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_005409_TTUQ1b1x1_9298_VNjWwIkO
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 991132045071645952,2461138.7275,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 991132045071645952 20260408.2275 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211657985506798336,2461138.7275,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211657985506798336 20260408.2275 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7275,13.41,0.05,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 20260408.2275 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.38,0.05,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
target 20260408.2275 13.38CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3686+43.2939,2461138.7275,13.21,0.05,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
ATO J084.3686+43.2939 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211569096866300928,2461138.7275,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211569096866300928 20260408.2275 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.56,0.05,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
target 20260408.2275 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7171+45.4803,2461138.7275,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.7171+45.4803 20260408.2275 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6295+48.7004,2461138.7275,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.6295+48.7004 20260408.2275 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967581128777104000,2461138.7275,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967581128777104000 20260408.2275 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195611128699499648,2461138.7275,13.10,0.05,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
Gaia DR3 195611128699499648 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.18,0.05,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
target 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.1606+41.4882,2461138.7275,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.1606+41.4882 20260408.2275 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 213675383188776320,2461138.7275,12.89,0.05,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
Gaia DR3 213675383188776320 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212135929471711616,2461138.7275,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212135929471711616 20260408.2275 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.1267+46.2073,2461138.7275,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.1267+46.2073 20260408.2275 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.7880+41.3772,2461138.7275,12.79,0.05,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
ATO J079.7880+41.3772 20260408.2275 12.79CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.2051+48.8339,2461138.7275,12.76,0.05,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 J081.2051+48.8339 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060214.12+474700.6,2461138.7275,12.96,0.05,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 J060214.12+474700.6 20260408.2275 12.96CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0152+49.4731,2461138.7275,12.54,0.05,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
ATO J082.0152+49.4731 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.3489+46.4839,2461138.7275,12.66,0.05,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
ATO J094.3489+46.4839 20260408.2275 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.3673+41.8196,2461138.7275,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.3673+41.8196 20260408.2275 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963105940357874176,2461138.7275,12.40,0.05,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 963105940357874176 20260408.2275 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.7908+47.0566,2461138.7275,12.22,0.05,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
ATO J092.7908+47.0566 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.9517+41.9846,2461138.7275,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.9517+41.9846 20260408.2275 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053755.31+425401.9,2461138.7275,11.55,0.05,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
ZTF J053755.31+425401.9 20260408.2275 11.55CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192332281946145280,2461138.7275,11.49,0.05,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
Gaia DR3 192332281946145280 20260408.2275 11.49CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207208674270841728,2461138.7275,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 207208674270841728 20260408.2275 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
STARE aur0 543,2461138.7275,9.71,0.05,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
STARE aur0 543 20260408.2275 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208934456550670592,2461138.7275,11.19,0.05,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 208934456550670592 20260408.2275 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 213256984656366976,2461138.7275,11.95,0.05,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 213256984656366976 20260408.2275 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J051714.56+431117.3,2461138.7275,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051714.56+431117.3 20260408.2275 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194505775916838272,2461138.7275,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194505775916838272 20260408.2275 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212655861031529216,2461138.7275,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212655861031529216 20260408.2275 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963614258326644864,2461138.7275,12.54,0.05,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
Gaia DR3 963614258326644864 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.4314+43.0363,2461138.7275,12.45,0.05,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 J084.4314+43.0363 20260408.2275 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209019462542689536,2461138.7275,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209019462542689536 20260408.2275 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211485843219678720,2461138.7275,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211485843219678720 20260408.2275 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6086+42.9942,2461138.7275,12.57,0.05,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
ATO J084.6086+42.9942 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J080.7154+50.4902,2461138.7275,12.74,0.05,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 J080.7154+50.4902 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.62,0.05,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
target 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207620613173739776,2461138.7275,12.59,0.05,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 207620613173739776 20260408.2275 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.73,0.05,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
target 20260408.2275 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0489+43.4659,2461138.7275,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.0489+43.4659 20260408.2275 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209517442528659072,2461138.7275,12.71,0.05,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 209517442528659072 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053146.43+444302.5,2461138.7275,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053146.43+444302.5 20260408.2275 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192624786395334400,2461138.7275,12.67,0.05,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 192624786395334400 20260408.2275 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.80,0.05,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 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3627+42.0135,2461138.7275,12.77,0.05,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
ATO J084.3627+42.0135 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.4978+48.5110,2461138.7275,12.71,0.05,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
ATO J081.4978+48.5110 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197945941638987264,2461138.7275,12.85,0.05,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
Gaia DR3 197945941638987264 20260408.2275 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J051728.60+465934.4,2461138.7275,12.90,0.05,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
ZTF J051728.60+465934.4 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.3147+42.1171,2461138.7275,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.3147+42.1171 20260408.2275 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.5793+41.6911,2461138.7275,12.95,0.05,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 J087.5793+41.6911 20260408.2275 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1460+42.0428,2461138.7275,12.90,0.05,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
ATO J084.1460+42.0428 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461138.7275,12.85,0.05,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
Gaia DR3 197388553666998656 20260408.2275 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461138.7275,13.10,0.05,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 J087.2776+47.3006 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4626+44.3866,2461138.7275,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.4626+44.3866 20260408.2275 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7275,13.07,0.05,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
VARIABLE_NAME 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,12.99,0.05,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 20260408.2275 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 213847422398656512,2461138.7275,13.13,0.05,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 213847422398656512 20260408.2275 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.8255+44.2002,2461138.7275,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.8255+44.2002 20260408.2275 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.6786+45.4850,2461138.7275,13.12,0.05,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
ATO J082.6786+45.4850 20260408.2275 13.12CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5805+44.4532,2461138.7275,13.18,0.05,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 J083.5805+44.4532 20260408.2275 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060116.96+484201.5,2461138.7275,13.49,0.05,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
ASASSN-V J060116.96+484201.5 20260408.2275 13.49CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209612206687413376,2461138.7275,13.27,0.05,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 209612206687413376 20260408.2275 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 960373177221975680,2461138.7275,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 960373177221975680 20260408.2275 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962241178758050304,2461138.7275,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962241178758050304 20260408.2275 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.70,0.05,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 20260408.2275 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1759+48.7398,2461138.7275,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1759+48.7398 20260408.2275 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.2784+47.0742,2461138.7275,13.63,0.05,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 J084.2784+47.0742 20260408.2275 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.0526+47.6845,2461138.7275,13.55,0.05,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 J088.0526+47.6845 20260408.2275 13.55CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7275,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2275 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.5654+45.6574,2461138.7275,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.5654+45.6574 20260408.2275 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 191876877973645312,2461138.7275,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 191876877973645312 20260408.2275 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J055713.26+483435.1,2461138.7275,13.74,0.05,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
ZTF J055713.26+483435.1 20260408.2275 13.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2743+50.0752,2461138.7275,13.66,0.05,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
