This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.8961,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.3961 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V6494 Sgr,2461146.8961,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V6494 Sgr 20260416.3961 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.8961,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.3961 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.8961,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.3961 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.8961,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.3961 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2109 Sgr,2461146.8961,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2109 Sgr 20260416.3961 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.0818-16.6101,2461146.8961,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.0818-16.6101 20260416.3961 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.8961,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.3961 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194507.69-161719.3,2461146.8961,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194507.69-161719.3 20260416.3961 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192726-2057.8,2461146.8961,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192726-2057.8 20260416.3961 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 16850142,2461146.8961,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16850142 20260416.3961 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193601.41-160336.0,2461146.8961,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193601.41-160336.0 20260416.3961 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190413.85-211936.5,2461146.8961,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190413.85-211936.5 20260416.3961 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191718-1953.4,2461146.8961,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J191718-1953.4 20260416.3961 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191921-2128.2,2461146.8961,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J191921-2128.2 20260416.3961 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194442-1722.2,2461146.8961,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J194442-1722.2 20260416.3961 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192805-2214.9,2461146.8961,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192805-2214.9 20260416.3961 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190815.15-194531.8,2461146.8961,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190815.15-194531.8 20260416.3961 12.67CV 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461146.89647326 16.04.2026 09:30:45.290 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.53
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: 5 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): 12047
Objects passed selection criteria: 12042
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 11194.5
Average stars matched: 10201.2 (91.1273 %)
Memory usage VmPeak: 116700 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 04:35:12 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461146.89647326 16.04.2026 09:30:45.290 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 168
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.17
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: 73 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): 103505
Objects passed selection criteria: 103379
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: 96682.5
Average stars matched: 86833.5 (89.813 %)
Memory usage VmPeak: 1886288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 04:37:54 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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: 2461146.89573638
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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 938.1'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:22.678 -18:00:40.27 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Image size: 938.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:18.991 -17:59:58.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:18.991 -17:59:58.37
Angular distance between the image centers 0.0187 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Image size: 938.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:16.378 -17:59:35.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:16.378 -17:59:35.15
Angular distance between the image centers 0.0308 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 19:33:18.991 -17:59:58.37
Second-epoch second image center 19:33:16.378 -17:59:35.15
Angular distance between the image centers 0.01220 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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.R8uTSPsqlt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.0bHUjrLXh3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits &> /tmp/tmp.92ytGmq0pU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits &> /tmp/tmp.qxUQ7Qae6d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 11017 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 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 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 deg
Loaded 13778 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): 8233 out of 8546 total matches.
Matched with Tycho-2 8546 out of 11017 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784657
a=0.000000 b=1.000000 c=22.784657
From vast_summary.log: estimated ref. image limiting mag.: -8.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
3.0 pix fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
3.0 pix fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.6 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (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.R8uTSPsqlt (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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0bHUjrLXh3 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13041 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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.92ytGmq0pU (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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=817, passed=12982
Got 12982 stars (including 12157 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat
util/solve_plate_with_UCAC5 got 12982 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 12526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 12527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 12527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.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.qxUQ7Qae6d (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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=833, passed=13071
Got 13071 stars (including 12228 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat
util/solve_plate_with_UCAC5 got 13071 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 12639 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 12637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 12632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 949 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_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22338.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22281_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22281_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:16:31.50 -18:01:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22302_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 22302_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22310_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22310_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:29:19.17 -15:11:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22318_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22318_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:19:06.50 -15:53:20.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22320_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22320_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:08:21.25 -17:01:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22323_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22323_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:53.07 -21:00:00.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 22324_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22324_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:19:32.59 -16:58:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.228 4180839367732835328 289.88530866406 -16.96875493507 10.5876 9.2837 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22325_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22325_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:14:48.50 -16:32:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.951 4088039486843265280 288.70160360319 -16.54215749164 9.9142 8.5559 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22328_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22328_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:20:28.33 -14:16:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22329_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22329_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:24:52.98 -18:09:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 2.127 4179717590991002752 291.22014627691 -18.15641425607 12.0827 10.1632 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22330_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22330_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:12.35 -16:41:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22331_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22331_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:43.05 -18:55:29.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22333_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22333_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:15:24.28 -16:07:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22337_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22337_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:15.11 -19:10:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 3.450 4087039824616552960 286.56195921617 -19.17308332192 10.8460 9.5385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22338_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 22338_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22340_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22340_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:19:03.03 -17:29:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.752 4084731945395693440 289.76241167922 -17.48948101078 10.9837 9.8818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22341_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22341_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:21:33.21 -15:55:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.551 4184012897581552000 290.38821713637 -15.92585233125 11.3077 10.8084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22343_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22343_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:04:53.91 -17:54:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22344_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22344_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:44:42.39 -17:22:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 2.106 6871657883570494464 296.17711741656 -17.36973480880 10.1358 8.5684 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22347_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 22347_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:18:14.93 -16:59:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01564_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 01564_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:13:27.15 -21:33:39.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:22:55.95 -19:03:01.6
