This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F
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!
TCP 2026 04 06.1258* 03 44 45.11 +33 15 17.3 11.2 U Per 9 0
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 1258,2461136.6258,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1258 20260406.1258 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1258* 04 37 54.06 +39 56 16.9 11.6 U Per 9 0
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
HL Per,2461136.6258,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
HL Per 20260406.1258 11.63CV 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!
TCP 2026 04 06.1258* 04 07 00.68 +41 17 30.1 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.6258,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1258 13.85CV 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!
TCP 2026 04 06.1258* 04 18 07.05 +36 22 28.3 13.2 U Per 9 0
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
NSVS J0418072+362229,2461136.6258,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0418072+362229 20260406.1258 13.19CV 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!
TCP 2026 04 06.1258* 04 15 00.36 +38 52 40.2 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041500.30+385239.7,2461136.6258,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041500.30+385239.7 20260406.1258 13.22CV 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!
TCP 2026 04 06.1258* 04 21 30.85 +35 35 38.6 13.3 U Per 9 0
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
CSS_J042130.8+353538,2461136.6258,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
CSS_J042130.8+353538 20260406.1258 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!
TCP 2026 04 06.1258* 04 13 38.97 +38 55 11.4 13.0 U Per 9 0
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
NSVS J0413388+385513,2461136.6258,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0413388+385513 20260406.1258 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!
TCP 2026 04 06.1258* 03 51 51.12 +43 02 46.1 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J035150.76+430249.6,2461136.6258,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J035150.76+430249.6 20260406.1258 12.97CV 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!
TCP 2026 04 06.1258* 04 43 16.26 +41 43 16.2 12.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J044316.36+414317.4,2461136.6258,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J044316.36+414317.4 20260406.1258 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1258* 03 42 33.10 +39 06 04.5 11.6 U Per 9 0
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
HU Per,2461136.6258,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
HU Per 20260406.1258 11.59CV 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!
TCP 2026 04 06.1258* 04 17 06.09 +37 22 18.2 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041706.01+372219.1,2461136.6258,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J041706.01+372219.1 20260406.1258 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1258* 03 54 35.01 +38 04 28.5 13.8 U Per 9 0
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
2MASS J03543503+3804273,2461136.6258,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
2MASS J03543503+3804273 20260406.1258 13.85CV 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!
TCP 2026 04 06.1258* 04 16 24.20 +39 25 45.5 12.3 U Per 9 0
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
NSVS J0416241+392545,2461136.6258,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0416241+392545 20260406.1258 12.26CV 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!
TCP 2026 04 06.1258* 04 21 52.33 +37 56 40.5 13.7 U Per 9 0
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
NSVS J0421526+375642,2461136.6258,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0421526+375642 20260406.1258 13.70CV 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!
TCP 2026 04 06.1258* 04 05 31.25 +38 05 12.7 12.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J040531.19+380511.8,2461136.6258,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J040531.19+380511.8 20260406.1258 12.69CV 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!
TCP 2026 04 06.1258* 04 42 28.59 +41 32 31.9 12.6 U Per 9 0
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
NSVS J0442287+413231,2461136.6258,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0442287+413231 20260406.1258 12.56CV 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: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
First image: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Last image: 2461136.62615184 06.04.2026 03:01:29.519 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 8 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): 18392
Objects passed selection criteria: 18375
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 17207
Average stars matched: 16722.5 (97.1843 %)
Memory usage VmPeak: 122372 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 23:44:10 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: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
First image: 2461083.59692772 12.02.2026 02:19:24.555 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Last image: 2461136.62615184 06.04.2026 03:01:29.519 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 102
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
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: 129 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): 133317
Objects passed selection criteria: 133066
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 115696
Average stars matched: 111627 (96.4832 %)
Memory usage VmPeak: 1961548 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 23:47:56 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
SExtractor catalog cache: saved Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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: 2461136.62538191
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits exists and is non-empty
Saving wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits exists and is non-empty
Saving wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits exists and is non-empty
Saving wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits'
wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits exists and is non-empty
Saving wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:49.625 +37:59:22.57
Angular distance between the image centers 0.0112 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 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:47.095 +38:00:02.18
Angular distance between the image centers 0.0084 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 04:21:49.625 +37:59:22.57
Second-epoch second image center 04:21:47.095 +38:00:02.18
Angular distance between the image centers 0.01379 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/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits &> /tmp/tmp.Fnwg86QboE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits &> /tmp/tmp.EEHbD0YYiH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits &> /tmp/tmp.IduutiHKKr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits &> /tmp/tmp.VindOIuYUc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
Found non-empty wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
The reference image (wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits) and catalog (wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat) found
'wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat' -> 'wcsmag.cat'
Read 18830 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9680 to 76.3320 deg, Dec +32.2038 to +43.3213 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 54.9680 to 76.3320 deg, Dec 32.2038 to 43.3213 deg
Loaded 9186 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): 6363 out of 7115 total matches.
