This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6028049306458524672,2461150.9264,10.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6028049306458524672 20260420.4264 10.35CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J252.2602-21.3708,2461150.9264,9.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J252.2602-21.3708 20260420.4264 9.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037645126698020224,2461150.9264,9.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6037645126698020224 20260420.4264 9.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127072420195118336,2461150.9264,9.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127072420195118336 20260420.4264 9.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031416187195473024,2461150.9264,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031416187195473024 20260420.4264 9.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.1067-28.7299,2461150.9264,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.1067-28.7299 20260420.4264 9.93CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046552781485318912,2461150.9264,9.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046552781485318912 20260420.4264 9.94CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032914203067481984,2461150.9264,10.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032914203067481984 20260420.4264 10.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034026359060051968,2461150.9264,10.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034026359060051968 20260420.4264 10.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126993740688980480,2461150.9264,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126993740688980480 20260420.4264 10.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6036992978870487680,2461150.9264,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6036992978870487680 20260420.4264 10.39CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 10.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6045465815462093696,2461150.9264,8.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6045465815462093696 20260420.4264 8.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J241.0543-22.7659,2461150.9264,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J241.0543-22.7659 20260420.4264 12.43CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6043053143356508160,2461150.9264,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6043053143356508160 20260420.4264 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.6225-28.6177,2461150.9264,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.6225-28.6177 20260420.4264 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J240.2677-25.1218,2461150.9264,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J240.2677-25.1218 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.6201-29.1946,2461150.9264,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.6201-29.1946 20260420.4264 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
PS1-3PI J165041.89-243430.8,2461150.9264,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
PS1-3PI J165041.89-243430.8 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6039206330125563904,2461150.9264,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6039206330125563904 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.3613-27.7734,2461150.9264,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.3613-27.7734 20260420.4264 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.8889-29.0883,2461150.9264,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.8889-29.0883 20260420.4264 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 204090458,2461150.9264,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 204090458 20260420.4264 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 12.14 16:37:35.07 -24:52:43.0
354.40826 14.67709 galactic Sco Second-epoch detections are separated by 7.9" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6047374533282026368 | 16:37:34.35 -24:52:43.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6047374533282026368,2461150.9264,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6047374533282026368 20260420.4264 12.14CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.2790-30.3074,2461150.9264,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J238.2790-30.3074 20260420.4264 12.25CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6239929427678153728,2461150.9264,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6239929427678153728 20260420.4264 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044906026610285824,2461150.9264,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044906026610285824 20260420.4264 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233697911171701376,2461150.9264,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233697911171701376 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233467219884944000,2461150.9264,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233467219884944000 20260420.4264 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J154955.86-252204.9,2461150.9264,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J154955.86-252204.9 20260420.4264 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J155020.78-211655.0,2461150.9264,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155020.78-211655.0 20260420.4264 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.81 16:50:08.90 -22:57:21.4
357.80906 13.64441 galactic Oph Second-epoch detections are separated by 6.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4125699306270803072 | 16:50:08.47 -22:57:13.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4125699306270803072,2461150.9264,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4125699306270803072 20260420.4264 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.1701-27.2760,2461150.9264,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.1701-27.2760 20260420.4264 11.94CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233482063292031872,2461150.9264,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233482063292031872 20260420.4264 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.8636-24.1625,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.8636-24.1625 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.7124-28.3666,2461150.9264,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.7124-28.3666 20260420.4264 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.1809-29.7168,2461150.9264,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.1809-29.7168 20260420.4264 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233999795833488384,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233999795833488384 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233710997932310144,2461150.9264,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233710997932310144 20260420.4264 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6240743306802555776,2461150.9264,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6240743306802555776 20260420.4264 11.50CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041801864765430784,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6041801864765430784 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.4331-29.1650,2461150.9264,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J238.4331-29.1650 20260420.4264 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033881872050362624,2461150.9264,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033881872050362624 20260420.4264 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6236755515566133120,2461150.9264,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6236755515566133120 20260420.4264 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034772961825422848,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034772961825422848 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.8901-28.3223,2461150.9264,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.8901-28.3223 20260420.4264 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6239915168382619136,2461150.9264,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6239915168382619136 20260420.4264 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032007209033561472,2461150.9264,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032007209033561472 20260420.4264 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6236024409061930240,2461150.9264,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6236024409061930240 20260420.4264 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165011.41-295741.5,2461150.9264,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165011.41-295741.5 20260420.4264 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6234884112415684352,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6234884112415684352 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233380633345899264,2461150.9264,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233380633345899264 20260420.4264 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040771656727666048,2461150.9264,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040771656727666048 20260420.4264 11.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030853679584654976,2461150.9264,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030853679584654976 20260420.4264 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161610-2821.6,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J161610-2821.6 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041678032274898176,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6041678032274898176 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.9057-22.4889,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.9057-22.4889 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J239.8526-30.1246,2461150.9264,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J239.8526-30.1246 20260420.4264 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233183683326213632,2461150.9264,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233183683326213632 20260420.4264 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233886580492864000,2461150.9264,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233886580492864000 20260420.4264 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J163913.26-302421.4,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J163913.26-302421.4 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040652943833096960,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040652943833096960 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.1207-26.6298,2461150.9264,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.1207-26.6298 20260420.4264 11.67CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233224433975744768,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233224433975744768 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046350269499290752,2461150.9264,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046350269499290752 20260420.4264 11.50CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6236663431466957056,2461150.9264,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6236663431466957056 20260420.4264 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J155453-2847.9,2461150.9264,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155453-2847.9 20260420.4264 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030750913928414592,2461150.9264,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030750913928414592 20260420.4264 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.2888-27.2423,2461150.9264,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.2888-27.2423 20260420.4264 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046256055091583104,2461150.9264,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046256055091583104 20260420.4264 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.73 16:43:45.54 -30:06:17.2
351.19973 10.27517 galactic Sco Second-epoch detections are separated by 2.9" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6031197212577436544 | 16:43:45.87 -30:06:23.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6031197212577436544,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6031197212577436544 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233861253066287488,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233861253066287488 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233923448492583040,2461150.9264,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233923448492583040 20260420.4264 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.2171-30.2145,2461150.9264,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.2171-30.2145 20260420.4264 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033865349333699456,2461150.9264,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033865349333699456 20260420.4264 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040949296571318016,2461150.9264,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040949296571318016 20260420.4264 11.62CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164948-2257.1,2461150.9264,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164948-2257.1 20260420.4264 11.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6016808041317590144,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6016808041317590144 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233089125324899712,2461150.9264,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233089125324899712 20260420.4264 11.62CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J163731-2832.0,2461150.9264,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J163731-2832.0 20260420.4264 11.53CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6234934891809835392,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6234934891809835392 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J154713-2302.7,2461150.9264,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J154713-2302.7 20260420.4264 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233242197960708608,2461150.9264,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233242197960708608 20260420.4264 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J155008.16-233320.8,2461150.9264,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155008.16-233320.8 20260420.4264 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6045449249772740864,2461150.9264,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6045449249772740864 20260420.4264 11.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165308.00-294202.9,2461150.9264,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165308.00-294202.9 20260420.4264 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J155026-2342.1,2461150.9264,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155026-2342.1 20260420.4264 10.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.2830-27.9600,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.2830-27.9600 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041301827482290432,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6041301827482290432 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1143 Sco,2461150.9264,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1143 Sco 20260420.4264 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030843650866211968,2461150.9264,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030843650866211968 20260420.4264 11.49CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030893949221116288,2461150.9264,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030893949221116288 20260420.4264 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030899279288214912,2461150.9264,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030899279288214912 20260420.4264 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233518518974463616,2461150.9264,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233518518974463616 20260420.4264 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030891101681918976,2461150.9264,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030891101681918976 20260420.4264 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6234921392732241280,2461150.9264,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6234921392732241280 20260420.4264 11.13CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031070940543552512,2461150.9264,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031070940543552512 20260420.4264 11.20CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J154345-2750.2,2461150.9264,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J154345-2750.2 20260420.4264 11.02CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031235283163065728,2461150.9264,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031235283163065728 20260420.4264 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048769431286098176,2461150.9264,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048769431286098176 20260420.4264 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J245.0884-25.1050,2461150.9264,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J245.0884-25.1050 20260420.4264 9.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031195593343974016,2461150.9264,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031195593343974016 20260420.4264 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6025800878211901568,2461150.9264,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6025800878211901568 20260420.4264 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J155335-2749.5,2461150.9264,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155335-2749.5 20260420.4264 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6027980312109196160,2461150.9264,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6027980312109196160 20260420.4264 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161949-2217.2,2461150.9264,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J161949-2217.2 20260420.4264 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034737055896419968,2461150.9264,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034737055896419968 20260420.4264 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032980616113959040,2461150.9264,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032980616113959040 20260420.4264 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034755850662482176,2461150.9264,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034755850662482176 20260420.4264 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044090085905116160,2461150.9264,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044090085905116160 20260420.4264 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034616728094251648,2461150.9264,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034616728094251648 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127075860479593984,2461150.9264,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127075860479593984 20260420.4264 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033509932221725568,2461150.9264,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033509932221725568 20260420.4264 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6244540500267763072,2461150.9264,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6244540500267763072 20260420.4264 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J251.9637-29.8711,2461150.9264,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J251.9637-29.8711 20260420.4264 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125657834075475200,2461150.9264,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125657834075475200 20260420.4264 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031459995840578816,2461150.9264,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031459995840578816 20260420.4264 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164907.53-231125.3,2461150.9264,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164907.53-231125.3 20260420.4264 10.62CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029564987601059968,2461150.9264,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6029564987601059968 20260420.4264 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030909239284931840,2461150.9264,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030909239284931840 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6045621946116752128,2461150.9264,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6045621946116752128 20260420.4264 10.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6038087473966871808,2461150.9264,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6038087473966871808 20260420.4264 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.03 16:48:57.44 -28:48:25.8
352.94854 10.22357 galactic Sco Second-epoch detections are separated by 4.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6032879499698289408 | 16:48:56.10 -28:48:50.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6032879499698289408,2461150.9264,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6032879499698289408 20260420.4264 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6042833137954581760,2461150.9264,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6042833137954581760 20260420.4264 10.93CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 203012217,2461150.9264,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 203012217 20260420.4264 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048065851223836032,2461150.9264,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048065851223836032 20260420.4264 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127018307918370304,2461150.9264,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127018307918370304 20260420.4264 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6038368708429129728,2461150.9264,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6038368708429129728 20260420.4264 11.14CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6235784749881197184,2461150.9264,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6235784749881197184 20260420.4264 10.72CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033115207536998144,2461150.9264,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033115207536998144 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032711789869516928,2461150.9264,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032711789869516928 20260420.4264 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 204599207,2461150.9264,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 204599207 20260420.4264 10.72CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032018066717532160,2461150.9264,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032018066717532160 20260420.4264 11.21CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J165325-2520.8,2461150.9264,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165325-2520.8 20260420.4264 10.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6049598226836647936,2461150.9264,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6049598226836647936 20260420.4264 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1039 Sco,2461150.9264,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1039 Sco 20260420.4264 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6028002134873267200,2461150.9264,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6028002134873267200 20260420.4264 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164704-2548.3,2461150.9264,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164704-2548.3 20260420.4264 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J252.9004-29.9367,2461150.9264,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J252.9004-29.9367 20260420.4264 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125532695914034816,2461150.9264,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125532695914034816 20260420.4264 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030940888934976384,2461150.9264,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030940888934976384 20260420.4264 11.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 203728604,2461150.9264,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 203728604 20260420.4264 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034335970356604032,2461150.9264,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034335970356604032 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233675405544548608,2461150.9264,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233675405544548608 20260420.4264 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048008779703250688,2461150.9264,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048008779703250688 20260420.4264 10.98CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046811102318227584,2461150.9264,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046811102318227584 20260420.4264 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 10.94CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125700886827399808,2461150.9264,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125700886827399808 20260420.4264 10.98CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033073082494247936,2461150.9264,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033073082494247936 20260420.4264 11.27CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127075860479593984,2461150.9264,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127075860479593984 20260420.4264 10.94CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034749872079039104,2461150.9264,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034749872079039104 20260420.4264 11.18CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034693212875978496,2461150.9264,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034693212875978496 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165301.90-264038.0,2461150.9264,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165301.90-264038.0 20260420.4264 11.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164418-2206.8,2461150.9264,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164418-2206.8 20260420.4264 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041016091906307328,2461150.9264,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6041016091906307328 20260420.4264 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J252.3706-22.1729,2461150.9264,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J252.3706-22.1729 20260420.4264 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032218349639104512,2461150.9264,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032218349639104512 20260420.4264 11.15CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046933869646677504,2461150.9264,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046933869646677504 20260420.4264 11.14CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6234861160110764160,2461150.9264,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6234861160110764160 20260420.4264 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034247635784064512,2461150.9264,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034247635784064512 20260420.4264 11.18CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6246866521418921728,2461150.9264,10.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6246866521418921728 20260420.4264 10.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126482463488713856,2461150.9264,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126482463488713856 20260420.4264 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J246.7118-30.6081,2461150.9264,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J246.7118-30.6081 20260420.4264 11.44CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046270657982273792,2461150.9264,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046270657982273792 20260420.4264 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164418-2206.8,2461150.9264,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164418-2206.8 20260420.4264 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030890173968968064,2461150.9264,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030890173968968064 20260420.4264 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031152678033073024,2461150.9264,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031152678033073024 20260420.4264 11.43CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126750611187648896,2461150.9264,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126750611187648896 20260420.4264 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.44 16:21:15.09 -29:00:34.9
348.71765 14.66609 galactic Sco Second-epoch detections are separated by 4.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6038924889508958080 | 16:21:14.16 -29:00:58.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6038924889508958080,2461150.9264,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6038924889508958080 20260420.4264 11.44CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032232780730314752,2461150.9264,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032232780730314752 20260420.4264 11.53CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031033930774957952,2461150.9264,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031033930774957952 20260420.4264 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125710606323941504,2461150.9264,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125710606323941504 20260420.4264 11.14CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.40 16:21:15.35 -29:00:17.6
