This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9
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
ZTF J193050.78+234016.2,2461138.8262,13.36,0.05,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 J193050.78+234016.2 20260408.3262 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461138.8262,13.15,0.05,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 20260408.3262 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1824073400887983104,2461138.8262,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1824073400887983104 20260408.3262 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1827719072206609536,2461138.8262,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1827719072206609536 20260408.3262 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193940.04+245200.4,2461138.8262,13.44,0.05,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
ASASSN-V J193940.04+245200.4 20260408.3262 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
NSVS 11255525,2461138.8262,12.36,0.05,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 11255525 20260408.3262 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+1800.2,2461138.8262,10.77,0.05,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 20260408.3262 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
ASASSN-V J190806.32+192518.2,2461138.8262,13.20,0.05,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 20260408.3262 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4515919796930120192,2461138.8262,13.20,0.05,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 4515919796930120192 20260408.3262 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 11222340,2461138.8262,13.28,0.05,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 11222340 20260408.3262 13.28CV 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
ASASSN-V J193642.64+240712.3,2461138.8262,12.67,0.05,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 J193642.64+240712.3 20260408.3262 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192109.89+194840.2,2461138.8262,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192109.89+194840.2 20260408.3262 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193736.61+201556.3,2461138.8262,12.92,0.05,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 J193736.61+201556.3 20260408.3262 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!
TCP 2026 04 08.3262* 18 54 11.01 +21 29 22.7 13.3 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185410.76+212922.4,2461138.8262,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185410.76+212922.4 20260408.3262 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J191714+2048.6,2461138.8262,12.35,0.05,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
ASAS J191714+2048.6 20260408.3262 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
NSVS 11248753,2461138.8262,12.17,0.05,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
NSVS 11248753 20260408.3262 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
NSVS J1914126+233323,2461138.8262,13.39,0.05,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 J1914126+233323 20260408.3262 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
ZTF J191002.68+200641.2,2461138.8262,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J191002.68+200641.2 20260408.3262 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1916569+185207,2461138.8262,12.28,0.05,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 J1916569+185207 20260408.3262 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 J1919040+250038,2461138.8262,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1919040+250038 20260408.3262 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8367053,2461138.8262,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8367053 20260408.3262 12.19CV 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
NSVS J1938420+242505,2461138.8262,11.59,0.05,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 20260408.3262 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J194042.70+221030.5,2461138.8262,13.36,0.05,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 J194042.70+221030.5 20260408.3262 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+174927,2461138.8262,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1931308+174927 20260408.3262 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IRAS 19397+2234,2461138.8262,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IRAS 19397+2234 20260408.3262 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11254924,2461138.8262,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11254924 20260408.3262 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192222.05+222801.3,2461138.8262,13.43,0.05,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 J192222.05+222801.3 20260408.3262 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+240339.3,2461138.8262,12.94,0.05,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 20260408.3262 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J192055.89+184728.7,2461138.8262,13.32,0.05,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 J192055.89+184728.7 20260408.3262 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
NSVS J1917440+195001,2461138.8262,12.32,0.05,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
NSVS J1917440+195001 20260408.3262 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
ASASSN-V J192909.90+210954.1,2461138.8262,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192909.90+210954.1 20260408.3262 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11259789,2461138.8262,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11259789 20260408.3262 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.6957+18.4797,2461138.8262,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J288.6957+18.4797 20260408.3262 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191441.69+191500.2,2461138.8262,13.20,0.05,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 20260408.3262 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+191042,2461138.8262,13.30,0.05,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 J1922349+191042 20260408.3262 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
NSVS 11213314,2461138.8262,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11213314 20260408.3262 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192555+2330.6,2461138.8262,12.60,0.05,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
ASAS J192555+2330.6 20260408.3262 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
NSVS 11249151,2461138.8262,13.02,0.05,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 20260408.3262 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 11252248,2461138.8262,12.54,0.05,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
NSVS 11252248 20260408.3262 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 J193308.12+182927.8,2461138.8262,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193308.12+182927.8 20260408.3262 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
ZTF J192044.14+174251.7,2461138.8262,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192044.14+174251.7 20260408.3262 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194051.39+255011.2,2461138.8262,13.14,0.05,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
ZTF J194051.39+255011.2 20260408.3262 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
Gaia DR3 4517794734810380800,2461138.8262,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4517794734810380800 20260408.3262 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1921463+241122,2461138.8262,12.52,0.05,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
NSVS J1921463+241122 20260408.3262 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 11259091,2461138.8262,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11259091 20260408.3262 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11243145,2461138.8262,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11243145 20260408.3262 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192026.83+235030.8,2461138.8262,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192026.83+235030.8 20260408.3262 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+223319.6,2461138.8262,13.37,0.05,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
ASASSN-V J192758.85+223319.6 20260408.3262 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
ASASSN-V J193550.28+231612.3,2461138.8262,13.02,0.05,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 J193550.28+231612.3 20260408.3262 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 11224206,2461138.8262,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11224206 20260408.3262 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191436.80+223939.9,2461138.8262,12.72,0.05,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 J191436.80+223939.9 20260408.3262 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193136.61+214503.6,2461138.8262,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193136.61+214503.6 20260408.3262 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191343.44+185207.7,2461138.8262,12.89,0.05,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 J191343.44+185207.7 20260408.3262 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 J193415.94+182027.2,2461138.8262,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193415.94+182027.2 20260408.3262 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0342 Vul,2461138.8262,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0342 Vul 20260408.3262 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.1717+24.2938,2461138.8262,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.1717+24.2938 20260408.3262 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11230768,2461138.8262,12.98,0.05,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 20260408.3262 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
NSVS J1941134+201548,2461138.8262,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1941134+201548 20260408.3262 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192716.44+200003.0,2461138.8262,12.91,0.05,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
ASASSN-V J192716.44+200003.0 20260408.3262 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
