This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RS Aur,2461139.6709,8.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RS Aur 20260409.1709 8.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AC Aur,2461139.6709,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AC Aur 20260409.1709 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.1430+41.9949,2461139.6709,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.1430+41.9949 20260409.1709 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963194489700296960,2461139.6709,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963194489700296960 20260409.1709 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.1299+41.0860,2461139.6709,13.18,0.05,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 J087.1299+41.0860 20260409.1709 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.4955+49.4786,2461139.6709,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.4955+49.4786 20260409.1709 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,13.07,0.05,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 20260409.1709 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.80,0.05,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
target 20260409.1709 12.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0655+44.9865,2461139.6709,12.86,0.05,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 J088.0655+44.9865 20260409.1709 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.94,0.05,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
target 20260409.1709 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.0609+41.2432,2461139.6709,12.81,0.05,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
ATO J086.0609+41.2432 20260409.1709 12.81CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.66,0.05,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
target 20260409.1709 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.3673+41.8196,2461139.6709,12.74,0.05,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 J095.3673+41.8196 20260409.1709 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.9474+50.2407,2461139.6709,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.9474+50.2407 20260409.1709 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194712136209681664,2461139.6709,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194712136209681664 20260409.1709 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.34,0.05,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 20260409.1709 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194505775916838272,2461139.6709,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194505775916838272 20260409.1709 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.6709,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.1709 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212655861031529216,2461139.6709,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212655861031529216 20260409.1709 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.29,0.05,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
target 20260409.1709 12.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.6798+40.3467,2461139.6709,12.55,0.05,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 J099.6798+40.3467 20260409.1709 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.37,0.05,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 20260409.1709 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6086+42.9942,2461139.6709,12.38,0.05,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 J084.6086+42.9942 20260409.1709 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967525667862574848,2461139.6709,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967525667862574848 20260409.1709 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.52,0.05,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 20260409.1709 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.9429+41.4474,2461139.6709,12.49,0.05,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 J080.9429+41.4474 20260409.1709 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 958053585643972736,2461139.6709,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 958053585643972736 20260409.1709 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.7523+42.9146,2461139.6709,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.7523+42.9146 20260409.1709 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.54,0.05,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
target 20260409.1709 12.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1606+41.4155,2461139.6709,12.76,0.05,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
ATO J089.1606+41.4155 20260409.1709 12.76CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.76,0.05,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
target 20260409.1709 12.76CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4452455,2461139.6709,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4452455 20260409.1709 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052211.91+413349.4,2461139.6709,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J052211.91+413349.4 20260409.1709 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.5580+44.6536,2461139.6709,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J080.5580+44.6536 20260409.1709 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J052600.42+411515.0,2461139.6709,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J052600.42+411515.0 20260409.1709 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VY Aur,2461139.6709,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VY Aur 20260409.1709 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060014.41+450400.4,2461139.6709,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J060014.41+450400.4 20260409.1709 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 02922-01985,2461139.6709,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 02922-01985 20260409.1709 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CGCS 6107,2461139.6709,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CGCS 6107 20260409.1709 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.6709,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.1709 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0546556+483237,2461139.6709,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0546556+483237 20260409.1709 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052315.65+472910.7,2461139.6709,11.51,0.05,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 J052315.65+472910.7 20260409.1709 11.51CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4521908,2461139.6709,10.37,0.05,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 4521908 20260409.1709 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.6709,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.1709 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054825.45+461817.6,2461139.6709,11.01,0.05,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 J054825.45+461817.6 20260409.1709 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Aur,2461139.6709,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Aur 20260409.1709 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4445192,2461139.6709,12.73,0.05,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 4445192 20260409.1709 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461139.67119133 09.04.2026 04:06:20.931 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 46
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23838
Objects passed selection criteria: 23824
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 22440
Average stars matched: 21875.5 (97.4844 %)
Memory usage VmPeak: 126876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 23:53:35 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461139.67119133 09.04.2026 04:06:20.931 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 156
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 88 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): 156394
Objects passed selection criteria: 156085
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: 133272
Average stars matched: 129303 (97.0219 %)
Memory usage VmPeak: 1982080 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 23:57:22 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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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: 2461139.67052920
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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits'
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:23.965 +45:59:27.32
Angular distance between the image centers 0.1063 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 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:24.273 +45:59:06.74
Angular distance between the image centers 0.1084 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:23.965 +45:59:27.32
Second-epoch second image center 06:00:24.273 +45:59:06.74
Angular distance between the image centers 0.00579 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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.mjxM8XMtxw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.mt5ppLAj8A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits &> /tmp/tmp.dhwjHzuT5O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits &> /tmp/tmp.wuPWioyREF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 24266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9190 to 102.4864 deg, Dec +39.9773 to +51.3461 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 77.9190 to 102.4864 deg, Dec 39.9773 to 51.3461 deg
Loaded 11816 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): 86 out of 101 total matches.
