This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW
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
V0484 Aur,2461136.7243,10.54,0.05,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
V0484 Aur 20260406.2243 10.54CV 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
GO Aur,2461136.7243,11.09,0.05,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
GO Aur 20260406.2243 11.09CV 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
V0494 Aur,2461136.7243,11.68,0.05,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
V0494 Aur 20260406.2243 11.68CV 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
AU Aur,2461136.7243,9.58,0.05,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
AU Aur 20260406.2243 9.58CV 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
AC Aur,2461136.7243,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AC Aur 20260406.2243 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
TX Cam,2461136.7243,10.29,0.05,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
TX Cam 20260406.2243 10.29CV 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,2461136.7243,14.04,0.05,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 20260406.2243 14.04CV 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 J079.9259+50.0461,2461136.7243,13.58,0.05,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 J079.9259+50.0461 20260406.2243 13.58CV 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 J051234.45+545151.9,2461136.7243,12.51,0.05,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 J051234.45+545151.9 20260406.2243 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J071.3491+55.1401,2461136.7243,13.06,0.05,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 J071.3491+55.1401 20260406.2243 13.06CV 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 J050937.96+560247.8,2461136.7243,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050937.96+560247.8 20260406.2243 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
V0507 Aur,2461136.7243,11.76,0.05,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
V0507 Aur 20260406.2243 11.76CV 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 J054136.03+524848.6,2461136.7243,11.81,0.05,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 J054136.03+524848.6 20260406.2243 11.81CV 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 J0507041+535141,2461136.7243,12.66,0.05,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 J0507041+535141 20260406.2243 12.66CV 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 4432199,2461136.7243,13.68,0.05,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 4432199 20260406.2243 13.68CV 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,2461136.7243,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2243 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J052608.36+501837.7,2461136.7243,12.94,0.05,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
ZTF J052608.36+501837.7 20260406.2243 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0449032+540251,2461136.7243,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0449032+540251 20260406.2243 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0539510+555305,2461136.7243,12.15,0.05,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 J0539510+555305 20260406.2243 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0492 Aur,2461136.7243,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0492 Aur 20260406.2243 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2259237,2461136.7243,9.83,0.05,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 2259237 20260406.2243 9.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J0517188+513740,2461136.7243,12.16,0.05,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
NSVS J0517188+513740 20260406.2243 12.16CV 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
NSVS 4415235,2461136.7243,12.94,0.05,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 4415235 20260406.2243 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0518182+501534,2461136.7243,13.05,0.05,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 J0518182+501534 20260406.2243 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0507259+534145,2461136.7243,12.72,0.05,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 J0507259+534145 20260406.2243 12.72CV 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 J0516398+535701,2461136.7243,10.80,0.05,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 J0516398+535701 20260406.2243 10.80CV 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
NSVS J0525270+500355,2461136.7243,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0525270+500355 20260406.2243 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0532372+501449,2461136.7243,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0532372+501449 20260406.2243 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
First image: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461136.72465856 06.04.2026 05:23:20.500 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 18
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 8 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): 20727
Objects passed selection criteria: 20651
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 17145.5
Average stars matched: 16529 (96.4043 %)
Memory usage VmPeak: 124296 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 00:25:25 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
First image: 2461049.69862881 09.01.2026 04:45:51.529 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461136.72465856 06.04.2026 05:23:20.500 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 120
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 175 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): 144636
Objects passed selection criteria: 144210
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 109976
Average stars matched: 105144 (95.6059 %)
Memory usage VmPeak: 1969764 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 00:30:57 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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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: 2461136.72391876
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
Saving wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits to local_wcs_cache/
'wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits exists and is non-empty
Saving wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits exists and is non-empty
Saving wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits to local_wcs_cache/
'wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits' -> 'local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits'
wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits exists and is non-empty
Saving wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits to local_wcs_cache/
'wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits' -> 'local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:49.946 +53:59:39.30
Angular distance between the image centers 0.0076 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 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:47.293 +53:59:40.38
Angular distance between the image centers 0.0013 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 05:38:49.946 +53:59:39.30
Second-epoch second image center 05:38:47.293 +53:59:40.38
Angular distance between the image centers 0.00651 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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.dHJmuifHxZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits &> /tmp/tmp.mTUb12uh8p
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits &> /tmp/tmp.vi9AWrAtVj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits &> /tmp/tmp.pHtqSFwkFV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat' -> 'wcsmag.cat'
Read 21171 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 69.2437 to 98.9738 deg, Dec +47.5207 to +59.4455 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 69.2437 to 98.9738 deg, Dec 47.5207 to 59.4455 deg
Loaded 11842 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): 7480 out of 8307 total matches.
