This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p
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
NSVS 7030662,2461136.7181,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 7030662 20260406.2181 10.98CV 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 J063055.93+401700.7,2461136.7181,10.28,0.05,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 J063055.93+401700.7 20260406.2181 10.28CV 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
ATO J090.2982+40.1543,2461136.7181,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.2982+40.1543 20260406.2181 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.0482+34.4325,2461136.7181,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.0482+34.4325 20260406.2181 13.16CV 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
ATO J100.0545+34.9104,2461136.7181,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.0545+34.9104 20260406.2181 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.7181,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.2181 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7181,13.43,0.05,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 20260406.2181 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7181,13.53,0.05,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 20260406.2181 13.53CV 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,2461136.7181,13.85,0.05,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 20260406.2181 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
ATO J097.4911+35.8255,2461136.7181,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.4911+35.8255 20260406.2181 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 7165253,2461136.7181,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 7165253 20260406.2181 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060950.24+403538.2,2461136.7181,12.92,0.05,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 J060950.24+403538.2 20260406.2181 12.92CV 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
NSVS J0557029+362753,2461136.7181,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0557029+362753 20260406.2181 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0605325+350722,2461136.7181,12.88,0.05,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
NSVS J0605325+350722 20260406.2181 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0557292+373720,2461136.7181,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0557292+373720 20260406.2181 13.61CV 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
V0391 Aur,2461136.7181,10.08,0.05,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
V0391 Aur 20260406.2181 10.08CV 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 J062136.94+401753.5,2461136.7181,13.28,0.05,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 J062136.94+401753.5 20260406.2181 13.28CV 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
NSVS J0608537+363513,2461136.7181,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0608537+363513 20260406.2181 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 7010930,2461136.7181,12.64,0.05,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
NSVS 7010930 20260406.2181 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
[D2006] LCG23,2461136.7181,9.24,0.05,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
[D2006] LCG23 20260406.2181 9.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063314.49+343035.0,2461136.7181,12.24,0.05,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 J063314.49+343035.0 20260406.2181 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061622.17+362125.6,2461136.7181,13.00,0.05,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 J061622.17+362125.6 20260406.2181 13.00CV 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
NSVS J0602440+351939,2461136.7181,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0602440+351939 20260406.2181 11.65CV 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 J062147.45+383332.2,2461136.7181,13.43,0.05,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 J062147.45+383332.2 20260406.2181 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461136.71858046 06.04.2026 05:14:35.352 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
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: 12 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): 22488
Objects passed selection criteria: 22450
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 20135.2
Average stars matched: 19497.8 (96.8339 %)
Memory usage VmPeak: 125488 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 00:21:18 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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461136.71858046 06.04.2026 05:14:35.352 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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: 135 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): 151188
Objects passed selection criteria: 150853
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 121799
Average stars matched: 116719 (95.829 %)
Memory usage VmPeak: 1974724 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 00:26:00 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/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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: 2461136.71771749
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
Saving wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits'
wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:40.319 +38:01:01.49
Angular distance between the image centers 0.0211 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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:41.391 +38:00:21.65
Angular distance between the image centers 0.0102 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 06:32:40.319 +38:01:01.49
Second-epoch second image center 06:32:41.391 +38:00:21.65
Angular distance between the image centers 0.01161 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/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.z238T9WdYX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.oRTxs6P4h5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits &> /tmp/tmp.8OLZsHPePG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits &> /tmp/tmp.tYeZHLoZu9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 22646 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.2031 to 108.5019 deg, Dec +32.0173 to +43.3852 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 87.2031 to 108.5019 deg, Dec 32.0173 to 43.3852 deg
Loaded 14726 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): 10210 out of 11206 total matches.