NSVS J1933344+260117,2461138.8262,12.36,0.05,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 J1933344+260117 20260408.3262 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J193251.22+213904.8,2461138.8262,13.49,0.05,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 J193251.22+213904.8 20260408.3262 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
ASAS J185904+1818.8,2461138.8262,10.63,0.05,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
ASAS J185904+1818.8 20260408.3262 10.63CV 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
## 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: 2461138.82654743 08.04.2026 07:50:03.698 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15555
Objects passed selection criteria: 15528
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 13860.5
Average stars matched: 13576.8 (97.9528 %)
Memory usage VmPeak: 122508 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 02:52:09 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: 2461138.82654743 08.04.2026 07:50:03.698 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 330
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: 67 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): 160323
Objects passed selection criteria: 159986
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 132416
Average stars matched: 126824 (95.7768 %)
Memory usage VmPeak: 2066276 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 02:55:34 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461138.82587536
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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits'
wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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 19:23:05.228 +21:59:41.78
Angular distance between the image centers 0.0020 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 19:23:03.109 +22:00:11.82
Angular distance between the image centers 0.0116 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 19:23:05.228 +21:59:41.78
Second-epoch second image center 19:23:03.109 +22:00:11.82
Angular distance between the image centers 0.01169 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.vbYBZ7hrvf
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.nixiikSrvT
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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits &> /tmp/tmp.vE98o1kcpQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits &> /tmp/tmp.SuMA96pxZb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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 7 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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
3.0 pix fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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
14.3 mag. fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
14.3 mag. fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.6 (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.vbYBZ7hrvf (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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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.nixiikSrvT (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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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.vE98o1kcpQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1051, passed=14023
Got 14023 stars (including 12967 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 14023 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 955 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(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 13956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
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(), 13958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
WARNING: Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 13958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.11"
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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.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.SuMA96pxZb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1110, passed=14010
Got 14010 stars (including 12894 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat
util/solve_plate_with_UCAC5 got 14010 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 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
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 13946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
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 16.5 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: 950 matched stars entering correct_measured_positions(), 13947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 13947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 31067_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 31067_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:53.07 +18:18:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31076_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 31076_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:05:00.98 +18:02:40.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31082_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 31082_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:00:53.72 +23:19:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03107_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 03107_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:33:24.03 +18:01:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21588_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 21588_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:02:34.27 +25:50:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10446_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 10446_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:38:24.27 +21:23:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12393_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 12393_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:35:41.29 +22:20:05.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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 ####
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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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 19:23:05.228 +21:59:41.78
Angular distance between the image centers 0.0020 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 19:23:03.109 +22:00:11.82
Angular distance between the image centers 0.0116 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 19:23:05.228 +21:59:41.78
Second-epoch second image center 19:23:03.109 +22:00:11.82
Angular distance between the image centers 0.01169 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.DXQHv5GUxC
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.KyFv1OtXjz
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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits &> /tmp/tmp.L279ERZtLY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits &> /tmp/tmp.wO7WdeGYKr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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 214 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
2.8 pix fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
2.7 pix fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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
14.3 mag. fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
14.3 mag. fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (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.DXQHv5GUxC (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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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.KyFv1OtXjz (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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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.L279ERZtLY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=11338, passed=100915
Got 100915 stars (including 89467 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 100915 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 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(), 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: 947 matched stars entering correct_measured_positions(), 100023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
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(), 100024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 100025 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.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.wO7WdeGYKr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=11889, passed=104315
Got 104315 stars (including 92283 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat
util/solve_plate_with_UCAC5 got 104315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 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(), 939 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(), 103377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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: 948 matched stars entering correct_measured_positions(), 103378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
WARNING: Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 103379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
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_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits -region wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/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_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-49-05_20.00sec_-5.00C_LIGHT_0148.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Vul-01-Q2b1x1_025050_TTUQ2b1x1_30838_8Nr2g4l9/wcs_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out130977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out174877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out233120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out233752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out253547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out42876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out43872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out96088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out253283.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out100525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130649.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__out144307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152156.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__out179701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183949.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__out253231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out253500.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__out31767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37369.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__out40590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42720.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__out45937.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__out55675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56514.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__out63989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81704.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__out89767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98496.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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: 25s
