This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd
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
VARIABLE_NAME,2461138.7323,7.08,0.05,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 20260408.2323 7.08CV 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,2461138.7323,7.11,0.05,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 20260408.2323 7.11CV 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,2461138.7323,7.35,0.05,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 20260408.2323 7.35CV 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
NSV 3413,2461138.7323,9.85,0.05,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
NSV 3413 20260408.2323 9.85CV 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,2461138.7323,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2323 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7323,7.58,0.05,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 20260408.2323 7.58CV 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,2461138.7323,7.60,0.05,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
VARIABLE_NAME 20260408.2323 7.60CV 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
VARIABLE_NAME,2461138.7323,7.65,0.05,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 20260408.2323 7.65CV 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,2461138.7323,7.65,0.05,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 20260408.2323 7.65CV 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,2461138.7323,12.11,0.05,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 20260408.2323 12.11CV 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,2461138.7323,12.03,0.05,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 20260408.2323 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7323,12.14,0.05,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
VARIABLE_NAME 20260408.2323 12.14CV 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
VARIABLE_NAME,2461138.7323,12.31,0.05,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 20260408.2323 12.31CV 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 3368198810490566784,2461138.7323,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368198810490566784 20260408.2323 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7323,12.89,0.05,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 20260408.2323 12.89CV 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,2461138.7323,13.10,0.05,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 20260408.2323 13.10CV 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,2461138.7323,13.37,0.05,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
VARIABLE_NAME 20260408.2323 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
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 3368198844850342016,2461138.7323,13.30,0.05,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 3368198844850342016 20260408.2323 13.30CV 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
Mean magnitude and position on the discovery images:
2026 04 08.2323 2461138.7323 13.48 07:09:09.85 +22:42:40.1
194.24270 13.85611 galactic Gem Second-epoch detections are separated by 1.5" and 7.9 pix This object is listed in planets.txt 564.7" Jupiter (-2.2mag)
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3368179946994581760 | 07:09:09.85 +22:42:40.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F9 (LAMOST DR5)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
Large-amplitude variable Gaia DR2 3368179946994581760,2461138.7323,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3368179946994581760 20260408.2323 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7323,13.60,0.05,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
target 20260408.2323 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
target,2461138.7323,13.72,0.05,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 20260408.2323 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7323,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.2323 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3368192557018249728,2461138.7323,13.86,0.05,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
Gaia DR3 3368192557018249728 20260408.2323 13.86CV 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
VARIABLE_NAME,2461138.7323,13.96,0.05,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 20260408.2323 13.96CV 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,2461138.7323,14.04,0.05,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
VARIABLE_NAME 20260408.2323 14.04CV 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
target,2461138.7323,14.15,0.05,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 20260408.2323 14.15CV 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,2461138.7323,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.2323 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7323,14.66,0.05,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 20260408.2323 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
First image: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461138.73256464 08.04.2026 05:34:43.585 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15137
Objects passed selection criteria: 15117
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 13883.2
Average stars matched: 13615 (98.0678 %)
Memory usage VmPeak: 122092 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 Wed Apr 8 01:23:17 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: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
First image: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461138.73256464 08.04.2026 05:34:43.585 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 159
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 60 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): 105362
Objects passed selection criteria: 105121
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 97022
Average stars matched: 93975.5 (96.86 %)
Memory usage VmPeak: 2010936 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 Wed Apr 8 01:25:23 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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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: 2461138.73194259
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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
Saving wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits to local_wcs_cache/
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
Saving wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits to local_wcs_cache/
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits'
wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:23:05.491 +22:00:09.66
Angular distance between the image centers 0.0038 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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:23:02.552 +22:00:30.97
Angular distance between the image centers 0.0123 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 07:23:05.491 +22:00:09.66
Second-epoch second image center 07:23:02.552 +22:00:30.97
Angular distance between the image centers 0.01280 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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits &> /tmp/tmp.ZQgZBsGgFa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits &> /tmp/tmp.ZWgyqlaeri
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits &> /tmp/tmp.p9u4zzTiLn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits &> /tmp/tmp.My3vp494vV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat' -> 'wcsmag.cat'
Read 24052 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 102.0354 to 119.5901 deg, Dec +16.4821 to +27.2938 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 102.0354 to 119.5901 deg, Dec 16.4821 to 27.2938 deg
Loaded 13967 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): 10770 out of 11768 total matches.