Matched with Tycho-2 8307 out of 21171 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.946929
a=0.000000 b=1.000000 c=22.946929
From vast_summary.log: estimated ref. image limiting mag.: -7.50
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 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
2.0 pix Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
4.2 pix fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
4.2 pix fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Limiting magnitude estimates:
15.4 mag. Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
15.4 mag. Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
14.5 mag. fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
14.4 mag. fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.9 (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.dHJmuifHxZ (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1951, passed=21171
Got 21171 stars (including 19188 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 21171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 687 to 749 (Dec 47.5 to 59.4)
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: 936 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 687 to 749 (Dec 47.5 to 59.4)
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: 936 matched stars entering correct_measured_positions(), 20569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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.mTUb12uh8p (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1992, passed=21135
Got 21135 stars (including 19116 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 21135 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 687 to 749 (Dec 47.5 to 59.4)
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: 932 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 20585 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 687 to 749 (Dec 47.5 to 59.4)
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: 932 matched stars entering correct_measured_positions(), 20584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 20584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits -region wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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.vi9AWrAtVj (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=659, passed=13436
Got 13436 stars (including 12772 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat
util/solve_plate_with_UCAC5 got 13436 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 688 to 748 (Dec 47.7 to 59.4)
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: 934 matched stars entering correct_measured_positions(), 929 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: 934 matched stars entering correct_measured_positions(), 13337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 936 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(), 13335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 13335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits -region wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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.pHtqSFwkFV (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=668, passed=13301
Got 13301 stars (including 12625 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat
util/solve_plate_with_UCAC5 got 13301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 688 to 748 (Dec 47.7 to 59.4)
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: 936 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 13187 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 13185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 13185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits -region wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
Saving fully-calibrated image wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits'
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits'
Preparing the HTML report for the field Aur-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17026.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
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Considering the candidate 31323_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 31323_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:09:06.90 +51:47:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 1.219 971915128735113216 092.27840343477 +51.79731752041 10.3963 10.0575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31787_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 31787_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:25:04.46 +51:46:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31800_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 31800_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:28:51.90 +52:06:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.852 992435039366525312 097.21603483249 +52.11044256723 11.4729 11.0713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31827_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 31827_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:36:46.17 +54:26:37.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31875_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 31875_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:29:56.11 +51:37:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.967 262038639086513792 082.48300676844 +51.62669155887 11.0832 9.5310 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32039_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 32039_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:41:36.03 +52:48:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 2.681 263684333114513024 085.40017663140 +52.81346641748 10.9847 9.5646 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32077_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 32077_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:38:21.25 +50:18:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32179_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 32179_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:17:31.84 +52:10:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32239_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 32239_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:33:00.92 +54:58:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.700 994669277057385600 098.25349455650 +54.98072526832 12.1303 11.7247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 12298_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 12298_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
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Considering the candidate 04199_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 04199_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13894_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 13894_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05858_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 05858_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15065_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 15065_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:46:25.65 +54:28:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04099_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 04099_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17026_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 17026_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07284_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 07284_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:03:16.52 +50:51:47.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Aur-01-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 ####
05:27:04.41 +50:07:28.6
06:26:01.53 +50:29:30.9
04:54:15.49 +49:54:02.5
05:13:20.03 +53:54:41.7
06:00:30.98 +55:27:13.6
05:00:51.86 +56:10:51.2
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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Creating symlink local_wcs_cache/wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits exists and is non-empty
wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits exists and is non-empty
wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:49.946 +53:59:39.30
Angular distance between the image centers 0.0076 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 05:38:46.898 +53:59:43.50
Second-epoch image center 05:38:47.293 +53:59:40.38
Angular distance between the image centers 0.0013 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 05:38:49.946 +53:59:39.30
Second-epoch second image center 05:38:47.293 +53:59:40.38
Angular distance between the image centers 0.00651 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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.UuYri0WMiD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits &> /tmp/tmp.JJRghX3vyL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits &> /tmp/tmp.yOSZCj7fZS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits &> /tmp/tmp.Y2nDREmele
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat' -> 'wcsmag.cat'
Read 155080 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 69.1098 to 99.0219 deg, Dec +47.5207 to +59.4472 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 69.1098 to 99.0219 deg, Dec 47.5207 to 59.4472 deg
Loaded 11908 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): 6184 out of 8396 total matches.