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Considering the candidate 253204_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253204_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:12:29.34 +24:30:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 4.655 2023567832870049280 288.12258269813 +24.50938177588 13.6448 12.8986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253214_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253214_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:38:05.34 +21:02:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.780 1826054037967124864 294.52351698407 +21.04714149247 13.0979 12.0565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253217_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253217_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 253218_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253218_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:17:25.92 +25:07:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253220_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253220_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:31:16.62 +23:52:31.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)
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Considering the candidate 253225_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253225_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:14:39.75 +19:07:39.2 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 253227_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253227_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:16:17.85 +25:22:49.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 253231_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 253231_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 253233_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253233_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:09:25.58 +25:54:34.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 253235_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253235_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:18:12.76 +22:49:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253239_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 253239_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 253246_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253246_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 253253_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253253_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:10:55.50 +24:02:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.214 2023337931864978944 287.73145055741 +24.04550521767 13.6157 12.9176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253258_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253258_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:05:54.72 +19:53:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.300 4519434214043174144 286.47764255988 +19.89588210551 12.3966 11.0935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253260_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253260_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:35:59.54 +18:46:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.917 1825140927928893312 293.99802222734 +18.76899693106 13.2098 12.6605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253262_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253262_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:55:38.70 +19:24:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.066 4518422835133148544 283.91103447268 +19.41691028798 13.5531 12.7468 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 253269_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 253269_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 253270_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253270_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:16:51.32 +23:34:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253273_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253273_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:37:13.48 +21:05:02.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 253283_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253283_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:42:07.22 +18:40:42.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 253284_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253284_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 253285_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253285_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:32.93 +18:45:22.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)
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Considering the candidate 253289_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 253289_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 253290_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253290_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:42:13.28 +23:15:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.066 2020093921570300416 295.55666091393 +23.25278519109 12.4155 11.4129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253294_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253294_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:37:07.56 +19:15:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.922 1825296641934754944 294.28255389933 +19.26361781438 12.3050 11.1163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253295_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253295_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:37:43.28 +24:48:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.047 2021254323008408448 294.42993941982 +24.81338644994 12.5306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253301_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253301_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:11:34.50 +25:01:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253303_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253303_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:52.77 +18:18:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253318_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253318_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:21:03.11 +20:02:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253322_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253322_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:54:38.14 +22:40:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253325_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253325_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:07:57.60 +21:42:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253338_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253338_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:01:01.30 +19:17:48.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253359_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253359_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:34.32 +18:29:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253360_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253360_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:25:27.11 +20:15:13.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253361_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253361_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:54:28.99 +20:20:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253363_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253363_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:36:25.41 +23:56:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253368_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253368_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:41:12.78 +18:08:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.421 1824098105545893504 295.30383991427 +18.14848958240 11.7449 10.3476 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 253369_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253369_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:09:08.71 +25:19:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253374_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253374_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:00:38.12 +18:27:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253375_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253375_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:25:28.79 +24:56:32.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253376_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253376_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:24:20.73 +20:00:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253385_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253385_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:08:11.77 +25:22:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253389_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253389_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:54:46.64 +23:08:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253390_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253390_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:10:46.75 +19:57:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253391_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253391_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:59:51.56 +22:49:01.