This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ
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
GO Aur,2461136.7166,11.22,0.05,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
GO Aur 20260406.2166 11.22CV 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
AC Aur,2461136.7166,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AC Aur 20260406.2166 10.75CV 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
RS Aur,2461136.7166,8.74,0.05,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
RS Aur 20260406.2166 8.74CV 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,2461136.7166,12.70,0.05,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 20260406.2166 12.70CV 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
target,2461136.7166,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195692664357841408,2461136.7166,12.74,0.05,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
Gaia DR3 195692664357841408 20260406.2166 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
ATO J088.0655+44.9865,2461136.7166,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.0655+44.9865 20260406.2166 12.75CV 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 194945546208281472,2461136.7166,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194945546208281472 20260406.2166 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.65,0.05,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
target 20260406.2166 12.65CV 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
target,2461136.7166,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.30,0.05,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
target 20260406.2166 12.30CV 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 J082.4441+48.1981,2461136.7166,12.40,0.05,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
ATO J082.4441+48.1981 20260406.2166 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
target,2461136.7166,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.28,0.05,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
target 20260406.2166 12.28CV 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
target,2461136.7166,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 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
Gaia DR3 262068806936707328,2461136.7166,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 262068806936707328 20260406.2166 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 207724517021610752,2461136.7166,11.90,0.05,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
Gaia DR3 207724517021610752 20260406.2166 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
target,2461136.7166,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 961627165936535680,2461136.7166,11.89,0.05,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 961627165936535680 20260406.2166 11.89CV 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 195701735329132160,2461136.7166,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195701735329132160 20260406.2166 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.7750+41.9301,2461136.7166,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.7750+41.9301 20260406.2166 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.5883+42.9989,2461136.7166,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.5883+42.9989 20260406.2166 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.39CV 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 212655861031529216,2461136.7166,12.25,0.05,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 20260406.2166 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.31,0.05,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
target 20260406.2166 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 967525667862574848,2461136.7166,12.54,0.05,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 967525667862574848 20260406.2166 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
target,2461136.7166,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.53CV 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
Gaia DR3 958053585643972736,2461136.7166,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 958053585643972736 20260406.2166 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.7523+42.9146,2461136.7166,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.7523+42.9146 20260406.2166 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
ATO J095.7693+49.1987,2461136.7166,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.7693+49.1987 20260406.2166 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.2073+40.8836,2461136.7166,12.78,0.05,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 J093.2073+40.8836 20260406.2166 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
ATO J095.6162+44.4906,2461136.7166,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.6162+44.4906 20260406.2166 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.3147+42.1171,2461136.7166,12.97,0.05,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 20260406.2166 12.97CV 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 J051831.38+410506.5,2461136.7166,11.45,0.05,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
ZTF J051831.38+410506.5 20260406.2166 11.45CV 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
GSC 02922-01985,2461136.7166,11.49,0.05,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
GSC 02922-01985 20260406.2166 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
ASASSN-V J052211.91+413349.4,2461136.7166,11.99,0.05,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
ASASSN-V J052211.91+413349.4 20260406.2166 11.99CV 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
ASASSN-V J053335.18+440000.9,2461136.7166,12.13,0.05,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
ASASSN-V J053335.18+440000.9 20260406.2166 12.13CV 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
NSVS 4452455,2461136.7166,12.31,0.05,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
NSVS 4452455 20260406.2166 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
ZTF J052600.42+411515.0,2461136.7166,11.80,0.05,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
ZTF J052600.42+411515.0 20260406.2166 11.80CV 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 J089.9789+46.9253,2461136.7166,12.45,0.05,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 J089.9789+46.9253 20260406.2166 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
ASASSN-V J053410.05+471722.3,2461136.7166,9.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053410.05+471722.3 20260406.2166 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0613426+473716,2461136.7166,10.55,0.05,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
NSVS J0613426+473716 20260406.2166 10.55CV 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
V0368 Aur,2461136.7166,10.49,0.05,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
V0368 Aur 20260406.2166 10.49CV 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
ATO J079.3306+44.0131,2461136.7166,11.18,0.05,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 J079.3306+44.0131 20260406.2166 11.18CV 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 J055539.96+473005.9,2461136.7166,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055539.96+473005.9 20260406.2166 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.7920+41.4353,2461136.7166,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.7920+41.4353 20260406.2166 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 J060603.21+452310.5,2461136.7166,11.21,0.05,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
ASASSN-V J060603.21+452310.5 20260406.2166 11.21CV 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
NSVS J0545473+473728,2461136.7166,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0545473+473728 20260406.2166 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060014.41+450400.4,2461136.7166,12.30,0.05,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
ASASSN-V J060014.41+450400.4 20260406.2166 12.30CV 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
ASASSN-V J052200.69+421149.0,2461136.7166,8.79,0.05,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
ASASSN-V J052200.69+421149.0 20260406.2166 8.79CV 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
VARIABLE_NAME,2461136.7166,11.04,0.05,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
