This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7291,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2291 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7291,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2291 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3161729768247327744,2461136.7291,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3161729768247327744 20260406.2291 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3168993966693303040,2461136.7291,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3168993966693303040 20260406.2291 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7291,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2291 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 601050440802124416,2461136.7291,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 601050440802124416 20260406.2291 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7291,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2291 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7291,14.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2291 14.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7291,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2291 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7291,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2291 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7291,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2291 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SU Cnc,2461136.7291,12.60,0.05,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
SU Cnc 20260406.2291 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3149446471018843776,2461136.7291,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3149446471018843776 20260406.2291 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CO CMi,2461136.7291,11.78,0.05,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
CO CMi 20260406.2291 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J073057.12+142455.7,2461136.7291,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J073057.12+142455.7 20260406.2291 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GR Cnc,2461136.7291,13.17,0.05,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
GR Cnc 20260406.2291 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.69311591 22.02.2026 04:37:55.215 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
First image: 2461093.69311591 22.02.2026 04:37:55.215 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Last image: 2461136.72947069 06.04.2026 05:30:16.268 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 5 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): 17591
Objects passed selection criteria: 17568
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 16290.2
Average stars matched: 15799.5 (96.9875 %)
Memory usage VmPeak: 121492 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:32:17 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: 2461093.69311591 22.02.2026 04:37:55.215 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
First image: 2461093.69311591 22.02.2026 04:37:55.215 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Last image: 2461136.72947069 06.04.2026 05:30:16.268 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 91
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 86 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): 113342
Objects passed selection criteria: 113082
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 93042.8
Average stars matched: 89625.5 (96.3272 %)
Memory usage VmPeak: 1885432 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:35:30 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/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat to cache
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.72868626
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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits exists and is non-empty
Saving wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits to local_wcs_cache/
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits' -> 'local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits'
wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits exists and is non-empty
Saving wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits to local_wcs_cache/
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> 'local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits exists and is non-empty
Saving wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits to local_wcs_cache/
'wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits' -> 'local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits'
wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits exists and is non-empty
Saving wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits to local_wcs_cache/
'wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits' -> 'local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:00:00.351 +14:00:01.54
Second-epoch image center 08:00:08.208 +13:59:31.86
Angular distance between the image centers 0.0328 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:00:00.351 +14:00:01.54
Second-epoch image center 08:00:06.329 +13:59:02.03
Angular distance between the image centers 0.0293 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:00:08.208 +13:59:31.86
Second-epoch second image center 08:00:06.329 +13:59:02.03
Angular distance between the image centers 0.01124 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/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits &> /tmp/tmp.yozchEx7O5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits &> /tmp/tmp.vtWgD6uXYL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits &> /tmp/tmp.3cjsjv2HcK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits &> /tmp/tmp.q1s9EzSI3A
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
The reference image (wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits) and catalog (wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat) found
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat' -> 'wcsmag.cat'
Read 17822 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.6007 to 128.1591 deg, Dec +8.4892 to +19.3325 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 111.6007 to 128.1591 deg, Dec 8.4892 to 19.3325 deg
Loaded 10956 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): 8480 out of 9314 total matches.
