This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc
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
ATO J082.3479+41.9432,2461136.6603,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J082.3479+41.9432 20260406.1603 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RS Aur,2461136.6603,8.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 8.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.7196+45.7293,2461136.6603,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.7196+45.7293 20260406.1603 13.45CV 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
target,2461136.6603,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.9390+42.9664,2461136.6603,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J089.9390+42.9664 20260406.1603 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209630073751279872,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 209630073751279872 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962623667068486144,2461136.6603,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 962623667068486144 20260406.1603 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.5183+47.0541,2461136.6603,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.5183+47.0541 20260406.1603 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.5748+43.1206,2461136.6603,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J082.5748+43.1206 20260406.1603 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,2461136.6603,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 969934835279075072,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 969934835279075072 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196620789610015744,2461136.6603,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 196620789610015744 20260406.1603 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.4778+43.6460,2461136.6603,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.4778+43.6460 20260406.1603 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
target,2461136.6603,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 957014684595431168,2461136.6603,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 957014684595431168 20260406.1603 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.1356+41.6818,2461136.6603,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J082.1356+41.6818 20260406.1603 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J052640.34+442519.6,2461136.6603,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J052640.34+442519.6 20260406.1603 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
target,2461136.6603,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.7332+42.1358,2461136.6603,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.7332+42.1358 20260406.1603 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3290+41.8878,2461136.6603,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J093.3290+41.8878 20260406.1603 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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,2461136.6603,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 191398418616402432,2461136.6603,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 191398418616402432 20260406.1603 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 J081.4213+45.9147,2461136.6603,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.4213+45.9147 20260406.1603 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
ATO J084.5690+41.6427,2461136.6603,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J084.5690+41.6427 20260406.1603 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 J092.7750+41.9301,2461136.6603,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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,2461136.6603,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
ATO J095.4512+46.7771,2461136.6603,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J095.4512+46.7771 20260406.1603 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 11.97CV 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
Gaia DR3 958745075379052800,2461136.6603,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 958745075379052800 20260406.1603 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
Gaia DR3 967138094309568128,2461136.6603,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 967138094309568128 20260406.1603 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967525667862574848,2461136.6603,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J095.6271+46.1946,2461136.6603,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J095.6271+46.1946 20260406.1603 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.5883+42.9989,2461136.6603,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
ATO J084.5883+42.9989,2461136.6603,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
ATO J095.6162+44.4906,2461136.6603,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.2659+42.5465,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J096.2659+42.5465 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J061756.72+460440.3,2461136.6603,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J061756.72+460440.3 20260406.1603 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
target,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193078403663338240,2461136.6603,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 193078403663338240 20260406.1603 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
ATO J099.6086+44.3324,2461136.6603,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.6086+44.3324 20260406.1603 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1509+45.4814,2461136.6603,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J089.1509+45.4814 20260406.1603 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.8155+42.6981,2461136.6603,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J090.8155+42.6981 20260406.1603 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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,2461136.6603,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970601104965241472,2461136.6603,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 970601104965241472 20260406.1603 13.25CV 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
ATO J097.4331+43.4722,2461136.6603,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.4331+43.4722 20260406.1603 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062211.34+473940.0,2461136.6603,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J062211.34+473940.0 20260406.1603 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.1603 2461136.6603 13.48 06:25:07.90 +48:56:16.1
165.70528 16.07254 galactic Aur Second-epoch detections are separated by 1.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 970575064579845120 | 06:25:07.56 +48:55:44.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G5 (LAMOST DR5) J-Ks=0.612+/-0.039 (K)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
Large-amplitude variable Gaia DR2 970575064579845120,2461136.6603,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 970575064579845120 20260406.1603 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.79CV 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
target,2461136.6603,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6603,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CGCS 6107,2461136.6603,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053410.05+471722.3,2461136.6603,9.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 9.22CV 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
NSVS 4445192,2461136.6603,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4445192 20260406.1603 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053335.18+440000.9,2461136.6603,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0525385+473410,2461136.6603,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4452455,2461136.6603,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0545473+473728,2461136.6603,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 02922-01985,2461136.6603,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
ASASSN-V J053052.29+435055.3,2461136.6603,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J053052.29+435055.3 20260406.1603 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
target,2461136.6603,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
NSVS J0546556+483237,2461136.6603,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 11.31CV 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
ASASSN-V J054825.45+461817.6,2461136.6603,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.1603 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
ZTF J052919.17+431550.8,2461136.6603,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J052919.17+431550.8 20260406.1603 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
## 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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461136.66059405 06.04.2026 03:51:05.326 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 48
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 19782
Objects passed selection criteria: 19754
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 18210.2
Average stars matched: 17580.2 (96.5404 %)
Memory usage VmPeak: 126488 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 Sun Apr 5 23:10:56 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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461136.66059405 06.04.2026 03:51:05.326 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 287
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 94 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): 135474
