This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 04 03.51 +04 40 45.0 11.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 28 11.15 +05 43 04.7 11.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,11.79,0.05,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
VARIABLE_NAME 20260416.2383 11.79CV 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!
TCP 2026 04 16.2383* 11 12 19.95 +01 33 23.0 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,12.47,0.05,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
VARIABLE_NAME 20260416.2383 12.47CV 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!
TCP 2026 04 16.2383* 10 50 33.32 +03 39 34.7 12.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 10 38 12.72 +08 44 35.4 12.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 16 40.36 +05 45 25.0 13.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 02 20.48 +02 52 47.6 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 02 03.32 +10 35 56.2 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 05 15.38 +08 51 34.4 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 05 21.03 +10 44 17.3 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 29 33.04 +09 26 16.7 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,14.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 14.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 27 22.67 +01 49 04.7 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.2383* 11 03 14.55 +10 28 51.4 14.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.7383,14.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.2383 14.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461146.73859822 16.04.2026 05:43:24.886 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 3 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): 6140
Objects passed selection criteria: 6136
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 5768.25
Average stars matched: 5506.5 (95.4622 %)
Memory usage VmPeak: 111816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 01:11:36 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: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461146.73859822 16.04.2026 05:43:24.886 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 11 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): 33412
Objects passed selection criteria: 33321
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 31791
Average stars matched: 30053.2 (94.5338 %)
Memory usage VmPeak: 134232 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 01:12:28 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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: 2461146.73791318
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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
Saving wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
Saving wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits'
wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Image size: 941.7'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: 11:08:11.175 +05:59:37.65 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_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Image size: 941.4'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: 11:08:39.010 +05:58:19.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:39.010 +05:58:19.42
Angular distance between the image centers 0.1174 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Image size: 941.4'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: 11:08:36.477 +05:58:38.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:36.477 +05:58:38.01
Angular distance between the image centers 0.1062 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 11:08:39.010 +05:58:19.42
Second-epoch second image center 11:08:36.477 +05:58:38.01
Angular distance between the image centers 0.01170 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.NbgYbWaZlC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.omqsInFkKs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits &> /tmp/tmp.RImrxCqwff
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits &> /tmp/tmp.24THBPTQgn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat' -> 'wcsmag.cat'
Read 5629 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0658 to 175.0329 deg, Dec +0.7091 to +11.2821 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 159.0658 to 175.0329 deg, Dec 0.7091 to 11.2821 deg
Loaded 3938 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): 3214 out of 3354 total matches.
Matched with Tycho-2 3354 out of 5629 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.832371
a=0.000000 b=1.000000 c=22.832371
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.1 pix Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.2 pix fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Limiting magnitude estimates:
15.2 mag. Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.2 mag. Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.2 mag. fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
15.2 mag. fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.NbgYbWaZlC (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=5629
Got 5629 stars (including 5225 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 5629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.omqsInFkKs (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=431, passed=5671
Got 5671 stars (including 5234 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 5671 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.RImrxCqwff (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=392, passed=5981
Got 5981 stars (including 5579 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat
util/solve_plate_with_UCAC5 got 5981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 450 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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.24THBPTQgn (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=402, passed=5931
Got 5931 stars (including 5525 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat
util/solve_plate_with_UCAC5 got 5931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 451 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
Saving fully-calibrated image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits'
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20431.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20401_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 20401_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20431_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 20431_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20459_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 20459_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:23:23.29 +06:07:13.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20473_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 20473_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:23:55.33 +10:18:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20474_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 20474_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:03:12.08 +07:11:09.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Leo-07-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 ####
11:04:03.51 +04:40:45.0
11:28:11.15 +05:43:04.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Image size: 941.7'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: 11:08:11.175 +05:59:37.65 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_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Image size: 941.4'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: 11:08:39.010 +05:58:19.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:39.010 +05:58:19.42
Angular distance between the image centers 0.1174 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Image size: 941.4'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: 11:08:36.477 +05:58:38.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:36.477 +05:58:38.01
Angular distance between the image centers 0.1062 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 11:08:39.010 +05:58:19.42
Second-epoch second image center 11:08:36.477 +05:58:38.01
Angular distance between the image centers 0.01170 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/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.tb4gj6EG97
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.6TJ7Zz3hCV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits &> /tmp/tmp.0sVWARomDp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits &> /tmp/tmp.tV0yykM4es
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat' -> 'wcsmag.cat'
Read 31032 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0537 to 175.0351 deg, Dec +0.7036 to +11.2819 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 159.0537 to 175.0351 deg, Dec 0.7036 to 11.2819 deg
Loaded 3942 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): 3142 out of 3441 total matches.
