This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt
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
ASAS J194552+2034.1,2461136.8295,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J194552+2034.1 20260406.3295 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3,2461136.8295,13.52,0.05,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
Gaia DR3 20260406.3295 13.52CV 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
target,2461136.8295,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.3295 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193150.66+225741.2,2461136.8295,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193150.66+225741.2 20260406.3295 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.3579+23.5240,2461136.8295,12.89,0.05,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
ATO J297.3579+23.5240 20260406.3295 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
target,2461136.8295,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.3295 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.2476+20.4859,2461136.8295,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J297.2476+20.4859 20260406.3295 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
Gaia DR3 1827574731283910912,2461136.8295,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827574731283910912 20260406.3295 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194904.91+214610.7,2461136.8295,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194904.91+214610.7 20260406.3295 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194816.35+204303.8,2461136.8295,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194816.35+204303.8 20260406.3295 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IV Sge,2461136.8295,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IV Sge 20260406.3295 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194853.15+200719.1,2461136.8295,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194853.15+200719.1 20260406.3295 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J290.0526+25.3900,2461136.8295,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J290.0526+25.3900 20260406.3295 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193617.54+175149.3,2461136.8295,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193617.54+175149.3 20260406.3295 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192716.44+200003.0,2461136.8295,12.98,0.05,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 J192716.44+200003.0 20260406.3295 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
ZTF J191441.69+191500.2,2461136.8295,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191441.69+191500.2 20260406.3295 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194051.39+255011.2,2461136.8295,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194051.39+255011.2 20260406.3295 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194153.49+212014.3,2461136.8295,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194153.49+212014.3 20260406.3295 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192555+2330.6,2461136.8295,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192555+2330.6 20260406.3295 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11213314,2461136.8295,13.37,0.05,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
NSVS 11213314 20260406.3295 13.37CV 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
Gaia DR3 1827481135313692032,2461136.8295,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827481135313692032 20260406.3295 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1948499+221010,2461136.8295,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1948499+221010 20260406.3295 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194718.16+201808.3,2461136.8295,12.49,0.05,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 J194718.16+201808.3 20260406.3295 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194641.71+204231.2,2461136.8295,12.85,0.05,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
ZTF J194641.71+204231.2 20260406.3295 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
NSVS 11252248,2461136.8295,12.55,0.05,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 11252248 20260406.3295 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193308.12+182927.8,2461136.8295,12.66,0.05,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
ASASSN-V J193308.12+182927.8 20260406.3295 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11249151,2461136.8295,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11249151 20260406.3295 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1922349+191042,2461136.8295,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1922349+191042 20260406.3295 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1931308+174927,2461136.8295,12.28,0.05,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 J1931308+174927 20260406.3295 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1938420+242505,2461136.8295,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1938420+242505 20260406.3295 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193340.36+255046.7,2461136.8295,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193340.36+255046.7 20260406.3295 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1825709375453586048,2461136.8295,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1825709375453586048 20260406.3295 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1919040+250038,2461136.8295,12.88,0.05,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 J1919040+250038 20260406.3295 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.4602+22.8901,2461136.8295,12.62,0.05,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
ATO J286.4602+22.8901 20260406.3295 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 J1916569+185207,2461136.8295,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1916569+185207 20260406.3295 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194558+2212.2,2461136.8295,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J194558+2212.2 20260406.3295 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0690,2461136.8295,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V0690 20260406.3295 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192044.14+174251.7,2461136.8295,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192044.14+174251.7 20260406.3295 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194826.65+233210.2,2461136.8295,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J194826.65+233210.2 20260406.3295 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192758.85+223319.6,2461136.8295,13.32,0.05,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 J192758.85+223319.6 20260406.3295 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J193334.87+231700.6,2461136.8295,12.92,0.05,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 J193334.87+231700.6 20260406.3295 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1944365+222849,2461136.8295,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1944365+222849 20260406.3295 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1921463+241122,2461136.8295,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1921463+241122 20260406.3295 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11259091,2461136.8295,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11259091 20260406.3295 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8367053,2461136.8295,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8367053 20260406.3295 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0342 Vul,2461136.8295,13.35,0.05,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
V0342 Vul 20260406.3295 13.35CV 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
ASAS J191714+2048.6,2461136.8295,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J191714+2048.6 20260406.3295 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.8295,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.3295 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0349 Vul,2461136.8295,12.52,0.05,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
V0349 Vul 20260406.3295 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
NSVS 11222340,2461136.8295,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11222340 20260406.3295 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11230768,2461136.8295,12.98,0.05,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
NSVS 11230768 20260406.3295 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
Gaia DR3 1827587719271430656,2461136.8295,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827587719271430656 20260406.3295 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1914126+233323,2461136.8295,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1914126+233323 20260406.3295 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194649.55+223310.2,2461136.8295,12.46,0.05,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 J194649.55+223310.2 20260406.3295 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 J190806.32+192518.2,2461136.8295,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190806.32+192518.2 20260406.3295 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190808.67+182812.6,2461136.8295,13.14,0.05,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 J190808.67+182812.6 20260406.3295 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1930177+240021,2461136.8295,13.30,0.05,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
NSVS J1930177+240021 20260406.3295 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193736.61+201556.3,2461136.8295,12.89,0.05,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 J193736.61+201556.3 20260406.3295 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
ZTF J193517.52+240339.3,2461136.8295,12.98,0.05,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
ZTF J193517.52+240339.3 20260406.3295 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
ATO J288.6957+18.4797,2461136.8295,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6957+18.4797 20260406.3295 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J185904+1818.8,2461136.8295,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J185904+1818.8 20260406.3295 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1947246+235035,2461136.8295,12.28,0.05,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 J1947246+235035 20260406.3295 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J190956+1800.2,2461136.8295,10.77,0.05,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
ASAS J190956+1800.2 20260406.3295 10.77CV 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
NSVS J1943476+215523,2461136.8295,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1943476+215523 20260406.3295 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194454+2042.4,2461136.8295,12.32,0.05,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 J194454+2042.4 20260406.3295 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J1917440+195001,2461136.8295,12.37,0.05,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
NSVS J1917440+195001 20260406.3295 12.37CV 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
ASASSN-V J194713.91+210539.2,2461136.8295,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J194713.91+210539.2 20260406.3295 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461136.82976815 06.04.2026 07:54:41.968 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17322
Objects passed selection criteria: 17276
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 14512.8
Average stars matched: 14206 (97.8863 %)
Memory usage VmPeak: 123760 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 02:59:16 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461136.82976815 06.04.2026 07:54:41.968 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 389
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 79 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): 171530
Objects passed selection criteria: 171144
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 137615
Average stars matched: 131695 (95.6982 %)
Memory usage VmPeak: 2519444 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 03:04:41 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.82918583
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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits'
wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:05.402 +21:59:28.62
Angular distance between the image centers 0.0053 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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:06.674 +21:58:58.98
Angular distance between the image centers 0.0142 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 19:23:05.402 +21:59:28.62
Second-epoch second image center 19:23:06.674 +21:58:58.98
Angular distance between the image centers 0.00959 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.POyj59QT0x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.ZxwmPjLn6Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits &> /tmp/tmp.xsiUtbcWXa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits &> /tmp/tmp.IhBY7Axkd5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 24236 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.8547 to 299.3973 deg, Dec +16.3386 to +27.3318 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 281.8547 to 299.3973 deg, Dec 16.3386 to 27.3318 deg
Loaded 19386 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): 13292 out of 14431 total matches.
