +62:12:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123975_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 123975_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:51:30.50 +63:46:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143593_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 143593_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:37:35.06 +64:38:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.278 482190519423303808 069.39425806688 +64.63452227624 11.9982 10.3327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35828_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 35828_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 124534_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 124534_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:31:43.48 +64:14:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121037_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 121037_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:19:45.90 +64:26:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28374_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 28374_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 126348_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 126348_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:35:45.79 +63:12:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81854_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 81854_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:35:18.46 +62:16:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29216_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 29216_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 73386_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 73386_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:23:28.78 +62:29:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92395_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 92395_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:19:51.82 +63:15:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81364_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 81364_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:17:09.65 +61:36:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142197_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 142197_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 05:12:27.83 +63:01:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127816_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 127816_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 141980_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 141980_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 146855_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 146855_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
**** FOUND 04:50:36.67 +58:17:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126152_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 126152_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 57134_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
Preparing report for the candidate 57134_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
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Considering the candidate 25949_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100
The candidate 25949_fd_Cam-09-Q2b1x1_2026-04-05_22-56-24_20.00sec_-4.90C_LIGHT_0100 did not pass the final checks
