This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2
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
NSVS J0608537+363513,2461136.6627,11.51,0.05,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 J0608537+363513 20260406.1627 11.51CV 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 7030662,2461136.6627,10.86,0.05,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
NSVS 7030662 20260406.1627 10.86CV 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
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 J094.3569+35.0541,2461136.6627,14.07,0.05,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
ATO J094.3569+35.0541 20260406.1627 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
target,2461136.6627,13.54,0.05,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 20260406.1627 13.54CV 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 J091.0506+33.6073,2461136.6627,13.59,0.05,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 J091.0506+33.6073 20260406.1627 13.59CV 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,2461136.6627,13.57,0.05,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 20260406.1627 13.57CV 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 3451648886883614208,2461136.6627,13.60,0.05,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 3451648886883614208 20260406.1627 13.60CV 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 J091.1529+35.5894,2461136.6627,13.51,0.05,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 J091.1529+35.5894 20260406.1627 13.51CV 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 J091.0384+38.9807,2461136.6627,12.99,0.05,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 J091.0384+38.9807 20260406.1627 12.99CV 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 3453420822888609152,2461136.6627,13.04,0.05,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 3453420822888609152 20260406.1627 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.8505+34.6613,2461136.6627,13.14,0.05,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 J090.8505+34.6613 20260406.1627 13.14CV 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 J090.9837+33.9671,2461136.6627,12.84,0.05,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 J090.9837+33.9671 20260406.1627 12.84CV 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
VARIABLE_NAME,2461136.6627,14.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1627 14.66CV 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 J061622.17+362125.6,2461136.6627,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J061622.17+362125.6 20260406.1627 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J062147.45+383332.2,2461136.6627,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062147.45+383332.2 20260406.1627 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J063055.93+401700.7,2461136.6627,10.37,0.05,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 J063055.93+401700.7 20260406.1627 10.37CV 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 J0605325+350722,2461136.6627,12.68,0.05,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
NSVS J0605325+350722 20260406.1627 12.68CV 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 J060950.24+403538.2,2461136.6627,12.79,0.05,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 J060950.24+403538.2 20260406.1627 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J060323.39+344527.5,2461136.6627,13.23,0.05,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 J060323.39+344527.5 20260406.1627 13.23CV 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 J0605234+342756,2461136.6627,12.24,0.05,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 J0605234+342756 20260406.1627 12.24CV 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 J0618234+343817,2461136.6627,13.34,0.05,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 J0618234+343817 20260406.1627 13.34CV 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 J062136.94+401753.5,2461136.6627,13.37,0.05,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 J062136.94+401753.5 20260406.1627 13.37CV 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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461136.66293168 06.04.2026 03:54:27.297 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 10 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): 21797
Objects passed selection criteria: 21718
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 18100
Average stars matched: 16932.2 (93.5483 %)
Memory usage VmPeak: 123724 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 23:20:59 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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461136.66293168 06.04.2026 03:54:27.297 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 179
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 75 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): 147442
Objects passed selection criteria: 147029
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 116418
Average stars matched: 108762 (93.4231 %)
Memory usage VmPeak: 1911244 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 23:24:06 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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: 2461136.66237964
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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
Saving wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits'
wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:44.466 +37:59:45.67
Angular distance between the image centers 0.0040 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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:44.319 +38:00:23.27
Angular distance between the image centers 0.0077 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:32:44.466 +37:59:45.67
Second-epoch second image center 06:32:44.319 +38:00:23.27
Angular distance between the image centers 0.01046 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.dZTHvEhfeB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.TRkMMMRdZ2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits &> /tmp/tmp.S9k7GmrDKw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits &> /tmp/tmp.AJAnx3zTTH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 22646 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.2031 to 108.5019 deg, Dec +32.0173 to +43.3852 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 87.2031 to 108.5019 deg, Dec 32.0173 to 43.3852 deg
Loaded 14726 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): 10210 out of 11206 total matches.
