This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC
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
Gaia DR3 3090796940244089344,2461147.6546,9.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090796940244089344 20260417.1546 9.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3090774228457552128,2461147.6546,9.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090774228457552128 20260417.1546 9.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 3090789346742248320,2461147.6546,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090789346742248320 20260417.1546 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 3090842810494841984,2461147.6546,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090842810494841984 20260417.1546 11.10CV 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 3090774881292386432,2461147.6546,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090774881292386432 20260417.1546 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J122.8957+02.5818,2461147.6546,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J122.8957+02.5818 20260417.1546 11.31CV 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 3090845524914121856,2461147.6546,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090845524914121856 20260417.1546 11.47CV 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 J123.0897+02.4276,2461147.6546,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.0897+02.4276 20260417.1546 11.96CV 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 3090789243663042432,2461147.6546,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090789243663042432 20260417.1546 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3090764332852775040,2461147.6546,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3090764332852775040 20260417.1546 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6546,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1546 12.82CV 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,2461147.6546,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1546 12.79CV 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,2461147.6546,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1546 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J123.1192+01.7528,2461147.6546,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J123.1192+01.7528 20260417.1546 13.11CV 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,2461147.6546,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1546 13.40CV 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,2461147.6546,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1546 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461147.6546,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1546 13.96CV 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: 2461049.80101628 09.01.2026 07:13:17.807 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
First image: 2461049.80101628 09.01.2026 07:13:17.807 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Last image: 2461147.65638696 17.04.2026 03:45:01.833 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 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): 25854
Objects passed selection criteria: 25813
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 22673.5
Average stars matched: 22006.2 (97.0571 %)
Memory usage VmPeak: 128704 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 22:52:29 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: 2461049.80101628 09.01.2026 07:13:17.807 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
First image: 2461049.80101628 09.01.2026 07:13:17.807 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Last image: 2461147.65638696 17.04.2026 03:45:01.833 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 185
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 181 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): 183728
Objects passed selection criteria: 183335
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 162455
Average stars matched: 156066 (96.0669 %)
Memory usage VmPeak: 2119940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 22:57:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
SExtractor catalog cache: saved Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat to cache
SExtractor catalog cache: saved Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.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/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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: 2461147.65288807
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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits exists and is non-empty
Saving wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits to local_wcs_cache/
'wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits' -> 'local_wcs_cache/wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits'
wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits exists and is non-empty
Saving wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits to local_wcs_cache/
'wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits' -> 'local_wcs_cache/wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits'
wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits exists and is non-empty
Saving wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits to local_wcs_cache/
'wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits' -> 'local_wcs_cache/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits'
wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits exists and is non-empty
Saving wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits to local_wcs_cache/
'wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits' -> 'local_wcs_cache/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits (1st reference image)
verification OK: wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:42:51.201 -02:00:05.03 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits (1st new image)
verification OK: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:42:46.760 -02:00:40.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:42:51.201 -02:00:05.03
Second-epoch image center 07:42:46.760 -02:00:40.58
Angular distance between the image centers 0.0210 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits (2nd new image)
verification OK: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:42:45.512 -02:00:34.92 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:42:51.201 -02:00:05.03
Second-epoch image center 07:42:45.512 -02:00:34.92
Angular distance between the image centers 0.0251 deg.
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# 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 07:42:46.760 -02:00:40.58
Second-epoch second image center 07:42:45.512 -02:00:34.92
Angular distance between the image centers 0.00543 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/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits &> /tmp/tmp.NoNY1Sq3L4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits &> /tmp/tmp.QwTS3Egj9n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits &> /tmp/tmp.UQpxVHa8aE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits &> /tmp/tmp.3I1BPEhi0u
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits and wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits and wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
Found non-empty wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits and wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
The reference image (wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits) and catalog (wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat) found
'wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat' -> 'wcsmag.cat'
Read 26599 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 107.8041 to 123.6659 deg, Dec -7.3133 to +3.3237 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 107.8041 to 123.6659 deg, Dec -7.3133 to 3.3237 deg
Loaded 18114 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): 13675 out of 15075 total matches.
