This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.2527+20.8388,2461143.8119,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.2527+20.8388 20260413.3119 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.8119,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.3119 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192339.54+255612.9,2461143.8119,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192339.54+255612.9 20260413.3119 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190407.39+204622.1,2461143.8119,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190407.39+204622.1 20260413.3119 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.6045+24.7767,2461143.8119,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.6045+24.7767 20260413.3119 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.8119,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.3119 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193744.80+253816.1,2461143.8119,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193744.80+253816.1 20260413.3119 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.8119,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.3119 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.5784+19.9292,2461143.8119,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.5784+19.9292 20260413.3119 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193632.62+234245.3,2461143.8119,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193632.62+234245.3 20260413.3119 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194034.62+235812.9,2461143.8119,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194034.62+235812.9 20260413.3119 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2021629904956216192,2461143.8119,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2021629904956216192 20260413.3119 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1908291+243347,2461143.8119,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1908291+243347 20260413.3119 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1914126+233323,2461143.8119,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1914126+233323 20260413.3119 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194146.39+192818.8,2461143.8119,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194146.39+192818.8 20260413.3119 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.3599+25.8629,2461143.8119,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.3599+25.8629 20260413.3119 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.3119* 18 55 15.73 +19 09 25.4 13.1 U Her 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J283.8121+19.1569,2461143.8119,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.8121+19.1569 20260413.3119 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193918.50+205242.9,2461143.8119,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193918.50+205242.9 20260413.3119 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191833.44+255913.1,2461143.8119,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191833.44+255913.1 20260413.3119 12.37CV 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: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461143.81221618 13.04.2026 07:29:25.478 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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: 4 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): 15485
Objects passed selection criteria: 15448
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 13023.2
Average stars matched: 12735.8 (97.7924 %)
Memory usage VmPeak: 122512 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 02:35:19 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461143.81221618 13.04.2026 07:29:25.478 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 243
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 60 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): 160356
Objects passed selection criteria: 159996
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 126623
Average stars matched: 120974 (95.5383 %)
Memory usage VmPeak: 2008932 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 02:39:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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: 2461143.81155038
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits'
wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:05.020 +22:03:07.46
Angular distance between the image centers 0.0556 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:07.995 +22:03:30.41
Angular distance between the image centers 0.0626 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:23:05.020 +22:03:07.46
Second-epoch second image center 19:23:07.995 +22:03:30.41
Angular distance between the image centers 0.01314 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.FFywEQz2Gp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.DmFqXhGGU7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits &> /tmp/tmp.ls69CtUX2p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits &> /tmp/tmp.Xrf82Vc9bu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 24236 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.8547 to 299.3973 deg, Dec +16.3386 to +27.3318 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 281.8547 to 299.3973 deg, Dec 16.3386 to 27.3318 deg
Loaded 19386 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): 13292 out of 14431 total matches.
Matched with Tycho-2 14431 out of 24236 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881026
a=0.000000 b=1.000000 c=22.881026
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
2.9 pix fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
3.0 pix fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Limiting magnitude estimates:
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
13.9 mag. fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
13.8 mag. fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FFywEQz2Gp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2379, passed=24232
Got 24232 stars (including 21810 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 24232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 531 to 588 (Dec 16.3 to 27.3)
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...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23277 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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.DmFqXhGGU7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2427, passed=23940
Got 23940 stars (including 21482 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 23940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 22698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 22701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 22701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.ls69CtUX2p (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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=688, passed=12334
Got 12334 stars (including 11638 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat
util/solve_plate_with_UCAC5 got 12334 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
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...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 12195 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 12196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 12196 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.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.Xrf82Vc9bu (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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=597, passed=11833
Got 11833 stars (including 11225 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat
util/solve_plate_with_UCAC5 got 11833 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
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...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 11720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 11719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 11719 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31123_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 31123_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:05:00.98 +18:02:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21588_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 21588_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:02:34.22 +25:50:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12393_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 12393_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:35:41.28 +22:20:04.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04605_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 04605_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:59:04.74 +18:18:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03107_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 03107_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:33:23.97 +18:01:02.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:05.020 +22:03:07.46
Angular distance between the image centers 0.0556 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:07.995 +22:03:30.41
Angular distance between the image centers 0.0626 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:23:05.020 +22:03:07.46
Second-epoch second image center 19:23:07.995 +22:03:30.41
Angular distance between the image centers 0.01314 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/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.FR6NlG3ElK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.YTzC9Rjqo2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits &> /tmp/tmp.lsVcxU9MZF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits &> /tmp/tmp.cyOky1AdTp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 221580 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.8126 to 299.4110 deg, Dec +16.3329 to +27.3345 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 281.8126 to 299.4110 deg, Dec 16.3329 to 27.3345 deg
Loaded 19480 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): 11172 out of 15518 total matches.