Matched with Tycho-2 11206 out of 22646 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.938798
a=0.000000 b=1.000000 c=22.938798
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
3.0 pix fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
3.0 pix fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Limiting magnitude estimates:
15.3 mag. Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.3 mag. Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.9 mag. fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
14.9 mag. fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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.dZTHvEhfeB (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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2024, passed=22646
Got 22646 stars (including 20590 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 22646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 934 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: 932 matched stars entering correct_measured_positions(), 923 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: 932 matched stars entering correct_measured_positions(), 21795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.TRkMMMRdZ2 (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/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2057, passed=22538
Got 22538 stars (including 20456 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 22538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 937 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: 934 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21822 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 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.S9k7GmrDKw (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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1889, passed=19422
Got 19422 stars (including 17524 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat
util/solve_plate_with_UCAC5 got 19422 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 924 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: 921 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 19088 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 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 19090 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 19090 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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.AJAnx3zTTH (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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1882, passed=19362
Got 19362 stars (including 17472 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat
util/solve_plate_with_UCAC5 got 19362 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 924 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: 921 matched stars entering correct_measured_positions(), 908 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: 921 matched stars entering correct_measured_positions(), 19056 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 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 19056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 19056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits'
Preparing the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out33743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32531.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31102_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 31102_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:07:43.20 +37:18:57.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32083_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 32083_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:28:01.82 +36:05:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32287_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 32287_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:06:39.06 +37:57:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32401_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 32401_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:42.33 +33:55:50.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32531_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 32531_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32594_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 32594_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:52.94 +37:33:09.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32813_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 32813_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:24:37.06 +35:14:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33284_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33284_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:44:54.94 +36:47:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.383 943630256534774784 101.22903116563 +36.79844627352 12.0115 11.3246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33403_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33403_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:38:15.65 +35:21:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.045 941944778225035008 099.56555036172 +35.36580312849 12.1818 11.6521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33453_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33453_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:35:00.58 +39:39:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.864 957081892243085824 098.75267325694 +39.66191911782 11.8508 11.0010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33517_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33517_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:35:30.92 +38:31:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.138 944985821229316992 098.87923520724 +38.52175601013 12.1967 11.7629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33676_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33676_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:29:04.95 +37:45:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.879 955367577521041792 097.27119862673 +37.76365816678 11.8890 11.0326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33704_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33704_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:27:43.37 +34:51:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.138 942458108418995968 096.93082397986 +34.85686522932 11.9671 11.1804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33707_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33707_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:34:12.57 +38:02:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.997 943471274024252544 098.55271527386 +38.04687497535 12.1369 11.6271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33743_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 33743_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:30:12.32 +35:38:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.483 942600087154585088 097.55149497609 +35.64022311624 12.1202 11.3788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10384_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 10384_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Aur-04-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 ####
06:02:31.21 +36:52:23.3
06:08:54.02 +36:35:14.2
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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits exists and is non-empty
wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:44.466 +37:59:45.67
Angular distance between the image centers 0.0040 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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:44.319 +38:00:23.27
Angular distance between the image centers 0.0077 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:32:44.466 +37:59:45.67
Second-epoch second image center 06:32:44.319 +38:00:23.27
Angular distance between the image centers 0.01046 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.8E8nZq9UCM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.ZbLnt0pir0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits &> /tmp/tmp.yU3wyWlvnh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits &> /tmp/tmp.8bME2TY3ef
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 160824 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.1754 to 108.5197 deg, Dec +31.9766 to +43.3901 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 87.1754 to 108.5197 deg, Dec 31.9766 to 43.3901 deg
Loaded 14824 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): 8279 out of 11458 total matches.
