This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461135.9241,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260405.4241 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.4244-17.7656,2461135.9241,12.64,0.05,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
ATO J288.4244-17.7656 20260405.4241 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4185551737133617280,2461135.9241,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4185551737133617280 20260405.4241 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.9241,12.66,0.05,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
target 20260405.4241 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
Gaia DR3 4088958266253025536,2461135.9241,12.41,0.05,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 4088958266253025536 20260405.4241 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191117.96-144837.2,2461135.9241,12.23,0.05,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 J191117.96-144837.2 20260405.4241 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
Gaia DR3 4089186410603490432,2461135.9241,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4089186410603490432 20260405.4241 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4088331785150876416,2461135.9241,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4088331785150876416 20260405.4241 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461135.9241,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260405.4241 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0923 Sgr,2461135.9241,11.66,0.05,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
V0923 Sgr 20260405.4241 11.66CV 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
Gaia DR3 4185047370525082624,2461135.9241,12.27,0.05,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 4185047370525082624 20260405.4241 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461135.92441486 05.04.2026 10:10:59.444 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.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.: -8.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 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): 9930
Objects passed selection criteria: 9923
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: 8437
Average stars matched: 7807.75 (92.5418 %)
Memory usage VmPeak: 116192 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 06:04:59 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461135.92441486 05.04.2026 10:10:59.444 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 88
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
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: 32 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): 95012
Objects passed selection criteria: 94877
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 84949.5
Average stars matched: 75334.8 (88.6818 %)
Memory usage VmPeak: 1877348 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 06:07:07 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.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: 2461135.92373721
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:33.692 -18:00:18.99
Angular distance between the image centers 0.0440 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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:36.240 -18:01:01.21
Angular distance between the image centers 0.0541 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:33.692 -18:00:18.99
Second-epoch second image center 19:33:36.240 -18:01:01.21
Angular distance between the image centers 0.01547 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.WX7RSV9t85
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.kec2Ql8qpc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits &> /tmp/tmp.upbJXd2wY0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits &> /tmp/tmp.K05QhFf305
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 11017 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 deg
Loaded 13778 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8233 out of 8546 total matches.
Matched with Tycho-2 8546 out of 11017 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784657
a=0.000000 b=1.000000 c=22.784657
From vast_summary.log: estimated ref. image limiting mag.: -8.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
3.0 pix fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
3.0 pix fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.6 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
13.7 mag. fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
13.7 mag. fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.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.WX7RSV9t85 (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_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kec2Ql8qpc (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.upbJXd2wY0 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=507, passed=6504
Got 6504 stars (including 5992 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 6504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 6260 with non-zero local correction accuracy
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 6259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 6259 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.K05QhFf305 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=481, passed=6411
Got 6411 stars (including 5924 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat
util/solve_plate_with_UCAC5 got 6411 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 6246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 6245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 6245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 960 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out22495.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22495_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 22495_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:11:04.54 -19:20:18.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:33.692 -18:00:18.99
Angular distance between the image centers 0.0440 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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:36.240 -18:01:01.21
Angular distance between the image centers 0.0541 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:33.692 -18:00:18.99
Second-epoch second image center 19:33:36.240 -18:01:01.21
Angular distance between the image centers 0.01547 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.RMMZxtOi0s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.6zoyE56MiQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits &> /tmp/tmp.jaatwrX9fj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits &> /tmp/tmp.FqLrynRy3g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 101850 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Loaded 13790 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10156 out of 11996 total matches.
Matched with Tycho-2 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 61 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Limiting magnitude estimates:
14.4 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
13.8 mag. fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
13.8 mag. fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.RMMZxtOi0s (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_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 98878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6zoyE56MiQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12676, passed=138124
Got 138124 stars (including 125221 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 138124 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jaatwrX9fj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=19, blended=4392, passed=64716
Got 64716 stars (including 60239 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 64716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 62900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 62900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 62822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 960 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FqLrynRy3g (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=4129, passed=63615
Got 63615 stars (including 59415 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat
util/solve_plate_with_UCAC5 got 63615 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 62113 with non-zero local correction accuracy
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 62112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 62111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-00_20.00sec_-5.00C_LIGHT_0233.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Sgr-03-Q2b1x1_060137_TTUQ2b1x1_16674_uSJ2ADus/wcs_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out117042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out113535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48852.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 6s
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Considering the candidate 148815_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148815_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:34:49.05 -21:01:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.042 6772277223721054208 293.70447234050 -21.03316361332 13.9876 13.4241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148816_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148816_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:52:10.30 -13:59:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 2.763 4188380123407355392 298.04224835709 -13.99696628900 13.7811 13.0699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148821_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148821_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:42:48.12 -14:47:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.891 4182460082227343616 295.70072717527 -14.79208620691 13.6729 13.1180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148823_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148823_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:56:29.32 -15:31:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.276 6872138580606920576 299.12212911050 -15.52865814625 13.8777 13.2631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148825_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148825_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:57:49.29 -13:39:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.296 6878656794773274752 299.45529053746 -13.65413703220 13.6025 12.7948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148826_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148826_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:52:55.25 -17:55:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.246 6870676882977752960 298.22989023465 -17.93064019769 13.5124 12.6976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148829_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148829_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 148833_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148833_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:22:19.83 -15:13:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.727 4184495003376742272 290.58258336772 -15.23132999890 13.0697 12.2318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148839_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148839_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:50:28.90 -20:43:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.951 6865515672317346176 297.61986790876 -20.71795158693 13.5014 13.0113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148847_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148847_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:49:00.30 -21:11:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.623 6865473856515319424 297.25087962283 -21.19251208821 14.0368 13.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148871_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148871_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:38:03.13 -13:53:03.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 148873_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148873_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:29:07.76 -14:44:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