Matched with Tycho-2 15075 out of 26599 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.910669
a=0.000000 b=1.000000 c=22.910669
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
2.1 pix Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
3.1 pix fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
2.4 pix fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Limiting magnitude estimates:
15.0 mag. Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
15.0 mag. Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
14.2 mag. fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
14.7 mag. fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.6 (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.NoNY1Sq3L4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits' -> 'wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
WCS_IMAGE_NAME=wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
WCS-calibrated image found: wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Checking if the catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits alredy exist and is non-empty...
Catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
WCS catalog name: wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2845, passed=26599
Got 26599 stars (including 23722 good ones) from the SExtractor catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
util/solve_plate_with_UCAC5 got 26599 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 26061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 26061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 26043 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits -region wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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.QwTS3Egj9n (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits' -> 'wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
WCS_IMAGE_NAME=wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
WCS-calibrated image found: wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
Checking if the catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits alredy exist and is non-empty...
Catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
WCS catalog name: wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2792, passed=26638
Got 26638 stars (including 23822 good ones) from the SExtractor catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat
util/solve_plate_with_UCAC5 got 26638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 26047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 26047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 26032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits -region wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.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.UQpxVHa8aE (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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
WCS_IMAGE_NAME=wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
WCS-calibrated image found: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Checking if the catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
WCS catalog name: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1499, passed=17078
Got 17078 stars (including 15563 good ones) from the SExtractor catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat
util/solve_plate_with_UCAC5 got 17078 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits -region wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.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.3I1BPEhi0u (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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
WCS_IMAGE_NAME=wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
WCS-calibrated image found: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Checking if the catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
WCS catalog name: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1724, passed=21005
Got 21005 stars (including 19258 good ones) from the SExtractor catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat
util/solve_plate_with_UCAC5 got 21005 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
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: 960 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 20157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 961 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(), 20156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 20156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits -region wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits'
Saving fully-calibrated image wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits'
Saving fully-calibrated image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits'
Saving fully-calibrated image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits'
Preparing the HTML report for the field Mon-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32360.dat to exclusion_list_gaiadr2.txt
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31648_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 31648_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:29:32.12 -03:14:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 2.096 3060639943339887360 112.38353092434 -03.24602998518 11.8477 11.1788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31731_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 31731_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:48:00.94 -02:35:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32360_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 32360_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:15:09.84 -04:30:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.314 3059335956907273472 108.79096705219 -04.51155313027 12.0990 11.7336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32377_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 32377_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:12:53.62 -04:09:31.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07666_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 07666_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:59.09 -04:30:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18216_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 18216_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:46:04.58 -00:23:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04544_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 04544_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:01:01.29 -05:37:34.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
SExtractor catalog cache: saved Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat to cache
SExtractor catalog cache: saved Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Creating symlink local_wcs_cache/wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits exists and is non-empty
wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits exists and is non-empty
wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits exists and is non-empty
wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits (1st reference image)
verification OK: wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:42:51.201 -02:00:05.03 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits (1st new image)
verification OK: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:42:46.760 -02:00:40.58 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:42:51.201 -02:00:05.03
Second-epoch image center 07:42:46.760 -02:00:40.58
Angular distance between the image centers 0.0210 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits (2nd new image)
verification OK: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Image size: 941.3'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:42:45.512 -02:00:34.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:42:51.201 -02:00:05.03
Second-epoch image center 07:42:45.512 -02:00:34.92
Angular distance between the image centers 0.0251 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 07:42:46.760 -02:00:40.58
Second-epoch second image center 07:42:45.512 -02:00:34.92
Angular distance between the image centers 0.00543 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/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits &> /tmp/tmp.RKoo3clRfm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits &> /tmp/tmp.OKB16pzB4F
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits &> /tmp/tmp.gML8f9Ihb1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits &> /tmp/tmp.atpkDuDMDQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits and wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits and wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
Found non-empty wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits and wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
The reference image (wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits) and catalog (wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat) found
'wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat' -> 'wcsmag.cat'
Read 189825 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 107.8012 to 123.6728 deg, Dec -7.3139 to +3.3238 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 107.8012 to 123.6728 deg, Dec -7.3139 to 3.3238 deg
Loaded 18129 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): 11376 out of 16248 total matches.