Matched with Tycho-2 8396 out of 155080 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.800893
a=0.000000 b=1.000000 c=22.800893
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 104 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
1.9 pix Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
3.7 pix fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
3.7 pix fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Limiting magnitude estimates:
15.6 mag. Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
15.6 mag. Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
14.5 mag. fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
14.5 mag. fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
All-image limiting magnitude estimate: 14.5 (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.UuYri0WMiD (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=52, blended=17009, passed=155028
Got 155028 stars (including 137750 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 155028 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 687 to 749 (Dec 47.5 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 153042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 687 to 749 (Dec 47.5 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 153041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 153039 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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.JJRghX3vyL (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits' -> 'wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Checking if the catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat corresponding to the image wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
WCS catalog name: wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=17172, passed=155797
Got 155797 stars (including 138353 good ones) from the SExtractor catalog wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 155797 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 687 to 749 (Dec 47.5 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 152852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 687 to 749 (Dec 47.5 to 59.4)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 152853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 152849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits -region wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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.yOSZCj7fZS (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=4864, passed=66258
Got 66258 stars (including 61340 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat
util/solve_plate_with_UCAC5 got 66258 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 939 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: 938 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 65771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 65771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 65771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits -region wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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.Y2nDREmele (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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=4816, passed=65698
Got 65698 stars (including 60825 good ones) from the SExtractor catalog wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat
util/solve_plate_with_UCAC5 got 65698 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 688 to 748 (Dec 47.7 to 59.4)
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: 936 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 65063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 65063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 65063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits -region wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_Aur-01-Q1b1x1_2026-01-08_22-45-51_20.00sec_-15.00C_LIGHT_0173.fits
Saving fully-calibrated image wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_Aur-01-Q1b1x1_2026-01-08_22-46-33_20.00sec_-14.90C_LIGHT_0174.fits
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-22-16_20.00sec_-4.90C_LIGHTs_0092.fits
Saving fully-calibrated image wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.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-01-Q1b1x1_002415_TTUQ1b1x1_785_P32FyUzW/wcs_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093.fits
Preparing the HTML report for the field Aur-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out136027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out15915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out179987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out180550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out181905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out130580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out141855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98166.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 9s
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Considering the candidate 179447_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179447_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:20:17.91 +51:42:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179450_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179450_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:51:47.09 +56:42:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.028 274662303884805120 072.94680894411 +56.70459881413 13.6406 12.9636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179451_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179451_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:26:23.67 +52:37:33.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
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Considering the candidate 179455_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179455_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:30:03.67 +52:23:07.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