Matched with Tycho-2 9314 out of 17822 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.894261
a=0.000000 b=1.000000 c=22.894261
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
2.0 pix Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
4.2 pix fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
4.2 pix fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Limiting magnitude estimates:
15.3 mag. Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
15.3 mag. Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
14.6 mag. fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
14.6 mag. fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 12.1 (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.yozchEx7O5 (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1660, passed=17822
Got 17822 stars (including 16133 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
util/solve_plate_with_UCAC5 got 17822 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 17410 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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 17409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 17409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits -region wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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.vtWgD6uXYL (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_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=1628, passed=17766
Got 17766 stars (including 16092 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat
util/solve_plate_with_UCAC5 got 17766 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 17373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 17372 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 17372 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits -region wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_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.3cjsjv2HcK (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=680, passed=15008
Got 15008 stars (including 14321 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat
util/solve_plate_with_UCAC5 got 15008 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 14715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 14714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 14714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.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.q1s9EzSI3A (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=676, passed=14959
Got 14959 stars (including 14277 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat
util/solve_plate_with_UCAC5 got 14959 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 14665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 14665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 14665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits'
Saving fully-calibrated image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits'
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits'
Preparing the HTML report for the field Cnc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out21257.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out21291.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 21101_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21101_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:21:14.87 +12:08:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.199 649318619008068480 125.31195823575 +12.14691692879 11.6561 11.2067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21102_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21102_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:22:10.58 +10:09:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21257_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21257_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:09:59.97 +16:59:52.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)
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Considering the candidate 21291_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 21291_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 21476_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21476_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:09:27.93 +14:39:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21496_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21496_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:46:14.89 +18:30:22.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21580_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21580_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:55:09.31 +12:34:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.114 3151252418866615552 118.78890086042 +12.57209834011 11.6939 11.0183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21622_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21622_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:46:56.77 +15:01:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.632 3164797813708752384 116.73721155203 +15.02517353177 12.1512 11.6725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21698_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21698_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:11:16.34 +16:04:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21699_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21699_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:53:39.13 +17:32:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.216 668276746389570176 118.41302670909 +17.54516404562 11.9433 10.9649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21701_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21701_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:57:16.42 +14:18:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.076 654467292660514816 119.31839923777 +14.30931267162 11.9730 11.2687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21762_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21762_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:59:19.78 +12:17:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.800 3151076595788155648 119.83257987983 +12.28453987164 12.1246 11.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21765_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21765_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:52:05.56 +13:55:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.437 3152462500132898944 118.02324782610 +13.91991425371 12.0933 11.4090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21788_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 21788_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:31:31.39 +10:04:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.648 3161565902357834880 112.88048154139 +10.06943654492 12.2255 11.6728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05325_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 05325_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:16:33.69 +11:43:34.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14568_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 14568_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:21:42.76 +17:17:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02717_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 02717_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:13:38.17 +10:11:52.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cnc-04-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 ####
08:10:30.17 +16:29:05.5
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/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat to cache
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Creating symlink local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits exists and is non-empty
wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits exists and is non-empty
wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits exists and is non-empty
wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:00:00.351 +14:00:01.54
Second-epoch image center 08:00:08.208 +13:59:31.86
Angular distance between the image centers 0.0328 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:00:00.351 +14:00:01.54
Second-epoch image center 08:00:06.329 +13:59:02.03
Angular distance between the image centers 0.0293 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:00:08.208 +13:59:31.86
Second-epoch second image center 08:00:06.329 +13:59:02.03
Angular distance between the image centers 0.01124 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/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits &> /tmp/tmp.INQuJ4smfd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits &> /tmp/tmp.nb7TFULjng
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits &> /tmp/tmp.3OMf6QAfan
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits &> /tmp/tmp.XAzwnpsXhw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
The reference image (wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits) and catalog (wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat) found
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat' -> 'wcsmag.cat'
Read 121572 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.5681 to 128.1591 deg, Dec +8.4600 to +19.3367 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 111.5681 to 128.1591 deg, Dec 8.4600 to 19.3367 deg
Loaded 11019 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): 7271 out of 9482 total matches.