Matched with Tycho-2 15518 out of 221580 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709941
a=0.000000 b=1.000000 c=22.709941
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 155 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
1.9 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
2.7 pix fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
2.7 pix fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Limiting magnitude estimates:
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.1 mag. fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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.FR6NlG3ElK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=30047, passed=221539
Got 221539 stars (including 191094 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 221539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 209246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 209246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 209247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.YTzC9Rjqo2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=30936, passed=228140
Got 228140 stars (including 196813 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 228140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 219012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 219015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 219013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.lsVcxU9MZF (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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=8194, passed=90448
Got 90448 stars (including 82151 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat
util/solve_plate_with_UCAC5 got 90448 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 89445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 89445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 89445 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 949 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.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.cyOky1AdTp (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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=7545, passed=87369
Got 87369 stars (including 79708 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat
util/solve_plate_with_UCAC5 got 87369 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 86335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 86335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 86337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-28-27_20.00sec_-5.00C_LIGHT_0470.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.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_2026-04-13_CI_Vul-01-Q2b1x1_023020_TTUQ2b1x1_21034_kc9XyUOr/wcs_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out233410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out139423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out180704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out181548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out233685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86936.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 26s
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: 9s
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Considering the candidate 253207_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253207_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:18:49.88 +25:22:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253213_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253213_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:26:52.50 +25:21:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 253214_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253214_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:24:50.41 +25:30:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.571 2023211041378177792 291.20986461715 +25.50119615135 13.3441 12.4513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253221_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 253221_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253224_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253224_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:32:56.67 +26:19:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253225_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253225_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:04:26.34 +24:41:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.109 4533683644210471296 286.10981085055 +24.68988879495 13.3977 12.5390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253230_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253230_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:30:34.10 +22:58:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.714 2019420818635376512 292.64036712726 +22.97137235979 13.0311 12.0558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253233_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253233_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:38:43.41 +19:54:13.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 253240_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 253240_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 253241_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253241_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:34:57.55 +18:46:51.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)
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Considering the candidate 253246_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253246_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:39:14.42 +26:13:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.840 2021950897982019712 294.81044354371 +26.21815543342 12.8940 12.4007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253251_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253251_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:36:51.10 +24:26:19.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 253253_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253253_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:28:12.76 +25:59:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253269_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253269_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:15:55.39 +22:59:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253275_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253275_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:34:58.75 +20:15:04.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 253277_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253277_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:53:10.19 +25:40:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253295_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253295_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:28:53.47 +24:38:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253391_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253391_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:04:45.18 +23:18:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253396_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253396_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:07:57.60 +21:42:40.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253397_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253397_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:04:53.26 +23:19:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253408_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253408_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:54:38.13 +22:40:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253409_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253409_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:21:03.11 +20:02:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253434_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253434_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:59:26.77 +24:47:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253449_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253449_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:01:01.28 +19:17:48.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253534_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253534_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:25:27.09 +20:15:12.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253540_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253540_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:07:57.04 +19:52:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253546_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253546_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:09:08.67 +25:19:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253562_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253562_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:36:25.42 +23:56:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253574_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253574_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:03:21.21 +23:38:46.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253585_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253585_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:00:37.99 +18:27:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253590_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253590_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:54:29.02 +20:20:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253594_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253594_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:04:34.54 +22:06:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253595_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253595_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:08:11.70 +25:22:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253602_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253602_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:08:46.18 +24:10:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253615_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253615_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:10:46.70 +19:57:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253620_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253620_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:09:50.57 +26:00:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253623_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253623_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:02.10 +24:52:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253624_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253624_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:25:28.79 +24:56:30.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253636_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253636_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:59:32.41 +19:28:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253645_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253645_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:01:19.70 +20:51:09.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253666_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253666_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:17:43.84 +25:49:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253670_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253670_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:06:20.21 +20:40:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253675_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253675_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:58:34.53 +22:23:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253679_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253679_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:06:20.14 +21:22:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253704_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253704_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:16:13.49 +21:21:51.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253714_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253714_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:24:20.70 +20:00:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253717_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253717_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:23:52.25 +20:15:22.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253724_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253724_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:18:13.58 +24:26:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253729_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253729_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:01:57.36 +19:09:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253734_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253734_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:17.69 +18:24:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253741_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253741_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:27:20.70 +20:41:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253768_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253768_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:37:50.05 +22:48:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253775_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253775_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:33:23.50 +21:49:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253778_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253778_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:36:27.93 +21:59:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253779_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253779_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:04:27.58 +24:21:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253781_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253781_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:20:56.44 +23:03:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253792_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253792_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:27.76 +21:04:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253823_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253823_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:58:21.19 +20:47:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.288 4519026192143350272 284.58779896401 +20.79927117797 14.0952 12.4239 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253824_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253824_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:06:26.03 +22:42:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253853_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253853_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:38:06.93 +23:23:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253892_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 253892_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:02:22.81 +19:56:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.335 4518125039285887616 285.59406778779 +19.94894786666 13.5864 11.4276 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 180704_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 180704_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 32774_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 32774_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:56:51.20 +18:01:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130977_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 130977_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:04:19.57 +23:01:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233410_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 