This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY
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
VARIABLE_NAME,2461138.8049,11.35,0.05,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
VARIABLE_NAME 20260408.3049 11.35CV 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
VARIABLE_NAME,2461138.8049,12.52,0.05,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
VARIABLE_NAME 20260408.3049 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8049,12.56,0.05,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
VARIABLE_NAME 20260408.3049 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.8049,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.3049 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165135.28-163833.3,2461138.8049,13.09,0.05,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 J165135.28-163833.3 20260408.3049 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2513 Oph,2461138.8049,12.85,0.05,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
V2513 Oph 20260408.3049 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J170332-2158.9,2461138.8049,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J170332-2158.9 20260408.3049 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 16461686,2461138.8049,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16461686 20260408.3049 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J163855.23-204923.9,2461138.8049,12.81,0.05,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
ASASSN-V J163855.23-204923.9 20260408.3049 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J170534-1733.9,2461138.8049,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J170534-1733.9 20260408.3049 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1651394-181306,2461138.8049,11.77,0.05,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
NSVS J1651394-181306 20260408.3049 11.77CV 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
ASAS J164116-1957.9,2461138.8049,9.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J164116-1957.9 20260408.3049 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J170006-2009.7,2461138.8049,9.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J170006-2009.7 20260408.3049 9.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164745.00-212418.8,2461138.8049,12.30,0.05,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 J164745.00-212418.8 20260408.3049 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 16446482,2461138.8049,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16446482 20260408.3049 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 8232,2461138.8049,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 8232 20260408.3049 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J165529-2136.0,2461138.8049,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J165529-2136.0 20260408.3049 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J165518-2201.1,2461138.8049,10.70,0.05,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 J165518-2201.1 20260408.3049 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127754048686632320,2461138.8049,12.30,0.05,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 4127754048686632320 20260408.3049 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J165932-2139.4,2461138.8049,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J165932-2139.4 20260408.3049 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
S Oph,2461138.8049,11.99,0.05,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
S Oph 20260408.3049 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164408.50-173803.5,2461138.8049,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J164408.50-173803.5 20260408.3049 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170907.71-213915.5,2461138.8049,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J170907.71-213915.5 20260408.3049 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170933.92-165617.4,2461138.8049,11.98,0.05,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 J170933.92-165617.4 20260408.3049 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J165610-2027.5,2461138.8049,11.85,0.05,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 J165610-2027.5 20260408.3049 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J163916-2151.9,2461138.8049,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J163916-2151.9 20260408.3049 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170451.90-163427.0,2461138.8049,12.98,0.05,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 J170451.90-163427.0 20260408.3049 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1354 Oph,2461138.8049,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1354 Oph 20260408.3049 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170532.53-192439.9,2461138.8049,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J170532.53-192439.9 20260408.3049 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1653229-190331,2461138.8049,12.64,0.05,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 J1653229-190331 20260408.3049 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J171032.22-180517.6,2461138.8049,12.52,0.05,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 J171032.22-180517.6 20260408.3049 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170526.85-174611.7,2461138.8049,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J170526.85-174611.7 20260408.3049 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164037.12-184816.5,2461138.8049,12.93,0.05,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
ASASSN-V J164037.12-184816.5 20260408.3049 12.93CV 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
ASAS J165608-1530.9,2461138.8049,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J165608-1530.9 20260408.3049 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1180 Oph,2461138.8049,11.66,0.05,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
V1180 Oph 20260408.3049 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1281 Oph,2461138.8049,10.37,0.05,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
V1281 Oph 20260408.3049 10.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1300 Oph,2461138.8049,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1300 Oph 20260408.3049 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165357.34-211828.1,2461138.8049,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J165357.34-211828.1 20260408.3049 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 16461335,2461138.8049,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16461335 20260408.3049 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170947.35-152559.3,2461138.8049,12.29,0.05,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
ASASSN-V J170947.35-152559.3 20260408.3049 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
V2068 Oph,2461138.8049,10.45,0.05,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
V2068 Oph 20260408.3049 10.45CV 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 J170813.88-220009.2,2461138.8049,12.73,0.05,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
ASASSN-V J170813.88-220009.2 20260408.3049 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
First image: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Last image: 2461138.80517613 08.04.2026 07:19:17.218 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.41
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: 2 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): 3964
Objects passed selection criteria: 3956
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 3561.25
Average stars matched: 3487.5 (97.9291 %)
Memory usage VmPeak: 110864 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 02:21:41 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: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
First image: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Last image: 2461138.80517613 08.04.2026 07:19:17.218 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 219
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.99
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: 15 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): 47146
Objects passed selection criteria: 47068
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 39666
Average stars matched: 38128.2 (96.1233 %)
Memory usage VmPeak: 155504 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 02:22:34 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat to cache
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461138.80457866
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits exists and is non-empty
Saving wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits to local_wcs_cache/
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> 'local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits exists and is non-empty
Saving wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits to local_wcs_cache/
'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> 'local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits exists and is non-empty
Saving wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits to local_wcs_cache/
'wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits' -> 'local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits'
wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits exists and is non-empty
Saving wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits to local_wcs_cache/
'wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits' -> 'local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:38.432 -18:00:30.56
Angular distance between the image centers 0.0742 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 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:37.876 -17:59:53.71
Angular distance between the image centers 0.0722 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 16:53:38.432 -18:00:30.56
Second-epoch second image center 16:53:37.876 -17:59:53.71
Angular distance between the image centers 0.01047 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits &> /tmp/tmp.kdwuGlQMD2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits &> /tmp/tmp.cJsI9E8p5n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits &> /tmp/tmp.Fj637L1DsO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits &> /tmp/tmp.9KCPF5fZkU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
The reference image (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits) and catalog (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat) found
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat' -> 'wcsmag.cat'
Read 6528 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 244.8483 to 261.6981 deg, Dec -23.2771 to -12.5709 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 244.8483 to 261.6981 deg, Dec -23.2771 to -12.5709 deg
Loaded 6005 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): 4226 out of 4388 total matches.