ATO J087.2743+50.0752 20260408.2275 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.5522+44.8128,2461138.7275,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.5522+44.8128 20260408.2275 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8570+46.6349,2461138.7275,13.93,0.05,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 J089.8570+46.6349 20260408.2275 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210084996686630656,2461138.7275,13.99,0.05,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 210084996686630656 20260408.2275 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.7880+41.3772,2461138.7275,11.73,0.05,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
ATO J079.7880+41.3772 20260408.2275 11.73CV 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: 2461138.72791211 08.04.2026 05:28:01.606 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
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): 22975
Objects passed selection criteria: 22945
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 19918.5
Average stars matched: 19482.5 (97.8111 %)
Memory usage VmPeak: 126872 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 01:00:24 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: 2461138.72791211 08.04.2026 05:28:01.606 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 332
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: 83 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): 159961
Objects passed selection criteria: 159640
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 146490
Average stars matched: 142040 (96.9626 %)
Memory usage VmPeak: 1930336 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 01:03:11 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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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: 2461138.72715877
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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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 06:00:06.290 +45:59:29.01
Angular distance between the image centers 0.0566 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 06:00:04.933 +45:59:00.93
Angular distance between the image centers 0.0561 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 06:00:06.290 +45:59:29.01
Second-epoch second image center 06:00:04.933 +45:59:00.93
Angular distance between the image centers 0.00873 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.C01UFuaRWa
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.SndtuzB0P2
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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits &> /tmp/tmp.23AscyhPPb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits &> /tmp/tmp.muq31uuVEC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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 8 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
2.3 pix fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
2.3 pix fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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
14.9 mag. fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
14.9 mag. fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (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.C01UFuaRWa (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_005409_TTUQ1b1x1_9298_VNjWwIkO/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.SndtuzB0P2 (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_005409_TTUQ1b1x1_9298_VNjWwIkO/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.23AscyhPPb (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_005409_TTUQ1b1x1_9298_VNjWwIkO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1160, passed=15879
Got 15879 stars (including 14691 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 15879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 15590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 15589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 15589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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.muq31uuVEC (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_005409_TTUQ1b1x1_9298_VNjWwIkO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1165, passed=15733
Got 15733 stars (including 14553 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 15733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 15343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 15341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 15341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 932 stars left (next iteration limit 1024)
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_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/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_005409_TTUQ1b1x1_9298_VNjWwIkO/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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31696.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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 31565_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 31565_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:59:43.38 +44:59:09.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31580_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 31580_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:14:59.09 +46:47:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31667_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 31667_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:38:21.17 +50:18:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31672_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 31672_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:45:42.88 +43:37:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31696_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 31696_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:19:01.64 +47:35:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.198 969127278346770560 094.75723151051 +47.58338683419 12.0379 11.3364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:26:01.64 +50:29:26.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:41:12.74 +44:10:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20752_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 20752_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:17:39.42 +41:49:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 1.717 195144484794132096 079.41456809148 +41.82600286361 11.3029 11.0833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
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 ####
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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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 06:00:06.290 +45:59:29.01
Angular distance between the image centers 0.0566 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 06:00:04.933 +45:59:00.93
Angular distance between the image centers 0.0561 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 06:00:06.290 +45:59:29.01
Second-epoch second image center 06:00:04.933 +45:59:00.93
Angular distance between the image centers 0.00873 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.hveCRVgYaH
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.n3fBj8Rexd
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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits &> /tmp/tmp.RAvrtIPeEn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits &> /tmp/tmp.cf9XTmvw89
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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 289 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
2.1 pix fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
2.1 pix fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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
13.9 mag. fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
13.9 mag. fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.hveCRVgYaH (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_005409_TTUQ1b1x1_9298_VNjWwIkO/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.n3fBj8Rexd (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_005409_TTUQ1b1x1_9298_VNjWwIkO/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.RAvrtIPeEn (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_005409_TTUQ1b1x1_9298_VNjWwIkO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=11285, passed=124563
Got 124563 stars (including 113070 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat
util/solve_plate_with_UCAC5 got 124563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 122872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 122874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 122875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 931 stars left (next iteration limit 1024)
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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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.cf9XTmvw89 (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_005409_TTUQ1b1x1_9298_VNjWwIkO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q1b1x1_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=11263, passed=124375
Got 124375 stars (including 112902 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat
util/solve_plate_with_UCAC5 got 124375 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 122401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 122401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 122400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/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_005409_TTUQ1b1x1_9298_VNjWwIkO/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_00-26-56_20.00sec_-5.00C_LIGHTs_0020.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_005409_TTUQ1b1x1_9298_VNjWwIkO/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-26-56_20.00sec_-5.00C_LIGHTs_0020.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.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_005409_TTUQ1b1x1_9298_VNjWwIkO/wcs_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out169071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out162175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197335.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 116s
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: 60s
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Considering the candidate 195197_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195197_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195199_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195199_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:45:39.15 +49:51:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.004 214125152162884096 086.41344826610 +49.85481448861 14.7067 14.0735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195229_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195229_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195239_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195239_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195245_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195245_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195250_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195250_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195251_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195251_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:54:04.11 +50:05:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.960 211551161082978432 088.51749029006 +50.09856694290 14.2592 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195261_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195261_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195266_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195266_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:05:45.82 +44:27:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.481 962934901876874880 091.44102792761 +44.45555912510 14.1989 13.6480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195268_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195268_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195272_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195272_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:29:02.06 +44:34:52.