Matched with Tycho-2 7115 out of 18830 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.972881
a=0.000000 b=1.000000 c=22.972881
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
2.0 pix Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
3.3 pix fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
3.3 pix fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Limiting magnitude estimates:
15.5 mag. Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
15.5 mag. Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
14.9 mag. fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
14.9 mag. fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.2 (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.Fnwg86QboE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> 'wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1807, passed=18830
Got 18830 stars (including 16990 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 18830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18389 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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits -region wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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.EEHbD0YYiH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> 'wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1869, passed=18776
Got 18776 stars (including 16879 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 18776 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 18312 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 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 18314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 18314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits -region wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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.IduutiHKKr (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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=966, passed=15865
Got 15865 stars (including 14887 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 15865 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 954 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: 952 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15544 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits -region wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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.VindOIuYUc (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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=965, passed=15853
Got 15853 stars (including 14874 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 15853 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 953 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: 952 matched stars entering correct_measured_positions(), 936 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: 952 matched stars entering correct_measured_positions(), 15532 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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15533 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits -region wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
Saving fully-calibrated image wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits'
Preparing the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out08101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18589.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: 1s
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Considering the candidate 21454_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21454_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:42:33.10 +39:06:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 1.545 224315322851403520 055.63821246019 +39.10099855513 11.4374 11.0252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21509_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21509_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:01:21.25 +38:50:58.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
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Considering the candidate 21514_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21514_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:52:20.46 +39:23:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21516_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21516_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:30:34.83 +38:56:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.617 179590965105796352 067.64517139589 +38.94666568595 11.7917 10.9076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21547_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21547_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:16:24.20 +39:25:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.919 227524762933447936 064.10092318827 +39.42919873036 11.3404 9.8732 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21549_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21549_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:28:50.27 +41:44:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 21557_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21557_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:47:39.81 +39:42:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.574 199821090002070528 071.91596097387 +39.71610486244 11.2357 9.9878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21560_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21560_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:25:52.22 +38:59:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21568_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21568_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:33:41.35 +37:55:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.780 178546811313696768 068.42211852083 +37.93088724099 12.2294 11.6546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21572_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21572_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:32:57.94 +40:44:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.895 179854744818138624 068.24157160714 +40.74211410542 12.0293 11.2239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21586_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21586_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:38:28.44 +40:22:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.492 203050871048071552 069.61843777107 +40.37115596168 12.0913 11.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21592_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21592_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:51:54.66 +40:46:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.660 200295524974479488 072.97791385553 +40.78258707925 12.0491 11.1547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21594_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21594_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:56:47.14 +40:30:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.563 200056587350463360 074.19661796907 +40.50024592106 11.7590 10.6214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21597_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21597_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:56:54.03 +40:05:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.788 200030306449627136 074.22515877032 +40.09944940163 12.2973 11.7517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21598_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21598_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:31:53.71 +39:39:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.014 179645837608423296 067.97385877518 +39.66402875353 12.1385 11.5381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21599_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21599_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:46:36.57 +38:52:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.707 199711826034561280 071.65262077496 +38.87845608745 11.0519 9.6405 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21602_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21602_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:42:25.71 +38:02:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.888 175562805475437184 070.60706265643 +38.04767483727 11.9319 10.9318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21603_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21603_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:20:09.50 +39:07:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.830 227467382170604928 065.03964101580 +39.12507932101 12.2318 11.6856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21605_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21605_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:51:48.03 +40:38:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21607_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21607_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:23:01.82 +36:23:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.759 176704403485628416 065.75748706025 +36.38591841762 12.3259 11.6512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21608_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21608_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:36:05.66 +40:52:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.689 203818364524771584 069.02333123761 +40.87768446741 11.8085 10.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21612_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21612_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:22:30.51 +38:37:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21622_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21622_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:31:30.42 +38:41:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.688 178821650564177792 067.87670678234 +38.68911745731 11.9987 11.1003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21629_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21629_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:25:01.03 +39:42:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.571 179555132196321536 066.25436571453 +39.71471311221 12.2302 11.6911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21630_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21630_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:25:38.41 +37:42:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.661 179058251722131328 066.41014113876 +37.70183399728 12.1961 11.5737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21633_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21633_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:40:11.14 +38:49:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.720 178659747478650880 070.04660666562 +38.82075445770 12.2509 11.6819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21649_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21649_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:34:22.46 +40:20:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.652 179784380370703616 068.59365824197 +40.34960582700 12.0274 11.1047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21654_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21654_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:31:42.33 +38:58:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.576 178840754578686848 067.92623621086 +38.98196503371 12.0158 11.0796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21664_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21664_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:26:06.86 +40:39:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.043 179991805813908736 066.52859265566 +40.65551605499 12.3922 11.9869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21671_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 21671_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:24:17.84 +36:14:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.164 176657021406429568 066.07427701783 +36.23482895751 11.8832 10.8194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06850_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 06850_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:19:09.03 +40:45:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03543_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 03543_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:00:21.11 +42:02:56.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18589_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 18589_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08101_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 08101_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08921_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 08921_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:48:28.68 +39:16:47.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:37:54.06 +39:56:16.9