Matched with Tycho-2 14431 out of 24236 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881026
a=0.000000 b=1.000000 c=22.881026
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
3.0 pix fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
2.9 pix fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Limiting magnitude estimates:
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.1 mag. fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
14.1 mag. fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.5 (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.POyj59QT0x (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2379, passed=24232
Got 24232 stars (including 21810 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 24232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 963 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: 960 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 23277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.ZxwmPjLn6Z (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2427, passed=23940
Got 23940 stars (including 21482 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 23940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 965 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: 963 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 22698 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 22701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 22701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.xsiUtbcWXa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=912, passed=12095
Got 12095 stars (including 11175 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat
util/solve_plate_with_UCAC5 got 12095 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 956 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: 949 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 12034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 12035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 12035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.09"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.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.IhBY7Axkd5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=965, passed=12139
Got 12139 stars (including 11164 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat
util/solve_plate_with_UCAC5 got 12139 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 952 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: 948 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 12042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 12042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 12042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.07"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out12103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out08878.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31198_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31198_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:00:28.13 +20:11:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 0.306 4518193994967854336 285.11712847042 +20.18929352157 10.2950 9.8542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31205_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31205_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:33.67 +22:44:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31210_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31210_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:05:00.98 +18:02:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31211_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31211_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:06:01.03 +17:34:35.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31214_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31214_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:57:18.96 +19:37:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03107_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 03107_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:33:24.05 +18:01:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30071_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 30071_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:46:16.39 +20:22:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12103_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 12103_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:04.56 +22:11:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.40, MAG_FAINT_SEARCH_LIMIT=11.38)GAIADR2_OUTPUT=# 4.448 1827587719271430656 297.27006722652 +22.19101938914 9.7197 8.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21588_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 21588_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:02:34.25 +25:50:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12393_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 12393_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:35:41.30 +22:20:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09662_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 09662_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:12.21 +20:58:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16193_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 16193_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:58.61 +24:09:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08878_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 08878_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Vul-01-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 ####
19:45:50.76 +20:34:05.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:05.402 +21:59:28.62
Angular distance between the image centers 0.0053 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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:06.674 +21:58:58.98
Angular distance between the image centers 0.0142 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 19:23:05.402 +21:59:28.62
Second-epoch second image center 19:23:06.674 +21:58:58.98
Angular distance between the image centers 0.00959 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.0tX9sHtq63
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.ZHUen7Mg2S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits &> /tmp/tmp.1ds9nk3lIm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits &> /tmp/tmp.TPwJ5Cjepk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Read 221580 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 281.8126 to 299.4110 deg, Dec +16.3329 to +27.3345 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 281.8126 to 299.4110 deg, Dec 16.3329 to 27.3345 deg
Loaded 19480 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): 11172 out of 15518 total matches.
Matched with Tycho-2 15518 out of 221580 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709941
a=0.000000 b=1.000000 c=22.709941
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 244 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
1.9 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
2.6 pix fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
2.5 pix fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Limiting magnitude estimates:
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.2 mag. fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
14.2 mag. fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (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.0tX9sHtq63 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=30047, passed=221539
Got 221539 stars (including 191094 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 221539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 961 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: 958 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 209246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 209246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 209247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.ZHUen7Mg2S (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=30936, passed=228140
Got 228140 stars (including 196813 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 228140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 965 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: 963 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 219012 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 219015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 219013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.1ds9nk3lIm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=9108, passed=93392
Got 93392 stars (including 84149 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat
util/solve_plate_with_UCAC5 got 93392 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 92666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 92666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 92666 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.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.TPwJ5Cjepk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=9584, passed=95038
Got 95038 stars (including 85347 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat
util/solve_plate_with_UCAC5 got 95038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 951 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: 948 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 94201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 94201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 94189 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 947 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-53-51_20.00sec_-4.90C_LIGHT_0282.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Vul-01-Q2b1x1_025526_TTUQ2b1x1_31810_jyS6CYzt/wcs_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out233822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out235508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out252809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out254579.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out103744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out233157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out233990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out238500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96267.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 44s
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: 31s
