This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184147.24-165948.0,2461132.8983,12.90,0.05,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
ASASSN-V J184147.24-165948.0 20260402.3983 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4101340279017089536,2461132.8983,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4101340279017089536 20260402.3983 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095633676202802432,2461132.8983,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095633676202802432 20260402.3983 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184523.28-160248.2,2461132.8983,12.70,0.05,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 J184523.28-160248.2 20260402.3983 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2058 Sgr,2461132.8983,12.38,0.05,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
V2058 Sgr 20260402.3983 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185719.20-210354.0,2461132.8983,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185719.20-210354.0 20260402.3983 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V6477 Sgr,2461132.8983,11.64,0.05,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
V6477 Sgr 20260402.3983 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J184720.82-152507.7,2461132.8983,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J184720.82-152507.7 20260402.3983 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4090006238313384576,2461132.8983,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4090006238313384576 20260402.3983 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1984 Sgr,2461132.8983,9.95,0.05,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
V1984 Sgr 20260402.3983 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DW Sgr,2461132.8983,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DW Sgr 20260402.3983 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J184836-2206.0,2461132.8983,12.38,0.05,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 J184836-2206.0 20260402.3983 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185754-2034.3,2461132.8983,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185754-2034.3 20260402.3983 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185226.48-200201.9,2461132.8983,12.09,0.05,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
ASASSN-V J185226.48-200201.9 20260402.3983 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J183946.75-140603.9,2461132.8983,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183946.75-140603.9 20260402.3983 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2035 Sgr,2461132.8983,12.52,0.05,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
V2035 Sgr 20260402.3983 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
First image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Last image: 2461132.89856343 02.04.2026 09:33:45.880 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.46
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: 6 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): 15391
Objects passed selection criteria: 15360
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 12761.5
Average stars matched: 12100.5 (94.8204 %)
Memory usage VmPeak: 121292 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:37:18 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: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
First image: 2461118.95649310 19.03.2026 10:57:11.004 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Last image: 2461132.89856343 02.04.2026 09:33:45.880 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 180
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 58 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): 171412
Objects passed selection criteria: 171094
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 139040
Average stars matched: 130244 (93.6736 %)
Memory usage VmPeak: 2005776 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:41:42 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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: 2461132.89794672
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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits exists and is non-empty
Saving wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits exists and is non-empty
Saving wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits to local_wcs_cache/
'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits'
wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
Saving wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits to local_wcs_cache/
'wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:19.690 -18:00:23.11
Angular distance between the image centers 0.07 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:19.384 -18:00:01.12
Angular distance between the image centers 0.07 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 18:40:19.690 -18:00:23.11
Second-epoch second image center 18:40:19.384 -18:00:01.12
Angular distance between the image centers 0.00623 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits &> /tmp/tmp.PpGYfwU5Mn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits &> /tmp/tmp.tg2LUNDApe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.43KC9HdUoE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.qE550r01cF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
The reference image (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits) and catalog (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat) found
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat' -> 'wcsmag.cat'
Read 18356 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.4398 to 288.3762 deg, Dec -23.2741 to -12.5442 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 271.4398 to 288.3762 deg, Dec -23.2741 to -12.5442 deg
Loaded 18433 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): 11463 out of 12239 total matches.