Matched with Tycho-2 11206 out of 22646 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.945670
a=0.000000 b=1.000000 c=22.945670
From vast_summary.log: estimated ref. image limiting mag.: -7.66
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
4.2 pix fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
4.2 pix fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Limiting magnitude estimates:
15.3 mag. Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.3 mag. Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.6 mag. fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
14.6 mag. fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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.z238T9WdYX (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2024, passed=22646
Got 22646 stars (including 20590 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 22646 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 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 934 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: 932 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21763 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.oRTxs6P4h5 (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2057, passed=22538
Got 22538 stars (including 20456 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 22538 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 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 937 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: 934 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.8OLZsHPePG (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=951, passed=18016
Got 18016 stars (including 17060 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat
util/solve_plate_with_UCAC5 got 18016 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 929 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: 926 matched stars entering correct_measured_positions(), 918 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: 926 matched stars entering correct_measured_positions(), 17788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 17787 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 17787 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits -region wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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.tYeZHLoZu9 (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=912, passed=17853
Got 17853 stars (including 16932 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat
util/solve_plate_with_UCAC5 got 17853 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 927 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: 924 matched stars entering correct_measured_positions(), 917 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: 924 matched stars entering correct_measured_positions(), 17627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 17625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 17625 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits -region wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits'
Preparing the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16258.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31604_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31604_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:54:39.64 +40:33:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31634_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31634_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:28:01.80 +36:04:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31751_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31751_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:06:38.74 +37:57:55.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31788_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31788_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:52:42.49 +33:55:51.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31799_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31799_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:13:14.95 +40:11:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.242 946881516713718400 108.31237953353 +40.19071998607 11.4133 10.7326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31830_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31830_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:54:38.33 +36:34:05.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31886_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31886_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:08:53.74 +36:35:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 5.272 3453982261013510016 092.22283482291 +36.58540435669 10.9246 9.5233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31889_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31889_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:50:52.83 +37:33:12.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31902_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 31902_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:02:44.45 +35:19:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 3.118 3453437075044849408 090.68434961865 +35.32793540216 10.6735 9.2447 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32341_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 32341_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:01:40.11 +35:39:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.921 939891745201937024 105.41694194421 +35.65990266062 12.5236 12.0379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10384_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 10384_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16231_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 16231_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:01:07.37 +39:40:12.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16258_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 16258_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Aur-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 ####
06:02:30.82 +36:52:21.5
06:30:55.92 +40:16:59.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits exists and is non-empty
wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:40.319 +38:01:01.49
Angular distance between the image centers 0.0211 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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:41.391 +38:00:21.65
Angular distance between the image centers 0.0102 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 06:32:40.319 +38:01:01.49
Second-epoch second image center 06:32:41.391 +38:00:21.65
Angular distance between the image centers 0.01161 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/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.3uGbzMAwV2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.i6YDQy4CJ2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits &> /tmp/tmp.0fzi9T9Pww
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits &> /tmp/tmp.yOs9NWOkHE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 160824 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.1754 to 108.5197 deg, Dec +31.9766 to +43.3901 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 87.1754 to 108.5197 deg, Dec 31.9766 to 43.3901 deg
Loaded 14824 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): 8279 out of 11458 total matches.
Matched with Tycho-2 11458 out of 160824 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.794737
a=0.000000 b=1.000000 c=22.794737
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 93 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
1.9 pix Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
3.8 pix fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
3.8 pix fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Limiting magnitude estimates:
15.5 mag. Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.5 mag. Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.7 mag. fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
14.7 mag. fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 13.9 (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.3uGbzMAwV2 (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=18360, passed=160783
Got 160783 stars (including 142151 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 160783 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 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: 929 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 156528 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 156527 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 156528 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 928 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.i6YDQy4CJ2 (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=18627, passed=162435
Got 162435 stars (including 143499 good ones) from the SExtractor catalog wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 162435 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 935 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: 932 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 159044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 159044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 159044 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.0fzi9T9Pww (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=7589, passed=83842
Got 83842 stars (including 76200 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat
util/solve_plate_with_UCAC5 got 83842 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 926 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: 923 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 83169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 83169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 83170 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits -region wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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.yOs9NWOkHE (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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Checking if the catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat corresponding to the image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
WCS catalog name: wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=7383, passed=83257
Got 83257 stars (including 75814 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat
util/solve_plate_with_UCAC5 got 83257 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 925 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: 922 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 82632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 82633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 82634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits -region wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_Aur-04-Q1b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_Aur-04-Q1b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-13-20_20.00sec_-4.90C_LIGHTs_0084.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.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_Aur-04-Q1b1x1_001530_TTUQ1b1x1_9464_GQiMfB9p/wcs_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085.fits
