This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i
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
Gaia DR3 1817869342108232192,2461132.8792,10.54,0.05,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
Gaia DR3 1817869342108232192 20260402.3792 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EH Vul,2461132.8792,10.73,0.05,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
EH Vul 20260402.3792 10.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.4640+23.9338,2461132.8792,13.21,0.05,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 J303.4640+23.9338 20260402.3792 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!
TCP 2026 04 02.3792* 20 26 20.46 +19 40 02.3 12.8 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1816646268560147968,2461132.8792,12.77,0.05,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 1816646268560147968 20260402.3792 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J311.1301+26.0758,2461132.8792,12.18,0.05,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 J311.1301+26.0758 20260402.3792 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J310.7152+22.6439,2461132.8792,12.35,0.05,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 J310.7152+22.6439 20260402.3792 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1818191808250396160,2461132.8792,12.08,0.05,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
Gaia DR3 1818191808250396160 20260402.3792 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
BL Sge,2461132.8792,11.82,0.05,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
BL Sge 20260402.3792 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 8407719,2461132.8792,12.78,0.05,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
NSVS 8407719 20260402.3792 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!
TCP 2026 04 02.3792* 20 33 53.97 +20 27 25.1 11.7 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2033540+202724,2461132.8792,11.69,0.05,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 J2033540+202724 20260402.3792 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J203530+2123.6,2461132.8792,10.54,0.05,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
ASAS J203530+2123.6 20260402.3792 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2021244+205435,2461132.8792,11.93,0.05,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 J2021244+205435 20260402.3792 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DL Vul,2461132.8792,10.81,0.05,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
DL Vul 20260402.3792 10.81CV 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
ASASSN-V J201620.98+185529.6,2461132.8792,12.48,0.05,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
ASASSN-V J201620.98+185529.6 20260402.3792 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3792* 20 29 26.82 +19 53 20.3 12.5 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J2029269+195319,2461132.8792,12.47,0.05,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 J2029269+195319 20260402.3792 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J308.3772+26.1324,2461132.8792,12.26,0.05,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
ATO J308.3772+26.1324 20260402.3792 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
ASASSN-V J195242.20+204120.3,2461132.8792,12.24,0.05,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
ASASSN-V J195242.20+204120.3 20260402.3792 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
Gaia DR3 1843155253388924672,2461132.8792,11.45,0.05,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
Gaia DR3 1843155253388924672 20260402.3792 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200314.71+205858.3,2461132.8792,13.10,0.05,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 J200314.71+205858.3 20260402.3792 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2029175+261731,2461132.8792,12.57,0.05,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
NSVS J2029175+261731 20260402.3792 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0375 Vul,2461132.8792,11.76,0.05,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
V0375 Vul 20260402.3792 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195754.01+193334.9,2461132.8792,12.50,0.05,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 J195754.01+193334.9 20260402.3792 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3792* 20 24 48.84 +19 22 50.2 12.3 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1816259554007911680,2461132.8792,12.29,0.05,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 1816259554007911680 20260402.3792 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J203429+2106.0,2461132.8792,11.03,0.05,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
ASAS J203429+2106.0 20260402.3792 11.03CV 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
ASAS J201913+1915.4,2461132.8792,10.51,0.05,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
ASAS J201913+1915.4 20260402.3792 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J202441+2239.0,2461132.8792,11.93,0.05,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
ASAS J202441+2239.0 20260402.3792 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J203112.67+261227.1,2461132.8792,11.80,0.05,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 J203112.67+261227.1 20260402.3792 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461132.87951676 02.04.2026 09:06:20.248 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
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: 4 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): 20296
Objects passed selection criteria: 20214
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 15287.5
Average stars matched: 14933.2 (97.6827 %)
Memory usage VmPeak: 125572 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:24:46 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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461132.87951676 02.04.2026 09:06:20.248 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 147
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 40 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): 193470
Objects passed selection criteria: 192944
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 142019
Average stars matched: 136980 (96.4521 %)
Memory usage VmPeak: 2022420 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:31:00 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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: 2461132.87889596
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits'
wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:27.958 +21:59:58.57
Angular distance between the image centers 0.01 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 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:25.013 +22:00:35.16
Angular distance between the image centers 0.02 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 20:18:27.958 +21:59:58.57
Second-epoch second image center 20:18:25.013 +22:00:35.16
Angular distance between the image centers 0.01526 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.oi5tt95h3a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.uqqh07sEyS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.YoEc80AGEJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits &> /tmp/tmp.odZvYM1uov
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 24638 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.6627 to 313.2570 deg, Dec +16.3767 to +27.3369 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 295.6627 to 313.2570 deg, Dec 16.3767 to 27.3369 deg
Loaded 24193 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): 13464 out of 14549 total matches.