Matched with Tycho-2 101 out of 24266 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 23.040760
a=0.000000 b=1.000000 c=23.040760
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
4.4 pix fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
4.4 pix fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.8 mag. fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
14.8 mag. fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.3 (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.mjxM8XMtxw (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2260, passed=24266
Got 24266 stars (including 21982 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 24266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 417 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 363 matched stars entering correct_measured_positions(), 321 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 354 matched stars entering correct_measured_positions(), 9707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 406 matched stars entering correct_measured_positions(), 9733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.27"
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 10903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.47"
Excluding outliers - 405 stars left (next iteration limit 389)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.mt5ppLAj8A (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2222, passed=24282
Got 24282 stars (including 22031 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 24282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
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...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.dhwjHzuT5O (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1086, passed=20889
Got 20889 stars (including 19794 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat
util/solve_plate_with_UCAC5 got 20889 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 20492 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 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 20493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 20493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 923 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.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.wuPWioyREF (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1060, passed=20858
Got 20858 stars (including 19795 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat
util/solve_plate_with_UCAC5 got 20858 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 20493 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 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 20493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 20493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09969.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31504_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31504_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:30:20.33 +41:49:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.460 958364433900404480 097.58487868126 +41.83115208556 12.1730 11.9144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31542_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31542_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:34:27.38 +44:52:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 1.997 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31548_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31548_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:14:59.08 +46:47:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31557_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31557_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:59:43.27 +44:59:10.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31612_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31612_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:57:23.89 +48:22:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31614_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31614_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31620_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31620_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:09:51.87 +46:34:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.319 963406141390333184 092.46702943046 +46.57449767313 10.4625 8.8819 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31641_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31641_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:38:21.21 +50:18:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31648_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31648_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:48:25.40 +46:18:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.444 197948278101166080 087.10599538582 +46.30486477628 10.9482 9.5176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31659_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31659_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:26:31.29 +42:40:36.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)
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Considering the candidate 31663_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31663_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:33:22.69 +44:56:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.212 965094475854599936 098.34501577089 +44.94719408903 11.9474 11.2883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31671_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31671_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:46:04.78 +47:26:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.613 966672004459585152 101.51999576409 +47.43461621313 12.0973 11.3733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31674_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31674_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:08:43.51 +45:39:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.068 963287669013037952 092.18113567353 +45.66109925881 12.1607 11.6916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31676_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31676_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:00:30.78 +45:57:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 5.232 963168612518998144 090.13025490050 +45.96688472581 12.1197 11.3966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31682_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31682_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:06:11.24 +47:25:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.865 969681535286381312 091.54712051726 +47.42216425873 12.0045 11.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31684_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31684_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:17:53.40 +46:49:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31685_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31685_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:55:20.80 +43:16:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.894 193310160099657216 088.83737940998 +43.28199553885 12.1323 11.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31693_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31693_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:55:39.95 +47:30:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.037 198116400300941440 088.91652348569 +47.50163196744 11.2016 9.7643 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31696_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31696_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:53:58.74 +49:52:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.838 211530575302864000 088.49486643244 +49.87363707682 11.0314 9.5472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31702_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31702_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:47:38.61 +48:43:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.247 990868338376216576 101.91139967351 +48.72968045974 12.1359 11.6220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31703_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31703_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:35:20.89 +45:39:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.256 965502085432232832 098.83730061204 +45.66028508244 12.0537 11.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31710_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31710_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:56:01.47 +45:16:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.128 196901195139135616 089.00656955459 +45.27723816857 11.6596 10.6140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31711_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31711_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:04:20.70 +44:13:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.926 961439389966178560 091.08660441363 +44.22495970976 11.6630 10.5517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31714_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31714_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:28:45.80 +48:34:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.730 967547868550025216 097.19110438442 +48.57701626020 12.2587 11.7628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31715_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31715_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:25:39.94 +42:46:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31718_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31718_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:17:36.23 +41:11:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.608 959891144453330048 094.40141098029 +41.18404437782 12.2330 11.7805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31719_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31719_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:13:13.45 +46:41:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.677 968656687370081664 093.30631491750 +46.69665373893 12.1592 11.6339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31720_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31720_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:19:01.68 +47:35:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.641 969127278346770560 094.75723151051 +47.58338683419 12.0379 11.3364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31721_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31721_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:05:59.59 +46:32:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.233 963535475742766720 091.49876147334 +46.54044169762 12.2781 12.2514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31722_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31722_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:01:01.78 +43:16:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.579 961326110207073536 090.25800534780 +43.26935134289 12.1538 11.6187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31725_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31725_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:14:42.32 +45:55:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.544 962611194483468800 093.67646354466 +45.92379583508 12.0293 11.2932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31737_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31737_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:26:22.88 +46:09:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 5.316 965438348116104064 096.59621591043 +46.15771144671 12.5443 12.3472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31741_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31741_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:42:33.36 +48:14:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.771 966926674543263232 100.63972497619 +48.23720462656 12.0215 11.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31742_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31742_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:12:38.21 +47:22:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.255 968789938733063296 093.15928054013 +47.36916252029 12.1836 11.4611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31744_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31744_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:33:12.54 +40:20:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.505 957347939697200896 098.30306630184 +40.34470034707 12.4442 11.8866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31746_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31746_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:21:33.15 +48:36:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.134 969099034643074176 095.38846833306 +48.60808700256 12.1105 11.3567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31749_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31749_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:29:08.88 +44:36:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.307 207848929338777088 082.28614226177 +44.60324184772 12.5643 11.7022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31750_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31750_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:10:20.90 +45:46:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.770 963262861282486656 092.58734909325 +45.77231020442 12.1039 11.4113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31751_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31751_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:12:35.10 +45:58:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.699 962606074882449920 093.14648896912 +45.96717746347 12.0488 11.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31771_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31771_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:07:09.24 +42:22:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31772_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 31772_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:15:15.15 +46:45:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.177 968664044651644032 093.81313075316 +46.76458975037 12.2101 11.6146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09969_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 09969_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:26:01.75 +50:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:41:12.73 +44:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Aur-02-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 ####
05:27:04.82 +50:07:24.0
06:03:53.74 +46:17:34.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits exists and is non-empty
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:23.965 +45:59:27.32
Angular distance between the image centers 0.1063 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 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:24.273 +45:59:06.74
Angular distance between the image centers 0.1084 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:23.965 +45:59:27.32
Second-epoch second image center 06:00:24.273 +45:59:06.74
Angular distance between the image centers 0.00579 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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.VwF43wPF3O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.BER65F7Xep
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits &> /tmp/tmp.rDYGPgxgrS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits &> /tmp/tmp.BrcFWf4L9T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 170851 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.8948 to 102.5178 deg, Dec +39.9772 to +51.3479 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 77.8948 to 102.5178 deg, Dec 39.9772 to 51.3479 deg
Loaded 11844 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): 101 out of 140 total matches.