Objects passed selection criteria: 135187
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 119702
Average stars matched: 115745 (96.6939 %)
Memory usage VmPeak: 2033356 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 Sun Apr 5 23:14:26 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/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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: 2461136.66000987
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits'
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:02.305 +46:00:21.72
Angular distance between the image centers 0.0421 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:04.753 +46:00:20.91
Angular distance between the image centers 0.0492 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:02.305 +46:00:21.72
Second-epoch second image center 06:00:04.753 +46:00:20.91
Angular distance between the image centers 0.00709 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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.C3L1ejDwNw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.5UnnAVCytR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits &> /tmp/tmp.VBzw4nJR8d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits &> /tmp/tmp.Fy9zE1Wh5r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_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 33 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.9 pix fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
2.9 pix fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
15.0 mag. fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
15.0 mag. fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.C3L1ejDwNw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.5UnnAVCytR (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.VBzw4nJR8d (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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2055, passed=19886
Got 19886 stars (including 17821 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat
util/solve_plate_with_UCAC5 got 19886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 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: 933 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 19288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 19288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 19288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.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.Fy9zE1Wh5r (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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1976, passed=19888
Got 19888 stars (including 17903 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 19888 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 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 651 to 708 (Dec 40.3 to 51.3)
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: 930 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 19462 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
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 651 to 708 (Dec 40.3 to 51.3)
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(), 19463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 19463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out09969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31196.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 31195_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31195_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:33:58.44 +49:58:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31196_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 31196_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 31324_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31324_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:59:43.38 +44:59:09.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31328_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31328_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:14:58.93 +46:47:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31440_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31440_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:43.02 +43:37:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31464_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31464_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:23.92 +48:22:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31497_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31497_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:33:22.71 +44:56:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.040 965094475854599936 098.34501577089 +44.94719408903 11.9474 11.2883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31509_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31509_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:09:51.75 +46:34:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.481 963406141390333184 092.46702943046 +46.57449767313 10.4625 8.8819 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31519_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31519_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:48:25.50 +46:18:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.695 197948278101166080 087.10599538582 +46.30486477628 10.9482 9.5176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31521_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31521_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:11:34.29 +48:44:36.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31522_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31522_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:13:22.44 +47:44:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31537_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31537_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:53.38 +46:49:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.676 968702905516098176 094.47268230885 +46.82026918802 11.9395 11.2437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31539_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31539_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:35:20.92 +45:39:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.379 965502085432232832 098.83730061204 +45.66028508244 12.0537 11.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31541_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31541_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:06:11.21 +47:25:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.010 969681535286381312 091.54712051726 +47.42216425873 12.0045 11.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31545_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31545_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:04:29.91 +43:09:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.502 961254401433213440 091.12410745222 +43.15702779599 12.3767 11.8423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31565_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31565_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:19.36 +45:53:01.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 31566_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31566_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:06:32.41 +48:42:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.495 969672464315450752 091.63600844831 +48.71267373519 12.0182 11.4092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31573_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31573_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:19:01.64 +47:35:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.973 969127278346770560 094.75723151051 +47.58338683419 12.0379 11.3364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31574_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31574_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:28:45.81 +48:34:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.548 967547868550025216 097.19110438442 +48.57701626020 12.2587 11.7628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31589_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31589_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:13:13.52 +46:41:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.054 968656687370081664 093.30631491750 +46.69665373893 12.1592 11.6339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31592_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31592_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:05:59.68 +46:32:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.635 963535475742766720 091.49876147334 +46.54044169762 12.2781 12.2514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31600_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31600_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:53:58.79 +49:52:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.104 211530575302864000 088.49486643244 +49.87363707682 11.0314 9.5472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31603_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31603_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:23:59.35 +50:01:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.356 970735661996851328 095.99711490452 +50.02155372410 12.3351 11.6239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31604_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31604_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:47.42 +47:37:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.024 209955048156786816 086.44725145162 +47.62439783660 11.1541 9.7804 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31612_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31612_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:22:58.66 +43:29:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.862 962081985793160064 095.74474387713 +43.48428034006 12.3690 11.9302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31614_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31614_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:21:33.13 +48:36:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.038 969099034643074176 095.38846833306 +48.60808700256 12.1105 11.3567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31616_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31616_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:55:39.96 +47:30:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.528 198116400300941440 088.91652348569 +47.50163196744 11.2016 9.7643 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31621_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31621_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:48.64 +45:31:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.935 962540653942188672 094.45298862422 +45.52468404500 12.2441 11.7736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31630_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31630_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:56:01.53 +45:16:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.733 196901195139135616 089.00656955459 +45.27723816857 11.6596 10.6140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31632_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31632_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:12:38.23 +47:22:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.486 968789938733063296 093.15928054013 +47.36916252029 12.1836 11.4611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31637_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31637_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:12:35.11 +45:58:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.495 962606074882449920 093.14648896912 +45.96717746347 12.0488 11.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31651_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 31651_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:10:20.90 +45:46:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.739 963262861282486656 092.58734909325 +45.77231020442 12.1039 11.4113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09969_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 09969_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 18s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:03:53.66 +46:17:34.9
05:29:22.21 +41:56:48.0
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits exists and is non-empty
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:02.305 +46:00:21.72
Angular distance between the image centers 0.0421 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:04.753 +46:00:20.91
Angular distance between the image centers 0.0492 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:00:02.305 +46:00:21.72
Second-epoch second image center 06:00:04.753 +46:00:20.91
Angular distance between the image centers 0.00709 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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.Mmzj0umr4s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.HBe0lvpmAZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits &> /tmp/tmp.pXi73CryfH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits &> /tmp/tmp.EkZOVHzFQq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_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.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 157 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.8 pix fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
2.8 pix fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.0 mag. fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
14.0 mag. fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Mmzj0umr4s (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.HBe0lvpmAZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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=44, blended=20075, passed=170060
Got 170060 stars (including 149712 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170060 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166998 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(), 166995 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(), 166995 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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.pXi73CryfH (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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=16229, passed=108046
Got 108046 stars (including 91724 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat
util/solve_plate_with_UCAC5 got 108046 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 105383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 105383 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 105381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.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.EkZOVHzFQq (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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=16128, passed=108173
Got 108173 stars (including 91964 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 108173 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 936 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: 933 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 106093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 106093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 106089 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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-Q2b1x1_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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-50-14_20.00sec_-5.00C_LIGHT_0093.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.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_2026-04-05_CI_Aur-02-Q2b1x1_225141_TTUQ2b1x1_11444_hyiv1xKc/wcs_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out143547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out193246.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out114208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59466.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
make_report_in_HTML.sh Phase 1 (network queries): 122s
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: 54s
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Considering the candidate 193147_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193147_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193153_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193153_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193154_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193154_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193165_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193165_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 193167_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193167_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193186_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193186_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193192_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193192_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193203_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193203_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193206_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193206_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193208_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193208_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:34:14.60 +41:35:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.995 194390498993755520 083.56205224695 +41.59275967874 13.7932 12.9960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193214_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193214_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:29:12.47 +41:48:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.214 194557796560271232 082.30342261931 +41.81081221937 13.0785 12.4346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193215_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193215_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:34:54.44 +41:59:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.973 194468942275982464 083.72741186821 +41.99479886195 13.4382 12.8182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193219_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193219_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193220_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193220_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:25:19.83 +45:55:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.298 208953148247641088 081.33351171919 +45.93080327383 13.0976 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193226_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193226_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193227_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193227_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:25:57.14 +44:48:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.300 208042134144553728 081.48943397320 +44.81178688210 13.1424 12.5493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193228_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193228_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193234_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193234_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193239_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193239_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193242_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193242_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:28:31.77 +44:31:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.552 207842439643428608 082.13290664695 +44.53304441652 13.3613 12.8704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193243_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193243_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:28:05.20 +41:51:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.063 194584803314683648 082.02058041384 +41.86520840978 12.9686 12.4554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193245_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193245_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193246_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193246_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:27:47.33 +43:26:53.