Matched with Tycho-2 4388 out of 6528 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.922522
a=0.000000 b=1.000000 c=22.922522
From vast_summary.log: estimated ref. image limiting mag.: -8.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.51
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
2.3 pix Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
3.0 pix fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
3.0 pix fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Limiting magnitude estimates:
14.5 mag. Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
14.5 mag. Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
13.6 mag. fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
13.7 mag. fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.kdwuGlQMD2 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=427, passed=6528
Got 6528 stars (including 6093 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 6528 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 6319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 6319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 6319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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.cJsI9E8p5n (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=6260
Got 6260 stars (including 5826 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 6260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.6)
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...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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.Fj637L1DsO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=278, passed=4156
Got 4156 stars (including 3874 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat
util/solve_plate_with_UCAC5 got 4156 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 4057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 4056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.04"
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 4053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 937 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits -region wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.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.9KCPF5fZkU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=285, passed=4211
Got 4211 stars (including 3921 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat
util/solve_plate_with_UCAC5 got 4211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.03"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.04"
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits -region wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
Saving fully-calibrated image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits'
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits'
Preparing the HTML report for the field Oph-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20263.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20214_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20214_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:05:18.17 -15:36:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20245_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20245_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:39:37.24 -17:53:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.878 4131888766456647424 249.90479179262 -17.88306373658 9.8416 8.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20247_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20247_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:10.11 -18:23:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20248_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20248_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:01:16.16 -14:59:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 2.673 4140077001351085184 255.31752911541 -14.99233768573 10.0480 8.6691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20257_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20257_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:48:58.00 -14:01:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 2.591 4326730713756877952 252.24165492105 -14.01889134906 10.2408 8.8571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20260_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20260_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:30:04.70 -17:48:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 2.395 4323905175031072384 247.51895731245 -17.81156549134 10.5988 9.2785 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20263_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20263_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:33:55.87 -16:47:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.728 4324366969915608576 248.48260629138 -16.79459750289 11.0529 10.0585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20265_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20265_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:31:58.89 -19:52:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20068_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20068_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:09:35.05 -19:02:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20136_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 20136_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:49:02.57 -19:27:51.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Oph-07-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 ####
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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat to cache
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Creating symlink local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits exists and is non-empty
wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits exists and is non-empty
wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits exists and is non-empty
wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:38.432 -18:00:30.56
Angular distance between the image centers 0.0742 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 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:37.876 -17:59:53.71
Angular distance between the image centers 0.0722 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 16:53:38.432 -18:00:30.56
Second-epoch second image center 16:53:37.876 -17:59:53.71
Angular distance between the image centers 0.01047 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits &> /tmp/tmp.n6tOzoeTdd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits &> /tmp/tmp.wGlnIm8h8m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits &> /tmp/tmp.ZevriEodPG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits &> /tmp/tmp.rt0BTszExU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
The reference image (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits) and catalog (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat) found
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat' -> 'wcsmag.cat'
Read 75508 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 244.7958 to 261.7403 deg, Dec -23.2809 to -12.5618 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 244.7958 to 261.7403 deg, Dec -23.2809 to -12.5618 deg
Loaded 6050 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): 4660 out of 5263 total matches.
Matched with Tycho-2 5263 out of 75508 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.684879
a=0.000000 b=1.000000 c=22.684879
From vast_summary.log: estimated ref. image limiting mag.: -7.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.69
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.69
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 147 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
2.0 pix Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
2.6 pix fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
2.6 pix fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Limiting magnitude estimates:
14.7 mag. Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
14.6 mag. Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
14.0 mag. fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