348.72194 14.66869 galactic Sco Second-epoch detections are separated by 2.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6038924889508958080 | 16:21:14.16 -29:00:58.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6038924889508958080,2461150.9264,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6038924889508958080 20260420.4264 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J155344.80-271625.8,2461150.9264,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155344.80-271625.8 20260420.4264 11.20CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048260499144912768,2461150.9264,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048260499144912768 20260420.4264 11.23CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034223652684958592,2461150.9264,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034223652684958592 20260420.4264 11.36CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6244055448144992256,2461150.9264,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6244055448144992256 20260420.4264 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125842719522931712,2461150.9264,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125842719522931712 20260420.4264 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040158782082084224,2461150.9264,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040158782082084224 20260420.4264 11.49CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037652307883164800,2461150.9264,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6037652307883164800 20260420.4264 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033079164168192256,2461150.9264,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033079164168192256 20260420.4264 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.29 16:44:34.89 -24:54:56.8
355.41634 13.42703 galactic Sco Second-epoch detections are separated by 6.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6046943421654417920 | 16:44:36.25 -24:54:28.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6046943421654417920,2461150.9264,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6046943421654417920 20260420.4264 11.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032090733247694592,2461150.9264,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032090733247694592 20260420.4264 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6039956540659158528,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6039956540659158528 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044844557036772608,2461150.9264,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044844557036772608 20260420.4264 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125849350952428288,2461150.9264,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125849350952428288 20260420.4264 11.23CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6243553658525961728,2461150.9264,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6243553658525961728 20260420.4264 11.15CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164742.55-261354.5,2461150.9264,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164742.55-261354.5 20260420.4264 11.30CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127067236182565760,2461150.9264,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127067236182565760 20260420.4264 11.14CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J245.9869-26.6598,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J245.9869-26.6598 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6047116079340845184,2461150.9264,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6047116079340845184 20260420.4264 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126587363768940928,2461150.9264,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126587363768940928 20260420.4264 11.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202842956,2461150.9264,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 202842956 20260420.4264 11.52CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J241.9544-26.9555,2461150.9264,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J241.9544-26.9555 20260420.4264 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034290138786440704,2461150.9264,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034290138786440704 20260420.4264 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.69 16:48:57.58 -28:48:19.0
352.95036 10.22435 galactic Sco Second-epoch detections are separated by 3.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6032879499698289408 | 16:48:56.10 -28:48:50.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6032879499698289408,2461150.9264,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6032879499698289408 20260420.4264 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125327804478967424,2461150.9264,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125327804478967424 20260420.4264 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6246874664675970560,2461150.9264,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6246874664675970560 20260420.4264 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037507790826859392,2461150.9264,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6037507790826859392 20260420.4264 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032483297567530112,2461150.9264,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032483297567530112 20260420.4264 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032126952732672256,2461150.9264,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032126952732672256 20260420.4264 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046724618851076864,2461150.9264,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046724618851076864 20260420.4264 11.39CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127014493981281792,2461150.9264,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127014493981281792 20260420.4264 11.36CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6242754725885697664,2461150.9264,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6242754725885697664 20260420.4264 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034657233904861056,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034657233904861056 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032703612248385408,2461150.9264,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032703612248385408 20260420.4264 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031536686779817344,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031536686779817344 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030800151435929344,2461150.9264,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030800151435929344 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164248-3019.4,2461150.9264,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164248-3019.4 20260420.4264 11.67CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033929842567706880,2461150.9264,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033929842567706880 20260420.4264 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046838452664720128,2461150.9264,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046838452664720128 20260420.4264 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031161959499553408,2461150.9264,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031161959499553408 20260420.4264 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032856135104192640,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032856135104192640 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125801663939781504,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125801663939781504 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J163912.98-232902.9,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J163912.98-232902.9 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6039853942478154368,2461150.9264,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6039853942478154368 20260420.4264 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165128.68-281401.3,2461150.9264,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165128.68-281401.3 20260420.4264 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030866358328110464,2461150.9264,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030866358328110464 20260420.4264 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034344354125575424,2461150.9264,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034344354125575424 20260420.4264 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164431.45-301334.9,2461150.9264,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164431.45-301334.9 20260420.4264 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041576602319058816,2461150.9264,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6041576602319058816 20260420.4264 11.62CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048614232651012480,2461150.9264,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048614232651012480 20260420.4264 11.53CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6045575693607508352,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6045575693607508352 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031337292902555520,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031337292902555520 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.8353-27.5360,2461150.9264,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J238.8353-27.5360 20260420.4264 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J160330.34-251111.3,2461150.9264,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J160330.34-251111.3 20260420.4264 11.62CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6042803244981775744,2461150.9264,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6042803244981775744 20260420.4264 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037918046102425728,2461150.9264,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6037918046102425728 20260420.4264 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J251.3841-29.3388,2461150.9264,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J251.3841-29.3388 20260420.4264 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J252.9863-21.3759,2461150.9264,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J252.9863-21.3759 20260420.4264 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040708056854371840,2461150.9264,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040708056854371840 20260420.4264 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032904513620246528,2461150.9264,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032904513620246528 20260420.4264 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6246782683656146176,2461150.9264,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6246782683656146176 20260420.4264 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6039934722224930560,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6039934722224930560 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6243521807047350656,2461150.9264,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6243521807047350656 20260420.4264 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.2154-29.8199,2461150.9264,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.2154-29.8199 20260420.4264 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048539534578287360,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048539534578287360 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0942 Sco,2461150.9264,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0942 Sco 20260420.4264 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6246611297280683136,2461150.9264,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6246611297280683136 20260420.4264 11.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126992121486581120,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126992121486581120 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6240790822019689088,2461150.9264,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6240790822019689088 20260420.4264 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.3222-22.2119,2461150.9264,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.3222-22.2119 20260420.4264 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127004426577825664,2461150.9264,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127004426577825664 20260420.4264 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J239.4058-20.6159,2461150.9264,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J239.4058-20.6159 20260420.4264 11.36CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.7552-29.9681,2461150.9264,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J238.7552-29.9681 20260420.4264 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034365558417289344,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034365558417289344 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125298912247836416,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125298912247836416 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032972129255113856,2461150.9264,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032972129255113856 20260420.4264 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 204193529,2461150.9264,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 204193529 20260420.4264 11.62CV 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
Mean magnitude and position on the discovery images:
2026 04 20.4264 2461150.9264 11.82 16:44:36.51 -26:29:54.1
354.15889 12.42572 galactic Sco Second-epoch detections are separated by 7.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6034215921743308288 | 16:44:37.89 -26:30:00.9 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 6034215921743308288,2461150.9264,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 6034215921743308288 20260420.4264 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6038881115208076160,2461150.9264,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6038881115208076160 20260420.4264 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6243008983649511424,2461150.9264,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6243008983649511424 20260420.4264 11.44CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J252.6507-22.3510,2461150.9264,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J252.6507-22.3510 20260420.4264 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202607322,2461150.9264,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 202607322 20260420.4264 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125830281297644032,2461150.9264,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125830281297644032 20260420.4264 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126986108539058432,2461150.9264,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126986108539058432 20260420.4264 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046470696070575744,2461150.9264,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046470696070575744 20260420.4264 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6025494492429646848,2461150.9264,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6025494492429646848 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044623138577197568,2461150.9264,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044623138577197568 20260420.4264 11.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032603178720923648,2461150.9264,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032603178720923648 20260420.4264 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046810208958023424,2461150.9264,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046810208958023424 20260420.4264 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044623138577197568,2461150.9264,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044623138577197568 20260420.4264 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6041190708097530496,2461150.9264,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6041190708097530496 20260420.4264 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4125809497960455552,2461150.9264,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4125809497960455552 20260420.4264 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 203655113,2461150.9264,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 203655113 20260420.4264 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CK Sco,2461150.9264,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CK Sco 20260420.4264 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030795031834597632,2461150.9264,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030795031834597632 20260420.4264 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6038090566344015104,2461150.9264,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6038090566344015104 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037027613487393664,2461150.9264,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6037027613487393664 20260420.4264 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126688454427240448,2461150.9264,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126688454427240448 20260420.4264 11.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4126988376275100544,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4126988376275100544 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J240.8748-28.1202,2461150.9264,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J240.8748-28.1202 20260420.4264 12.09CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6246607930026294528,2461150.9264,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6246607930026294528 20260420.4264 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4127021052386266624,2461150.9264,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4127021052386266624 20260420.4264 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6048045097947992832,2461150.9264,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6048045097947992832 20260420.4264 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J239.8684-28.5778,2461150.9264,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J239.8684-28.5778 20260420.4264 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040896726175962496,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040896726175962496 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.0904-28.4155,2461150.9264,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.0904-28.4155 20260420.4264 11.36CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164836.92-245013.4,2461150.9264,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164836.92-245013.4 20260420.4264 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6246855869898980992,2461150.9264,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6246855869898980992 20260420.4264 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZZ Sco,2461150.9264,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZZ Sco 20260420.4264 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J163913.26-302421.4,2461150.9264,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J163913.26-302421.4 20260420.4264 11.44CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040444788234836480,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040444788234836480 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031311733554619520,2461150.9264,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031311733554619520 20260420.4264 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.0705-28.3285,2461150.9264,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.0705-28.3285 20260420.4264 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046197742307386240,2461150.9264,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046197742307386240 20260420.4264 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6030760706453607168,2461150.9264,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6030760706453607168 20260420.4264 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031147872005817856,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031147872005817856 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 203566940,2461150.9264,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 203566940 20260420.4264 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J238.2149-27.4201,2461150.9264,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J238.2149-27.4201 20260420.4264 11.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164755-2809.5,2461150.9264,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164755-2809.5 20260420.4264 10.89CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J241.7560-28.0375,2461150.9264,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J241.7560-28.0375 20260420.4264 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 203720222,2461150.9264,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 203720222 20260420.4264 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034196336678055424,2461150.9264,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034196336678055424 20260420.4264 11.52CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034646861585145472,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034646861585145472 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034378954384259328,2461150.9264,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034378954384259328 20260420.4264 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6033920050041580032,2461150.9264,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6033920050041580032 20260420.4264 11.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J162319.11-295356.1,2461150.9264,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J162319.11-295356.1 20260420.4264 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032266208433826560,2461150.9264,10.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032266208433826560 20260420.4264 10.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J155700.97-285630.5,2461150.9264,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J155700.97-285630.5 20260420.4264 11.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031119589602675456,2461150.9264,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031119589602675456 20260420.4264 12.20CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044856514226590720,2461150.9264,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044856514226590720 20260420.4264 11.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032914203067481984,2461150.9264,10.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032914203067481984 20260420.4264 10.28CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046705854122196864,2461150.9264,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046705854122196864 20260420.4264 11.53CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.1022-25.9063,2461150.9264,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.1022-25.9063 20260420.4264 10.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6046237157235120000,2461150.9264,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6046237157235120000 20260420.4264 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165308.00-294202.9,2461150.9264,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165308.00-294202.9 20260420.4264 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034178705826271872,2461150.9264,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034178705826271872 20260420.4264 11.43CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.3405-29.8117,2461150.9264,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.3405-29.8117 20260420.4264 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164907.36-272443.3,2461150.9264,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164907.36-272443.3 20260420.4264 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J164948-2257.1,2461150.9264,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J164948-2257.1 20260420.4264 11.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J252.5528-29.7410,2461150.9264,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J252.5528-29.7410 20260420.4264 11.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6040702112619509376,2461150.9264,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6040702112619509376 20260420.4264 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6043114406769759232,2461150.9264,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6043114406769759232 20260420.4264 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032698282139528320,2461150.9264,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032698282139528320 20260420.4264 10.80CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CZ Sco,2461150.9264,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CZ Sco 20260420.4264 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6044614484233409920,2461150.9264,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6044614484233409920 20260420.4264 11.54CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6045718600059051520,2461150.9264,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6045718600059051520 20260420.4264 11.15CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J253.1776-26.6058,2461150.9264,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J253.1776-26.6058 20260420.4264 11.20CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J165253-2929.9,2461150.9264,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165253-2929.9 20260420.4264 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J236.4427-28.8826,2461150.9264,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J236.4427-28.8826 20260420.4264 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J246.8152-26.0183,2461150.9264,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J246.8152-26.0183 20260420.4264 11.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6233081360023848576,2461150.9264,10.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6233081360023848576 20260420.4264 10.09CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6047356253906223616,2461150.9264,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6047356253906223616 20260420.4264 11.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032220067619988096,2461150.9264,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032220067619988096 20260420.4264 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6034766600952894208,2461150.9264,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6034766600952894208 20260420.4264 11.44CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6031424154325514112,2461150.9264,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6031424154325514112 20260420.4264 11.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165242.43-285830.3,2461150.9264,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J165242.43-285830.3 20260420.4264 11.18CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J240.8109-28.4333,2461150.9264,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J240.8109-28.4333 20260420.4264 11.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J237.9585-28.9566,2461150.9264,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J237.9585-28.9566 20260420.4264 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6029572164422743424,2461150.9264,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6029572164422743424 20260420.4264 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6027951797863362944,2461150.9264,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6027951797863362944 20260420.4264 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J242.0224-28.7894,2461150.9264,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J242.0224-28.7894 20260420.4264 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6032057679178881664,2461150.9264,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 6032057679178881664 20260420.4264 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461150.92681596 20.04.2026 10:14:26.899 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 51
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.24
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): 8320
Objects passed selection criteria: 8282
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 5715.25
Average stars matched: 5502.25 (96.2731 %)
Memory usage VmPeak: 114068 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:16:40 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: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461150.92681596 20.04.2026 10:14:26.899 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 778
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.99
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 21 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): 77660
Objects passed selection criteria: 77475
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 51000.5
Average stars matched: 48271 (94.6481 %)
Memory usage VmPeak: 176740 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:19:14 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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: 2461150.92596440
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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
Saving wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits'
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Image size: 941.6'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:16.444 -25:59:35.75 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Image size: 942.0'x627.8' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:19:16.837 -26:00:02.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:16.837 -26:00:02.17
Angular distance between the image centers 0.0075 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Image size: 942.0'x627.8' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:19:14.051 -25:59:55.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:14.051 -25:59:55.32
Angular distance between the image centers 0.0105 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:19:16.837 -26:00:02.17
Second-epoch second image center 16:19:14.051 -25:59:55.32
Angular distance between the image centers 0.01061 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/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.gJL66PewjM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.CKt2Nwj7kA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits &> /tmp/tmp.QkxKHnVUkX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits &> /tmp/tmp.l2eWBFxhKr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat' -> 'wcsmag.cat'
Read 8752 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.6487 to 253.8106 deg, Dec -31.3044 to -20.4499 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 235.6487 to 253.8106 deg, Dec -31.3044 to -20.4499 deg
Loaded 8190 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): 5578 out of 5823 total matches.