Matched with Tycho-2 140 out of 170851 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.801794
a=0.000000 b=1.000000 c=21.801794
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 147 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
3.9 pix fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
3.9 pix fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
13.8 mag. fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
13.8 mag. fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.1 (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.VwF43wPF3O (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=20120, passed=170805
Got 170805 stars (including 150422 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 170805 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 406 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 356 matched stars entering correct_measured_positions(), 310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.13"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 60456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.06"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 442 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 410 matched stars entering correct_measured_positions(), 60493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.05"
Accuracy estimation diagnostic: 409 matched stars entering correct_measured_positions(), 73193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.14"
Excluding outliers - 409 stars left (next iteration limit 387)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.BER65F7Xep (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=20075, passed=170053
Got 170053 stars (including 149705 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170053 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166991 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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.rDYGPgxgrS (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=9909, passed=97829
Got 97829 stars (including 87839 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat
util/solve_plate_with_UCAC5 got 97829 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 95999 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 95999 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 95999 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 926 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.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.BrcFWf4L9T (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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9754, passed=97753
Got 97753 stars (including 87925 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat
util/solve_plate_with_UCAC5 got 97753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 96436 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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 96436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 96435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 925 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-05-23_20.00sec_-4.90C_LIGHTs_0078.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.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_2026-04-08_CI_Aur-02-Q1b1x1_230712_TTUQ1b1x1_6057_O3mhjkjG/wcs_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94834.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 66s
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: 31s
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Considering the candidate 195180_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195180_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:29:19.68 +50:20:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.328 968210461745076096 097.33326150704 +50.33468463451 14.3264 13.8778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195186_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195186_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:06:24.67 +44:03:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.171 961235263057938816 091.60316081965 +44.06225606595 14.1328 13.3338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195205_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195207_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195207_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195209_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195209_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:34:02.64 +42:41:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.076 194726365436042880 083.51097375056 +42.69890962511 13.9531 13.3362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195210_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195210_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:18:00.13 +47:12:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.419 212124109721433600 079.50075091805 +47.20571929477 13.9128 13.0148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195211_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195211_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195242_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195242_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195249_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195249_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195250_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195250_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:18:14.39 +43:31:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.665 207510279754544256 079.55985573493 +43.52397470013 13.5851 13.1834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195267_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195267_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195269_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195269_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195270_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195270_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195275_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195275_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195279_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195279_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:17:19.19 +48:21:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 5.061 213039212632567040 079.33065556945 +48.36149408427 13.3205 12.4901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195292_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195292_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195298_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195298_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195302_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195302_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195303_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195303_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:15:01.12 +49:27:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.838 261375461777311872 078.75544378429 +49.45171242748 13.0743 12.5170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195305_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195305_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:16:30.15 +49:28:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.403 261378725952342528 079.12663729479 +49.48189247217 13.3847 13.0415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195311_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195311_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:17:48.87 +44:23:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 5.036 208356633129826048 079.45407367324 +44.38244388445 13.1523 12.6333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195313_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:17:22.46 +49:24:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 