14.0 mag. fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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.n6tOzoeTdd (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=4239, passed=75506
Got 75506 stars (including 71154 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 75506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 73590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 73590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
WARNING: Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 73590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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.wGlnIm8h8m (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=4544, passed=72943
Got 72943 stars (including 68297 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 72943 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 71099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 71100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 71100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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.ZevriEodPG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2264, passed=35254
Got 35254 stars (including 32961 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat
util/solve_plate_with_UCAC5 got 35254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 34642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 34642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 34640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits -region wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.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.rt0BTszExU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2312, passed=35502
Got 35502 stars (including 33162 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat
util/solve_plate_with_UCAC5 got 35502 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 34863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 34863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 34863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits -region wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Saving fully-calibrated image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-18-25_20.00sec_-5.00C_LIGHT_0126.fits
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Oph-07-Q2b1x1_022005_TTUQ2b1x1_1316_SgMDiUfY/wcs_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127.fits
Preparing the HTML report for the field Oph-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out41146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out90724.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out07295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90939.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 17s
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Considering the candidate 90480_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90480_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:46:49.32 -15:55:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90481_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90481_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:07:17.68 -21:25:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.275 4115676192660508416 256.82329101019 -21.42538957991 12.1373 10.7097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90484_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90484_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:30:25.46 -17:15:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.081 4323997534008539520 247.60610117828 -17.26031864461 14.0531 13.3478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90487_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90487_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:47:04.25 -15:37:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.481 4326271354116142720 251.76792172735 -15.62950037070 13.2242 12.2249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90490_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90490_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:43:49.34 -14:05:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90492_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90492_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:07:46.93 -20:47:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90493_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90493_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 90497_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90497_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 90560_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 90560_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 90592_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90592_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:04:38.42 -18:28:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90602_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 90602_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 90640_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90640_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:32:32.06 -18:30:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90652_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90652_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:57:22.20 -18:24:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90658_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90658_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:44:50.14 -20:12:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90664_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90664_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:48:20.29 -15:22:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90673_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90673_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:42:53.77 -15:13:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90695_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90695_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:55:10.65 -21:56:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90701_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90701_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:09:39.78 -19:08:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90709_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90709_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:59.08 -18:53:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90721_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90721_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:25:04.29 -14:02:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.533 4328961863366204672 246.26744219086 -14.04115044695 12.9556 12.0733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90724_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90724_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:39:47.83 -20:52:38.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 90725_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90725_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:37:36.25 -16:49:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90730_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 90730_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 90764_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90764_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:51:06.24 -17:28:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90766_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90766_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:25:24.07 -19:04:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90781_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90781_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:38:30.77 -19:24:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90804_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90804_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:37:28.47 -15:18:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90814_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90814_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:46:52.18 -20:05:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90829_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90829_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:35.71 -14:09:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90874_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90874_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:12:02.63 -20:00:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90875_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90875_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:09:29.92 -21:07:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.252 4115699557283938688 257.37469885775 -21.11850782654 13.1085 11.3135 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90900_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90900_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:25:37.81 -18:06:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.747 4323835493482524288 246.40623486577 -18.10289049311 12.6606 10.8789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90915_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90915_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:41:08.51 -14:39:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.578 4326266582412414592 250.28452403101 -14.65355904938 12.8552 11.5096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90929_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90929_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:27:03.19 -15:37:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.553 4325533070714445568 246.76261427670 -15.62530512412 12.7177 11.0320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90935_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90935_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:03:07.45 -15:27:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.265 4139249648912399232 255.78111384251 -15.45410763895 11.4091 9.6884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90939_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 90939_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 90945_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90945_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:29:53.32 -13:52:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90949_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90949_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:36:15.14 -18:51:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.928 4131403774453846656 249.06256211437 -18.86590291229 12.1180 10.5498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90954_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90954_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:06:12.41 -20:51:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.224 4127722334647691264 256.55224161747 -20.86554952980 12.4096 10.9506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90957_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90957_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:31:45.79 -14:30:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.502 4327198796471827200 247.94090157927 -14.51224323314 13.5808 12.6003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90960_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90960_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:25:54.39 -15:38:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90961_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90961_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:30:18.73 -14:53:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90965_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90965_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:01:16.79 -15:13:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.748 4139225322217291776 255.31982767805 -15.23283671431 12.2407 10.6933 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90967_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90967_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:28:50.83 -14:46:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90974_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90974_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:30:23.67 -13:48:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 0.956 4330270076046643328 247.59847106907 -13.81474730938 14.3500 13.6990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90976_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90976_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:37:17.40 -16:22:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90983_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 90983_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:50:29.51 -20:57:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91028_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91028_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:47.95 -14:21:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.846 4328773365841665280 246.69931544523 -14.35005375900 13.9227 13.1509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91037_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91037_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:48:16.72 -14:05:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91045_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91045_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:27:27.79 -14:22:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.889 4328770754501410944 246.86527141425 -14.37977008709 13.9388 13.2049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91060_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91060_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:38:37.72 -14:21:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.279 4327082935434341760 249.65733096832 -14.35165467269 13.2836 12.0850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91070_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91070_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:43:30.28 -15:45:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.423 4325929165481067264 250.87631516215 -15.75295190217 13.5174 12.7985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91072_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91072_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:35:31.21 -16:15:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91078_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91078_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:36:49.44 -15:22:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 2.454 4326846162476654976 249.20529308918 -15.36734510003 13.6366 12.6035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91079_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91079_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:27:56.78 -13:54:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.182 4330300793652057472 246.98635513919 -13.91199238584 13.8797 13.2095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91080_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91080_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:31:45.95 -13:53:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91082_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91082_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:40:48.77 -14:38:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 0.705 4326267235247463168 250.20302611403 -14.63972031155 13.8963 12.9202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91088_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91088_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:47:43.21 -13:50:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.196 4326749164936452480 251.92996916147 -13.83892539102 13.0951 11.7849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91089_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91089_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:34:47.37 -14:48:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.764 4326961473758879232 248.69738983395 -14.81371180607 13.8413 13.0529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91095_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91095_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:39:00.51 -13:50:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91097_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91097_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:42:10.28 -15:52:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91099_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91099_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:27:13.63 -16:25:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.154 4324861715786982144 246.80689925780 -16.41800596979 13.8229 12.