Preparing the HTML report for the field Aur-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out104125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out131604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95476.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 26s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 17s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185692_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185692_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:15:06.59 +39:39:29.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185697_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185697_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:02:58.58 +36:36:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185709_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185709_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:41:51.09 +32:57:28.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185712_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185712_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:58:48.58 +38:22:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.599 3457815119889719040 089.70114150946 +38.36829098191 13.3683 12.4912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185713_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185713_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:25:56.57 +34:28:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.799 3440442737388984704 096.48697875473 +34.47558513398 14.2116 13.6626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185718_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185718_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:12:21.54 +37:15:43.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185720_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185720_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:11:09.58 +39:33:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.723 946836608535739264 107.78956660565 +39.56216039424 14.1535 13.6946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185722_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185722_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:05:10.42 +40:37:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.067 960413756073349376 091.29341806921 +40.62667583104 13.5127 12.9297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185741_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185741_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:57:27.92 +38:58:07.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185743_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185743_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:00:30.89 +38:36:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.268 3457446615994138112 090.12843731698 +38.60630180877 13.1593 12.5765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185744_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185744_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:02:47.58 +33:51:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.635 3451595667944602368 090.69848927955 +33.86250556700 13.2406 12.5074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185746_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185746_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185754_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185754_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:57:29.41 +34:36:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.003 3451847726688373504 089.37243464918 +34.60305944183 13.1794 12.5150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185756_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 185756_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185758_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 185758_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185765_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185765_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:14:07.40 +33:37:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.636 3452151539792648448 093.53068986438 +33.62870046479 13.1357 12.5980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185768_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 185768_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:01:19.53 +38:16:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.165 947008338507875456 105.33106581804 +38.28059137287 13.1172 12.5943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186303_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 186303_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:13:15.02 +40:11:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 0.827 946881516713718400 108.31237953353 +40.19071998607 11.4133 10.7326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186368_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 186368_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:54:38.37 +36:34:06.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186449_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 186449_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:50:52.95 +37:33:12.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186645_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 186645_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:42:32.69 +36:12:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.984 942090566594783360 100.63577605693 +36.20465652947 11.1259 9.7737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186670_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 186670_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:57:29.13 +37:23:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.795 940932334174069504 104.37144967043 +37.39317608856 12.1122 11.7116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187214_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 187214_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:32:09.92 +34:19:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187534_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 187534_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:01:18.81 +38:30:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.266 947019677221519616 105.32868457391 +38.50041173542 13.2650 11.1344 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187824_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 187824_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:17:39.47 +39:50:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.057 956429160294119808 094.41429103472 +39.83285506748 12.8257 12.0413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188028_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188028_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:59:23.74 +40:02:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.007 3458339380778900608 089.84993195227 +40.04350027872 13.2496 12.6453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188476_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188476_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:08:30.35 +41:02:24.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188502_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188502_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:11:52.83 +41:41:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.495 960200347738513920 092.96924329661 +41.69561680889 13.6661 13.0980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188528_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188528_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:28:04.40 +36:11:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.695 942828785574237184 097.01844758965 +36.18312154877 13.2973 12.5291 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188540_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188540_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:56:25.15 +33:37:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188553_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188553_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:59:43.73 +36:49:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.046 3456639849337435392 089.93241848812 +36.83268171479 13.3776 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188617_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188617_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:42:48.16 +40:06:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.498 945528460279928320 100.69976992903 +40.10738381638 13.8640 13.5051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188820_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 188820_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188847_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 188847_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188872_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 188872_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188954_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188954_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:34:24.66 +42:50:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.903 958853445994235008 098.60338007263 +42.84750692909 13.8453 13.3129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188965_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188965_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:54:03.94 +37:32:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.001 941090320251063168 103.51738573679 +37.54581486371 13.7777 13.2571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188997_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 188997_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:52:52.89 +38:52:33.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189021_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189021_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:42:21.57 +37:43:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.668 943920944216478464 100.58929406653 +37.71853222822 13.6675 13.0001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189022_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189022_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:12:54.10 +38:51:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.647 946746104985156992 108.22525825723 +38.85100378652 13.5418 13.