Matched with Tycho-2 11458 out of 160824 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.781706
a=0.000000 b=1.000000 c=22.781706
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 118 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
1.9 pix Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
2.9 pix fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
2.9 pix fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Limiting magnitude estimates:
15.5 mag. Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.5 mag. Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
15.0 mag. fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
15.0 mag. fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (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.8E8nZq9UCM (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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=18360, passed=160792
Got 160792 stars (including 142160 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 160792 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 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: 929 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 156537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 156535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 156536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 928 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.ZbLnt0pir0 (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/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=18627, passed=162444
Got 162444 stars (including 143508 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 162444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 935 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: 932 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 158932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 158932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 158932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.yU3wyWlvnh (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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=14278, passed=98552
Got 98552 stars (including 84200 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat
util/solve_plate_with_UCAC5 got 98552 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 925 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: 922 matched stars entering correct_measured_positions(), 908 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: 922 matched stars entering correct_measured_positions(), 97262 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 97259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 97258 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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.8bME2TY3ef (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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=14404, passed=98773
Got 98773 stars (including 84294 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat
util/solve_plate_with_UCAC5 got 98773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 924 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: 921 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 97102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 97102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 921 matched stars entering correct_measured_positions(), 97102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-53-39_20.00sec_-5.00C_LIGHT_0097.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.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_Aur-04-Q2b1x1_225511_TTUQ2b1x1_14824_ihZTxSm2/wcs_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098.fits
Preparing the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out104125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out184314.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out196192.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out131604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out184476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95476.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 10s
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Considering the candidate 184301_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184301_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:41:35.50 +39:59:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 2.836 945500530109499776 100.39695856212 +39.99193608540 14.7980 14.0815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184303_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184303_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:51:13.04 +38:04:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.266 944128477036312576 102.80433920439 +38.08100935802 15.0564 14.5644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184307_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184307_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:54:20.83 +38:55:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.239 944275777234706176 103.58723378038 +38.92720577499 14.7787 14.2489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184314_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184314_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:32:31.05 +36:45:39.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 184324_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184324_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184329_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184329_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:57:35.35 +41:03:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.915 950743585665907968 104.39782740725 +41.05712629108 14.6127 14.0939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184330_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184330_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:03:19.89 +35:07:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.899 3453419341123599104 090.83317820883 +35.13066738293 13.3926 12.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184331_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184331_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:58:30.03 +38:58:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 0.855 947287408302994048 104.62483694955 +38.98166278742 14.7244 14.2300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184338_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184338_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:54:28.22 +40:37:51.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)
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Considering the candidate 184343_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184343_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:18:49.25 +41:08:31.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
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Considering the candidate 184344_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184344_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:31.71 +36:33:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.130 940612582449265792 103.13223929677 +36.56047751292 14.1307 13.6132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184365_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184365_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:17:32.14 +38:33:06.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 184367_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184367_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:28.53 +36:33:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.735 940612548089529728 103.11866471722 +36.56014813841 14.3062 13.6539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184369_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184369_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:01:17.39 +39:03:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.161 3458213319195270016 090.32285153428 +39.05897975256 13.1143 12.5359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184371_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184371_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184376_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184376_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:03:46.25 +34:58:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 0.762 3453227102682134528 090.94245005507 +34.97908345647 13.3250 12.8401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184378_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184378_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184381_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184381_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184382_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184382_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:00:27.06 +38:53:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 2.321 947231470649008128 105.11218226980 +38.89083593966 14.4666 14.1254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184384_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184384_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:02:40.70 +38:01:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.552 3457358478968658560 090.67068559029 +38.02816918759 13.1273 12.5218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184388_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184388_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:04:14.31 +34:16:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.082 3451648886882450560 091.06062329274 +34.28172905816 13.2457 12.4915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184389_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184389_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:03:37.79 +34:19:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.050 3451647134535790976 090.90580444354 +34.32395802463 13.1923 12.7343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184403_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184403_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184410_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184410_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:03:20.53 +35:24:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.113 3453433188095896704 090.83550060159 +35.40958061824 12.8398 12.1249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184418_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184418_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184435_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184435_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:01:22.00 +37:56:21.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 184442_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184442_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:49:37.15 +34:06:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184450_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184450_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:06:20.97 +33:50:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.431 3450858892074536960 091.58638385042 +33.83701350493 12.5443 12.0351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184452_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184452_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184453_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184453_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:00:37.15 +40:32:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.967 950469459376609664 105.15537872655 +40.54474020927 13.4760 12.7585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184456_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184456_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184458_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 184458_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:38:19.31 +35:49:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 184461_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184461_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 184476_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 184476_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 186172_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 186172_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:53.03 +37:33:09.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)