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Considering the candidate 254439_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254439_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:24:47.04 +23:57:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.794 2022736803930269312 291.19593732075 +23.95541300541 12.1421 10.6004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254442_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254442_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:39:20.92 +25:39:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254448_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254448_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:37:25.51 +22:12:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.736 2018416960179535744 294.35612602059 +22.20005907359 12.9787 11.6561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254451_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254451_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:18:13.28 +22:49:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254456_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254456_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254463_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254463_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:32:48.19 +25:46:22.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 254469_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254469_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:42:08.33 +24:29:58.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 254471_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254471_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:31:32.08 +20:18:41.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)
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Considering the candidate 254472_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254472_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:33.49 +24:32:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.565 2020645773326307584 297.13961069431 +24.53354209216 12.7010 12.1810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254474_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254474_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:33:54.45 +18:31:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.608 4323150875720496128 293.47744994665 +18.52155071144 13.9582 12.7832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254479_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254479_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:15:11.46 +25:01:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.982 2023513132177942400 288.79927686412 +25.02625000726 14.1350 13.5055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254481_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254481_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254491_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254491_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:57:52.19 +24:08:55.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 254496_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254496_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:09:11.10 +25:04:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254501_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254501_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254505_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254505_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:11:57.19 +24:20:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.859 2023371673129342848 287.98815143827 +24.33675043532 11.8845 10.2845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254516_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254516_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 254520_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254520_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:16:51.77 +23:34:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.235 2022513057632138368 289.21533544185 +23.58260868465 13.3131 12.2213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254521_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254521_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:11:20.98 +21:24:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254533_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254533_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:21.45 +22:43:59.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 254535_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254535_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254554_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254554_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254557_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254557_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:45:17.26 +25:21:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.810 2020947559236332672 296.32293526186 +25.36216308685 12.4307 11.2506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254560_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254560_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:55:17.24 +18:45:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.616 4517613216623520512 283.82261016847 +18.76093905412 13.2945 12.6921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254565_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254565_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:19:14.25 +19:12:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.251 4515402889018864128 289.80930449382 +19.20435364165 12.7311 12.0716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254575_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254575_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:40:32.71 +18:45:22.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)
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Considering the candidate 254577_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254577_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:00:25.10 +25:26:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254579_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254579_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:42:07.53 +18:40:51.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 254580_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254580_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:26:42.13 +26:09:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254581_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254581_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254584_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254584_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254587_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254587_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:22:02.44 +23:55:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.447 2022771683406009344 290.50948727079 +23.91955417788 12.6641 11.5738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254588_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254588_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:39:34.45 +18:29:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254589_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254589_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254593_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254593_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:34.52 +24:44:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254595_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254595_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 254596_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254596_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:42:30.34 +25:25:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254597_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254597_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:33.76 +21:09:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.517 1825918179574136960 295.88972098923 +21.16577390525 12.0936 11.5943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254598_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254598_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:57:55.78 +25:58:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.755 4534788099328026624 284.48264375599 +25.97393685140 12.9234 12.1786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254600_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254600_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:41.22 +23:43:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254601_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254601_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:24.21 +20:19:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254605_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254605_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:20.41 +20:33:28.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)
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Considering the candidate 254610_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254610_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:42:42.13 +23:16:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254613_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254613_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:44:07.59 +26:00:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.001 2021800397976540672 296.03131808990 +26.01318730549 11.7816 11.2685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254615_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254615_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:53:10.16 +25:40:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254618_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254618_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:39:53.25 +18:18:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254621_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254621_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:28:53.47 +24:38:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254626_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254626_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:04:42.14 +23:19:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254639_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254639_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:19.66 +21:11:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254645_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254645_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:07:22.18 +25:57:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254648_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254648_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:54:38.18 +22:40:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254649_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254649_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:12.12 +20:52:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254651_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254651_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:07:57.59 +21:42:40.