This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.8879,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.3879 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.5987-16.6342,2461149.8879,13.28,0.05,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 J288.5987-16.6342 20260419.3879 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.8879,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.3879 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.8879,13.18,0.05,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 20260419.3879 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4088000071911756672,2461149.8879,12.98,0.05,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 4088000071911756672 20260419.3879 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.0377-14.4954,2461149.8879,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.0377-14.4954 20260419.3879 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191217-1646.1,2461149.8879,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J191217-1646.1 20260419.3879 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191954.36-173421.2,2461149.8879,12.53,0.05,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 J191954.36-173421.2 20260419.3879 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190518.96-160710.8,2461149.8879,11.53,0.05,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 J190518.96-160710.8 20260419.3879 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.8879,12.25,0.05,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 20260419.3879 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.8879,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.3879 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461149.88831221 19.04.2026 09:19:00.175 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9462
Objects passed selection criteria: 9453
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 8513
Average stars matched: 7930.5 (93.1575 %)
Memory usage VmPeak: 115876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 04:21:19 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: 2461149.88831221 19.04.2026 09:19:00.175 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 81
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.17
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 39 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): 91297
Objects passed selection criteria: 91177
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 86081
Average stars matched: 76667.8 (89.0647 %)
Memory usage VmPeak: 1878748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 04:23:13 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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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: 2461149.88756848
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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 938.1'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:22.678 -18:00:40.27 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Image size: 938.9'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:19.088 -18:00:18.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:19.088 -18:00:18.31
Angular distance between the image centers 0.0155 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
Image size: 938.9'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:21.405 -17:59:45.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:21.405 -17:59:45.13
Angular distance between the image centers 0.0161 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 19:33:19.088 -18:00:18.31
Second-epoch second image center 19:33:21.405 -17:59:45.13
Angular distance between the image centers 0.01301 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.ANTig7XCEj
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.3KExlhYGeE
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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits &> /tmp/tmp.UjQfgUjZfv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits &> /tmp/tmp.P8FFFjmV6U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.8 pix fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
2.8 pix fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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
13.8 mag. fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
13.8 mag. fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ANTig7XCEj (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3KExlhYGeE (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UjQfgUjZfv (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=518, passed=7488
Got 7488 stars (including 6966 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat
util/solve_plate_with_UCAC5 got 7488 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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7306 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 957 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_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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.P8FFFjmV6U (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=512, passed=7486
Got 7486 stars (including 6968 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat
util/solve_plate_with_UCAC5 got 7486 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...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 7327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 7328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 7328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 961 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_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out22295.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 22289_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 22289_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:16:31.60 -18:01:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22295_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 22295_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01564_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 01564_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:13:27.11 -21:33:38.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field 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 ####
19:25:47.68 -18:58:44.5
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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 938.1'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:22.678 -18:00:40.27 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits (1st new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Image size: 938.9'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:19.088 -18:00:18.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:19.088 -18:00:18.31
Angular distance between the image centers 0.0155 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits (2nd new image)
verification OK: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
Image size: 938.9'x624.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:33:21.405 -17:59:45.13 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:21.405 -17:59:45.13
Angular distance between the image centers 0.0161 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 19:33:19.088 -18:00:18.31
Second-epoch second image center 19:33:21.405 -17:59:45.13
Angular distance between the image centers 0.01301 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.b0bLBq4eV9
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.vlAzTIdxpv
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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits &> /tmp/tmp.4ZFak8yhvd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits &> /tmp/tmp.jCfauJhZ9G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 101850 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Loaded 13790 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10156 out of 11996 total matches.