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 253393_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253393_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:05:21.71 +23:45:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.406 4521455253845023744 286.33943079535 +23.75542542872 13.2619 12.2745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253394_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253394_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:56:37.11 +21:22:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253405_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253405_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:01:17.32 +21:29:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253406_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253406_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:03:21.25 +23:38:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253410_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253410_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:06:20.18 +20:40:16.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253412_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253412_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:41:02.08 +24:52:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253413_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253413_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:17.76 +18:24:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253415_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253415_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:28:19.51 +24:59:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253416_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253416_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:08:46.12 +24:10:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253418_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253418_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:16:17.07 +21:22:04.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253420_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253420_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:06:20.18 +21:22:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253422_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253422_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:37.98 +20:24:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253424_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253424_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:58:13.77 +25:22:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253428_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253428_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:01:19.72 +20:51:09.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253431_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253431_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:57:00.40 +24:07:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253433_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253433_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:09:50.59 +26:00:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253441_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253441_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:58:56.30 +18:15:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253446_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253446_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:06:23.77 +21:24:18.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253448_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253448_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:34:36.42 +23:54:07.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253451_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253451_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:01:57.41 +19:09:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253464_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253464_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:04:34.48 +22:06:42.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253466_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253466_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:36:27.88 +21:59:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253470_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253470_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:34:29.72 +19:47:39.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253473_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253473_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:23:52.35 +20:15:24.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253475_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253475_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:58:02.29 +22:30:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253481_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253481_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:43.68 +24:31:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253496_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253496_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:06:26.09 +22:42:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253500_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 253500_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253510_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253510_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:03:36.68 +24:39:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253515_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253515_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:39.96 +18:30:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253520_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253520_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:31:17.74 +18:50:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253522_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253522_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:38:06.90 +23:23:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253523_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253523_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:21:55.79 +20:12:10.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253525_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253525_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:34:49.68 +21:08:18.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253527_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253527_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:17:13.09 +18:52:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253534_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253534_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:38.54 +19:23:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253535_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253535_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:59:58.95 +25:07:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 3.560 4533934264139210112 284.99499958638 +25.11769943897 11.8335 10.1011 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253546_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253546_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:11:48.13 +18:58:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253547_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253547_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:30:49.80 +22:50:32.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253548_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253548_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:26:19.15 +22:21:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 253556_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 253556_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:22:18.11 +22:30:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81704_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 81704_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163069_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 163069_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:37:02.31 +24:45:06.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65894_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 65894_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:54:15.50 +19:33:19.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29846_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 29846_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58717_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 58717_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66497_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 66497_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237905_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 237905_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:36:17.09 +17:51:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26083_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 26083_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:33:24.01 +18:01:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58930_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 58930_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 148786_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 148786_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 63989_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 63989_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 71876_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 71876_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 96543_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 96543_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:24:48.00 +21:28:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103459_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 103459_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 25825_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 25825_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:27.89 +18:04:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85013_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 