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254655_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254655_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:21:03.16 +20:02:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254656_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254656_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:59:26.81 +24:47:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254657_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254657_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:04:45.22 +23:18:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254659_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254659_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:04:53.28 +23:19:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254678_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254678_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:01:01.29 +19:17:48.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254679_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254679_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254700_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254700_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:54:29.04 +20:20:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254710_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254710_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:07:57.17 +19:52:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254715_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254715_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:09:08.73 +25:19:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254717_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254717_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:25:27.06 +20:15:14.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254722_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254722_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:17:43.70 +25:49:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254725_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254725_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:36:25.46 +23:56:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254728_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254728_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:09.02 +25:33:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254733_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254733_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:24:19.76 +25:14:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254735_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254735_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:24:20.84 +20:00:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254736_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254736_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:25:28.80 +24:56:31.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254738_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254738_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:45:00.98 +25:00:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254739_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254739_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:04:34.53 +22:06:35.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 254744_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254744_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:41:12.75 +18:08:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.554 1824098105545893504 295.30383991427 +18.14848958240 11.7449 10.3476 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254747_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254747_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:00:38.03 +18:27:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254749_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254749_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:56:37.20 +21:22:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254751_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254751_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:05:40.61 +25:18:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.995 2035718913827066624 286.41907631136 +25.30388810201 13.3765 12.6530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254754_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254754_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:08:11.72 +25:22:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254756_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254756_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:11.35 +20:10:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254758_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254758_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:16.60 +23:17:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254762_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254762_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:41:02.07 +24:52:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 5.402 2021561292890091264 295.25975326216 +24.87626409326 11.9474 10.2643 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254763_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254763_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:15:13.64 +21:14:52.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254764_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254764_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:08:46.10 +24:10:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254767_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254767_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:06:20.05 +21:22:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254769_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254769_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:07:12.11 +25:15:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.926 2035708842111647744 286.79955981868 +25.25579168613 13.2436 12.3814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254770_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254770_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:06:20.21 +20:40:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254777_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254777_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:55:44.67 +25:42:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.312 4534692583562568320 283.93614030715 +25.70669761258 13.6007 12.9591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254780_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254780_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:28:19.76 +24:59:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254787_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254787_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:37:55.72 +18:36:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254789_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254789_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:18:13.57 +24:26:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254790_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254790_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:54:41.93 +23:50:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.836 4533372551136275584 283.67546908877 +23.84626959248 13.8424 13.0502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254792_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254792_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:01.52 +21:02:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254793_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254793_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:05:02.34 +20:37:09.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254795_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254795_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:03:21.23 +23:38:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254796_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254796_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:01:57.36 +19:09:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254798_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254798_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:20:56.54 +23:03:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254800_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254800_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:54:46.74 +23:08:34.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254801_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254801_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:34:36.44 +23:54:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254802_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254802_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:37:50.14 +22:48:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254803_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254803_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254805_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254805_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:34:29.85 +19:47:40.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254813_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254813_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:58:34.50 +22:23:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254817_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254817_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:09:50.57 +26:00:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.387 2035854119398349696 287.46056690203 +26.00366936659 13.6883 11.8609 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254818_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254818_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:01:17.43 +21:29:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254820_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254820_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:53:05.70 +24:32:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.763 4534172617639516032 283.27331440865 +24.53439822444 13.7141 12.9647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254821_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254821_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:58:02.30 +22:29:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254823_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254823_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:58:13.74 +25:22:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254828_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254828_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:36:27.97 +21:59:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254829_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254829_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:40:17.75 +18:24:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254836_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254836_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:06:23.73 +21:24:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254840_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254840_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:44:52.00 +20:31:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254843_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254843_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:39:43.51 +24:31:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254845_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 254845_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 254850_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254850_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:41:27.78 +21:04:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254877_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254877_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:38:07.01 +23:23:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.066 2020252908408934784 294.52972199965 +23.39820913585 13.9419 12.2357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254893_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254893_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:55:56.92 +18:08:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254904_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254904_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:57:26.43 +23:10:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254905_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 254905_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:22:18.09 +22:30:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.648 2019236955337605760 290.57530307910 +22.50609177979 13.2154 11.1480 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 246135_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 246135_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:25:31.08 +21:10:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192271_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 192271_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 238500_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 238500_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 67272_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 67272_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 84895_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 84895_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:35:01.26 +20:55:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61230_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 61230_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:34:27.08 +19:45:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.485 1825528295291049344 293.61269030610 +19.75031014002 11.7413 10.1710 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121912_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 121912_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:45:37.42 +22:51:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143051_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 143051_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:32:37.28 +23:50:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233830_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 233830_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:48.38 +24:46:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53661_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 53661_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 183949_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 183949_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 92689_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 92689_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 94148_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 94148_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:38:24.28 +21:23:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136507_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 136507_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 235508_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 235508_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:08.22 +25:39:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 5.813 2026926050621345408 297.28554572135 +25.66753179348 11.6492 10.6905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 252809_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 252809_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:19:47.22 +22:48:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.562 2022182620037258496 289.94655180786 +22.80613230777 13.6766 11.8326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57952_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 57952_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 30752_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:05:00.94 +18:02:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96267_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 96267_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 88716_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 88716_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:45:29.41 +21:08:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109583_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 109583_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 235195_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 235195_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 80439_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 80439_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 29436_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 29436_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 35095_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 35095_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 78573_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 78573_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:15.08 +20:36:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45264_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 45264_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 50626_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 50626_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 71341_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 71341_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:04.61 +20:14:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136123_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 136123_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:10:13.63 +23:20:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21856_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 21856_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 154477_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 154477_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:30:08.03 +24:22:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155543_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 155543_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 177832_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:02:34.30 +25:50:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234337_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 234337_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:46:16.30 +20:22:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234184_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 234184_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:54:32.15 +19:01:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233990_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 233990_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 32268_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 32268_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:57:40.17 +18:01:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150311_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 150311_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:58.58 +24:09:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 52335_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:27:53.56 +19:17:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95637_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 95637_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:44:27.32 +21:30:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233822_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 233822_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:20:12.41 +26:01:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.730 2024043470421500800 290.05179391795 +26.03014322777 11.3856 9.8922 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50420_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 50420_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:58:54.89 +18:54:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92079_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 92079_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:18:39.52 +21:12:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101939_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 101939_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:17.31 +21:50:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69433_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 69433_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 136213_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 136213_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 170393_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 170393_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 233157_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 233157_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 78391_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 78391_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:45:50.70 +20:34:06.