VARIABLE_NAME 20260406.2166 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.5182+42.0514,2461136.7166,11.57,0.05,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 J079.5182+42.0514 20260406.2166 11.57CV 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
NSVS J0546556+483237,2461136.7166,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0546556+483237 20260406.2166 11.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055405.34+505910.7,2461136.7166,11.57,0.05,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
ASASSN-V J055405.34+505910.7 20260406.2166 11.57CV 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
NSVS 4521908,2461136.7166,10.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4521908 20260406.2166 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052315.65+472910.7,2461136.7166,11.54,0.05,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
ASASSN-V J052315.65+472910.7 20260406.2166 11.54CV 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
CGCS 6107,2461136.7166,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CGCS 6107 20260406.2166 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7166,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2166 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0517572+453434,2461136.7166,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0517572+453434 20260406.2166 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Aur,2461136.7166,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Aur 20260406.2166 10.35CV 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 J054825.45+461817.6,2461136.7166,10.93,0.05,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
ASASSN-V J054825.45+461817.6 20260406.2166 10.93CV 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
ATO J079.7880+41.3772,2461136.7166,11.49,0.05,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
ATO J079.7880+41.3772 20260406.2166 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
NSVS J0525385+473410,2461136.7166,11.73,0.05,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
NSVS J0525385+473410 20260406.2166 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
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 J089.8770+46.9968,2461136.7166,12.79,0.05,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 J089.8770+46.9968 20260406.2166 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 J094.7726+43.4752,2461136.7166,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.7726+43.4752 20260406.2166 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.2557+43.1607,2461136.7166,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J079.2557+43.1607 20260406.2166 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461136.71696778 06.04.2026 05:12:16.016 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
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: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23213
Objects passed selection criteria: 23192
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: 21069.8
Average stars matched: 20596.8 (97.7551 %)
Memory usage VmPeak: 126880 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:15:15 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: 2461136.71696778 06.04.2026 05:12:16.016 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 151
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: 201 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): 155977
Objects passed selection criteria: 155664
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 128078
Average stars matched: 124109 (96.9011 %)
Memory usage VmPeak: 1916584 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:20:59 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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.71617378
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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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 05:59:59.527 +45:59:52.56
Angular distance between the image centers 0.0359 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 06:00:02.479 +46:00:31.64
Angular distance between the image centers 0.0424 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:59:59.527 +45:59:52.56
Second-epoch second image center 06:00:02.479 +46:00:31.64
Angular distance between the image centers 0.01381 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.BZwmpT0smF
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.P5gKfOydaV
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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits &> /tmp/tmp.tXUQJ9jRq2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits &> /tmp/tmp.OmeyTLrPlR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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 23 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
4.3 pix fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
4.3 pix fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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
14.6 mag. fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
14.6 mag. fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BZwmpT0smF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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.P5gKfOydaV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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.tXUQJ9jRq2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=909, passed=18227
Got 18227 stars (including 17313 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat
util/solve_plate_with_UCAC5 got 18227 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 931 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: 928 matched stars entering correct_measured_positions(), 914 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: 928 matched stars entering correct_measured_positions(), 17901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 17901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 17901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.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.OmeyTLrPlR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=883, passed=18017
Got 18017 stars (including 17124 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat
util/solve_plate_with_UCAC5 got 18017 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 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 916 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: 927 matched stars entering correct_measured_positions(), 17650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 17650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 17650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out00905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out02325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09969.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 31503_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31503_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:27:06.86 +45:54:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.854 965425673669110144 096.77841941447 +45.90099330353 12.3490 11.8735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31504_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31504_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:33:58.57 +49:58:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31557_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31557_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:14:59.04 +46:47:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31560_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31560_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:59:43.25 +44:59:10.