Matched with Tycho-2 5823 out of 8752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.802561
a=0.000000 b=1.000000 c=22.802561
From vast_summary.log: estimated ref. image limiting mag.: -8.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.2 pix Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
10.1 pix fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
10.3 pix fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
12.9 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
12.9 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gJL66PewjM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=696, passed=8752
Got 8752 stars (including 8042 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 8752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 349 (Dec -31.3 to -20.4)
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...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8524 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.CKt2Nwj7kA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=689, passed=8852
Got 8852 stars (including 8148 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 8852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.QkxKHnVUkX (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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=653, passed=2896
Got 2896 stars (including 2243 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat
util/solve_plate_with_UCAC5 got 2896 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 2831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.47"
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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.17"
Excluding outliers - 956 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.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.l2eWBFxhKr (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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=728, passed=2998
Got 2998 stars (including 2270 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat
util/solve_plate_with_UCAC5 got 2998 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 2921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.47"
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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 2922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.18"
Excluding outliers - 956 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits'
Preparing the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20747.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 27s
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: 10s
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Considering the candidate 20614_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20614_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 20624_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20624_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20644_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20644_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:15.00 -21:40:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.78, MAG_FAINT_SEARCH_LIMIT=9.76)GAIADR2_OUTPUT=# 3.437 4127001540359719424 253.31341790164 -21.67487696011 7.5751 6.2190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20677_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20677_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 20678_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20678_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20680_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20680_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:01.97 -24:10:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.60, MAG_FAINT_SEARCH_LIMIT=10.58)GAIADR2_OUTPUT=# 5.078 4125326400039294592 253.25972939729 -24.16996984394 8.6065 7.4126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20683_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20683_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20685_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20685_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20688_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20688_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20695_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20695_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20703_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20703_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:39.38 -21:45:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.03, MAG_FAINT_SEARCH_LIMIT=11.01)GAIADR2_OUTPUT=# 3.048 4126993740699126784 253.16498858559 -21.76201743639 9.1964 8.1841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20708_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20708_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:04.61 -22:05:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 0.505 4126231195034615424 253.26930339035 -22.08525205720 9.9454 9.1972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20713_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20713_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 20720_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20720_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20721_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20721_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:51.55 -21:17:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 3.078 4127093864980986240 253.21518572571 -21.29631113180 9.7221 8.8608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20726_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20726_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20728_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20728_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20736_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20736_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20747_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20747_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20748_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20748_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 20755_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20755_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:51.93 -21:17:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.43, MAG_FAINT_SEARCH_LIMIT=11.41)GAIADR2_OUTPUT=# 3.989 4127093864980986240 253.21518572571 -21.29631113180 9.7221 8.8608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20761_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20761_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 04757_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 04757_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 05578_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 05578_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:21:10.99 -25:35:31.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 06622_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 06622_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:20:37.99 -24:10:12.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 04509_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 04509_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:29:23.99 -26:25:52.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 03563_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 03563_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:12:18.47 -27:55:27.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 02916_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 02916_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:18:17.81 -28:36:43.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06022_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 06022_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:30:11.89 -25:06:55.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 04856_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 04856_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:08:08.12 -26:19:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06970_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 06970_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:25:34.66 -23:26:54.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 01791_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 01791_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:24:39.77 -29:42:11.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 05284_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 05284_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:03:20.97 -25:51:53.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 02018_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 02018_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:11:02.10 -29:24:52.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 03269_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 03269_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:35:52.22 -28:12:48.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 00374_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 00374_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:19:32.64 -30:54:14.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 05009_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 05009_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:58:51.79 -26:06:45.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 05631_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 05631_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:53:37.18 -25:19:36.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 05250_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 05250_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:50:59.22 -25:45:03.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 02052_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 02052_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:56:53.51 -29:12:43.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 08272_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 08272_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:07:24.60 -20:52:13.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 07316_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 07316_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:00:20.45 -22:37:21.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08675_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 08675_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:32:07.89 -21:28:01.5 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 38s
Prepared the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:23:35.43 -26:31:39.8
16:53:24.81 -30:14:14.2
16:48:58.98 -21:22:51.1
16:24:16.86 -31:10:19.4
16:51:56.60 -21:19:44.4
16:46:15.63 -29:09:39.9
16:52:26.43 -28:44:09.7
16:43:46.48 -25:13:34.2
16:50:22.79 -28:32:20.3
16:46:20.11 -27:18:39.2
16:52:38.83 -21:45:47.4
16:07:46.50 -30:41:54.8
16:46:54.25 -30:07:53.2
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits exists and is non-empty
wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Image size: 941.6'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:16.444 -25:59:35.75 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Image size: 942.0'x627.8' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:19:16.837 -26:00:02.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:16.837 -26:00:02.17
Angular distance between the image centers 0.0075 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Image size: 942.0'x627.8' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 16:19:14.051 -25:59:55.32 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:14.051 -25:59:55.32
Angular distance between the image centers 0.0105 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:19:16.837 -26:00:02.17
Second-epoch second image center 16:19:14.051 -25:59:55.32
Angular distance between the image centers 0.01061 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/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.BaKZZ0vS00
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.ev04hgFMmC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits &> /tmp/tmp.7Sqxkle0nv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits &> /tmp/tmp.RGQ8x0TqXn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat' -> 'wcsmag.cat'
Read 85371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.5879 to 253.8599 deg, Dec -31.3044 to -20.3796 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 235.5879 to 253.8599 deg, Dec -31.3044 to -20.3796 deg
Loaded 8263 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): 6163 out of 6991 total matches.
Matched with Tycho-2 6991 out of 85371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.625106
a=0.000000 b=1.000000 c=22.625106
From vast_summary.log: estimated ref. image limiting mag.: -7.99
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.64
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 652 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.0 pix Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
4.2 pix fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
4.3 pix fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.6 mag. Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
12.9 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
13.0 mag. fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BaKZZ0vS00 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=4769, passed=85362
Got 85362 stars (including 80423 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 85362 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.ev04hgFMmC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=4773, passed=84608
Got 84608 stars (including 79674 good ones) from the SExtractor catalog wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 84608 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.7Sqxkle0nv (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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=5228, passed=18566
Got 18566 stars (including 13329 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat
util/solve_plate_with_UCAC5 got 18566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 18064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.34"
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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 18062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.32"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 18062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.13"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.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.RGQ8x0TqXn (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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Checking if the catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat corresponding to the image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
WCS catalog name: wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=5504, passed=19170
Got 19170 stars (including 13653 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat
util/solve_plate_with_UCAC5 got 19170 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 18575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 18573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.35"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 18573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits -region wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_Sco-02-Q1b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Saving fully-calibrated image wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_Sco-02-Q1b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-13-13_20.00sec_-4.90C_LIGHTs_0010.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.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_2026-04-20_CI_Sco-02-Q1b1x1_051528_TTUQ1b1x1_1645701_dsXLw9X4/wcs_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011.fits
Preparing the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out103006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103261.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103513.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103554.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103590.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103613.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103651.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103777.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103852.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103895.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103956.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103978.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out103992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104106.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out104110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104240.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out104351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104360.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out104406.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out41124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out01694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out01750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102994.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out103803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95817.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 497s
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: 218s
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Considering the candidate 102992_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 102992_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102993_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 102993_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102994_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 102994_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102995_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 102995_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103001_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103001_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103002_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103002_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103006_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103006_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:06:28.19 -26:21:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 4.864 6043392342695597696 241.61779721741 -26.36478870460 12.0818 11.6150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103010_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103010_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103014_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103014_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103017_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103017_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103018_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103018_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:26:58.11 -27:52:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 4.499 6045098746079988224 246.74118476748 -27.87217800012 11.6281 10.9646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103021_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103021_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103022_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103022_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103027_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103027_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103029_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103029_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:49:07.57 -29:34:14.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)
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Considering the candidate 103036_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103036_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:54:45.70 -21:01:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 3.126 6246809724770512640 238.68959533054 -21.01928676504 11.8782 11.0906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103040_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103040_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103041_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103041_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:17:01.66 -28:33:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.492 6039108641087769984 244.25735509446 -28.55164695968 11.6586 10.8360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103044_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103044_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:16:30.86 -26:16:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.443 6048629728885464576 244.12824986152 -26.27309428640 10.8539 9.9036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103062_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103062_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103070_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103070_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103079_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103079_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103084_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103084_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103088_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103088_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:50:39.61 -21:00:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.856 6240854838509809152 237.66413552622 -21.00253255696 11.5911 10.7148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103089_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103089_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 103091_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103091_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103099_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103099_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103102_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103102_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:43:40.12 -28:24:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 4.555 6233331769498012416 235.91859489466 -28.40053941609 12.1553 11.6683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103104_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103104_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103108_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103108_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103109_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103109_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103110_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103110_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:10.30 -29:41:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103112_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103112_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 103113_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103113_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:55:51.63 -21:48:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.606 6246499215808200832 238.96495709498 -21.80910981355 11.5294 11.0548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103115_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103115_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103119_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103119_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:56:10.09 -29:10:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103124_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103124_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:53:29.33 -21:49:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.952 6240553331809309312 238.37186075847 -21.82942519140 11.2937 10.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103132_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103132_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103135_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103135_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103137_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103137_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 103138_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103138_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103141_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103141_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 103147_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103147_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103149_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103149_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103152_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103152_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 103153_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103153_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:04.71 -21:26:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.678 6240815084296134144 237.01941157969 -21.43742163912 11.6036 10.7767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103154_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103154_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103155_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103155_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103158_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103158_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:09.86 -29:36:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103162_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103162_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103166_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103166_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 103168_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103168_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103169_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103169_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103170_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103170_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103173_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103173_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103174_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103174_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:46:33.15 -23:01:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.654 6239983200668646912 236.63776798911 -23.02720648806 11.5698 10.9614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103177_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103177_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:40.25 -30:05:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103178_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103178_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103182_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103182_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:50:10.89 -21:11:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 3.827 6240834325744385664 237.54479216028 -21.18414178094 11.7024 11.1291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103184_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103184_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103185_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103185_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103186_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103186_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103187_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103187_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:45:51.80 -25:41:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 4.152 6235102704773499136 236.46459803174 -25.68635704008 11.4669 10.9039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103189_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103189_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103198_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103198_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103199_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103199_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103202_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103202_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103208_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103208_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103210_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103210_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103211_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103211_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:49:04.08 -29:22:29.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)