03:44:45.11 +33:15:17.3
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
SExtractor catalog cache: saved Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits exists and is non-empty
wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:49.625 +37:59:22.57
Angular distance between the image centers 0.0112 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 04:21:49.659 +38:00:02.98
Second-epoch image center 04:21:47.095 +38:00:02.18
Angular distance between the image centers 0.0084 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 04:21:49.625 +37:59:22.57
Second-epoch second image center 04:21:47.095 +38:00:02.18
Angular distance between the image centers 0.01379 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/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits &> /tmp/tmp.XEFmEVGSbo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits &> /tmp/tmp.uADhC2bVf6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits &> /tmp/tmp.dPRANUKJUO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits &> /tmp/tmp.mBT5sU5GUK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
Found non-empty wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits and wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
The reference image (wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits) and catalog (wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat) found
'wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat' -> 'wcsmag.cat'
Read 145138 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 54.9680 to 76.3546 deg, Dec +32.1479 to +43.3235 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 54.9680 to 76.3546 deg, Dec 32.1479 to 43.3235 deg
Loaded 9259 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): 5279 out of 7192 total matches.
Matched with Tycho-2 7192 out of 145138 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.835078
a=0.000000 b=1.000000 c=22.835078
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 78 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
1.8 pix Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
3.1 pix fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
3.1 pix fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Limiting magnitude estimates:
15.6 mag. Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
15.6 mag. Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
15.0 mag. fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
15.0 mag. fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (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.XEFmEVGSbo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits' -> 'wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=15711, passed=145113
Got 145113 stars (including 129125 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 145113 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 938 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: 961 matched stars entering correct_measured_positions(), 141858 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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 141857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 141856 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits -region wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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.uADhC2bVf6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits' -> 'wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=15921, passed=145724
Got 145724 stars (including 129496 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 145724 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 142056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 142057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 142057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits -region wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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.dPRANUKJUO (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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=7771, passed=87433
Got 87433 stars (including 79539 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 87433 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 955 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: 953 matched stars entering correct_measured_positions(), 940 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: 953 matched stars entering correct_measured_positions(), 86289 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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 86288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 86287 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits -region wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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.mBT5sU5GUK (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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=7891, passed=88015
Got 88015 stars (including 80003 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 88015 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 955 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: 954 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 86682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 86683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 86682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits -region wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_Per-05-Q1b1x1_2026-02-11_20-19-24_20.00sec_-14.90C_LIGHT_0025.fits
Saving fully-calibrated image wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_Per-05-Q1b1x1_2026-02-11_20-20-03_20.00sec_-14.90C_LIGHT_0026.fits
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-00-22_20.00sec_-4.90C_LIGHTs_0020.fits
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.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_Per-05-Q1b1x1_220230_TTUQ1b1x1_4750_vqSiAq7F/wcs_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021.fits
Preparing the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out08066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out158061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out170617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out155690.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out03460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92682.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 168831_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168831_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:48:29.62 +35:31:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 2.434 219884737667157888 057.12289723846 +35.51722196521 13.5999 12.8038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168838_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168838_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:45:40.24 +40:15:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.478 202852645421163776 071.41801787595 +40.25010570582 14.4509 13.7548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168854_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168854_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:47:06.11 +33:44:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.780 218020069026945152 056.77655664102 +33.73287103255 13.5807 12.9747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168858_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168858_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:08:04.01 +35:23:30.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 168864_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168864_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:47:48.11 +38:46:45.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)
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Considering the candidate 168869_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168869_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:37:30.47 +41:48:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.637 204013046802471040 069.37672936661 +41.80796362148 13.8662 12.9303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168872_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168872_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:51:53.56 +36:27:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.953 220028670611942400 057.97215082064 +36.45023893884 13.6557 12.9864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168877_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168877_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:49:13.08 +42:15:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.228 203682643560740992 072.30471748854 +42.26203255723 13.5828 12.6285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168878_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168878_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:54:34.58 +34:32:05.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 168879_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168879_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:44:02.74 +42:06:05.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
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Considering the candidate 168901_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 168901_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:14:03.54 +43:01:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169171_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169171_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:35:11.70 +39:19:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169214_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169214_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:12:12.35 +39:26:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.859 226249569962168320 063.05173661736 +39.44747992668 11.0835 9.5891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169269_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169269_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:08:20.16 +43:10:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169341_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169341_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:00:09.37 +39:38:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169376_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169376_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:24:33.00 +34:09:21.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169444_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169444_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:17:52.24 +42:00:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169481_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169481_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:15:31.60 +33:49:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169515_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169515_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:13:29.50 +33:27:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169553_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169553_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:00:18.13 +39:25:03.