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31628_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31628_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:57:23.88 +48:22:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31630_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31630_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:45:42.87 +43:37:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31638_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31638_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:09:51.89 +46:34:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.121 963406141390333184 092.46702943046 +46.57449767313 10.4625 8.8819 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31659_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31659_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:38:21.18 +50:18:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31660_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31660_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:48:25.41 +46:18:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.489 197948278101166080 087.10599538582 +46.30486477628 10.9482 9.5176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31692_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31692_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:55:39.94 +47:30:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.865 198116400300941440 088.91652348569 +47.50163196744 11.2016 9.7643 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31693_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31693_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:53:58.73 +49:52:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.966 211530575302864000 088.49486643244 +49.87363707682 11.0314 9.5472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31695_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31695_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:06:11.20 +47:25:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.370 969681535286381312 091.54712051726 +47.42216425873 12.0045 11.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31699_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31699_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:35:20.93 +45:39:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.099 965502085432232832 098.83730061204 +45.66028508244 12.0537 11.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31703_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31703_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:13:22.38 +47:44:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31725_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31725_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:13:13.49 +46:41:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.269 968656687370081664 093.30631491750 +46.69665373893 12.1592 11.6339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31727_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31727_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:21:33.14 +48:36:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.208 969099034643074176 095.38846833306 +48.60808700256 12.1105 11.3567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31728_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31728_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:33:12.54 +40:20:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.462 957347939697200896 098.30306630184 +40.34470034707 12.4442 11.8866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31733_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 31733_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:33:42.85 +48:18:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.828 967387954030959104 098.42879552557 +48.30414948255 12.1394 11.2668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:41:12.74 +44:09:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09969_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 09969_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09643_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 09643_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:16:41.20 +45:59:42.6 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 9s
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 ####
06:26:01.73 +50:29:26.9
05:27:04.78 +50:07:23.7
06:03:53.72 +46:17:34.3
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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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 05:59:59.527 +45:59:52.56
Angular distance between the image centers 0.0359 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 06:00:02.479 +46:00:31.64
Angular distance between the image centers 0.0424 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:59:59.527 +45:59:52.56
Second-epoch second image center 06:00:02.479 +46:00:31.64
Angular distance between the image centers 0.01381 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.DPuoW10mpw
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.20TFJQg3PF
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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits &> /tmp/tmp.q04t1qRK16
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits &> /tmp/tmp.BtO5TwFNg9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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 131 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
3.8 pix fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
3.8 pix fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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
13.6 mag. fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
13.6 mag. fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DPuoW10mpw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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.20TFJQg3PF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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.q04t1qRK16 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=8010, passed=87569
Got 87569 stars (including 79515 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat
util/solve_plate_with_UCAC5 got 87569 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 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 86017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 86018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 86018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 930 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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.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.BtO5TwFNg9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=8013, passed=87039
Got 87039 stars (including 78965 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat
util/solve_plate_with_UCAC5 got 87039 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 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 85409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 85409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 85409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 925 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/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_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-11-07_20.00sec_-4.90C_LIGHTs_0082.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Aur-02-Q1b1x1_001315_TTUQ1b1x1_5378_oZXScxpJ/wcs_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out157613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94834.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 72s
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: 44s
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Considering the candidate 195207_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195207_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:22:49.72 +45:37:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.209 208571033597249664 080.70758417939 +45.62952871076 13.4829 12.9722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195209_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195209_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195215_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195215_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195224_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195224_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195225_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195225_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195233_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195236_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195236_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195244_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195244_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:18:21.23 +43:44:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.283 207563880947465728 079.58895102421 +43.74009212587 12.9066 11.8921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195248_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195248_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195259_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195259_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195260_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195260_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:19:21.65 +41:23:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 5.389 194909434122574720 079.84196688077 +41.39712556863 13.2920 12.7899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195263_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195263_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195267_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195267_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:23:02.67 +42:06:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.603 195025428303778560 080.76189238585 +42.10331574225 13.0028 12.4903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195270_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195270_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195271_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195271_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:57:24.89 +48:02:36.