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Considering the candidate 103214_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103214_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103216_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103216_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103218_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103218_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103219_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103219_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103224_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103224_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:34:24.46 -26:26:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 3.767 6044916334531889536 248.60097609346 -26.43984320913 11.3646 10.6449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103226_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103226_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:44:38.60 -27:36:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 4.853 6033993030111038336 251.16230645238 -27.61236402157 10.8607 10.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103229_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103229_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:04.40 -28:35:12.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)
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Considering the candidate 103236_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103236_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103238_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103238_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103242_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103242_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103245_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103245_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103247_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103247_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:44:28.62 -24:12:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 2.932 6047049352732073472 251.12014277583 -24.20673653802 10.4189 9.6131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103248_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103248_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103249_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103249_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103250_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103250_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103252_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103252_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 103253_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103253_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103255_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103255_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103258_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103258_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103261_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103261_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:50:18.85 -23:00:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 1.807 6240320475863184256 237.57816494956 -23.00727579993 11.2532 10.5271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103262_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103262_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103263_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103263_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103264_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103264_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103267_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103267_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103271_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103271_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:09.66 -21:32:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.713 6240717124679730560 237.03951652254 -21.54334679564 11.1865 10.2014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103273_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103273_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 103274_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103274_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 103277_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103277_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103279_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103279_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 103280_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103280_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103282_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103282_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103284_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103284_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103286_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103286_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103288_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103288_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103296_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103296_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103297_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103297_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:47:50.82 -24:26:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 5.896 6236753247823187584 236.95996211474 -24.44098609992 10.2342 8.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103299_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103299_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103303_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103303_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 103308_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103308_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103316_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103316_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:24.02 -30:01:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103321_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103321_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 103324_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103324_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:57:54.46 -21:35:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 3.560 6246530345736828288 239.47607361183 -21.59081385668 11.4035 10.8219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103327_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103327_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103328_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103328_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 103329_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103329_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103332_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103332_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:51:56.01 -21:22:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.897 6240778181937372544 237.98265209336 -21.37914252528 11.2174 10.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103334_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103334_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103339_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103339_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:33.48 -30:25:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103341_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103341_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:48:54.43 -30:04:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103344_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103344_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:43:04.95 -28:42:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103346_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103346_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103347_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103347_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103348_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103348_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 103350_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103350_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:30.81 -27:09:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103354_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103354_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103355_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103355_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103356_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103356_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103359_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103359_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103362_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103362_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:52:43.86 -22:06:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 4.998 6240521789569193984 238.18140685480 -22.10096788518 10.9899 10.2331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103363_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103363_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103364_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103364_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 103366_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103366_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:19.56 -30:34:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103373_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103373_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103374_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103374_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103375_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103375_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 103379_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103379_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103380_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103380_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103382_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103382_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103387_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103387_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:41:09.27 -24:25:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 0.967 6047778225851639424 250.28885807833 -24.42616886654 9.8744 8.7590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103390_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103390_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103392_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103392_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:01.35 -28:49:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103396_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103396_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103400_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103400_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:48:47.84 -29:01:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103404_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103404_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 103408_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103408_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103409_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103409_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103412_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103412_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103421_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103421_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:08.57 -31:01:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103422_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103422_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:03.79 -30:55:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103424_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103424_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103430_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103430_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:49:34.79 -21:51:10.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 103440_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103440_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:02.33 -22:54:33.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 103442_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103442_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:30.65 -21:39:18.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 103453_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103453_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:48:13.91 -21:24:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.41, MAG_FAINT_SEARCH_LIMIT=9.39)GAIADR2_OUTPUT=# 0.667 4126889115290261120 252.05815455843 -21.41519190783 8.1949 7.2062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103454_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103454_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:14.96 -21:40:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.47, MAG_FAINT_SEARCH_LIMIT=9.45)GAIADR2_OUTPUT=# 4.609 4127001540359719424 253.31341790164 -21.67487696011 7.5751 6.2190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103456_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103456_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:49:00.20 -21:22:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.48, MAG_FAINT_SEARCH_LIMIT=9.46)GAIADR2_OUTPUT=# 4.091 4126895952878763776 252.24977896956 -21.37857220613 8.3926 7.4575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103463_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103463_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 103466_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103466_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 103467_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103467_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:23:35.98 -26:31:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103472_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103472_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:32.18 -24:25:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.15, MAG_FAINT_SEARCH_LIMIT=10.13)GAIADR2_OUTPUT=# 1.805 4113296952570601600 253.38357617548 -24.42013799673 9.0821 8.4041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103474_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103474_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:41.96 -24:56:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.21, MAG_FAINT_SEARCH_LIMIT=10.19)GAIADR2_OUTPUT=# 4.134 6034800277818832256 253.42609624197 -24.94088666096 8.1823 6.8343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103476_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103476_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:52.76 -22:12:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.14, MAG_FAINT_SEARCH_LIMIT=10.12)GAIADR2_OUTPUT=# 1.068 4126604096961519488 252.71993845242 -22.20585872899 9.2706 8.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103478_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103478_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:56.48 -21:19:47.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103479_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103479_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:02.69 -21:57:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.13, MAG_FAINT_SEARCH_LIMIT=10.11)GAIADR2_OUTPUT=# 3.547 4126623170921689600 252.51034355628 -21.96393337074 9.1035 8.2575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103483_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103483_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:02.28 -24:10:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.32, MAG_FAINT_SEARCH_LIMIT=10.30)GAIADR2_OUTPUT=# 0.814 4125326400039294592 253.25972939729 -24.16996984394 8.6065 7.4126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103487_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103487_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:39.54 -21:45:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.24, MAG_FAINT_SEARCH_LIMIT=10.22)GAIADR2_OUTPUT=# 0.800 4126993740699126784 253.16498858559 -21.76201743639 9.1964 8.1841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103493_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103493_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103497_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103497_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:09.08 -22:08:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.43, MAG_FAINT_SEARCH_LIMIT=10.41)GAIADR2_OUTPUT=# 1.005 4126605883667911424 252.78804597455 -22.14327449663 9.4068 8.5810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103499_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103499_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:24.91 -23:03:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.48, MAG_FAINT_SEARCH_LIMIT=10.46)GAIADR2_OUTPUT=# 1.687 4125694736432784000 252.60425234805 -23.06332812914 9.2788 8.4189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103503_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103503_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:22.54 -22:38:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.54, MAG_FAINT_SEARCH_LIMIT=10.52)GAIADR2_OUTPUT=# 0.519 4125814136525201152 252.59377880774 -22.63757081802 9.5657 8.8167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103506_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103506_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:44.32 -23:54:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.63, MAG_FAINT_SEARCH_LIMIT=10.61)GAIADR2_OUTPUT=# 3.703 4125383505927935232 252.93570540338 -23.90241037212 9.4433 8.5773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103507_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103507_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 103513_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103513_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:42.30 -21:43:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.63, MAG_FAINT_SEARCH_LIMIT=10.61)GAIADR2_OUTPUT=# 0.278 4127000402183524864 253.17625107717 -21.73085511241 9.8438 9.0498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103515_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103515_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:04.92 -22:05:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.71, MAG_FAINT_SEARCH_LIMIT=10.69)GAIADR2_OUTPUT=# 3.993 4126231195034615424 253.26930339035 -22.08525205720 9.9454 9.1972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103525_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103525_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 103528_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103528_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:46:54.40 -30:07:54.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103529_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103529_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:43:46.50 -25:13:36.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103538_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103538_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 103545_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103545_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:51.07 -23:18:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.96, MAG_FAINT_SEARCH_LIMIT=10.94)GAIADR2_OUTPUT=# 3.565 4125532008719318144 253.21174335338 -23.30714902303 10.0953 9.6264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103554_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103554_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:27.82 -24:21:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.05, MAG_FAINT_SEARCH_LIMIT=11.03)GAIADR2_OUTPUT=# 2.518 4125305573728248064 253.11667707219 -24.36262445936 9.1991 8.0172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103558_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103558_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 103566_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103566_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103567_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103567_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103569_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103569_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 103572_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103572_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:56.86 -23:34:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.18, MAG_FAINT_SEARCH_LIMIT=11.16)GAIADR2_OUTPUT=# 2.696 4125427653881549184 252.98618160624 -23.57399367137 10.2517 9.7120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103579_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103579_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103586_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103586_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 103590_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103590_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:32.52 -22:19:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.23, MAG_FAINT_SEARCH_LIMIT=11.21)GAIADR2_OUTPUT=# 0.689 4126576407316316160 252.63565668622 -22.33254156527 10.1914 9.3417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103593_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103593_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:48:53.91 -21:37:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.19, MAG_FAINT_SEARCH_LIMIT=11.17)GAIADR2_OUTPUT=# 5.779 4126694879698349568 252.22633745422 -21.62707160384 9.5863 8.3655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103595_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103595_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 103602_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103602_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:26.40 -23:43:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.33, MAG_FAINT_SEARCH_LIMIT=11.31)GAIADR2_OUTPUT=# 4.101 4125412295079664384 253.35879713761 -23.73359740771 10.1488 9.1473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103604_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103604_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 103608_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103608_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103613_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103613_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:23.53 -22:09:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 1.924 4125858288790594688 253.09749067962 -22.15115891537 10.6014 10.0224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103628_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103628_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:57.70 -21:32:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 5.423 4127018307912322944 252.98899974336 -21.54367420110 10.6975 10.