85013_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 90716_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 90716_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 96088_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 96088_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:40.06 +21:32:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 5.734 1826180275641004544 295.16798099076 +21.53428005035 12.5382 11.9446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139423_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 139423_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 69848_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 69848_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:57:26.99 +19:48:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76961_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 76961_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:42:13.44 +20:28:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49116_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 49116_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:17:55.46 +19:03:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72509_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 72509_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 45496_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 45496_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 143051_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 143051_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:32:37.18 +23:50:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170393_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 170393_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 233120_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233120_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:05:50.78 +22:53:26.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)
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Considering the candidate 233946_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233946_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:55:10.81 +18:05:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175957_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 175957_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 155543_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 155543_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 234093_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 234093_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:54:32.14 +19:01:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 251576_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 251576_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:19:47.24 +22:48:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108556_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 108556_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 61578_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 61578_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:11:17.99 +19:35:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21856_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 21856_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 118633_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 118633_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 55774_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 55774_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 115742_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 115742_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 147350_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 147350_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 31149_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 31149_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:13:30.45 +18:09:36.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 42720_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 42720_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 65361_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 65361_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 89767_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 89767_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 78663_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 78663_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 56514_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 56514_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 37369_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 37369_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 177832_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 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 174877_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 174877_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:37:40.15 +26:14:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.600 2021959930239516928 294.41802494729 +26.24669763409 12.8490 12.1704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 59216_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 59216_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:32:25.13 +19:38:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94148_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 94148_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:38:24.24 +21:23:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136123_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 136123_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:10:13.60 +23:20:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53661_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 53661_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 92079_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 92079_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:18:39.35 +21:12:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50626_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 50626_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 57952_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 57952_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 234358_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 234358_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:11.37 +18:04:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51013_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 51013_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:46.38 +19:16:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136507_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 136507_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 154477_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 154477_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:30:08.04 +24:22:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 30752_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:05:00.98 +18:02:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45264_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 45264_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 29436_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 29436_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 35095_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 35095_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 233919_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233919_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:22:54.87 +24:37:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233756_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233756_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:57:35.52 +17:35:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233752_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233752_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:20:12.43 +26:01:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 0.216 2024043470421500800 290.05179391795 +26.03014322777 11.3856 9.8922 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20613_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 20613_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 233540_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233540_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:41:41.56 +25:25:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233153_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 233153_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 183949_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 183949_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 52335_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:27:53.51 +19:17:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42876_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 42876_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:09:26.55 +18:41:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.343 4514756234422452224 287.35938790747 +18.68564791622 12.0437 10.