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 195275_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195275_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195276_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195276_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195280_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195280_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195283_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195283_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:36:10.55 +43:24:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 2.770 195531963862337408 084.04372618786 +43.40619362145 13.2991 12.4824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195291_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195291_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195292_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195292_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:16:49.84 +46:11:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 5.568 211786727154003712 079.20741462905 +46.19909221871 12.8515 11.9153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195296_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195297_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195297_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195298_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195298_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:18:22.34 +41:46:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.445 195119917581201408 079.59348671544 +41.78045645928 12.9569 12.4995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195301_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195301_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195428_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195428_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:45:42.87 +43:37:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195542_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195542_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:19:01.32 +41:06:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195563_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195563_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:13:42.01 +45:31:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195607_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195607_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:13:46.59 +44:43:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.052 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195660_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195660_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:05:50.11 +44:39:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 2.075 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195684_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195684_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195689_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195689_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:55:43.78 +41:06:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195707_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195707_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195736_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195736_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:57:45.81 +45:53:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.687 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195739_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195739_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:27:50.17 +42:19:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195744_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195744_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:24:52.19 +41:16:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.655 194180797215485440 081.21738962468 +41.28187659990 12.4521 11.0529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195749_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195749_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195754_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195754_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:24:10.77 +43:58:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195763_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195763_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195766_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195766_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:03:13.62 +42:56:26.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195777_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195777_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:15:42.94 +42:02:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195783_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195783_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:17:56.25 +46:08:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195789_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195789_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:49:32.77 +43:42:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.594 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195808_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195808_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:59:52.56 +44:00:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.885 193367472142815360 089.96999756978 +44.00566216941 13.1290 12.3826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195811_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195811_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195819_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195819_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195829_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195829_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:17:34.55 +46:23:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195839_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195839_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195857_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195857_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:04:07.24 +41:10:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 4.154 960491409081781632 091.03016848749 +41.17145719032 13.1574 12.1684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195881_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195881_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:11:00.83 +47:29:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.798 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195884_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195884_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195887_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195887_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:43:06.16 +44:51:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 5.271 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195889_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195889_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195890_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195890_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:17:28.52 +45:52:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.047 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195901_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195901_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:52:03.66 +49:32:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.613 211244191180148352 088.01550768143 +49.54892102579 13.3825 12.6034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195905_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195905_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:40:14.12 +50:00:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195908_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195908_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195914_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195914_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:17:15.67 +41:56:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.814 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 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 195935_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195935_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:29:04.51 +42:17:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195936_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195936_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:28:50.29 +49:26:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195942_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195942_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:25:57.36 +43:06:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.052 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195946_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 195946_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 195965_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195965_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:38:46.54 +46:04:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.502 209541769223400064 084.69366740623 +46.06689801652 13.5146 12.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195970_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 195970_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:24:40.83 +48:21:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196005_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 196005_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:25:45.36 +45:22:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196006_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196006_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196017_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196017_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196051_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196051_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196057_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196057_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196138_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196138_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196167_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 196167_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 196190_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 196190_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:57:24.83 +49:14:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.932 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196218_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 196218_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:25:21.99 +44:07:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.466 959204602520168832 096.34257438144 +44.11709696304 12.9853 11.6271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 137224_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 137224_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:18:16.29 +42:47:34.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75417_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 75417_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:03:53.72 +46:17:34.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:14:59.04 +46:47:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157613_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 157613_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 118976_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 118976_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 13408_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 13408_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:38:21.16 +50:18:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163833_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 163833_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:41:12.69 +44:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114208_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 114208_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:37:57.00 +44:41:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47690_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 47690_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:57:23.91 +48:22:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159256_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 159256_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 63593_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 63593_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 59466_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 59466_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 50811_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 50811_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 159017_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 159017_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 111171_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 111171_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 55080_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 55080_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 162505_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 162505_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 88600_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 88600_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:27:04.78 +50:07:23.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53793_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 53793_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 94834_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 94834_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 158883_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 158883_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:15:48.52 +41:02:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169188_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 169188_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:19:21.42 +41:53:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126199_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 126199_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 161576_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 161576_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:32:37.66 +41:28:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138651_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 138651_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:26:32.98 +42:55:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46369_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 46369_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 124757_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 124757_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 39411_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 39411_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:21:29.88 +43:44:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04399_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 04399_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 160506_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 160506_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 53491_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 53491_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 69975_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 69975_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 167541_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 167541_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 83697_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 83697_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 144933_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 144933_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 75263_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 75263_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 181590_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 181590_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:20:18.79 +41:18:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:59:43.97 +47:37:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162175_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 162175_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 48194_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 48194_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:13:22.36 +47:44:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 06:26:01.70 +50:29:26.