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 45496_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 45496_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 109502_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 109502_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 33243_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 33243_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:40:48.29 +18:25:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36436_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 36436_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 20613_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 20613_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 21011_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 21011_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:06:01.04 +17:34:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 110128_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:58:11.60 +21:52:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45827_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 45827_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:41:53.62 +19:01:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148949_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 148949_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:41:30.60 +24:07:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136378_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 136378_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 116825_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 116825_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 131093_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 131093_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 40590_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 40590_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 73259_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 73259_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:04.93 +20:20:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112797_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 112797_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:35:41.31 +22:20:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114725_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 114725_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 68990_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 68990_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:42:35.13 +20:07:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151575_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 151575_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 82826_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 82826_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 175957_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 175957_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 82475_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 82475_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:12:25.19 +20:39:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128412_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 128412_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 70013_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 70013_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:26:09.25 +20:07:41.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74440_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 74440_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:25.90 +20:23:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31767_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31767_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 76961_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 76961_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:42:13.46 +20:28:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85013_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 85013_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 38764_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 38764_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:32:51.85 +18:40:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192502_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 192502_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 182417_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 182417_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:28:47.23 +25:53:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135961_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 135961_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 86251_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 86251_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:12.17 +20:58:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58930_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 58930_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 39707_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 39707_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 23513_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 23513_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:23:20.46 +17:49:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69848_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 69848_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:57:26.98 +19:48:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109104_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 109104_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 139423_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 139423_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 80776_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 80776_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:16.62 +20:42:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69096_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 69096_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:33.76 +20:08:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240013_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 240013_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:35:26.65 +18:48:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116320_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 116320_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 64063_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 64063_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:36:19.69 +19:53:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25825_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 25825_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:40:27.90 +18:04:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58717_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 58717_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 38720_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 38720_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 96543_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 96543_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:24:48.02 +21:28:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146608_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 146608_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 140690_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:39:20.30 +23:44:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32774_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 32774_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 18:56:51.27 +18:01:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90334_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 90334_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:28:55.17 +21:11:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93934_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 93934_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:29:30.08 +21:22:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24448_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 24448_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:38:55.12 +17:59:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71876_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 71876_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26860_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 26860_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:37:38.76 +18:06:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71055_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 71055_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:46:27.32 +20:13:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 147350_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 147350_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26083_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 26083_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:33:24.03 +18:01:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178253_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 178253_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:18:33.34 +25:59:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37369_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 37369_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39197_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 39197_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143043_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 143043_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96854_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 96854_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:48:41.70 +21:33:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29846_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 29846_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174572_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 174572_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:25:20.45 +26:12:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103744_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 103744_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80706_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 80706_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80490_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 80490_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:31:53.94 +20:40:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70074_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 70074_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:03.84 +20:10:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61578_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 61578_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:11:18.01 +19:35:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163069_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 163069_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:37:02.19 +24:45:07.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71451_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 71451_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:47:32.48 +20:15:12.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82945_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 82945_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:49:05.27 +20:49:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65361_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 65361_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31149_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 31149_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:13:30.44 +18:09:35.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120276_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 120276_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:43:33.67 +22:44:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87838_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
