This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J081925-2925.1,2461136.5962,11.28,0.05,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
ASAS J081925-2925.1 20260406.0962 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5644588308386259456,2461136.5962,13.62,0.05,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 5644588308386259456 20260406.0962 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J126.2477-26.0772,2461136.5962,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J126.2477-26.0772 20260406.0962 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5693433700135766528,2461136.5962,13.17,0.05,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 5693433700135766528 20260406.0962 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5696376405562711808,2461136.5962,12.99,0.05,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 5696376405562711808 20260406.0962 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5696854207783253120,2461136.5962,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5696854207783253120 20260406.0962 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5697798898733278208,2461136.5962,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5697798898733278208 20260406.0962 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J123.8526-24.7767,2461136.5962,12.71,0.05,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 J123.8526-24.7767 20260406.0962 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J124.2951-27.9157,2461136.5962,12.83,0.05,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 J124.2951-27.9157 20260406.0962 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IX Pup,2461136.5962,12.62,0.05,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
IX Pup 20260406.0962 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J123.1580-25.3314,2461136.5962,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.1580-25.3314 20260406.0962 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.5962,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.0962 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J125.3095-24.1927,2461136.5962,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J125.3095-24.1927 20260406.0962 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.0962 2461136.5962 12.13 08:15:16.70 -28:12:50.7
247.38185 3.72482 galactic Pup Second-epoch detections are separated by 8.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 5692999216936375680 | 08:15:15.35 -28:13:26.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A9V 1982MSS...C03....0H HD 69278
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 5692999216936375680,2461136.5962,12.13,0.05,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
Large-amplitude variable Gaia DR2 5692999216936375680 20260406.0962 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5700212223674452992,2461136.5962,11.76,0.05,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 5700212223674452992 20260406.0962 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5694498577146663808,2461136.5962,11.85,0.05,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 5694498577146663808 20260406.0962 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5696590947769954048,2461136.5962,11.87,0.05,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 5696590947769954048 20260406.0962 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 3939,2461136.5962,12.29,0.05,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
NSV 3939 20260406.0962 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IX Pup,2461136.5962,12.45,0.05,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
IX Pup 20260406.0962 12.45CV 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: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
First image: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Last image: 2461136.59646833 06.04.2026 02:18:44.864 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17592
Objects passed selection criteria: 17541
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 14175.5
Average stars matched: 13202.8 (93.1378 %)
Memory usage VmPeak: 121364 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 21:20:49 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: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
First image: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Last image: 2461136.59646833 06.04.2026 02:18:44.864 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 245
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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: 59 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): 131964
Objects passed selection criteria: 131687
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 109627
Average stars matched: 100782 (91.9319 %)
Memory usage VmPeak: 2083816 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 21:22:53 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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat to cache
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.59591929
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits exists and is non-empty
Saving wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits to local_wcs_cache/
'wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits'
wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits exists and is non-empty
Saving wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits to local_wcs_cache/
'wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits' -> 'local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:30.645 -25:59:58.27
Angular distance between the image centers 0.0243 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:28.642 -25:59:49.64
Angular distance between the image centers 0.0175 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 08:38:30.645 -25:59:58.27
Second-epoch second image center 08:38:28.642 -25:59:49.64
Angular distance between the image centers 0.00788 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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits &> /tmp/tmp.B9rR5OibSZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits &> /tmp/tmp.fcqjKnc4wJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits &> /tmp/tmp.y9WHWSRNiW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits &> /tmp/tmp.tr9HhkavXb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
The reference image (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits) and catalog (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat) found
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat' -> 'wcsmag.cat'
Read 20994 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6669 to 138.8549 deg, Dec -31.3522 to -20.3052 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 120.6669 to 138.8549 deg, Dec -31.3522 to -20.3052 deg
Loaded 21131 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): 13845 out of 14623 total matches.