19:06:13.07 -15:49:55.4
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 938.1'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:22.678 -18:00:40.27 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Image size: 938.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:18.991 -17:59:58.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:18.991 -17:59:58.37
Angular distance between the image centers 0.0187 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Image size: 938.2'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:16.378 -17:59:35.15 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:16.378 -17:59:35.15
Angular distance between the image centers 0.0308 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 19:33:18.991 -17:59:58.37
Second-epoch second image center 19:33:16.378 -17:59:35.15
Angular distance between the image centers 0.01220 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/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.ToGUkOrnJn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.5D7s3SFT1c
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits &> /tmp/tmp.Qv8AwpoDn4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits &> /tmp/tmp.y0FBTD87OL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 101850 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 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 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Loaded 13790 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): 10156 out of 11996 total matches.
Matched with Tycho-2 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 120 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.9 pix fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
2.9 pix fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Limiting magnitude estimates:
14.4 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
14.3 mag. fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.6 (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.ToGUkOrnJn (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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 98878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5D7s3SFT1c (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12676, passed=138124
Got 138124 stars (including 125221 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 138124 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.Qv8AwpoDn4 (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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=9195, passed=92283
Got 92283 stars (including 82996 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat
util/solve_plate_with_UCAC5 got 92283 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 89404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 89405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 89390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.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.y0FBTD87OL (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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=6, blended=9493, passed=93319
Got 93319 stars (including 83740 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat
util/solve_plate_with_UCAC5 got 93319 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010424 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 90496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 90499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 90483 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-29-41_20.00sec_-5.00C_LIGHT_0375.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.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_2026-04-16_CI_Sgr-03-Q2b1x1_043134_TTUQ2b1x1_31758_Fc3Y2rg2/wcs_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out114544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out122280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out148175.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out07863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70897.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 31s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 10s
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Considering the candidate 148149_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148149_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:20:50.80 -20:44:11.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 148175_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148175_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:45:52.70 -14:42:28.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 148178_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148178_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:33:55.35 -15:56:47.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 148181_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148181_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:31:21.76 -20:27:35.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 148191_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148191_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:44:58.41 -17:23:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.091 6871470283695632256 296.24288622008 -17.39093147361 12.9506 12.1017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148192_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148192_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:14:40.84 -20:14:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.074 4083677930371122816 288.66896457644 -20.24101869399 12.4158 11.0551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148208_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148208_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:22:15.94 -20:40:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148209_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148209_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:58.69 -18:57:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.649 4087047074521128448 286.99416911983 -18.95656844464 13.5608 13.0480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148211_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148211_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:34:10.84 -14:27:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148212_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 148212_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 148220_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148220_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:10:16.54 -14:37:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.946 4185282940907315968 287.56918008336 -14.62551976652 13.4252 12.3865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148222_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 148222_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 148224_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148224_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:32.29 -14:50:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.579 4185270949358569216 287.38438075301 -14.83829197729 13.8589 13.2466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148232_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148232_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:54.36 -15:07:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.666 4184347423995152896 289.47652734146 -15.13020566688 13.3574 12.3471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148234_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148234_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:08:47.16 -16:46:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.656 4087964720056931840 287.19634960313 -16.77502818313 13.7299 12.9211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148239_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148239_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:25.01 -15:40:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.287 4089127999048297216 286.85369558515 -15.67773913595 12.6722 11.3377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148243_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148243_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:11:31.27 -14:01:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.474 4185467796301086080 287.88065635141 -14.01703090258 14.0391 13.4643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148246_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148246_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:08:02.77 -16:55:22.