4.187 261385219942865408 079.34361875635 +49.40767038106 13.3949 12.8273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195328_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195328_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195329_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195329_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:55:45.45 +41:06:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195337_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195337_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:22:18.32 +42:58:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.330 195308247605939200 080.57627853880 +42.96758954826 12.6828 11.9990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195339_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195339_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195394_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 195396_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195396_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 195451_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195451_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:45:42.92 +43:37:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195453_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195453_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 195474_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195474_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 195491_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195491_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 195493_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195493_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 195506_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195506_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 195546_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195546_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:19:01.41 +41:06:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195562_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195562_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 195586_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195586_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:19:04.15 +47:21:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.728 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195607_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195607_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:13:42.02 +45:31:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195640_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195640_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:13:46.63 +44:43:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 1.112 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195663_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195663_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 195674_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195674_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 195684_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195684_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:05:50.20 +44:39:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.741 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195701_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195701_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 195721_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195721_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:17:56.42 +46:08:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195729_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195729_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195732_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195732_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195744_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195744_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:27:50.39 +42:19:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195745_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195745_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:24:10.98 +43:58:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195750_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195750_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:03:13.63 +42:56:27.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195754_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195754_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:57:45.91 +45:53:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 3.345 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195769_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195769_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195778_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195778_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:49:32.65 +43:42:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.229 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195787_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195787_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195789_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195789_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:12:10.13 +50:14:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195801_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195801_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 195808_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195808_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:29:04.53 +42:17:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195811_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195811_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:59:52.66 +44:00:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.531 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195812_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195812_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195815_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195815_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:17:34.63 +46:23:47.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195816_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195816_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:17:28.53 +45:52:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.795 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195819_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195819_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:42:29.90 +44:44:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.090 197245582797409152 085.62447289270 +44.74687417395 12.5370 11.1711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195828_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195828_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195845_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195845_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195846_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195846_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195849_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195849_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195854_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195854_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195862_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195862_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:11:00.96 +47:29:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.706 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195916_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195916_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:17:15.68 +41:56:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.720 