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91104_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91104_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:25:28.63 -15:43:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.716 4325517024716769408 246.36913517194 -15.71704635527 14.0313 13.2487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91106_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91106_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:41:42.27 -14:48:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 2.005 4326249024586041088 250.42605104228 -14.80678101199 13.7886 12.8513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91113_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91113_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:29.73 -15:16:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.848 4325557805430497408 246.62305566068 -15.26874598741 13.4375 12.2997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91117_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91117_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:43:23.83 -14:43:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.755 4326576575968492288 250.84890000123 -14.71791782253 14.1755 13.3001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91119_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91119_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:33:19.80 -13:52:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.545 4327348570570719616 248.33268480043 -13.87191759620 13.9263 13.2071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91133_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91133_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:38:14.42 -14:01:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91136_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91136_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:44:39.85 -15:08:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91143_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91143_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:48:21.00 -14:20:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.992 4326511464262647552 252.08739943615 -14.33314968781 14.0701 13.0290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91149_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91149_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:43:28.33 -14:20:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.864 4326663196872499712 250.86784927975 -14.33420517206 13.9325 13.0163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91158_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91158_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:34:36.74 -14:52:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 0.275 4326934398285038080 248.65303799023 -14.87503471487 13.9352 13.1559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91159_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91159_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:44:30.06 -15:08:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91162_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91162_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:40:21.81 -14:06:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.534 4327421688095163392 250.09104359511 -14.10427307843 13.4910 12.2989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91163_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91163_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:08:48.38 -17:32:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91167_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91167_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:33.03 -16:26:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.445 4325048181791411968 246.63737931123 -16.43681390186 13.6300 12.6365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91173_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91173_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:41:48.54 -15:26:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91182_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91182_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:35:37.77 -17:47:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.823 4324046737154875904 248.90715034014 -17.78569180209 13.2934 12.0678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91199_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91199_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:42:09.62 -16:52:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91200_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91200_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:41:11.85 -14:07:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91263_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91263_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:58:57.03 -14:19:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91269_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 91269_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:03:45.29 -15:10:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.343 4139263775064926848 255.93897294143 -15.17695022626 13.1549 11.8806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62663_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 62663_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 41882_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 41882_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:50:35.72 -18:03:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20486_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 20486_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 51257_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 51257_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:50:42.99 -16:59:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07864_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 07864_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 73959_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 73959_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 15819_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 15819_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 07846_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 07846_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:06:00.41 -21:57:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46074_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 46074_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 40324_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 40324_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 22890_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 22890_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 21531_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 21531_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 32447_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 32447_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:09:35.04 -19:02:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86323_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 86323_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:59:02.56 -21:56:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11704_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 11704_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 38986_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 38986_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:49:55.10 -18:20:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48442_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 48442_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:46:55.78 -17:18:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24363_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 24363_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 19435_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 19435_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:08:18.96 -20:30:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42219_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 42219_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 29565_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 29565_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:01:02.70 -19:23:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10379_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 10379_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 07295_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 07295_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 18469_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 18469_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 36865_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 36865_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:26:10.12 -18:23:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10064_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 10064_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 48950_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 48950_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 45615_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 45615_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 88492_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 88492_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:53:28.34 -20:27:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10031_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 10031_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
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Considering the candidate 68777_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 68777_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:05:18.18 -15:36:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57591_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 57591_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19776_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 19776_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86028_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 86028_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:01:15.94 -19:14:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07405_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 07405_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63733_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 63733_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14672_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 14672_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29369_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 29369_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29642_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 29642_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:03:37.00 -19:22:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32451_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 32451_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41636_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 41636_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44742_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 44742_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12243_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 12243_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:09:57.43 -21:20:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55967_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 55967_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:58:31.44 -13:46:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34351_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 34351_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69379_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 69379_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27431_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 27431_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:04:35.53 -19:38:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11393_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 11393_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:10:49.93 -21:27:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28308_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 28308_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08789_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 08789_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15433_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 15433_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55911_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 55911_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:10:15.07 -13:46:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.023 4139853555674478208 257.56335860306 -13.77688477735 11.6407 9.9688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12554_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 12554_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25341_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 25341_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:43:43.68 -19:48:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23203_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 23203_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:46:39.47 -20:03:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61091_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 61091_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68843_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 68843_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27735_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 27735_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:49:02.57 -19:27:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41146_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 41146_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:08:36.18 -18:09:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.022 4129429704406019840 257.15160830878 -18.15446790448 12.1358 10.6521 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11065_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 11065_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:07:04.46 -21:30:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39572_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 39572_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:59:37.24 -18:19:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60987_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 60987_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09296_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 09296_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 17:10:35.04 -21:44:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07627_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
Preparing report for the candidate 07627_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66299_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127
The candidate 66299_fd_Oph-07-Q2b1x1_2026-04-08_02-19-17_20.00sec_-4.90C_LIGHT_0127 did not pass the final checks
**** FOUND 16:59:27.13 -15:03:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.982 4139995804990592896 254.86293854845 -15.06235721497 12.7752 11.5197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 39s
Prepared the HTML report for the field Oph-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:55:18.02 -22:01:03.4
16:39:15.82 -21:51:48.6
17:08:13.84 -22:00:10.0
17:03:31.62 -21:58:53.7
17:03:25.95 -21:48:16.4
17:09:07.45 -21:39:13.3
16:59:31.32 -21:39:24.7
16:55:28.79 -21:36:04.7
16:47:45.05 -21:24:17.2
16:53:57.41 -21:18:26.9
17:05:58.48 -21:02:19.0
17:04:16.44 -20:56:12.3
16:38:55.38 -20:49:22.7
17:08:14.05 -20:36:00.7
16:56:09.73 -20:27:29.4
16:58:24.05 -20:23:35.7
17:00:05.84 -20:09:40.3
16:41:16.57 -19:57:53.2
16:58:04.40 -19:57:38.2
16:59:30.38 -19:31:09.4
17:05:32.42 -19:24:38.6
16:53:22.92 -19:03:30.2
16:40:37.20 -18:48:16.1
16:51:39.70 -18:13:07.7
17:10:32.14 -18:05:18.2
17:09:06.71 -18:02:11.1
17:05:26.79 -17:46:12.6
16:44:08.59 -17:38:04.2
17:05:33.82 -17:33:55.7
16:34:15.45 -17:09:40.4
17:09:33.72 -16:56:20.6
17:06:46.40 -16:46:50.7
17:08:13.35 -16:45:37.2
16:51:35.31 -16:38:37.0
17:04:51.80 -16:34:27.8