Matched with Tycho-2 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 58 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.3 pix fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
2.3 pix fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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
13.9 mag. fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
13.9 mag. fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.b0bLBq4eV9 (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 98878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vlAzTIdxpv (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/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...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4ZFak8yhvd (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=17, blended=5124, passed=74798
Got 74798 stars (including 69583 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat
util/solve_plate_with_UCAC5 got 74798 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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 73044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 73045 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 72979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 957 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_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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.jCfauJhZ9G (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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=5219, passed=74838
Got 74838 stars (including 69521 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat
util/solve_plate_with_UCAC5 got 74838 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...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 73013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 73012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 73013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 962 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_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/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_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-17-55_20.00sec_-5.00C_LIGHT_0678.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.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_2026-04-19_CI_Sgr-03-Q2b1x1_041950_TTUQ2b1x1_1437764_VhUWB3Ci/wcs_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out148158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out148171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148861.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 8s
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Considering the candidate 148158_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148158_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:13:36.56 -14:10:37.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 148169_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148169_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:11:51.42 -19:24:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.281 4083982632533058048 287.96462334368 -19.41521746324 12.9530 12.2657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148171_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148171_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148172_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148172_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:06:06.41 -14:26:30.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 148179_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148179_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148194_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148194_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:35:14.14 -19:19:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.455 6869543217769190400 293.80819436198 -19.31859444086 13.4213 12.7479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148200_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148200_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:08:00.62 -16:49:57.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 148201_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148201_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148206_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148206_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:42:24.38 -16:16:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.153 4181649119382598912 295.60157090253 -16.27959653132 13.0754 12.4032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148211_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148211_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:05:52.81 -17:22:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148212_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148212_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:04:53.71 -13:53:17.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
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Considering the candidate 148223_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148223_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:12:18.89 -15:32:32.2 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 148228_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148228_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148229_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148229_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:11:02.71 -13:48:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148240_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148240_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:22:51.04 -14:52:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148249_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148249_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:46:32.26 -20:21:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148250_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148250_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148253_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148253_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:45:58.22 -21:14:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148254_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148254_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:44:36.92 -18:35:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148256_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148256_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148258_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148258_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:48:35.92 -19:56:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148266_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148266_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:44:28.96 -19:42:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148268_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148268_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148272_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148272_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:05:37.50 -14:45:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
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Considering the candidate 148275_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148275_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:08:19.48 -16:13:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148276_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148276_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:12:44.17 -14:57:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148277_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148277_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:32:44.46 -18:44:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.435 4179482913976312960 293.18516975051 -18.74162166380 12.3993 11.9031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148279_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148279_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:11:07.80 -18:10:52.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 148282_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148282_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:27:08.84 -20:50:11.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 148283_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148283_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:44:33.86 -20:38:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.316 6868191123404436352 296.14069451669 -20.64364600356 11.9213 11.2333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148285_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148285_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:17:42.29 -18:54:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148288_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148288_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148330_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148330_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:25:47.63 -18:58:44.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 148403_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148403_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:30:00.13 -20:21:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.749 6773300005754475392 292.50036481779 -20.36168145887 11.9193 11.1842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148484_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148484_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:08:52.16 -18:57:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148488_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148488_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148493_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148493_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:04:37.27 -21:46:03.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 148530_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148530_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:09:20.54 -21:00:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.911 4082114734072827008 287.33642371029 -21.00466513530 12.5405 12.0248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148542_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148542_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:26:21.64 -21:14:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148576_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148576_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:29:32.83 -21:19:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148612_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148612_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:46:25.89 -21:31:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148718_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148718_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:40:49.52 -21:42:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148728_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148728_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:09:02.16 -17:06:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148757_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148757_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:40:15.78 -21:02:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.041 6868118663016475136 295.06484531774 -21.03999987532 13.3770 12.6510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148764_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148764_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:51:27.53 -15:37:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.188 6872275332366736000 297.86451742595 -15.62469064763 13.8296 13.0461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148776_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148776_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:32:27.13 -20:28:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148852_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148852_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:42:50.80 -17:18:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.539 6870169733239488256 295.71113563426 -17.31660161896 13.8743 13.4094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148861_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
Preparing report for the candidate 148861_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
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Considering the candidate 148936_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148936_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:48:11.01 -21:09:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.307 6865103252376415488 297.04558273641 -21.16368422771 13.6071 12.8133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148963_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 148963_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:51:06.40 -18:59:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:13:27.10 -21:33:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:16:31.61 -18:01:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124612_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 124612_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:37:52.04 -14:08:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114202_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 114202_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:08:22.55 -17:11:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:26:18.46 -19:10:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:49:31.45 -17:40:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116965_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 116965_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
**** FOUND 19:12:28.67 -20:05:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07863_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679
The candidate 07863_fd_Sgr-03-Q2b1x1_2026-04-19_04-19-00_20.00sec_-4.90C_LIGHT_0679 did not pass the final checks