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195919_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195919_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195944_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195944_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195960_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195960_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:28:50.27 +44:16:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195963_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195963_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195967_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 195967_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 195977_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195977_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 195979_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195979_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:25:45.40 +45:22:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195982_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 195982_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 196004_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 196004_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 196013_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196013_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:40:14.21 +50:00:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196028_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196028_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:52:03.73 +49:32:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196033_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196033_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:12:49.82 +40:52:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196039_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 196039_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 196043_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 196043_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 196046_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196046_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:25:57.41 +43:06:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.179 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196054_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 196054_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 196063_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 196063_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 196066_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196066_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:47:28.43 +41:25:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196075_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196075_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:47:49.44 +51:04:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196076_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196076_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:38:22.25 +42:59:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.489 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196094_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196094_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:31:17.80 +46:25:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196097_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196097_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:28:45.57 +49:11:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196098_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196098_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 196113_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 196113_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 196115_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196115_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:38:50.64 +49:49:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.769 214265786572414464 084.71026707144 +49.83277338684 13.8138 13.2353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196130_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196130_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:43:56.34 +47:43:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.850 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196146_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196146_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:57:25.02 +49:14:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196179_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196179_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:46:39.73 +43:21:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196199_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196199_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:17:15.20 +42:06:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196206_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196206_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:25:22.23 +44:07:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.566 959204602520168832 096.34257438144 +44.11709696304 12.9853 11.6271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196223_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196223_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 196242_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196242_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:26:29.64 +49:54:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.586 971091731965538688 096.62459838265 +49.90271527912 14.1099 13.5701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196265_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196265_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:12:20.07 +50:12:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.153 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196302_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196302_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 196310_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196310_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196313_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:02:57.97 +46:27:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.217 963568667249950592 090.74225943407 +46.46168855447 13.3894 11.9357 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196330_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196330_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:57:13.74 +44:55:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196352_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196352_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 196392_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 196392_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 75417_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 75417_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:03:53.72 +46:17:34.