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52562_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 52562_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 62592_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 62592_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 83859_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 83859_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:59:56.13 +45:56:13.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118143_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 118143_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 144551_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
Preparing report for the candidate 144551_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
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Considering the candidate 100668_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 100668_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:59:31.53 +44:56:54.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 75511_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 75511_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:16:41.22 +45:59:43.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 167147_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 167147_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:21:48.35 +41:48:17.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 157199_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083
The candidate 157199_fd_Aur-02-Q1b1x1_2026-04-06_00-12-16_20.00sec_-4.90C_LIGHTs_0083 did not pass the final checks
**** FOUND 05:20:14.54 +41:05:11.7 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 120s
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 ####
06:26:01.73 +50:29:26.9
05:27:04.78 +50:07:23.7
06:03:53.72 +46:17:34.3
05:54:05.24 +50:59:09.0
05:17:17.09 +44:00:21.7
05:33:35.13 +44:00:01.9
06:19:05.47 +43:29:07.7
05:38:54.71 +43:45:43.2
05:18:03.82 +42:02:40.3
05:22:01.28 +42:11:50.3
05:17:01.70 +43:09:38.8
06:12:08.10 +43:09:52.3
05:18:33.32 +41:04:59.6
05:41:19.88 +41:19:14.1
05:26:00.61 +41:15:17.5
05:46:54.85 +41:24:32.1
05:19:10.10 +41:22:38.5
06:03:07.87 +41:26:38.5
05:22:12.25 +41:33:53.4
05:18:22.11 +41:47:11.0
05:22:49.43 +45:00:55.2
05:14:30.05 +49:07:01.6
05:53:23.42 +46:34:58.1
05:29:36.30 +43:37:34.7
05:52:16.15 +44:59:44.4
05:22:20.46 +41:29:35.7
05:32:45.56 +49:03:59.4
06:29:54.13 +41:02:26.2
06:02:01.54 +43:50:48.4
05:38:27.46 +41:13:49.5
05:25:10.75 +47:49:05.9
05:29:47.79 +48:12:25.2
05:18:18.39 +44:55:40.5
05:37:44.47 +50:23:56.8
06:16:43.96 +44:42:40.2
05:21:36.07 +50:54:50.9
05:22:46.80 +44:44:56.2
05:42:01.50 +46:28:27.8
06:19:42.24 +42:48:49.6
05:25:48.87 +43:15:18.0
06:11:06.10 +41:55:49.3
06:12:10.12 +50:14:54.8
06:26:19.78 +41:59:09.4
05:38:23.06 +42:59:54.9
06:22:17.29 +40:31:18.8
05:28:01.12 +48:14:58.5
05:39:19.18 +44:01:50.3
06:25:49.06 +48:15:43.3
06:00:13.72 +47:43:15.3
06:38:26.60 +42:30:59.0
05:38:50.77 +49:49:58.3
05:31:00.39 +42:54:52.7
06:23:05.62 +49:11:44.3
06:12:49.78 +40:52:58.2
06:22:29.71 +44:29:26.8
05:51:18.89 +43:17:46.1
06:17:15.05 +42:06:48.2
05:46:55.56 +48:32:36.1
05:54:00.62 +48:02:58.0
05:43:00.54 +47:58:50.7
06:13:42.73 +47:37:14.5
05:25:38.76 +47:34:08.2
05:23:15.85 +47:29:09.4
05:45:47.26 +47:37:27.2
05:55:39.93 +47:30:06.3
05:34:10.23 +47:17:21.0
05:59:31.82 +46:59:51.3
05:59:57.15 +46:56:08.1
05:49:32.25 +46:35:57.7
05:48:25.41 +46:18:17.5
05:17:57.57 +45:34:35.3
06:06:03.04 +45:23:10.2
06:00:14.30 +45:04:00.4
########### 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 ####
06:26:01.73 +50:29:26.9
05:27:04.78 +50:07:23.7
06:03:53.72 +46:17:34.3
05:22:49.43 +45:00:55.2
05:14:30.05 +49:07:01.6
05:53:23.42 +46:34:58.1
05:29:36.30 +43:37:34.7
05:52:16.15 +44:59:44.4
05:22:20.46 +41:29:35.7
05:32:45.56 +49:03:59.4
06:29:54.13 +41:02:26.2
06:02:01.54 +43:50:48.4
05:38:27.46 +41:13:49.5
05:25:10.75 +47:49:05.9
05:29:47.79 +48:12:25.2
05:18:18.39 +44:55:40.5
05:37:44.47 +50:23:56.8
06:16:43.96 +44:42:40.2
05:21:36.07 +50:54:50.9
05:22:46.80 +44:44:56.2
05:42:01.50 +46:28:27.8
06:19:42.24 +42:48:49.6
05:25:48.87 +43:15:18.0
06:11:06.10 +41:55:49.3
06:12:10.12 +50:14:54.8
06:26:19.78 +41:59:09.4
05:38:23.06 +42:59:54.9
06:22:17.29 +40:31:18.8
05:28:01.12 +48:14:58.5
05:39:19.18 +44:01:50.3
06:25:49.06 +48:15:43.3
06:00:13.72 +47:43:15.3
06:38:26.60 +42:30:59.0
05:38:50.77 +49:49:58.3
05:31:00.39 +42:54:52.7
06:23:05.62 +49:11:44.3
06:12:49.78 +40:52:58.2
06:22:29.71 +44:29:26.8
05:51:18.89 +43:17:46.1
06:17:15.05 +42:06:48.2
05:18:33.32 +41:04:59.6
05:38:54.71 +43:45:43.2
05:22:12.25 +41:33:53.4
05:33:35.13 +44:00:01.9
05:43:00.54 +47:58:50.7
05:26:00.61 +41:15:17.5
05:59:57.15 +46:56:08.1
05:34:10.23 +47:17:21.0
06:13:42.73 +47:37:14.5
05:41:19.88 +41:19:14.1
05:17:17.09 +44:00:21.7
05:55:39.93 +47:30:06.3
06:03:07.87 +41:26:38.5
06:06:03.04 +45:23:10.2
05:45:47.26 +47:37:27.2
06:00:14.30 +45:04:00.4
05:22:01.28 +42:11:50.3
05:54:00.62 +48:02:58.0
05:18:03.82 +42:02:40.3
05:46:55.56 +48:32:36.1
05:54:05.24 +50:59:09.0
05:46:54.85 +41:24:32.1
05:23:15.85 +47:29:09.4
05:49:32.25 +46:35:57.7
05:18:22.11 +41:47:11.0
05:17:57.57 +45:34:35.3
06:12:08.10 +43:09:52.3
05:48:25.41 +46:18:17.5
05:19:10.10 +41:22:38.5
05:25:38.76 +47:34:08.2
05:59:31.82 +46:59:51.3
06:19:05.47 +43:29:07.7
05:17:01.70 +43:09:38.8
###################################################################################
06:26:01.73 +50:29:26.9 -- not an asteroid (will add it to exclusion list)
05:27:04.78 +50:07:23.7 -- not an asteroid (will add it to exclusion list)
06:03:53.72 +46:17:34.3 -- not an asteroid (will add it to exclusion list)
05:22:49.43 +45:00:55.2 -- not an asteroid (will add it to exclusion list)
05:14:30.05 +49:07:01.6 -- not an asteroid (will add it to exclusion list)
05:53:23.42 +46:34:58.1 -- not an asteroid (will add it to exclusion list)
05:29:36.30 +43:37:34.7 -- not an asteroid (will add it to exclusion list)
05:52:16.15 +44:59:44.4 -- not an asteroid (will add it to exclusion list)
05:22:20.46 +41:29:35.7 -- not an asteroid (will add it to exclusion list)
05:32:45.56 +49:03:59.4 -- not an asteroid (will add it to exclusion list)
06:29:54.13 +41:02:26.2 -- not an asteroid (will add it to exclusion list)
06:02:01.54 +43:50:48.4 -- not an asteroid (will add it to exclusion list)
05:38:27.46 +41:13:49.5 -- not an asteroid (will add it to exclusion list)
05:25:10.75 +47:49:05.9 -- not an asteroid (will add it to exclusion list)
05:29:47.79 +48:12:25.2 -- not an asteroid (will add it to exclusion list)
05:18:18.39 +44:55:40.5 -- not an asteroid (will add it to exclusion list)
05:37:44.47 +50:23:56.8 -- not an asteroid (will add it to exclusion list)
06:16:43.96 +44:42:40.2 -- not an asteroid (will add it to exclusion list)
05:21:36.07 +50:54:50.9 -- not an asteroid (will add it to exclusion list)
05:22:46.80 +44:44:56.2 -- not an asteroid (will add it to exclusion list)
05:42:01.50 +46:28:27.8 -- not an asteroid (will add it to exclusion list)
06:19:42.24 +42:48:49.6 -- not an asteroid (will add it to exclusion list)
05:25:48.87 +43:15:18.0 -- not an asteroid (will add it to exclusion list)
06:11:06.10 +41:55:49.3 -- not an asteroid (will add it to exclusion list)
06:12:10.12 +50:14:54.8 -- not an asteroid (will add it to exclusion list)
06:26:19.78 +41:59:09.4 -- not an asteroid (will add it to exclusion list)
05:38:23.06 +42:59:54.9 -- not an asteroid (will add it to exclusion list)