Matched with Tycho-2 3441 out of 31032 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714936
a=0.000000 b=1.000000 c=22.714936
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.0 pix Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
2.0 pix fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Limiting magnitude estimates:
15.3 mag. Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.3 mag. Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.4 mag. fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
15.4 mag. fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tb4gj6EG97 (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1190, passed=31016
Got 31016 stars (including 29781 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 31016 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.6TJ7Zz3hCV (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1251, passed=31400
Got 31400 stars (including 30103 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 31400 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31073 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.0sVWARomDp (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1287, passed=32635
Got 32635 stars (including 31283 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat
util/solve_plate_with_UCAC5 got 32635 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 32312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 32312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 32312 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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.tV0yykM4es (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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1335, passed=33023
Got 33023 stars (including 31631 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat
util/solve_plate_with_UCAC5 got 33023 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 32697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 32697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 32697 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Saving fully-calibrated image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-42-25_20.00sec_-4.90C_LIGHTs_0164.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.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_Leo-07-Q1b1x1_004416_TTUQ1b1x1_15469_J1I25vV8/wcs_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165.fits
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53387.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53417.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 52333_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52333_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:54:56.66 +10:13:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 4.693 3870891781495924352 163.73691119637 +10.21762125294 14.9607 14.4121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52336_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52336_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:13:28.49 +07:15:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52337_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52337_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:33:58.83 +09:15:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.789 3914351421692944512 173.49509557380 +09.25711596999 14.1257 13.5310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52441_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52441_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:04:03.50 +04:40:44.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52473_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52473_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:28:11.14 +05:43:04.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52561_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52561_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 52601_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52601_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52606_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52606_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52629_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52629_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:50:09.92 +08:50:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52664_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52664_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 52702_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52702_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 52731_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52731_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 52809_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52809_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:10:21.04 +11:03:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52822_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 52822_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:06:16.25 +07:50:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52922_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 52922_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 53093_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53093_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:55:50.13 +09:56:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53119_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 53119_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 53172_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 53172_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 53181_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 53181_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 53193_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53193_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:47:58.40 +06:54:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53252_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53252_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:59:52.01 +01:04:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53273_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53273_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:49:55.17 +04:29:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 2.504 3858051306750066048 162.47994264597 +04.49085900842 14.8464 14.0215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53309_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53309_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:06:01.65 +01:10:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.785 3805202009050243072 166.50669182976 +01.17524248813 14.5182 13.8337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53311_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53311_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:38:37.28 +10:24:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53325_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53325_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:46:07.02 +02:03:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.726 3809044557376026752 161.52908196834 +02.06194524768 14.7120 14.2186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53335_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53335_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:16:58.63 +10:35:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53344_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53344_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:30:32.65 +10:23:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53350_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53350_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:40:41.99 +11:02:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.962 3870721700791212544 160.17507200759 +11.04320161967 14.8588 14.4645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53352_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53352_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:41:50.40 +06:24:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 3.243 3859473318881459456 160.46086465650 +06.41209067652 14.8600 14.3515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53358_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53358_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:41:59.40 +06:18:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53378_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53378_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:39:42.02 +07:55:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53379_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53379_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:23:19.90 +09:46:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53383_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53383_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:39:34.59 +10:17:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.595 3915932175816185856 174.89368054894 +10.29056694623 14.8243 14.3228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53384_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53384_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:47:48.90 +01:50:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53387_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53387_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:00:23.01 +10:19:23.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)
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Considering the candidate 53401_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53401_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:43:05.05 +08:48:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.040 3869051916290651392 160.77089880113 +08.80780336295 14.9861 14.9334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53404_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53404_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:49:57.42 +06:24:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53416_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53416_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:12:01.40 +08:11:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53417_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
Preparing report for the candidate 53417_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
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Considering the candidate 53423_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53423_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:05:35.90 +11:01:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 2.030 3868294391433635456 166.39966248376 +11.02683035302 15.2699 14.7856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53437_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53437_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:40:41.68 +09:26:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.584 3869151838704683648 160.17331378904 +09.43617511457 14.8018 14.3744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53449_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53449_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:39:55.66 +07:48:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 0.728 3868688978668958208 159.98181636650 +07.80446291665 14.7690 14.2138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53462_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53462_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:38:33.52 +04:37:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.468 3858629718585265920 159.63944879539 +04.62362718920 14.9568 14.3944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53464_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53464_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:58:46.00 +07:16:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53473_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53473_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:59:42.96 +02:30:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53489_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53489_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:49:30.17 +04:52:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.755 3858143837525405056 162.37616334001 +04.86957045308 15.3338 14.8854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53491_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53491_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 11:19:44.70 +01:18:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.608 3810238218982105856 169.93580337445 +01.30343089980 14.6869 13.9347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53493_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53493_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:54:13.89 +05:49:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53503_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53503_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:38:43.80 +04:42:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 0.357 3858633429437005312 159.68240895451 +04.70262700196 14.8324 14.3268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53547_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53547_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:38:07.29 +03:01:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.161 3856114482657300096 159.53011028172 +03.01746250829 14.8225 14.2287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53557_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 53557_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
**** FOUND 10:54:58.82 +01:28:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.002 3808060086447438848 163.74497917611 +01.47776955790 14.7664 13.9059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 24599_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165
The candidate 24599_fd_Leo-07-Q1b1x1_2026-04-16_00-43-24_20.00sec_-4.90C_LIGHTs_0165 did not pass the final checks