Matched with Tycho-2 16248 out of 189825 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.732856
a=0.000000 b=1.000000 c=22.732856
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.08
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.08
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 148 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
2.0 pix Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
2.6 pix fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
2.1 pix fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Limiting magnitude estimates:
15.1 mag. Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
15.1 mag. Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
14.3 mag. fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
14.8 mag. fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.8 (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.RKoo3clRfm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits' -> 'wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
WCS_IMAGE_NAME=wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
WCS-calibrated image found: wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Checking if the catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits alredy exist and is non-empty...
Catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
WCS catalog name: wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=26167, passed=189790
Got 189790 stars (including 163341 good ones) from the SExtractor catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat
util/solve_plate_with_UCAC5 got 189790 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 950 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(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 185548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 950 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(), 185547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 185547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits -region wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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.OKB16pzB4F (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits' -> 'wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
WCS_IMAGE_NAME=wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
WCS-calibrated image found: wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
Checking if the catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits alredy exist and is non-empty...
Catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat corresponding to the image wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
WCS catalog name: wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=25761, passed=187971
Got 187971 stars (including 161894 good ones) from the SExtractor catalog wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat
util/solve_plate_with_UCAC5 got 187971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
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: 949 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 184550 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 951 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(), 184547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 184547 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits -region wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.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.gML8f9Ihb1 (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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
WCS_IMAGE_NAME=wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
WCS-calibrated image found: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Checking if the catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
WCS catalog name: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=15760, passed=113240
Got 113240 stars (including 97299 good ones) from the SExtractor catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat
util/solve_plate_with_UCAC5 got 113240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 960 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(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 111908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 411 to 470 (Dec -7.7 to 3.8)
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(), 111908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 111908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits -region wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.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.atpkDuDMDQ (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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
WCS_IMAGE_NAME=wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
WCS-calibrated image found: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Checking if the catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat corresponding to the image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
WCS catalog name: wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=84, blended=16629, passed=163056
Got 163056 stars (including 146191 good ones) from the SExtractor catalog wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat
util/solve_plate_with_UCAC5 got 163056 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 158347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 954 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(), 158346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 158346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits -region wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_Mon-03-Q1b1x1_2026-01-09_01-13-17_20.00sec_-15.00C_LIGHT_0283.fits
Saving fully-calibrated image wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_Mon-03-Q1b1x1_2026-01-09_01-14-21_20.00sec_-15.00C_LIGHT_0284.fits
Saving fully-calibrated image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-39-59_20.00sec_-4.90C_LIGHTs_0058.fits
Saving fully-calibrated image wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.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_2026-04-16_CI_Mon-03-Q1b1x1_224552_TTUQ1b1x1_3417200_iRY73RhC/wcs_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059.fits
Preparing the HTML report for the field Mon-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out215348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out216490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out217823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out218626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out215728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out215734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out215869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out218073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out218755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219785.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 42s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 11s
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Considering the candidate 215348_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215348_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:26:12.51 -01:39:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.417 3061808659779322112 111.55251514591 -01.65122377980 14.6490 14.2707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215353_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215353_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:38:58.89 +02:29:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.437 3135270020926534784 114.74549290816 +02.48772055066 13.4815 13.0282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215359_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215359_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:28:29.39 +00:30:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.154 3134583547713981568 112.12333436571 +00.50785343173 14.2775 13.5758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215361_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215361_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:50:37.74 +01:01:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215365_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215365_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:27:42.08 -06:03:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 1.972 3055464855645323008 111.92567072123 -06.06020597219 13.8793 13.2016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215375_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215375_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:34:15.63 +02:09:10.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 215380_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215380_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:26:35.04 -06:39:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.185 3055033464832253440 111.64547735153 -06.66000592475 13.3850 12.4040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215381_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215381_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:18:21.58 -00:04:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215388_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215388_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:56:13.25 -04:30:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215393_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215393_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:01:27.65 -06:31:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215400_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215400_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:01:59.60 -04:07:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215402_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215402_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:19:33.01 -00:59:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.927 3110166796077738240 109.88789548836 -00.99890369965 13.7298 13.2233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215405_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215405_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:08:58.69 +01:22:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215420_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215420_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:44:22.03 -07:06:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215421_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215421_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:34:42.29 -06:25:03.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 215433_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215433_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:47:45.12 -06:57:30.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 215437_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215437_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:31:06.07 -02:25:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215446_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215446_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:36:16.57 -03:30:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215447_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215447_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:56:19.64 -06:53:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.033 3043143006787101568 119.08066707885 -06.89707739099 13.9763 13.1462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215448_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215448_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:07:58.61 -05:25:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215460_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215460_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:28:53.26 -03:06:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215462_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215462_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:51:18.55 -04:46:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215465_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215465_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:27.77 -06:52:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.707 3043181558414108544 119.61574423191 -06.86908272714 13.4927 13.1981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215467_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215467_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:02:34.35 -01:00:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.160 3083061120030052608 120.64280668376 -01.01504992252 13.3855 12.7191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215470_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215470_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:31:11.83 -04:27:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215473_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215473_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:48:21.06 -06:04:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215480_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215480_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:23:27.73 -03:25:47.