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 195274_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195274_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195277_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195277_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:28:02.12 +42:38:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.169 195426582545397248 082.00946868790 +42.63640778349 13.7854 12.7883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195279_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195279_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:21:43.40 +45:44:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195280_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195280_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:37:24.02 +42:46:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195290_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195290_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:29:51.79 +50:44:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.736 213903978527738880 082.46610898592 +50.74757302018 13.9878 13.1090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.736#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_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195292_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195294_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195294_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:20:23.35 +41:10:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195296_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:41:02.57 +45:28:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195297_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195297_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:40:40.42 +44:00:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195302_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195302_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:25:11.91 +42:49:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.004 195267943632599552 081.29907206185 +42.81579780671 13.6094 12.5389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195303_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195303_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195305_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195305_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:20:14.47 +43:58:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.009 962154519200831744 095.06033911674 +43.97886072638 14.1367 13.5587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195306_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195306_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195308_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195308_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195309_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195309_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:25:44.33 +50:48:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195314_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195314_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:22:09.05 +50:01:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195318_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195318_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:44:40.08 +48:38:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195319_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195319_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195321_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195321_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:35.22 +44:22:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.010 208437786533924608 079.64667318958 +44.37233610085 13.8030 13.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195329_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195329_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195330_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195330_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195331_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195332_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195332_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:35:35.15 +50:55:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195334_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195334_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:34:24.11 +42:20:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195336_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195336_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:27:46.02 +48:02:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195342_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195342_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:35:00.14 +50:18:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195348_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195348_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:52:21.10 +42:50:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195350_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195350_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:11:03.88 +44:42:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195355_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195355_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:23:18.52 +43:23:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.245 207361811325203456 080.82725760692 +43.39412213298 13.6024 12.7355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195357_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195357_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:36:49.62 +41:27:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.344 191392199503897728 084.20686554759 +41.46595927300 13.6795 13.3475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195360_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195360_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:19:54.09 +43:11:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195361_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195361_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:36:25.34 +41:59:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195364_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195364_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195365_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195365_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:50:36.53 +42:33:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195366_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195366_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:32.60 +46:16:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.207 211837721303196800 079.63671201134 +46.28305578216 13.5567 13.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195367_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195367_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:57.04 +44:10:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.702 195847695498306304 083.23830725925 +44.18141561184 13.5222 12.6700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195373_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195373_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:18.92 +41:30:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195374_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195374_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:16:49.27 +43:14:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.112 207488225101913088 079.20559264339 +43.23633786381 13.3006 12.3304 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 195375_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195375_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:28:13.03 +41:54:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195376_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195376_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195377_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195377_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:16:52.69 +43:05:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.109 207483380378835840 079.21938510756 +43.09026955576 13.4096 12.4872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195380_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195380_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:20:27.51 +46:35:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195382_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:15:57.61 +41:11:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195383_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195383_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 195386_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195386_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:07:19.16 +43:29:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195391_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195391_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:28:36.19 +43:09:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195393_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195393_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:21.63 +41:01:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195394_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:26.48 +43:26:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195396_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195396_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:25:52.63 +46:29:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195397_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195397_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:05.15 +42:02:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.831 195173866669311232 079.52213253988 +42.04860559525 13.4566 12.9969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195399_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195399_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:26:53.32 +43:56:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195400_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:43:44.16 +50:59:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.073 215225007387998592 085.93446186108 +50.98390711228 13.5660 12.9195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195405_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195405_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195406_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195406_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:03.20 +46:55:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195409_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195409_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:28:33.98 +44:21:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195414_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195414_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:30:25.49 +44:55:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195419_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195419_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:21.86 +42:50:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195422_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195422_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:31:53.83 +48:02:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.088 212426368042295552 082.97440695807 +48.04640221426 13.1212 12.2563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195423_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195423_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195424_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195424_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:00.05 +43:23:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195426_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195426_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:20:55.20 +49:27:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195427_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195427_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:19:25.27 +44:38:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195428_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195428_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:11:06.23 +41:55:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 5.176 960956566924526336 092.77506168430 +41.93017064148 13.2400 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195432_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195432_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:19:27.75 +41:10:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.917 194880022186588160 079.86581223003 +41.17478774766 12.8919 11.9618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195434_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195434_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:17:41.72 +41:49:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.488 195144484795142528 079.42435035584 +41.82632278598 12.6599 11.5820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195437_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195437_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:22:19.81 +41:15:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195438_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195438_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:35.43 +42:44:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195440_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195440_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:19:17.95 +48:31:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.186 969270734551986176 094.82536550396 +48.52310964378 13.2217 12.