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 193250_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193250_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193251_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193251_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193253_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193253_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:27:49.43 +42:36:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 2.395 195427918276928000 081.95634841222 +42.61198917573 13.0955 12.6192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193254_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193254_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193257_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193257_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193266_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193266_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193268_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193268_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193270_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193270_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:38.40 +42:29:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.923 192981818439022976 086.41053095514 +42.49285014338 13.6163 12.6787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193273_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193273_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:31:37.85 +41:27:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.683 194344972340231808 082.90636024770 +41.46586618038 13.1153 12.0565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193275_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193275_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193276_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193276_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:34:29.28 +41:50:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.706 194441591924304128 083.62153400813 +41.84813882000 13.2269 12.3848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193278_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193278_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193279_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193279_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193280_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193280_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:36:40.75 +49:11:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193288_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193288_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193307_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193307_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:29:22.12 +41:54:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.835 194605659675784320 082.34209376028 +41.90018664058 12.6280 12.1139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193309_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193309_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193312_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193312_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193313_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193313_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193323_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193323_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:52:03.99 +49:32:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193329_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193329_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:26:53.29 +43:56:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193330_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193330_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 193335_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193335_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193340_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193340_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:15.62 +41:56:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.618 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193343_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193343_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 193347_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193347_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:29:21.26 +41:49:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.833 194557727840783744 082.33958376411 +41.81900533891 12.3438 11.8326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193354_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193354_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193356_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193356_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 193357_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193357_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 193366_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193366_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193370_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193370_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 193374_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193374_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:29:21.89 +41:56:47.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193619_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193619_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:42.99 +43:37:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193690_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193690_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:11:34.46 +48:44:35.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193874_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193874_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:37:43.96 +45:09:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193966_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 193966_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 193977_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 193977_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:13:46.53 +44:43:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194000_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194000_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:36:52.18 +44:44:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194024_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194024_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194063_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194063_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:13:41.86 +45:31:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.156 962485506560815104 093.42562997977 +45.51967529314 11.4649 9.7766 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194099_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194099_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:05:50.11 +44:39:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194195_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194195_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194200_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194200_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194203_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194203_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:03:13.47 +42:56:26.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194251_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194251_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:28.65 +45:52:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.535 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194265_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194265_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 194289_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194289_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194329_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194329_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:34.50 +46:23:45.