233410_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:04.93 +19:29:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.615 1825271735458911488 295.27173292879 +19.49799303129 12.8538 12.2358 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 86936_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 86936_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 35095_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 35095_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:33:08.00 +18:29:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234093_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 234093_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:54:32.02 +19:01:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61578_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 61578_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:11:17.95 +19:35:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55774_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 55774_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:37:20.94 +19:28:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94148_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 94148_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:38:24.26 +21:23:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243705_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 243705_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:36:08.33 +25:45:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147350_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 147350_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:35:17.95 +24:03:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174877_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 174877_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:37:40.09 +26:14:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56514_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 56514_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:48.79 +19:31:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163016_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 163016_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 31149_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 31149_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:13:30.36 +18:09:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251576_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 251576_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:19:47.33 +22:48:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154477_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 154477_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:30:08.08 +24:22:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136123_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 136123_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:10:13.64 +23:20:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234358_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 234358_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:39:11.45 +18:04:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 177832_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:02:34.28 +25:50:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64217_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 64217_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 65361_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 65361_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:17:44.14 +19:50:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234168_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 234168_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:20:33.39 +17:45:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234131_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 234131_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:56:54.01 +18:32:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)
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Considering the candidate 136507_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 136507_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:25:54.43 +23:30:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188685_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 188685_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 52335_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:27:53.64 +19:17:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234025_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 234025_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 155543_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 155543_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:38:42.13 +24:24:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108556_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 108556_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:42.50 +22:10:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175957_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 175957_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:32:35.69 +26:12:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64786_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 64786_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 233946_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 233946_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:55:10.83 +18:05:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233919_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 233919_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:22:54.92 +24:37:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233752_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 233752_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:20:12.67 +26:01:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233685_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 233685_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 145550_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 145550_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 233540_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 233540_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:41.62 +25:25:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50626_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 50626_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:22:35.21 +19:10:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170393_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 170393_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:19:04.25 +25:00:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45827_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 45827_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:53.56 +19:01:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109418_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 109418_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:14:57.14 +22:04:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143051_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 143051_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:32:37.19 +23:50:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200199_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 200199_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 110128_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:58:11.52 +21:52:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 30752_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:05:01.00 +18:02:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148949_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 148949_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:30.64 +24:07:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112797_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 112797_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:35:41.25 +22:20:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151575_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 151575_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:21:47.53 +24:11:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130649_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 130649_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:35:49.91 +23:16:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33243_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 33243_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:48.32 +18:25:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163035_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 163035_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 32268_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 32268_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:57:40.11 +18:01:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43562_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 43562_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:30.51 +18:55:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82826_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 82826_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:12.31 +20:45:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96543_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 96543_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:24:47.97 +21:28:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69848_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 69848_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:57:26.87 +19:48:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139423_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 139423_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 191767_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 191767_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:31:24.54 +25:28:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 140690_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:39:20.27 +23:44:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239260_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 239260_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:35:26.65 +18:48:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76961_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 76961_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:42:13.47 +20:28:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84895_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 84895_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:35:01.30 +20:55:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70013_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 70013_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:26:09.28 +20:07:42.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 96088_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 96088_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:40.08 +21:32:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67272_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 67272_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:27:16.68 +20:00:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182417_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 182417_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:28:47.22 +25:53:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128412_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 128412_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:22:01.02 +23:06:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64063_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 64063_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:36:19.51 +19:53:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25825_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 25825_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:27.97 +18:03:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55065_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 55065_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 71583_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 71583_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:41:13.80 +20:15:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135961_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 135961_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:31:10.29 +23:30:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181548_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 181548_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 43872_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 43872_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:03:06.00 +18:38:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179701_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 179701_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:33:34.32 +26:01:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152156_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 152156_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:40:40.31 +24:17:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58717_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 58717_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:08:06.32 +19:25:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93934_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 93934_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:29:30.13 +21:22:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237905_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 237905_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:36:17.25 +17:51:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56986_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 56986_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 120698_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 120698_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:03:36.25 +22:30:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83710_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 83710_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 39197_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 39197_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:59:04.76 +18:18:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178253_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
Preparing report for the candidate 178253_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
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Considering the candidate 26860_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 26860_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:37:38.84 +18:06:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65894_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 65894_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 18:54:15.44 +19:33:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82939_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 82939_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:12:25.21 +20:39:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174572_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 174572_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:25:20.41 +26:12:28.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24448_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 24448_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:38:55.13 +17:59:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81704_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 81704_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:37:37.78 +20:45:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65594_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 65594_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
**** FOUND 19:34:34.72 +19:46:27.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 28662_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471
The candidate 28662_fd_Vul-01-Q2b1x1_2026-04-13_02-29-25_20.00sec_-4.90C_LIGHT_0471 did not pass the final checks