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103636_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103636_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103638_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103638_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 103639_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103639_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103646_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103646_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:44.25 -24:26:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)GAIADR2_OUTPUT=# 0.517 4125301008192076800 253.18438529111 -24.43527329592 10.6716 10.2903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103651_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103651_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:47:27.27 -22:08:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 5.337 4126652200594182144 251.86512098810 -22.14530627195 10.7494 10.2563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103652_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103652_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103662_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103662_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103664_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103664_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103666_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103666_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:00.56 -23:15:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 4.790 4125629899604061952 253.00099944321 -23.25887949127 10.6041 9.9260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103671_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103671_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103673_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103673_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:41.12 -21:07:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 5.153 6241576732315374848 237.17007848108 -21.11670376471 10.4292 9.6695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103674_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103674_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103679_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103679_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103681_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103681_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:50.92 -21:27:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.50, MAG_FAINT_SEARCH_LIMIT=11.48)GAIADR2_OUTPUT=# 1.741 4127066166722746368 252.96190385876 -21.46216715949 10.8580 10.2650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103684_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103684_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103688_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103688_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:05.92 -22:36:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.57, MAG_FAINT_SEARCH_LIMIT=11.55)GAIADR2_OUTPUT=# 1.195 4125813926058704896 252.52487582358 -22.61202012439 10.6698 9.8652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103700_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103700_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103706_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103706_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:40.95 -22:03:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.67, MAG_FAINT_SEARCH_LIMIT=11.65)GAIADR2_OUTPUT=# 2.682 4126609903757294208 252.92141202450 -22.05143231487 10.7183 9.8807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103708_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103708_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103709_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103709_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103714_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103714_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103717_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103717_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:58.89 -21:55:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.56, MAG_FAINT_SEARCH_LIMIT=11.54)GAIADR2_OUTPUT=# 3.348 4126615435675162880 252.99440365199 -21.93056336080 10.9180 10.5366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103723_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103723_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103724_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103724_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103726_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103726_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 103728_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103728_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 103738_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103738_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:41.11 -23:59:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 3.503 4125352857039581312 253.42036851184 -23.99693003560 10.2919 9.2171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103739_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103739_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103741_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103741_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103743_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103743_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 103747_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103747_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:25.36 -22:10:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103752_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103752_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103755_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103755_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:52.10 -21:21:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 5.057 4127072012186226048 252.96571293603 -21.35644817688 11.1399 10.8297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103757_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103757_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103758_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103758_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:41.34 -24:52:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 3.136 6034813815556252416 252.92314018434 -24.87409007886 10.9882 10.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103765_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103765_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:36.90 -26:46:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103773_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103773_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 103776_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103776_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 103777_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103777_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:15.23 -23:21:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 2.683 4125625153657586560 253.06388706811 -23.35347836741 11.2102 10.6234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103779_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103779_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:08.23 -25:24:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.255 6034715615417470208 253.03492461319 -25.40145009150 10.6434 9.8173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103780_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103780_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:03.64 -22:03:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 0.627 4126607636014563072 252.76535030752 -22.06165791199 10.9055 10.0424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103782_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103782_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103783_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103783_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:51.68 -22:18:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.76, MAG_FAINT_SEARCH_LIMIT=11.74)GAIADR2_OUTPUT=# 0.626 4125849350952428288 252.96514733924 -22.31380291112 11.0429 10.5485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103784_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103784_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:27.27 -21:43:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 1.302 4126680341220932736 252.61333852114 -21.72643929449 11.1113 10.7605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103790_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103790_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:23.46 -22:08:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.70, MAG_FAINT_SEARCH_LIMIT=11.68)GAIADR2_OUTPUT=# 1.651 4126218447571569536 253.34760670749 -22.14603322875 11.0200 10.4027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103797_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103797_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103799_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103799_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103802_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103802_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103803_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103803_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103804_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103804_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 103808_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103808_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 103809_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103809_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103810_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103810_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:13.95 -21:32:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 2.284 4127027134059966080 253.30772306730 -21.54029029069 11.1286 10.5404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103813_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103813_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103820_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103820_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103821_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103821_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 103822_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103822_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:47:35.06 -22:13:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 5.491 4126546166446713344 251.89767527651 -22.21738457575 11.0852 10.5067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103823_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103823_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:44.88 -21:24:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 2.506 4127067236182565760 252.93639846587 -21.41502464025 10.7595 9.7801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103827_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103827_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103836_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103836_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103841_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103841_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103846_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103846_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103849_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103849_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 103852_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103852_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:08.05 -23:06:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 1.672 4125688311161692800 252.53304851264 -23.11454416872 10.7450 9.8645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103854_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103854_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:05.66 -25:04:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 3.276 6034794745901144320 253.02425102093 -25.06779231755 10.1661 8.9537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103855_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103855_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:49:47.52 -23:59:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 1.191 4125390790192264960 252.44835091109 -23.99355387477 10.7234 9.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103858_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103858_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103864_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103864_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 103869_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103869_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 103871_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103871_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103872_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103872_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103875_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103875_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103878_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103878_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103881_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103881_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:01.38 -25:12:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 2.911 6034743343728751872 253.25632938606 -25.20324556246 10.2431 9.2745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103884_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103884_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:51.22 -21:04:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 5.301 6241578385877828224 237.21197028203 -21.07252220588 11.0172 10.3571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103889_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103889_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103893_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103893_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103895_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103895_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:20.10 -21:32:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 5.648 4127017655077244416 253.08538443775 -21.54258193251 10.8048 10.2654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103896_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103896_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:34.46 -21:27:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 4.660 4127066686426737792 252.89227118503 -21.46395682743 10.9391 10.0464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103897_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103897_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:53.12 -22:36:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 2.893 4125817400700271232 252.72207165193 -22.61171310274 11.2441 10.7901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103898_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103898_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103899_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103899_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103900_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103900_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103901_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103901_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103902_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103902_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 103905_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103905_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103907_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103907_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:34.08 -24:24:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 2.497 4125304100568556800 253.14224170051 -24.41099117022 10.9361 9.9445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103909_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103909_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103912_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103912_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 103923_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103923_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 103926_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103926_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103929_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103929_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:04.82 -21:29:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 0.729 4126700132430226816 252.52000993167 -21.49138517746 11.0229 10.4477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103930_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103930_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103932_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103932_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 103938_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103938_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:04.66 -25:13:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 2.444 6034743270693278464 253.26975845262 -25.22527107073 10.9015 10.3164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103943_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103943_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 103944_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103944_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:11.55 -23:02:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 5.526 4125739301011635712 253.04913627134 -23.04730414104 11.2733 10.7060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103945_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103945_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 103946_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103946_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:30.61 -23:31:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 5.387 4125513072193453440 253.37592285080 -23.51736622667 10.8598 9.8781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103948_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103948_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103951_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103951_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:59.06 -21:28:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 1.318 4127065857485102336 252.99569308791 -21.48300876294 11.1914 10.6261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103952_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103952_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103953_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103953_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:22.37 -22:18:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 2.267 4125840971482348416 253.34254609344 -22.30388234672 11.1327 10.2204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103954_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103954_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 103955_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103955_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103956_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103956_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:21.51 -24:12:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.023 4125313515137390336 253.33942159935 -24.21117359077 11.4080 10.9212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103959_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103959_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:03.57 -22:43:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 1.045 4125798193593559296 252.76458428005 -22.72124982904 11.1399 10.2912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103963_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103963_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103969_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103969_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:49:09.82 -22:16:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 3.662 4126588742462623744 252.29194706140 -22.28113196194 11.3654 10.7432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103972_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103972_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103975_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103975_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103978_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103978_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:56.91 -21:23:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 1.503 4127044112076984704 253.23757099103 -21.39904293532 11.0825 10.2011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103980_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103980_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103981_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103981_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 103982_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103982_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:49:21.52 -22:34:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 4.278 4126568332777777408 252.34034677026 -22.56913004621 11.0815 10.1270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103989_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103989_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103992_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103992_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:48:07.14 -23:14:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 3.898 4125676796341393024 252.03080221855 -23.23881803225 10.