Matched with Tycho-2 11768 out of 24052 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914404
a=0.000000 b=1.000000 c=22.914404
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
2.2 pix Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
2.6 pix fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
2.6 pix fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Limiting magnitude estimates:
15.3 mag. Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
15.3 mag. Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
14.9 mag. fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
14.9 mag. fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (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.ZQgZBsGgFa (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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2144, passed=24052
Got 24052 stars (including 21876 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
util/solve_plate_with_UCAC5 got 24052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 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: 948 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 22932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 22932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 947 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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.ZWgyqlaeri (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/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2184, passed=23896
Got 23896 stars (including 21676 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 23896 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 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: 948 matched stars entering correct_measured_positions(), 922 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: 948 matched stars entering correct_measured_positions(), 22789 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 22792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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.p9u4zzTiLn (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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=17270
Got 17270 stars (including 16072 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 17270 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 941 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: 940 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 16936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 16934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 16934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.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.My3vp494vV (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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1203, passed=17130
Got 17130 stars (including 15910 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 17130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 941 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: 940 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 16899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 16901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 16902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
Saving fully-calibrated image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits'
Preparing the HTML report for the field Gem-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31009.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30875_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 30875_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:41:44.03 +18:03:20.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30876_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 30876_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30877_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 30877_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30878_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 30878_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30893_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 30893_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31008_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 31008_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:38:45.27 +21:14:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31009_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 31009_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:45:16.48 +21:29:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.155 674512416129702784 116.31880125363 +21.48639918118 12.2317 11.5780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31017_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 31017_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:19:22.46 +22:04:20.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07610_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 07610_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:43:02.35 +23:26:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09360_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 09360_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:07:21.54 +22:42:12.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Gem-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 ####
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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Creating symlink local_wcs_cache/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits exists and is non-empty
wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:23:05.491 +22:00:09.66
Angular distance between the image centers 0.0038 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 07:23:04.817 +21:59:59.72
Second-epoch image center 07:23:02.552 +22:00:30.97
Angular distance between the image centers 0.0123 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 07:23:05.491 +22:00:09.66
Second-epoch second image center 07:23:02.552 +22:00:30.97
Angular distance between the image centers 0.01280 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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits &> /tmp/tmp.TjyA5X8V4X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits &> /tmp/tmp.0kF4i8bzco
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits &> /tmp/tmp.C72nB1k3me
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits &> /tmp/tmp.EzD1fXKMDv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat' -> 'wcsmag.cat'
Read 150538 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 102.0340 to 119.6236 deg, Dec +16.4753 to +27.2952 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 102.0340 to 119.6236 deg, Dec 16.4753 to 27.2952 deg
Loaded 13999 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): 9026 out of 11981 total matches.
Matched with Tycho-2 11981 out of 150538 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774089
a=0.000000 b=1.000000 c=22.774089
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 116 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
2.0 pix Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
2.4 pix fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
2.3 pix fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Limiting magnitude estimates:
15.5 mag. Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
15.5 mag. Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
15.0 mag. fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
15.1 mag. fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TjyA5X8V4X (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/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=16511, passed=150509
Got 150509 stars (including 133763 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
util/solve_plate_with_UCAC5 got 150509 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 147846 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 147844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 147844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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.0kF4i8bzco (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/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Checking if the catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS catalog name: wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=16925, passed=153524
Got 153524 stars (including 136352 good ones) from the SExtractor catalog wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 153524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 149228 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 149228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 149227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits -region wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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.C72nB1k3me (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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9441, passed=102599
Got 102599 stars (including 93041 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 102599 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 943 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: 943 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 100563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 100561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 100561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.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.EzD1fXKMDv (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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=9859, passed=104627
Got 104627 stars (including 94674 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 104627 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 945 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: 945 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 102418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 102418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
WARNING: Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 102417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits -region wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Saving fully-calibrated image wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_Gem-04-Q2b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-33-49_20.00sec_-4.90C_LIGHT_0039.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.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_2026-04-08_CI_Gem-04-Q2b1x1_003732_TTUQ2b1x1_16353_eLjqmSzd/wcs_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040.fits
Preparing the HTML report for the field Gem-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out170774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out170847.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out170874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171806.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 26s