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 148247_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148247_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:18:59.04 -14:51:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148250_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148250_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:23:09.43 -17:08:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148252_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148252_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:11:29.43 -14:06:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148258_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148258_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:15:50.75 -18:49:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.918 4084108148656542848 288.96199710115 -18.82242949411 13.3499 12.7788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148266_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148266_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:30:21.67 -16:47:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148273_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148273_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:10:50.58 -16:11:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.050 4088849101045847936 287.71105144296 -16.18822989847 13.0484 12.2124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148279_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148279_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:14:05.83 -20:17:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148282_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148282_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:15:37.78 -17:28:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148283_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148283_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:12.16 -15:50:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.448 4089028939922762624 286.54997307475 -15.83363027091 12.1729 11.3022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148323_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148323_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:22:55.97 -19:03:02.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 148367_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148367_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:40:04.42 -14:04:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148373_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148373_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:05:15.86 -16:52:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148411_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148411_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:29:32.82 -21:19:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148427_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148427_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:14:01.52 -14:01:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148433_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 148433_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 148468_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148468_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:36.64 -15:57:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148472_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148472_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:18:07.55 -18:52:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148520_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148520_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:21:24.56 -19:06:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148522_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148522_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:34:17.84 -16:20:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148538_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148538_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:41.26 -17:21:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148548_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148548_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:11:56.70 -14:41:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148559_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148559_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:28.52 -15:19:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148560_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148560_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:38.55 -17:18:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148562_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148562_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:24:45.10 -18:37:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148578_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148578_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:16:26.42 -15:26:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.537 4184244825818320768 289.11071355367 -15.43347633289 13.3288 12.5757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148581_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148581_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:51.11 -20:04:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148603_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148603_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:02.02 -17:06:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148627_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148627_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:21:37.10 -17:19:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148628_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 148628_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 148647_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148647_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:56.50 -14:40:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148658_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148658_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:04:39.98 -15:07:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148663_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148663_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:14:07.84 -18:04:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148685_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148685_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:26:05.75 -15:02:44.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148711_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148711_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:43.76 -17:01:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 148717_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148717_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:46.56 -17:27:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148725_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148725_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:11:57.24 -20:13:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148739_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148739_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:05:40.50 -18:17:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.273 4087351639246250880 286.41842848247 -18.29258629971 13.0363 11.9469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148769_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148769_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:25:21.96 -17:39:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148773_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148773_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:05:23.51 -14:10:15.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 148806_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148806_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:10:19.78 -17:45:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148817_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148817_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:57.08 -19:21:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148830_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148830_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:30:03.30 -19:22:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148832_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148832_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:06.37 -15:51:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.105 4088843569136078464 286.77607703483 -15.85383972268 13.7540 12.9893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148838_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148838_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:25.29 -14:56:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.214 4089227955842101376 286.60629697268 -14.93766897797 14.1318 13.4982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148844_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148844_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:20:08.93 -21:27:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.057 4082556492923022976 290.03605958748 -21.45660652964 12.4265 10.9435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148846_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148846_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:08:26.81 -18:31:11.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 148859_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148859_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 148860_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148860_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:10:32.48 -14:34:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.056 4185285002491613056 287.63434505689 -14.56994386228 12.6889 10.8679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148870_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148870_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:22.66 -15:14:28.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