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 169652_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169652_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:01:49.45 +41:11:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169729_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169729_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 169794_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169794_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:53:41.89 +38:47:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169797_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169797_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:13:21.20 +33:28:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169801_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169801_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:13:17.87 +33:49:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.476 169989999513495808 063.32519637357 +33.82982742853 13.2833 12.4022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169816_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169816_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:19:57.10 +41:05:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.537 227916738829266560 064.98737424698 +41.09012946092 13.4942 12.8107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169927_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169927_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:21:15.67 +41:09:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 4.615 228280814617652992 065.31439802050 +41.15446454253 13.8884 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169945_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169945_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:48:13.41 +39:57:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169957_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169957_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:00:28.11 +33:18:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.822 170505636105084288 060.11788175990 +33.31274077496 13.9085 13.1768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169964_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169964_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:35:31.49 +37:29:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.433 178463660747111552 068.88224295822 +37.49368150163 13.6119 12.6455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169986_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169986_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:58:21.65 +38:42:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 2.083 198955976211050752 074.59030802270 +38.70948225207 13.8043 13.3366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 169989_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 169989_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:23:59.65 +41:56:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.425 228327818739227136 065.99845055406 +41.94102678352 14.0373 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170050_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170050_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:04:45.88 +42:16:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170055_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170055_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:00:23.44 +41:58:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170067_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170067_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:56:36.89 +35:05:07.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170108_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 170108_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 170122_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170122_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:30:00.01 +42:56:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.950 252492885295387008 067.49904120756 +42.93454403892 14.1575 13.3288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170147_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170147_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:08:23.64 +41:28:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170169_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170169_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:39:25.04 +42:11:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 2.900 204048609131506432 069.85384131430 +42.19528154271 13.7812 12.7858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170184_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170184_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:55:59.74 +40:10:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170211_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170211_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 170219_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170219_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:43:29.29 +34:32:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170223_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170223_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:23:12.29 +35:29:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170265_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170265_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:35:22.86 +38:55:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 4.447 178883566814763136 068.84515702374 +38.92126692194 14.0146 13.2828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170278_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170278_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:54:49.63 +40:39:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170286_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170286_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 170290_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170290_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:44:51.27 +42:10:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.137 203620452432784256 071.21407176046 +42.16807609497 14.1741 13.5494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170309_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170309_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:44:57.01 +35:36:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 2.763 174286753511957760 071.23774967941 +35.60708466206 14.1117 13.3623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170390_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170390_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:00:58.46 +40:30:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170393_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170393_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:50:31.95 +41:29:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170457_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170457_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:56:01.41 +40:10:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170473_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170473_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:12:00.02 +35:20:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 5.570 176895551011541888 062.99909299158 +35.34331940930 14.1104 13.4941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 170617_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 170617_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:02:05.72 +39:55:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 2.715 200728255816946304 075.52442193028 +39.93382638853 14.4208 13.3908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58905_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 58905_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:37:54.05 +39:56:16.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 129629_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 129629_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 118886_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 118886_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:27:10.58 +35:29:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77091_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 77091_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 93060_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 93060_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:16:01.34 +37:20:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119373_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 119373_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 60877_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 60877_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:23:32.71 +40:01:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.066 227610657982197376 065.88627348198 +40.02640705102 12.4276 10.7854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103465_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 103465_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:44:45.12 +33:15:17.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 28944_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 28944_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:27:32.44 +41:47:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76697_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 76697_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 03460_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 03460_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 158061_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 158061_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:11:07.99 +40:08:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.579 227063376068008192 062.78278483879 +40.14917774138 12.0847 10.3159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08066_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 08066_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 03:58:51.49 +42:51:54.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
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Considering the candidate 26080_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 26080_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 71848_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 71848_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 48567_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 48567_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:19:09.05 +40:45:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25134_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 25134_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:00:21.14 +42:02:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92682_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 92682_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 85208_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 85208_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 69838_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 69838_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 66200_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 66200_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
**** FOUND 04:48:28.67 +39:16:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86548_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 86548_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 85442_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 85442_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 29987_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
Preparing report for the candidate 29987_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
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Considering the candidate 155690_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021
The candidate 155690_fd_Per-05-Q1b1x1_2026-04-05_22-01-29_20.00sec_-4.90C_LIGHTs_0021 did not pass the final checks