Matched with Tycho-2 12239 out of 18356 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.804368
a=0.000000 b=1.000000 c=22.804368
From vast_summary.log: estimated ref. image limiting mag.: -8.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
2.1 pix Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
2.9 pix fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
2.9 pix fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Limiting magnitude estimates:
14.3 mag. Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
14.5 mag. Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
13.7 mag. fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
13.7 mag. fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.PpGYfwU5Mn (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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1700, passed=18356
Got 18356 stars (including 16644 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 18356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.73"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits -region wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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.tg2LUNDApe (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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1941, passed=20338
Got 20338 stars (including 18376 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
util/solve_plate_with_UCAC5 got 20338 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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits -region wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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.43KC9HdUoE (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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=737, passed=9509
Got 9509 stars (including 8767 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 9509 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 -12.6)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.00"
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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.01"
Estimated accuracy of the plate solution: 1.15"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.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.qE550r01cF (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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=739, passed=9573
Got 9573 stars (including 8830 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 9573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 -12.6)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.98"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.00"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.01"
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
Saving fully-calibrated image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits'
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits'
Preparing the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat to cache
SExtractor catalog cache: saved Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits exists and is non-empty
wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits exists and is non-empty
wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:19.690 -18:00:23.11
Angular distance between the image centers 0.07 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:40:02.901 -17:59:22.60
Second-epoch image center 18:40:19.384 -18:00:01.12
Angular distance between the image centers 0.07 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 18:40:19.690 -18:00:23.11
Second-epoch second image center 18:40:19.384 -18:00:01.12
Angular distance between the image centers 0.00623 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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits &> /tmp/tmp.niWnbNKHxc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits &> /tmp/tmp.JVzB7Vy1BJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.BfD4rpwKa3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.945q7kbWHZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
Found non-empty wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits and wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
The reference image (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits) and catalog (wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat) found
'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat' -> 'wcsmag.cat'
Read 204414 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 271.4398 to 288.4080 deg, Dec -23.2845 to -12.4926 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 271.4398 to 288.4080 deg, Dec -23.2845 to -12.4926 deg
Loaded 18533 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): 11851 out of 16072 total matches.
Matched with Tycho-2 16072 out of 204414 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.510618
a=0.000000 b=1.000000 c=22.510618
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 133 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
2.1 pix Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
2.6 pix fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
2.6 pix fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Limiting magnitude estimates:
14.5 mag. Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
14.6 mag. Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
13.7 mag. fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
13.7 mag. fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (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.niWnbNKHxc (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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=26568, passed=204377
Got 204377 stars (including 177585 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat
util/solve_plate_with_UCAC5 got 204377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits -region wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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.JVzB7Vy1BJ (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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits' -> 'wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS_IMAGE_NAME=wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS-calibrated image found: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Checking if the catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits alredy exist and is non-empty...
Catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat corresponding to the image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
WCS catalog name: wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=30504, passed=224228
Got 224228 stars (including 193440 good ones) from the SExtractor catalog wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat
util/solve_plate_with_UCAC5 got 224228 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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits -region wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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.BfD4rpwKa3 (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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=5, blended=7863, passed=89464
Got 89464 stars (including 81535 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 89464 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.85"
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 923 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.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.945q7kbWHZ (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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=8098, passed=89900
Got 89900 stars (including 81724 good ones) from the SExtractor catalog wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 89900 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
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 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.86"
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 926 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_Sgr-02-Q2b1x1_2026-03-19_05-57-11_20.00sec_-14.90C_LIGHT_0200.fits
Saving fully-calibrated image wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_Sgr-02-Q2b1x1_2026-03-22_05-44-55_20.00sec_-14.90C_LIGHT_0338.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-32-52_20.00sec_-14.90C_LIGHT_0053.fits
Saving fully-calibrated image wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.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_2026-04-02_CI_Sgr-02-Q2b1x1_043455_TTUQ2b1x1_895_kdIKNO4K/wcs_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054.fits
Preparing the HTML report for the field Sgr-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out217251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out223118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out248938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out249236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out249117.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out120901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92127.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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: 7s
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Considering the candidate 248266_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248266_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:15:26.21 -13:55:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248269_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248269_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:37.91 -13:49:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.052 4104553704924150528 278.15774075652 -13.81715124787 12.9971 11.8953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248270_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248270_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:09.22 -15:07:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.609 4103292187110048512 278.03850436312 -15.12225764327 13.0215 11.8561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248282_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248282_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:34:11.58 -14:28:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248287_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248287_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:14:20.62 -15:54:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.174 4145733091023268480 273.58585233299 -15.90609793512 13.2820 12.9209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248300_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248300_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:28:13.64 -16:03:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.699 4097122999137229056 277.05561285717 -16.06378842224 13.1559 12.3905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248305_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 248305_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 248308_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248308_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:31:34.48 -14:52:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248324_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248324_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:31:24.74 -21:40:34.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