Preparing report for the candidate 87838_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59216_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283
The candidate 59216_fd_Vul-01-Q2b1x1_2026-04-06_02-54-41_20.00sec_-5.00C_LIGHT_0283 did not pass the final checks
**** FOUND 19:32:25.28 +19:38:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.710 1825476893118409344 293.10573051239 +19.64837463496 12.1265 10.5677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 79s
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:45:50.76 +20:34:05.5
19:43:47.28 +21:55:23.0
19:49:04.60 +22:11:25.4
19:45:57.31 +22:12:09.3
19:48:49.60 +22:10:12.0
19:44:36.12 +22:28:49.9
19:46:49.49 +22:33:10.7
19:27:58.67 +22:33:19.5
19:22:00.90 +23:06:22.3
19:33:34.63 +23:16:56.5
19:31:10.20 +23:30:30.7
19:48:27.54 +23:31:56.0
19:25:54.47 +23:30:29.5
19:14:12.46 +23:33:27.9
19:47:24.24 +23:50:30.1
19:30:17.92 +24:00:17.3
19:35:18.02 +24:03:34.1
19:21:47.46 +24:11:02.6
19:38:42.14 +24:24:59.7
19:19:04.21 +25:00:32.7
19:32:35.69 +26:12:08.0
19:40:51.24 +25:50:07.3
19:20:12.71 +25:23:09.8
19:44:00.25 +25:27:04.0
19:20:44.16 +17:42:56.0
19:31:30.74 +17:49:29.5
19:05:50.69 +22:53:26.9
19:33:40.37 +25:50:37.0
19:47:17.58 +20:18:05.5
19:36:17.24 +17:51:53.6
19:25:55.23 +25:50:03.0
19:05:24.13 +20:38:26.4
19:31:49.88 +22:57:26.7
19:49:26.15 +23:31:12.0
19:44:41.31 +25:16:56.1
19:49:02.02 +20:28:13.8
19:48:21.76 +22:07:17.7
19:49:04.05 +21:45:43.3
19:48:15.90 +20:43:01.6
19:10:46.73 +19:57:11.4
19:48:52.85 +20:07:11.8
19:35:38.29 +18:13:39.5
19:09:56.41 +18:00:07.6
19:33:07.99 +18:29:29.0
19:01:23.59 +18:16:16.6
19:14:45.81 +18:28:50.5
19:08:08.29 +18:28:27.1
18:59:04.83 +18:18:51.6
19:29:41.12 +18:42:10.7
19:33:22.34 +18:58:39.0
19:16:57.10 +18:52:07.5
19:22:35.18 +19:10:42.0
19:14:41.72 +19:15:00.4
19:17:18.88 +19:29:05.2
19:08:06.43 +19:25:17.0
19:23:49.64 +19:34:58.8
19:17:44.19 +19:50:02.8
19:27:16.68 +20:00:05.7
19:42:29.27 +20:09:06.9
19:37:36.53 +20:15:55.7
19:46:42.85 +20:42:27.6
19:44:53.81 +20:42:29.3
19:40:12.37 +20:45:01.8
19:17:13.65 +20:48:41.6
19:47:13.46 +21:05:38.3
19:41:53.39 +21:20:13.4
19:49:23.25 +21:31:30.5
########### Completed Vul-01-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 ####
19:45:50.76 +20:34:05.5
19:25:55.23 +25:50:03.0
19:05:24.13 +20:38:26.4
19:31:49.88 +22:57:26.7
19:49:26.15 +23:31:12.0
19:44:41.31 +25:16:56.1
19:49:02.02 +20:28:13.8
19:48:21.76 +22:07:17.7
19:49:04.05 +21:45:43.3
19:48:15.90 +20:43:01.6
19:10:46.73 +19:57:11.4
19:48:52.85 +20:07:11.8
19:20:12.71 +25:23:09.8
19:36:17.24 +17:51:53.6
19:27:16.68 +20:00:05.7
19:14:41.72 +19:15:00.4
19:40:51.24 +25:50:07.3
19:41:53.39 +21:20:13.4
19:25:54.47 +23:30:29.5
19:17:18.88 +19:29:05.2
19:49:23.25 +21:31:30.5
19:48:49.60 +22:10:12.0
19:47:17.58 +20:18:05.5
19:46:42.85 +20:42:27.6
19:35:38.29 +18:13:39.5
19:33:07.99 +18:29:29.0
19:33:22.34 +18:58:39.0
19:22:35.18 +19:10:42.0
19:31:30.74 +17:49:29.5
19:38:42.14 +24:24:59.7
19:33:40.37 +25:50:37.0
19:42:29.27 +20:09:06.9
19:19:04.21 +25:00:32.7
19:05:50.69 +22:53:26.9
19:16:57.10 +18:52:07.5
19:45:57.31 +22:12:09.3
19:01:23.59 +18:16:16.6
19:20:44.16 +17:42:56.0
19:48:27.54 +23:31:56.0
19:27:58.67 +22:33:19.5
19:33:34.63 +23:16:56.5
19:44:36.12 +22:28:49.9
19:21:47.46 +24:11:02.6
19:40:12.37 +20:45:01.8
19:32:35.69 +26:12:08.0
19:22:00.90 +23:06:22.3
19:17:13.65 +20:48:41.6
19:44:00.25 +25:27:04.0
19:31:10.20 +23:30:30.7
19:23:49.64 +19:34:58.8
19:29:41.12 +18:42:10.7
19:49:04.60 +22:11:25.4
19:14:12.46 +23:33:27.9
19:46:49.49 +22:33:10.7
19:08:06.43 +19:25:17.0
19:08:08.29 +18:28:27.1
19:30:17.92 +24:00:17.3
19:37:36.53 +20:15:55.7
19:35:18.02 +24:03:34.1
19:14:45.81 +18:28:50.5
18:59:04.83 +18:18:51.6
19:47:24.24 +23:50:30.1
19:09:56.41 +18:00:07.6
19:43:47.28 +21:55:23.0
19:44:53.81 +20:42:29.3
19:17:44.19 +19:50:02.8
19:47:13.46 +21:05:38.3
###################################################################################
19:45:50.76 +20:34:05.5 -- not an asteroid (will add it to exclusion list)
19:25:55.23 +25:50:03.0 -- not an asteroid (will add it to exclusion list)
19:05:24.13 +20:38:26.4 -- not an asteroid (will add it to exclusion list)
19:31:49.88 +22:57:26.7 -- not an asteroid (will add it to exclusion list)
19:49:26.15 +23:31:12.0 -- not an asteroid (will add it to exclusion list)
19:44:41.31 +25:16:56.1 -- not an asteroid (will add it to exclusion list)
19:49:02.02 +20:28:13.8 -- not an asteroid (will add it to exclusion list)
19:48:21.76 +22:07:17.7 -- not an asteroid (will add it to exclusion list)
19:49:04.05 +21:45:43.3 -- not an asteroid (will add it to exclusion list)
19:48:15.90 +20:43:01.6 -- not an asteroid (will add it to exclusion list)
19:10:46.73 +19:57:11.4 -- not an asteroid (will add it to exclusion list)
19:48:52.85 +20:07:11.8 -- not an asteroid (will add it to exclusion list)
19:20:12.71 +25:23:09.8 -- not an asteroid (will add it to exclusion list)
19:36:17.24 +17:51:53.6 -- not an asteroid (will add it to exclusion list)
19:27:16.68 +20:00:05.7 -- not an asteroid (will add it to exclusion list)
19:14:41.72 +19:15:00.4 -- not an asteroid (will add it to exclusion list)
19:40:51.24 +25:50:07.3 -- not an asteroid (will add it to exclusion list)
19:41:53.39 +21:20:13.4 -- not an asteroid (will add it to exclusion list)
19:25:54.47 +23:30:29.5 -- not an asteroid (will add it to exclusion list)
19:17:18.88 +19:29:05.2 -- not an asteroid (will add it to exclusion list)
19:49:23.25 +21:31:30.5 -- not an asteroid (will add it to exclusion list)
19:48:49.60 +22:10:12.0 -- not an asteroid (will add it to exclusion list)
19:47:17.58 +20:18:05.5 -- not an asteroid (will add it to exclusion list)
19:46:42.85 +20:42:27.6 -- not an asteroid (will add it to exclusion list)
19:35:38.29 +18:13:39.5 -- not an asteroid (will add it to exclusion list)
19:33:07.99 +18:29:29.0 -- not an asteroid (will add it to exclusion list)
19:33:22.34 +18:58:39.0 -- not an asteroid (will add it to exclusion list)
19:22:35.18 +19:10:42.0 -- not an asteroid (will add it to exclusion list)
19:31:30.74 +17:49:29.5 -- not an asteroid (will add it to exclusion list)
19:38:42.14 +24:24:59.7 -- not an asteroid (will add it to exclusion list)
19:33:40.37 +25:50:37.0 -- not an asteroid (will add it to exclusion list)
19:42:29.27 +20:09:06.9 -- not an asteroid (will add it to exclusion list)
19:19:04.21 +25:00:32.7 -- not an asteroid (will add it to exclusion list)
19:05:50.69 +22:53:26.9 -- not an asteroid (will add it to exclusion list)
19:16:57.10 +18:52:07.5 -- not an asteroid (will add it to exclusion list)
19:45:57.31 +22:12:09.3 -- not an asteroid (will add it to exclusion list)
19:01:23.59 +18:16:16.6 -- not an asteroid (will add it to exclusion list)
19:20:44.16 +17:42:56.0 -- not an asteroid (will add it to exclusion list)
19:48:27.54 +23:31:56.0 -- not an asteroid (will add it to exclusion list)
19:27:58.67 +22:33:19.5 -- not an asteroid (will add it to exclusion list)
19:33:34.63 +23:16:56.5 -- not an asteroid (will add it to exclusion list)
19:44:36.12 +22:28:49.9 -- not an asteroid (will add it to exclusion list)
19:21:47.46 +24:11:02.6 -- not an asteroid (will add it to exclusion list)
19:40:12.37 +20:45:01.8 -- not an asteroid (will add it to exclusion list)
19:32:35.69 +26:12:08.0 -- not an asteroid (will add it to exclusion list)
19:22:00.90 +23:06:22.3 -- not an asteroid (will add it to exclusion list)
19:17:13.65 +20:48:41.6 -- not an asteroid (will add it to exclusion list)
19:44:00.25 +25:27:04.0 -- not an asteroid (will add it to exclusion list)
19:31:10.20 +23:30:30.7 -- not an asteroid (will add it to exclusion list)
19:23:49.64 +19:34:58.8 -- not an asteroid (will add it to exclusion list)
19:29:41.12 +18:42:10.7 -- not an asteroid (will add it to exclusion list)
19:49:04.60 +22:11:25.4 -- not an asteroid (will add it to exclusion list)
19:14:12.46 +23:33:27.9 -- not an asteroid (will add it to exclusion list)
19:46:49.49 +22:33:10.7 -- not an asteroid (will add it to exclusion list)
19:08:06.43 +19:25:17.0 -- not an asteroid (will add it to exclusion list)
19:08:08.29 +18:28:27.1 -- not an asteroid (will add it to exclusion list)
19:30:17.92 +24:00:17.3 -- not an asteroid (will add it to exclusion list)
19:37:36.53 +20:15:55.7 -- not an asteroid (will add it to exclusion list)
19:35:18.02 +24:03:34.1 -- not an asteroid (will add it to exclusion list)
19:14:45.81 +18:28:50.5 -- not an asteroid (will add it to exclusion list)
18:59:04.83 +18:18:51.6 -- not an asteroid (will add it to exclusion list)
19:47:24.24 +23:50:30.1 -- not an asteroid (will add it to exclusion list)
19:09:56.41 +18:00:07.6 -- not an asteroid (will add it to exclusion list)
19:43:47.28 +21:55:23.0 -- not an asteroid (will add it to exclusion list)
19:44:53.81 +20:42:29.3 -- not an asteroid (will add it to exclusion list)
19:17:44.19 +19:50:02.8 -- not an asteroid (will add it to exclusion list)
19:47:13.46 +21:05:38.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:59:04.83 +18:18:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:23.59 +18:16:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:24.13 +20:38:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:50.69 +22:53:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:06.43 +19:25:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:08.29 +18:28:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:56.41 +18:00:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:46.73 +19:57:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:12.46 +23:33:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:41.72 +19:15:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:45.81 +18:28:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:57.10 +18:52:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:13.65 +20:48:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:18.88 +19:29:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:44.19 +19:50:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:04.21 +25:00:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:12.71 +25:23:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:44.16 +17:42:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:47.46 +24:11:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:00.90 +23:06:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:35.18 +19:10:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:49.64 +19:34:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:54.47 +23:30:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:55.23 +25:50:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:16.68 +20:00:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:58.67 +22:33:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:41.12 +18:42:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:17.92 +24:00:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:10.20 +23:30:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:30.74 +17:49:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:49.88 +22:57:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:35.69 +26:12:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:07.99 +18:29:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:22.34 +18:58:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:34.63 +23:16:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:40.37 +25:50:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:18.02 +24:03:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:38.29 +18:13:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:17.24 +17:51:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:36.53 +20:15:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:42.14 +24:24:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:12.37 +20:45:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:51.24 +25:50:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:53.39 +21:20:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:29.27 +20:09:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:47.28 +21:55:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:00.25 +25:27:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:36.12 +22:28:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:41.31 +25:16:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:53.81 +20:42:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:50.76 +20:34:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:57.31 +22:12:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:42.85 +20:42:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:49.49 +22:33:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:13.46 +21:05:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:17.58 +20:18:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:24.24 +23:50:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:15.90 +20:43:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:21.76 +22:07:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:27.54 +23:31:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:49.60 +22:10:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:52.85 +20:07:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:02.02 +20:28:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:04.05 +21:45:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:04.60 +22:11:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:23.25 +21:31:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:26.15 +23:31:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
18:59:04.83 +18:18:51.6 -- a known variable star
19:01:23.59 +18:16:16.6 -- a known variable star
19:05:24.13 +20:38:26.4 -- not a known variable star
19:05:50.69 +22:53:26.9 -- not a known variable star
19:08:06.43 +19:25:17.0 -- a known variable star
19:08:08.29 +18:28:27.1 -- a known variable star
19:09:56.41 +18:00:07.6 -- a known variable star
19:10:46.73 +19:57:11.4 -- a known variable star
19:14:12.46 +23:33:27.9 -- a known variable star
19:14:41.72 +19:15:00.4 -- a known variable star
19:14:45.81 +18:28:50.5 -- not a known variable star
19:16:57.10 +18:52:07.5 -- a known variable star
19:17:13.65 +20:48:41.6 -- a known variable star
19:17:18.88 +19:29:05.2 -- a known variable star
19:17:44.19 +19:50:02.8 -- a known variable star
19:19:04.21 +25:00:32.7 -- a known variable star
19:20:12.71 +25:23:09.8 -- not a known variable star
19:20:44.16 +17:42:56.0 -- a known variable star
19:21:47.46 +24:11:02.6 -- a known variable star
19:22:00.90 +23:06:22.3 -- a known variable star
19:22:35.18 +19:10:42.0 -- a known variable star
19:23:49.64 +19:34:58.8 -- a known variable star
19:25:54.47 +23:30:29.5 -- a known variable star
19:25:55.23 +25:50:03.0 -- not a known variable star
19:27:16.68 +20:00:05.7 -- a known variable star
19:27:58.67 +22:33:19.5 -- a known variable star
19:29:41.12 +18:42:10.7 -- a known variable star
19:30:17.92 +24:00:17.3 -- a known variable star
19:31:10.20 +23:30:30.7 -- a known variable star
19:31:30.74 +17:49:29.5 -- a known variable star
19:31:49.88 +22:57:26.7 -- a known variable star
19:32:35.69 +26:12:08.0 -- a known variable star
19:33:07.99 +18:29:29.0 -- a known variable star
19:33:22.34 +18:58:39.0 -- a known variable star
19:33:34.63 +23:16:56.5 -- a known variable star
19:33:40.37 +25:50:37.0 -- a known variable star
19:35:18.02 +24:03:34.1 -- a known variable star
19:35:38.29 +18:13:39.5 -- a known variable star
19:36:17.24 +17:51:53.6 -- a known variable star
19:37:36.53 +20:15:55.7 -- a known variable star
19:38:42.14 +24:24:59.7 -- a known variable star
19:40:12.37 +20:45:01.8 -- a known variable star
19:40:51.24 +25:50:07.3 -- a known variable star
19:41:53.39 +21:20:13.4 -- a known variable star
19:42:29.27 +20:09:06.9 -- not a known variable star
19:43:47.28 +21:55:23.0 -- a known variable star
19:44:00.25 +25:27:04.0 -- not a known variable star
19:44:36.12 +22:28:49.9 -- a known variable star
19:44:41.31 +25:16:56.1 -- not a known variable star
19:44:53.81 +20:42:29.3 -- a known variable star
19:45:50.76 +20:34:05.5 -- a known variable star
19:45:57.31 +22:12:09.3 -- a known variable star
19:46:42.85 +20:42:27.6 -- a known variable star
19:46:49.49 +22:33:10.7 -- a known variable star
19:47:13.46 +21:05:38.3 -- a known variable star
19:47:17.58 +20:18:05.5 -- a known variable star
19:47:24.24 +23:50:30.1 -- a known variable star
19:48:15.90 +20:43:01.6 -- a known variable star
19:48:21.76 +22:07:17.7 -- not a known variable star
19:48:27.54 +23:31:56.0 -- a known variable star
19:48:49.60 +22:10:12.0 -- a known variable star
19:48:52.85 +20:07:11.8 -- a known variable star
19:49:02.02 +20:28:13.8 -- not a known variable star
19:49:04.05 +21:45:43.3 -- not a known variable star
19:49:04.60 +22:11:25.4 -- not a known variable star
19:49:23.25 +21:31:30.5 -- a known variable star
19:49:26.15 +23:31:12.0 -- not a known variable star
Found 13 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
67 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 67 (excluding asteroids and hot pixels, 13 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.82918583 -observatory V36
23:20:59.63 -06:22:49.7 Mercury (0.3mag)
02:22:08.69 +13:54:36.0 Venus (-3.9mag)
23:50:17.87 -02:10:02.8 Mars (1.2mag)
07:08:45.01 +22:52:22.1 Jupiter (-2.2mag)
00:24:49.40 +00:21:36.8 Saturn (0.9mag)
03:45:44.91 +19:41:10.6 Uranus (5.8mag)
00:09:32.89 -00:23:33.3 Neptune (7.8mag)
20:33:14.68 -22:52:29.2 Pluto (14.5mag)
16:04:42.77 -26:41:03.1 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 6 02:59 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461136.82918583:
07:08:45.23 +22:52:18.7 Io (5.7mag)
07:08:56.94 +22:51:56.4 Europa (5.8mag)
07:08:41.78 +22:52:35.8 Ganymede (5.3mag)
07:08:14.37 +22:53:15.8 Callisto (6.5mag)
07:12:27.70 +22:44:47.9 Himalia (15.3mag)
07:08:47.13 +22:52:19.8 Thebe (16.2mag)
07:12:25.59 +23:13:35.8 Elara (17.2mag)
07:06:58.40 +23:37:26.2 Pasiphae (17.3mag)
07:17:16.68 +22:49:19.2 Carme (18.4mag)
00:24:44.54 +00:21:37.1 Titan (8.8mag)
00:24:46.07 +00:21:50.0 Rhea (10.1mag)
00:24:49.67 +00:23:09.4 Iapetus (11.5mag)
00:24:51.67 +00:21:24.8 Hyperion (14.8mag)
00:26:33.54 +00:31:25.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 02:59 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.82918583:
14:47:33.17 -08:27:38.9 JWST
17:13:16.05 +43:55:11.2 Chandra
08:24:48.83 -45:39:15.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 02:59 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.82918583 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:12.38 -28:14:34.3 13.9mag P/2010 H2 (Vales)
05:00:10.40 -70:08:26.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:35.52 +31:22:36.1 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.69 +09:23:12.6 17.6mag C/2021 G2 (ATLAS)
23:07:23.81 +28:52:21.8 17.0mag C/2022 E2 (ATLAS)
04:18:08.86 +25:46:05.3 15.9mag C/2022 N2 (PANSTARRS)
09:01:52.71 +31:54:31.8 16.1mag C/2022 QE78 (ATLAS)
08:29:59.69 -01:13:01.0 17.3mag C/2022 R6 (PANSTARRS)
18:55:34.21 +17:42:24.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:28.56 -11:39:31.3 17.6mag P/2023 B1 (PANSTARRS)
09:12:45.20 -13:28:47.2 17.5mag C/2023 F3 (ATLAS)
21:43:38.46 +62:22:41.9 17.5mag C/2023 H5 (Lemmon)
19:26:19.70 -03:36:35.3 14.3mag C/2023 R1 (PANSTARRS)
21:42:37.14 +84:37:41.7 17.8mag C/2023 X2 (Lemmon)
06:14:33.48 +63:34:55.6 17.0mag C/2024 A1 (ATLAS)
04:51:23.83 +14:36:57.6 10.4mag C/2024 E1 (Wierzchos)
16:25:01.68 +04:48:01.5 17.4mag C/2024 G6 (ATLAS)
20:17:36.15 +12:43:07.9 14.7mag C/2024 J3 (ATLAS)
03:17:53.08 -23:54:02.3 16.4mag C/2024 T5 (ATLAS)
05:08:48.73 +47:47:49.6 17.7mag C/2025 J1 (Borisov)
14:18:33.13 +37:31:49.0 14.8mag C/2025 L1 (ATLAS)
03:10:34.21 -24:46:06.3 17.8mag C/2025 Q3 (ATLAS)
22:53:56.40 +19:50:14.9 10.1mag C/2025 R3 (PANSTARRS)
12:58:19.85 +02:24:04.3 17.5mag C/2025 Y1 (ATLAS)
01:33:33.74 +04:39:13.7 7.4mag C/2026 A1 (MAPS)
23:31:13.67 +35:16:27.6 14.3mag C/2026 B2 (Sun-Gao)
18:24:03.61 -10:12:43.4 12.4mag 10P/Tempel
15:12:44.10 +04:06:04.3 13.1mag 24P/Schaumasse
11:05:43.41 -01:51:31.6 15.7mag 29P/Schwassmann-Wachmann
17:56:50.43 -09:59:15.1 17.7mag 40P/Vaisala
10:38:50.98 -04:56:07.0 16.7mag 43P/Wolf-Harrington
01:33:45.91 +15:49:12.3 17.1mag 47P/Ashbrook-Jackson
06:53:33.89 +39:03:06.9 17.0mag 63P/Wild
23:16:29.55 -12:38:16.0 15.7mag 65P/Gunn
03:38:01.70 +17:47:21.1 15.8mag 76P/West-Kohoutek-Ikemura
00:44:22.81 +06:18:45.5 14.4mag 78P/Gehrels
22:32:59.38 -12:13:53.8 14.5mag 88P/Howell
01:43:32.86 +17:59:10.7 15.1mag 93P/Lovas
04:37:10.10 +31:44:11.1 16.3mag 123P/West-Hartley
08:18:03.44 +42:49:36.2 16.2mag 124P/Mrkos
02:18:25.61 +13:16:22.2 16.4mag 128P/Shoemaker-Holt
02:28:40.01 +13:16:18.1 17.5mag 131P/Mueller
00:36:34.24 +09:39:49.8 11.2mag 141P/Machholz
00:46:32.12 +01:15:03.4 11.3mag 141P-A/Machholz
23:37:01.40 -02:22:47.5 14.0mag 141P-D/Machholz
01:15:40.73 +02:55:04.5 17.9mag 141P-I/Machholz
00:35:31.25 -06:20:59.8 15.2mag 162P/SidingSpring
10:30:55.75 +31:29:53.3 17.8mag 164P/Christensen
06:18:40.88 +24:31:10.8 17.8mag 198P/ODAS
15:08:27.69 -01:10:42.0 17.4mag 210P/Christensen
21:09:21.70 -13:47:18.2 17.4mag 218P/LINEAR
17:12:40.80 -15:03:28.9 16.2mag 235P/LINEAR
05:13:56.80 +33:52:08.6 16.6mag 240P/NEAT
07:34:15.15 -06:16:13.4 17.6mag 242P/Spahr
15:45:53.98 +06:19:09.3 17.5mag 391P/Kowalski
07:30:57.37 +21:18:45.6 17.6mag 450P/LONEOS
05:22:06.45 +45:36:10.3 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 02:59 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 6 02:59 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 6 02:59 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
14:19:10.599 -33:29:33.62 AT 2026huk 2026-03-29.24 19.7
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
-rw-r--r-- 1 apache apache 30K Apr 6 02:59 tns_transients_list.txt