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 190349_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 190349_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 47690_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 47690_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:57:23.96 +48:22:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:37:57.00 +44:41:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163833_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 163833_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:41:12.73 +44:09:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13408_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 13408_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:38:21.23 +50:18:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100835_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 100835_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 159256_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 159256_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158883_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 158883_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:15:48.59 +41:02:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94834_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 94834_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118976_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 118976_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:27:04.78 +50:07:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69975_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 69975_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161576_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 161576_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:32:37.63 +41:28:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:21:29.95 +43:44:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156126_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 156126_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 138651_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 138651_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:26:33.02 +42:55:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39411_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 39411_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 53491_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 53491_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 160506_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 160506_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 46369_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 46369_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 181993_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 181993_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 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 75263_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 75263_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:14:59.08 +46:47:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144933_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 144933_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:59:44.15 +47:37:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37886_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
Preparing report for the candidate 37886_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:26:01.75 +50:29:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83859_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 83859_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:59:56.14 +45:56:13.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100668_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 100668_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:59:31.54 +44:56:53.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38089_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 38089_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18929_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 18929_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 06:24:53.53 +49:17:14.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75511_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 75511_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:16:41.17 +45:59:44.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137224_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079
The candidate 137224_fd_Aur-02-Q1b1x1_2026-04-08_23-06-20_20.00sec_-4.90C_LIGHTs_0079 did not pass the final checks
**** FOUND 05:18:16.31 +42:47:34.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 100s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:27:04.82 +50:07:24.0
06:03:53.74 +46:17:34.5
05:22:16.21 +44:38:46.1
05:38:54.79 +43:45:43.8
06:12:08.12 +43:09:52.4
06:33:07.79 +40:29:07.8
05:26:00.73 +41:15:18.2
05:46:54.89 +41:24:32.3
05:22:12.34 +41:33:53.0
06:36:34.82 +41:59:53.7
06:00:28.16 +46:08:06.7
05:48:31.27 +41:05:15.6
06:05:59.72 +49:28:32.8
05:42:23.88 +50:28:46.4
05:54:25.80 +48:11:00.1
06:00:55.57 +49:35:18.5
05:52:15.51 +44:59:41.2
06:33:52.08 +48:52:40.4
05:44:15.35 +41:14:56.9
05:24:11.12 +47:43:22.9
05:48:23.98 +50:34:49.3
06:21:31.70 +41:49:30.4
05:27:44.81 +50:14:21.8
05:32:11.42 +42:21:14.1
06:16:43.06 +44:42:56.2
05:38:27.90 +45:32:12.0
05:28:44.33 +41:18:11.0
06:26:19.86 +41:59:10.5
06:11:06.04 +41:55:48.8
05:28:01.12 +48:14:57.0
05:33:56.59 +46:11:54.3
06:38:45.76 +40:20:56.4
05:25:00.65 +50:58:24.2
05:38:23.88 +42:59:52.9
06:25:49.11 +48:15:43.6
06:00:13.79 +47:43:15.9
05:23:51.18 +41:27:40.6
06:38:26.70 +42:30:58.4
05:57:44.82 +45:54:52.3
05:31:00.46 +42:54:53.5
06:24:22.28 +41:49:34.6
05:19:56.70 +42:41:27.5
05:56:40.61 +41:24:48.1
06:03:20.56 +42:41:50.5
05:39:19.09 +44:01:52.4
05:51:18.86 +43:17:49.5
05:35:44.82 +48:35:20.3
05:46:55.60 +48:32:36.7
05:54:00.66 +48:02:58.3
05:43:00.45 +47:58:52.4
05:23:15.95 +47:29:09.8
06:09:51.84 +46:34:28.7
05:49:32.27 +46:35:58.9
05:48:25.44 +46:18:17.7
06:00:14.43 +45:04:01.7
########### Completed Aur-02-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 ####
06:03:53.74 +46:17:34.5
05:27:04.82 +50:07:24.0
06:36:34.82 +41:59:53.7
06:00:28.16 +46:08:06.7
05:48:31.27 +41:05:15.6
06:05:59.72 +49:28:32.8
05:42:23.88 +50:28:46.4
05:54:25.80 +48:11:00.1
06:00:55.57 +49:35:18.5
05:52:15.51 +44:59:41.2
06:33:52.08 +48:52:40.4
05:44:15.35 +41:14:56.9
05:24:11.12 +47:43:22.9
05:48:23.98 +50:34:49.3
06:21:31.70 +41:49:30.4
05:27:44.81 +50:14:21.8
05:32:11.42 +42:21:14.1
06:16:43.06 +44:42:56.2
05:38:27.90 +45:32:12.0
05:28:44.33 +41:18:11.0
06:26:19.86 +41:59:10.5
06:11:06.04 +41:55:48.8
05:28:01.12 +48:14:57.0
05:33:56.59 +46:11:54.3
06:38:45.76 +40:20:56.4
05:25:00.65 +50:58:24.2
05:38:23.88 +42:59:52.9
06:25:49.11 +48:15:43.6
06:00:13.79 +47:43:15.9
05:23:51.18 +41:27:40.6
06:38:26.70 +42:30:58.4
05:57:44.82 +45:54:52.3
05:31:00.46 +42:54:53.5
06:24:22.28 +41:49:34.6
05:19:56.70 +42:41:27.5
05:56:40.61 +41:24:48.1
06:03:20.56 +42:41:50.5
05:39:19.09 +44:01:52.4
05:51:18.86 +43:17:49.5
05:43:00.45 +47:58:52.4
05:22:12.34 +41:33:53.0
05:22:16.21 +44:38:46.1
05:26:00.73 +41:15:18.2
06:09:51.84 +46:34:28.7
06:00:14.43 +45:04:01.7
05:38:54.79 +43:45:43.8
05:49:32.27 +46:35:58.9
06:33:07.79 +40:29:07.8
05:46:55.60 +48:32:36.7
05:23:15.95 +47:29:09.8
05:46:54.89 +41:24:32.3
05:54:00.66 +48:02:58.3
05:48:25.44 +46:18:17.7
06:12:08.12 +43:09:52.4
05:35:44.82 +48:35:20.3
###################################################################################
06:03:53.74 +46:17:34.5 -- not an asteroid (will add it to exclusion list)
05:27:04.82 +50:07:24.0 -- not an asteroid (will add it to exclusion list)
06:36:34.82 +41:59:53.7 -- not an asteroid (will add it to exclusion list)
06:00:28.16 +46:08:06.7 -- not an asteroid (will add it to exclusion list)
05:48:31.27 +41:05:15.6 -- not an asteroid (will add it to exclusion list)
06:05:59.72 +49:28:32.8 -- not an asteroid (will add it to exclusion list)
05:42:23.88 +50:28:46.4 -- not an asteroid (will add it to exclusion list)
05:54:25.80 +48:11:00.1 -- not an asteroid (will add it to exclusion list)
06:00:55.57 +49:35:18.5 -- not an asteroid (will add it to exclusion list)
05:52:15.51 +44:59:41.2 -- not an asteroid (will add it to exclusion list)
06:33:52.08 +48:52:40.4 -- not an asteroid (will add it to exclusion list)
05:44:15.35 +41:14:56.9 -- not an asteroid (will add it to exclusion list)
05:24:11.12 +47:43:22.9 -- not an asteroid (will add it to exclusion list)
05:48:23.98 +50:34:49.3 -- not an asteroid (will add it to exclusion list)
06:21:31.70 +41:49:30.4 -- not an asteroid (will add it to exclusion list)
05:27:44.81 +50:14:21.8 -- not an asteroid (will add it to exclusion list)
