This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3368198844850342016,2461136.7212,6.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368198844850342016 20260406.2212 6.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,6.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 6.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,7.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 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,2461136.7212,10.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 10.03CV 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,2461136.7212,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7212,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2212 12.33CV 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 3381727854392915072,2461136.7212,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3381727854392915072 20260406.2212 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7212,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2212 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,7.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 7.05CV 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 3368198844850342016,2461136.7212,7.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368198844850342016 20260406.2212 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,2461136.7212,7.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 7.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,10.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 10.05CV 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
VARIABLE_NAME,2461136.7212,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3368195129700664576,2461136.7212,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368195129700664576 20260406.2212 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J065527.09+253420.2,2461136.7212,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J065527.09+253420.2 20260406.2212 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 3368194996559622400,2461136.7212,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3368194996559622400 20260406.2212 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 13.15CV 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
target,2461136.7212,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2212 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 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
VARIABLE_NAME,2461136.7212,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 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
VARIABLE_NAME,2461136.7212,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 14.03CV 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,2461136.7212,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 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,2461136.7212,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7212,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2212 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.9209+23.0572,2461136.7212,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.9209+23.0572 20260406.2212 13.50CV 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
KY Gem,2461136.7212,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KY Gem 20260406.2212 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070234+2205.1,2461136.7212,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070234+2205.1 20260406.2212 11.48CV 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
ASAS J070733+2455.8,2461136.7212,9.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070733+2455.8 20260406.2212 9.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J065324.2+263905,2461136.7212,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J065324.2+263905 20260406.2212 13.35CV 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
target,2461136.7212,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2212 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461136.72156667 06.04.2026 05:18:53.360 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23256
Objects passed selection criteria: 23222
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: 21084.8
Average stars matched: 20558.5 (97.5041 %)
Memory usage VmPeak: 126584 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 Mon Apr 6 00:25:59 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.70160177 12.02.2026 04:50:08.393 /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Last image: 2461136.72156667 06.04.2026 05:18:53.360 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 113
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 143 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): 140937
Objects passed selection criteria: 140612
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 116310
Average stars matched: 112077 (96.3606 %)
Memory usage VmPeak: 2032428 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 Mon Apr 6 00:30:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
SExtractor catalog cache: saved Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.72087454
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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
Saving wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits to local_wcs_cache/
'wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
Saving wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits to local_wcs_cache/
'wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits'
wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits exists and is non-empty
Saving wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits to local_wcs_cache/
'wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits' -> 'local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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 07:22:57.077 +22:00:56.59
Angular distance between the image centers 0.0338 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 07:22:55.007 +22:00:44.89
Angular distance between the image centers 0.0399 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 07:22:57.077 +22:00:56.59
Second-epoch second image center 07:22:55.007 +22:00:44.89
Angular distance between the image centers 0.00863 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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits &> /tmp/tmp.ejAZXrw7hY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits &> /tmp/tmp.1JE8jUeuu5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits &> /tmp/tmp.t1URL11F8t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits &> /tmp/tmp.1KEOX2qdRf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Gem-04-Q1b1x1_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 22.921036
a=0.000000 b=1.000000 c=22.921036
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
2.2 pix Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
4.2 pix fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
4.3 pix fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Limiting magnitude estimates:
15.3 mag. Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
15.3 mag. Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
14.6 mag. fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
14.6 mag. fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 12.1 (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.ejAZXrw7hY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_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-Q1b1x1_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(), 926 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(), 23000 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(), 23002 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(), 23002 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits -region wcs_Gem-04-Q1b1x1_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-Q1b1x1_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.1JE8jUeuu5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_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-Q1b1x1_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(), 924 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(), 22807 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(), 22805 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(), 22805 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits -region wcs_Gem-04-Q1b1x1_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-Q1b1x1_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.t1URL11F8t (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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=991, passed=18547
Got 18547 stars (including 17545 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat