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Considering the candidate 186495_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 186495_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:57:29.10 +37:23:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186936_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 186936_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:02:18.09 +38:52:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.267 947307160855918336 105.57512935621 +38.87945462007 12.3463 11.8333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187630_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 187630_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:54:03.14 +33:42:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.626 939284990877534080 103.51254454022 +33.70436175828 12.9884 12.4656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189284_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 189284_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:01:18.71 +38:30:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.489 947019677221519616 105.32868457391 +38.50041173542 13.2650 11.1344 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189493_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 189493_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:17:37.68 +35:07:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189573_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 189573_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:30:54.04 +39:45:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190814_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 190814_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:51:24.34 +38:34:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191096_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191096_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:02:25.99 +36:21:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.842 940040011768384000 105.60859546589 +36.35071725279 13.6301 12.8294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191153_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191153_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:54:04.00 +37:32:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.412 941090320251063168 103.51738573679 +37.54581486371 13.7777 13.2571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191292_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191292_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:43:22.31 +37:01:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.871 943827004692012288 100.84267749313 +37.02440920383 13.4830 12.7221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191318_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191318_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:52.72 +38:52:34.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191585_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191585_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:28:04.30 +36:11:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191679_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191679_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:42:21.42 +37:43:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.404 943920944216478464 100.58929406653 +37.71853222822 13.6675 13.0001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191793_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191793_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:55:07.51 +36:03:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.990 940712706726664320 103.78127785115 +36.06253085775 13.8839 13.4480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191952_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 191952_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:40:14.57 +34:55:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192022_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 192022_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:15:42.89 +42:02:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192049_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 192049_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:00:57.42 +39:55:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.585 947435189537411072 105.23915698937 +39.92628772839 14.0552 13.4467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192134_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 192134_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:46:49.99 +40:15:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192413_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 192413_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:37:14.27 +38:26:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192561_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 192561_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:56:31.19 +36:12:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.642 940718341723821184 104.12945283167 +36.20774040824 14.1851 13.7172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192997_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 192997_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:51:25.81 +41:46:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193134_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193134_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:30:55.57 +39:45:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193333_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193333_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:56:10.74 +36:24:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.515 940724492116857344 104.04449090598 +36.40077348408 14.2775 13.7105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193463_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193463_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:57.59 +37:33:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193498_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193498_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:45:37.77 +37:28:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193615_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193615_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:55:30.52 +38:58:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.776 950278389167778688 103.87705186561 +38.97605373243 14.0252 13.1126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193713_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193713_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:06.14 +33:41:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.758 937799138351555840 103.02615901541 +33.69746090687 14.1803 13.7545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193756_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193756_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:47:03.22 +35:26:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.508 940433804433382656 101.76417547525 +35.44209562315 14.1742 13.4219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193980_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 193980_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:46:25.59 +35:23:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.141 940478716908578048 101.60654900572 +35.38796693365 13.7969 13.2137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194131_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194131_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:59:07.28 +38:01:41.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194193_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194193_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:24:22.59 +41:49:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194223_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194223_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:42:25.40 +39:00:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194336_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194336_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:16.38 +35:09:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.746 940191740077691648 103.06847184943 +35.15914800441 14.0693 13.3479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194376_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194376_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:37:48.18 +35:30:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.407 942137089680056192 099.45157036011 +35.50052396743 14.3166 13.7898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194383_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194383_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:13.38 +34:12:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.987 938624974663906048 102.55586179254 +34.21432536078 14.1870 13.7647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194405_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194405_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:13.24 +34:14:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 5.248 938625764937885696 102.55672026378 +34.23910610741 14.1996 13.6547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194452_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194452_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:34:22.71 +39:27:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194746_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194746_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:44:06.06 +35:03:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.632 938947062851461504 101.02508992936 +35.05766087159 14.3597 13.6444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194783_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194783_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:30:01.55 +35:49:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.526 942618091657468032 097.50691650834 +35.81968450233 13.9453 13.3472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194952_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 194952_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:18.77 +36:25:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195221_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 195221_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:40:53.40 +34:09:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.669 938796945154651008 100.22303775899 +34.15481479532 14.2826 13.6993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196192_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 196192_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:18.35 +37:23:29.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)