05:32:11.42 +42:21:14.1 -- not an asteroid (will add it to exclusion list)
06:16:43.06 +44:42:56.2 -- not an asteroid (will add it to exclusion list)
05:38:27.90 +45:32:12.0 -- not an asteroid (will add it to exclusion list)
05:28:44.33 +41:18:11.0 -- not an asteroid (will add it to exclusion list)
06:26:19.86 +41:59:10.5 -- not an asteroid (will add it to exclusion list)
06:11:06.04 +41:55:48.8 -- asteroid (will NOT add it to exclusion list)
05:28:01.12 +48:14:57.0 -- not an asteroid (will add it to exclusion list)
05:33:56.59 +46:11:54.3 -- not an asteroid (will add it to exclusion list)
06:38:45.76 +40:20:56.4 -- not an asteroid (will add it to exclusion list)
05:25:00.65 +50:58:24.2 -- not an asteroid (will add it to exclusion list)
05:38:23.88 +42:59:52.9 -- not an asteroid (will add it to exclusion list)
06:25:49.11 +48:15:43.6 -- not an asteroid (will add it to exclusion list)
06:00:13.79 +47:43:15.9 -- not an asteroid (will add it to exclusion list)
05:23:51.18 +41:27:40.6 -- not an asteroid (will add it to exclusion list)
06:38:26.70 +42:30:58.4 -- not an asteroid (will add it to exclusion list)
05:57:44.82 +45:54:52.3 -- not an asteroid (will add it to exclusion list)
05:31:00.46 +42:54:53.5 -- not an asteroid (will add it to exclusion list)
06:24:22.28 +41:49:34.6 -- not an asteroid (will add it to exclusion list)
05:19:56.70 +42:41:27.5 -- not an asteroid (will add it to exclusion list)
05:56:40.61 +41:24:48.1 -- not an asteroid (will add it to exclusion list)
06:03:20.56 +42:41:50.5 -- not an asteroid (will add it to exclusion list)
05:39:19.09 +44:01:52.4 -- not an asteroid (will add it to exclusion list)
05:51:18.86 +43:17:49.5 -- not an asteroid (will add it to exclusion list)
05:43:00.45 +47:58:52.4 -- not an asteroid (will add it to exclusion list)
05:22:12.34 +41:33:53.0 -- not an asteroid (will add it to exclusion list)
05:22:16.21 +44:38:46.1 -- not an asteroid (will add it to exclusion list)
05:26:00.73 +41:15:18.2 -- not an asteroid (will add it to exclusion list)
06:09:51.84 +46:34:28.7 -- not an asteroid (will add it to exclusion list)
06:00:14.43 +45:04:01.7 -- not an asteroid (will add it to exclusion list)
05:38:54.79 +43:45:43.8 -- not an asteroid (will add it to exclusion list)
05:49:32.27 +46:35:58.9 -- not an asteroid (will add it to exclusion list)
06:33:07.79 +40:29:07.8 -- not an asteroid (will add it to exclusion list)
05:46:55.60 +48:32:36.7 -- not an asteroid (will add it to exclusion list)
05:23:15.95 +47:29:09.8 -- not an asteroid (will add it to exclusion list)
05:46:54.89 +41:24:32.3 -- not an asteroid (will add it to exclusion list)
05:54:00.66 +48:02:58.3 -- not an asteroid (will add it to exclusion list)
05:48:25.44 +46:18:17.7 -- not an asteroid (will add it to exclusion list)
06:12:08.12 +43:09:52.4 -- not an asteroid (will add it to exclusion list)
05:35:44.82 +48:35:20.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:19:56.70 +42:41:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:12.34 +41:33:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:16.21 +44:38:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:15.95 +47:29:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:51.18 +41:27:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:11.12 +47:43:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:00.65 +50:58:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:00.73 +41:15:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.82 +50:07:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:44.81 +50:14:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.12 +48:14:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:44.33 +41:18:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:00.46 +42:54:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:11.42 +42:21:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:56.59 +46:11:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:44.82 +48:35:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:23.88 +42:59:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.90 +45:32:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:54.79 +43:45:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.09 +44:01:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:23.88 +50:28:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:00.45 +47:58:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:15.35 +41:14:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:54.89 +41:24:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:55.60 +48:32:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.98 +50:34:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:25.44 +46:18:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:31.27 +41:05:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:32.27 +46:35:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.86 +43:17:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:15.51 +44:59:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:00.66 +48:02:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:25.80 +48:11:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:40.61 +41:24:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:44.82 +45:54:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:13.79 +47:43:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:14.43 +45:04:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:28.16 +46:08:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:55.57 +49:35:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:20.56 +42:41:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:53.74 +46:17:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:59.72 +49:28:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:51.84 +46:34:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:08.12 +43:09:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:43.06 +44:42:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.70 +41:49:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:22.28 +41:49:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:49.11 +48:15:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.86 +41:59:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:07.79 +40:29:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:52.08 +48:52:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:34.82 +41:59:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:26.70 +42:30:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:45.76 +40:20:56.4 -- 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)
05:19:56.70 +42:41:27.5 -- not a known variable star
05:22:12.34 +41:33:53.0 -- a known variable star
05:22:16.21 +44:38:46.1 -- not a known variable star
05:23:15.95 +47:29:09.8 -- a known variable star
05:23:51.18 +41:27:40.6 -- not a known variable star
05:24:11.12 +47:43:22.9 -- not a known variable star
05:25:00.65 +50:58:24.2 -- not a known variable star
05:26:00.73 +41:15:18.2 -- a known variable star
05:27:04.82 +50:07:24.0 -- a known variable star
05:27:44.81 +50:14:21.8 -- not a known variable star
05:28:01.12 +48:14:57.0 -- a known variable star
05:28:44.33 +41:18:11.0 -- not a known variable star
05:31:00.46 +42:54:53.5 -- not a known variable star
05:32:11.42 +42:21:14.1 -- a known variable star
05:33:56.59 +46:11:54.3 -- not a known variable star
05:35:44.82 +48:35:20.3 -- a known variable star
05:38:23.88 +42:59:52.9 -- not a known variable star
05:38:27.90 +45:32:12.0 -- not a known variable star
05:38:54.79 +43:45:43.8 -- a known variable star
05:39:19.09 +44:01:52.4 -- not a known variable star
05:42:23.88 +50:28:46.4 -- not a known variable star
05:43:00.45 +47:58:52.4 -- a known variable star
05:44:15.35 +41:14:56.9 -- not a known variable star
05:46:54.89 +41:24:32.3 -- a known variable star
05:46:55.60 +48:32:36.7 -- a known variable star
05:48:23.98 +50:34:49.3 -- not a known variable star