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103996_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 103996_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 103999_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 103999_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 104002_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104002_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104007_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104007_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:07.60 -23:51:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 3.688 4125407312916436864 253.03271076910 -23.85360094948 10.6865 9.8131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104008_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104008_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104011_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104011_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104014_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104014_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104017_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104017_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104020_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104020_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104029_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104029_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104030_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104030_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104031_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104031_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104034_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104034_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 104035_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104035_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:11.07 -22:37:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 2.513 4125816472987254784 252.79688048142 -22.62347718585 11.1953 10.5846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104039_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104039_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 104048_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104048_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104049_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104049_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104050_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104050_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104051_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104051_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104054_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104054_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104058_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104058_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 104060_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104060_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104061_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104061_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104064_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104064_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104066_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104066_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104069_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104069_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104071_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104071_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 104072_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104072_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104073_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104073_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 104077_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104077_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104083_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104083_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 104085_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104085_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:09.71 -22:25:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.506 4125835095967055232 253.28970589356 -22.42608551529 11.0536 10.1018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104087_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104087_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104089_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104089_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104091_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104091_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 104096_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104096_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104099_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104099_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104100_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104100_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:03.69 -22:27:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 3.654 4125831453834671872 253.01513373120 -22.46048193789 10.9740 10.1710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104101_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104101_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104103_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104103_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104104_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104104_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104106_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104106_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:48:23.49 -22:07:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 5.796 4126641480356859520 252.09960107136 -22.12386674830 10.9308 9.8565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104107_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104107_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:21.85 -22:18:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 5.404 4125840971482348416 253.34254609344 -22.30388234672 11.1327 10.2204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104110_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104110_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:04.87 -21:22:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.461 4127068748011032448 253.02057933631 -21.37755498595 11.2337 10.3998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104111_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104111_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 104113_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104113_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:05.59 -22:36:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 5.315 4125813926058704896 252.52487582358 -22.61202012439 10.6698 9.8652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104122_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104122_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104126_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104126_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104134_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104134_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 104136_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104136_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 104137_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104137_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:47:06.98 -21:46:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 3.043 4126852968845384576 251.77952694189 -21.76698400018 11.3404 10.7107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104143_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104143_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:09.25 -21:49:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.444 4126632276252467840 252.78821463636 -21.82020662740 11.2878 10.4821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104145_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104145_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104157_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104157_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 104158_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104158_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 104159_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104159_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:34.50 -22:31:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 1.300 4125828597670464512 253.14413797625 -22.52443303922 11.5321 11.1548 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 104162_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104162_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104166_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104166_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 104167_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104167_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104169_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104169_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 104170_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104170_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:31.77 -25:19:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 2.450 6034738155407974784 253.38310686901 -25.31802068550 10.9343 9.9386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104171_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104171_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104178_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104178_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:35.98 -23:09:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 3.186 4125723083215048576 253.14904075128 -23.15524440793 11.3923 10.3786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104179_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104179_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104185_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104185_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:44.91 -21:55:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 0.165 4126616195894872320 252.93714482843 -21.93098591630 11.3915 10.5683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104186_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104186_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:49:58.17 -21:27:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104188_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104188_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104196_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104196_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104198_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104198_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 104200_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104200_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104203_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104203_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:10.82 -22:32:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 5.044 4125780910656569600 253.29361653019 -22.53944027998 11.1974 10.2795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104204_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104204_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:33.78 -21:27:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 5.359 4127066686426737792 252.89227118503 -21.46395682743 10.9391 10.0464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104207_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104207_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 104214_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104214_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:00.20 -23:07:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 2.028 4125722739617641984 253.25040142493 -23.12256605925 11.0585 10.0224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104220_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104220_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104221_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104221_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:58.93 -21:17:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 1.284 4127084416051935616 252.74561070356 -21.28312149042 11.0655 10.0296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104222_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104222_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104223_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104223_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104228_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104228_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:06.15 -21:46:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 3.910 4127004426577825664 253.02463553847 -21.77857887035 11.4014 10.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104232_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104232_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 104233_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104233_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104237_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104237_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104240_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104240_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:46:45.86 -21:41:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.931 4126866162985029248 251.69175841026 -21.68286983009 10.8994 9.8504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104244_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104244_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104249_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104249_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 104250_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104250_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104251_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104251_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 104252_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104252_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104255_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104255_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 104256_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104256_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104259_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104259_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104262_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104262_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 104266_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104266_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 104267_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104267_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 104270_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104270_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:08.97 -23:08:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 1.896 4125725518451897728 253.03731902398 -23.14603142169 11.0603 10.0103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104272_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104272_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104274_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104274_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 104278_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104278_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:41.43 -22:07:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 1.819 4126605608790003072 252.67217447388 -22.12417352475 11.4794 10.6887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104281_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104281_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 104288_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104288_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104293_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104293_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:07.19 -21:48:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 1.356 4126992572468063616 253.02956631630 -21.81145816455 11.3231 10.4801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104294_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104294_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104295_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104295_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104296_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104296_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 104298_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104298_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:53.16 -22:12:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 1.668 4125854062530054912 253.22113695044 -22.20329097820 11.5005 10.6702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104316_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104316_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104318_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104318_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:10.12 -21:42:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.696 4127009541880624256 252.79083670616 -21.70752905994 11.6996 11.1646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104319_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104319_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104322_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104322_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:19.08 -22:04:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 3.815 4125859628820417024 253.07873025661 -22.07018846516 11.7990 11.1751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104325_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104325_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:38:35.21 -21:17:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 5.656 4130083299648049152 249.64838244105 -21.29508959868 10.6323 9.5936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104333_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104333_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104339_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104339_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104349_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104349_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 104351_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104351_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:11.66 -21:57:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 2.166 4126626293352489728 252.79804249055 -21.95791549152 11.5316 10.7077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104353_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104353_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104354_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104354_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 104357_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104357_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104360_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104360_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:07.91 -22:24:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.626 4125824508861593600 252.78278708356 -22.41261746336 11.4338 10.6287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104361_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104361_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104362_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104362_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104363_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104363_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 104367_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104367_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104370_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104370_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104371_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104371_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104377_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104377_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104380_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104380_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:46.72 -21:37:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 2.253 4127010817489321728 252.94399372896 -21.63285256134 11.3178 10.4864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104384_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104384_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 104398_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104398_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104399_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104399_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104406_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104406_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:07.14 -22:48:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 1.773 4125796544338834304 252.78025892954 -22.80137189688 11.1568 10.3949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104409_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104409_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:03.71 -21:26:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 3.263 4127078501875526656 252.51475257542 -21.44126339070 11.6913 11.4625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104419_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104419_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 104429_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104429_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104431_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104431_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:01.46 -21:36:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.985 4127003017828792064 253.25463061713 -21.61469414480 11.7152 11.1380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104432_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104432_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 104436_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104436_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 104439_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104439_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:04.52 -21:18:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 4.621 4127072561942044544 253.01761825465 -21.31204968666 11.7239 11.1528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104440_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104440_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 104443_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104443_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104448_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104448_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 104450_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104450_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104451_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104451_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104452_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104452_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104453_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104453_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104456_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104456_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:36.49 -22:46:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 3.079 4125796265153191808 252.65291982476 -22.78058592535 10.5718 9.2779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104458_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104458_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104461_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104461_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104463_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104463_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 104467_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104467_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104469_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104469_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104471_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104471_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104472_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104472_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:58.36 -21:21:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 4.770 4127045069843379968 253.24225480122 -21.35385027206 11.7329 11.1657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104480_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104480_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104482_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104482_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 104486_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104486_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104489_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104489_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 104490_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104490_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104492_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104492_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104496_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104496_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104501_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104501_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104504_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104504_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104506_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104506_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104508_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104508_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104510_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104510_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104514_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104514_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 104519_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104519_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104523_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104523_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104527_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104527_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:18.09 -22:30:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 4.551 4125830281297644032 253.07403412069 -22.50955731548 11.5554 10.7172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104528_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104528_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:37.90 -21:49:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 4.889 4126992877400825472 253.15662630483 -21.83216784813 11.6852 11.0811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104532_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104532_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:14.72 -22:00:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 3.630 4126236280276113664 253.31034741514 -22.00156468747 11.4176 10.4999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104533_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104533_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:44.25 -21:14:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 3.873 4127085751778680448 252.93336100934 -21.23606936918 11.7510 11.1510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104544_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104544_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 