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194357_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194357_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:11:49.18 +45:03:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.730 963207786918929408 092.95523434237 +45.05495257659 13.4231 12.7204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194359_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194359_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194375_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194375_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194377_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194377_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:30.03 +44:44:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194384_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194384_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:11:00.88 +47:29:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194544_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194544_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194572_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194572_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:06.21 +44:51:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194578_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194578_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194590_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194590_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:14.05 +50:00:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194601_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194601_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:25:57.47 +43:06:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.523 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194621_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194621_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194623_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194623_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:56:30.68 +46:14:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.818 197751809117411712 089.12908358575 +46.24714326154 13.6175 12.8385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194629_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194629_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:33:57.02 +46:11:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194642_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194642_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:25:45.33 +45:22:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194657_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194657_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:52:20.96 +42:50:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194667_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194667_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:28:45.57 +49:11:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194680_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194680_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194687_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194687_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194691_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194691_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194722_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194722_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:00:13.77 +47:43:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194733_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194733_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 194739_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194739_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194741_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194741_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194757_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194757_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194771_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194771_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:15.18 +42:06:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194804_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194804_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194806_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194806_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194823_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194823_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194829_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194829_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194851_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194851_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:46:39.79 +43:21:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.162 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194854_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194854_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:39.91 +43:57:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194873_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194873_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194898_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 194898_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:08:19.01 +41:46:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194903_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194903_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194917_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194917_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194924_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194924_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 194979_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 194979_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195009_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195009_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:08:04.80 +45:02:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.103 962871027122871040 092.02043346573 +45.03427793519 13.9306 13.3249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195011_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195011_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195042_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195042_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195050_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195050_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195054_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195054_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:12:19.67 +50:12:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195060_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195060_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195063_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195063_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:26:12.58 +49:06:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.400 970669347702108288 096.55228667167 +49.11057778149 13.8025 12.7263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195078_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195078_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:24.79 +49:14:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.448 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195100_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195100_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195128_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195128_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:27.98 +47:51:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.140 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195233_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195233_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195249_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195249_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195254_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195254_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:25:22.02 +44:07:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.173 959204602520168832 096.34257438144 +44.11709696304 12.9853 11.6271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195292_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195292_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195298_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195298_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195416_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195416_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195443_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195443_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195463_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195463_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195482_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195482_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195510_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195510_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195512_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195512_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:20:38.12 +44:44:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.926 962295089187534080 095.15952019092 +44.74827521966 14.7389 14.1190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195530_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195530_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:18:12.28 +42:25:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.154 960105480500646528 094.55157956652 +42.41948448381 14.6678 13.7716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195535_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195535_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:34:58.71 +49:41:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 4.950 967942558864680832 098.74639018076 +49.69009938631 14.5201 13.5004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195538_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195538_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195562_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 195562_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 195642_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 195642_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 75417_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 75417_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:03:53.69 +46:17:34.