05:48:25.44 +46:18:17.7 -- a known variable star
05:48:31.27 +41:05:15.6 -- not a known variable star
05:49:32.27 +46:35:58.9 -- a known variable star
05:51:18.86 +43:17:49.5 -- not a known variable star
05:52:15.51 +44:59:41.2 -- not a known variable star
05:54:00.66 +48:02:58.3 -- a known variable star
05:54:25.80 +48:11:00.1 -- not a known variable star
05:56:40.61 +41:24:48.1 -- not a known variable star
05:57:44.82 +45:54:52.3 -- not a known variable star
06:00:13.79 +47:43:15.9 -- not a known variable star
06:00:14.43 +45:04:01.7 -- a known variable star
06:00:28.16 +46:08:06.7 -- a known variable star
06:00:55.57 +49:35:18.5 -- not a known variable star
06:03:20.56 +42:41:50.5 -- not a known variable star
06:03:53.74 +46:17:34.5 -- a known variable star
06:05:59.72 +49:28:32.8 -- not a known variable star
06:09:51.84 +46:34:28.7 -- a known variable star
06:12:08.12 +43:09:52.4 -- a known variable star
06:16:43.06 +44:42:56.2 -- not a known variable star
06:21:31.70 +41:49:30.4 -- not a known variable star
06:24:22.28 +41:49:34.6 -- not a known variable star
06:25:49.11 +48:15:43.6 -- not a known variable star
06:26:19.86 +41:59:10.5 -- not a known variable star
06:33:07.79 +40:29:07.8 -- not a known variable star
06:33:52.08 +48:52:40.4 -- not a known variable star
06:36:34.82 +41:59:53.7 -- not a known variable star
06:38:26.70 +42:30:58.4 -- a known variable star
06:38:45.76 +40:20:56.4 -- not a known variable star
Found 34 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
54 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 54 (excluding asteroids and hot pixels, 34 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461139.67052920 -observatory V36
23:33:30.65 -05:20:07.0 Mercury (0.2mag)
02:35:38.52 +15:07:58.3 Venus (-3.9mag)
23:58:24.44 -01:16:31.8 Mars (1.2mag)
07:09:46.84 +22:50:47.6 Jupiter (-2.1mag)
00:26:06.75 +00:29:45.2 Saturn (0.9mag)
03:46:18.10 +19:42:58.7 Uranus (5.8mag)
00:09:55.98 -00:21:06.5 Neptune (7.8mag)
20:33:24.74 -22:52:27.0 Pluto (14.5mag)
18:36:58.77 -27:55:15.9 Moon (-10.7mag)
-rw-r--r-- 1 apache apache 362 Apr 8 23:53 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461139.67052920:
07:09:51.54 +22:50:40.2 Io (5.7mag)
07:09:55.31 +22:50:32.3 Europa (5.9mag)
07:10:01.65 +22:50:12.5 Ganymede (5.3mag)
07:09:16.29 +22:51:52.2 Callisto (6.5mag)
07:13:23.64 +22:41:44.9 Himalia (15.3mag)
07:09:51.04 +22:50:38.0 Thebe (16.2mag)
07:13:25.68 +23:11:06.6 Elara (17.3mag)
07:08:11.82 +23:34:22.3 Pasiphae (17.4mag)
07:18:15.20 +22:48:05.2 Carme (18.5mag)
00:26:13.44 +00:29:34.4 Titan (8.8mag)
00:26:11.48 +00:29:54.0 Rhea (10.1mag)
00:26:00.53 +00:30:56.5 Iapetus (11.5mag)
00:26:18.12 +00:29:31.5 Hyperion (14.8mag)
00:27:48.86 +00:39:16.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 23:53 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.67052920:
15:04:33.57 -10:57:49.5 JWST
17:36:28.51 +39:10:37.4 Chandra
17:15:26.62 -48:38:30.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 23:53 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.67052920 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:47.87 -28:23:36.9 13.9mag P/2010 H2 (Vales)
05:02:00.81 -69:59:44.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:05.00 +31:23:36.6 17.2mag C/2017 K2 (PANSTARRS)
17:30:53.61 +09:43:50.6 17.6mag C/2021 G2 (ATLAS)
23:08:16.90 +28:58:15.2 17.0mag C/2022 E2 (ATLAS)
04:21:21.77 +25:50:57.3 15.9mag C/2022 N2 (PANSTARRS)
09:02:12.76 +31:57:09.7 16.2mag C/2022 QE78 (ATLAS)
08:30:13.25 -00:53:44.5 17.3mag C/2022 R6 (PANSTARRS)
18:55:07.85 +17:57:07.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:43.80 -11:37:11.0 17.6mag P/2023 B1 (PANSTARRS)
09:11:06.37 -13:00:02.5 17.6mag C/2023 F3 (ATLAS)
21:46:56.22 +62:31:28.1 17.5mag C/2023 H5 (Lemmon)
19:24:29.86 -03:38:18.4 14.2mag C/2023 R1 (PANSTARRS)
21:41:18.21 +84:59:25.4 17.8mag C/2023 X2 (Lemmon)
06:15:16.29 +63:33:23.3 17.1mag C/2024 A1 (ATLAS)
04:58:05.72 +15:48:48.2 10.6mag C/2024 E1 (Wierzchos)
16:23:26.73 +05:16:04.5 17.4mag C/2024 G6 (ATLAS)
20:18:39.20 +13:27:12.5 14.7mag C/2024 J3 (ATLAS)
03:20:19.77 -23:26:45.7 16.4mag C/2024 T5 (ATLAS)
05:11:03.53 +47:02:12.0 17.7mag C/2025 J1 (Borisov)
14:07:07.13 +40:14:02.1 14.9mag C/2025 L1 (ATLAS)
03:14:45.57 -25:10:42.9 17.8mag C/2025 Q3 (ATLAS)
23:02:47.45 +19:46:20.3 9.6mag C/2025 R3 (PANSTARRS)
12:57:05.63 +02:35:08.4 17.5mag C/2025 Y1 (ATLAS)
02:17:14.96 +03:44:02.8 10.3mag C/2026 A1 (MAPS)
23:39:45.74 +35:53:03.0 14.4mag C/2026 B2 (Sun-Gao)
18:29:36.93 -10:04:25.9 12.2mag 10P/Tempel
15:09:16.99 +03:51:51.6 13.4mag 24P/Schaumasse
11:04:47.62 -01:45:24.4 15.7mag 29P/Schwassmann-Wachmann
17:58:20.84 -09:52:21.2 17.8mag 40P/Vaisala
10:38:16.50 -04:40:30.3 16.8mag 43P/Wolf-Harrington
01:38:07.71 +16:18:51.7 17.2mag 47P/Ashbrook-Jackson
06:58:27.73 +38:27:42.0 17.0mag 63P/Wild
23:20:14.07 -12:17:00.7 15.7mag 65P/Gunn
03:45:17.71 +18:50:20.3 15.9mag 76P/West-Kohoutek-Ikemura
00:50:33.71 +06:52:43.1 14.4mag 78P/Gehrels
22:41:58.24 -11:24:12.7 14.6mag 88P/Howell
01:51:18.97 +18:47:00.0 15.1mag 93P/Lovas
04:42:12.58 +31:54:22.3 16.3mag 123P/West-Hartley
08:20:49.58 +41:30:55.0 16.2mag 124P/Mrkos
02:22:43.97 +13:35:57.2 16.4mag 128P/Shoemaker-Holt
02:34:11.07 +13:38:23.7 17.5mag 131P/Mueller
00:50:50.47 +10:45:36.2 11.0mag 141P/Machholz
01:00:34.65 +02:18:32.3 11.0mag 141P-A/Machholz
23:49:25.72 -01:28:45.1 13.7mag 141P-D/Machholz
01:30:09.13 +04:01:03.7 17.9mag 141P-I/Machholz
00:43:23.12 -04:56:37.8 15.2mag 162P/SidingSpring
10:30:06.14 +31:19:12.7 17.9mag 164P/Christensen
06:23:53.48 +24:26:57.6 17.9mag 198P/ODAS
15:03:32.05 -00:49:44.0 17.4mag 210P/Christensen
21:18:21.74 -13:06:04.8 17.5mag 218P/LINEAR
17:14:09.01 -14:44:13.6 16.2mag 235P/LINEAR
05:19:53.62 +34:08:06.6 16.6mag 240P/NEAT
07:35:22.77 -05:56:01.7 17.7mag 242P/Spahr
15:45:03.88 +06:31:23.5 17.5mag 391P/Kowalski
07:31:47.90 +21:20:01.6 17.6mag 450P/LONEOS
05:26:04.04 +45:26:03.3 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 23:53 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
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
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
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
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
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
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
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
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
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
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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 8 23:53 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:06:48.970 +28:22:45.47 AT 2026ifn 2026-03-27.85 21.37
16:26:20.250 +28:06:35.30 AT 2026ifm 2026-03-27.85 20.13
17:01:36.800 +29:43:13.81 AT 2026ifl 2026-03-27.85 20.62
17:06:26.770 +28:47:25.16 AT 2026ifk 2026-03-27.85 21.39
16:47:18.680 +27:13:25.92 AT 2026ifj 2026-03-27.85 20.26
15:55:49.720 +37:36:32.33 AT 2026ifi 2026-03-24.80 21.32
16:05:53.820 +48:45:26.80 AT 2026ifh 2026-03-23.81 21.26
16:27:03.110 +44:45:26.84 AT 2026ifg 2026-03-23.81 21.9
16:41:17.580 +44:27:03.47 AT 2026iff 2026-03-23.81 22.17
16:30:53.670 +55:47:08.39 AT 2026ife 2026-03-30.85 20.99
16:07:35.060 +52:45:21.40 AT 2026ifd 2026-03-30.82 20.79
12:49:57.980 +19:52:49.93 AT 2026ifc 2026-03-20.70 19.71
15:58:08.890 +36:23:36.27 AT 2026ifb 2026-03-18.81 20.34
15:47:02.670 +48:09:28.72 AT 2026ifa 2026-03-30.81 20.31
15:30:58.600 +53:17:16.37 AT 2026iez 2026-03-23.80 21.21
10:25:53.600 +03:15:54.45 AT 2026iey 2026-03-24.63 22.18
19:10:17.892 -22:37:27.97 AT 2026iex 2026-03-30.80 18.87
12:44:39.935 -44:03:37.93 AT 2026iew 2026-03-31.50 19.02
14:52:16.530 -15:21:39.90 AT 2026iev 2026-04-02.23 19.3
17:43:01.293 -27:00:33.19 AT 2026ieu 2026-04-04.35 19.44
-rw-r--r-- 1 apache apache 30K Apr 8 23:53 tns_transients_list.txt