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Considering the candidate 179457_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179457_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:31:00.92 +54:58:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.421 994590013437123328 097.75390249059 +54.97633713865 13.7815 13.2142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179460_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179460_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:50:09.66 +53:59:57.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 179467_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179467_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:53:41.17 +51:24:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.342 259889196933863808 073.42175512872 +51.40734631818 13.0266 12.3914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179475_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179475_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:06:27.35 +57:30:29.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 179480_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179480_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:00:04.18 +58:00:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.654 280768506130951680 075.01847106328 +58.00519515157 13.3342 12.2700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179482_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179482_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:52:02.83 +56:33:16.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 179486_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179486_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:07:00.49 +58:22:01.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 179491_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179491_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:24:38.75 +50:19:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.994 971119181099438080 096.16166680246 +50.32646415030 13.4093 12.9234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179492_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179492_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:02:29.63 +49:51:32.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 179493_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179493_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:55:27.79 +49:10:58.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 179497_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179497_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:29:12.42 +54:07:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179499_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179499_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:11:29.06 +57:01:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 179565_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179565_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:59:32.22 +58:25:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.13, MAG_FAINT_SEARCH_LIMIT=10.11)GAIADR2_OUTPUT=# 2.523 283841714146631936 074.88337423918 +58.42761346186 8.6846 7.6974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179983_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179983_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:29:44.88 +59:09:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 2.546 281857233098228992 082.43669242552 +59.15771716869 10.3810 8.9784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 179987_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 179987_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:28:51.89 +52:06:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.491 992435039366525312 097.21603483249 +52.11044256723 11.4729 11.0713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180103_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 180103_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:29:55.73 +51:37:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 180550_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 180550_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:36:44.55 +54:23:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.321 264918844154100480 084.18576485139 +54.39392507302 11.8056 10.8338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181021_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181021_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:34:03.62 +56:25:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.479 995136878737304576 098.51578923933 +56.41879432732 12.6884 12.0495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181076_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181076_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 181246_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181246_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:11:44.53 +54:17:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181509_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181509_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:12:10.40 +50:14:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.937 971692301536466048 093.04186881097 +50.24848156099 13.4393 12.9237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 181648_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181648_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:56:15.91 +52:52:55.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181806_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181806_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:47:00.24 +56:56:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181831_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181831_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:11:35.78 +52:39:14.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181871_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181871_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:52:07.01 +49:32:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.339 211244191180147968 088.02792423332 +49.54687980867 13.2983 12.6336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 181877_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181877_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:59:46.40 +55:17:33.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181905_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 181905_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:06:22.70 +55:21:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.718 279381717028489472 076.59325600329 +55.35221616126 12.9586 11.9655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182109_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182109_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:34:08.76 +56:32:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.498 995233159021292800 098.53651856210 +56.53397144241 13.2760 12.6880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182247_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182247_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:52:03.91 +49:32:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.831 211244191180148352 088.01550768143 +49.54892102579 13.3825 12.6034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182282_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182282_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:25:10.23 +56:43:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.734 998208471845148672 096.29126529159 +56.72547485073 13.6151 