Matched with Tycho-2 9482 out of 121572 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.755863
a=0.000000 b=1.000000 c=22.755863
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 72 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
1.8 pix Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
3.7 pix fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
3.7 pix fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Limiting magnitude estimates:
15.5 mag. Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
15.5 mag. Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
14.7 mag. fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
14.7 mag. fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.0 (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.INQuJ4smfd (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=52, blended=11688, passed=121520
Got 121520 stars (including 109618 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat
util/solve_plate_with_UCAC5 got 121520 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119565 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits -region wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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.nb7TFULjng (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=11718, passed=121750
Got 121750 stars (including 109795 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat
util/solve_plate_with_UCAC5 got 121750 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 119926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits -region wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_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.3OMf6QAfan (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=4554, passed=65971
Got 65971 stars (including 61365 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat
util/solve_plate_with_UCAC5 got 65971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 65256 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 65257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 65257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.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.XAzwnpsXhw (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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=4449, passed=65539
Got 65539 stars (including 61024 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat
util/solve_plate_with_UCAC5 got 65539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 64938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 64938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 64938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.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_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_Cnc-04-Q1b1x1_2026-02-21_22-37-55_20.00sec_-15.00C_LIGHT_0163.fits
Saving fully-calibrated image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-29-08_20.00sec_-5.00C_LIGHTs_0098.fits
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.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_2026-04-06_CI_Cnc-04-Q1b1x1_003115_TTUQ1b1x1_9826_gSfPe3RT/wcs_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099.fits
Preparing the HTML report for the field Cnc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out131833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out144440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out19207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out48311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out142142.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out144095.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out09933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94727.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 9s
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Considering the candidate 141907_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141907_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:29:24.53 +17:05:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141911_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141911_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:41:35.49 +10:02:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.775 3149734096387839104 115.39774574262 +10.04075700184 14.0614 13.5721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141912_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141912_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:31:11.10 +16:01:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141913_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141913_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:27:37.56 +10:19:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.646 600731307552241408 126.90691166463 +10.32867644907 13.7710 13.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141919_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141919_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:28:48.19 +12:22:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.564 3163239775669666432 112.20049695680 +12.36993667097 13.2234 12.1580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141924_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141924_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:46:10.36 +11:39:11.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)
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Considering the candidate 141937_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141937_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:33:29.77 +10:09:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.696 3149653969478223232 113.37379890840 +10.15595971011 13.4727 13.0045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141938_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141938_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:10:20.28 +13:14:27.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 141941_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141941_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:30:39.64 +17:27:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141942_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141942_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:07:22.95 +17:31:17.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 141947_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141947_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:31:16.91 +10:55:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.175 3161766430088039680 112.82074149678 +10.92110749916 13.7413 13.3873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141949_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141949_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:30:00.37 +17:17:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141955_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141955_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:32:24.49 +16:10:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.889 658680999174842496 128.10248250242 +16.18188446020 13.9039 13.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141957_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 141957_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 141963_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141963_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:28:47.82 +11:02:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.957 3161877549482926848 112.19935284719 +11.04139532722 13.0375 12.6464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141967_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141967_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:29:20.09 +09:52:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.260 3161546630842185984 112.33519050598 +09.86986369379 13.3013 12.7210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141973_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141973_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:14:26.51 +15:06:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.401 655356694488087296 123.60981122437 +15.11365503892 13.6906 13.0528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141975_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 141975_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:16:47.44 +09:45:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.096 600486769294672512 124.19708301065 +09.75877107618 13.7609 13.2474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142050_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 142050_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:32:30.30 +15:49:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 2.275 657903507014610048 128.12677172183 +15.82355077620 9.8706 9.0855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142142_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 142142_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:09:59.98 +16:59:51.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142164_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 142164_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:10:30.15 +16:29:05.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 142891_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 142891_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142904_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 142904_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:37:56.83 +14:02:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142947_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 142947_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:01:23.49 +16:26:43.