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Considering the candidate 148872_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148872_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:26.93 -17:37:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148874_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148874_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:07:48.53 -18:02:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.285 4087442791314075520 286.95188379403 -18.04062386754 14.2001 13.4318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148900_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148900_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:18:32.07 -15:27:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.171 4184274482579670272 289.63443523018 -15.45146308723 14.0401 13.5400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148904_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148904_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:18.58 -17:49:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.327 4084695764591498112 289.32674965405 -17.81890708029 13.1808 12.1379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148910_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148910_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:21:10.44 -19:21:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.339 4083467507026374144 290.29286859001 -19.36407405178 12.6809 11.1770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148913_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148913_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:11:41.22 -14:39:30.3 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 148928_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148928_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:20:04.06 -14:12:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148935_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148935_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:25.49 -16:04:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.364 4088865460596781568 287.35554112890 -16.06925252958 13.9341 13.1264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148956_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148956_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:43.88 -17:24:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.842 4087867069677966464 287.43234918084 -17.40788651777 13.7242 12.9791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148958_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148958_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:15:23.05 -19:47:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.120 4083800697703076736 288.84484672687 -19.79578633905 14.1348 13.5264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148968_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148968_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:12:07.21 -18:36:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.417 4084185767306965632 288.02954584437 -18.60857586439 13.6090 12.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148970_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148970_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:13:50.33 -15:17:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.047 4184987206635953152 288.45889676109 -15.28959493338 12.7567 11.3789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148988_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 148988_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:00.59 -16:51:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.066 4180105065758587520 294.75308876251 -16.86578790691 10.2734 8.3891 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149008_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149008_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:13:49.12 -16:34:57.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 149012_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149012_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:04:17.50 -20:22:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 5.206 4082359066181525504 286.07137417696 -20.36968139426 11.9822 10.4392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149021_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 149021_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 149024_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149024_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:09:59.13 -18:07:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.552 4087267354805670144 287.49565296545 -18.11860045098 13.5483 12.7763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149030_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 149030_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 149039_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149039_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:36:44.61 -15:19:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 5.643 4182754781405305856 294.18568025831 -15.32372164135 12.8492 10.8392 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149079_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149079_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:17.56 -20:30:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149181_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149181_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:19:03.92 -19:33:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.839 4083074534702772992 289.76611828448 -19.55864262715 13.9304 13.2198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149324_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 149324_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:22:12.72 -21:41:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.716 6772690433938702848 290.55219668641 -21.68435935096 12.3243 10.5926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 122280_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 122280_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:34:12.21 -14:11:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.629 4183069933224809344 293.55116433044 -14.18683735395 11.9534 10.4948 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91182_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 91182_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:29:19.17 -15:11:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70897_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 70897_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 114202_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 114202_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:08:22.66 -17:11:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15661_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 15661_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:42:56.58 -21:23:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114544_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 114544_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:32:53.35 -14:21:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.115 4183107041742317568 293.22225433509 -14.36130211073 11.2646 9.8461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 19154_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 19154_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 10464_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 10464_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:44:41.77 -21:58:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53152_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 53152_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 70317_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 70317_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 13586_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 13586_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:13:27.15 -21:33:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72586_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 72586_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:39:12.36 -16:41:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29275_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 29275_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 119960_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 119960_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:11:02.15 -19:43:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.247 4083936345657195264 287.75800288965 -19.71987328419 12.4263 11.0704 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13891_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 13891_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 119699_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 119699_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:06:54.38 -14:46:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.394 4089254550280542976 286.72644842739 -14.77894082806 12.4147 10.9996 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70068_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 70068_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:50:22.73 -15:59:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:16:31.54 -18:01:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57470_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 57470_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 124612_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 124612_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:37:52.15 -14:08:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124491_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 124491_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:21:52.29 -17:23:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.836 4180751986611804544 290.46707255820 -17.38809235447 11.4896 9.7402 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07863_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 07863_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:49:31.33 -17:40:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124108_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 124108_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:29:36.51 -16:44:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.001 4181035836713589760 292.40176114040 -16.74440035244 11.7896 10.3992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:26:18.49 -19:10:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83150_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 83150_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:20:28.35 -14:16:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29711_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
Preparing report for the candidate 29711_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
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Considering the candidate 117472_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 117472_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:17:30.78 -17:45:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117252_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 117252_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
**** FOUND 19:27:04.58 -14:50:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116965_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376
The candidate 116965_fd_Sgr-03-Q2b1x1_2026-04-16_04-30-45_20.00sec_-5.00C_LIGHT_0376 did not pass the final checks