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189042_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 189042_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189071_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189071_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:57:18.62 +33:39:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.986 939066909617870464 104.32796520503 +33.65564525503 13.8876 13.3573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189074_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189074_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:01:41.22 +39:50:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.809 947430035576650624 105.42246977960 +39.83344942669 13.9725 13.3255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189112_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189112_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:49:37.24 +34:06:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.683 938617793478608768 102.40503882778 +34.10946142319 13.5827 12.8262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189115_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189115_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:02:26.02 +36:21:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189121_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189121_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:00:57.69 +39:55:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.054 947435189537411072 105.23915698937 +39.92628772839 14.0552 13.4467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189178_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189178_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:07:44.31 +40:31:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.598 959671860602776704 091.93339636946 +40.52161614212 12.5733 10.7018 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189228_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189228_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:51:25.87 +41:46:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.078 951617491251931392 102.85733255307 +41.78386677139 13.8548 13.1289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189268_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189268_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:20:52.39 +43:06:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.090 961684173039804544 095.21797907260 +43.11327168205 13.5310 12.7858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189289_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189289_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:43:22.36 +37:01:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.741 943827004692012288 100.84267749313 +37.02440920383 13.4830 12.7221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189381_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189381_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:41:35.09 +35:57:30.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189440_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189440_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:19:31.74 +37:30:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.812 955158743327060736 094.88287000346 +37.49928452063 13.6817 13.1127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189453_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 189453_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189508_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189508_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:46:50.09 +40:15:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.781 945418960091083776 101.70920532785 +40.25162300814 13.9287 13.4228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189515_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189515_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:43:43.09 +42:38:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.814 963826846323452160 100.92779554385 +42.64059381719 13.9503 13.3576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189596_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 189596_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189697_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189697_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:31:48.81 +33:09:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189857_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189857_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:52:16.37 +35:09:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.586 940191740077691648 103.06847184943 +35.15914800441 14.0693 13.3479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189987_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 189987_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 07:12:59.03 +39:10:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.448 946768988570876672 108.24588819230 +39.17155464709 14.2113 13.7503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190199_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 190199_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:45:37.70 +37:28:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.706 943936852775553920 101.40652964588 +37.47588999360 14.1597 13.4739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190240_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 190240_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:57:23.50 +36:52:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 2.382 940901857086379392 104.34739174235 +36.87290543031 14.3115 13.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66497_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 66497_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131604_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 131604_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125587_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 125587_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:54:39.66 +40:33:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75651_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 75651_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:02:30.86 +36:52:21.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53350_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 53350_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:28:01.84 +36:04:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141066_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 141066_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:30:55.94 +40:16:59.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40251_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 40251_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:03:23.59 +34:45:31.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91158_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 91158_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:06:38.79 +37:57:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70961_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 70961_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33022_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 33022_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:18:22.95 +34:38:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45204_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 45204_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35275_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 35275_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:05:23.44 +34:27:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89538_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 89538_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49781_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 49781_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139889_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 139889_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:09:05.33 +39:58:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138649_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 138649_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67916_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 67916_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50442_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 50442_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127321_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 127321_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:15:48.73 +41:02:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43774_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 43774_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140924_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 140924_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:01:07.39 +39:40:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27922_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 27922_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09192_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 09192_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:38:32.17 +33:21:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83364_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 83364_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:43:42.56 +38:01:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61342_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 61342_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50060_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 50060_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95476_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
Preparing report for the candidate 95476_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10835_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 10835_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:17:14.45 +33:12:25.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104125_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 104125_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:06:44.09 +38:47:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.433 3457314605879491840 091.68412264631 +38.78508952853 13.6883 13.2182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171631_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 171631_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 05:58:23.91 +34:30:17.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171254_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 171254_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
**** FOUND 06:06:00.47 +36:20:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.896 3453614401357270400 091.50128751529 +36.34370976483 12.0369 10.2043 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80784_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085
The candidate 80784_fd_Aur-04-Q1b1x1_2026-04-06_00-14-35_20.00sec_-4.90C_LIGHTs_0085 did not pass the final checks