06:22:17.29 +40:31:18.8 -- not an asteroid (will add it to exclusion list)
05:28:01.12 +48:14:58.5 -- not an asteroid (will add it to exclusion list)
05:39:19.18 +44:01:50.3 -- not an asteroid (will add it to exclusion list)
06:25:49.06 +48:15:43.3 -- not an asteroid (will add it to exclusion list)
06:00:13.72 +47:43:15.3 -- not an asteroid (will add it to exclusion list)
06:38:26.60 +42:30:59.0 -- not an asteroid (will add it to exclusion list)
05:38:50.77 +49:49:58.3 -- not an asteroid (will add it to exclusion list)
05:31:00.39 +42:54:52.7 -- not an asteroid (will add it to exclusion list)
06:23:05.62 +49:11:44.3 -- not an asteroid (will add it to exclusion list)
06:12:49.78 +40:52:58.2 -- not an asteroid (will add it to exclusion list)
06:22:29.71 +44:29:26.8 -- not an asteroid (will add it to exclusion list)
05:51:18.89 +43:17:46.1 -- not an asteroid (will add it to exclusion list)
06:17:15.05 +42:06:48.2 -- not an asteroid (will add it to exclusion list)
05:18:33.32 +41:04:59.6 -- not an asteroid (will add it to exclusion list)
05:38:54.71 +43:45:43.2 -- not an asteroid (will add it to exclusion list)
05:22:12.25 +41:33:53.4 -- not an asteroid (will add it to exclusion list)
05:33:35.13 +44:00:01.9 -- not an asteroid (will add it to exclusion list)
05:43:00.54 +47:58:50.7 -- not an asteroid (will add it to exclusion list)
05:26:00.61 +41:15:17.5 -- not an asteroid (will add it to exclusion list)
05:59:57.15 +46:56:08.1 -- not an asteroid (will add it to exclusion list)
05:34:10.23 +47:17:21.0 -- not an asteroid (will add it to exclusion list)
06:13:42.73 +47:37:14.5 -- not an asteroid (will add it to exclusion list)
05:41:19.88 +41:19:14.1 -- not an asteroid (will add it to exclusion list)
05:17:17.09 +44:00:21.7 -- not an asteroid (will add it to exclusion list)
05:55:39.93 +47:30:06.3 -- not an asteroid (will add it to exclusion list)
06:03:07.87 +41:26:38.5 -- not an asteroid (will add it to exclusion list)
06:06:03.04 +45:23:10.2 -- not an asteroid (will add it to exclusion list)
05:45:47.26 +47:37:27.2 -- not an asteroid (will add it to exclusion list)
06:00:14.30 +45:04:00.4 -- not an asteroid (will add it to exclusion list)
05:22:01.28 +42:11:50.3 -- not an asteroid (will add it to exclusion list)
05:54:00.62 +48:02:58.0 -- not an asteroid (will add it to exclusion list)
05:18:03.82 +42:02:40.3 -- not an asteroid (will add it to exclusion list)
05:46:55.56 +48:32:36.1 -- not an asteroid (will add it to exclusion list)
05:54:05.24 +50:59:09.0 -- not an asteroid (will add it to exclusion list)
05:46:54.85 +41:24:32.1 -- not an asteroid (will add it to exclusion list)
05:23:15.85 +47:29:09.4 -- not an asteroid (will add it to exclusion list)
05:49:32.25 +46:35:57.7 -- not an asteroid (will add it to exclusion list)
05:18:22.11 +41:47:11.0 -- not an asteroid (will add it to exclusion list)
05:17:57.57 +45:34:35.3 -- not an asteroid (will add it to exclusion list)
06:12:08.10 +43:09:52.3 -- not an asteroid (will add it to exclusion list)
05:48:25.41 +46:18:17.5 -- not an asteroid (will add it to exclusion list)
05:19:10.10 +41:22:38.5 -- not an asteroid (will add it to exclusion list)
05:25:38.76 +47:34:08.2 -- not an asteroid (will add it to exclusion list)
05:59:31.82 +46:59:51.3 -- not an asteroid (will add it to exclusion list)
06:19:05.47 +43:29:07.7 -- not an asteroid (will add it to exclusion list)
05:17:01.70 +43:09:38.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:14:30.05 +49:07:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:01.70 +43:09:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:17.09 +44:00:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:57.57 +45:34:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:03.82 +42:02:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:18.39 +44:55:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:22.11 +41:47:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:33.32 +41:04:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:10.10 +41:22:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:36.07 +50:54:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:01.28 +42:11:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:12.25 +41:33:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:20.46 +41:29:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:46.80 +44:44:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:49.43 +45:00:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:15.85 +47:29:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:10.75 +47:49:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:38.76 +47:34:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:48.87 +43:15:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:00.61 +41:15:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.78 +50:07:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.12 +48:14:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:36.30 +43:37:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:47.79 +48:12:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:00.39 +42:54:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:45.56 +49:03:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:35.13 +44:00:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:10.23 +47:17:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:44.47 +50:23:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:23.06 +42:59:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.46 +41:13:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:50.77 +49:49:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:54.71 +43:45:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.18 +44:01:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:19.88 +41:19:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:01.50 +46:28:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:00.54 +47:58:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:47.26 +47:37:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:54.85 +41:24:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:55.56 +48:32:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:25.41 +46:18:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:32.25 +46:35:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.89 +43:17:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:16.15 +44:59:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:23.42 +46:34:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:00.62 +48:02:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:05.24 +50:59:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:39.93 +47:30:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:31.82 +46:59:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:57.15 +46:56:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:13.72 +47:43:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:14.30 +45:04:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:01.54 +43:50:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:07.87 +41:26:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:53.72 +46:17:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:03.04 +45:23:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:06.10 +41:55:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:08.10 +43:09:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.12 +50:14:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:49.78 +40:52:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:42.73 +47:37:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:43.96 +44:42:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:15.05 +42:06:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:05.47 +43:29:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:42.24 +42:48:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:17.29 +40:31:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:29.71 +44:29:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:05.62 +49:11:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:49.06 +48:15:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:01.73 +50:29:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.78 +41:59:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:54.13 +41:02:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:26.60 +42:30:59.0 -- 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)
05:14:30.05 +49:07:01.6 -- not a known variable star
05:17:01.70 +43:09:38.8 -- not a known variable star