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195441_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195441_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195443_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195443_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:17.29 +50:38:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195444_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195444_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:36.98 +41:20:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195445_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195445_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:53:59.25 +45:07:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195448_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195448_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195451_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195451_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:25:35.58 +49:58:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195456_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195456_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195457_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:54:42.14 +43:39:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 0.349 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195458_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195458_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195460_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195460_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:19:51.30 +43:00:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195461_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195461_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:43.94 +41:49:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195463_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195463_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:57:45.92 +43:34:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195464_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195464_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:26:44.01 +41:42:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195524_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195524_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195535_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195535_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:44:52.55 +49:21:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.39, MAG_FAINT_SEARCH_LIMIT=11.37)GAIADR2_OUTPUT=# 0.733 991088339485440640 101.21871255640 +49.35207015053 11.2541 10.7323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195544_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195544_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:43:27.53 +42:19:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.09, MAG_FAINT_SEARCH_LIMIT=11.07)GAIADR2_OUTPUT=# 0.371 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195652_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195652_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:11:34.59 +48:44:37.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195660_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195660_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:45:42.88 +43:37:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195678_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195678_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:32.45 +43:37:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195698_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195698_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195727_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195727_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:23:23.04 +43:35:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195729_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195729_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:33:38.32 +45:26:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195738_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195738_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:19:04.15 +47:21:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.074 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195742_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195742_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:19:01.48 +41:06:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195832_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195832_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:40:23.57 +49:53:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195841_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195841_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:39:07.42 +44:53:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 2.548 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195854_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195854_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195871_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195871_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:05:50.19 +44:39:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.156 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195877_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195877_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:23.52 +48:55:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195893_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195893_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:51.81 +42:57:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195895_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195895_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195921_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195921_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:26:51.39 +41:14:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.176 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195930_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195930_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:31:06.76 +48:10:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195943_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195943_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:49:02.39 +49:49:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.078 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195952_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195952_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:47:58.16 +50:54:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195962_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195962_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:12:10.17 +50:14:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195966_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195966_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:30:40.26 +48:57:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195971_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195971_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:40:25.96 +48:47:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195983_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 195983_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 195990_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 195990_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:03:13.60 +42:56:28.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196001_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196001_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:57:46.07 +45:53:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.055 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196008_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196008_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:17:56.61 +46:08:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196051_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196051_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196076_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196076_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:28:43.88 +42:26:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196081_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196081_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:47:45.33 +50:03:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.670 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196106_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196106_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:17:34.59 +46:23:47.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196108_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196108_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:49:32.63 +43:42:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.392 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196119_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196119_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196121_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196121_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:30:40.67 +41:28:15.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196124_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196124_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:18:48.24 +44:06:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.426 207680158599604608 079.70193351269 +44.11312538601 13.3106 12.6161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196128_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196128_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:15.61 +45:06:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196149_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196149_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:55:48.13 +42:30:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196150_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196150_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:35:17.68 +42:18:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196161_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196161_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:53.72 +48:33:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196165_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196165_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:17:09.19 +43:26:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196166_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196166_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:29:04.62 +42:17:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196177_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196177_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196190_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196190_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:01:04.67 +50:00:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.622 970368734350565760 090.26951411061 +50.00316418749 13.2862 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196195_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196195_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196202_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196202_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:42.69 +47:53:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 0.645 212586385641158912 080.67776024297 +47.89856027064 13.3715 12.5283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196212_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196212_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:59.34 +46:40:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196215_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196215_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196218_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196218_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:33:56.54 +46:11:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.012 208282721033602560 083.48553101272 +46.19874907056 13.4787 12.6535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.012#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_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196223_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:08.19 +41:29:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196225_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196225_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:20:41.58 +49:23:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.940 213710327042533248 080.17355762524 +49.39641569149 13.4063 12.7696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196235_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196235_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 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 196237_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196237_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:41.57 +50:41:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.196 