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 68382_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 68382_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 69975_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 69975_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 59466_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 59466_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 37886_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 37886_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:59:44.06 +47:37:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114208_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 114208_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 52562_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 52562_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 48194_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 48194_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:13:22.40 +47:44:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:57.23 +44:41:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47690_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 47690_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 143547_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 143547_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:26:50.48 +43:12:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.674 195657273827629184 081.70911664199 +43.20722736772 12.9351 12.1541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56237_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 56237_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:23.95 +48:22:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53793_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 53793_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
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Considering the candidate 118976_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 118976_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116553_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 116553_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18647_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 18647_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39411_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 39411_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75263_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 75263_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
**** FOUND 06:14:58.91 +46:47:46.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143937_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
Preparing report for the candidate 143937_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84847_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094
The candidate 84847_fd_Aur-02-Q2b1x1_2026-04-05_22-51-05_20.00sec_-5.00C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 180s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:03:53.66 +46:17:34.9
05:29:22.21 +41:56:48.0
05:33:35.60 +44:00:04.8
05:30:53.09 +43:50:50.2
05:38:54.92 +43:45:45.7
05:29:19.59 +43:15:50.9
05:34:25.67 +49:54:08.6
05:42:51.49 +45:43:44.7
05:56:51.64 +43:51:24.0
06:25:07.57 +45:26:09.4
05:59:46.70 +42:58:02.2
05:41:41.66 +46:17:27.7
06:14:05.52 +46:10:08.6
05:50:05.07 +47:03:25.5
05:57:42.18 +42:08:18.6
05:33:56.30 +44:18:19.6
06:29:36.03 +44:18:38.4
05:30:19.43 +43:07:57.7
05:39:55.28 +46:26:23.1
06:02:17.27 +49:12:47.0
05:55:59.21 +44:31:37.9
05:33:54.48 +43:39:02.7
05:37:53.94 +45:12:06.1
05:43:48.52 +48:57:27.7
06:22:26.34 +41:45:15.7
05:28:35.16 +41:41:18.8
05:26:39.86 +44:25:14.5
05:40:46.61 +41:59:38.2
05:38:54.01 +42:08:09.4
06:13:18.96 +41:52:43.5
05:26:15.66 +44:02:47.0
06:36:45.28 +42:57:52.8
05:37:43.69 +41:40:08.7
05:25:42.14 +45:54:21.6
05:38:17.06 +41:38:39.4
06:11:05.95 +41:55:48.5
06:25:09.18 +41:48:31.5
06:21:48.15 +46:46:30.9
06:29:20.82 +45:46:47.2
06:32:53.61 +42:26:18.2
06:12:10.05 +50:14:54.6
06:40:11.18 +49:27:38.2
06:25:48.98 +48:15:45.0
05:40:42.61 +48:20:00.6
06:22:30.62 +46:12:18.0
05:38:22.71 +42:59:57.1
05:38:23.72 +42:59:53.3
06:22:29.70 +44:29:25.8
06:25:04.79 +42:33:12.8
06:17:58.86 +46:05:16.1
06:26:29.53 +49:54:10.9
06:17:09.73 +47:00:37.6
05:39:18.88 +44:01:48.1
06:13:29.59 +47:17:45.2
05:46:47.33 +43:03:07.2
06:38:26.60 +44:19:50.9
06:11:51.61 +45:03:23.3
06:03:20.88 +42:41:50.4
05:51:18.76 +43:17:46.8
06:23:09.72 +49:10:02.2
05:56:33.72 +45:29:09.2
06:03:18.88 +42:41:42.3
06:34:46.37 +45:56:36.5
05:57:11.25 +42:50:26.7
05:43:56.07 +47:43:50.3
06:21:46.38 +48:41:42.8
06:29:45.09 +43:28:18.8
06:22:14.67 +47:39:08.3
06:25:07.90 +48:56:16.1
06:31:49.42 +49:27:24.3
06:11:58.25 +44:42:24.6
06:11:00.59 +43:04:00.2
06:27:36.22 +50:07:55.7
06:25:12.22 +43:57:33.0
06:37:04.08 +47:59:59.1
06:32:48.50 +42:28:50.6
06:32:39.94 +45:40:37.4
06:17:58.01 +47:16:16.7
05:35:44.89 +48:35:19.3
05:46:55.66 +48:32:35.5
05:43:00.68 +47:58:51.1
05:25:39.23 +47:34:08.4
05:45:47.38 +47:37:27.1
05:34:10.59 +47:17:21.5
05:49:32.31 +46:35:57.6
05:48:25.46 +46:18:17.7
########### Completed Aur-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:29:22.21 +41:56:48.0
06:03:53.66 +46:17:34.9
05:42:51.49 +45:43:44.7
05:56:51.64 +43:51:24.0
06:25:07.57 +45:26:09.4
05:59:46.70 +42:58:02.2
05:41:41.66 +46:17:27.7
06:14:05.52 +46:10:08.6
05:50:05.07 +47:03:25.5
05:57:42.18 +42:08:18.6
05:33:56.30 +44:18:19.6
06:29:36.03 +44:18:38.4
05:30:19.43 +43:07:57.7
05:39:55.28 +46:26:23.1
06:02:17.27 +49:12:47.0
05:55:59.21 +44:31:37.9
05:33:54.48 +43:39:02.7
05:37:53.94 +45:12:06.1
05:43:48.52 +48:57:27.7
06:22:26.34 +41:45:15.7
05:28:35.16 +41:41:18.8
05:26:39.86 +44:25:14.5
05:40:46.61 +41:59:38.2
05:38:54.01 +42:08:09.4
06:13:18.96 +41:52:43.5
05:26:15.66 +44:02:47.0
06:36:45.28 +42:57:52.8
05:37:43.69 +41:40:08.7
05:25:42.14 +45:54:21.6
05:38:17.06 +41:38:39.4
06:11:05.95 +41:55:48.5
06:25:09.18 +41:48:31.5
06:21:48.15 +46:46:30.9
06:29:20.82 +45:46:47.2
06:32:53.61 +42:26:18.2
06:12:10.05 +50:14:54.6
06:40:11.18 +49:27:38.2
06:25:48.98 +48:15:45.0
05:40:42.61 +48:20:00.6
06:22:30.62 +46:12:18.0
05:38:22.71 +42:59:57.1
05:38:23.72 +42:59:53.3
06:22:29.70 +44:29:25.8
06:25:04.79 +42:33:12.8
06:17:58.86 +46:05:16.1
06:26:29.53 +49:54:10.9
06:17:09.73 +47:00:37.6
05:39:18.88 +44:01:48.1
06:13:29.59 +47:17:45.2
05:46:47.33 +43:03:07.2
06:38:26.60 +44:19:50.9
06:11:51.61 +45:03:23.3
06:03:20.88 +42:41:50.4
05:51:18.76 +43:17:46.8
06:23:09.72 +49:10:02.2
05:56:33.72 +45:29:09.2
06:03:18.88 +42:41:42.3
06:34:46.37 +45:56:36.5
05:57:11.25 +42:50:26.7
05:43:56.07 +47:43:50.3
06:21:46.38 +48:41:42.8
06:29:45.09 +43:28:18.8
06:22:14.67 +47:39:08.3
06:25:07.90 +48:56:16.1
06:31:49.42 +49:27:24.3
06:11:58.25 +44:42:24.6
06:11:00.59 +43:04:00.2
06:27:36.22 +50:07:55.7
06:25:12.22 +43:57:33.0
06:37:04.08 +47:59:59.1
06:32:48.50 +42:28:50.6
06:32:39.94 +45:40:37.4
06:17:58.01 +47:16:16.7
05:49:32.31 +46:35:57.6
05:34:10.59 +47:17:21.5
05:35:44.89 +48:35:19.3
05:33:35.60 +44:00:04.8
05:25:39.23 +47:34:08.4
05:43:00.68 +47:58:51.1
05:45:47.38 +47:37:27.1
05:38:54.92 +43:45:45.7
05:30:53.09 +43:50:50.2
05:34:25.67 +49:54:08.6
05:46:55.66 +48:32:35.5
05:48:25.46 +46:18:17.7
05:29:19.59 +43:15:50.9
###################################################################################
05:29:22.21 +41:56:48.0 -- not an asteroid (will add it to exclusion list)
06:03:53.66 +46:17:34.9 -- not an asteroid (will add it to exclusion list)
05:42:51.49 +45:43:44.7 -- not an asteroid (will add it to exclusion list)
05:56:51.64 +43:51:24.0 -- not an asteroid (will add it to exclusion list)
06:25:07.57 +45:26:09.4 -- not an asteroid (will add it to exclusion list)
05:59:46.70 +42:58:02.2 -- not an asteroid (will add it to exclusion list)
05:41:41.66 +46:17:27.7 -- not an asteroid (will add it to exclusion list)
06:14:05.52 +46:10:08.6 -- not an asteroid (will add it to exclusion list)
05:50:05.07 +47:03:25.5 -- not an asteroid (will add it to exclusion list)
05:57:42.18 +42:08:18.6 -- not an asteroid (will add it to exclusion list)
05:33:56.30 +44:18:19.6 -- not an asteroid (will add it to exclusion list)
06:29:36.03 +44:18:38.4 -- not an asteroid (will add it to exclusion list)
05:30:19.43 +43:07:57.7 -- not an asteroid (will add it to exclusion list)
05:39:55.28 +46:26:23.1 -- not an asteroid (will add it to exclusion list)
06:02:17.27 +49:12:47.0 -- not an asteroid (will add it to exclusion list)
05:55:59.21 +44:31:37.9 -- not an asteroid (will add it to exclusion list)
05:33:54.48 +43:39:02.7 -- not an asteroid (will add it to exclusion list)
05:37:53.94 +45:12:06.1 -- not an asteroid (will add it to exclusion list)
05:43:48.52 +48:57:27.7 -- not an asteroid (will add it to exclusion list)
06:22:26.34 +41:45:15.7 -- not an asteroid (will add it to exclusion list)
05:28:35.16 +41:41:18.8 -- not an asteroid (will add it to exclusion list)
05:26:39.86 +44:25:14.5 -- not an asteroid (will add it to exclusion list)
05:40:46.61 +41:59:38.2 -- not an asteroid (will add it to exclusion list)
05:38:54.01 +42:08:09.4 -- not an asteroid (will add it to exclusion list)
06:13:18.96 +41:52:43.5 -- not an asteroid (will add it to exclusion list)
05:26:15.66 +44:02:47.0 -- not an asteroid (will add it to exclusion list)