12.8662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182373_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182373_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:40:14.27 +50:00:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182448_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182448_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:39:25.77 +52:43:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.200 263691548659363456 084.85594508721 +52.72710512436 13.3191 12.4350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182476_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182476_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:19:02.08 +56:30:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.754 998044129216427392 094.75578843059 +56.50771081848 13.8774 13.3409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182573_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182573_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:34:00.16 +56:51:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.129 269204530025667968 083.49976764186 +56.86489304848 13.5024 12.8462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182635_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182635_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:00:46.21 +56:55:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182707_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182707_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:13:11.59 +53:10:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.661 996435131388354816 093.30089759080 +53.17787779392 13.9599 13.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182837_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182837_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:24:06.74 +55:41:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.606 997684451474732416 096.02770276391 +55.69183025610 13.9120 13.3120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182841_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182841_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:53:08.95 +50:16:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.501 211522573779759616 088.28546899307 +50.27832306218 13.9989 13.3902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182867_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182867_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:42:06.61 +54:48:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.622 264858160559896064 085.52797222088 +54.80217641092 13.6919 13.0786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182902_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182902_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:09:12.77 +56:22:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.524 997258764380573824 092.30195571984 +56.38409093408 13.6916 13.0101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182971_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182971_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:32:50.13 +50:34:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.868 215329804590479232 083.20880219627 +50.57276672158 13.7737 13.2194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182997_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 182997_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:47:49.42 +51:04:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.938 214838937071416704 086.95477035927 +51.07718960466 13.8637 13.3461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183181_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183181_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 183246_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183246_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:49:01.87 +51:43:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.171 215625745016344320 087.25940310779 +51.72621727915 13.6330 12.7320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183255_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183255_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 183334_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183334_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:22:05.18 +54:39:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 2.882 996291232804030208 095.52030777344 +54.66477278523 14.5342 13.9547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183342_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183342_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:08:03.87 +57:49:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183384_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183384_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:57:24.96 +49:14:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.932 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183517_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 183517_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
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Considering the candidate 183537_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183537_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:12:36.66 +53:51:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.861 266258427275275904 078.15206594535 +53.85056591448 13.9052 13.0287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183546_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183546_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:34:51.23 +57:27:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.167 1001292086565277696 098.71317067710 +57.46066824985 14.1480 13.6073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183621_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183621_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 183704_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183704_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 183763_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 183763_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:12:48.77 +54:54:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.411 997014230418254464 093.20347509726 +54.91074950448 14.2941 13.7782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59734_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 59734_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:06:40.74 +51:35:52.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95529_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 95529_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:57:17.28 +53:45:10.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88867_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 88867_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:36:35.17 +54:25:44.