util/solve_plate_with_UCAC5 got 18547 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 530 to 589 (Dec 16.1 to 27.6)
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: 939 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 18191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 530 to 589 (Dec 16.1 to 27.6)
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: 938 matched stars entering correct_measured_positions(), 18191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 18191 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits -region wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.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.1KEOX2qdRf (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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=971, passed=18398
Got 18398 stars (including 17412 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat
util/solve_plate_with_UCAC5 got 18398 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 530 to 589 (Dec 16.1 to 27.5)
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: 939 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 17992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 530 to 589 (Dec 16.1 to 27.5)
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: 938 matched stars entering correct_measured_positions(), 17994 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 17994 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits -region wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits'
Saving fully-calibrated image wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits'
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits'
Preparing the HTML report for the field Gem-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31881.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 6s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31367_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 31367_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31368_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 31368_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31369_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 31369_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31432_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 31432_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31721_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 31721_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31849_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 31849_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:19:22.41 +22:04:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.702 866193439295807360 109.84352341543 +22.07202849007 11.9919 11.3118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31855_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 31855_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:55:00.80 +25:20:29.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31857_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 31857_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:30:04.34 +22:16:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.852 866387503098113408 112.51829073104 +22.27713936467 12.1833 11.7819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31878_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 31878_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:29:06.48 +21:53:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.513 865996214397591040 112.27710131979 +21.89194857254 12.1436 11.6397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31881_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 31881_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31897_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 31897_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:52:07.28 +17:22:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31900_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 31900_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:56:50.76 +24:19:57.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09360_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 09360_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:07:21.48 +22:42:12.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07610_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 07610_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:43:02.49 +23:26:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03720_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 03720_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 25s
Prepared the HTML report for the field Gem-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:55:30.74 +25:23:23.6
07:50:37.70 +18:54:19.4
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
SExtractor catalog cache: saved Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat to cache
SExtractor catalog cache: saved Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Creating symlink local_wcs_cache/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
Creating symlink local_wcs_cache/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits exists and is non-empty
wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits exists and is non-empty
wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits exists and is non-empty
wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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 07:22:57.077 +22:00:56.59
Angular distance between the image centers 0.0338 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 07:22:55.007 +22:00:44.89
Angular distance between the image centers 0.0399 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 07:22:57.077 +22:00:56.59
Second-epoch second image center 07:22:55.007 +22:00:44.89
Angular distance between the image centers 0.00863 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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits &> /tmp/tmp.vzvX0NG9nS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits &> /tmp/tmp.kQcV9l0h9X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits &> /tmp/tmp.9xWeTZoIMH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits &> /tmp/tmp.tagKQ2t0i9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Calibrating the magnitude scale
Found non-empty wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
Found non-empty wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits and wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
The reference image (wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits) and catalog (wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat) found
'wcs_Gem-04-Q1b1x1_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 22.786665
a=0.000000 b=1.000000 c=22.786665
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 92 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
2.0 pix Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
3.8 pix fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
3.8 pix fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Limiting magnitude estimates:
15.5 mag. Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
15.5 mag. Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
14.7 mag. fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
14.7 mag. fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.0 (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.vzvX0NG9nS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits' -> 'wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_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=40, blended=16511, passed=150498
Got 150498 stars (including 133752 good ones) from the SExtractor catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits.cat
util/solve_plate_with_UCAC5 got 150498 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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(), 929 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(), 147441 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: 953 matched stars entering correct_measured_positions(), 147440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 147440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits -region wcs_Gem-04-Q1b1x1_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-Q1b1x1_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.kQcV9l0h9X (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits' -> 'wcs_Gem-04-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS_IMAGE_NAME=wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS-calibrated image found: wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Checking if the catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits alredy exist and is non-empty...
Catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat corresponding to the image wcs_Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
WCS catalog name: wcs_Gem-04-Q1b1x1_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=51, blended=16925, passed=153514
Got 153514 stars (including 136342 good ones) from the SExtractor catalog wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits.cat
util/solve_plate_with_UCAC5 got 153514 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 950 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: 950 matched stars entering correct_measured_positions(), 927 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: 950 matched stars entering correct_measured_positions(), 149218 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: 950 matched stars entering correct_measured_positions(), 149218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 149217 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Gem-04-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits -region wcs_Gem-04-Q1b1x1_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-Q1b1x1_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.9xWeTZoIMH (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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6947, passed=82082
Got 82082 stars (including 75061 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat
util/solve_plate_with_UCAC5 got 82082 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 944 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(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 81229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 81231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 81232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 942 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-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits -region wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.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.tagKQ2t0i9 (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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
WCS_IMAGE_NAME=wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
WCS-calibrated image found: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Checking if the catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat corresponding to the image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
WCS catalog name: wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=7009, passed=82110
Got 82110 stars (including 75026 good ones) from the SExtractor catalog wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat
util/solve_plate_with_UCAC5 got 82110 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 530 to 589 (Dec 16.1 to 27.6)
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: 942 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 81173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 530 to 589 (Dec 16.1 to 27.6)
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: 941 matched stars entering correct_measured_positions(), 81173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 81173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 941 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits -region wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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-Q1b1x1_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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-08_20.00sec_-15.00C_LIGHT_0179.fits
Saving fully-calibrated image wcs_Gem-04-Q1b1x1_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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_Gem-04-Q1b1x1_2026-02-11_22-50-59_20.00sec_-15.00C_LIGHT_0180.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-17-53_20.00sec_-5.00C_LIGHTs_0088.fits
Saving fully-calibrated image wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.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_2026-04-06_CI_Gem-04-Q1b1x1_001945_TTUQ1b1x1_5828_Vg5a6amX/wcs_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089.fits
Preparing the HTML report for the field Gem-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out161071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out161126.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out174651.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out101401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70707.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 32s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 16s
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Considering the candidate 174602_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174602_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:51:26.54 +26:24:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174614_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174614_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:53:19.00 +24:22:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.496 3381245855983424640 103.32886870107 +24.38258434409 13.5140 13.0491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174625_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174625_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:24:07.40 +17:07:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 4.946 3169835780284035840 111.02957298034 +17.13178366340 14.2926 13.6651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174634_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174634_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:35:41.15 +17:07:01.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)
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Considering the candidate 174636_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174636_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:47:52.85 +24:48:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174641_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174641_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:59:14.23 +25:32:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.079 3381788671130046208 104.80834390602 +25.53410024396 13.7633 13.1139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174646_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174646_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:54:14.88 +21:57:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.548 3378457112242422144 103.56169939347 +21.95661038015 13.8002 13.4031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174647_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174647_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:53:43.54 +20:07:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.532 3365971852768159232 103.43147618912 +20.12155755498 13.4228 12.9580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174650_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174650_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:18:11.02 +26:56:02.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)
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Considering the candidate 174651_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174651_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:55:14.45 +18:18:52.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 174662_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174662_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:51:51.37 +20:02:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.003 3365780331587225728 102.96446235464 +20.03319187710 13.2894 12.8801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174669_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174669_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:38:02.69 +19:15:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174671_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174671_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:23:42.98 +25:33:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 174687_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174687_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:48:29.33 +16:52:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 174688_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174688_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:58:47.59 +22:35:55.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 174689_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174689_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:51:23.00 +20:58:01.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 174696_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 174696_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:00:22.99 +23:39:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.493 3380585118214333696 105.09544218437 +23.66595832006 13.3001 12.8677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174700_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 174700_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 174704_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 174704_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 174705_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 174705_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 174706_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 174706_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 174773_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 174773_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 174887_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 174887_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175015_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175015_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175157_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175157_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:58:38.63 +19:12:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.084 3365055268089047040 104.66087203895 +19.21470642779 11.8311 11.1762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175231_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175231_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:43:14.52 +22:23:12.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 175270_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175270_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175300_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175300_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175316_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175316_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:36:01.16 +26:51:16.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 175385_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175385_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175439_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175439_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:49:38.21 +19:18:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.978 3365634577577720576 102.40909818905 +19.30820624005 12.4239 11.7503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175465_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175465_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:59:37.39 +26:03:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.806 3381842096226402432 104.90575184022 +26.05755602596 12.6785 12.0214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175467_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175467_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:32:08.86 +23:56:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.013 866848271486423168 113.03643355898 +23.94742803196 12.8833 12.4343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175483_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175483_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:56:53.88 +20:58:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.612 3366310055673449472 104.22461329347 +20.98078354955 12.5858 11.8741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175489_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175489_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175534_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175534_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175701_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175701_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:31:54.30 +24:32:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.118 868430674877262720 112.97624590890 +24.53432858922 12.9633 12.2403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175716_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175716_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:09:15.34 +21:47:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175745_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 175745_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 175815_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175815_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:49:37.76 +19:21:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.031 3365635539650389760 102.40726954287 +19.35875551632 12.8771 12.1632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175861_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175861_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:26:55.41 +21:31:09.