261875155450928384 080.42251070654 +50.69932540948 13.4670 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196244_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196244_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:23:23.78 +50:13:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.605 261808836861057408 080.84799330687 +50.23144343721 13.3252 12.3513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196245_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196245_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:52:03.62 +49:32:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196251_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196251_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196256_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196256_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:00:13.75 +47:43:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 4.390 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196259_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196259_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:40:14.18 +50:00:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196270_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196270_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:33:11.52 +40:20:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196278_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196278_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:17:17.56 +40:45:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196282_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196282_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:15.00 +40:57:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196291_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:24:18.07 +43:22:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196292_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196292_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196293_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196293_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196295_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196295_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:49:31.29 +47:51:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.169 210289196612409472 087.38044179706 +47.86209697171 13.6067 12.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.169#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_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196302_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:31:40.17 +42:51:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196311_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196311_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196313_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:27:50.38 +42:19:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196314_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196314_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:16:53.92 +43:54:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196316_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196316_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:38:22.18 +42:59:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 2.635 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196321_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196321_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:41.08 +48:21:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196326_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196326_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196336_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196336_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196341_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196341_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:27:30.92 +42:33:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 0.834 195427372819457152 081.87865762868 +42.56269207473 13.7210 13.1823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196342_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196342_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196345_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196345_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:47:08.05 +41:09:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196347_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196347_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:47.22 +41:40:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196352_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196352_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196353_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196353_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:34:02.49 +46:44:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196357_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196357_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196358_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196358_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196368_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196368_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:42.39 +49:50:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196376_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196376_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:47:49.04 +51:04:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196377_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196377_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:56:33.83 +45:29:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196388_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196388_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196402_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196402_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196404_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196404_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196421_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196421_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:49:27.87 +47:51:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196423_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196423_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196427_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196427_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:28:50.32 +44:16:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196430_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196430_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:01.91 +42:43:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.552 195300447945544064 080.50775878561 +42.71881683081 13.4492 12.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196438_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196438_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 196440_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196440_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:24:38.75 +43:41:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196455_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196455_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:58.14 +44:19:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196456_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196456_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196463_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196463_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196468_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196468_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:35.12 +49:30:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.862 213712938382573312 080.39689795590 +49.51491271206 13.5503 12.7305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196477_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196477_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:25:04.81 +42:33:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196486_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196486_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:36:57.38 +42:25:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196489_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196489_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:31:00.34 +42:54:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.724 195412735570512896 082.75232236264 +42.91460805837 13.6478 12.8067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196490_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196490_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:30.31 +41:38:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196500_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196500_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:31:02.04 +44:18:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196515_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196515_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196518_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196518_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:25:45.37 +45:22:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196522_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196522_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:05.53 +48:44:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196525_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196525_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:48:07.63 +50:26:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.307 214568598946171264 087.03234717596 +50.43577947810 13.9372 13.3806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196543_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196543_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196551_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196551_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:36:30.30 +43:50:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.240 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196554_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196554_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:51:18.82 +43:17:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.832 193427528667708288 087.82879815788 +43.29576806055 13.9092 13.2559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196558_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196558_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:22:17.41 +46:57:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.049 211927228421172992 080.57195142662 +46.96253291072 13.6003 12.8490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196561_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196561_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:50:06.41 +46:08:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196570_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196570_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:46:39.80 +43:21:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196571_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196571_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:57:24.91 +49:14:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196581_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196581_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:17:43.70 +43:11:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196584_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196584_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:20:02.75 +46:37:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196587_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196587_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:23:43.13 +50:10:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.332 213769219633738112 080.92960190688 +50.17639561905 13.7633 12.