Matched with Tycho-2 14623 out of 20994 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.840297
a=0.000000 b=1.000000 c=22.840297
From vast_summary.log: estimated ref. image limiting mag.: -8.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
2.4 pix Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
3.1 pix fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
3.1 pix fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Limiting magnitude estimates:
14.6 mag. Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
14.6 mag. Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
14.1 mag. fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
14.1 mag. fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (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.B9rR5OibSZ (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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1631, passed=20994
Got 20994 stars (including 19342 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
util/solve_plate_with_UCAC5 got 20994 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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.fcqjKnc4wJ (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/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1680, passed=20656
Got 20656 stars (including 18951 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
util/solve_plate_with_UCAC5 got 20656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 19523 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 19518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 19518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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.y9WHWSRNiW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1141, passed=14017
Got 14017 stars (including 12865 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 14017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13549 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.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.tr9HhkavXb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=8, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1191, passed=13991
Got 13991 stars (including 12791 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 13991 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 13500 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 13498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 13498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 934 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
Saving fully-calibrated image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits'
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits'
Preparing the HTML report for the field Pyx-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out33389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out30927.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 0s
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Considering the candidate 30927_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 30927_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 32356_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 32356_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:42.80 -25:14:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33000_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 33000_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:04.02 -28:21:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33389_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 33389_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:31.07 -30:06:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 1.711 5644495498428811392 124.12895473712 -30.10011538265 11.5751 11.1143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13946_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 13946_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:45:30.64 -28:12:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05977_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 05977_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:26.03 -24:21:25.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Pyx-01-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 ####
08:19:24.39 -29:24:57.7
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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat to cache
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Creating symlink local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
Creating symlink local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits exists and is non-empty
wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits exists and is non-empty
wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits exists and is non-empty
wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:30.645 -25:59:58.27
Angular distance between the image centers 0.0243 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:28.642 -25:59:49.64
Angular distance between the image centers 0.0175 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 08:38:30.645 -25:59:58.27
Second-epoch second image center 08:38:28.642 -25:59:49.64
Angular distance between the image centers 0.00788 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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits &> /tmp/tmp.MNgl7PzDaQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits &> /tmp/tmp.55XBP4PrHk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits &> /tmp/tmp.SgXWjlQKtE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits &> /tmp/tmp.Yq5M01dn1l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
The reference image (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits) and catalog (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat) found
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat' -> 'wcsmag.cat'
Read 149517 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6583 to 138.9412 deg, Dec -31.3581 to -20.2738 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 120.6583 to 138.9412 deg, Dec -31.3581 to -20.2738 deg
Loaded 21265 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): 13597 out of 17470 total matches.
Matched with Tycho-2 17470 out of 149517 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.675683
a=0.000000 b=1.000000 c=22.675683
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.73
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.73
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 152 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
2.3 pix Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
2.5 pix fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
2.5 pix fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Limiting magnitude estimates:
14.7 mag. Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
14.8 mag. Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
14.2 mag. fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
14.2 mag. fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.MNgl7PzDaQ (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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=17301, passed=149496
Got 149496 stars (including 131962 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
util/solve_plate_with_UCAC5 got 149496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 145847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 145847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 145849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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.55XBP4PrHk (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/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=18384, passed=157885
Got 157885 stars (including 139292 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
util/solve_plate_with_UCAC5 got 157885 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 151938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 151939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 151937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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.SgXWjlQKtE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=12468, passed=106257
Got 106257 stars (including 93660 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 106257 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 103795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 103793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 103791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.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.Yq5M01dn1l (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=12858, passed=108006
Got 108006 stars (including 95017 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 108006 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 105414 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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 105416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 105416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Saving fully-calibrated image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-17-57_20.00sec_-4.90C_LIGHT_0014.fits
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Pyx-01-Q2b1x1_211926_TTUQ2b1x1_11707_mSymz8RR/wcs_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015.fits
Preparing the HTML report for the field Pyx-01-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__out174491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out178694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out180117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out135858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40269.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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: 11s
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Considering the candidate 174491_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174491_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:25.02 -29:17:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.072 5645367965209466240 129.35428505244 -29.28587040305 13.5865 13.0534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174496_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174496_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:49:53.30 -29:53:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.927 5641701197007901440 132.47181427126 -29.89669662878 14.2491 13.5398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174507_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174507_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:40.20 -28:52:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.174 5645055429030087040 125.41754419032 -28.87419583128 13.7271 13.2695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174508_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174508_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:58:11.17 -27:49:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.515 5648037682514099584 134.54670244221 -27.81698881299 14.1653 13.6883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174515_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174515_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:05.45 -22:37:57.