05:17:17.09 +44:00:21.7 -- not a known variable star
05:17:57.57 +45:34:35.3 -- a known variable star
05:18:03.82 +42:02:40.3 -- not a known variable star
05:18:18.39 +44:55:40.5 -- not a known variable star
05:18:22.11 +41:47:11.0 -- not a known variable star
05:18:33.32 +41:04:59.6 -- a known variable star
05:19:10.10 +41:22:38.5 -- not a known variable star
05:21:36.07 +50:54:50.9 -- a known variable star
05:22:01.28 +42:11:50.3 -- a known variable star
05:22:12.25 +41:33:53.4 -- a known variable star
05:22:20.46 +41:29:35.7 -- a known variable star
05:22:46.80 +44:44:56.2 -- a known variable star
05:22:49.43 +45:00:55.2 -- not a known variable star
05:23:15.85 +47:29:09.4 -- a known variable star
05:25:10.75 +47:49:05.9 -- not a known variable star
05:25:38.76 +47:34:08.2 -- a known variable star
05:25:48.87 +43:15:18.0 -- a known variable star
05:26:00.61 +41:15:17.5 -- a known variable star
05:27:04.78 +50:07:23.7 -- a known variable star
05:28:01.12 +48:14:58.5 -- a known variable star
05:29:36.30 +43:37:34.7 -- a known variable star
05:29:47.79 +48:12:25.2 -- not a known variable star
05:31:00.39 +42:54:52.7 -- not a known variable star
05:32:45.56 +49:03:59.4 -- not a known variable star
05:33:35.13 +44:00:01.9 -- a known variable star
05:34:10.23 +47:17:21.0 -- a known variable star
05:37:44.47 +50:23:56.8 -- not a known variable star
05:38:23.06 +42:59:54.9 -- not a known variable star
05:38:27.46 +41:13:49.5 -- not a known variable star
05:38:50.77 +49:49:58.3 -- not a known variable star
05:38:54.71 +43:45:43.2 -- a known variable star
05:39:19.18 +44:01:50.3 -- not a known variable star
05:41:19.88 +41:19:14.1 -- a known variable star
05:42:01.50 +46:28:27.8 -- not a known variable star
05:43:00.54 +47:58:50.7 -- a known variable star
05:45:47.26 +47:37:27.2 -- a known variable star
05:46:54.85 +41:24:32.1 -- a known variable star
05:46:55.56 +48:32:36.1 -- a known variable star
05:48:25.41 +46:18:17.5 -- a known variable star
05:49:32.25 +46:35:57.7 -- a known variable star
05:51:18.89 +43:17:46.1 -- not a known variable star
05:52:16.15 +44:59:44.4 -- not a known variable star
05:53:23.42 +46:34:58.1 -- not a known variable star
05:54:00.62 +48:02:58.0 -- a known variable star
05:54:05.24 +50:59:09.0 -- a known variable star
05:55:39.93 +47:30:06.3 -- a known variable star
05:59:31.82 +46:59:51.3 -- not a known variable star
05:59:57.15 +46:56:08.1 -- not a known variable star
06:00:13.72 +47:43:15.3 -- not a known variable star
06:00:14.30 +45:04:00.4 -- a known variable star
06:02:01.54 +43:50:48.4 -- not a known variable star
06:03:07.87 +41:26:38.5 -- not a known variable star
06:03:53.72 +46:17:34.3 -- a known variable star
06:06:03.04 +45:23:10.2 -- a known variable star
06:11:06.10 +41:55:49.3 -- not a known variable star
06:12:08.10 +43:09:52.3 -- a known variable star
06:12:10.12 +50:14:54.8 -- not a known variable star
06:12:49.78 +40:52:58.2 -- not a known variable star
06:13:42.73 +47:37:14.5 -- a known variable star
06:16:43.96 +44:42:40.2 -- not a known variable star
06:17:15.05 +42:06:48.2 -- not a known variable star
06:19:05.47 +43:29:07.7 -- not a known variable star
06:19:42.24 +42:48:49.6 -- not a known variable star
06:22:17.29 +40:31:18.8 -- not a known variable star
06:22:29.71 +44:29:26.8 -- not a known variable star
06:23:05.62 +49:11:44.3 -- not a known variable star
06:25:49.06 +48:15:43.3 -- not a known variable star
06:26:01.73 +50:29:26.9 -- a known variable star
06:26:19.78 +41:59:09.4 -- not a known variable star
06:29:54.13 +41:02:26.2 -- not a known variable star
06:38:26.60 +42:30:59.0 -- a known variable star
Found 39 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
73 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 73 (excluding asteroids and hot pixels, 39 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)2461136.71617378 -observatory V36
23:20:30.65 -06:25:03.9 Mercury (0.3mag)
02:21:36.43 +13:51:37.9 Venus (-3.9mag)
23:49:58.34 -02:12:10.4 Mars (1.2mag)
07:08:42.69 +22:52:26.0 Jupiter (-2.2mag)
00:24:46.29 +00:21:17.3 Saturn (0.9mag)
03:45:43.61 +19:41:06.4 Uranus (5.8mag)
00:09:31.96 -00:23:39.2 Neptune (7.8mag)
20:33:14.25 -22:52:29.4 Pluto (14.5mag)
16:00:15.72 -26:13:24.2 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 6 00:15 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461136.71617378:
07:08:46.03 +22:52:16.7 Io (5.7mag)
07:08:55.36 +22:51:59.4 Europa (5.8mag)
07:08:37.46 +22:52:43.5 Ganymede (5.3mag)
07:08:12.85 +22:53:17.8 Callisto (6.5mag)
07:12:25.59 +22:44:55.4 Himalia (15.3mag)
07:08:40.54 +22:52:32.3 Thebe (16.2mag)
07:12:23.32 +23:13:41.8 Elara (17.2mag)
07:06:55.61 +23:37:33.7 Pasiphae (17.3mag)
07:17:14.48 +22:49:22.3 Carme (18.4mag)
00:24:41.03 +00:21:18.4 Titan (8.8mag)
00:24:43.07 +00:21:31.4 Rhea (10.1mag)
00:24:46.81 +00:22:50.7 Iapetus (11.5mag)
00:24:48.14 +00:21:05.6 Hyperion (14.8mag)
00:26:30.50 +00:31:06.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 00:15 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.71617378:
14:47:24.31 -08:20:36.1 JWST
17:02:04.87 +44:53:05.1 Chandra
08:03:00.04 -39:17:34.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 00:15 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.71617378 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:08.39 -28:14:12.3 14.0mag P/2010 H2 (Vales)
05:00:06.07 -70:08:47.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:34.40 +31:22:34.0 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.73 +09:22:23.1 17.6mag C/2021 G2 (ATLAS)
23:07:21.59 +28:52:08.0 17.0mag C/2022 E2 (ATLAS)
04:18:01.19 +25:45:54.0 15.9mag C/2022 N2 (PANSTARRS)
09:01:52.09 +31:54:25.2 16.1mag C/2022 QE78 (ATLAS)
08:29:59.28 -01:13:47.5 17.3mag C/2022 R6 (PANSTARRS)
18:55:35.15 +17:41:49.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:30.29 -11:39:36.6 17.6mag P/2023 B1 (PANSTARRS)
09:12:49.32 -13:29:56.5 17.5mag C/2023 F3 (ATLAS)
21:43:30.29 +62:22:21.0 17.5mag C/2023 H5 (Lemmon)
19:26:23.79 -03:36:31.5 14.3mag C/2023 R1 (PANSTARRS)
21:42:38.48 +84:36:50.2 17.8mag C/2023 X2 (Lemmon)
06:14:32.05 +63:35:00.6 17.0mag C/2024 A1 (ATLAS)
04:51:07.45 +14:33:59.0 10.4mag C/2024 E1 (Wierzchos)
16:25:05.38 +04:46:54.5 17.4mag C/2024 G6 (ATLAS)
20:17:33.50 +12:41:23.5 14.7mag C/2024 J3 (ATLAS)
03:17:47.24 -23:55:08.3 16.4mag C/2024 T5 (ATLAS)
05:08:43.41 +47:49:41.0 17.7mag C/2025 J1 (Borisov)
14:19:00.32 +37:24:58.4 14.8mag C/2025 L1 (ATLAS)
03:10:24.23 -24:45:08.9 17.8mag C/2025 Q3 (ATLAS)
22:53:38.50 +19:50:14.1 10.1mag C/2025 R3 (PANSTARRS)
12:58:22.87 +02:23:37.6 17.5mag C/2025 Y1 (ATLAS)
01:31:28.19 +04:42:14.0 7.2mag C/2026 A1 (MAPS)
23:30:52.92 +35:14:57.5 14.3mag C/2026 B2 (Sun-Gao)
18:23:50.35 -10:13:02.0 12.4mag 10P/Tempel
15:12:52.46 +04:06:36.4 13.1mag 24P/Schaumasse
11:05:45.76 -01:51:46.5 15.7mag 29P/Schwassmann-Wachmann
17:56:46.57 -09:59:31.2 17.7mag 40P/Vaisala
10:38:52.70 -04:56:45.1 16.7mag 43P/Wolf-Harrington
01:33:35.42 +15:48:01.4 17.1mag 47P/Ashbrook-Jackson
06:53:22.40 +39:04:32.7 17.0mag 63P/Wild
23:16:20.48 -12:39:07.0 15.7mag 65P/Gunn
03:37:44.38 +17:44:49.5 15.8mag 76P/West-Kohoutek-Ikemura
00:44:07.98 +06:17:24.3 14.4mag 78P/Gehrels
22:32:37.62 -12:15:51.5 14.5mag 88P/Howell
01:43:14.31 +17:57:15.9 15.1mag 93P/Lovas
04:36:58.15 +31:43:47.3 16.3mag 123P/West-Hartley
08:17:57.29 +42:52:46.2 16.2mag 124P/Mrkos
02:18:15.29 +13:15:35.4 16.4mag 128P/Shoemaker-Holt
02:28:26.78 +13:15:25.0 17.5mag 131P/Mueller
00:36:00.32 +09:37:10.7 11.2mag 141P/Machholz
00:45:58.66 +01:12:32.8 11.3mag 141P-A/Machholz
23:36:31.95 -02:24:54.4 14.0mag 141P-D/Machholz
01:15:06.17 +02:52:27.2 17.9mag 141P-I/Machholz
00:35:12.34 -06:24:20.3 15.2mag 162P/SidingSpring
10:30:58.11 +31:30:17.7 17.8mag 164P/Christensen
06:18:28.49 +24:31:21.1 17.8mag 198P/ODAS
15:08:39.54 -01:11:33.1 17.4mag 210P/Christensen
21:08:59.68 -13:48:55.6 17.4mag 218P/LINEAR
17:12:37.05 -15:04:13.2 16.2mag 235P/LINEAR
05:13:42.65 +33:51:30.3 16.6mag 240P/NEAT
07:34:12.61 -06:17:02.5 17.6mag 242P/Spahr
15:45:55.91 +06:18:39.7 17.5mag 391P/Kowalski
07:30:55.49 +21:18:42.6 17.6mag 450P/LONEOS
05:21:57.05 +45:36:35.5 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 00:15 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 6 00:15 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 6 00:15 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
13:18:12.570 +29:05:16.56 AT 2026htq 2026-03-15.74 21.89
-rw-r--r-- 1 apache apache 30K Apr 6 00:15 tns_transients_list.txt