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165659_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 165659_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165886_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 165886_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:43:59.96 +57:27:53.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165890_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 165890_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:20:55.52 +49:27:40.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148333_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 148333_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51762_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 51762_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:03:16.52 +50:51:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131670_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 131670_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29073_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 29073_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:27:04.38 +50:07:28.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 140800_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 140800_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:46:25.63 +54:28:49.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130580_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 130580_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88976_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 88976_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66885_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 66885_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124117_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 124117_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:00:51.87 +56:10:51.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94357_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 94357_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69604_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 69604_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 150174_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 150174_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:00:30.99 +55:27:13.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136027_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 136027_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:13:23.80 +55:49:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.347 267775272285297152 078.34826197016 +55.82238034034 12.4353 10.9261 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56402_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 56402_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133856_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 133856_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:19:56.83 +56:05:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153163_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 153163_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:32:40.24 +58:57:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31829_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 31829_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91599_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 91599_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:13:20.08 +53:54:41.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148807_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 148807_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51083_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 51083_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:59:37.55 +50:43:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50775_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 50775_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:25:04.44 +51:46:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141855_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 141855_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56837_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 56837_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98166_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 98166_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27904_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 27904_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:38:21.23 +50:18:57.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57109_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 57109_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69531_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 69531_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42001_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 42001_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:54:15.43 +49:54:02.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33827_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 33827_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91864_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 91864_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90917_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 90917_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27559_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 27559_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121974_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 121974_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:19:48.09 +57:15:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28410_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
Preparing report for the candidate 28410_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15915_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 15915_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:01:29.37 +49:50:27.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29380_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 29380_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 06:26:01.49 +50:29:31.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24830_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 24830_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:15:58.02 +49:32:49.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84710_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 84710_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:59:31.34 +54:17:03.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112359_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 112359_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 05:23:28.21 +57:32:34.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119880_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093
The candidate 119880_fd_Aur-01-Q1b1x1_2026-04-06_00-23-20_20.00sec_-4.90C_LIGHTs_0093 did not pass the final checks