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Considering the candidate 248327_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248327_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:14:21.94 -20:29:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.744 4094031619087121920 273.59008846835 -20.48796181899 11.4652 9.9281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248329_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248329_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:15:47.57 -16:32:44.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 248330_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248330_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:35.22 -16:13:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.856 4102878564580768896 278.14757146476 -16.21699764029 13.0833 12.5774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248333_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248333_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:48:52.72 -13:46:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.429 4102176728162520576 282.21946096893 -13.77706855467 12.4361 11.3877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248335_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248335_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:35:15.44 -20:25:28.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 248341_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248341_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:30:47.60 -14:56:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248346_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248346_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:26:13.58 -15:00:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248356_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248356_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:22:10.44 -21:35:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248357_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 248357_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 248359_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248359_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:44.58 -14:39:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248361_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248361_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:48:20.93 -19:12:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248362_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248362_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:29:37.42 -21:38:17.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
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Considering the candidate 248363_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248363_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:33:40.13 -20:28:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.210 4091950995146845952 278.41690976994 -20.46723028673 12.3302 11.3605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248364_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248364_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:17:09.43 -20:49:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.108 4090955834047478656 274.28985039277 -20.82522927509 12.2182 10.9914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248366_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248366_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:13:55.73 -18:58:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.207 4094755372597100032 273.48257673343 -18.96629134551 12.6063 11.5560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248369_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248369_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:17:02.40 -16:43:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248372_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248372_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 19:01:03.55 -19:22:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 3.012 4085661204520018304 285.26468848125 -19.37969667582 11.8140 10.6281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248375_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248375_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 248377_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248377_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:27:58.90 -13:55:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248381_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248381_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:13:36.58 -19:12:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248383_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248383_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:26:46.05 -15:14:12.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 248384_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248384_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:16:47.15 -16:23:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248389_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248389_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:27:34.69 -14:26:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248393_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248393_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:27:06.16 -17:20:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.310 4096711399459036160 276.77602600713 -17.34493371085 11.7021 10.8530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248397_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248397_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:18:05.90 -18:44:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248399_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248399_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:28:06.45 -16:52:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248400_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248400_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:48.15 -17:13:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248401_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248401_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:32.21 -16:23:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248407_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248407_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:12:33.89 -15:36:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 1.222 4145802875651853312 273.14153126343 -15.60289200848 11.5709 10.7316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248409_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248409_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:18:40.71 -13:46:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 0.953 4146600640059736704 274.66982508970 -13.78112599271 10.9038 10.1654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248597_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248597_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:20:03.68 -17:05:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248624_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248624_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:15:26.89 -18:40:34.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248629_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248629_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:29:42.68 -14:34:02.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248638_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248638_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:29:13.92 -14:32:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248648_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248648_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:24:54.33 -18:32:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248684_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248684_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:14:49.92 -18:48:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248690_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248690_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:50.79 -16:16:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248696_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248696_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:17:16.89 -17:20:47.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248700_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248700_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:16:36.56 -18:18:34.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)
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Considering the candidate 248726_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248726_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:15:10.48 -18:59:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248728_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248728_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:42:58.87 -19:14:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248740_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248740_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:57:40.00 -21:08:13.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 248761_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248761_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:15:08.26 -20:44:34.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248768_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248768_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:41:22.28 -14:40:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248783_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248783_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:34:01.94 -15:21:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248784_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248784_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:19.62 -14:40:08.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 248786_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248786_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:13:45.30 -21:01:35.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 248794_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248794_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:12:31.17 -18:50:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248796_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248796_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:14:36.46 -18:07:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248803_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248803_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:20:22.32 -16:10:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248812_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248812_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:23:30.18 -21:39:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248815_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248815_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:37:13.31 -19:12:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248825_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248825_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:27:28.08 -15:21:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248828_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 248828_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 248836_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248836_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:15:16.60 -19:07:29.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)