Matched with Tycho-2 14549 out of 24638 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758582
a=0.000000 b=1.000000 c=22.758582
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
2.9 pix fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
2.9 pix fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Limiting magnitude estimates:
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
13.6 mag. fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
13.7 mag. fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oi5tt95h3a (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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2463, passed=24638
Got 24638 stars (including 22152 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 24638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 531 to 588 (Dec 16.4 to 27.3)
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...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 935 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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.uqqh07sEyS (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/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2477, passed=24779
Got 24779 stars (including 22281 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 24779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 531 to 588 (Dec 16.4 to 27.3)
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...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.YoEc80AGEJ (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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=680, passed=9721
Got 9721 stars (including 9031 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 9721 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 532 to 588 (Dec 16.4 to 27.3)
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...
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.86"
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.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.odZvYM1uov (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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=677, passed=9770
Got 9770 stars (including 9085 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 9770 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 532 to 588 (Dec 16.4 to 27.3)
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...
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.87"
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits'
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out11771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22014.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31404_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 31404_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:52:33.34 +19:06:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31410_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 31410_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:26:15.21 +20:27:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12160_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 12160_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:06:35.65 +21:35:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11771_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 11771_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17681_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 17681_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:56:28.93 +23:54:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22014_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 22014_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 17s
Prepared the HTML report for the field Vul-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 ####
20:41:56.30 +21:36:21.2
20:28:01.78 +26:03:32.0
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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:27.958 +21:59:58.57
Angular distance between the image centers 0.01 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 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:25.013 +22:00:35.16
Angular distance between the image centers 0.02 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 20:18:27.958 +21:59:58.57
Second-epoch second image center 20:18:25.013 +22:00:35.16
Angular distance between the image centers 0.01526 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.klQF78AhXQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.0DmqJgzKIM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.lil56KOQyP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits &> /tmp/tmp.9H3a0Z3TFs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 232861 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 295.6471 to 313.2612 deg, Dec +16.3395 to +27.3423 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 295.6471 to 313.2612 deg, Dec 16.3395 to 27.3423 deg
Loaded 24297 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): 12337 out of 17496 total matches.
Matched with Tycho-2 17496 out of 232861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547121
a=0.000000 b=1.000000 c=22.547121
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 89 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
1.9 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
2.7 pix fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
2.7 pix fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Limiting magnitude estimates:
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
13.6 mag. fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
13.6 mag. fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.0 (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.klQF78AhXQ (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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=33174, passed=232827
Got 232827 stars (including 199306 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 232827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.0DmqJgzKIM (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/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=32901, passed=232172
Got 232172 stars (including 198927 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 232172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.lil56KOQyP (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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=5821, passed=74558
Got 74558 stars (including 68681 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 74558 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 532 to 588 (Dec 16.4 to 27.3)
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...
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
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_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.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.9H3a0Z3TFs (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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=5783, passed=74868
Got 74868 stars (including 69028 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 74868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (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 0.010430 (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 532 to 588 (Dec 16.4 to 27.3)
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...