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: 13s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170774_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170774_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:39:25.64 +19:04:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.998 672312572537302016 114.85654182626 +19.08264209040 14.4753 13.5119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170788_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170788_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:31:39.98 +25:15:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 3.214 871495288661426944 112.91593836702 +25.25193528795 14.7436 13.8035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170789_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170789_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:35:27.42 +18:36:07.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170796_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170796_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:40:30.45 +19:25:40.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170805_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170805_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:44:52.36 +17:52:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170819_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170819_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:35:09.66 +21:20:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.968 865335790162964608 113.78948937990 +21.33842186841 14.2214 13.5720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170824_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170824_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:19:05.84 +19:57:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170827_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170827_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:16:15.34 +18:20:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.215 3362326834281858944 109.06340001041 +18.34148974351 14.1468 13.3130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170828_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170828_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:37:22.94 +19:34:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170830_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170830_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:45:04.98 +19:51:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170832_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170832_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:20:41.92 +18:46:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170835_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170835_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:15:05.96 +19:49:20.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170836_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170836_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:28:18.66 +18:24:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 2.094 3170320493112787456 112.07743036344 +18.40744802352 14.0813 13.5683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170840_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170840_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:43:38.16 +18:59:43.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170842_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170842_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:51:03.35 +26:03:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.570 874043131982113408 117.76392903897 +26.05948117508 14.1539 13.6798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170845_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170845_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:47:06.35 +25:27:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170847_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170847_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:49:18.82 +21:49:59.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170855_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170855_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:18:22.88 +17:52:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170857_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170857_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:07:00.33 +18:26:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.249 3361814736742205952 106.75104633379 +18.43956870338 14.0233 13.6121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170858_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170858_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:38:19.26 +21:34:48.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170860_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170860_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:38:11.20 +20:05:26.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170863_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170863_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:39:57.08 +18:32:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.823 671482028942095872 114.98749387797 +18.53738670317 13.7748 13.1425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170866_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170866_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:17:42.41 +19:59:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170869_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170869_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:13:49.38 +19:58:20.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170871_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170871_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:48:52.93 +25:41:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170873_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170873_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:32:01.82 +19:06:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.139 672463239990155136 113.00765786320 +19.11110819999 13.3844 12.8502 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170874_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170874_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170877_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170877_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:12:14.90 +20:00:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.038 3363565498554729984 108.06195231444 +20.00448939331 12.7468 11.9948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170878_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170878_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:06:18.70 +24:28:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170879_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170879_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:48:36.80 +17:57:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.736 668527190225240192 117.15301076051 +17.95754464440 12.8427 12.3789 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170880_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170880_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:08:29.71 +19:50:29.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170886_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170886_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170887_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170887_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170888_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170888_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170889_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170889_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170989_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 170989_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:12:19.27 +24:07:15.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170995_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170995_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170997_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 170997_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171012_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171012_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171025_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171025_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171066_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171066_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171086_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171086_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:32:08.84 +23:56:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171104_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171104_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171138_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171138_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:09:15.40 +21:47:43.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171155_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171155_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171177_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171177_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:26:55.47 +21:31:10.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171191_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171191_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171199_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171199_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171209_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171209_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:41:33.16 +18:14:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171223_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171223_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:48:28.41 +18:20:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171234_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171234_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:34:37.71 +19:32:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171269_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171269_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171287_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171287_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171289_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171289_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:16:17.10 +22:39:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171290_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171290_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:22:13.62 +22:40:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171303_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171303_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:27:24.68 +19:09:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171308_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171308_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:26:22.91 +18:10:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171309_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171309_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:10:22.66 +20:00:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171310_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171310_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:12:40.86 +21:21:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171329_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171329_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:10:01.78 +21:28:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171330_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171330_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:05:47.40 +18:57:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171331_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171331_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:30:28.11 +25:27:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171372_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171372_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:24:29.38 +18:53:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171378_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171378_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:36:41.71 +20:16:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.292 672652081112064896 114.17324155771 +20.28076587635 13.8377 13.3647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171408_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171408_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171436_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171436_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171443_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171443_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:08:42.60 +20:49:19.