06:36:45.28 +42:57:52.8 -- not an asteroid (will add it to exclusion list)
05:37:43.69 +41:40:08.7 -- not an asteroid (will add it to exclusion list)
05:25:42.14 +45:54:21.6 -- not an asteroid (will add it to exclusion list)
05:38:17.06 +41:38:39.4 -- not an asteroid (will add it to exclusion list)
06:11:05.95 +41:55:48.5 -- not an asteroid (will add it to exclusion list)
06:25:09.18 +41:48:31.5 -- not an asteroid (will add it to exclusion list)
06:21:48.15 +46:46:30.9 -- not an asteroid (will add it to exclusion list)
06:29:20.82 +45:46:47.2 -- not an asteroid (will add it to exclusion list)
06:32:53.61 +42:26:18.2 -- not an asteroid (will add it to exclusion list)
06:12:10.05 +50:14:54.6 -- not an asteroid (will add it to exclusion list)
06:40:11.18 +49:27:38.2 -- not an asteroid (will add it to exclusion list)
06:25:48.98 +48:15:45.0 -- not an asteroid (will add it to exclusion list)
05:40:42.61 +48:20:00.6 -- not an asteroid (will add it to exclusion list)
06:22:30.62 +46:12:18.0 -- not an asteroid (will add it to exclusion list)
05:38:22.71 +42:59:57.1 -- not an asteroid (will add it to exclusion list)
05:38:23.72 +42:59:53.3 -- not an asteroid (will add it to exclusion list)
06:22:29.70 +44:29:25.8 -- not an asteroid (will add it to exclusion list)
06:25:04.79 +42:33:12.8 -- not an asteroid (will add it to exclusion list)
06:17:58.86 +46:05:16.1 -- not an asteroid (will add it to exclusion list)
06:26:29.53 +49:54:10.9 -- not an asteroid (will add it to exclusion list)
06:17:09.73 +47:00:37.6 -- not an asteroid (will add it to exclusion list)
05:39:18.88 +44:01:48.1 -- not an asteroid (will add it to exclusion list)
06:13:29.59 +47:17:45.2 -- not an asteroid (will add it to exclusion list)
05:46:47.33 +43:03:07.2 -- not an asteroid (will add it to exclusion list)
06:38:26.60 +44:19:50.9 -- not an asteroid (will add it to exclusion list)
06:11:51.61 +45:03:23.3 -- not an asteroid (will add it to exclusion list)
06:03:20.88 +42:41:50.4 -- not an asteroid (will add it to exclusion list)
05:51:18.76 +43:17:46.8 -- not an asteroid (will add it to exclusion list)
06:23:09.72 +49:10:02.2 -- not an asteroid (will add it to exclusion list)
05:56:33.72 +45:29:09.2 -- not an asteroid (will add it to exclusion list)
06:03:18.88 +42:41:42.3 -- not an asteroid (will add it to exclusion list)
06:34:46.37 +45:56:36.5 -- not an asteroid (will add it to exclusion list)
05:57:11.25 +42:50:26.7 -- not an asteroid (will add it to exclusion list)
05:43:56.07 +47:43:50.3 -- not an asteroid (will add it to exclusion list)
06:21:46.38 +48:41:42.8 -- not an asteroid (will add it to exclusion list)
06:29:45.09 +43:28:18.8 -- not an asteroid (will add it to exclusion list)
06:22:14.67 +47:39:08.3 -- not an asteroid (will add it to exclusion list)
06:25:07.90 +48:56:16.1 -- not an asteroid (will add it to exclusion list)
06:31:49.42 +49:27:24.3 -- not an asteroid (will add it to exclusion list)
06:11:58.25 +44:42:24.6 -- not an asteroid (will add it to exclusion list)
06:11:00.59 +43:04:00.2 -- not an asteroid (will add it to exclusion list)
06:27:36.22 +50:07:55.7 -- not an asteroid (will add it to exclusion list)
06:25:12.22 +43:57:33.0 -- not an asteroid (will add it to exclusion list)
06:37:04.08 +47:59:59.1 -- not an asteroid (will add it to exclusion list)
06:32:48.50 +42:28:50.6 -- not an asteroid (will add it to exclusion list)
06:32:39.94 +45:40:37.4 -- not an asteroid (will add it to exclusion list)
06:17:58.01 +47:16:16.7 -- not an asteroid (will add it to exclusion list)
05:49:32.31 +46:35:57.6 -- not an asteroid (will add it to exclusion list)
05:34:10.59 +47:17:21.5 -- not an asteroid (will add it to exclusion list)
05:35:44.89 +48:35:19.3 -- not an asteroid (will add it to exclusion list)
05:33:35.60 +44:00:04.8 -- not an asteroid (will add it to exclusion list)
05:25:39.23 +47:34:08.4 -- not an asteroid (will add it to exclusion list)
05:43:00.68 +47:58:51.1 -- not an asteroid (will add it to exclusion list)
05:45:47.38 +47:37:27.1 -- not an asteroid (will add it to exclusion list)
05:38:54.92 +43:45:45.7 -- not an asteroid (will add it to exclusion list)
05:30:53.09 +43:50:50.2 -- not an asteroid (will add it to exclusion list)
05:34:25.67 +49:54:08.6 -- not an asteroid (will add it to exclusion list)
05:46:55.66 +48:32:35.5 -- not an asteroid (will add it to exclusion list)
05:48:25.46 +46:18:17.7 -- not an asteroid (will add it to exclusion list)
05:29:19.59 +43:15:50.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:25:39.23 +47:34:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:42.14 +45:54:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:15.66 +44:02:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:39.86 +44:25:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:35.16 +41:41:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:19.59 +43:15:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:22.21 +41:56:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:19.43 +43:07:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:53.09 +43:50:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:35.60 +44:00:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:54.48 +43:39:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:56.30 +44:18:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:10.59 +47:17:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:25.67 +49:54:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:44.89 +48:35:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:43.69 +41:40:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:53.94 +45:12:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:17.06 +41:38:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:22.71 +42:59:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:23.72 +42:59:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:54.01 +42:08:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:54.92 +43:45:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:18.88 +44:01:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:55.28 +46:26:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:42.61 +48:20:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:46.61 +41:59:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:41.66 +46:17:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:51.49 +45:43:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:00.68 +47:58:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:48.52 +48:57:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:56.07 +47:43:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:47.38 +47:37:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:47.33 +43:03:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:55.66 +48:32:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:25.46 +46:18:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:32.31 +46:35:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:05.07 +47:03:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.76 +43:17:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:59.21 +44:31:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.72 +45:29:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:51.64 +43:51:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.25 +42:50:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:42.18 +42:08:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:46.70 +42:58:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:17.27 +49:12:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:18.88 +42:41:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:20.88 +42:41:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:53.66 +46:17:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:00.59 +43:04:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:05.95 +41:55:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:51.61 +45:03:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:58.25 +44:42:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.05 +50:14:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:18.96 +41:52:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:29.59 +47:17:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:05.52 +46:10:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:09.73 +47:00:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:58.01 +47:16:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:58.86 +46:05:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:46.38 +48:41:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:48.15 +46:46:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:14.67 +47:39:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:26.34 +41:45:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:29.70 +44:29:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:30.62 +46:12:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:09.72 +49:10:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:04.79 +42:33:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:07.57 +45:26:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:07.90 +48:56:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:09.18 +41:48:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:12.22 +43:57:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:48.98 +48:15:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.53 +49:54:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:36.22 +50:07:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:20.82 +45:46:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:36.03 +44:18:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:45.09 +43:28:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:49.42 +49:27:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:39.94 +45:40:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:48.50 +42:28:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:53.61 +42:26:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:46.37 +45:56:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:45.28 +42:57:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:04.08 +47:59:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:26.60 +44:19:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:11.18 +49:27:38.2 -- 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)