Estimated accuracy of the plate solution: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.87"
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_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits -region wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-05-26_20.00sec_-15.00C_LIGHT_0035.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.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_2026-04-02_CI_Vul-02-Q2b1x1_041900_TTUQ2b1x1_31389_S3YRdV6i/wcs_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036.fits
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out107136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out262861.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out101804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out217792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out220829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99221.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
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: 12s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262694_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262694_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:12:06.63 +22:38:00.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262697_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 262697_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262698_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262698_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:34:57.67 +26:05:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 5.213 1855872758940679552 308.74154621717 +26.08832638361 12.9162 12.0403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262699_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262699_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:09:17.16 +24:05:08.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262703_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 262703_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262713_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262713_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:25:36.61 +23:47:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262723_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262723_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:12:38.59 +25:28:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262725_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262725_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:39:19.88 +22:09:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.570 1818146277300187776 309.83354873736 +22.16494409780 12.4616 11.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262734_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262734_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:41:44.50 +21:27:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262746_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 262746_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262748_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 262748_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262750_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262750_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:57:34.83 +21:45:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262752_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262752_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:44:40.37 +25:08:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 3.137 1843559323909756544 311.16835329013 +25.13522184043 11.7234 11.4489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262753_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262753_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:36:24.38 +21:40:13.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262756_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262756_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:58:50.79 +19:37:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262757_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262757_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:25:23.78 +17:58:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 3.049 1815081697874429952 306.34973575223 +17.97413204592 12.4392 11.9630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262758_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262758_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:59:44.73 +20:34:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262759_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 262759_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262761_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262761_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:11:30.41 +21:49:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262762_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262762_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:41:46.27 +22:24:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262768_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262768_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:51:31.10 +18:52:28.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262775_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262775_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:41:22.02 +25:14:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 4.035 1843610623003967360 310.34298395745 +25.23831562217 11.3807 10.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262777_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262777_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262795_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262795_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:00:57.60 +20:01:20.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262800_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262800_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:38:30.14 +21:10:11.