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 175952_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 175952_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:14:03.64 +19:28:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176014_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176014_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:02:22.25 +17:47:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.444 3361348951831265536 105.59175304550 +17.79318043179 13.4080 12.7559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176015_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176015_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:02:55.20 +24:28:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.545 3380731628138375680 105.72927396160 +24.47033427466 13.4295 12.7395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176019_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176019_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:00:56.05 +27:08:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.386 884151320333715200 105.23286915253 +27.13371214785 13.5034 12.8038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176030_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176030_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:58:49.12 +25:18:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176077_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176077_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:03:32.92 +19:14:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.228 3364963772403604224 105.88800742462 +19.23711569256 13.7612 13.1126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176098_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176098_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176147_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176147_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:46:39.54 +26:00:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176148_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176148_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:06:09.56 +19:03:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176155_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176155_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:10:22.60 +20:00:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.254 3363483859814957568 107.59441711102 +20.01356241930 13.5746 12.9182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176169_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176169_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:56:43.68 +26:07:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176189_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176189_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:46:53.87 +23:53:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.611 867540517135131520 116.72553891508 +23.89428467435 13.9658 13.5385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176194_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176194_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:22:13.59 +22:40:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176226_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176226_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:02:28.48 +25:50:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176235_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176235_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176371_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176371_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:27:24.61 +19:10:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.600 3362655553898934400 111.85239983042 +19.16627076972 13.6253 13.1669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176389_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176389_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:49:46.70 +18:31:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.821 3365337567699408896 102.44512495936 +18.51834895004 13.5820 13.3350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176399_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176399_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:05:47.36 +18:57:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.657 3361897749870228224 106.44714084385 +18.96034794383 13.6519 13.4020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176412_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176412_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:24:29.50 +18:53:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176430_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176430_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:13:12.77 +17:29:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.146 3360704298715322240 108.30302236482 +17.48898579564 14.3151 13.6279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176444_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176444_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:31:30.05 +22:53:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.224 866448392851782912 112.87364820631 +22.88635494458 13.9925 13.4333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176463_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176463_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176467_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176467_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:30:28.04 +25:27:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.466 871555315124181760 112.61708052216 +25.46270163062 13.8982 13.3178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176538_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176538_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:20:30.19 +22:26:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176556_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176556_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176564_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176564_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176569_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176569_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:44:35.47 +22:37:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176570_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176570_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176589_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176589_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176592_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176592_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:09:33.66 +24:10:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176629_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176629_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176691_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176691_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:34:46.80 +26:33:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 4.192 872090639848249088 113.69410667559 +26.56540295890 14.4007 13.9657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176775_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176775_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:33:38.44 +26:01:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.600 871647463646406400 113.41065979997 +26.01816247502 14.2870 13.9497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176787_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 176787_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 176799_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 176799_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:09:48.33 +22:46:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.702 3368181149585044352 107.45130547084 +22.77036480139 13.8751 13.2816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114417_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 114417_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:02:25.70 +17:45:24.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 96197_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 96197_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:04:06.74 +20:34:16.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 98485_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 98485_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:21:56.69 +20:26:40.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 56309_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 56309_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 61021_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 61021_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:07:21.42 +22:42:12.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22608_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 22608_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:55:30.79 +25:23:23.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 101401_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 101401_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 70707_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 70707_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 27088_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 27088_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 69772_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 69772_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:26:27.95 +22:07:53.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 47884_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 47884_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:43:02.47 +23:26:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69368_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 69368_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 07:20:07.21 +21:58:58.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 161126_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 161126_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
**** FOUND 06:50:57.69 +17:23:30.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 161117_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 161117_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 161078_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
Preparing report for the candidate 161078_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
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Considering the candidate 161071_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089
The candidate 161071_fd_Gem-04-Q1b1x1_2026-04-06_00-18-53_20.00sec_-5.00C_LIGHTs_0089 did not pass the final checks