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215483_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215483_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:08:55.59 -04:45:20.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215494_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215494_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:30:14.83 +03:06:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.366 3136302324905255296 112.56214142779 +03.10465696422 13.1091 12.6804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215499_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215499_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:41:26.48 -05:56:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215500_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215500_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:13:18.14 -04:02:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215501_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215501_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:55:09.02 -05:39:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215508_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215508_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:30:51.60 -06:43:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.274 3055170392687515648 112.71526313793 -06.72949008648 13.9234 13.4353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215521_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215521_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:40:21.10 +02:58:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215539_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215539_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:12:45.24 -05:37:10.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 215551_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215551_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:10:59.28 +02:14:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215555_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215555_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:21:08.52 +01:13:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.010 3111648422352574336 110.28573706906 +01.21761654809 13.0398 12.5484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215556_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215556_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 215570_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215570_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:16:21.12 +02:52:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215577_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215577_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:13:16.11 -00:31:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.665 3110967854717435136 108.31761756494 -00.52631091626 13.8028 13.4234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215581_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215581_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:24.48 -00:22:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215587_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215587_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:37:26.64 +01:02:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.071 3087009535005360512 114.36087547529 +01.04804946931 13.2252 12.5906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215589_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215589_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:32:25.88 +00:19:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.824 3086500426761617920 113.10833907216 +00.33063415379 12.7213 12.3884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215598_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215598_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:48.60 -02:25:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215606_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215606_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:56:56.83 -06:21:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215607_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215607_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:05:45.18 -05:32:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215611_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215611_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:29:26.54 +00:18:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215612_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215612_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:10:49.04 -03:20:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215617_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215617_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:31:06.68 +01:32:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215619_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215619_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:06:08.37 -01:18:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 0.749 3082887431553356928 121.53466777366 -01.30795390124 11.2003 10.8607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215620_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215620_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:49:58.40 +01:35:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215720_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215720_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:48:00.93 -02:35:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215728_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 215728_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215734_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 215734_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 215750_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215750_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:11:26.53 -05:05:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215824_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215824_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 215869_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 215869_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
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Considering the candidate 215964_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 215964_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 216038_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 216038_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216062_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216062_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 216091_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 216091_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216107_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 216107_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216176_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216176_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 216203_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 216203_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216222_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216222_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 216280_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216280_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 216401_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216401_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 216459_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216459_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 216490_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216490_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:13:13.12 +01:05:52.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)
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Considering the candidate 216522_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 216522_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216554_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 216554_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 216581_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216581_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 216606_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216606_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:24:37.40 -06:31:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216737_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216737_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:59:15.56 -07:12:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 216796_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 216796_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 217106_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217106_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:11:48.44 -05:41:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217146_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217146_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 217180_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217180_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:46:34.94 -06:56:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217213_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217213_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:10:12.01 +02:25:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.535 3090830715866779136 122.55047176083 +02.43125216075 12.6653 12.1382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217224_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217224_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:20.78 -05:49:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217278_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217278_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:29:09.41 -04:31:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217292_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217292_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:13:17.69 +00:47:47.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217324_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 217324_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217501_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217501_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:51:34.27 -06:59:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217535_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 217535_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217551_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 217551_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217668_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 217668_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