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 182961_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 182961_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:29:19.54 +25:51:34.6 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 55675_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 55675_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 32268_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 32268_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:57:40.16 +18:01:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26141_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 26141_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:41:21.93 +18:05:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148949_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 148949_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:41:30.52 +24:07:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151575_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 151575_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 112797_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 112797_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:35:41.26 +22:20:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82826_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 82826_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 52703_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 52703_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:01:38.30 +19:03:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.346 4517786698949893120 285.40863172263 +19.05487256204 12.8329 10.7837 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 40590_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 40590_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 73036_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 73036_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:30:35.82 +20:15:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 110128_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 18:58:11.56 +21:52:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33243_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 33243_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:40:48.35 +18:25:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84895_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 84895_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:35:01.29 +20:55:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45827_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 45827_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:41:53.60 +19:01:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109418_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 109418_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:14:57.19 +22:04:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82699_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 82699_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:33:03.29 +20:45:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61230_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 61230_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:34:27.01 +19:45:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.698 1825528295291049344 293.61269030610 +19.75031014002 11.7413 10.1710 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 144307_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 144307_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 116825_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 116825_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 130649_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 130649_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 64063_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 64063_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:36:19.78 +19:53:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182417_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 182417_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:28:47.21 +25:53:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112394_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 112394_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 120679_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 120679_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 23513_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 23513_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:23:20.44 +17:49:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239260_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 239260_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:35:26.66 +18:48:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38764_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 38764_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:32:51.83 +18:40:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100525_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 100525_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 70013_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 70013_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:26:09.32 +20:07:44.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 43872_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 43872_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:03:06.08 +18:38:52.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)
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Considering the candidate 45937_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 45937_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 130977_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 130977_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:04:19.60 +23:01:41.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 31767_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 31767_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 165991_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 165991_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:27:21.69 +24:52:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246206_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 246206_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:24:48.73 +19:48:23.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 140690_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:39:20.25 +23:44:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135961_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 135961_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:31:10.19 +23:30:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128412_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 128412_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 152156_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 152156_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 39707_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 39707_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 71583_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 71583_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 67272_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 67272_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 179701_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 179701_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 93934_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 93934_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:29:30.15 +21:22:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98496_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 98496_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 39197_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
Preparing report for the candidate 39197_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
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Considering the candidate 190056_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 190056_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:42:22.61 +25:33:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26860_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 26860_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:37:38.78 +18:06:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120698_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 120698_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:03:36.30 +22:30:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90334_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 90334_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:28:55.18 +21:11:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178253_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 178253_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:18:33.43 +25:59:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174572_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 174572_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:25:20.45 +26:12:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80490_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 80490_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:31:54.01 +20:40:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24448_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 24448_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:38:55.11 +17:59:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 245027_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149
The candidate 245027_fd_Vul-01-Q2b1x1_2026-04-08_02-50-03_20.00sec_-4.90C_LIGHT_0149 did not pass the final checks
**** FOUND 19:25:31.25 +21:10:01.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 59s
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 ####
19:31:36.52 +21:45:02.7
18:54:11.01 +21:29:22.7
19:40:42.43 +22:10:29.0
19:25:27.05 +22:19:09.1
19:22:21.97 +22:27:59.5
19:27:58.50 +22:33:20.4
19:41:52.90 +22:41:37.0
19:14:36.83 +22:39:31.4
19:22:01.05 +23:06:22.4
19:35:49.86 +23:16:08.6
19:25:54.51 +23:30:30.1
19:14:12.51 +23:33:28.5
19:20:26.97 +23:50:28.7
19:35:17.98 +24:03:35.2
19:36:42.35 +24:07:04.3
19:21:47.46 +24:11:02.2
19:40:40.22 +24:17:21.0
19:38:42.13 +24:24:59.4
19:19:04.17 +25:00:34.0
19:32:35.73 +26:12:07.2
19:33:34.33 +26:01:13.7
19:40:51.21 +25:50:07.2
19:20:44.17 +17:42:53.7
19:31:30.73 +17:49:28.9
19:30:49.80 +23:40:05.6
19:37:39.48 +18:44:26.6
19:41:45.72 +17:48:19.9
19:42:19.94 +22:11:01.2
19:39:39.79 +24:51:54.2
19:35:38.32 +18:13:40.6
19:09:56.45 +18:00:07.4
19:34:15.67 +18:20:28.5
19:33:08.00 +18:29:30.1
19:14:45.88 +18:28:50.1
18:59:04.83 +18:18:51.6
19:29:40.99 +18:42:10.2
19:29:05.62 +18:44:01.4
19:20:55.73 +18:47:26.9
19:33:22.26 +18:58:40.0
19:16:57.11 +18:52:08.1
19:13:43.48 +18:52:08.0
19:22:35.12 +19:10:44.1
19:14:41.60 +19:15:00.1
19:02:35.53 +19:11:58.5
19:37:20.91 +19:28:56.6
19:40:48.75 +19:31:45.5
19:17:18.83 +19:29:05.7
19:08:06.46 +19:25:16.6
19:23:49.62 +19:35:00.9
19:21:10.00 +19:48:39.5
19:17:44.15 +19:50:03.2
19:22:33.25 +19:56:13.2
19:27:16.59 +20:00:06.3
19:41:13.78 +20:15:49.3
19:37:36.58 +20:15:55.8
19:10:03.05 +20:06:41.6
19:37:37.79 +20:45:06.0
19:40:12.32 +20:45:02.0
19:17:13.74 +20:48:41.2
19:29:09.86 +21:09:52.5
19:32:47.20 +21:12:34.7
19:32:51.07 +21:39:03.6
########### 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 ####
19:30:49.80 +23:40:05.6
19:37:39.48 +18:44:26.6
19:41:45.72 +17:48:19.9
19:42:19.94 +22:11:01.2
19:39:39.79 +24:51:54.2
19:37:37.79 +20:45:06.0
19:09:56.45 +18:00:07.4
19:08:06.46 +19:25:16.6
19:22:33.25 +19:56:13.2
19:23:49.62 +19:35:00.9
19:36:42.35 +24:07:04.3
19:21:10.00 +19:48:39.5
19:37:36.58 +20:15:55.8
18:54:11.01 +21:29:22.7
19:17:13.74 +20:48:41.2
19:32:47.20 +21:12:34.7
19:14:12.51 +23:33:28.5
19:10:03.05 +20:06:41.6
19:16:57.11 +18:52:08.1
19:19:04.17 +25:00:34.0
19:32:35.73 +26:12:07.2
19:38:42.13 +24:24:59.4
19:40:42.43 +22:10:29.0
19:31:30.73 +17:49:28.9
19:41:52.90 +22:41:37.0
19:37:20.91 +19:28:56.6