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Considering the candidate 196238_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 196238_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:57:23.25 +36:52:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.875 940901857086379392 104.34739174235 +36.87290543031 14.3115 13.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196321_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 196321_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:48:04.28 +38:03:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.975 944351025061776384 102.01692888283 +38.05194695455 14.7326 14.3923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196852_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 196852_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 196943_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 196943_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:00:15.31 +37:11:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 4.748 940886120326073856 105.06361256544 +37.19074441279 14.8145 14.2749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197089_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197089_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:34:05.01 +34:40:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.822 941701648716393728 098.52112000830 +34.68310723676 14.1997 13.4636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197167_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197167_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:23.79 +38:31:02.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)
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Considering the candidate 197271_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197271_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:55:25.13 +33:53:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 0.505 939129066384518528 103.85485903230 +33.88940865637 14.5357 14.0165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197325_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197325_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:49:43.41 +37:39:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 2.411 944092777268247424 102.43144012459 +37.65325154237 14.7134 14.1883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197408_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197408_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:14.11 +35:57:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 4.344 940371274006768768 103.05929045511 +35.95547040540 15.0458 14.3852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197482_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197482_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:33:58.18 +41:53:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197596_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197596_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:58:52.08 +37:12:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.139 940912542964746880 104.71734521535 +37.20812103071 14.7750 14.2781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197768_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197768_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:03:11.47 +40:31:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 2.875 947830945003751040 105.79839099843 +40.52528852557 14.8992 14.3809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197790_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197790_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:48:36.31 +35:10:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.330 940416835019832064 102.15134664889 +35.16657766486 14.7125 14.0358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197824_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 197824_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:03:54.15 +38:58:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.334 947146980052510208 105.97608743737 +38.97152152353 14.7441 14.2213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198004_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198004_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 07:01:01.70 +38:46:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 3.126 947215184133017088 105.25731796481 +38.77542879319 15.0811 14.6063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198019_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198019_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:58:16.41 +37:11:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.736 940916150737297280 104.56863455013 +37.19811984519 14.9692 14.3291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198025_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198025_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:49:42.42 +41:36:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.523 951705138648348032 102.42684943033 +41.61518083967 15.3345 14.6658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198086_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198086_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:50:18.01 +35:22:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 2.756 940253828123712256 102.57501737997 +35.37240430457 15.0279 14.3099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198172_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198172_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:48:17.75 +35:43:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.682 940466106884474624 102.07411922625 +35.71796805579 14.9958 14.4831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198479_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198479_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:52:42.67 +36:08:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 2.070 940398177681596032 103.17738033994 +36.14516948234 14.8526 14.3173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198557_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198557_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:59:38.24 +39:20:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.071 947393133217789056 104.90964017496 +39.33540154919 14.7473 14.2207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198716_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198716_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:45:20.64 +34:34:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 3.007 938873498651830784 101.33619369660 +34.58248567569 14.3335 13.1870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198719_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198719_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:53:44.03 +34:14:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 2.114 939340447495094784 103.43372185621 +34.23578808961 14.7613 14.1618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198722_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 198722_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:59:54.60 +38:31:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.303 947204493957678336 104.97769257932 +38.52867086129 15.0271 14.2980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61342_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 61342_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 95476_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 95476_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 104125_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 104125_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:06:43.88 +38:47:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 4.623 3457314605879491840 091.68412264631 +38.78508952853 13.6883 13.2182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53350_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 53350_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:28:01.85 +36:05:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141066_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 141066_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 91158_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 91158_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:06:39.07 +37:57:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45204_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 45204_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 131604_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 131604_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 75651_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 75651_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:02:31.23 +36:52:23.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 40251_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 40251_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 35275_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 35275_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 33022_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 33022_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 138649_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
Preparing report for the candidate 138649_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
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Considering the candidate 67916_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 67916_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:08:54.06 +36:35:14.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 127321_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 127321_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:15:48.71 +41:02:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171468_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 171468_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
**** FOUND 06:06:00.79 +36:20:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97629_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098
The candidate 97629_fd_Aur-04-Q2b1x1_2026-04-05_22-54-27_20.00sec_-4.90C_LIGHT_0098 did not pass the final checks