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262805_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262805_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:50:13.41 +17:43:50.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262809_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262809_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:57:54.63 +20:31:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262810_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262810_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:52:39.53 +22:27:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 3.749 1827925956529136128 298.16583202005 +22.45608892717 12.6682 12.1413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262818_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262818_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:03:52.03 +21:04:40.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262820_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262820_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:50:40.32 +20:12:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262823_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262823_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:11:13.04 +21:52:38.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262824_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262824_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:53:38.76 +17:51:54.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262827_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262827_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:50:59.35 +24:37:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.349 2020623886179976832 297.74768029101 +24.63216604235 12.5279 11.4806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262831_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262831_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:59:10.78 +23:04:37.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262832_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262832_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:16:14.23 +21:34:58.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262837_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262837_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:14:09.20 +22:13:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262842_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262842_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:53:18.31 +20:20:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262843_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262843_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:14:00.14 +18:37:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262846_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262846_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:27:08.22 +20:27:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262850_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262850_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:48:56.56 +24:42:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262856_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262856_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:08:38.38 +22:10:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262857_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262857_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:04:21.18 +22:35:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262861_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262861_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:58:10.28 +22:50:26.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262865_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262865_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:10:31.90 +20:57:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262869_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262869_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:27:00.26 +22:20:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262877_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 262877_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:30:11.38 +20:23:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176744_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 176744_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:56:29.01 +23:54:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26281_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 26281_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170272_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 170272_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90998_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 90998_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:32:06.70 +20:39:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86212_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 86212_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111392_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 111392_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108249_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 108249_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:49:13.12 +20:52:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99221_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 99221_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151163_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 151163_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61062_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 61062_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:32:24.80 +19:29:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194740_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 194740_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:25:58.46 +24:48:40.