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Considering the candidate 248864_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248864_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:53:51.17 -19:46:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.820 4086045621277324928 283.46419733605 -19.78018464662 12.0909 11.6701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248903_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248903_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:33.14 -18:57:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248924_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248924_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:16.12 -16:06:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248938_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248938_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:12:33.43 -18:22:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.175 4095677102617236096 273.13865504138 -18.38284742170 13.0873 12.5356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 248948_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248948_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:24.08 -18:57:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248963_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248963_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:16:13.22 -18:48:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248965_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248965_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:25:01.48 -18:30:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248968_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248968_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:19.45 -13:44:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248977_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248977_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:17:54.65 -18:46:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248979_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248979_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:38:55.80 -15:02:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248986_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248986_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:25:12.44 -13:57:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248991_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248991_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:40:56.00 -14:53:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248995_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248995_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:24.98 -18:57:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 248996_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 248996_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:19:46.35 -17:44:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249003_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249003_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:54:36.06 -15:36:06.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249010_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249010_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:31:32.63 -14:16:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249014_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249014_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:48:16.29 -14:42:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249015_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249015_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:35:07.34 -14:13:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249016_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249016_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:29:40.27 -16:39:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249029_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249029_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:12:14.34 -17:23:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249030_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249030_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:35:27.52 -20:50:41.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249048_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249048_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:29:48.68 -14:33:44.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249051_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249051_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:11:52.06 -20:21:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249056_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249056_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:49:39.34 -19:09:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249060_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249060_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:24:09.49 -19:24:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249066_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249066_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:44.57 -17:14:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249069_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249069_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:22:36.28 -16:02:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249071_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249071_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:42:13.50 -15:50:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249085_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249085_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:18:08.17 -18:44:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249089_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249089_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:18.20 -14:39:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 249094_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249094_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:12:03.85 -13:49:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249107_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249107_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:39:38.91 -15:10:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.318 4103375883039991424 279.91099383461 -15.17805890217 11.8785 10.5357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 249109_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249109_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:26:24.40 -18:03:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249117_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249117_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:12:26.38 -15:11:27.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 249132_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249132_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:58.91 -16:18:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249133_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249133_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:50:57.94 -15:15:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249136_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249136_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:28:04.98 -16:45:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249144_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249144_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:25:53.69 -17:03:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249155_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249155_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:24:48.04 -16:47:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249164_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249164_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:27:45.13 -13:46:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249167_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249167_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:20:54.92 -14:55:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249177_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249177_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:36:54.32 -15:57:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249200_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249200_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 249212_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249212_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:35:45.57 -15:25:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249213_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249213_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:26:03.63 -14:48:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 249236_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249236_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:27:04.66 -14:30:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 249269_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 249269_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:33:19.39 -14:25:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26309_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 26309_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:14:57.70 -21:28:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217502_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 217502_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:50:57.41 -21:50:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148991_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 148991_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:29:32.23 -15:48:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171485_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 171485_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:59:51.62 -14:05:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145867_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 145867_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 40177_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 40177_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 92371_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 92371_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:32:49.84 -18:22:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110948_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 110948_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:55:57.07 -17:39:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37894_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 37894_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 92127_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 92127_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 228357_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 228357_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 18:58:31.03 -17:02:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.108 4088503854410666112 284.62964605141 -17.04191143389 12.4571 10.4861 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 217251_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 217251_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
**** FOUND 19:05:47.37 -19:40:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 5.744 4085508342358531328 286.44905275843 -19.66991710236 11.4174 10.3212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195804_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 195804_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 17492_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 17492_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 23039_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 23039_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 120901_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 120901_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 19584_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 19584_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 46759_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
Preparing report for the candidate 46759_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
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Considering the candidate 223118_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054
The candidate 223118_fd_Sgr-02-Q2b1x1_2026-04-02_04-33-45_20.00sec_-14.90C_LIGHT_0054 did not pass the final checks