05:25:39.23 +47:34:08.4 -- a known variable star
05:25:42.14 +45:54:21.6 -- not a known variable star
05:26:15.66 +44:02:47.0 -- not a known variable star
05:26:39.86 +44:25:14.5 -- a known variable star
05:28:35.16 +41:41:18.8 -- not a known variable star
05:29:19.59 +43:15:50.9 -- a known variable star
05:29:22.21 +41:56:48.0 -- not a known variable star
05:30:19.43 +43:07:57.7 -- not a known variable star
05:30:53.09 +43:50:50.2 -- a known variable star
05:33:35.60 +44:00:04.8 -- a known variable star
05:33:54.48 +43:39:02.7 -- not a known variable star
05:33:56.30 +44:18:19.6 -- not a known variable star
05:34:10.59 +47:17:21.5 -- a known variable star
05:34:25.67 +49:54:08.6 -- not a known variable star
05:35:44.89 +48:35:19.3 -- a known variable star
05:37:43.69 +41:40:08.7 -- a known variable star
05:37:53.94 +45:12:06.1 -- not a known variable star
05:38:17.06 +41:38:39.4 -- not a known variable star
05:38:22.71 +42:59:57.1 -- not a known variable star
05:38:23.72 +42:59:53.3 -- not a known variable star
05:38:54.01 +42:08:09.4 -- not a known variable star
05:38:54.92 +43:45:45.7 -- a known variable star
05:39:18.88 +44:01:48.1 -- not a known variable star
05:39:55.28 +46:26:23.1 -- not a known variable star
05:40:42.61 +48:20:00.6 -- not a known variable star
05:40:46.61 +41:59:38.2 -- not a known variable star
05:41:41.66 +46:17:27.7 -- a known variable star
05:42:51.49 +45:43:44.7 -- not a known variable star
05:43:00.68 +47:58:51.1 -- a known variable star
05:43:48.52 +48:57:27.7 -- not a known variable star
05:43:56.07 +47:43:50.3 -- not a known variable star
05:45:47.38 +47:37:27.1 -- a known variable star
05:46:47.33 +43:03:07.2 -- a known variable star
05:46:55.66 +48:32:35.5 -- a known variable star
05:48:25.46 +46:18:17.7 -- a known variable star
05:49:32.31 +46:35:57.6 -- a known variable star
05:50:05.07 +47:03:25.5 -- not a known variable star
05:51:18.76 +43:17:46.8 -- not a known variable star
05:55:59.21 +44:31:37.9 -- a known variable star
05:56:33.72 +45:29:09.2 -- not a known variable star
05:56:51.64 +43:51:24.0 -- not a known variable star
05:57:11.25 +42:50:26.7 -- not a known variable star
05:57:42.18 +42:08:18.6 -- not a known variable star
05:59:46.70 +42:58:02.2 -- not a known variable star
06:02:17.27 +49:12:47.0 -- not a known variable star
06:03:18.88 +42:41:42.3 -- not a known variable star
06:03:20.88 +42:41:50.4 -- not a known variable star
06:03:53.66 +46:17:34.9 -- a known variable star
06:11:00.59 +43:04:00.2 -- not a known variable star
06:11:05.95 +41:55:48.5 -- not a known variable star
06:11:51.61 +45:03:23.3 -- not a known variable star
06:11:58.25 +44:42:24.6 -- not a known variable star
06:12:10.05 +50:14:54.6 -- not a known variable star
06:13:18.96 +41:52:43.5 -- not a known variable star
06:13:29.59 +47:17:45.2 -- not a known variable star
06:14:05.52 +46:10:08.6 -- not a known variable star
06:17:09.73 +47:00:37.6 -- not a known variable star
06:17:58.01 +47:16:16.7 -- not a known variable star
06:17:58.86 +46:05:16.1 -- not a known variable star
06:21:46.38 +48:41:42.8 -- not a known variable star
06:21:48.15 +46:46:30.9 -- not a known variable star
06:22:14.67 +47:39:08.3 -- not a known variable star
06:22:26.34 +41:45:15.7 -- a known variable star
06:22:29.70 +44:29:25.8 -- not a known variable star
06:22:30.62 +46:12:18.0 -- not a known variable star
06:23:09.72 +49:10:02.2 -- not a known variable star
06:25:04.79 +42:33:12.8 -- not a known variable star
06:25:07.57 +45:26:09.4 -- not a known variable star
06:25:07.90 +48:56:16.1 -- not a known variable star
06:25:09.18 +41:48:31.5 -- not a known variable star
06:25:12.22 +43:57:33.0 -- not a known variable star
06:25:48.98 +48:15:45.0 -- not a known variable star
06:26:29.53 +49:54:10.9 -- not a known variable star
06:27:36.22 +50:07:55.7 -- not a known variable star
06:29:20.82 +45:46:47.2 -- not a known variable star
06:29:36.03 +44:18:38.4 -- not a known variable star
06:29:45.09 +43:28:18.8 -- not a known variable star
06:31:49.42 +49:27:24.3 -- not a known variable star
06:32:39.94 +45:40:37.4 -- not a known variable star
06:32:48.50 +42:28:50.6 -- not a known variable star
06:32:53.61 +42:26:18.2 -- not a known variable star
06:34:46.37 +45:56:36.5 -- not a known variable star
06:36:45.28 +42:57:52.8 -- not a known variable star
06:37:04.08 +47:59:59.1 -- not a known variable star
06:38:26.60 +44:19:50.9 -- not a known variable star
06:40:11.18 +49:27:38.2 -- not a known variable star
Found 67 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
86 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 86 (excluding asteroids and hot pixels, 67 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)2461136.66000987 -observatory V36
23:20:16.28 -06:26:10.3 Mercury (0.3mag)
02:21:20.44 +13:50:09.4 Venus (-3.9mag)
23:49:48.63 -02:13:13.9 Mars (1.2mag)
07:08:41.56 +22:52:27.9 Jupiter (-2.2mag)
00:24:44.74 +00:21:07.6 Saturn (0.9mag)
03:45:42.97 +19:41:04.4 Uranus (5.8mag)
00:09:31.50 -00:23:42.1 Neptune (7.8mag)
20:33:14.03 -22:52:29.5 Pluto (14.5mag)
15:57:31.15 -25:58:01.9 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 5 23:10 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461136.66000987:
07:08:46.27 +22:52:16.2 Io (5.7mag)
07:08:54.41 +22:52:01.3 Europa (5.8mag)
07:08:35.35 +22:52:47.2 Ganymede (5.3mag)
07:08:12.14 +22:53:18.7 Callisto (6.5mag)
07:12:24.57 +22:44:59.1 Himalia (15.3mag)
07:08:37.87 +22:52:36.4 Thebe (16.2mag)
07:12:22.21 +23:13:44.7 Elara (17.2mag)
07:06:54.25 +23:37:37.4 Pasiphae (17.3mag)
07:17:13.41 +22:49:23.8 Carme (18.4mag)
00:24:39.29 +00:21:09.1 Titan (8.8mag)
00:24:41.63 +00:21:22.1 Rhea (10.1mag)
00:24:45.39 +00:22:41.3 Iapetus (11.5mag)
00:24:46.38 +00:20:56.1 Hyperion (14.8mag)
00:26:28.99 +00:30:56.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 5 23:11 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.66000987:
14:47:12.43 -08:16:51.1 JWST
16:53:47.46 +45:17:38.2 Chandra
07:54:47.70 -35:25:17.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 5 23:10 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.66000987 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:06.38 -28:14:01.4 14.0mag P/2010 H2 (Vales)
05:00:03.94 -70:08:58.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:33.85 +31:22:33.0 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.73 +09:21:58.5 17.6mag C/2021 G2 (ATLAS)
23:07:20.48 +28:52:01.3 17.0mag C/2022 E2 (ATLAS)
04:17:57.40 +25:45:48.5 15.9mag C/2022 N2 (PANSTARRS)
09:01:51.79 +31:54:21.7 16.1mag C/2022 QE78 (ATLAS)
08:29:59.08 -01:14:10.7 17.3mag C/2022 R6 (PANSTARRS)
18:55:35.60 +17:41:31.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:31.14 -11:39:39.2 17.6mag P/2023 B1 (PANSTARRS)
09:12:51.38 -13:30:30.9 17.5mag C/2023 F3 (ATLAS)
21:43:26.20 +62:22:10.8 17.5mag C/2023 H5 (Lemmon)
19:26:25.79 -03:36:29.7 14.3mag C/2023 R1 (PANSTARRS)
21:42:39.02 +84:36:24.9 17.8mag C/2023 X2 (Lemmon)
06:14:31.39 +63:35:03.0 17.0mag C/2024 A1 (ATLAS)
04:50:59.34 +14:32:30.0 10.4mag C/2024 E1 (Wierzchos)
16:25:07.20 +04:46:21.3 17.4mag C/2024 G6 (ATLAS)
20:17:32.17 +12:40:31.7 14.7mag C/2024 J3 (ATLAS)
03:17:44.36 -23:55:41.1 16.4mag C/2024 T5 (ATLAS)
05:08:40.80 +47:50:36.5 17.7mag C/2025 J1 (Borisov)
14:19:13.75 +37:21:33.2 14.8mag C/2025 L1 (ATLAS)
03:10:19.31 -24:44:40.5 17.8mag C/2025 Q3 (ATLAS)
22:53:29.67 +19:50:13.9 10.1mag C/2025 R3 (PANSTARRS)
12:58:24.36 +02:23:24.4 17.5mag C/2025 Y1 (ATLAS)
01:30:24.91 +04:43:46.0 7.1mag C/2026 A1 (MAPS)
23:30:42.61 +35:14:12.9 14.3mag C/2026 B2 (Sun-Gao)
18:23:43.70 -10:13:11.2 12.4mag 10P/Tempel
15:12:56.51 +04:06:52.2 13.1mag 24P/Schaumasse
11:05:46.94 -01:51:53.8 15.7mag 29P/Schwassmann-Wachmann
17:56:44.59 -09:59:39.2 17.7mag 40P/Vaisala
10:38:53.58 -04:57:04.0 16.7mag 43P/Wolf-Harrington
01:33:30.22 +15:47:26.2 17.1mag 47P/Ashbrook-Jackson
06:53:16.75 +39:05:15.1 17.0mag 63P/Wild
23:16:15.97 -12:39:32.4 15.7mag 65P/Gunn
03:37:35.82 +17:43:34.2 15.8mag 76P/West-Kohoutek-Ikemura
00:44:00.63 +06:16:44.0 14.4mag 78P/Gehrels
22:32:26.78 -12:16:50.1 14.5mag 88P/Howell
01:43:05.11 +17:56:18.9 15.1mag 93P/Lovas
04:36:52.25 +31:43:35.5 16.3mag 123P/West-Hartley
08:17:54.30 +42:54:20.2 16.2mag 124P/Mrkos
02:18:10.18 +13:15:12.2 16.4mag 128P/Shoemaker-Holt
02:28:20.22 +13:14:58.7 17.5mag 131P/Mueller
00:35:43.48 +09:35:51.7 11.3mag 141P/Machholz
00:45:42.06 +01:11:18.0 11.3mag 141P-A/Machholz
23:36:17.33 -02:25:57.5 14.0mag 141P-D/Machholz
01:14:49.02 +02:51:09.0 17.9mag 141P-I/Machholz
00:35:02.95 -06:26:00.0 15.2mag 162P/SidingSpring
10:30:59.31 +31:30:29.5 17.8mag 164P/Christensen
06:18:22.38 +24:31:26.2 17.8mag 198P/ODAS
15:08:45.37 -01:11:58.6 17.4mag 210P/Christensen
21:08:48.68 -13:49:44.2 17.4mag 218P/LINEAR
17:12:35.11 -15:04:35.2 16.2mag 235P/LINEAR
05:13:35.66 +33:51:11.2 16.6mag 240P/NEAT
07:34:11.37 -06:17:26.9 17.6mag 242P/Spahr
15:45:56.84 +06:18:24.9 17.5mag 391P/Kowalski
07:30:54.58 +21:18:41.1 17.6mag 450P/LONEOS
05:21:52.41 +45:36:48.0 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 5 23:10 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 5 23:10 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 5 23:10 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 5 23:11 tns_transients_list.txt