**** FOUND 04:48:00.43 +56:45:23.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 31s
Prepared the HTML report for the field Aur-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:27:04.41 +50:07:28.6
06:26:01.53 +50:29:30.9
04:54:15.49 +49:54:02.5
05:13:20.03 +53:54:41.7
06:00:30.98 +55:27:13.6
05:00:51.86 +56:10:51.2
05:09:38.15 +56:02:47.2
04:45:27.47 +55:08:13.0
05:39:50.95 +55:53:05.5
05:12:34.70 +54:51:53.7
04:49:03.81 +54:02:32.0
05:19:38.61 +50:03:01.9
06:01:17.82 +54:42:38.1
05:25:25.76 +50:04:05.7
05:32:37.13 +50:14:48.0
05:26:08.35 +50:18:37.8
05:18:18.04 +50:15:34.2
04:59:27.82 +51:03:18.3
05:36:56.73 +52:02:31.3
05:17:19.05 +51:37:36.5
05:41:35.94 +52:48:43.8
05:05:49.73 +52:09:59.2
05:24:18.55 +52:39:28.0
05:51:49.43 +54:21:40.7
05:16:39.81 +53:56:59.8
05:07:26.08 +53:41:44.7
05:07:04.20 +53:51:40.8
05:35:38.88 +54:54:32.7
########### Completed Aur-01-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:13:20.03 +53:54:41.7
06:26:01.53 +50:29:30.9
06:00:30.98 +55:27:13.6
04:54:15.49 +49:54:02.5
05:27:04.41 +50:07:28.6
05:00:51.86 +56:10:51.2
06:01:17.82 +54:42:38.1
05:19:38.61 +50:03:01.9
05:12:34.70 +54:51:53.7
04:45:27.47 +55:08:13.0
05:09:38.15 +56:02:47.2
05:51:49.43 +54:21:40.7
05:41:35.94 +52:48:43.8
05:07:04.20 +53:51:40.8
05:24:18.55 +52:39:28.0
04:59:27.82 +51:03:18.3
05:26:08.35 +50:18:37.8
04:49:03.81 +54:02:32.0
05:39:50.95 +55:53:05.5
05:36:56.73 +52:02:31.3
05:35:38.88 +54:54:32.7
05:17:19.05 +51:37:36.5
05:05:49.73 +52:09:59.2
05:18:18.04 +50:15:34.2
05:07:26.08 +53:41:44.7
05:16:39.81 +53:56:59.8
05:25:25.76 +50:04:05.7
05:32:37.13 +50:14:48.0
###################################################################################
05:13:20.03 +53:54:41.7 -- not an asteroid (will add it to exclusion list)
06:26:01.53 +50:29:30.9 -- not an asteroid (will add it to exclusion list)
06:00:30.98 +55:27:13.6 -- not an asteroid (will add it to exclusion list)
04:54:15.49 +49:54:02.5 -- not an asteroid (will add it to exclusion list)
05:27:04.41 +50:07:28.6 -- not an asteroid (will add it to exclusion list)
05:00:51.86 +56:10:51.2 -- not an asteroid (will add it to exclusion list)
06:01:17.82 +54:42:38.1 -- not an asteroid (will add it to exclusion list)
05:19:38.61 +50:03:01.9 -- not an asteroid (will add it to exclusion list)
05:12:34.70 +54:51:53.7 -- not an asteroid (will add it to exclusion list)
04:45:27.47 +55:08:13.0 -- not an asteroid (will add it to exclusion list)
05:09:38.15 +56:02:47.2 -- not an asteroid (will add it to exclusion list)
05:51:49.43 +54:21:40.7 -- not an asteroid (will add it to exclusion list)
05:41:35.94 +52:48:43.8 -- not an asteroid (will add it to exclusion list)
05:07:04.20 +53:51:40.8 -- not an asteroid (will add it to exclusion list)
05:24:18.55 +52:39:28.0 -- not an asteroid (will add it to exclusion list)
04:59:27.82 +51:03:18.3 -- not an asteroid (will add it to exclusion list)
05:26:08.35 +50:18:37.8 -- not an asteroid (will add it to exclusion list)
04:49:03.81 +54:02:32.0 -- not an asteroid (will add it to exclusion list)
05:39:50.95 +55:53:05.5 -- not an asteroid (will add it to exclusion list)
05:36:56.73 +52:02:31.3 -- not an asteroid (will add it to exclusion list)
05:35:38.88 +54:54:32.7 -- not an asteroid (will add it to exclusion list)
05:17:19.05 +51:37:36.5 -- not an asteroid (will add it to exclusion list)
05:05:49.73 +52:09:59.2 -- not an asteroid (will add it to exclusion list)
05:18:18.04 +50:15:34.2 -- not an asteroid (will add it to exclusion list)
05:07:26.08 +53:41:44.7 -- not an asteroid (will add it to exclusion list)
05:16:39.81 +53:56:59.8 -- not an asteroid (will add it to exclusion list)
05:25:25.76 +50:04:05.7 -- not an asteroid (will add it to exclusion list)
05:32:37.13 +50:14:48.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:45:27.47 +55:08:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:03.81 +54:02:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:15.49 +49:54:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:27.82 +51:03:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:51.86 +56:10:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:49.73 +52:09:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:04.20 +53:51:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:26.08 +53:41:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:38.15 +56:02:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:34.70 +54:51:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:20.03 +53:54:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:39.81 +53:56:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:19.05 +51:37:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:18.04 +50:15:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:38.61 +50:03:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:18.55 +52:39:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:25.76 +50:04:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:08.35 +50:18:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.41 +50:07:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:37.13 +50:14:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:38.88 +54:54:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:56.73 +52:02:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:50.95 +55:53:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:35.94 +52:48:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:49.43 +54:21:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:30.98 +55:27:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:17.82 +54:42:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:01.53 +50:29:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:45:27.47 +55:08:13.0 -- not a known variable star
04:49:03.81 +54:02:32.0 -- a known variable star
04:54:15.49 +49:54:02.5 -- a known variable star
04:59:27.82 +51:03:18.3 -- not a known variable star
05:00:51.86 +56:10:51.2 -- a known variable star
05:05:49.73 +52:09:59.2 -- a known variable star
05:07:04.20 +53:51:40.8 -- a known variable star
05:07:26.08 +53:41:44.7 -- a known variable star
05:09:38.15 +56:02:47.2 -- a known variable star
05:12:34.70 +54:51:53.7 -- a known variable star
05:13:20.03 +53:54:41.7 -- a known variable star
05:16:39.81 +53:56:59.8 -- a known variable star
05:17:19.05 +51:37:36.5 -- a known variable star
05:18:18.04 +50:15:34.2 -- a known variable star
05:19:38.61 +50:03:01.9 -- not a known variable star
05:24:18.55 +52:39:28.0 -- a known variable star
05:25:25.76 +50:04:05.7 -- a known variable star
05:26:08.35 +50:18:37.8 -- a known variable star
05:27:04.41 +50:07:28.6 -- a known variable star
05:32:37.13 +50:14:48.0 -- a known variable star
05:35:38.88 +54:54:32.7 -- a known variable star
05:36:56.73 +52:02:31.3 -- a known variable star
05:39:50.95 +55:53:05.5 -- a known variable star