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196599_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196599_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196602_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196602_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196604_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196604_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:48:44.62 +49:34:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.081 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196615_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196615_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:33:32.23 +48:16:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.151 212436955138189696 083.38339755979 +48.28147147774 13.9515 13.4567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196634_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196634_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196641_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196641_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:40:34.19 +46:53:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196642_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196642_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196644_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196644_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196646_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196646_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:23:54.18 +46:06:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196658_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196658_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:12:19.91 +50:12:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.399 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196665_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196665_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196674_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196674_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196678_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196678_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:45:24.59 +43:50:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196681_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196681_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:40:15.96 +46:51:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196684_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196684_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:36:07.12 +47:47:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.380 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196696_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196696_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196704_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196704_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:03:43.64 +50:12:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196717_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196717_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:35:41.21 +44:16:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196728_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196728_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:36:18.62 +47:12:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.634 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196750_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196750_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:37:44.72 +42:36:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.550 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196763_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196763_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:29:34.01 +51:10:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.403 261966208758451968 082.39187092852 +51.16684242895 14.0311 13.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196777_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196777_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:23:51.83 +48:16:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.895 212612670840480000 080.96704413027 +48.26814712789 14.0705 13.5224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196779_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196779_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196784_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196784_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 196794_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196794_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:45.33 +44:42:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196865_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196865_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196866_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196866_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196872_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196872_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:56.34 +50:48:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.625 215347568575186688 083.23502356000 +50.80367783911 13.8986 12.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196888_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196888_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:41:07.33 +47:58:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196891_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196891_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196894_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196894_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196899_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196899_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:57:13.64 +44:55:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196922_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196922_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:54:37.57 +42:21:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196948_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196948_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:52:41.93 +41:07:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196951_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196951_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196966_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196966_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196974_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196974_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:46:01.50 +49:53:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.530 991219254384148992 101.50644388813 +49.89019966890 14.4079 13.6620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196983_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196983_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196990_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 196990_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 196992_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 196992_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:32:38.58 +50:06:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197007_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197007_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:56:00.71 +49:05:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.068 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197025_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197025_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197032_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197032_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:43:30.47 +42:27:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197072_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197072_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:15:35.92 +49:33:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.814 970884267865221376 093.89986975315 +49.55164951166 14.7017 14.1530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197077_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197077_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197080_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197080_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197084_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197084_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197087_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197087_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197094_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197094_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197107_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197107_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197108_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197108_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:10:00.36 +46:40:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.617 963408275991729408 092.50144899849 +46.67091546199 14.6329 14.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197126_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197126_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:17:51.59 +49:20:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.461 970828055333430528 094.46557100988 +49.34237179177 14.7323 14.1385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197137_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197137_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:50:04.15 +41:09:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.423 191888697723652352 087.51777393945 +41.15337129012 14.4955 13.7407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197145_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197145_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197147_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197147_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:37:01.05 +49:53:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197159_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197159_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:58:41.77 +49:31:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197181_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 197181_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:03:30.48 +46:27:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.521 963522315963058944 090.87753282894 +46.45115210222 14.7556 14.4748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197188_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197188_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197198_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197198_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197246_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197246_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197316_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197316_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
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Considering the candidate 169071_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 169071_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:17:39.41 +41:49:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.35, MAG_FAINT_SEARCH_LIMIT=11.33)GAIADR2_OUTPUT=# 0.971 195144484794132096 079.41456809148 +41.82600286361 11.3029 11.0833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:41:12.74 +44:10:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:37:56.92 +44:41:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:57:23.97 +48:22:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:21:29.84 +43:44:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:14:59.07 +46:47:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169188_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 169188_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:19:21.24 +41:53:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181590_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 181590_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:20:18.83 +41:18:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 05:59:44.06 +47:37:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021 did not pass the final checks
**** FOUND 06:26:01.63 +50:29:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162175_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
Preparing report for the candidate 162175_fd_Aur-02-Q1b1x1_2026-04-08_00-28-01_20.00sec_-5.00C_LIGHTs_0021
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 180s
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 ####
05:19:10.22 +41:22:36.0
06:14:15.59 +49:58:37.5
06:43:21.22 +49:42:47.4
05:56:59.83 +50:54:43.3
06:09:32.92 +41:55:40.7
05:50:33.18 +42:41:22.4
05:37:29.65 +43:17:39.3
05:57:24.43 +50:20:03.0
06:12:04.61 +50:30:17.3
05:42:47.60 +50:23:01.7
05:50:52.67 +45:28:53.6
05:38:30.89 +48:42:03.1
06:31:45.94 +48:30:00.5
05:34:27.50 +43:48:14.9
05:40:27.47 +47:56:11.7
05:28:38.19 +41:29:28.0
05:24:16.80 +49:23:37.8
05:21:06.96 +47:13:40.9
05:40:29.60 +46:12:11.8
05:19:11.38 +41:22:56.0
05:24:48.30 +48:50:23.2
06:02:14.11 +47:47:01.9
05:28:04.03 +49:28:30.8
06:17:25.61 +46:28:27.3
05:27:16.16 +45:33:34.5
06:21:31.90 +41:49:29.5
06:05:28.43 +45:37:50.4
06:11:13.08 +47:02:39.8
05:35:49.68 +41:58:30.5
05:37:56.64 +42:54:19.7
05:50:23.49 +41:49:04.4
05:18:09.64 +42:30:19.1
05:17:56.34 +41:11:55.7
05:25:37.70 +45:40:56.8
05:17:50.97 +48:39:29.8
05:17:16.96 +43:11:16.4
05:28:43.86 +41:18:09.2
05:28:01.37 +48:15:00.4
06:01:24.99 +46:54:18.1
05:37:46.31 +43:03:14.5
05:30:09.22 +46:12:57.4
05:48:23.18 +49:46:58.5
05:27:51.05 +42:20:25.7
05:38:24.44 +42:59:48.2
05:22:55.54 +50:29:42.3
05:27:26.06 +44:48:54.8
05:20:50.91 +44:04:37.4
05:44:39.89 +43:57:55.5
05:28:11.67 +43:27:56.2
05:37:49.78 +45:56:19.9
05:31:42.70 +44:43:26.3
05:40:57.41 +41:07:45.7
05:38:50.56 +49:49:58.3
05:37:28.50 +42:00:44.8
06:26:29.65 +49:54:12.3
06:03:21.18 +42:41:51.7
05:25:59.81 +48:30:09.3
05:53:28.89 +46:52:05.6
05:17:29.37 +46:59:10.5
06:17:15.30 +42:06:45.6
05:50:23.98 +41:41:27.4