104545_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104545_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104546_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104546_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104552_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104552_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 104553_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104553_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 104557_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104557_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 104571_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104571_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104572_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104572_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 104573_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104573_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104576_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104576_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 104578_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104578_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 104580_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104580_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:18.86 -20:35:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 3.947 6241675245984215040 237.07742495178 -20.59714312169 11.6976 10.9077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104585_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104585_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104588_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104588_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104590_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104590_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104593_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104593_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104595_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104595_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104604_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104604_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104605_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104605_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 104612_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104612_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104615_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104615_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 104622_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104622_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:51:45.89 -21:30:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 5.028 4127065380756623616 252.94070614732 -21.51112186126 11.8557 11.0765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104625_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104625_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104630_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104630_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104633_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104633_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104636_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104636_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 104637_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104637_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104643_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104643_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104654_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104654_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104659_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104659_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104660_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104660_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 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 104672_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104672_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104673_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104673_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104686_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104686_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 104688_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104688_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 104692_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104692_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104706_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104706_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104713_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104713_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104714_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104714_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104720_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104720_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104745_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104745_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104775_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104775_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104801_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104801_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104827_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104827_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 104865_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104865_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 104875_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104875_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 104894_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104894_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 104907_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 104907_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 104911_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 104911_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 13060_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 13060_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 25052_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 25052_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 72954_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 72954_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 61209_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 61209_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 27226_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 27226_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 26638_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 26638_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:38:12.80 -28:34:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26595_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 26595_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 37457_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 37457_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 08395_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 08395_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 22210_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 22210_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 26077_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 26077_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:52:34.82 -28:33:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13957_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 13957_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 28287_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 28287_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 47527_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 47527_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 12444_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 12444_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:55:39.68 -29:47:51.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)
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Considering the candidate 09796_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 09796_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:46:39.76 -29:52:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01694_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 01694_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 14266_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 14266_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 52385_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 52385_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 35377_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 35377_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 30225_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 30225_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 31358_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 31358_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 57086_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 57086_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 33479_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 33479_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:31:41.14 -27:54:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28999_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 28999_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:24:09.31 -28:22:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14582_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 14582_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:53:14.10 -29:40:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43467_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 43467_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 53054_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 53054_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 47897_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 47897_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 37577_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 37577_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 13918_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 13918_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 57034_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 57034_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:50:55.76 -25:10:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28705_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 28705_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 21315_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 21315_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 12879_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 12879_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 32189_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 32189_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 43860_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 43860_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 26227_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 26227_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 57483_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 57483_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 50966_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 50966_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 14833_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 14833_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:46:02.09 -29:43:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48123_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 48123_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 14192_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 14192_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 44834_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 44834_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 13178_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 13178_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 37099_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 37099_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 69689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 69689_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 14446_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 14446_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 11614_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 11614_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 40086_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 40086_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 68519_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 68519_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 21597_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 21597_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 67931_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 67931_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:03:35.39 -22:41:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01750_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 01750_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 95817_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 95817_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 95803_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 95803_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 44236_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 44236_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 95793_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 95793_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:21.82 -20:34:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 5.758 6241675585282641664 237.08938048392 -20.57291104806 12.0093 11.1522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 16594_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 16594_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 95679_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 95679_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 95610_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 95610_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 95591_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 95591_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 58822_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 58822_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 41124_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 41124_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:57:34.39 -26:50:43.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)
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Considering the candidate 69181_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 69181_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:17:40.76 -22:53:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22985_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 22985_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 55654_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 55654_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 21875_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 21875_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 21677_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 21677_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 27133_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 27133_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20389_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 20389_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 66847_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 66847_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 12820_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 12820_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 01708_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 01708_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 20449_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 20449_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:46:15.47 -29:09:41.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 78893_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 78893_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 24054_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 24054_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 19032_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
Preparing report for the candidate 19032_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
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Considering the candidate 52768_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 52768_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:21:11.02 -25:35:31.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 54378_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 54378_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:14:53.47 -25:28:37.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 81135_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 81135_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:20:37.94 -24:10:12.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 42152_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 42152_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:29:23.96 -26:25:53.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 45130_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 45130_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:31:22.72 -26:32:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 57619_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 57619_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:30:11.95 -25:06:54.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 24915_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 24915_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:18:17.83 -28:36:44.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31742_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 31742_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:12:18.47 -27:55:27.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45724_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 45724_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:08:08.11 -26:19:33.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 27338_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 27338_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:12:16.11 -28:25:00.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 07372_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 07372_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:45:46.34 -30:02:29.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 73423_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 73423_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:25:34.66 -23:26:53.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 59377_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 59377_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:03:54.74 -24:43:34.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77383_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 77383_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:08:43.67 -23:41:08.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 49830_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 49830_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:03:20.93 -25:51:53.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 14702_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 14702_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:24:39.78 -29:42:12.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 16992_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 16992_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:11:02.11 -29:24:52.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77140_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 77140_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:06:06.39 -23:36:23.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 81524_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 81524_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:48:26.57 -23:50:03.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 28857_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 28857_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:35:52.20 -28:12:48.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27268_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 27268_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:46:12.77 -28:03:42.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10177_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 10177_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:52:12.67 -29:53:12.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19168_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 19168_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:02:39.67 -29:08:07.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43915_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 43915_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:50:34.83 -26:17:23.4 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02768_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 02768_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:19:32.64 -30:54:13.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46946_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 46946_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:58:51.79 -26:06:45.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84434_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 84434_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:41:36.11 -24:28:04.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35726_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 35726_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:54:30.24 -27:20:18.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58372_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 58372_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:58:35.14 -24:49:54.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25979_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 25979_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:44:59.92 -28:30:33.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54623_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 54623_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:54:39.57 -25:14:38.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67349_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 67349_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:00:20.45 -22:37:20.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45501_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 45501_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:55:30.22 -26:15:57.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17193_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 17193_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:56:53.50 -29:12:42.7 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48797_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 48797_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:50:59.21 -25:45:03.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81996_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 81996_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:53:56.04 -23:58:42.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53620_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 53620_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:53:37.22 -25:19:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62014_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 62014_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 15:57:40.51 -20:59:00.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60722_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 60722_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:07:24.61 -20:52:13.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63548_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011
The candidate 63548_fd_Sco-02-Q1b1x1_2026-04-20_05-14-26_20.00sec_-4.90C_LIGHTs_0011 did not pass the final checks
**** FOUND 16:32:07.92 -21:28:00.9 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 18s
make_report_in_HTML.sh TOTAL: 733s
Prepared the HTML report for the field Sco-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:23:35.43 -26:31:39.8
16:53:24.81 -30:14:14.2
16:48:58.98 -21:22:51.1
16:24:16.86 -31:10:19.4
16:51:56.60 -21:19:44.4
16:46:15.63 -29:09:39.9
16:52:26.43 -28:44:09.7
16:43:46.48 -25:13:34.2
16:50:22.79 -28:32:20.3
16:46:20.11 -27:18:39.2
16:52:38.83 -21:45:47.4
16:07:46.50 -30:41:54.8
16:46:54.25 -30:07:53.2
16:40:44.60 -31:05:26.1
16:51:55.89 -30:58:30.0
16:46:18.58 -31:02:19.5
16:39:14.52 -30:24:21.8
16:04:10.16 -22:45:50.0
16:00:10.44 -27:06:36.6
15:50:28.72 -28:37:06.5
16:01:03.66 -25:07:15.5
15:50:30.03 -29:11:38.0
16:50:41.80 -24:34:10.1
16:18:32.15 -28:19:41.4
15:49:27.63 -27:46:20.6
15:47:32.84 -29:05:20.0
16:11:18.88 -23:42:24.9
16:37:35.07 -24:52:43.0
15:53:07.65 -30:18:19.2
15:49:58.93 -23:14:53.7
16:33:52.07 -26:41:24.5
15:54:26.43 -27:36:03.4
15:46:16.16 -27:50:46.9
15:49:56.64 -25:22:14.1
15:50:20.73 -21:17:01.1
16:50:08.90 -22:57:21.4
15:48:44.45 -27:16:29.7
15:43:46.99 -28:00:52.3
15:47:28.10 -24:09:46.1
15:46:51.43 -28:21:58.1
15:44:46.19 -29:42:57.7
15:50:13.58 -26:44:26.1
15:52:38.30 -27:32:19.4
15:50:27.14 -21:40:20.2
16:10:05.64 -28:37:12.8
15:53:43.63 -29:10:22.3
16:51:07.46 -27:20:02.8
15:48:30.82 -24:25:40.0
16:50:47.24 -25:20:34.5
15:51:36.51 -28:19:07.7