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 174516_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174516_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:24.59 -28:58:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.501 5645379888038313600 129.60233510237 -28.98026385063 13.8762 13.4602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174529_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174529_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:28.26 -22:57:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 174535_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174535_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:43.11 -29:40:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.282 5643842392826973952 128.42953173406 -29.66731976963 13.8144 13.1474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174551_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174551_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:02.80 -30:06:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174556_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174556_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:59.79 -29:57:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.708 5642260092513201536 129.49902164069 -29.95350628763 13.8152 13.0857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174567_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174567_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:43.91 -29:15:31.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 174572_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174572_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174575_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174575_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:54.04 -28:59:07.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 174582_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174582_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:10:56.99 -28:54:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174592_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174592_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:33.62 -29:34:41.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 174594_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174594_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:40.01 -21:59:36.3 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 174596_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174596_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174598_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174598_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:28.92 -29:50:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.240 5643998381734543616 128.12087810304 -29.84324405204 13.3751 12.6433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174599_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174599_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:11:14.71 -29:06:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.623 5596773296478107648 122.81148981478 -29.10197233765 13.4786 13.1095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174601_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174601_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:01.45 -28:20:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174603_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174603_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:30:46.88 -29:17:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.647 5644080780690718464 127.69483824358 -29.28671019416 13.5524 12.9969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174611_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174611_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 174612_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174612_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:42:03.03 -29:15:42.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 174617_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174617_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:29.97 -29:53:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.115 5642267136259433088 129.62516054312 -29.89063040963 13.6096 12.8759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174619_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174619_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:20:35.75 -22:41:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 174621_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174621_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:31.80 -28:48:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.652 5645575051352053376 128.63213149281 -28.81453515962 14.4420 13.9433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174627_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174627_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:20.10 -29:00:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.688 5644813227235770624 126.58397265181 -29.00270442800 13.5578 13.0753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174631_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174631_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:43.85 -28:53:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.167 5644821542292340992 126.68312432291 -28.89313179742 13.3989 12.9391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174636_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174636_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:12:29.47 -28:19:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174638_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174638_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:03.76 -29:30:21.1 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 174645_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174645_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:54:52.13 -27:30:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.221 5648762363756572288 133.71722398463 -27.51474571936 13.8494 13.2957 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174647_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174647_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:13.16 -29:01:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.979 5692704071088408960 124.55505898695 -29.01959080484 13.2614 12.8058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174659_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174659_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:20.77 -30:01:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.350 5644367100393926656 125.33614487890 -30.01709484694 13.4183 12.6729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174661_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174661_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:07.05 -29:04:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174662_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174662_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:34:42.58 -29:11:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.678 5645545467617644800 128.67751392112 -29.18920531253 13.7552 13.2466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174665_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174665_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:36.93 -24:20:24.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 174670_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174670_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:28.31 -30:04:54.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 174671_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174671_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:15:28.69 -27:50:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174672_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174672_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174677_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174677_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:11:33.64 -29:58:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.530 5596512128106880768 122.88968690756 -29.96988350018 13.1100 12.3540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174683_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174683_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:16.21 -21:48:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174685_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174685_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:17.78 -30:08:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174686_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174686_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:16.06 -30:03:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.481 5643944991006041856 126.81723976899 -30.06328166394 13.1773 12.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174690_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174690_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:49:49.00 -27:00:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.402 5652028566126159488 132.45408368302 -27.00700041457 13.4604 12.9620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174694_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174694_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:26.02 -29:03:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174697_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174697_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:35.92 -30:10:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.680 5644491585727120512 124.14933743804 -30.17445323553 13.1418 12.3587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174701_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174701_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174707_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174707_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:46:37.46 -24:04:41.6 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 174709_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174709_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:16.28 -29:45:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.061 5644706231008123264 126.56792824154 -29.76491145162 12.9865 12.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174715_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174715_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:29.94 -29:53:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.404 5641663332575664128 133.12531889828 -29.89327906548 13.3466 12.6334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174723_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174723_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:29:26.86 -29:47:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.507 5643964266820040960 127.36187418836 -29.79458364634 13.3264 12.9017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174729_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174729_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:08.75 -26:30:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.410 5694291044328525184 124.28633483540 -26.50772604626 12.8989 12.1979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174731_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174731_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:05.46 -29:55:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174742_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174742_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174744_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174744_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 174749_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174749_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:39.55 -29:30:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174751_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174751_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174760_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174760_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:06.19 -26:29:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.369 5647012284847036032 129.52589820426 -26.48881513091 12.6445 11.9064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174762_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174762_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174774_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174774_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:23.32 -29:59:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.372 5644475642807265152 124.59728244216 -29.99284001903 12.9215 12.7549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174778_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174778_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:12:03.31 -29:43:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174780_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174780_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:42.38 -28:42:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 5.564 5692724996168718976 124.42788818140 -28.71040004396 13.7016 12.8803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174786_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174786_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174793_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174793_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174794_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174794_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:12:35.49 -29:03:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.544 5692841647483725568 123.14827300406 -29.05899923862 12.7011 12.3287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174795_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174795_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:14:07.59 -28:40:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174796_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174796_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174798_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174798_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:15.63 -24:20:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 3.921 5696360565723516288 125.31624471075 -24.34977083638 12.4392 11.7061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174801_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174801_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:32:42.54 -24:40:13.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)
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Considering the candidate 174806_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174806_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:07.23 -28:07:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174808_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174808_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:55.50 -29:55:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174809_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174809_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:18.63 -24:55:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174812_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174812_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174817_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174817_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:11:09.25 -27:51:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174819_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174819_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:30.90 -29:47:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174821_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174821_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:15:15.66 -29:05:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174823_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174823_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:58.51 -29:55:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 0.233 5644523913932421504 124.49376647381 -29.92266127094 12.4947 12.1445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174824_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174824_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:35:57.25 -24:05:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.724 5701634441960740224 128.98855791943 -24.09658995508 12.2391 11.7609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174827_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174827_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:05.92 -26:19:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.752 5694355537559875584 124.02519977673 -26.32704678958 11.8450 10.7952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174828_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174828_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:50.28 -29:10:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.565 5644646234601412608 124.96094628201 -29.17269168401 12.7503 11.7140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174832_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174832_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:11.68 -27:38:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174834_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174834_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:40.27 -24:23:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.804 5696192782819722880 125.66894823565 -24.38502634958 12.0782 11.4364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174836_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174836_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174837_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174837_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:36:48.92 -29:15:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.918 5645348345797775360 129.20358346451 -29.25036791337 12.5640 11.8062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174838_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174838_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:06.57 -26:12:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.183 5694404225302708608 124.27771560216 -26.20800989233 12.0778 11.4143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174840_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174840_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:11.01 -28:31:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 2.178 5692789004055900160 124.04651761493 -28.52517185859 12.2574 11.7296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174849_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174849_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:54:24.43 -29:49:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174851_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174851_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174853_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174853_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:49.12 -26:44:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)
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Considering the candidate 174854_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174854_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174855_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174855_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174857_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 174857_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 174860_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174860_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:57:47.77 -29:04:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.310 5647805337666336128 134.44894908891 -29.07688706091 11.8551 11.6038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174861_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174861_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:55.54 -25:39:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.858 5694683088937248128 123.48229266067 -25.66452908982 10.9373 10.0635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174862_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174862_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:23.28 -29:24:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174863_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 174863_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:43.93 -30:15:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178694_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 178694_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:51:36.35 -28:49:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.084 5642616604854609664 132.90146847828 -28.83033953157 12.4459 11.9236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179327_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 179327_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:44:45.53 -28:48:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.628 5642802564062760960 131.18932196022 -28.81581124489 12.2398 11.5884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180117_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 180117_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:54.79 -28:45:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 2.796 5692765059625701632 124.22911704652 -28.75652326387 11.9241 11.1413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180121_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 180121_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:45:55.36 -27:09:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180511_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 180511_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:22:36.18 -29:42:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180845_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 180845_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:02.99 -29:33:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181193_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 181193_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:53:50.71 -29:33:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.279 5641768847028960000 133.46093681549 -29.55784271063 12.5489 11.6823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181387_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 181387_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:14:05.71 -28:33:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.616 5692883149743291648 123.52430283855 -28.56238125383 12.3841 11.6640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182151_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 182151_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:26:59.59 -29:04:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182689_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 182689_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:59:35.37 -24:13:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183569_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 183569_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:36.69 -29:56:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.405 5641660068400523392 133.15303985195 -29.93589086069 13.3460 12.6349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183797_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 183797_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:40.88 -29:56:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183880_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 183880_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:53:18.96 -29:42:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.325 5641765793313565440 133.32868615485 -29.70952518332 13.2643 12.8447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185008_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 185008_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:19:39.78 -22:15:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 5.459 5699999433816295680 124.91737543670 -22.26580166195 13.3661 13.2077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185129_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 185129_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:51:39.87 -29:52:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.216 5641710302339384448 132.91617611864 -29.88021928621 13.5947 13.2090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185612_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 185612_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:06:00.75 -27:06:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.391 5648502187518874880 136.50270336510 -27.11317477204 13.6777 13.1792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185698_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 185698_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:16:10.32 -29:58:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.051 5644509658949097344 124.04375936928 -29.96902128732 13.0744 12.7685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185738_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 185738_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:27:01.50 -29:35:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186096_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 186096_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:53.45 -22:58:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186515_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 186515_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:46:04.55 -29:46:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188200_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 188200_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:58:29.28 -27:29:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188796_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 188796_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:13:31.56 -29:44:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.837 5596495738510536704 123.38190199477 -29.73559993199 13.8393 13.3351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189149_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 189149_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:43:19.10 -29:56:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189214_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 189214_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:23:58.82 -29:48:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.676 5644385723372940416 125.99567572720 -29.80418536197 13.3002 12.8332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189424_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 189424_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:21:34.02 -29:33:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.242 5644574633210296064 125.39289469521 -29.56000892607 13.9122 13.6069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189803_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 189803_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:17:11.87 -28:45:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.940 5692770076147480576 124.29972130734 -28.75240053379 13.7141 13.3078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189901_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 189901_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:15:46.57 -28:43:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.496 5692779456355942528 123.94445073978 -28.72806810923 12.9491 11.7299 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190207_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190207_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:49:10.43 -29:55:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.695 5641698894905494272 132.29324553373 -29.92188712742 14.0088 13.2700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190250_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190250_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:30.12 -29:13:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.594 5641839013916937472 133.12499936225 -29.22476570241 14.0354 13.6164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190473_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190473_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:57:35.13 -29:25:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 0.567 5641598461390008192 134.39627121028 -29.42909318961 14.0792 13.3406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190499_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190499_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:00:31.84 -26:36:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.790 5649260923558817792 135.13320798843 -26.60564475194 14.2399 13.5123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190653_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190653_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:51:44.01 -28:25:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.935 5642700824875815040 132.93362315518 -28.41741494920 14.0007 13.4111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190742_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190742_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:57:33.40 -29:17:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.683 5647607979626044416 134.38950350922 -29.29391933571 14.4529 13.9375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190830_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190830_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:47:44.87 -27:55:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.637 5642954949498906880 131.93665909165 -27.92324124637 14.1924 13.5770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190890_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190890_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:51:29.75 -28:19:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 0.278 5642702405423770368 132.87388663486 -28.31778887596 14.3101 13.7755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190900_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190900_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:55:32.60 -28:02:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.222 5648683027121483648 133.88548188416 -28.03775108731 14.2036 13.5762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190926_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190926_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:55:36.50 -29:18:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.260 5641799637656274816 133.90212457639 -29.30722940213 13.9961 13.3855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190935_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190935_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:03:01.76 -27:24:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.455 5648388942120694400 135.75687808944 -27.40333088984 13.8639 13.3289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190960_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190960_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:53:26.59 -29:06:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.746 5641844477115157504 133.36069536752 -29.10363375393 14.3730 13.6454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190975_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190975_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:49:22.64 -30:09:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.889 5641315680743044224 132.34410149267 -30.15868892766 14.3218 13.8150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190985_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190985_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:50:23.93 -29:06:46.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
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Considering the candidate 190990_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 190990_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:55:46.66 -28:55:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.659 5647866193060902784 133.94485944820 -28.92550067457 14.4506 13.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191093_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 191093_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:44:19.57 -29:24:38.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
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Considering the candidate 191124_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 191124_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:49:38.49 -29:18:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.312 5642503874856059520 132.41038838009 -29.30953021131 14.1696 13.7224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191210_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 191210_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 09:02:01.23 -24:00:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.835 5654315241071198848 135.50559135934 -24.01375196679 14.3135 13.4863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191295_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 191295_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:38:47.83 -29:37:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.480 5645274128761344256 129.69901414323 -29.62930600681 13.8897 13.3787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120332_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 120332_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:33:02.83 -29:51:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34846_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 34846_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:25:42.92 -23:37:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11914_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 11914_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:31:01.17 -21:47:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136310_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 136310_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:37:18.43 -28:30:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135858_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 135858_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 165464_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 165464_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:52:41.16 -29:42:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40269_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
Preparing report for the candidate 40269_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
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Considering the candidate 45596_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 45596_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:24:26.02 -24:21:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138665_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 138665_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
**** FOUND 08:18:03.99 -28:21:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61781_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015
The candidate 61781_fd_Pyx-01-Q2b1x1_2026-04-05_21-18-44_20.00sec_-4.90C_LIGHT_0015 did not pass the final checks