19:22:21.97 +22:27:59.5
19:35:17.98 +24:03:35.2
19:20:55.73 +18:47:26.9
19:17:44.15 +19:50:03.2
19:29:09.86 +21:09:52.5
19:40:48.75 +19:31:45.5
19:14:45.88 +18:28:50.1
19:14:41.60 +19:15:00.1
19:22:35.12 +19:10:44.1
19:17:18.83 +19:29:05.7
19:25:54.51 +23:30:30.1
19:33:22.26 +18:58:40.0
19:35:38.32 +18:13:40.6
19:33:08.00 +18:29:30.1
19:20:44.17 +17:42:53.7
19:40:51.21 +25:50:07.2
19:02:35.53 +19:11:58.5
19:21:47.46 +24:11:02.2
19:40:12.32 +20:45:02.0
19:29:05.62 +18:44:01.4
19:20:26.97 +23:50:28.7
19:27:58.50 +22:33:20.4
19:35:49.86 +23:16:08.6
19:25:27.05 +22:19:09.1
19:14:36.83 +22:39:31.4
19:31:36.52 +21:45:02.7
19:13:43.48 +18:52:08.0
19:34:15.67 +18:20:28.5
19:22:01.05 +23:06:22.4
19:40:40.22 +24:17:21.0
19:29:40.99 +18:42:10.2
19:41:13.78 +20:15:49.3
19:27:16.59 +20:00:06.3
19:33:34.33 +26:01:13.7
19:32:51.07 +21:39:03.6
18:59:04.83 +18:18:51.6
###################################################################################
19:30:49.80 +23:40:05.6 -- not an asteroid (will add it to exclusion list)
19:37:39.48 +18:44:26.6 -- not an asteroid (will add it to exclusion list)
19:41:45.72 +17:48:19.9 -- not an asteroid (will add it to exclusion list)
19:42:19.94 +22:11:01.2 -- not an asteroid (will add it to exclusion list)
19:39:39.79 +24:51:54.2 -- not an asteroid (will add it to exclusion list)
19:37:37.79 +20:45:06.0 -- not an asteroid (will add it to exclusion list)
19:09:56.45 +18:00:07.4 -- not an asteroid (will add it to exclusion list)
19:08:06.46 +19:25:16.6 -- not an asteroid (will add it to exclusion list)
19:22:33.25 +19:56:13.2 -- not an asteroid (will add it to exclusion list)
19:23:49.62 +19:35:00.9 -- not an asteroid (will add it to exclusion list)
19:36:42.35 +24:07:04.3 -- not an asteroid (will add it to exclusion list)
19:21:10.00 +19:48:39.5 -- not an asteroid (will add it to exclusion list)
19:37:36.58 +20:15:55.8 -- not an asteroid (will add it to exclusion list)
18:54:11.01 +21:29:22.7 -- not an asteroid (will add it to exclusion list)
19:17:13.74 +20:48:41.2 -- not an asteroid (will add it to exclusion list)
19:32:47.20 +21:12:34.7 -- not an asteroid (will add it to exclusion list)
19:14:12.51 +23:33:28.5 -- not an asteroid (will add it to exclusion list)
19:10:03.05 +20:06:41.6 -- not an asteroid (will add it to exclusion list)
19:16:57.11 +18:52:08.1 -- not an asteroid (will add it to exclusion list)
19:19:04.17 +25:00:34.0 -- not an asteroid (will add it to exclusion list)
19:32:35.73 +26:12:07.2 -- not an asteroid (will add it to exclusion list)
19:38:42.13 +24:24:59.4 -- not an asteroid (will add it to exclusion list)
19:40:42.43 +22:10:29.0 -- not an asteroid (will add it to exclusion list)
19:31:30.73 +17:49:28.9 -- not an asteroid (will add it to exclusion list)
19:41:52.90 +22:41:37.0 -- not an asteroid (will add it to exclusion list)
19:37:20.91 +19:28:56.6 -- not an asteroid (will add it to exclusion list)
19:22:21.97 +22:27:59.5 -- not an asteroid (will add it to exclusion list)
19:35:17.98 +24:03:35.2 -- not an asteroid (will add it to exclusion list)
19:20:55.73 +18:47:26.9 -- not an asteroid (will add it to exclusion list)
19:17:44.15 +19:50:03.2 -- not an asteroid (will add it to exclusion list)
19:29:09.86 +21:09:52.5 -- not an asteroid (will add it to exclusion list)
19:40:48.75 +19:31:45.5 -- not an asteroid (will add it to exclusion list)
19:14:45.88 +18:28:50.1 -- not an asteroid (will add it to exclusion list)
19:14:41.60 +19:15:00.1 -- not an asteroid (will add it to exclusion list)
19:22:35.12 +19:10:44.1 -- not an asteroid (will add it to exclusion list)
19:17:18.83 +19:29:05.7 -- not an asteroid (will add it to exclusion list)
19:25:54.51 +23:30:30.1 -- not an asteroid (will add it to exclusion list)
19:33:22.26 +18:58:40.0 -- not an asteroid (will add it to exclusion list)
19:35:38.32 +18:13:40.6 -- not an asteroid (will add it to exclusion list)
19:33:08.00 +18:29:30.1 -- not an asteroid (will add it to exclusion list)
19:20:44.17 +17:42:53.7 -- not an asteroid (will add it to exclusion list)
19:40:51.21 +25:50:07.2 -- not an asteroid (will add it to exclusion list)
19:02:35.53 +19:11:58.5 -- not an asteroid (will add it to exclusion list)
19:21:47.46 +24:11:02.2 -- not an asteroid (will add it to exclusion list)
19:40:12.32 +20:45:02.0 -- not an asteroid (will add it to exclusion list)
19:29:05.62 +18:44:01.4 -- not an asteroid (will add it to exclusion list)
19:20:26.97 +23:50:28.7 -- not an asteroid (will add it to exclusion list)
19:27:58.50 +22:33:20.4 -- not an asteroid (will add it to exclusion list)
19:35:49.86 +23:16:08.6 -- not an asteroid (will add it to exclusion list)
19:25:27.05 +22:19:09.1 -- not an asteroid (will add it to exclusion list)
19:14:36.83 +22:39:31.4 -- not an asteroid (will add it to exclusion list)
19:31:36.52 +21:45:02.7 -- not an asteroid (will add it to exclusion list)
19:13:43.48 +18:52:08.0 -- not an asteroid (will add it to exclusion list)
19:34:15.67 +18:20:28.5 -- not an asteroid (will add it to exclusion list)
19:22:01.05 +23:06:22.4 -- not an asteroid (will add it to exclusion list)
19:40:40.22 +24:17:21.0 -- not an asteroid (will add it to exclusion list)
19:29:40.99 +18:42:10.2 -- not an asteroid (will add it to exclusion list)
19:41:13.78 +20:15:49.3 -- not an asteroid (will add it to exclusion list)
19:27:16.59 +20:00:06.3 -- not an asteroid (will add it to exclusion list)
19:33:34.33 +26:01:13.7 -- not an asteroid (will add it to exclusion list)
19:32:51.07 +21:39:03.6 -- 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)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:54:11.01 +21:29:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:04.83 +18:18:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:35.53 +19:11:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:06.46 +19:25:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:56.45 +18:00:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:03.05 +20:06:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:13:43.48 +18:52:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:12.51 +23:33:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:36.83 +22:39:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:41.60 +19:15:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:14:45.88 +18:28:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:57.11 +18:52:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:13.74 +20:48:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:18.83 +19:29:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:17:44.15 +19:50:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:04.17 +25:00:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:26.97 +23:50:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:44.17 +17:42:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:20:55.73 +18:47:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:10.00 +19:48:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:21:47.46 +24:11:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:01.05 +23:06:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:21.97 +22:27:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:33.25 +19:56:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:22:35.12 +19:10:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:49.62 +19:35:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:27.05 +22:19:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:54.51 +23:30:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:16.59 +20:00:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:58.50 +22:33:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:05.62 +18:44:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:09.86 +21:09:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:40.99 +18:42:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:49.80 +23:40:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:30.73 +17:49:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:36.52 +21:45:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:35.73 +26:12:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:47.20 +21:12:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:51.07 +21:39:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:08.00 +18:29:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:22.26 +18:58:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:34.33 +26:01:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:15.67 +18:20:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:17.98 +24:03:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:38.32 +18:13:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:49.86 +23:16:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:42.35 +24:07:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:20.91 +19:28:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:36.58 +20:15:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:37.79 +20:45:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:39.48 +18:44:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:42.13 +24:24:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:39.79 +24:51:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:12.32 +20:45:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:40.22 +24:17:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:42.43 +22:10:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:48.75 +19:31:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:51.21 +25:50:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:13.78 +20:15:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:45.72 +17:48:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:52.90 +22:41:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:19.94 +22:11:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
18:54:11.01 +21:29:22.7 -- a known variable star
18:59:04.83 +18:18:51.6 -- a known variable star
19:02:35.53 +19:11:58.5 -- a known variable star
19:08:06.46 +19:25:16.6 -- a known variable star
19:09:56.45 +18:00:07.4 -- a known variable star
19:10:03.05 +20:06:41.6 -- a known variable star
19:13:43.48 +18:52:08.0 -- a known variable star
19:14:12.51 +23:33:28.5 -- a known variable star
19:14:36.83 +22:39:31.4 -- a known variable star
19:14:41.60 +19:15:00.1 -- a known variable star
19:14:45.88 +18:28:50.1 -- not a known variable star
19:16:57.11 +18:52:08.1 -- a known variable star
19:17:13.74 +20:48:41.2 -- a known variable star
19:17:18.83 +19:29:05.7 -- a known variable star
19:17:44.15 +19:50:03.2 -- a known variable star