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Considering the candidate 217789_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217789_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:24:00.45 +02:00:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217823_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217823_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:20:04.58 +02:28:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.006 3136010816885313280 110.01951799753 +02.47026567525 13.4213 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217854_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217854_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 217901_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217901_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:15:46.81 -01:58:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217910_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217910_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:34:46.53 -03:39:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217936_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 217936_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:11:49.89 -03:36:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218059_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218059_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:25:46.30 -05:50:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218073_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 218073_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218096_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218096_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:26:51.63 +00:34:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218137_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218137_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:12:41.61 -03:14:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218183_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218183_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 218213_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218213_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 218289_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218289_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:25:37.93 -05:49:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218300_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218300_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:34:45.46 -03:39:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218327_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218327_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:26:34.67 -02:09:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218391_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218391_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:11:46.78 -04:57:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218399_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218399_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:11:17.23 -05:20:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.801 3067565977536210944 122.82165724891 -05.33689991433 12.9274 12.9429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218401_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218401_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:09:11.19 +02:00:56.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218406_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218406_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:15:05.04 +01:43:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.680 3114847588874036608 108.77116999390 +01.72408257522 13.6119 13.1600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218437_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218437_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:18:12.00 -03:52:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218509_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218509_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:22:42.94 +02:00:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218522_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218522_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:19:41.62 -03:33:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218536_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218536_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:16:48.33 -04:49:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218626_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218626_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:12:03.40 +01:41:06.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218673_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218673_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:51:34.19 -07:00:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218741_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218741_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:25:28.47 +00:35:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218755_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 218755_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 218863_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 218863_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:29:12.67 -03:21:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219007_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 219007_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219075_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219075_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:21:14.53 -02:33:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219101_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219101_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:31:25.67 -05:31:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219246_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219246_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:17:40.96 -06:11:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219354_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219354_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:29.61 -00:26:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.308 3083948494633088128 119.62310155513 -00.44670508859 13.7568 13.2837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219449_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219449_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:22:25.24 -03:39:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219476_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219476_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 219512_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219512_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:20:41.56 -05:23:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219520_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219520_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:47:44.86 -06:02:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.365 3044240800427857536 116.93778450780 -06.04130785352 13.9199 13.4018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219536_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219536_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:35:29.06 -05:23:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219605_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219605_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:39:43.52 -04:41:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219647_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219647_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:28:15.10 -04:55:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 4.066 3058688314500402048 112.06401818727 -04.93167720817 14.3482 13.6193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219704_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219704_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:53:22.25 -05:23:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.847 3044348793086332160 118.34251355311 -05.39444166825 13.9590 13.4826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219709_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219709_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:14:26.35 +01:07:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.679 3111784177680101120 108.61017650614 +01.12679154945 14.4010 13.6983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219763_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219763_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:23:38.99 -01:54:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219785_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
Preparing report for the candidate 219785_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
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Considering the candidate 219820_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219820_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:25:31.41 -02:43:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219832_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219832_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:47:05.00 -04:49:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.402 3056488741486641280 116.77063287661 -04.82391890413 14.2309 13.7133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219835_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219835_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:13:21.48 -01:37:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.782 3108578207934380288 108.33995256542 -01.61887362664 14.2128 13.5005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219853_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219853_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:53:31.48 -06:04:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 219870_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219870_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:22:13.81 -04:09:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.650 3059023940425632768 110.55765165305 -04.16166597192 14.1568 13.4049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219949_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219949_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:24:56.52 +01:22:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.455 3135640384546481920 111.23542778069 +01.37762001188 14.2411 13.7165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219955_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 219955_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:31:13.19 -02:38:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180895_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 180895_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:17:32.04 +01:05:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30048_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 30048_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 08:01:01.29 -05:37:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140947_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 140947_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 172700_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 172700_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:54:00.71 +01:44:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123073_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 123073_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:39:36.63 -00:53:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108633_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 108633_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:31:13.98 -01:40:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95244_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 95244_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:43:25.36 -02:18:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38026_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 38026_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:45:27.24 -05:13:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51571_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 51571_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
**** FOUND 07:58:59.10 -04:30:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133716_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059
The candidate 133716_fd_Mon-03-Q1b1x1_2026-04-16_22-45-01_20.00sec_-5.00C_LIGHTs_0059 did not pass the final checks