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171444_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171444_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171446_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171446_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:09:14.36 +19:32:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171451_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171451_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171455_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171455_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:44:35.47 +22:37:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171461_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171461_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:05:22.19 +21:31:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171470_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171470_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:15:18.24 +18:00:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 3.424 3362244577068316032 108.82677405969 +18.00703646801 14.2522 13.7284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171473_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171473_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:20:30.17 +22:26:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171475_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171475_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171480_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171480_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:09:22.33 +21:13:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171494_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171494_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:34:08.29 +24:52:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171503_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171503_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:29:17.30 +18:31:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171506_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171506_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:21:31.21 +25:14:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171508_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171508_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:33:32.93 +25:09:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 2.162 868579212026124288 113.38664919003 +25.16062136813 14.0466 13.4287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171515_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171515_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:25:32.35 +20:28:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 3.931 3363040726566027008 111.38407956958 +20.47663559416 14.2349 13.5668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171516_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171516_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:51:08.65 +20:50:29.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171517_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171517_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171519_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171519_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:10:10.91 +18:56:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 3.364 3363346047201920000 107.54455945374 +18.94688995385 13.9722 13.2567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171520_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171520_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:24:12.08 +21:26:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171527_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171527_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:08:01.25 +20:09:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171528_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171528_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:18:59.26 +25:56:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171531_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171531_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:04:04.98 +23:41:32.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171538_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171538_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:32:40.01 +21:25:14.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171549_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171549_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:11:39.90 +20:41:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171553_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171553_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:17:31.11 +18:03:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171570_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171570_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:14:39.41 +25:20:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 5.171 870805035877717632 108.66493414647 +25.34105538975 14.2098 13.6351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171575_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171575_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:08:14.67 +23:46:04.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171577_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171577_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:30:19.70 +20:47:10.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171613_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171613_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:32:09.25 +20:50:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 3.124 864919315774540032 113.03767014489 +20.84371629659 14.5937 13.9816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171615_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171615_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:14:11.59 +24:02:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171639_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171639_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:18:50.38 +19:50:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.602 3363653188903750144 109.71001477285 +19.84928699144 14.4272 13.9460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171642_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171642_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:09:34.01 +24:10:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171650_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171650_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:10:10.75 +23:34:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.238 3368384009480289024 107.54473009109 +23.58099401420 14.2104 13.5824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171674_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171674_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:08:19.35 +22:50:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.568 3368197126863452544 107.08078426901 +22.84656207451 14.4420 13.9676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171679_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171679_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:06:41.61 +18:57:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.941 3361884177773068800 106.67343047107 +18.96141049714 14.4505 14.0266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171719_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171719_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:18:54.50 +18:09:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 1.424 3362076729746197632 109.72683752967 +18.15843078384 14.6933 14.0635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171720_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171720_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171721_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171721_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:08:49.59 +22:36:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.004 3368173281205055360 107.20659990305 +22.61572199975 14.0729 13.6719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171737_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171737_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:17:43.10 +21:19:14.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171750_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171750_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171759_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171759_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:25:20.54 +19:04:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 0.767 3362615215565987200 111.33538193905 +19.07679043039 14.7369 14.2271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171761_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171761_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:34:02.69 +20:57:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 2.863 864901139472619520 113.51036809143 +20.96064747954 14.8606 14.3169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171767_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171767_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:22:50.96 +22:15:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171782_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171782_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:46:50.41 +17:46:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 3.930 668193320943079168 116.70889549057 +17.77340176047 15.1347 14.7488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171785_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171785_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:26:26.86 +17:57:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171806_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
Preparing report for the candidate 171806_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171832_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171832_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:34:58.90 +20:50:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.485 864884131402348672 113.74512667924 +20.83936671017 15.5428 14.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171866_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 171866_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:21:29.73 +18:40:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.968 3362214890254164736 110.37337124358 +18.67301124469 14.9653 14.5296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47884_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 47884_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
**** FOUND 07:43:02.35 +23:26:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61021_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040
The candidate 61021_fd_Gem-04-Q2b1x1_2026-04-08_00-34-43_20.00sec_-4.90C_LIGHT_0040 did not pass the final checks