05:41:35.94 +52:48:43.8 -- a known variable star
05:51:49.43 +54:21:40.7 -- a known variable star
06:00:30.98 +55:27:13.6 -- a known variable star
06:01:17.82 +54:42:38.1 -- not a known variable star
06:26:01.53 +50:29:30.9 -- a known variable star
Found 4 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
28 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
04:45:27.47 +55:08:13.0
04:49:03.81 +54:02:32.0
04:54:15.49 +49:54:02.5
04:59:27.82 +51:03:18.3
05:00:51.86 +56:10:51.2
05:05:49.73 +52:09:59.2
05:07:04.20 +53:51:40.8
05:07:26.08 +53:41:44.7
05:09:38.15 +56:02:47.2
05:12:34.70 +54:51:53.7
05:13:20.03 +53:54:41.7
05:16:39.81 +53:56:59.8
05:17:19.05 +51:37:36.5
05:18:18.04 +50:15:34.2
05:19:38.61 +50:03:01.9
05:24:18.55 +52:39:28.0
05:25:25.76 +50:04:05.7
05:26:08.35 +50:18:37.8
05:27:04.41 +50:07:28.6
05:32:37.13 +50:14:48.0
05:35:38.88 +54:54:32.7
05:36:56.73 +52:02:31.3
05:39:50.95 +55:53:05.5
05:41:35.94 +52:48:43.8
05:51:49.43 +54:21:40.7
06:00:30.98 +55:27:13.6
06:01:17.82 +54:42:38.1
06:26:01.53 +50:29:30.9
06:09:06.90 +51:47:49.4
06:28:51.90 +52:06:38.3
05:29:56.11 +51:37:35.2
05:41:36.03 +52:48:45.8
06:33:00.92 +54:58:50.6
05:13:23.80 +55:49:19.1
06:01:29.37 +49:50:27.6
04:43:59.96 +57:27:53.4
04:51:47.09 +56:42:18.2
06:26:23.67 +52:37:33.1
05:30:03.67 +52:23:07.6
06:31:00.92 +54:58:33.4
05:50:09.66 +53:59:57.8
04:53:41.17 +51:24:27.7
05:06:27.35 +57:30:29.1
05:00:04.18 +58:00:22.9
04:52:02.83 +56:33:16.1
05:07:00.49 +58:22:01.2
06:24:38.75 +50:19:34.4
06:02:29.63 +49:51:32.4
04:55:27.79 +49:10:58.2
04:59:32.22 +58:25:37.5
05:29:44.88 +59:09:25.3
06:28:51.89 +52:06:37.9
05:36:44.55 +54:23:38.0
06:34:03.62 +56:25:07.2
06:12:10.40 +50:14:52.5
05:52:07.01 +49:32:47.3
05:06:22.70 +55:21:07.9
06:34:08.76 +56:32:00.8
05:52:03.91 +49:32:56.1
06:25:10.23 +56:43:31.2
05:39:25.77 +52:43:38.3
06:19:02.08 +56:30:28.4
05:34:00.16 +56:51:54.8
06:13:11.59 +53:10:39.7
06:24:06.74 +55:41:28.1
05:53:08.95 +50:16:43.6
05:42:06.61 +54:48:10.3
06:09:12.77 +56:22:57.8
05:32:50.13 +50:34:20.1
05:47:49.42 +51:04:36.5
05:49:01.87 +51:43:36.5
06:22:05.18 +54:39:54.3
05:57:24.96 +49:14:29.9
05:12:36.66 +53:51:03.2
06:34:51.23 +57:27:40.5
06:12:48.77 +54:54:37.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.72391876 -observatory V36
23:20:32.64 -06:24:54.7 Mercury (0.3mag)
02:21:38.64 +13:51:50.1 Venus (-3.9mag)
23:49:59.67 -02:12:01.7 Mars (1.2mag)
07:08:42.85 +22:52:25.8 Jupiter (-2.2mag)
00:24:46.50 +00:21:18.6 Saturn (0.9mag)
03:45:43.70 +19:41:06.7 Uranus (5.8mag)
00:09:32.02 -00:23:38.8 Neptune (7.8mag)
20:33:14.28 -22:52:29.3 Pluto (14.5mag)
16:00:36.61 -26:15:28.6 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 6 00:25 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461136.72391876:
07:08:45.98 +22:52:16.8 Io (5.7mag)
07:08:55.48 +22:51:59.2 Europa (5.8mag)
07:08:37.75 +22:52:43.0 Ganymede (5.3mag)
07:08:12.95 +22:53:17.6 Callisto (6.5mag)
07:12:25.74 +22:44:54.9 Himalia (15.3mag)
07:08:40.97 +22:52:31.6 Thebe (16.2mag)
07:12:23.47 +23:13:41.4 Elara (17.2mag)
07:06:55.80 +23:37:33.2 Pasiphae (17.3mag)
07:17:14.63 +22:49:22.1 Carme (18.4mag)
00:24:41.27 +00:21:19.7 Titan (8.8mag)
00:24:43.27 +00:21:32.7 Rhea (10.1mag)
00:24:47.01 +00:22:51.9 Iapetus (11.5mag)
00:24:48.38 +00:21:06.9 Hyperion (14.8mag)
00:26:30.71 +00:31:07.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 00:25 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.72391876:
14:47:25.48 -08:21:06.6 JWST
17:03:04.34 +44:49:37.7 Chandra
08:04:14.58 -39:47:02.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 00:25 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.72391876 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:08.67 -28:14:13.8 14.0mag P/2010 H2 (Vales)
05:00:06.37 -70:08:46.5 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:34.48 +31:22:34.2 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.73 +09:22:26.5 17.6mag C/2021 G2 (ATLAS)
23:07:21.74 +28:52:09.0 17.0mag C/2022 E2 (ATLAS)
04:18:01.72 +25:45:54.8 15.9mag C/2022 N2 (PANSTARRS)
09:01:52.13 +31:54:25.6 16.1mag C/2022 QE78 (ATLAS)
08:29:59.31 -01:13:44.3 17.3mag C/2022 R6 (PANSTARRS)
18:55:35.09 +17:41:51.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:30.18 -11:39:36.3 17.6mag P/2023 B1 (PANSTARRS)
09:12:49.03 -13:29:51.7 17.5mag C/2023 F3 (ATLAS)
21:43:30.85 +62:22:22.4 17.5mag C/2023 H5 (Lemmon)
19:26:23.51 -03:36:31.8 14.3mag C/2023 R1 (PANSTARRS)
21:42:38.40 +84:36:53.8 17.8mag C/2023 X2 (Lemmon)
06:14:32.14 +63:35:00.2 17.0mag C/2024 A1 (ATLAS)
04:51:08.57 +14:34:11.3 10.4mag C/2024 E1 (Wierzchos)
16:25:05.13 +04:46:59.1 17.4mag C/2024 G6 (ATLAS)
20:17:33.69 +12:41:30.7 14.7mag C/2024 J3 (ATLAS)
03:17:47.64 -23:55:03.7 16.4mag C/2024 T5 (ATLAS)
05:08:43.77 +47:49:33.4 17.7mag C/2025 J1 (Borisov)
14:18:58.46 +37:25:26.7 14.8mag C/2025 L1 (ATLAS)
03:10:24.92 -24:45:12.8 17.8mag C/2025 Q3 (ATLAS)
22:53:39.72 +19:50:14.1 10.1mag C/2025 R3 (PANSTARRS)
12:58:22.66 +02:23:39.5 17.5mag C/2025 Y1 (ATLAS)
01:31:36.87 +04:42:01.4 7.2mag C/2026 A1 (MAPS)
23:30:54.35 +35:15:03.6 14.3mag C/2026 B2 (Sun-Gao)
18:23:51.27 -10:13:00.7 12.4mag 10P/Tempel
15:12:51.90 +04:06:34.2 13.1mag 24P/Schaumasse
11:05:45.60 -01:51:45.4 15.7mag 29P/Schwassmann-Wachmann
17:56:46.84 -09:59:30.1 17.7mag 40P/Vaisala
10:38:52.58 -04:56:42.5 16.7mag 43P/Wolf-Harrington
01:33:36.14 +15:48:06.3 17.1mag 47P/Ashbrook-Jackson
06:53:23.18 +39:04:26.8 17.0mag 63P/Wild
23:16:21.10 -12:39:03.5 15.7mag 65P/Gunn
03:37:45.57 +17:44:59.9 15.8mag 76P/West-Kohoutek-Ikemura
00:44:09.00 +06:17:29.8 14.4mag 78P/Gehrels
22:32:39.11 -12:15:43.4 14.5mag 88P/Howell
01:43:15.58 +17:57:23.7 15.1mag 93P/Lovas
04:36:58.97 +31:43:48.9 16.3mag 123P/West-Hartley
08:17:57.70 +42:52:33.2 16.2mag 124P/Mrkos
02:18:16.00 +13:15:38.6 16.4mag 128P/Shoemaker-Holt
02:28:27.68 +13:15:28.6 17.5mag 131P/Mueller
00:36:02.64 +09:37:21.6 11.2mag 141P/Machholz
00:46:00.95 +01:12:43.1 11.3mag 141P-A/Machholz
23:36:33.97 -02:24:45.8 14.0mag 141P-D/Machholz
01:15:08.54 +02:52:37.9 17.9mag 141P-I/Machholz
00:35:13.63 -06:24:06.5 15.2mag 162P/SidingSpring
10:30:57.95 +31:30:16.1 17.8mag 164P/Christensen
06:18:29.33 +24:31:20.4 17.8mag 198P/ODAS
15:08:38.73 -01:11:29.6 17.4mag 210P/Christensen
21:09:01.19 -13:48:48.9 17.4mag 218P/LINEAR
17:12:37.31 -15:04:10.2 16.2mag 235P/LINEAR
05:13:43.61 +33:51:32.9 16.6mag 240P/NEAT
07:34:12.78 -06:16:59.1 17.6mag 242P/Spahr
15:45:55.78 +06:18:41.7 17.5mag 391P/Kowalski
07:30:55.62 +21:18:42.8 17.6mag 450P/LONEOS
05:21:57.69 +45:36:33.7 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 00:25 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 6 00:25 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 6 00:25 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
13:18:12.570 +29:05:16.56 AT 2026htq 2026-03-15.74 21.89
-rw-r--r-- 1 apache apache 30K Apr 6 00:25 tns_transients_list.txt