05:36:34.65 +42:02:19.0
05:37:19.42 +44:51:38.6
05:49:06.57 +47:17:59.1
05:45:50.37 +44:23:04.9
05:49:38.62 +47:49:49.7
06:09:10.16 +42:04:44.6
05:42:16.24 +43:16:26.8
05:31:09.05 +50:39:12.3
06:44:26.89 +49:51:42.8
05:35:22.43 +44:11:27.9
05:30:42.52 +45:28:56.7
05:34:19.15 +44:27:43.5
06:01:14.24 +48:42:21.7
05:44:47.07 +46:28:22.0
06:13:27.04 +43:04:01.7
06:21:34.63 +44:28:59.6
06:39:25.26 +49:36:18.0
05:56:44.64 +48:44:14.2
05:37:05.30 +47:05:22.9
05:52:19.74 +47:40:10.0
06:32:49.61 +49:31:42.4
06:39:21.95 +48:22:26.2
06:34:13.39 +45:40:04.5
05:50:42.75 +41:04:50.5
05:57:12.94 +48:34:35.5
05:49:03.36 +50:04:18.5
05:50:10.12 +44:48:36.7
05:59:25.43 +46:37:20.1
05:49:53.41 +47:39:03.5
########### 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 ####
06:14:15.59 +49:58:37.5
06:43:21.22 +49:42:47.4
05:56:59.83 +50:54:43.3
06:09:32.92 +41:55:40.7
05:50:33.18 +42:41:22.4
05:37:29.65 +43:17:39.3
05:57:24.43 +50:20:03.0
06:12:04.61 +50:30:17.3
05:42:47.60 +50:23:01.7
05:50:52.67 +45:28:53.6
05:38:30.89 +48:42:03.1
06:31:45.94 +48:30:00.5
05:34:27.50 +43:48:14.9
05:40:27.47 +47:56:11.7
05:28:38.19 +41:29:28.0
05:24:16.80 +49:23:37.8
05:21:06.96 +47:13:40.9
05:40:29.60 +46:12:11.8
05:19:11.38 +41:22:56.0
05:24:48.30 +48:50:23.2
06:02:14.11 +47:47:01.9
05:28:04.03 +49:28:30.8
06:17:25.61 +46:28:27.3
05:27:16.16 +45:33:34.5
06:21:31.90 +41:49:29.5
06:05:28.43 +45:37:50.4
06:11:13.08 +47:02:39.8
05:35:49.68 +41:58:30.5
05:37:56.64 +42:54:19.7
05:50:23.49 +41:49:04.4
05:18:09.64 +42:30:19.1
05:17:56.34 +41:11:55.7
05:25:37.70 +45:40:56.8
05:17:50.97 +48:39:29.8
05:17:16.96 +43:11:16.4
05:28:43.86 +41:18:09.2
05:28:01.37 +48:15:00.4
06:01:24.99 +46:54:18.1
05:37:46.31 +43:03:14.5
05:30:09.22 +46:12:57.4
05:48:23.18 +49:46:58.5
05:27:51.05 +42:20:25.7
05:38:24.44 +42:59:48.2
05:22:55.54 +50:29:42.3
05:27:26.06 +44:48:54.8
05:20:50.91 +44:04:37.4
05:44:39.89 +43:57:55.5
05:28:11.67 +43:27:56.2
05:37:49.78 +45:56:19.9
05:31:42.70 +44:43:26.3
05:40:57.41 +41:07:45.7
05:38:50.56 +49:49:58.3
05:37:28.50 +42:00:44.8
06:26:29.65 +49:54:12.3
06:03:21.18 +42:41:51.7
05:25:59.81 +48:30:09.3
05:53:28.89 +46:52:05.6
05:17:29.37 +46:59:10.5
06:17:15.30 +42:06:45.6
05:50:23.98 +41:41:27.4
05:36:34.65 +42:02:19.0
05:37:19.42 +44:51:38.6
05:49:06.57 +47:17:59.1
05:45:50.37 +44:23:04.9
05:49:38.62 +47:49:49.7
06:09:10.16 +42:04:44.6
05:42:16.24 +43:16:26.8
05:31:09.05 +50:39:12.3
06:44:26.89 +49:51:42.8
05:35:22.43 +44:11:27.9
05:30:42.52 +45:28:56.7
05:34:19.15 +44:27:43.5
06:01:14.24 +48:42:21.7
05:44:47.07 +46:28:22.0
06:13:27.04 +43:04:01.7
06:21:34.63 +44:28:59.6
06:39:25.26 +49:36:18.0
05:56:44.64 +48:44:14.2
05:37:05.30 +47:05:22.9
05:52:19.74 +47:40:10.0
06:32:49.61 +49:31:42.4
06:39:21.95 +48:22:26.2
06:34:13.39 +45:40:04.5
05:50:42.75 +41:04:50.5
05:57:12.94 +48:34:35.5
05:49:03.36 +50:04:18.5
05:50:10.12 +44:48:36.7
05:59:25.43 +46:37:20.1
05:49:53.41 +47:39:03.5
05:19:10.22 +41:22:36.0
###################################################################################
06:14:15.59 +49:58:37.5 -- not an asteroid (will add it to exclusion list)
06:43:21.22 +49:42:47.4 -- not an asteroid (will add it to exclusion list)
05:56:59.83 +50:54:43.3 -- not an asteroid (will add it to exclusion list)
06:09:32.92 +41:55:40.7 -- asteroid (will NOT add it to exclusion list)
05:50:33.18 +42:41:22.4 -- not an asteroid (will add it to exclusion list)
05:37:29.65 +43:17:39.3 -- not an asteroid (will add it to exclusion list)
05:57:24.43 +50:20:03.0 -- not an asteroid (will add it to exclusion list)
06:12:04.61 +50:30:17.3 -- not an asteroid (will add it to exclusion list)
05:42:47.60 +50:23:01.7 -- not an asteroid (will add it to exclusion list)
05:50:52.67 +45:28:53.6 -- not an asteroid (will add it to exclusion list)
05:38:30.89 +48:42:03.1 -- not an asteroid (will add it to exclusion list)
06:31:45.94 +48:30:00.5 -- not an asteroid (will add it to exclusion list)
05:34:27.50 +43:48:14.9 -- not an asteroid (will add it to exclusion list)
05:40:27.47 +47:56:11.7 -- not an asteroid (will add it to exclusion list)
05:28:38.19 +41:29:28.0 -- not an asteroid (will add it to exclusion list)
05:24:16.80 +49:23:37.8 -- not an asteroid (will add it to exclusion list)
05:21:06.96 +47:13:40.9 -- not an asteroid (will add it to exclusion list)
05:40:29.60 +46:12:11.8 -- not an asteroid (will add it to exclusion list)
05:19:11.38 +41:22:56.0 -- not an asteroid (will add it to exclusion list)
05:24:48.30 +48:50:23.2 -- not an asteroid (will add it to exclusion list)
06:02:14.11 +47:47:01.9 -- not an asteroid (will add it to exclusion list)
05:28:04.03 +49:28:30.8 -- not an asteroid (will add it to exclusion list)
06:17:25.61 +46:28:27.3 -- not an asteroid (will add it to exclusion list)
05:27:16.16 +45:33:34.5 -- not an asteroid (will add it to exclusion list)
06:21:31.90 +41:49:29.5 -- not an asteroid (will add it to exclusion list)
06:05:28.43 +45:37:50.4 -- not an asteroid (will add it to exclusion list)
06:11:13.08 +47:02:39.8 -- not an asteroid (will add it to exclusion list)
05:35:49.68 +41:58:30.5 -- not an asteroid (will add it to exclusion list)
05:37:56.64 +42:54:19.7 -- not an asteroid (will add it to exclusion list)
05:50:23.49 +41:49:04.4 -- not an asteroid (will add it to exclusion list)
05:18:09.64 +42:30:19.1 -- not an asteroid (will add it to exclusion list)
05:17:56.34 +41:11:55.7 -- not an asteroid (will add it to exclusion list)
05:25:37.70 +45:40:56.8 -- not an asteroid (will add it to exclusion list)
05:17:50.97 +48:39:29.8 -- not an asteroid (will add it to exclusion list)
05:17:16.96 +43:11:16.4 -- not an asteroid (will add it to exclusion list)
05:28:43.86 +41:18:09.2 -- not an asteroid (will add it to exclusion list)
05:28:01.37 +48:15:00.4 -- not an asteroid (will add it to exclusion list)
06:01:24.99 +46:54:18.1 -- not an asteroid (will add it to exclusion list)
05:37:46.31 +43:03:14.5 -- not an asteroid (will add it to exclusion list)
05:30:09.22 +46:12:57.4 -- not an asteroid (will add it to exclusion list)
05:48:23.18 +49:46:58.5 -- not an asteroid (will add it to exclusion list)
05:27:51.05 +42:20:25.7 -- not an asteroid (will add it to exclusion list)
05:38:24.44 +42:59:48.2 -- not an asteroid (will add it to exclusion list)
05:22:55.54 +50:29:42.3 -- not an asteroid (will add it to exclusion list)
05:27:26.06 +44:48:54.8 -- not an asteroid (will add it to exclusion list)
05:20:50.91 +44:04:37.4 -- not an asteroid (will add it to exclusion list)
05:44:39.89 +43:57:55.5 -- not an asteroid (will add it to exclusion list)
05:28:11.67 +43:27:56.2 -- not an asteroid (will add it to exclusion list)
05:37:49.78 +45:56:19.9 -- not an asteroid (will add it to exclusion list)
05:31:42.70 +44:43:26.3 -- not an asteroid (will add it to exclusion list)
05:40:57.41 +41:07:45.7 -- not an asteroid (will add it to exclusion list)
05:38:50.56 +49:49:58.3 -- not an asteroid (will add it to exclusion list)
05:37:28.50 +42:00:44.8 -- not an asteroid (will add it to exclusion list)
06:26:29.65 +49:54:12.3 -- not an asteroid (will add it to exclusion list)
06:03:21.18 +42:41:51.7 -- not an asteroid (will add it to exclusion list)
05:25:59.81 +48:30:09.3 -- not an asteroid (will add it to exclusion list)
05:53:28.89 +46:52:05.6 -- not an asteroid (will add it to exclusion list)
05:17:29.37 +46:59:10.5 -- not an asteroid (will add it to exclusion list)
06:17:15.30 +42:06:45.6 -- not an asteroid (will add it to exclusion list)
05:50:23.98 +41:41:27.4 -- not an asteroid (will add it to exclusion list)
05:36:34.65 +42:02:19.0 -- not an asteroid (will add it to exclusion list)
05:37:19.42 +44:51:38.6 -- not an asteroid (will add it to exclusion list)
05:49:06.57 +47:17:59.1 -- not an asteroid (will add it to exclusion list)
05:45:50.37 +44:23:04.9 -- not an asteroid (will add it to exclusion list)
05:49:38.62 +47:49:49.7 -- not an asteroid (will add it to exclusion list)
06:09:10.16 +42:04:44.6 -- asteroid (will NOT add it to exclusion list)
05:42:16.24 +43:16:26.8 -- not an asteroid (will add it to exclusion list)
05:31:09.05 +50:39:12.3 -- not an asteroid (will add it to exclusion list)
06:44:26.89 +49:51:42.8 -- not an asteroid (will add it to exclusion list)
05:35:22.43 +44:11:27.9 -- not an asteroid (will add it to exclusion list)
05:30:42.52 +45:28:56.7 -- not an asteroid (will add it to exclusion list)
05:34:19.15 +44:27:43.5 -- not an asteroid (will add it to exclusion list)
06:01:14.24 +48:42:21.7 -- not an asteroid (will add it to exclusion list)
05:44:47.07 +46:28:22.0 -- not an asteroid (will add it to exclusion list)
06:13:27.04 +43:04:01.7 -- not an asteroid (will add it to exclusion list)
06:21:34.63 +44:28:59.6 -- not an asteroid (will add it to exclusion list)
06:39:25.26 +49:36:18.0 -- not an asteroid (will add it to exclusion list)
05:56:44.64 +48:44:14.2 -- not an asteroid (will add it to exclusion list)
05:37:05.30 +47:05:22.9 -- not an asteroid (will add it to exclusion list)
05:52:19.74 +47:40:10.0 -- not an asteroid (will add it to exclusion list)
06:32:49.61 +49:31:42.4 -- not an asteroid (will add it to exclusion list)
06:39:21.95 +48:22:26.2 -- not an asteroid (will add it to exclusion list)
06:34:13.39 +45:40:04.5 -- not an asteroid (will add it to exclusion list)
05:50:42.75 +41:04:50.5 -- not an asteroid (will add it to exclusion list)
05:57:12.94 +48:34:35.5 -- not an asteroid (will add it to exclusion list)
05:49:03.36 +50:04:18.5 -- not an asteroid (will add it to exclusion list)
05:50:10.12 +44:48:36.7 -- not an asteroid (will add it to exclusion list)
05:59:25.43 +46:37:20.1 -- not an asteroid (will add it to exclusion list)
05:49:53.41 +47:39:03.5 -- not an asteroid (will add it to exclusion list)
05:19:10.22 +41:22:36.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:17:16.96 +43:11:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:29.37 +46:59:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:50.97 +48:39:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:56.34 +41:11:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:09.64 +42:30:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:10.22 +41:22:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:11.38 +41:22:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.91 +44:04:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:06.96 +47:13:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:55.54 +50:29:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:16.80 +49:23:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:48.30 +48:50:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:37.70 +45:40:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:59.81 +48:30:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:16.16 +45:33:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.06 +44:48:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:51.05 +42:20:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.37 +48:15:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:04.03 +49:28:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.67 +43:27:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:38.19 +41:29:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:43.86 +41:18:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:09.22 +46:12:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:42.52 +45:28:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:09.05 +50:39:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:42.70 +44:43:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:19.15 +44:27:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:27.50 +43:48:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:22.43 +44:11:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:49.68 +41:58:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:34.65 +42:02:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:05.30 +47:05:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.42 +44:51:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:28.50 +42:00:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:29.65 +43:17:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:46.31 +43:03:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:49.78 +45:56:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:56.64 +42:54:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:24.44 +42:59:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:30.89 +48:42:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:50.56 +49:49:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:27.47 +47:56:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:29.60 +46:12:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:57.41 +41:07:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:16.24 +43:16:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:47.60 +50:23:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:39.89 +43:57:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:47.07 +46:28:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.37 +44:23:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.18 +49:46:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:03.36 +50:04:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.57 +47:17:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:38.62 +47:49:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:53.41 +47:39:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.12 +44:48:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:23.49 +41:49:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:23.98 +41:41:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:33.18 +42:41:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:42.75 +41:04:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:52.67 +45:28:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:19.74 +47:40:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:28.89 +46:52:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:44.64 +48:44:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:59.83 +50:54:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.94 +48:34:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:24.43 +50:20:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:25.43 +46:37:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:14.24 +48:42:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:24.99 +46:54:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:14.11 +47:47:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:21.18 +42:41:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:28.43 +45:37:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:13.08 +47:02:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:04.61 +50:30:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:27.04 +43:04:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:15.59 +49:58:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:15.30 +42:06:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:25.61 +46:28:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.90 +41:49:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:34.63 +44:28:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.65 +49:54:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:45.94 +48:30:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:49.61 +49:31:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:13.39 +45:40:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:21.95 +48:22:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:25.26 +49:36:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:21.22 +49:42:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:26.89 +49:51:42.8 -- 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)
05:17:16.96 +43:11:16.4 -- not a known variable star
05:17:29.37 +46:59:10.5 -- not a known variable star
05:17:50.97 +48:39:29.8 -- not a known variable star
05:17:56.34 +41:11:55.7 -- a known variable star
05:18:09.64 +42:30:19.1 -- a known variable star
05:19:10.22 +41:22:36.0 -- not a known variable star
05:19:11.38 +41:22:56.0 -- not a known variable star
05:20:50.91 +44:04:37.4 -- not a known variable star
05:21:06.96 +47:13:40.9 -- a known variable star
05:22:55.54 +50:29:42.3 -- not a known variable star
05:24:16.80 +49:23:37.8 -- a known variable star
05:24:48.30 +48:50:23.2 -- not a known variable star
05:25:37.70 +45:40:56.8 -- not a known variable star
05:25:59.81 +48:30:09.3 -- not a known variable star
05:27:16.16 +45:33:34.5 -- not a known variable star
05:27:26.06 +44:48:54.8 -- not a known variable star
05:27:51.05 +42:20:25.7 -- not a known variable star
05:28:01.37 +48:15:00.4 -- a known variable star
05:28:04.03 +49:28:30.8 -- not a known variable star
05:28:11.67 +43:27:56.2 -- not a known variable star
05:28:38.19 +41:29:28.0 -- not a known variable star
05:28:43.86 +41:18:09.2 -- not a known variable star
05:30:09.22 +46:12:57.4 -- not a known variable star
05:30:42.52 +45:28:56.7 -- not a known variable star
05:31:09.05 +50:39:12.3 -- not a known variable star
05:31:42.70 +44:43:26.3 -- not a known variable star
05:34:19.15 +44:27:43.5 -- not a known variable star
05:34:27.50 +43:48:14.9 -- a known variable star
05:35:22.43 +44:11:27.9 -- not a known variable star
05:35:49.68 +41:58:30.5 -- not a known variable star
05:36:34.65 +42:02:19.0 -- not a known variable star
05:37:05.30 +47:05:22.9 -- not a known variable star
05:37:19.42 +44:51:38.6 -- not a known variable star
05:37:28.50 +42:00:44.8 -- not a known variable star
05:37:29.65 +43:17:39.3 -- not a known variable star
05:37:46.31 +43:03:14.5 -- not a known variable star
05:37:49.78 +45:56:19.9 -- a known variable star
05:37:56.64 +42:54:19.7 -- a known variable star
05:38:24.44 +42:59:48.2 -- not a known variable star
05:38:30.89 +48:42:03.1 -- not a known variable star
05:38:50.56 +49:49:58.3 -- not a known variable star
05:40:27.47 +47:56:11.7 -- not a known variable star
05:40:29.60 +46:12:11.8 -- not a known variable star
05:40:57.41 +41:07:45.7 -- a known variable star
05:42:16.24 +43:16:26.8 -- not a known variable star
05:42:47.60 +50:23:01.7 -- not a known variable star
05:44:39.89 +43:57:55.5 -- not a known variable star
05:44:47.07 +46:28:22.0 -- not a known variable star
05:45:50.37 +44:23:04.9 -- not a known variable star
05:48:23.18 +49:46:58.5 -- not a known variable star
05:49:03.36 +50:04:18.5 -- not a known variable star
05:49:06.57 +47:17:59.1 -- not a known variable star
05:49:38.62 +47:49:49.7 -- not a known variable star
05:49:53.41 +47:39:03.5 -- a known variable star
05:50:10.12 +44:48:36.7 -- not a known variable star
05:50:23.49 +41:49:04.4 -- not a known variable star
05:50:23.98 +41:41:27.4 -- not a known variable star
05:50:33.18 +42:41:22.4 -- not a known variable star
05:50:42.75 +41:04:50.5 -- not a known variable star
05:50:52.67 +45:28:53.6 -- not a known variable star
05:52:19.74 +47:40:10.0 -- not a known variable star
05:53:28.89 +46:52:05.6 -- not a known variable star
05:56:44.64 +48:44:14.2 -- not a known variable star
05:56:59.83 +50:54:43.3 -- a known variable star
05:57:12.94 +48:34:35.5 -- a known variable star
05:57:24.43 +50:20:03.0 -- not a known variable star
05:59:25.43 +46:37:20.1 -- not a known variable star
06:01:14.24 +48:42:21.7 -- not a known variable star
06:01:24.99 +46:54:18.1 -- not a known variable star
06:02:14.11 +47:47:01.9 -- a known variable star
06:03:21.18 +42:41:51.7 -- not a known variable star
06:05:28.43 +45:37:50.4 -- not a known variable star
06:11:13.08 +47:02:39.8 -- not a known variable star
06:12:04.61 +50:30:17.3 -- not a known variable star
06:13:27.04 +43:04:01.7 -- not a known variable star
06:14:15.59 +49:58:37.5 -- not a known variable star
06:17:15.30 +42:06:45.6 -- not a known variable star
06:17:25.61 +46:28:27.3 -- not a known variable star
06:21:31.90 +41:49:29.5 -- not a known variable star
06:21:34.63 +44:28:59.6 -- not a known variable star
06:26:29.65 +49:54:12.3 -- not a known variable star
06:31:45.94 +48:30:00.5 -- a known variable star
06:32:49.61 +49:31:42.4 -- not a known variable star
06:34:13.39 +45:40:04.5 -- not a known variable star
06:39:21.95 +48:22:26.2 -- not a known variable star
06:39:25.26 +49:36:18.0 -- not a known variable star
06:43:21.22 +49:42:47.4 -- not a known variable star
06:44:26.89 +49:51:42.8 -- not a known variable star
Found 74 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
88 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 88 (excluding asteroids and hot pixels, 74 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)2461138.72715877 -observatory V36
23:29:14.70 -05:42:16.4 Mercury (0.3mag)
02:31:08.77 +14:43:55.7 Venus (-3.9mag)
23:55:43.02 -01:34:18.0 Mars (1.2mag)
07:09:25.68 +22:51:20.2 Jupiter (-2.2mag)
00:25:41.11 +00:27:03.5 Saturn (0.9mag)
03:46:06.96 +19:42:22.5 Uranus (5.8mag)
00:09:48.34 -00:21:55.0 Neptune (7.8mag)
20:33:21.50 -22:52:27.3 Pluto (14.5mag)
17:46:56.94 -28:41:17.9 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 01:00 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461138.72715877:
07:09:22.39 +22:51:23.9 Io (5.7mag)
07:09:15.45 +22:51:42.8 Europa (5.8mag)
07:09:46.04 +22:50:39.8 Ganymede (5.3mag)
07:08:50.64 +22:52:29.9 Callisto (6.5mag)
07:13:04.51 +22:42:46.6 Himalia (15.3mag)
07:09:23.16 +22:51:27.1 Thebe (16.2mag)
07:13:05.17 +23:11:57.8 Elara (17.3mag)
07:07:46.81 +23:35:24.6 Pasiphae (17.3mag)
07:17:55.15 +22:48:31.1 Carme (18.4mag)
00:25:44.00 +00:26:54.0 Titan (8.8mag)
00:25:46.20 +00:27:03.6 Rhea (10.1mag)
00:25:37.03 +00:28:22.3 Iapetus (11.5mag)
00:25:49.85 +00:26:48.9 Hyperion (14.8mag)
00:27:23.90 +00:36:40.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 01:00 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.72715877:
14:59:07.22 -10:09:34.5 JWST
13:44:20.88 +56:18:24.4 Chandra
08:05:25.08 -40:16:45.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 01:00 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.72715877 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:17.14 -28:20:34.6 13.9mag P/2010 H2 (Vales)
05:01:23.67 -70:02:36.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:54.91 +31:23:15.9 17.2mag C/2017 K2 (PANSTARRS)
17:30:55.19 +09:37:00.3 17.6mag C/2021 G2 (ATLAS)
23:07:59.57 +28:56:15.6 17.0mag C/2022 E2 (ATLAS)
04:20:17.46 +25:49:20.7 15.9mag C/2022 N2 (PANSTARRS)
09:02:05.44 +31:56:21.4 16.2mag C/2022 QE78 (ATLAS)
08:30:08.26 -01:00:05.8 17.3mag C/2022 R6 (PANSTARRS)
18:55:17.16 +17:52:14.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:59.12 -11:37:58.2 17.6mag P/2023 B1 (PANSTARRS)
09:11:38.37 -13:09:32.2 17.6mag C/2023 F3 (ATLAS)
21:45:51.61 +62:28:30.3 17.5mag C/2023 H5 (Lemmon)
19:25:07.74 -03:37:42.0 14.2mag C/2023 R1 (PANSTARRS)
21:41:51.59 +84:52:07.0 17.8mag C/2023 X2 (Lemmon)
06:15:00.51 +63:33:52.2 17.1mag C/2024 A1 (ATLAS)
04:55:53.93 +15:25:37.8 10.5mag C/2024 E1 (Wierzchos)
16:23:58.88 +05:06:45.3 17.4mag C/2024 G6 (ATLAS)
20:18:18.85 +13:12:29.0 14.7mag C/2024 J3 (ATLAS)
03:19:30.79 -23:35:46.0 16.4mag C/2024 T5 (ATLAS)
05:10:18.33 +47:17:12.6 17.7mag C/2025 J1 (Borisov)
14:10:57.08 +39:22:11.0 14.9mag C/2025 L1 (ATLAS)
03:13:21.39 -25:02:28.1 17.8mag C/2025 Q3 (ATLAS)
22:59:30.26 +19:48:34.9 9.8mag C/2025 R3 (PANSTARRS)
12:57:30.31 +02:31:29.3 17.5mag C/2025 Y1 (ATLAS)
02:04:11.39 +03:59:12.0 9.6mag C/2026 A1 (MAPS)
23:36:56.89 +35:41:07.3 14.3mag C/2026 B2 (Sun-Gao)
18:27:46.36 -10:07:13.8 12.3mag 10P/Tempel
15:10:27.18 +03:56:42.8 13.3mag 24P/Schaumasse
11:05:05.76 -01:47:25.1 15.7mag 29P/Schwassmann-Wachmann
17:57:52.48 -09:54:37.8 17.8mag 40P/Vaisala
10:38:26.84 -04:45:37.0 16.8mag 43P/Wolf-Harrington
01:36:40.70 +16:09:02.2 17.2mag 47P/Ashbrook-Jackson
06:56:49.20 +38:39:30.2 17.0mag 63P/Wild
23:18:59.82 -12:24:02.4 15.7mag 65P/Gunn
03:42:52.15 +18:29:35.4 15.9mag 76P/West-Kohoutek-Ikemura
00:48:30.33 +06:41:27.3 14.4mag 78P/Gehrels
22:39:00.26 -11:40:45.4 14.5mag 88P/Howell
01:48:43.55 +18:31:12.2 15.1mag 93P/Lovas
04:40:31.35 +31:51:01.5 16.3mag 123P/West-Hartley
08:19:52.79 +41:57:03.3 16.2mag 124P/Mrkos
02:21:17.98 +13:29:28.2 16.4mag 128P/Shoemaker-Holt
02:32:21.00 +13:31:06.4 17.5mag 131P/Mueller
00:46:04.43 +10:23:58.1 11.1mag 141P/Machholz
00:55:53.58 +01:57:23.4 11.1mag 141P-A/Machholz
23:45:16.76 -01:46:52.1 13.8mag 141P-D/Machholz
01:25:19.89 +03:39:09.4 17.9mag 141P-I/Machholz
00:40:46.35 -05:24:42.8 15.2mag 162P/SidingSpring
10:30:21.30 +31:22:54.2 17.9mag 164P/Christensen
06:22:09.40 +24:28:25.8 17.9mag 198P/ODAS
15:05:10.89 -00:56:35.2 17.4mag 210P/Christensen
21:15:24.40 -13:19:47.0 17.5mag 218P/LINEAR
17:13:41.52 -14:50:40.9 16.2mag 235P/LINEAR
05:17:54.61 +34:02:55.6 16.6mag 240P/NEAT
07:34:59.62 -06:02:39.8 17.6mag 242P/Spahr
15:45:21.22 +06:27:21.5 17.5mag 391P/Kowalski
07:31:30.48 +21:19:38.2 17.6mag 450P/LONEOS
05:24:44.65 +45:29:24.2 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 01:00 comets.txt
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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
-rw-r--r-- 1 apache apache 5.8K Apr 8 01:00 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 8 01:00 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:11:03.633 -05:31:15.36 AT 2026ics 2026-04-02.23 18.6573
11:09:42.183 +10:32:49.70 AT 2026icr 2026-03-24.33 20.476
10:16:29.552 -18:01:01.61 AT 2026icq 2026-03-25.18 20.2716
18:12:46.220 -18:40:42.30 AT 2026icp 2026-04-02.23 18.9
07:46:30.650 +27:23:24.16 AT 2026ico 2026-03-30.16 19.803
07:04:53.063 +10:28:54.71 AT 2026icn 2026-03-29.17 19.8144
10:09:06.230 +29:30:55.76 AT 2026icm 2026-03-27.16 20.1135
08:07:47.384 -00:23:25.65 AT 2026icl 2026-03-30.25 19.1418
07:33:52.396 +16:18:53.23 AT 2026ick 2026-03-30.19 19.5464
03:49:33.049 -49:30:53.67 AT 2026icj 2026-02-23.11 23.84
15:40:04.940 -18:30:53.00 AT 2026ici 2026-03-29.36 18.4
16:52:58.870 -62:16:14.10 AT 2026ich 2026-04-01.35 16.9
19:13:48.516 +60:10:55.03 AT 2026icg 2026-03-28.56 18.844
07:51:19.796 +21:17:20.06 AT 2026icf 2026-03-30.91 18.372
16:10:07.169 +56:12:02.29 AT 2026ice 2026-04-01.56 19.57
11:37:39.020 -44:29:30.90 AT 2026icd 2026-03-30.96 17.1
17:57:05.380 +48:58:47.80 AT 2026icc 2026-03-27.87 21.55
18:55:04.390 +55:02:09.27 AT 2026icb 2026-03-26.80 20.48
13:10:36.900 +47:58:12.10 AT 2026ica 2026-03-24.69 22.02
16:45:33.510 +54:24:32.89 AT 2026ibz 2026-03-30.82 20.28
-rw-r--r-- 1 apache apache 30K Apr 8 01:00 tns_transients_list.txt