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49430_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 49430_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57832_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 57832_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:24:58.20 +19:20:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71589_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 71589_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53589_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 53589_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:20:03.65 +19:07:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 220829_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 220829_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 221934_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 221934_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:28:01.75 +26:03:31.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37789_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 37789_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:19:18.77 +18:25:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166677_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 166677_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:42:21.76 +23:43:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101804_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 101804_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148186_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 148186_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:50:01.36 +22:29:28.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173395_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 173395_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121456_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 121456_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:08:48.77 +21:40:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105089_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 105089_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 217792_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 217792_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120622_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 120622_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:06:35.62 +21:35:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107136_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 107136_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:43:04.38 +21:16:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.380 1817798762908036736 310.76824785873 +21.27292220741 12.0644 11.6708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178649_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 178649_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112934_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 112934_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:30:44.21 +21:26:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69805_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 69805_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245355_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 245355_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245127_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 245127_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:01:44.62 +21:28:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.388 1823912601637791488 300.43577282337 +21.46863929313 11.0459 9.6570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103236_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 103236_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58059_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 58059_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87318_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 87318_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:26:15.16 +20:27:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 149736_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 149736_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:11:00.07 +22:51:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35196_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 35196_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:52:11.97 +18:03:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60371_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 60371_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 19:52:33.30 +19:06:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142738_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 142738_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219541_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
Preparing report for the candidate 219541_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34531_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 34531_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:07:12.62 +18:12:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168819_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 168819_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:43:23.90 +23:47:29.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96374_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036
The candidate 96374_fd_Vul-02-Q2b1x1_2026-04-02_04-06-20_20.00sec_-14.90C_LIGHT_0036 did not pass the final checks
**** FOUND 20:30:41.91 +20:52:05.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 37s
Prepared the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:41:56.30 +21:36:21.2
20:28:01.78 +26:03:32.0
19:52:42.22 +20:41:25.6
20:34:28.84 +21:05:58.0
20:03:14.64 +20:58:57.8
20:35:29.93 +21:23:35.7
20:24:40.60 +22:39:04.0
20:07:17.54 +22:48:40.8
20:01:09.14 +23:39:09.1
20:44:07.06 +24:01:34.6
20:27:28.08 +24:17:18.5
20:29:17.15 +26:17:25.6
20:31:12.40 +26:12:23.7
20:33:28.11 +26:07:34.3
20:24:48.84 +19:22:50.2
20:13:50.77 +23:56:03.4
20:26:20.46 +19:40:02.3
20:44:33.51 +26:04:43.9
20:42:51.62 +22:38:11.8
20:43:22.89 +22:13:00.7
20:04:21.87 +17:48:39.0
20:16:20.92 +18:55:30.1
20:19:13.12 +19:15:23.2
19:57:54.05 +19:33:34.7
20:29:26.82 +19:53:20.3