19:19:04.17 +25:00:34.0 -- a known variable star
19:20:26.97 +23:50:28.7 -- a known variable star
19:20:44.17 +17:42:53.7 -- a known variable star
19:20:55.73 +18:47:26.9 -- a known variable star
19:21:10.00 +19:48:39.5 -- a known variable star
19:21:47.46 +24:11:02.2 -- a known variable star
19:22:01.05 +23:06:22.4 -- a known variable star
19:22:21.97 +22:27:59.5 -- a known variable star
19:22:33.25 +19:56:13.2 -- a known variable star
19:22:35.12 +19:10:44.1 -- a known variable star
19:23:49.62 +19:35:00.9 -- a known variable star
19:25:27.05 +22:19:09.1 -- a known variable star
19:25:54.51 +23:30:30.1 -- a known variable star
19:27:16.59 +20:00:06.3 -- a known variable star
19:27:58.50 +22:33:20.4 -- a known variable star
19:29:05.62 +18:44:01.4 -- a known variable star
19:29:09.86 +21:09:52.5 -- a known variable star
19:29:40.99 +18:42:10.2 -- a known variable star
19:30:49.80 +23:40:05.6 -- a known variable star
19:31:30.73 +17:49:28.9 -- a known variable star
19:31:36.52 +21:45:02.7 -- a known variable star
19:32:35.73 +26:12:07.2 -- a known variable star
19:32:47.20 +21:12:34.7 -- a known variable star
19:32:51.07 +21:39:03.6 -- a known variable star
19:33:08.00 +18:29:30.1 -- a known variable star
19:33:22.26 +18:58:40.0 -- a known variable star
19:33:34.33 +26:01:13.7 -- a known variable star
19:34:15.67 +18:20:28.5 -- a known variable star
19:35:17.98 +24:03:35.2 -- a known variable star
19:35:38.32 +18:13:40.6 -- a known variable star
19:35:49.86 +23:16:08.6 -- a known variable star
19:36:42.35 +24:07:04.3 -- a known variable star
19:37:20.91 +19:28:56.6 -- a known variable star
19:37:36.58 +20:15:55.8 -- a known variable star
19:37:37.79 +20:45:06.0 -- a known variable star
19:37:39.48 +18:44:26.6 -- not a known variable star
19:38:42.13 +24:24:59.4 -- a known variable star
19:39:39.79 +24:51:54.2 -- a known variable star
19:40:12.32 +20:45:02.0 -- a known variable star
19:40:40.22 +24:17:21.0 -- not a known variable star
19:40:42.43 +22:10:29.0 -- a known variable star
19:40:48.75 +19:31:45.5 -- a known variable star
19:40:51.21 +25:50:07.2 -- a known variable star
19:41:13.78 +20:15:49.3 -- a known variable star
19:41:45.72 +17:48:19.9 -- a known variable star
19:41:52.90 +22:41:37.0 -- a known variable star
19:42:19.94 +22:11:01.2 -- a known variable star
Found 3 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
62 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
18:54:11.01 +21:29:22.7
18:59:04.83 +18:18:51.6
19:02:35.53 +19:11:58.5
19:08:06.46 +19:25:16.6
19:09:56.45 +18:00:07.4
19:10:03.05 +20:06:41.6
19:13:43.48 +18:52:08.0
19:14:12.51 +23:33:28.5
19:14:36.83 +22:39:31.4
19:14:41.60 +19:15:00.1
19:14:45.88 +18:28:50.1
19:16:57.11 +18:52:08.1
19:17:13.74 +20:48:41.2
19:17:18.83 +19:29:05.7
19:17:44.15 +19:50:03.2
19:19:04.17 +25:00:34.0
19:20:26.97 +23:50:28.7
19:20:44.17 +17:42:53.7
19:20:55.73 +18:47:26.9
19:21:10.00 +19:48:39.5
19:21:47.46 +24:11:02.2
19:22:01.05 +23:06:22.4
19:22:21.97 +22:27:59.5
19:22:33.25 +19:56:13.2
19:22:35.12 +19:10:44.1
19:23:49.62 +19:35:00.9
19:25:27.05 +22:19:09.1
19:25:54.51 +23:30:30.1
19:27:16.59 +20:00:06.3
19:27:58.50 +22:33:20.4
19:29:05.62 +18:44:01.4
19:29:09.86 +21:09:52.5
19:29:40.99 +18:42:10.2
19:30:49.80 +23:40:05.6
19:31:30.73 +17:49:28.9
19:31:36.52 +21:45:02.7
19:32:35.73 +26:12:07.2
19:32:47.20 +21:12:34.7
19:32:51.07 +21:39:03.6
19:33:08.00 +18:29:30.1
19:33:22.26 +18:58:40.0
19:33:34.33 +26:01:13.7
19:34:15.67 +18:20:28.5
19:35:17.98 +24:03:35.2
19:35:38.32 +18:13:40.6
19:35:49.86 +23:16:08.6
19:36:42.35 +24:07:04.3
19:37:20.91 +19:28:56.6
19:37:36.58 +20:15:55.8
19:37:37.79 +20:45:06.0
19:37:39.48 +18:44:26.6
19:38:42.13 +24:24:59.4
19:39:39.79 +24:51:54.2
19:40:12.32 +20:45:02.0
19:40:40.22 +24:17:21.0
19:40:42.43 +22:10:29.0
19:40:48.75 +19:31:45.5
19:40:51.21 +25:50:07.2
19:41:13.78 +20:15:49.3
19:41:45.72 +17:48:19.9
19:41:52.90 +22:41:37.0
19:42:19.94 +22:11:01.2
19:04:19.60 +23:01:41.0
19:37:40.15 +26:14:45.4
19:29:19.54 +25:51:34.6
19:05:50.78 +22:53:26.4
19:20:12.43 +26:01:48.3
19:24:48.73 +19:48:23.2
19:12:29.34 +24:30:38.3
19:38:05.34 +21:02:45.8
19:31:16.62 +23:52:31.8
19:14:39.75 +19:07:39.2
19:16:17.85 +25:22:49.6
19:09:25.58 +25:54:34.3
19:10:55.50 +24:02:42.8
19:05:54.72 +19:53:44.7
19:35:59.54 +18:46:12.3
18:55:38.70 +19:24:57.9
19:37:13.48 +21:05:02.4
19:40:32.93 +18:45:22.9
19:42:13.28 +23:15:07.5
19:37:07.56 +19:15:52.4
19:37:43.28 +24:48:46.6
19:41:12.78 +18:08:55.9
19:05:21.71 +23:45:19.9
18:59:58.95 +25:07:00.8
19:30:49.80 +22:50:32.4
19:13:30.45 +18:09:36.4
19:09:26.55 +18:41:07.3
19:03:06.08 +18:38:52.5
19:01:38.30 +19:03:16.7
19:34:27.01 +19:45:01.6
19:40:40.06 +21:32:07.9
19:42:07.22 +18:40:42.9
####################################################
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461138.82587536 -observatory V36
23:29:41.51 -05:40:01.1 Mercury (0.3mag)
02:31:37.14 +14:46:27.1 Venus (-3.9mag)
23:56:00.06 -01:32:26.4 Mars (1.2mag)
07:09:27.84 +22:51:16.5 Jupiter (-2.2mag)
00:25:43.82 +00:27:20.4 Saturn (0.9mag)
03:46:08.13 +19:42:26.1 Uranus (5.8mag)
00:09:49.15 -00:21:49.9 Neptune (7.8mag)
20:33:21.86 -22:52:27.3 Pluto (14.5mag)
17:51:45.62 -28:53:29.4 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 02:52 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461138.82587536:
07:09:22.26 +22:51:25.3 Io (5.7mag)
07:09:19.09 +22:51:36.5 Europa (5.9mag)
07:09:48.26 +22:50:35.3 Ganymede (5.3mag)
07:08:53.09 +22:52:26.1 Callisto (6.5mag)
07:13:06.47 +22:42:39.8 Himalia (15.3mag)
07:09:29.01 +22:51:16.3 Thebe (16.2mag)
07:13:07.28 +23:11:52.2 Elara (17.3mag)
07:07:49.39 +23:35:17.7 Pasiphae (17.4mag)
07:17:57.21 +22:48:28.1 Carme (18.4mag)
00:25:47.14 +00:27:10.7 Titan (8.8mag)
00:25:49.23 +00:27:21.1 Rhea (10.1mag)
00:25:39.52 +00:28:38.4 Iapetus (11.5mag)
00:25:52.87 +00:27:05.9 Hyperion (14.8mag)
00:27:26.55 +00:36:56.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 02:52 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.82587536:
14:59:13.07 -10:15:34.0 JWST
14:34:16.90 +56:14:34.4 Chandra
08:25:03.28 -45:43:15.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 02:52 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.82587536 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:20.40 -28:20:54.3 13.9mag P/2010 H2 (Vales)
05:01:27.57 -70:02:17.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:55.96 +31:23:17.8 17.2mag C/2017 K2 (PANSTARRS)
17:30:55.03 +09:37:43.4 17.6mag C/2021 G2 (ATLAS)
23:08:01.45 +28:56:28.2 17.0mag C/2022 E2 (ATLAS)
04:20:24.21 +25:49:30.5 15.9mag C/2022 N2 (PANSTARRS)
09:02:06.14 +31:56:26.3 16.2mag C/2022 QE78 (ATLAS)
08:30:08.73 -00:59:25.7 17.3mag C/2022 R6 (PANSTARRS)
18:55:16.22 +17:52:45.3 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:57.50 -11:37:53.4 17.6mag P/2023 B1 (PANSTARRS)
09:11:34.95 -13:08:32.3 17.6mag C/2023 F3 (ATLAS)
21:45:58.52 +62:28:49.3 17.5mag C/2023 H5 (Lemmon)
19:25:03.86 -03:37:45.8 14.2mag C/2023 R1 (PANSTARRS)
21:41:48.93 +84:52:53.3 17.8mag C/2023 X2 (Lemmon)
06:15:02.11 +63:33:48.2 17.1mag C/2024 A1 (ATLAS)
04:56:07.87 +15:28:04.5 10.5mag C/2024 E1 (Wierzchos)
16:23:55.51 +05:07:43.9 17.4mag C/2024 G6 (ATLAS)
20:18:21.03 +13:14:01.5 14.7mag C/2024 J3 (ATLAS)
03:19:35.95 -23:34:49.1 16.4mag C/2024 T5 (ATLAS)
05:10:23.08 +47:15:37.2 17.7mag C/2025 J1 (Borisov)
14:10:32.80 +39:27:43.2 14.9mag C/2025 L1 (ATLAS)
03:13:30.27 -25:03:19.2 17.8mag C/2025 Q3 (ATLAS)
22:59:50.14 +19:48:24.4 9.7mag C/2025 R3 (PANSTARRS)
12:57:27.66 +02:31:52.3 17.5mag C/2025 Y1 (ATLAS)
02:05:36.98 +03:57:30.0 9.7mag C/2026 A1 (MAPS)
23:37:14.76 +35:42:23.1 14.3mag C/2026 B2 (Sun-Gao)
18:27:57.92 -10:06:57.0 12.3mag 10P/Tempel
15:10:19.54 +03:56:13.0 13.3mag 24P/Schaumasse
11:05:03.79 -01:47:12.4 15.7mag 29P/Schwassmann-Wachmann
17:57:55.49 -09:54:23.9 17.8mag 40P/Vaisala
10:38:25.58 -04:45:04.6 16.8mag 43P/Wolf-Harrington
01:36:49.88 +16:10:03.8 17.2mag 47P/Ashbrook-Jackson
06:56:59.45 +38:38:14.8 17.0mag 63P/Wild
23:19:07.68 -12:23:18.3 15.7mag 65P/Gunn
03:43:07.45 +18:31:45.7 15.9mag 76P/West-Kohoutek-Ikemura
00:48:43.33 +06:42:38.1 14.4mag 78P/Gehrels
22:39:19.07 -11:39:01.9 14.5mag 88P/Howell
01:48:59.90 +18:32:51.4 15.1mag 93P/Lovas
04:40:41.97 +31:51:21.8 16.3mag 123P/West-Hartley
08:19:58.53 +41:54:17.2 16.2mag 124P/Mrkos
02:21:27.04 +13:30:08.9 16.4mag 128P/Shoemaker-Holt
02:32:32.60 +13:31:52.2 17.5mag 131P/Mueller
00:46:34.46 +10:26:14.5 11.1mag 141P/Machholz
00:56:23.11 +01:59:36.0 11.1mag 141P-A/Machholz
23:45:42.89 -01:44:58.8 13.8mag 141P-D/Machholz
01:25:50.29 +03:41:27.0 17.9mag 141P-I/Machholz
00:41:02.89 -05:21:46.7 15.2mag 162P/SidingSpring
10:30:19.52 +31:22:30.9 17.9mag 164P/Christensen
06:22:20.29 +24:28:15.9 17.9mag 198P/ODAS
15:05:00.37 -00:55:51.9 17.4mag 210P/Christensen
21:15:43.20 -13:18:21.7 17.5mag 218P/LINEAR
17:13:44.40 -14:50:01.3 16.2mag 235P/LINEAR
05:18:07.09 +34:03:27.5 16.6mag 240P/NEAT
07:35:01.99 -06:01:57.8 17.6mag 242P/Spahr
15:45:19.38 +06:27:47.0 17.5mag 391P/Kowalski
07:31:32.26 +21:19:40.4 17.6mag 450P/LONEOS
05:24:52.97 +45:29:02.4 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 02:52 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 8 02:52 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 8 02:52 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:46:09.818 -61:19:51.60 AT 2026icy 2026-04-02.36 18.325
15:30:09.406 +58:57:13.42 AT 2026icx 2026-03-30.43 19.684
11:28:54.874 +21:06:30.69 AT 2026icw 2026-04-02.30 19.2031
12:10:50.697 +66:55:30.99 SN 2026icv 2026-04-02.28 18.5118
07:36:32.513 +50:19:24.81 AT 2026icu 2026-04-02.24 19.2237
08:38:37.560 +02:03:38.03 AT 2026ict 2026-04-02.15 19.0837
10:11:03.633 -05:31:15.36 AT 2026ics 2026-04-02.23 18.6573
11:09:42.183 +10:32:49.70 AT 2026icr 2026-03-24.33 20.476
10:16:29.552 -18:01:01.61 AT 2026icq 2026-03-25.18 20.2716
18:12:46.220 -18:40:42.30 AT 2026icp 2026-04-02.23 18.9
07:46:30.650 +27:23:24.16 AT 2026ico 2026-03-30.16 19.803
07:04:53.063 +10:28:54.71 AT 2026icn 2026-03-29.17 19.8144
10:09:06.230 +29:30:55.76 AT 2026icm 2026-03-27.16 20.1135
08:07:47.384 -00:23:25.65 AT 2026icl 2026-03-30.25 19.1418
07:33:52.396 +16:18:53.23 AT 2026ick 2026-03-30.19 19.5464
03:49:33.049 -49:30:53.67 AT 2026icj 2026-02-23.11 23.84
15:40:04.940 -18:30:53.00 AT 2026ici 2026-03-29.36 18.4
16:52:58.870 -62:16:14.10 AT 2026ich 2026-04-01.35 16.9
19:13:48.516 +60:10:55.03 AT 2026icg 2026-03-28.56 18.844
07:51:19.796 +21:17:20.06 AT 2026icf 2026-03-30.91 18.372
-rw-r--r-- 1 apache apache 30K Apr 8 02:52 tns_transients_list.txt