17:09:47.30 -15:26:02.8
16:56:07.86 -15:30:57.4
17:08:27.65 -16:18:59.2
16:55:25.89 -20:41:21.9
16:26:49.11 -14:15:10.6
17:10:36.50 -15:59:22.2
16:28:36.32 -20:06:42.1
########### Completed Oph-07-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 ####
16:55:25.89 -20:41:21.9
16:26:49.11 -14:15:10.6
17:10:36.50 -15:59:22.2
16:28:36.32 -20:06:42.1
16:51:35.31 -16:38:37.0
16:58:24.05 -20:23:35.7
17:03:31.62 -21:58:53.7
17:08:27.65 -16:18:59.2
16:38:55.38 -20:49:22.7
17:05:33.82 -17:33:55.7
16:51:39.70 -18:13:07.7
16:41:16.57 -19:57:53.2
17:00:05.84 -20:09:40.3
16:47:45.05 -21:24:17.2
16:58:04.40 -19:57:38.2
17:09:06.71 -18:02:11.1
16:55:28.79 -21:36:04.7
16:55:18.02 -22:01:03.4
17:08:14.05 -20:36:00.7
16:59:31.32 -21:39:24.7
16:34:15.45 -17:09:40.4
16:44:08.59 -17:38:04.2
17:09:07.45 -21:39:13.3
17:09:33.72 -16:56:20.6
16:56:09.73 -20:27:29.4
16:39:15.82 -21:51:48.6
17:04:51.80 -16:34:27.8
17:05:58.48 -21:02:19.0
17:05:32.42 -19:24:38.6
16:53:22.92 -19:03:30.2
17:10:32.14 -18:05:18.2
17:05:26.79 -17:46:12.6
16:40:37.20 -18:48:16.1
16:56:07.86 -15:30:57.4
16:59:30.38 -19:31:09.4
17:03:25.95 -21:48:16.4
17:04:16.44 -20:56:12.3
16:53:57.41 -21:18:26.9
17:08:13.35 -16:45:37.2
17:09:47.30 -15:26:02.8
17:06:46.40 -16:46:50.7
17:08:13.84 -22:00:10.0
###################################################################################
16:55:25.89 -20:41:21.9 -- asteroid (will NOT add it to exclusion list)
16:26:49.11 -14:15:10.6 -- asteroid (will NOT add it to exclusion list)
17:10:36.50 -15:59:22.2 -- asteroid (will NOT add it to exclusion list)
16:28:36.32 -20:06:42.1 -- asteroid (will NOT add it to exclusion list)
16:51:35.31 -16:38:37.0 -- not an asteroid (will add it to exclusion list)
16:58:24.05 -20:23:35.7 -- not an asteroid (will add it to exclusion list)
17:03:31.62 -21:58:53.7 -- not an asteroid (will add it to exclusion list)
17:08:27.65 -16:18:59.2 -- not an asteroid (will add it to exclusion list)
16:38:55.38 -20:49:22.7 -- not an asteroid (will add it to exclusion list)
17:05:33.82 -17:33:55.7 -- not an asteroid (will add it to exclusion list)
16:51:39.70 -18:13:07.7 -- not an asteroid (will add it to exclusion list)
16:41:16.57 -19:57:53.2 -- not an asteroid (will add it to exclusion list)
17:00:05.84 -20:09:40.3 -- not an asteroid (will add it to exclusion list)
16:47:45.05 -21:24:17.2 -- not an asteroid (will add it to exclusion list)
16:58:04.40 -19:57:38.2 -- not an asteroid (will add it to exclusion list)
17:09:06.71 -18:02:11.1 -- not an asteroid (will add it to exclusion list)
16:55:28.79 -21:36:04.7 -- not an asteroid (will add it to exclusion list)
16:55:18.02 -22:01:03.4 -- not an asteroid (will add it to exclusion list)
17:08:14.05 -20:36:00.7 -- not an asteroid (will add it to exclusion list)
16:59:31.32 -21:39:24.7 -- not an asteroid (will add it to exclusion list)
16:34:15.45 -17:09:40.4 -- not an asteroid (will add it to exclusion list)
16:44:08.59 -17:38:04.2 -- not an asteroid (will add it to exclusion list)
17:09:07.45 -21:39:13.3 -- not an asteroid (will add it to exclusion list)
17:09:33.72 -16:56:20.6 -- not an asteroid (will add it to exclusion list)
16:56:09.73 -20:27:29.4 -- not an asteroid (will add it to exclusion list)
16:39:15.82 -21:51:48.6 -- not an asteroid (will add it to exclusion list)
17:04:51.80 -16:34:27.8 -- not an asteroid (will add it to exclusion list)
17:05:58.48 -21:02:19.0 -- not an asteroid (will add it to exclusion list)
17:05:32.42 -19:24:38.6 -- not an asteroid (will add it to exclusion list)
16:53:22.92 -19:03:30.2 -- not an asteroid (will add it to exclusion list)
17:10:32.14 -18:05:18.2 -- not an asteroid (will add it to exclusion list)
17:05:26.79 -17:46:12.6 -- not an asteroid (will add it to exclusion list)
16:40:37.20 -18:48:16.1 -- not an asteroid (will add it to exclusion list)
16:56:07.86 -15:30:57.4 -- not an asteroid (will add it to exclusion list)
16:59:30.38 -19:31:09.4 -- not an asteroid (will add it to exclusion list)
17:03:25.95 -21:48:16.4 -- not an asteroid (will add it to exclusion list)
17:04:16.44 -20:56:12.3 -- not an asteroid (will add it to exclusion list)
16:53:57.41 -21:18:26.9 -- not an asteroid (will add it to exclusion list)
17:08:13.35 -16:45:37.2 -- not an asteroid (will add it to exclusion list)
17:09:47.30 -15:26:02.8 -- not an asteroid (will add it to exclusion list)
17:06:46.40 -16:46:50.7 -- not an asteroid (will add it to exclusion list)
17:08:13.84 -22:00:10.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:34:15.45 -17:09:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:55.38 -20:49:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:15.82 -21:51:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:37.20 -18:48:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:16.57 -19:57:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:08.59 -17:38:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:45.05 -21:24:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:35.31 -16:38:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:39.70 -18:13:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:22.92 -19:03:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:57.41 -21:18:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:18.02 -22:01:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:28.79 -21:36:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:07.86 -15:30:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:09.73 -20:27:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:04.40 -19:57:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:24.05 -20:23:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:30.38 -19:31:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:31.32 -21:39:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:05.84 -20:09:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:25.95 -21:48:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:03:31.62 -21:58:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:16.44 -20:56:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:04:51.80 -16:34:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:26.79 -17:46:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:32.42 -19:24:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:33.82 -17:33:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:05:58.48 -21:02:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:46.40 -16:46:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:13.35 -16:45:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:13.84 -22:00:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:14.05 -20:36:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:27.65 -16:18:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:06.71 -18:02:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:07.45 -21:39:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:33.72 -16:56:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:09:47.30 -15:26:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:10:32.14 -18:05:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
16:34:15.45 -17:09:40.4 -- a known variable star
16:38:55.38 -20:49:22.7 -- a known variable star
16:39:15.82 -21:51:48.6 -- a known variable star
16:40:37.20 -18:48:16.1 -- a known variable star
16:41:16.57 -19:57:53.2 -- a known variable star
16:44:08.59 -17:38:04.2 -- a known variable star
16:47:45.05 -21:24:17.2 -- a known variable star
16:51:35.31 -16:38:37.0 -- a known variable star
16:51:39.70 -18:13:07.7 -- a known variable star
16:53:22.92 -19:03:30.2 -- a known variable star
16:53:57.41 -21:18:26.9 -- a known variable star
16:55:18.02 -22:01:03.4 -- a known variable star
16:55:28.79 -21:36:04.7 -- a known variable star
16:56:07.86 -15:30:57.4 -- a known variable star
16:56:09.73 -20:27:29.4 -- a known variable star
16:58:04.40 -19:57:38.2 -- a known variable star
16:58:24.05 -20:23:35.7 -- a known variable star
16:59:30.38 -19:31:09.4 -- a known variable star
16:59:31.32 -21:39:24.7 -- a known variable star
17:00:05.84 -20:09:40.3 -- a known variable star
17:03:25.95 -21:48:16.4 -- a known variable star
17:03:31.62 -21:58:53.7 -- a known variable star
17:04:16.44 -20:56:12.3 -- a known variable star
17:04:51.80 -16:34:27.8 -- a known variable star
17:05:26.79 -17:46:12.6 -- a known variable star
17:05:32.42 -19:24:38.6 -- a known variable star
17:05:33.82 -17:33:55.7 -- a known variable star