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Considering the candidate 148875_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148875_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:17:54.37 -16:15:58.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
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Considering the candidate 148878_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148878_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:44:21.20 -19:27:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.773 6868892375605013248 296.08787563949 -19.46307044689 13.3142 12.7523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148893_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148893_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:43:05.24 -18:02:01.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 148894_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148894_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148895_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148895_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:46:32.19 -20:21:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.416 6868574273146892160 296.63400192305 -20.36461684113 12.8405 12.3795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148897_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148897_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:17:24.90 -16:27:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 148900_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148900_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:25:18.35 -18:58:08.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 148901_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148901_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:11:02.76 -13:48:06.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
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Considering the candidate 148903_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148903_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:48:35.90 -19:56:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.489 6868617875655424128 297.14918075636 -19.93499988916 12.7070 11.8833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148908_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148908_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:48:42.09 -16:10:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148910_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148910_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:45:58.21 -21:14:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.191 6865133553366087936 296.49220468817 -21.23507634331 12.7165 12.0333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148916_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148916_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:19:26.74 -18:56:58.5 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 148920_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148920_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148924_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148924_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148927_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148927_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148929_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148929_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:44:36.89 -18:35:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148938_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148938_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:08:20.24 -16:13:53.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
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Considering the candidate 148940_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148940_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:21:11.47 -14:45:17.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)
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Considering the candidate 148942_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148942_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148950_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148950_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:44:29.01 -19:42:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.267 6868850692942919680 296.12056113569 -19.70463584133 12.4101 11.5299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148953_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148953_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148958_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148958_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:55:26.17 -15:29:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.917 6872183591864253056 298.85889727937 -15.50010231354 12.1875 11.2856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148963_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148963_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:30:34.61 -14:02:08.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)
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Considering the candidate 148966_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 148966_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 148967_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 148967_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:50:01.09 -19:35:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.104 6868723669289437952 297.50452970339 -19.58585998388 10.7472 9.6679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149055_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149055_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:55:55.35 -18:51:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.084 6867375736752381440 298.98033976880 -18.86597762927 11.3502 10.5427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149056_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149056_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:11:04.59 -19:20:18.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 149175_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149175_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:57:29.01 -17:05:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.481 6871129675609228672 299.37058948206 -17.09225244266 12.2648 11.4892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149250_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149250_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:04:37.33 -21:46:00.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 149351_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149351_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:51:58.98 -20:23:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.863 6865618678515170176 297.99560248635 -20.38400125332 12.9250 12.2220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149360_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149360_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:46:25.92 -21:31:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149394_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 149394_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 149399_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149399_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:40:49.51 -21:42:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.249 6868010464199527040 295.20633450334 -21.70827871798 13.1784 12.4945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149421_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149421_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:17:36.49 -15:57:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149449_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149449_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:46:26.62 -19:44:30.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 149597_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149597_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:32:27.11 -20:28:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.960 6773117074508601088 293.11239711446 -20.47789137384 13.2848 12.5575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149601_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149601_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:46:32.90 -18:53:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149648_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149648_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:57:12.18 -13:38:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.723 6878669061199917568 299.30001516879 -13.64897183513 13.6339 13.0753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149705_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149705_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:55:15.15 -14:53:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.294 6878411088284181632 298.81275440196 -14.88483661931 14.0172 13.3102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149717_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149717_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:49:52.13 -14:34:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149718_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149718_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:51:06.40 -18:59:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.410 6870318201669479040 297.77656509522 -18.98669992325 13.7194 12.9410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149756_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149756_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:53:23.84 -19:23:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149759_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149759_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:46:18.37 -18:04:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.706 6871372702039079552 296.57697386903 -18.07144395108 13.8925 13.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149783_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 149783_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:39:38.61 -18:53:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.794 6869756832262363520 294.91070164540 -18.89754704767 13.9179 13.1801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113268_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 113268_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
**** FOUND 19:58:31.17 -14:44:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113369_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 113369_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 113535_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
Preparing report for the candidate 113535_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
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Considering the candidate 117042_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234
The candidate 117042_fd_Sgr-03-Q2b1x1_2026-04-05_05-10-59_20.00sec_-4.90C_LIGHT_0234 did not pass the final checks