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 143030_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143030_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:44:11.28 +14:12:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.506 3164649727533562624 116.04634357799 +14.20810671567 13.0805 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143054_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143054_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:09:58.43 +12:58:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.082 650187752887683968 122.49405250368 +12.98053595534 12.9327 12.3748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143080_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143080_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:21:48.17 +13:37:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.449 651932643481183744 125.45065350062 +13.62962111225 13.2620 12.4505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143150_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143150_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:32:30.40 +16:05:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.110 658668079913223424 128.12679277027 +16.08827196909 13.0911 12.5664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143153_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143153_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:16:38.35 +16:23:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.388 655758119311624448 124.15989873389 +16.39505045321 13.0910 12.4249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143157_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143157_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:10:09.86 +12:38:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.915 650122916061755392 122.54089609567 +12.64710097785 13.2262 12.7491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143166_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143166_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:04:32.54 +09:17:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143269_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 143269_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 143358_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143358_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:52:00.50 +11:10:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.000 3150714998199402112 118.00183573709 +11.17622615599 13.2600 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143430_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143430_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:32:32.86 +17:19:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.705 659089467744704640 128.13728865382 +17.31893665939 13.2211 12.5328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143446_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143446_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:29:47.41 +15:32:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143518_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143518_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:19:57.67 +15:18:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.272 652441854804522880 124.99043107107 +15.31074440350 13.7668 13.2478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143621_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143621_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:05:02.80 +10:31:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.952 3147570738541698048 121.26271265563 +10.52377324473 13.4792 12.8705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143656_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143656_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:10:01.16 +14:29:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.076 653820264427927808 122.50487129493 +14.49664674906 13.6133 13.2500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143726_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143726_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:53:30.94 +17:47:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.523 668289700010888448 118.37957751547 +17.80003095317 13.7780 13.4140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143821_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143821_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:08:28.04 +16:28:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.539 656499224508442496 122.11811182135 +16.46648367524 13.6855 13.2519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143825_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143825_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:53:15.35 +15:44:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143906_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143906_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:07:59.44 +14:19:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.353 653908156638281216 121.99797675041 +14.33141218308 13.7910 13.3390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143910_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 143910_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 143917_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143917_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:18:40.22 +18:31:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.704 657221088251660288 124.66755965592 +18.51780494184 14.0557 13.6053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143920_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143920_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:49:55.25 +16:34:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.996 667806739527286016 117.47936172493 +16.57042689417 13.8947 13.1837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143969_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143969_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:15:19.31 +15:42:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.695 655507327581111936 123.83006540085 +15.70077543074 13.8827 13.2966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143986_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143986_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:08:47.89 +12:52:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.665 650190639105753728 122.19961600204 +12.87982103649 14.2855 13.9101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143993_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143993_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:08:48.30 +16:43:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.065 656530251352082688 122.20156424676 +16.72303949267 13.9591 13.4851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143997_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 143997_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:14:55.15 +18:03:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.481 657099660937265920 123.73002550870 +18.05258665725 14.0760 13.5895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 144080_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 144080_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 144095_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 144095_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:04:38.87 +15:21:22.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)
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Considering the candidate 144096_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 144096_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 144280_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 144280_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:01:11.32 +10:24:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144380_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 144380_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:16:37.57 +15:00:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144440_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 144440_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:32:32.30 +16:49:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 3.772 658880212644562688 128.13472385233 +16.81846089820 14.2356 13.6085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 144692_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 144692_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 94727_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 94727_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 73846_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 73846_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 68457_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 68457_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 16361_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 16361_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:13:38.12 +10:11:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19207_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 19207_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:34:23.86 +10:05:24.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 61197_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 61197_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 99935_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 99935_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:21:42.76 +17:17:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48311_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 48311_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 07:33:30.79 +12:25:47.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 09933_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 09933_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 21500_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 21500_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 70812_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 70812_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:09:27.87 +14:39:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72747_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 72747_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 33589_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 33589_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:16:33.70 +11:43:35.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12253_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
Preparing report for the candidate 12253_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
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Considering the candidate 131889_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 131889_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
**** FOUND 08:27:41.50 +09:48:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.185 599927049155664512 126.92321450483 +09.81139536275 13.8170 13.3232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131833_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099
The candidate 131833_fd_Cnc-04-Q1b1x1_2026-04-06_00-30-16_20.00sec_-4.90C_LIGHTs_0099 did not pass the final checks