17:05:58.48 -21:02:19.0 -- a known variable star
17:06:46.40 -16:46:50.7 -- a known variable star
17:08:13.35 -16:45:37.2 -- a known variable star
17:08:13.84 -22:00:10.0 -- a known variable star
17:08:14.05 -20:36:00.7 -- not a known variable star
17:08:27.65 -16:18:59.2 -- a known variable star
17:09:06.71 -18:02:11.1 -- a known variable star
17:09:07.45 -21:39:13.3 -- a known variable star
17:09:33.72 -16:56:20.6 -- a known variable star
17:09:47.30 -15:26:02.8 -- a known variable star
17:10:32.14 -18:05:18.2 -- a known variable star
Found 1 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
38 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 ####
16:34:15.45 -17:09:40.4
16:38:55.38 -20:49:22.7
16:39:15.82 -21:51:48.6
16:40:37.20 -18:48:16.1
16:41:16.57 -19:57:53.2
16:44:08.59 -17:38:04.2
16:47:45.05 -21:24:17.2
16:51:35.31 -16:38:37.0
16:51:39.70 -18:13:07.7
16:53:22.92 -19:03:30.2
16:53:57.41 -21:18:26.9
16:55:18.02 -22:01:03.4
16:55:28.79 -21:36:04.7
16:56:07.86 -15:30:57.4
16:56:09.73 -20:27:29.4
16:58:04.40 -19:57:38.2
16:58:24.05 -20:23:35.7
16:59:30.38 -19:31:09.4
16:59:31.32 -21:39:24.7
17:00:05.84 -20:09:40.3
17:03:25.95 -21:48:16.4
17:03:31.62 -21:58:53.7
17:04:16.44 -20:56:12.3
17:04:51.80 -16:34:27.8
17:05:26.79 -17:46:12.6
17:05:32.42 -19:24:38.6
17:05:33.82 -17:33:55.7
17:05:58.48 -21:02:19.0
17:06:46.40 -16:46:50.7
17:08:13.35 -16:45:37.2
17:08:13.84 -22:00:10.0
17:08:14.05 -20:36:00.7
17:08:27.65 -16:18:59.2
17:09:06.71 -18:02:11.1
17:09:07.45 -21:39:13.3
17:09:33.72 -16:56:20.6
17:09:47.30 -15:26:02.8
17:10:32.14 -18:05:18.2
16:39:37.24 -17:53:00.4
17:01:16.16 -14:59:35.0
16:48:58.00 -14:01:10.6
16:30:04.70 -17:48:42.7
16:33:55.87 -16:47:40.9
17:08:36.18 -18:09:16.8
17:10:15.07 -13:46:41.4
16:59:27.13 -15:03:45.4
17:07:17.68 -21:25:31.2
16:30:25.46 -17:15:37.2
16:47:04.25 -15:37:42.8
16:25:04.29 -14:02:28.4
17:09:29.92 -21:07:06.4
16:25:37.81 -18:06:12.0
16:41:08.51 -14:39:14.3
16:27:03.19 -15:37:32.1
17:03:07.45 -15:27:14.7
16:36:15.14 -18:51:56.5
17:06:12.41 -20:51:53.3
16:31:45.79 -14:30:44.4
17:01:16.79 -15:13:59.9
16:30:23.67 -13:48:52.3
16:26:47.95 -14:21:01.0
16:27:27.79 -14:22:47.7
16:38:37.72 -14:21:07.1
16:43:30.28 -15:45:09.3
16:36:49.44 -15:22:02.4
16:27:56.78 -13:54:42.3
16:40:48.77 -14:38:23.3
16:47:43.21 -13:50:21.3
16:34:47.37 -14:48:48.6
16:27:13.63 -16:25:02.7
16:25:28.63 -15:43:00.9
16:41:42.27 -14:48:26.4
16:26:29.73 -15:16:07.6
16:43:23.83 -14:43:03.4
16:33:19.80 -13:52:17.5
16:48:21.00 -14:20:01.3
16:43:28.33 -14:20:01.4
16:34:36.74 -14:52:29.9
16:40:21.81 -14:06:16.8
16:26:33.03 -16:26:13.7
16:35:37.77 -17:47:08.2
17:03:45.29 -15:10:38.0
16:39:47.83 -20:52:38.9
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461138.80457866 -observatory V36
23:29:35.73 -05:40:30.3 Mercury (0.3mag)
02:31:31.02 +14:45:54.4 Venus (-3.9mag)
23:55:56.38 -01:32:50.5 Mars (1.2mag)
07:09:27.37 +22:51:17.3 Jupiter (-2.2mag)
00:25:43.24 +00:27:16.8 Saturn (0.9mag)
03:46:07.87 +19:42:25.3 Uranus (5.8mag)
00:09:48.97 -00:21:51.0 Neptune (7.8mag)
20:33:21.78 -22:52:27.3 Pluto (14.5mag)
17:50:49.38 -28:51:06.7 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 02:21 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461138.80457866:
07:09:22.24 +22:51:25.1 Io (5.7mag)
07:09:18.28 +22:51:37.9 Europa (5.9mag)
07:09:47.79 +22:50:36.2 Ganymede (5.3mag)
07:08:52.55 +22:52:26.9 Callisto (6.5mag)
07:13:06.05 +22:42:41.3 Himalia (15.3mag)
07:09:27.71 +22:51:18.8 Thebe (16.2mag)
07:13:06.82 +23:11:53.4 Elara (17.3mag)
07:07:48.83 +23:35:19.2 Pasiphae (17.4mag)
07:17:56.76 +22:48:28.8 Carme (18.4mag)
00:25:46.46 +00:27:07.1 Titan (8.8mag)
00:25:48.58 +00:27:17.3 Rhea (10.1mag)
00:25:38.98 +00:28:34.9 Iapetus (11.5mag)
00:25:52.22 +00:27:02.2 Hyperion (14.8mag)
00:27:25.98 +00:36:53.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 02:21 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.80457866:
14:59:12.70 -10:14:20.5 JWST
14:25:31.25 +56:26:30.8 Chandra
08:20:13.76 -44:38:26.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 02:21 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.80457866 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:19.70 -28:20:50.1 13.9mag P/2010 H2 (Vales)
05:01:26.72 -70:02:21.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:55.73 +31:23:17.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:55.07 +09:37:34.1 17.6mag C/2021 G2 (ATLAS)
23:08:01.04 +28:56:25.5 17.0mag C/2022 E2 (ATLAS)
04:20:22.75 +25:49:28.3 15.9mag C/2022 N2 (PANSTARRS)
09:02:05.98 +31:56:25.2 16.2mag C/2022 QE78 (ATLAS)
08:30:08.63 -00:59:34.4 17.3mag C/2022 R6 (PANSTARRS)
18:55:16.43 +17:52:38.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:57.85 -11:37:54.5 17.6mag P/2023 B1 (PANSTARRS)
09:11:35.69 -13:08:45.3 17.6mag C/2023 F3 (ATLAS)
21:45:57.04 +62:28:45.2 17.5mag C/2023 H5 (Lemmon)
19:25:04.70 -03:37:44.9 14.2mag C/2023 R1 (PANSTARRS)
21:41:49.54 +84:52:43.2 17.8mag C/2023 X2 (Lemmon)
06:15:01.76 +63:33:49.1 17.1mag C/2024 A1 (ATLAS)
04:56:04.86 +15:27:32.9 10.5mag C/2024 E1 (Wierzchos)
16:23:56.24 +05:07:31.2 17.4mag C/2024 G6 (ATLAS)
20:18:20.57 +13:13:41.5 14.7mag C/2024 J3 (ATLAS)
03:19:34.84 -23:35:01.3 16.4mag C/2024 T5 (ATLAS)
05:10:22.05 +47:15:57.8 17.7mag C/2025 J1 (Borisov)
14:10:38.04 +39:26:31.8 14.9mag C/2025 L1 (ATLAS)
03:13:28.35 -25:03:08.1 17.8mag C/2025 Q3 (ATLAS)
22:59:45.84 +19:48:26.7 9.8mag C/2025 R3 (PANSTARRS)
12:57:28.23 +02:31:47.3 17.5mag C/2025 Y1 (ATLAS)
02:05:18.58 +03:57:51.8 9.7mag C/2026 A1 (MAPS)
23:37:10.91 +35:42:06.7 14.3mag C/2026 B2 (Sun-Gao)
18:27:55.44 -10:07:00.6 12.3mag 10P/Tempel
15:10:21.20 +03:56:19.5 13.3mag 24P/Schaumasse
11:05:04.21 -01:47:15.1 15.7mag 29P/Schwassmann-Wachmann
17:57:54.85 -09:54:26.9 17.8mag 40P/Vaisala
10:38:25.85 -04:45:11.6 16.8mag 43P/Wolf-Harrington
01:36:47.90 +16:09:50.5 17.2mag 47P/Ashbrook-Jackson
06:56:57.23 +38:38:31.0 17.0mag 63P/Wild
23:19:05.98 -12:23:27.8 15.7mag 65P/Gunn
03:43:04.15 +18:31:17.6 15.9mag 76P/West-Kohoutek-Ikemura
00:48:40.53 +06:42:22.8 14.4mag 78P/Gehrels
22:39:15.02 -11:39:24.2 14.5mag 88P/Howell
01:48:56.37 +18:32:30.0 15.1mag 93P/Lovas
04:40:39.67 +31:51:17.4 16.3mag 123P/West-Hartley
08:19:57.28 +41:54:53.0 16.2mag 124P/Mrkos
02:21:25.09 +13:30:00.1 16.4mag 128P/Shoemaker-Holt
02:32:30.09 +13:31:42.3 17.5mag 131P/Mueller
00:46:27.98 +10:25:45.1 11.1mag 141P/Machholz
00:56:16.73 +01:59:07.4 11.1mag 141P-A/Machholz
23:45:37.25 -01:45:23.3 13.8mag 141P-D/Machholz
01:25:43.73 +03:40:57.3 17.9mag 141P-I/Machholz
00:40:59.32 -05:22:24.7 15.2mag 162P/SidingSpring
10:30:19.90 +31:22:35.9 17.9mag 164P/Christensen
06:22:17.94 +24:28:18.0 17.9mag 198P/ODAS
15:05:02.65 -00:56:01.2 17.4mag 210P/Christensen
21:15:39.16 -13:18:40.1 17.5mag 218P/LINEAR
17:13:43.79 -14:50:09.9 16.2mag 235P/LINEAR
05:18:04.39 +34:03:20.6 16.6mag 240P/NEAT
07:35:01.48 -06:02:06.8 17.6mag 242P/Spahr
15:45:19.78 +06:27:41.5 17.5mag 391P/Kowalski
07:31:31.87 +21:19:39.9 17.6mag 450P/LONEOS
05:24:51.17 +45:29:07.1 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 02:21 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 8 02:21 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:30:09.406 +58:57:13.42 AT 2026icx 2026-03-30.43 19.684
11:28:54.874 +21:06:30.69 AT 2026icw 2026-04-02.30 19.2031
12:10:50.697 +66:55:30.99 SN 2026icv 2026-04-02.28 18.5118
07:36:32.513 +50:19:24.81 AT 2026icu 2026-04-02.24 19.2237
08:38:37.560 +02:03:38.03 AT 2026ict 2026-04-02.15 19.0837
10:11:03.633 -05:31:15.36 AT 2026ics 2026-04-02.23 18.6573
11:09:42.183 +10:32:49.70 AT 2026icr 2026-03-24.33 20.476
10:16:29.552 -18:01:01.61 AT 2026icq 2026-03-25.18 20.2716
18:12:46.220 -18:40:42.30 AT 2026icp 2026-04-02.23 18.9
07:46:30.650 +27:23:24.16 AT 2026ico 2026-03-30.16 19.803
07:04:53.063 +10:28:54.71 AT 2026icn 2026-03-29.17 19.8144
10:09:06.230 +29:30:55.76 AT 2026icm 2026-03-27.16 20.1135
08:07:47.384 -00:23:25.65 AT 2026icl 2026-03-30.25 19.1418
07:33:52.396 +16:18:53.23 AT 2026ick 2026-03-30.19 19.5464
03:49:33.049 -49:30:53.67 AT 2026icj 2026-02-23.11 23.84
15:40:04.940 -18:30:53.00 AT 2026ici 2026-03-29.36 18.4
16:52:58.870 -62:16:14.10 AT 2026ich 2026-04-01.35 16.9
19:13:48.516 +60:10:55.03 AT 2026icg 2026-03-28.56 18.844
07:51:19.796 +21:17:20.06 AT 2026icf 2026-03-30.91 18.372
16:10:07.169 +56:12:02.29 AT 2026ice 2026-04-01.56 19.57
-rw-r--r-- 1 apache apache 30K Apr 8 02:21 tns_transients_list.txt