20:33:53.97 +20:27:25.1
20:21:24.93 +20:54:35.7
########### Completed Vul-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 ####
20:41:56.30 +21:36:21.2
20:28:01.78 +26:03:32.0
20:13:50.77 +23:56:03.4
20:26:20.46 +19:40:02.3
20:44:33.51 +26:04:43.9
20:42:51.62 +22:38:11.8
20:43:22.89 +22:13:00.7
20:04:21.87 +17:48:39.0
20:01:09.14 +23:39:09.1
20:33:53.97 +20:27:25.1
20:35:29.93 +21:23:35.7
20:21:24.93 +20:54:35.7
20:07:17.54 +22:48:40.8
20:16:20.92 +18:55:30.1
20:29:26.82 +19:53:20.3
20:33:28.11 +26:07:34.3
19:52:42.22 +20:41:25.6
20:44:07.06 +24:01:34.6
20:03:14.64 +20:58:57.8
20:29:17.15 +26:17:25.6
20:27:28.08 +24:17:18.5
19:57:54.05 +19:33:34.7
20:24:48.84 +19:22:50.2
20:34:28.84 +21:05:58.0
20:19:13.12 +19:15:23.2
20:24:40.60 +22:39:04.0
20:31:12.40 +26:12:23.7
###################################################################################
20:41:56.30 +21:36:21.2 -- not an asteroid (will add it to exclusion list)
20:28:01.78 +26:03:32.0 -- not an asteroid (will add it to exclusion list)
20:13:50.77 +23:56:03.4 -- not an asteroid (will add it to exclusion list)
20:26:20.46 +19:40:02.3 -- not an asteroid (will add it to exclusion list)
20:44:33.51 +26:04:43.9 -- not an asteroid (will add it to exclusion list)
20:42:51.62 +22:38:11.8 -- not an asteroid (will add it to exclusion list)
20:43:22.89 +22:13:00.7 -- not an asteroid (will add it to exclusion list)
20:04:21.87 +17:48:39.0 -- not an asteroid (will add it to exclusion list)
20:01:09.14 +23:39:09.1 -- not an asteroid (will add it to exclusion list)
20:33:53.97 +20:27:25.1 -- not an asteroid (will add it to exclusion list)
20:35:29.93 +21:23:35.7 -- not an asteroid (will add it to exclusion list)
20:21:24.93 +20:54:35.7 -- not an asteroid (will add it to exclusion list)
20:07:17.54 +22:48:40.8 -- not an asteroid (will add it to exclusion list)
20:16:20.92 +18:55:30.1 -- not an asteroid (will add it to exclusion list)
20:29:26.82 +19:53:20.3 -- not an asteroid (will add it to exclusion list)
20:33:28.11 +26:07:34.3 -- not an asteroid (will add it to exclusion list)
19:52:42.22 +20:41:25.6 -- not an asteroid (will add it to exclusion list)
20:44:07.06 +24:01:34.6 -- not an asteroid (will add it to exclusion list)
20:03:14.64 +20:58:57.8 -- not an asteroid (will add it to exclusion list)
20:29:17.15 +26:17:25.6 -- not an asteroid (will add it to exclusion list)
20:27:28.08 +24:17:18.5 -- not an asteroid (will add it to exclusion list)
19:57:54.05 +19:33:34.7 -- not an asteroid (will add it to exclusion list)
20:24:48.84 +19:22:50.2 -- not an asteroid (will add it to exclusion list)
20:34:28.84 +21:05:58.0 -- not an asteroid (will add it to exclusion list)
20:19:13.12 +19:15:23.2 -- not an asteroid (will add it to exclusion list)
20:24:40.60 +22:39:04.0 -- not an asteroid (will add it to exclusion list)
20:31:12.40 +26:12:23.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:52:42.22 +20:41:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:54.05 +19:33:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:09.14 +23:39:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:14.64 +20:58:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:21.87 +17:48:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:17.54 +22:48:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:50.77 +23:56:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:20.92 +18:55:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:13.12 +19:15:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:24.93 +20:54:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:40.60 +22:39:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:24:48.84 +19:22:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:26:20.46 +19:40:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:28.08 +24:17:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:28:01.78 +26:03:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:17.15 +26:17:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:29:26.82 +19:53:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:31:12.40 +26:12:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:28.11 +26:07:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:53.97 +20:27:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:34:28.84 +21:05:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:35:29.93 +21:23:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:56.30 +21:36:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:42:51.62 +22:38:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:22.89 +22:13:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:07.06 +24:01:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:44:33.51 +26:04:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:52:42.22 +20:41:25.6 -- a known variable star
19:57:54.05 +19:33:34.7 -- a known variable star
20:01:09.14 +23:39:09.1 -- a known variable star
20:03:14.64 +20:58:57.8 -- a known variable star
20:04:21.87 +17:48:39.0 -- a known variable star
20:07:17.54 +22:48:40.8 -- a known variable star
20:13:50.77 +23:56:03.4 -- not a known variable star
20:16:20.92 +18:55:30.1 -- a known variable star
20:19:13.12 +19:15:23.2 -- a known variable star
20:21:24.93 +20:54:35.7 -- a known variable star
20:24:40.60 +22:39:04.0 -- a known variable star
20:24:48.84 +19:22:50.2 -- a known variable star
20:26:20.46 +19:40:02.3 -- a known variable star
20:27:28.08 +24:17:18.5 -- a known variable star
20:28:01.78 +26:03:32.0 -- a known variable star
20:29:17.15 +26:17:25.6 -- a known variable star
20:29:26.82 +19:53:20.3 -- a known variable star
20:31:12.40 +26:12:23.7 -- a known variable star
20:33:28.11 +26:07:34.3 -- not a known variable star
20:33:53.97 +20:27:25.1 -- a known variable star
20:34:28.84 +21:05:58.0 -- a known variable star
20:35:29.93 +21:23:35.7 -- a known variable star
20:41:56.30 +21:36:21.2 -- not a known variable star
20:42:51.62 +22:38:11.8 -- not a known variable star
20:43:22.89 +22:13:00.7 -- not a known variable star
20:44:07.06 +24:01:34.6 -- not a known variable star
20:44:33.51 +26:04:43.9 -- not a known variable star
Found 7 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
27 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
19:52:42.22 +20:41:25.6
19:57:54.05 +19:33:34.7
20:01:09.14 +23:39:09.1
20:03:14.64 +20:58:57.8
20:04:21.87 +17:48:39.0
20:07:17.54 +22:48:40.8
20:13:50.77 +23:56:03.4
20:16:20.92 +18:55:30.1
20:19:13.12 +19:15:23.2
20:21:24.93 +20:54:35.7
20:24:40.60 +22:39:04.0
20:24:48.84 +19:22:50.2
20:26:20.46 +19:40:02.3
20:27:28.08 +24:17:18.5
20:28:01.78 +26:03:32.0
20:29:17.15 +26:17:25.6
20:29:26.82 +19:53:20.3
20:31:12.40 +26:12:23.7
20:33:28.11 +26:07:34.3
20:33:53.97 +20:27:25.1
20:34:28.84 +21:05:58.0
20:35:29.93 +21:23:35.7
20:41:56.30 +21:36:21.2
20:42:51.62 +22:38:11.8
20:43:22.89 +22:13:00.7
20:44:07.06 +24:01:34.6
20:44:33.51 +26:04:43.9
20:43:04.38 +21:16:25.9
19:50:01.36 +22:29:28.4
20:01:44.62 +21:28:05.8
20:12:06.63 +22:38:00.7
20:34:57.67 +26:05:14.7
20:09:17.16 +24:05:08.1
20:39:19.88 +22:09:49.9
20:41:44.50 +21:27:37.6
20:44:40.37 +25:08:09.9
20:36:24.38 +21:40:13.4
20:25:23.78 +17:58:24.8
20:41:46.27 +22:24:42.7
19:51:31.10 +18:52:28.5
20:41:22.02 +25:14:18.3
19:52:39.53 +22:27:22.2
19:50:59.35 +24:37:52.7
19:58:10.28 +22:50:26.9
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461132.87889596 -observatory V36
23:05:25.21 -07:28:45.6 Mercury (0.4mag)
02:03:34.65 +12:08:09.0 Venus (-3.9mag)
23:38:59.07 -03:24:20.5 Mars (1.2mag)
07:07:28.63 +22:54:16.1 Jupiter (-2.2mag)
00:23:01.30 +00:10:11.2 Saturn (0.9mag)
03:45:00.53 +19:38:45.3 Uranus (5.8mag)
00:09:00.45 -00:27:00.1 Neptune (7.8mag)
20:32:59.23 -22:52:38.1 Pluto (14.5mag)
12:50:59.21 -09:38:35.3 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 04:24 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461132.87889596:
07:07:36.66 +22:54:00.1 Io (5.7mag)
07:07:41.06 +22:53:51.9 Europa (5.8mag)
07:07:38.22 +22:53:50.3 Ganymede (5.3mag)
07:07:45.05 +22:53:35.2 Callisto (6.5mag)
07:11:18.37 +22:48:49.4 Himalia (15.3mag)
07:07:32.84 +22:54:07.9 Thebe (16.1mag)
07:11:10.41 +23:16:37.9 Elara (17.2mag)
07:05:25.97 +23:41:24.6 Pasiphae (17.3mag)
07:16:04.62 +22:50:42.1 Carme (18.4mag)
00:22:53.94 +00:10:36.2 Titan (8.8mag)
00:22:59.07 +00:10:18.7 Rhea (10.1mag)
00:23:10.57 +00:12:06.7 Iapetus (11.5mag)
00:22:51.70 +00:10:19.5 Hyperion (14.8mag)
00:24:48.12 +00:20:22.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 04:24 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.87889596:
14:22:21.47 -04:37:31.8 JWST
19:46:50.70 +06:04:11.5 Chandra
08:34:57.03 -47:33:22.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 04:24 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.87889596 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:45.35 -28:02:28.6 14.0mag P/2010 H2 (Vales)
04:57:44.40 -70:20:53.3 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.28 +31:21:18.3 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.76 +08:54:23.7 17.6mag C/2021 G2 (ATLAS)
23:06:05.73 +28:44:46.1 17.0mag C/2022 E2 (ATLAS)
04:13:44.52 +25:39:14.9 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.83 +31:49:51.5 16.1mag C/2022 QE78 (ATLAS)
08:29:48.57 -01:40:28.4 17.2mag C/2022 R6 (PANSTARRS)
18:56:02.48 +17:21:49.9 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:23.94 -11:42:37.2 17.6mag P/2023 B1 (PANSTARRS)
09:15:14.59 -14:09:25.1 17.5mag C/2023 F3 (ATLAS)
21:38:47.82 +62:11:16.9 17.4mag C/2023 H5 (Lemmon)
19:28:32.18 -03:34:41.4 14.3mag C/2023 R1 (PANSTARRS)
21:42:54.92 +84:08:55.8 17.8mag C/2023 X2 (Lemmon)
06:13:57.72 +63:37:27.9 17.0mag C/2024 A1 (ATLAS)
04:41:37.86 +12:46:04.8 10.1mag C/2024 E1 (Wierzchos)
16:27:04.45 +04:09:09.7 17.4mag C/2024 G6 (ATLAS)
20:16:00.16 +11:43:12.9 14.8mag C/2024 J3 (ATLAS)
03:14:33.23 -24:32:43.5 16.4mag C/2024 T5 (ATLAS)
05:05:48.45 +48:53:25.4 17.6mag C/2025 J1 (Borisov)
14:33:46.15 +33:17:24.8 14.7mag C/2025 L1 (ATLAS)
03:04:55.18 -24:12:54.6 17.7mag C/2025 Q3 (ATLAS)
22:45:37.74 +19:45:17.8 10.7mag C/2025 R3 (PANSTARRS)
13:00:02.05 +02:08:25.3 17.5mag C/2025 Y1 (ATLAS)
01:20:41.17 +02:40:56.0 8.4mag C/2026 A1 (MAPS)
23:19:04.50 +34:22:07.1 14.1mag C/2026 B2 (Sun-Gao)
18:16:19.63 -10:23:30.1 12.6mag 10P/Tempel
15:17:08.60 +04:23:53.9 12.8mag 24P/Schaumasse
11:07:06.54 -02:00:19.0 15.7mag 29P/Schwassmann-Wachmann
17:54:20.91 -10:08:58.7 17.6mag 40P/Vaisala
10:39:55.20 -05:18:46.8 16.6mag 43P/Wolf-Harrington
01:27:43.15 +15:07:39.4 17.1mag 47P/Ashbrook-Jackson
06:46:59.96 +39:51:48.0 17.1mag 63P/Wild
23:11:13.15 -13:08:13.0 15.7mag 65P/Gunn
03:28:06.90 +16:17:23.5 15.8mag 76P/West-Kohoutek-Ikemura
00:35:50.54 +05:31:23.9 14.5mag 78P/Gehrels
22:20:16.38 -13:22:03.1 14.5mag 88P/Howell
01:32:54.44 +16:51:34.1 15.1mag 93P/Lovas
04:30:21.44 +31:29:32.1 16.3mag 123P/West-Hartley
08:14:37.74 +44:38:50.1 16.2mag 124P/Mrkos
02:12:29.57 +12:48:52.4 16.4mag 128P/Shoemaker-Holt
02:21:01.84 +12:44:53.6 17.4mag 131P/Mueller
00:17:11.03 +08:05:54.5 11.6mag 141P/Machholz
00:27:21.52 -00:11:46.7 11.6mag 141P-A/Machholz
23:20:13.79 -03:35:09.4 14.5mag 141P-D/Machholz
00:55:48.38 +01:23:43.3 18.0mag 141P-I/Machholz
00:24:36.17 -08:17:04.5 15.3mag 162P/SidingSpring
10:32:24.06 +31:42:29.3 17.7mag 164P/Christensen
06:11:30.59 +24:36:03.4 17.8mag 198P/ODAS
15:15:06.56 -01:41:17.0 17.2mag 210P/Christensen
20:56:21.39 -14:44:07.3 17.3mag 218P/LINEAR
17:10:11.87 -15:29:13.5 16.2mag 235P/LINEAR
05:05:48.55 +33:28:10.8 16.5mag 240P/NEAT
07:32:51.56 -06:45:15.3 17.6mag 242P/Spahr
15:46:53.16 +06:01:45.4 17.6mag 391P/Kowalski
07:29:56.52 +21:16:34.3 17.6mag 450P/LONEOS
05:16:43.65 +45:50:25.3 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 04:24 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
-rw-r--r-- 1 apache apache 5.8K Apr 2 04:24 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
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
-rw-r--r-- 1 apache apache 187K Apr 2 04:24 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:03:36.117 -67:58:13.34 SN 2026hkg 2026-03-27.12 18.505
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
-rw-r--r-- 1 apache apache 29K Apr 2 04:24 tns_transients_list.txt