15:49:12.32 -23:31:25.0
16:35:47.49 -28:43:59.3
16:03:55.48 -24:32:34.5
16:50:10.44 -29:57:32.8
15:46:41.78 -26:10:08.5
15:43:34.12 -28:17:14.9
15:45:36.62 -28:09:48.1
15:49:07.62 -30:12:46.9
16:40:44.19 -30:29:36.1
16:16:10.20 -28:21:22.8
16:06:34.08 -29:10:15.5
15:47:37.33 -22:29:40.5
15:59:25.19 -30:07:27.5
15:48:35.33 -28:31:41.6
15:48:35.89 -27:11:31.0
16:39:12.36 -30:24:21.1
15:53:42.53 -29:56:33.4
15:44:29.49 -26:37:44.4
15:46:13.69 -28:27:47.4
15:45:59.73 -28:13:50.2
16:43:46.00 -25:35:49.2
15:46:39.62 -24:59:07.4
15:54:53.43 -28:47:47.8
16:41:54.80 -31:12:09.5
15:49:10.22 -27:14:31.1
16:43:38.83 -26:03:37.7
16:43:45.54 -30:06:17.2
15:47:47.45 -27:18:21.4
15:46:19.66 -27:13:14.2
15:44:51.62 -30:12:55.3
15:48:53.16 -25:30:29.1
16:49:47.93 -27:33:22.9
15:49:25.39 -29:27:58.5
16:49:47.58 -22:57:12.9
15:44:54.08 -30:06:40.1
15:45:03.08 -29:12:25.9
16:37:29.39 -28:31:54.7
15:47:03.06 -25:44:33.7
16:50:01.33 -23:33:25.1
15:47:13.46 -23:02:44.4
15:48:16.61 -28:18:26.7
15:50:09.06 -23:33:22.9
16:22:54.64 -26:55:12.2
16:53:07.37 -29:42:10.4
15:50:26.53 -23:42:09.1
15:45:07.91 -27:57:05.0
15:53:06.77 -29:13:38.0
15:51:23.37 -21:43:04.6
16:39:22.04 -30:33:06.5
16:47:53.86 -31:06:09.0
16:47:42.42 -30:55:25.9
15:46:43.13 -25:15:20.0
15:45:39.57 -27:45:32.5
16:46:52.02 -31:06:41.6
15:48:11.82 -25:42:19.6
16:51:54.48 -30:00:45.4
15:43:46.25 -27:50:10.6
16:42:51.93 -30:17:17.3
16:19:42.33 -25:34:49.3
16:20:22.29 -25:07:09.3
16:43:37.99 -30:11:07.0
16:29:18.48 -30:20:42.1
15:53:36.45 -27:49:21.2
16:53:20.29 -30:49:22.1
16:19:49.03 -22:17:39.4
16:53:00.80 -25:21:14.1
16:49:20.97 -28:13:29.4
16:51:28.07 -25:27:43.8
16:33:53.68 -28:12:39.2
16:48:36.15 -26:02:25.4
16:50:27.52 -21:25:47.3
16:52:32.87 -27:16:35.1
16:15:26.23 -21:10:42.1
16:47:51.76 -29:52:43.9
16:48:13.17 -23:20:44.0
16:36:11.89 -31:01:26.4
16:47:02.37 -30:17:57.7
16:49:07.37 -23:11:32.2
16:53:02.11 -30:03:48.3
16:46:51.68 -31:01:17.6
16:28:07.17 -26:26:38.7
16:24:27.62 -29:35:28.2
16:48:57.44 -28:48:25.8
16:01:07.76 -27:36:05.5
16:29:27.26 -27:33:28.7
16:39:23.35 -23:36:07.6
16:51:56.57 -21:32:40.3
16:15:49.28 -30:17:29.3
15:55:07.43 -24:57:15.4
16:53:00.64 -27:34:26.9
16:52:20.76 -28:41:48.4
16:12:23.58 -21:40:12.9
16:41:59.49 -29:44:47.8
16:53:23.82 -25:20:45.7
16:12:51.64 -24:45:30.3
15:47:38.45 -22:05:25.2
16:50:43.90 -30:56:36.7
16:11:29.63 -27:12:40.6
16:47:04.16 -25:48:41.1
16:51:35.64 -29:55:36.7
16:53:15.95 -23:17:12.8
16:47:22.38 -30:41:08.3
16:49:07.80 -25:08:26.0
16:50:57.35 -26:46:44.2
15:50:03.55 -27:32:21.7
16:41:52.23 -23:10:25.4
16:49:14.55 -24:52:12.0
16:48:12.86 -24:15:55.7
16:50:11.80 -22:54:53.5
16:51:44.42 -28:06:23.1
16:53:40.28 -23:59:48.6
16:50:26.68 -21:25:56.3
16:53:25.14 -25:07:59.7
16:53:10.75 -25:41:37.8
16:53:03.34 -26:41:13.6
16:44:17.56 -22:06:56.7
15:56:21.89 -29:57:32.9
16:49:26.10 -22:10:24.6
16:45:41.32 -28:23:19.5
16:43:52.83 -25:04:31.2
15:49:28.26 -25:56:51.9
16:45:43.14 -26:19:30.8
15:50:58.03 -20:48:32.4
16:47:10.39 -22:36:47.2
16:26:48.51 -30:35:37.0
16:46:25.12 -25:57:10.1
16:44:17.35 -22:07:01.0
16:47:11.52 -31:07:37.1
16:48:29.27 -29:37:42.0
16:46:02.40 -22:04:22.4
16:21:15.09 -29:00:34.9
16:43:36.42 -28:35:42.0
16:50:16.55 -30:23:53.1
16:48:54.85 -22:51:09.3
16:21:15.35 -29:00:17.6
15:53:46.10 -27:16:25.1
16:42:25.84 -22:30:19.8
16:45:23.85 -26:22:16.2
16:02:18.90 -20:39:23.2
16:51:46.27 -22:28:36.5
16:03:43.99 -29:39:59.2
16:24:50.84 -31:02:24.8
16:51:28.12 -27:55:29.0
16:44:34.89 -24:54:56.8
16:41:01.84 -29:19:59.2
16:02:56.45 -30:30:55.1
16:35:56.46 -26:49:37.3
16:51:50.67 -22:18:52.1
16:02:47.56 -21:35:35.6
16:47:41.73 -26:13:54.6
16:51:44.11 -21:24:51.7
16:23:58.00 -26:39:22.5
16:48:41.84 -24:02:01.8
16:48:19.54 -22:20:22.5
16:40:41.60 -28:09:47.8
16:07:52.10 -26:57:35.6
16:53:02.49 -26:45:29.8
16:48:57.58 -28:48:19.0
16:52:46.80 -24:05:24.5
15:52:16.10 -20:33:54.5
16:19:12.54 -31:06:40.5
16:43:19.89 -27:50:23.8
16:42:14.64 -28:57:21.4
16:46:09.04 -25:26:40.9
16:52:23.70 -21:34:50.8
16:17:14.07 -21:58:16.4
16:50:30.49 -25:41:49.7
16:51:48.69 -28:49:04.8
16:34:10.65 -30:41:25.2
16:41:42.96 -30:41:04.3
16:42:47.42 -30:19:03.0
16:47:48.96 -27:16:00.3
16:51:49.38 -24:30:49.6
16:49:13.21 -29:25:16.6
16:50:15.44 -29:08:36.9
16:52:15.68 -22:40:30.2
16:39:12.14 -23:29:15.4
15:54:49.42 -30:25:54.7
16:01:45.27 -28:21:33.0
16:51:28.65 -28:14:26.0
16:40:20.92 -30:27:12.1
16:51:31.62 -26:38:49.8
16:44:32.91 -30:13:50.9
15:55:59.06 -27:23:29.9
16:21:41.99 -25:22:56.4
16:30:50.79 -26:38:04.3
16:46:11.16 -29:29:07.1
15:55:20.65 -27:31:47.7
16:03:29.05 -25:11:27.5
16:00:33.92 -27:50:41.7
16:27:10.40 -29:24:39.5
16:45:33.74 -29:20:02.2
16:51:58.95 -21:22:10.7
15:53:25.97 -29:39:59.3
16:52:00.09 -28:32:13.1
15:53:21.42 -21:06:10.6
16:04:17.61 -30:47:14.9
15:58:44.21 -21:46:42.4
16:52:50.85 -29:49:05.4
16:23:38.72 -25:46:45.0
16:32:46.15 -27:17:49.5
15:57:19.63 -21:00:25.4
16:51:59.57 -21:49:38.2
15:52:04.50 -21:11:00.6
16:53:18.90 -22:13:08.4
16:52:05.45 -21:46:49.2
15:57:37.63 -20:37:03.3
15:55:05.01 -29:58:22.0
16:51:05.22 -26:20:59.4
16:52:28.10 -24:31:50.9
16:50:04.08 -28:20:07.2
15:56:13.09 -23:17:57.5
16:44:36.51 -26:29:54.1
16:19:44.43 -28:59:29.8
16:13:08.91 -21:25:56.2
16:50:33.82 -22:21:20.6
16:23:42.41 -29:01:39.2
16:52:17.12 -22:30:35.4
16:52:30.19 -22:01:24.3
16:38:11.01 -25:53:54.7
16:31:27.14 -31:12:46.3
16:36:31.43 -27:21:34.2
16:52:23.00 -29:29:23.6
16:48:29.85 -24:53:56.9
16:36:31.05 -27:21:46.1
15:59:14.11 -28:41:19.5
16:50:24.00 -22:41:40.0
16:49:09.35 -25:23:43.8
16:45:02.13 -28:54:23.9
16:42:01.13 -30:49:13.3
16:24:30.94 -29:27:57.1
16:05:19.32 -30:42:02.3
16:48:44.76 -21:46:49.1
16:52:49.56 -21:55:47.7
16:03:31.22 -28:07:05.4
15:57:02.62 -21:08:35.9
16:52:28.93 -21:24:57.2
16:44:13.38 -22:52:49.5
15:59:26.63 -28:34:42.2
15:53:56.23 -29:50:40.8
16:53:07.52 -29:51:08.5
16:47:15.85 -29:54:43.8
15:50:13.76 -29:38:23.2
16:53:21.60 -29:48:56.7
16:23:17.83 -29:53:49.9
16:46:51.19 -29:48:14.3
16:53:06.70 -29:42:18.7
16:48:47.88 -29:45:43.7
16:50:11.85 -29:43:31.3
16:52:51.23 -29:29:33.0
16:43:07.58 -29:20:35.2
15:51:52.27 -28:56:46.4
15:57:02.38 -28:56:18.8
16:52:04.57 -28:59:34.4
16:52:42.70 -28:58:50.8
16:47:07.52 -29:00:50.9
16:02:07.12 -28:54:34.3
16:42:39.36 -28:55:45.7
16:08:06.13 -28:47:30.5
15:48:22.29 -28:24:51.2
16:50:22.30 -28:32:21.1
16:03:13.83 -28:26:08.0
16:52:17.79 -28:19:33.9
16:45:13.98 -28:20:12.5
16:47:54.36 -28:09:24.7
16:07:01.00 -28:01:35.1
15:52:50.84 -27:25:24.9
16:49:08.47 -27:24:45.1
16:41:02.29 -27:26:49.2
16:49:14.37 -27:19:36.7
15:58:10.89 -26:58:07.2
16:45:07.48 -26:44:16.6
16:36:50.02 -26:45:10.9
16:52:44.02 -26:36:32.6
16:47:10.40 -26:35:34.9
16:41:58.85 -26:21:43.4
16:53:35.91 -26:13:48.4
16:44:43.62 -26:16:33.3
16:52:27.08 -25:54:30.4
16:02:38.92 -25:41:54.2
16:48:01.17 -25:41:15.8
16:51:21.99 -25:20:18.3
16:51:18.21 -25:10:26.1
16:47:41.78 -25:09:59.4
16:38:24.19 -25:03:02.5
15:52:57.93 -20:46:48.5
16:49:46.92 -22:57:17.9
16:48:34.10 -24:50:18.3
15:43:56.24 -29:08:47.0
16:27:12.77 -26:01:17.3
15:45:46.99 -28:52:51.0
16:33:01.34 -25:57:40.9
16:37:47.50 -27:20:55.0
########### Completed Sco-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
16:53:24.81 -30:14:14.2
16:48:58.98 -21:22:51.1
16:24:16.86 -31:10:19.4
16:51:56.60 -21:19:44.4
16:46:15.63 -29:09:39.9
16:52:26.43 -28:44:09.7
16:43:46.48 -25:13:34.2
16:50:22.79 -28:32:20.3
16:46:20.11 -27:18:39.2
16:52:38.83 -21:45:47.4
16:07:46.50 -30:41:54.8
16:46:54.25 -30:07:53.2
16:23:35.43 -26:31:39.8
16:04:10.16 -22:45:50.0
16:00:10.44 -27:06:36.6
15:50:28.72 -28:37:06.5
16:01:03.66 -25:07:15.5
15:50:30.03 -29:11:38.0
16:50:41.80 -24:34:10.1
16:18:32.15 -28:19:41.4
15:49:27.63 -27:46:20.6
15:47:32.84 -29:05:20.0
16:11:18.88 -23:42:24.9
16:37:35.07 -24:52:43.0
15:53:07.65 -30:18:19.2
15:49:58.93 -23:14:53.7
16:33:52.07 -26:41:24.5
15:54:26.43 -27:36:03.4
15:46:16.16 -27:50:46.9
15:49:56.64 -25:22:14.1
15:50:20.73 -21:17:01.1
16:50:08.90 -22:57:21.4
15:48:44.45 -27:16:29.7
15:43:46.99 -28:00:52.3
15:47:28.10 -24:09:46.1
15:46:51.43 -28:21:58.1
15:44:46.19 -29:42:57.7
15:50:13.58 -26:44:26.1
15:52:38.30 -27:32:19.4
15:50:27.14 -21:40:20.2
16:10:05.64 -28:37:12.8
15:53:43.63 -29:10:22.3
16:51:07.46 -27:20:02.8
15:48:30.82 -24:25:40.0
16:50:47.24 -25:20:34.5
15:51:36.51 -28:19:07.7
15:49:12.32 -23:31:25.0
16:35:47.49 -28:43:59.3
16:03:55.48 -24:32:34.5
16:50:10.44 -29:57:32.8
15:46:41.78 -26:10:08.5
15:43:34.12 -28:17:14.9
15:45:36.62 -28:09:48.1
15:49:07.62 -30:12:46.9
16:40:44.19 -30:29:36.1
16:16:10.20 -28:21:22.8
16:06:34.08 -29:10:15.5
15:47:37.33 -22:29:40.5
15:59:25.19 -30:07:27.5
15:48:35.33 -28:31:41.6
15:48:35.89 -27:11:31.0
16:39:12.36 -30:24:21.1
15:53:42.53 -29:56:33.4
15:44:29.49 -26:37:44.4
15:46:13.69 -28:27:47.4
15:45:59.73 -28:13:50.2
16:43:46.00 -25:35:49.2
15:46:39.62 -24:59:07.4
15:54:53.43 -28:47:47.8
16:41:54.80 -31:12:09.5
15:49:10.22 -27:14:31.1
16:43:38.83 -26:03:37.7
16:43:45.54 -30:06:17.2
15:47:47.45 -27:18:21.4
15:46:19.66 -27:13:14.2
15:44:51.62 -30:12:55.3
15:48:53.16 -25:30:29.1
16:49:47.93 -27:33:22.9
15:49:25.39 -29:27:58.5
16:49:47.58 -22:57:12.9
15:44:54.08 -30:06:40.1
15:45:03.08 -29:12:25.9
16:37:29.39 -28:31:54.7
15:47:03.06 -25:44:33.7
16:50:01.33 -23:33:25.1
15:47:13.46 -23:02:44.4
15:48:16.61 -28:18:26.7
15:50:09.06 -23:33:22.9
16:22:54.64 -26:55:12.2
16:53:07.37 -29:42:10.4
15:50:26.53 -23:42:09.1
15:45:07.91 -27:57:05.0
15:53:06.77 -29:13:38.0
15:51:23.37 -21:43:04.6
16:39:22.04 -30:33:06.5
16:47:53.86 -31:06:09.0
16:47:42.42 -30:55:25.9
15:46:43.13 -25:15:20.0
15:45:39.57 -27:45:32.5
16:46:52.02 -31:06:41.6
15:48:11.82 -25:42:19.6
16:51:54.48 -30:00:45.4
15:43:46.25 -27:50:10.6
16:42:51.93 -30:17:17.3
16:19:42.33 -25:34:49.3
16:20:22.29 -25:07:09.3
16:43:37.99 -30:11:07.0
16:29:18.48 -30:20:42.1
15:53:36.45 -27:49:21.2
16:53:20.29 -30:49:22.1
16:19:49.03 -22:17:39.4
16:53:00.80 -25:21:14.1
16:49:20.97 -28:13:29.4
16:51:28.07 -25:27:43.8
16:33:53.68 -28:12:39.2
16:48:36.15 -26:02:25.4
16:50:27.52 -21:25:47.3
16:52:32.87 -27:16:35.1
16:15:26.23 -21:10:42.1
16:47:51.76 -29:52:43.9
16:48:13.17 -23:20:44.0
16:36:11.89 -31:01:26.4
16:47:02.37 -30:17:57.7
16:49:07.37 -23:11:32.2
16:53:02.11 -30:03:48.3
16:46:51.68 -31:01:17.6
16:28:07.17 -26:26:38.7
16:24:27.62 -29:35:28.2
16:48:57.44 -28:48:25.8
16:01:07.76 -27:36:05.5
16:29:27.26 -27:33:28.7
16:39:23.35 -23:36:07.6
16:51:56.57 -21:32:40.3
16:15:49.28 -30:17:29.3
15:55:07.43 -24:57:15.4
16:53:00.64 -27:34:26.9
16:52:20.76 -28:41:48.4
16:12:23.58 -21:40:12.9
16:41:59.49 -29:44:47.8
16:53:23.82 -25:20:45.7
16:12:51.64 -24:45:30.3
15:47:38.45 -22:05:25.2
16:50:43.90 -30:56:36.7
16:11:29.63 -27:12:40.6
16:47:04.16 -25:48:41.1
16:51:35.64 -29:55:36.7
16:53:15.95 -23:17:12.8
16:47:22.38 -30:41:08.3
16:49:07.80 -25:08:26.0
16:50:57.35 -26:46:44.2
15:50:03.55 -27:32:21.7
16:41:52.23 -23:10:25.4
16:49:14.55 -24:52:12.0
16:48:12.86 -24:15:55.7
16:50:11.80 -22:54:53.5
16:51:44.42 -28:06:23.1
16:53:40.28 -23:59:48.6
16:50:26.68 -21:25:56.3
16:53:25.14 -25:07:59.7
16:53:10.75 -25:41:37.8
16:53:03.34 -26:41:13.6
16:44:17.56 -22:06:56.7
15:56:21.89 -29:57:32.9
16:49:26.10 -22:10:24.6
16:45:41.32 -28:23:19.5
16:43:52.83 -25:04:31.2
15:49:28.26 -25:56:51.9
16:45:43.14 -26:19:30.8
15:50:58.03 -20:48:32.4
16:47:10.39 -22:36:47.2
16:26:48.51 -30:35:37.0
16:46:25.12 -25:57:10.1
16:44:17.35 -22:07:01.0
16:47:11.52 -31:07:37.1
16:48:29.27 -29:37:42.0
16:46:02.40 -22:04:22.4
16:21:15.09 -29:00:34.9
16:43:36.42 -28:35:42.0
16:50:16.55 -30:23:53.1
16:48:54.85 -22:51:09.3
16:21:15.35 -29:00:17.6
15:53:46.10 -27:16:25.1
16:42:25.84 -22:30:19.8
16:45:23.85 -26:22:16.2
16:02:18.90 -20:39:23.2
16:51:46.27 -22:28:36.5
16:03:43.99 -29:39:59.2
16:24:50.84 -31:02:24.8
16:51:28.12 -27:55:29.0
16:44:34.89 -24:54:56.8
16:41:01.84 -29:19:59.2
16:02:56.45 -30:30:55.1
16:35:56.46 -26:49:37.3
16:51:50.67 -22:18:52.1
16:02:47.56 -21:35:35.6
16:47:41.73 -26:13:54.6
16:51:44.11 -21:24:51.7
16:23:58.00 -26:39:22.5
16:48:41.84 -24:02:01.8
16:48:19.54 -22:20:22.5
16:40:41.60 -28:09:47.8
16:07:52.10 -26:57:35.6
16:53:02.49 -26:45:29.8
16:48:57.58 -28:48:19.0
16:52:46.80 -24:05:24.5
15:52:16.10 -20:33:54.5
16:19:12.54 -31:06:40.5
16:43:19.89 -27:50:23.8
16:42:14.64 -28:57:21.4
16:46:09.04 -25:26:40.9
16:52:23.70 -21:34:50.8
16:17:14.07 -21:58:16.4
16:50:30.49 -25:41:49.7
16:51:48.69 -28:49:04.8
16:34:10.65 -30:41:25.2
16:41:42.96 -30:41:04.3
16:42:47.42 -30:19:03.0
16:47:48.96 -27:16:00.3
16:51:49.38 -24:30:49.6
16:49:13.21 -29:25:16.6
16:50:15.44 -29:08:36.9
16:52:15.68 -22:40:30.2
16:39:12.14 -23:29:15.4
15:54:49.42 -30:25:54.7
16:01:45.27 -28:21:33.0
16:51:28.65 -28:14:26.0
16:40:20.92 -30:27:12.1
16:51:31.62 -26:38:49.8
16:44:32.91 -30:13:50.9
15:55:59.06 -27:23:29.9
16:21:41.99 -25:22:56.4
16:30:50.79 -26:38:04.3
16:46:11.16 -29:29:07.1
15:55:20.65 -27:31:47.7
16:03:29.05 -25:11:27.5
16:00:33.92 -27:50:41.7
16:27:10.40 -29:24:39.5
16:45:33.74 -29:20:02.2
16:51:58.95 -21:22:10.7
15:53:25.97 -29:39:59.3
16:52:00.09 -28:32:13.1
15:53:21.42 -21:06:10.6
16:04:17.61 -30:47:14.9
15:58:44.21 -21:46:42.4
16:52:50.85 -29:49:05.4
16:23:38.72 -25:46:45.0
16:32:46.15 -27:17:49.5
15:57:19.63 -21:00:25.4
16:51:59.57 -21:49:38.2
15:52:04.50 -21:11:00.6
16:53:18.90 -22:13:08.4
16:52:05.45 -21:46:49.2
15:57:37.63 -20:37:03.3
15:55:05.01 -29:58:22.0
16:51:05.22 -26:20:59.4
16:52:28.10 -24:31:50.9
16:50:04.08 -28:20:07.2
15:56:13.09 -23:17:57.5
16:44:36.51 -26:29:54.1
16:19:44.43 -28:59:29.8
16:13:08.91 -21:25:56.2
16:50:33.82 -22:21:20.6
16:23:42.41 -29:01:39.2
16:52:17.12 -22:30:35.4
16:52:30.19 -22:01:24.3
16:38:11.01 -25:53:54.7
16:31:27.14 -31:12:46.3
16:36:31.43 -27:21:34.2
16:52:23.00 -29:29:23.6
16:48:29.85 -24:53:56.9
16:36:31.05 -27:21:46.1
15:59:14.11 -28:41:19.5
16:50:24.00 -22:41:40.0
16:49:09.35 -25:23:43.8
16:45:02.13 -28:54:23.9
16:42:01.13 -30:49:13.3
16:24:30.94 -29:27:57.1
16:05:19.32 -30:42:02.3
16:48:44.76 -21:46:49.1
16:52:49.56 -21:55:47.7
16:03:31.22 -28:07:05.4
15:57:02.62 -21:08:35.9
16:52:28.93 -21:24:57.2
16:44:13.38 -22:52:49.5
15:59:26.63 -28:34:42.2
15:50:13.76 -29:38:23.2
15:48:22.29 -28:24:51.2
16:48:34.10 -24:50:18.3
15:52:57.93 -20:46:48.5
16:41:02.29 -27:26:49.2
16:39:14.52 -30:24:21.8
16:02:07.12 -28:54:34.3
16:46:51.19 -29:48:14.3
16:52:17.79 -28:19:33.9
16:41:58.85 -26:21:43.4
16:40:44.60 -31:05:26.1
16:48:47.88 -29:45:43.7
16:02:38.92 -25:41:54.2
15:52:50.84 -27:25:24.9
16:47:54.36 -28:09:24.7
16:07:01.00 -28:01:35.1
16:51:18.21 -25:10:26.1
16:45:07.48 -26:44:16.6
16:48:01.17 -25:41:15.8
16:53:35.91 -26:13:48.4
16:49:14.37 -27:19:36.7
16:23:17.83 -29:53:49.9
16:45:13.98 -28:20:12.5
15:57:02.38 -28:56:18.8
16:47:15.85 -29:54:43.8
16:36:50.02 -26:45:10.9
16:50:22.30 -28:32:21.1
16:47:41.78 -25:09:59.4
16:52:27.08 -25:54:30.4
16:44:43.62 -26:16:33.3
16:53:06.70 -29:42:18.7
16:47:10.40 -26:35:34.9
16:53:21.60 -29:48:56.7
16:49:08.47 -27:24:45.1
16:49:46.92 -22:57:17.9
16:50:11.85 -29:43:31.3
15:53:56.23 -29:50:40.8
15:58:10.89 -26:58:07.2
16:52:04.57 -28:59:34.4
16:46:18.58 -31:02:19.5
16:37:47.50 -27:20:55.0
16:33:01.34 -25:57:40.9
16:52:44.02 -26:36:32.6
16:52:51.23 -29:29:33.0
15:45:46.99 -28:52:51.0
16:27:12.77 -26:01:17.3
15:43:56.24 -29:08:47.0
16:38:24.19 -25:03:02.5
16:42:39.36 -28:55:45.7
16:51:21.99 -25:20:18.3
16:47:07.52 -29:00:50.9
16:52:42.70 -28:58:50.8
16:03:13.83 -28:26:08.0
15:51:52.27 -28:56:46.4
16:53:07.52 -29:51:08.5
16:51:55.89 -30:58:30.0
16:08:06.13 -28:47:30.5
16:43:07.58 -29:20:35.2
###################################################################################
16:53:24.81 -30:14:14.2 -- not an asteroid (will add it to exclusion list)
16:48:58.98 -21:22:51.1 -- not an asteroid (will add it to exclusion list)
16:24:16.86 -31:10:19.4 -- not an asteroid (will add it to exclusion list)
16:51:56.60 -21:19:44.4 -- not an asteroid (will add it to exclusion list)
16:46:15.63 -29:09:39.9 -- not an asteroid (will add it to exclusion list)
16:52:26.43 -28:44:09.7 -- not an asteroid (will add it to exclusion list)
16:43:46.48 -25:13:34.2 -- not an asteroid (will add it to exclusion list)
16:50:22.79 -28:32:20.3 -- not an asteroid (will add it to exclusion list)
16:46:20.11 -27:18:39.2 -- not an asteroid (will add it to exclusion list)
16:52:38.83 -21:45:47.4 -- not an asteroid (will add it to exclusion list)
16:07:46.50 -30:41:54.8 -- not an asteroid (will add it to exclusion list)
16:46:54.25 -30:07:53.2 -- asteroid (will NOT add it to exclusion list)
16:23:35.43 -26:31:39.8 -- not an asteroid (will add it to exclusion list)
16:04:10.16 -22:45:50.0 -- not an asteroid (will add it to exclusion list)
16:00:10.44 -27:06:36.6 -- not an asteroid (will add it to exclusion list)
15:50:28.72 -28:37:06.5 -- not an asteroid (will add it to exclusion list)
16:01:03.66 -25:07:15.5 -- not an asteroid (will add it to exclusion list)
15:50:30.03 -29:11:38.0 -- not an asteroid (will add it to exclusion list)
16:50:41.80 -24:34:10.1 -- not an asteroid (will add it to exclusion list)
16:18:32.15 -28:19:41.4 -- not an asteroid (will add it to exclusion list)
15:49:27.63 -27:46:20.6 -- not an asteroid (will add it to exclusion list)
15:47:32.84 -29:05:20.0 -- not an asteroid (will add it to exclusion list)
16:11:18.88 -23:42:24.9 -- not an asteroid (will add it to exclusion list)
16:37:35.07 -24:52:43.0 -- not an asteroid (will add it to exclusion list)
15:53:07.65 -30:18:19.2 -- not an asteroid (will add it to exclusion list)
15:49:58.93 -23:14:53.7 -- not an asteroid (will add it to exclusion list)
16:33:52.07 -26:41:24.5 -- not an asteroid (will add it to exclusion list)
15:54:26.43 -27:36:03.4 -- not an asteroid (will add it to exclusion list)
15:46:16.16 -27:50:46.9 -- not an asteroid (will add it to exclusion list)
15:49:56.64 -25:22:14.1 -- not an asteroid (will add it to exclusion list)
15:50:20.73 -21:17:01.1 -- not an asteroid (will add it to exclusion list)
16:50:08.90 -22:57:21.4 -- not an asteroid (will add it to exclusion list)
15:48:44.45 -27:16:29.7 -- not an asteroid (will add it to exclusion list)
15:43:46.99 -28:00:52.3 -- not an asteroid (will add it to exclusion list)
15:47:28.10 -24:09:46.1 -- not an asteroid (will add it to exclusion list)
15:46:51.43 -28:21:58.1 -- not an asteroid (will add it to exclusion list)
15:44:46.19 -29:42:57.7 -- not an asteroid (will add it to exclusion list)
15:50:13.58 -26:44:26.1 -- not an asteroid (will add it to exclusion list)
15:52:38.30 -27:32:19.4 -- not an asteroid (will add it to exclusion list)
15:50:27.14 -21:40:20.2 -- not an asteroid (will add it to exclusion list)
16:10:05.64 -28:37:12.8 -- not an asteroid (will add it to exclusion list)
15:53:43.63 -29:10:22.3 -- not an asteroid (will add it to exclusion list)
16:51:07.46 -27:20:02.8 -- not an asteroid (will add it to exclusion list)
15:48:30.82 -24:25:40.0 -- not an asteroid (will add it to exclusion list)
16:50:47.24 -25:20:34.5 -- not an asteroid (will add it to exclusion list)
15:51:36.51 -28:19:07.7 -- not an asteroid (will add it to exclusion list)
15:49:12.32 -23:31:25.0 -- not an asteroid (will add it to exclusion list)
16:35:47.49 -28:43:59.3 -- not an asteroid (will add it to exclusion list)
16:03:55.48 -24:32:34.5 -- not an asteroid (will add it to exclusion list)
16:50:10.44 -29:57:32.8 -- not an asteroid (will add it to exclusion list)
15:46:41.78 -26:10:08.5 -- not an asteroid (will add it to exclusion list)
15:43:34.12 -28:17:14.9 -- not an asteroid (will add it to exclusion list)
15:45:36.62 -28:09:48.1 -- asteroid (will NOT add it to exclusion list)
15:49:07.62 -30:12:46.9 -- not an asteroid (will add it to exclusion list)
16:40:44.19 -30:29:36.1 -- not an asteroid (will add it to exclusion list)
16:16:10.20 -28:21:22.8 -- not an asteroid (will add it to exclusion list)
16:06:34.08 -29:10:15.5 -- not an asteroid (will add it to exclusion list)
15:47:37.33 -22:29:40.5 -- not an asteroid (will add it to exclusion list)
15:59:25.19 -30:07:27.5 -- not an asteroid (will add it to exclusion list)
15:48:35.33 -28:31:41.6 -- not an asteroid (will add it to exclusion list)
15:48:35.89 -27:11:31.0 -- not an asteroid (will add it to exclusion list)
16:39:12.36 -30:24:21.1 -- not an asteroid (will add it to exclusion list)
15:53:42.53 -29:56:33.4 -- not an asteroid (will add it to exclusion list)
15:44:29.49 -26:37:44.4 -- not an asteroid (will add it to exclusion list)
15:46:13.69 -28:27:47.4 -- not an asteroid (will add it to exclusion list)
15:45:59.73 -28:13:50.2 -- asteroid (will NOT add it to exclusion list)
16:43:46.00 -25:35:49.2 -- not an asteroid (will add it to exclusion list)
15:46:39.62 -24:59:07.4 -- not an asteroid (will add it to exclusion list)
15:54:53.43 -28:47:47.8 -- not an asteroid (will add it to exclusion list)
16:41:54.80 -31:12:09.5 -- not an asteroid (will add it to exclusion list)
15:49:10.22 -27:14:31.1 -- not an asteroid (will add it to exclusion list)
16:43:38.83 -26:03:37.7 -- not an asteroid (will add it to exclusion list)
16:43:45.54 -30:06:17.2 -- not an asteroid (will add it to exclusion list)
15:47:47.45 -27:18:21.4 -- not an asteroid (will add it to exclusion list)
15:46:19.66 -27:13:14.2 -- not an asteroid (will add it to exclusion list)
15:44:51.62 -30:12:55.3 -- not an asteroid (will add it to exclusion list)
15:48:53.16 -25:30:29.1 -- asteroid (will NOT add it to exclusion list)
16:49:47.93 -27:33:22.9 -- not an asteroid (will add it to exclusion list)
15:49:25.39 -29:27:58.5 -- not an asteroid (will add it to exclusion list)
16:49:47.58 -22:57:12.9 -- not an asteroid (will add it to exclusion list)
15:44:54.08 -30:06:40.1 -- not an asteroid (will add it to exclusion list)
15:45:03.08 -29:12:25.9 -- not an asteroid (will add it to exclusion list)
16:37:29.39 -28:31:54.7 -- not an asteroid (will add it to exclusion list)
15:47:03.06 -25:44:33.7 -- not an asteroid (will add it to exclusion list)
16:50:01.33 -23:33:25.1 -- asteroid (will NOT add it to exclusion list)
15:47:13.46 -23:02:44.4 -- not an asteroid (will add it to exclusion list)
15:48:16.61 -28:18:26.7 -- not an asteroid (will add it to exclusion list)
15:50:09.06 -23:33:22.9 -- not an asteroid (will add it to exclusion list)
16:22:54.64 -26:55:12.2 -- not an asteroid (will add it to exclusion list)
16:53:07.37 -29:42:10.4 -- not an asteroid (will add it to exclusion list)
15:50:26.53 -23:42:09.1 -- not an asteroid (will add it to exclusion list)
15:45:07.91 -27:57:05.0 -- not an asteroid (will add it to exclusion list)
15:53:06.77 -29:13:38.0 -- not an asteroid (will add it to exclusion list)
15:51:23.37 -21:43:04.6 -- not an asteroid (will add it to exclusion list)
16:39:22.04 -30:33:06.5 -- not an asteroid (will add it to exclusion list)
16:47:53.86 -31:06:09.0 -- not an asteroid (will add it to exclusion list)
16:47:42.42 -30:55:25.9 -- not an asteroid (will add it to exclusion list)
15:46:43.13 -25:15:20.0 -- asteroid (will NOT add it to exclusion list)
15:45:39.57 -27:45:32.5 -- not an asteroid (will add it to exclusion list)
16:46:52.02 -31:06:41.6 -- not an asteroid (will add it to exclusion list)
15:48:11.82 -25:42:19.6 -- not an asteroid (will add it to exclusion list)
16:51:54.48 -30:00:45.4 -- not an asteroid (will add it to exclusion list)
15:43:46.25 -27:50:10.6 -- not an asteroid (will add it to exclusion list)
16:42:51.93 -30:17:17.3 -- not an asteroid (will add it to exclusion list)
16:19:42.33 -25:34:49.3 -- not an asteroid (will add it to exclusion list)
16:20:22.29 -25:07:09.3 -- not an asteroid (will add it to exclusion list)
16:43:37.99 -30:11:07.0 -- not an asteroid (will add it to exclusion list)
16:29:18.48 -30:20:42.1 -- not an asteroid (will add it to exclusion list)
15:53:36.45 -27:49:21.2 -- not an asteroid (will add it to exclusion list)
16:53:20.29 -30:49:22.1 -- not an asteroid (will add it to exclusion list)
16:19:49.03 -22:17:39.4 -- not an asteroid (will add it to exclusion list)
16:53:00.80 -25:21:14.1 -- not an asteroid (will add it to exclusion list)
16:49:20.97 -28:13:29.4 -- not an asteroid (will add it to exclusion list)
16:51:28.07 -25:27:43.8 -- not an asteroid (will add it to exclusion list)
16:33:53.68 -28:12:39.2 -- not an asteroid (will add it to exclusion list)
16:48:36.15 -26:02:25.4 -- not an asteroid (will add it to exclusion list)
16:50:27.52 -21:25:47.3 -- not an asteroid (will add it to exclusion list)
16:52:32.87 -27:16:35.1 -- not an asteroid (will add it to exclusion list)
16:15:26.23 -21:10:42.1 -- not an asteroid (will add it to exclusion list)
16:47:51.76 -29:52:43.9 -- not an asteroid (will add it to exclusion list)
16:48:13.17 -23:20:44.0 -- not an asteroid (will add it to exclusion list)
16:36:11.89 -31:01:26.4 -- not an asteroid (will add it to exclusion list)
16:47:02.37 -30:17:57.7 -- asteroid (will NOT add it to exclusion list)
16:49:07.37 -23:11:32.2 -- not an asteroid (will add it to exclusion list)
16:53:02.11 -30:03:48.3 -- not an asteroid (will add it to exclusion list)
16:46:51.68 -31:01:17.6 -- not an asteroid (will add it to exclusion list)
16:28:07.17 -26:26:38.7 -- not an asteroid (will add it to exclusion list)
16:24:27.62 -29:35:28.2 -- not an asteroid (will add it to exclusion list)
16:48:57.44 -28:48:25.8 -- not an asteroid (will add it to exclusion list)
16:01:07.76 -27:36:05.5 -- not an asteroid (will add it to exclusion list)
16:29:27.26 -27:33:28.7 -- not an asteroid (will add it to exclusion list)
16:39:23.35 -23:36:07.6 -- asteroid (will NOT add it to exclusion list)
16:51:56.57 -21:32:40.3 -- not an asteroid (will add it to exclusion list)
16:15:49.28 -30:17:29.3 -- not an asteroid (will add it to exclusion list)
15:55:07.43 -24:57:15.4 -- not an asteroid (will add it to exclusion list)
16:53:00.64 -27:34:26.9 -- not an asteroid (will add it to exclusion list)
16:52:20.76 -28:41:48.4 -- not an asteroid (will add it to exclusion list)
16:12:23.58 -21:40:12.9 -- not an asteroid (will add it to exclusion list)
16:41:59.49 -29:44:47.8 -- not an asteroid (will add it to exclusion list)
16:53:23.82 -25:20:45.7 -- not an asteroid (will add it to exclusion list)
16:12:51.64 -24:45:30.3 -- not an asteroid (will add it to exclusion list)
15:47:38.45 -22:05:25.2 -- not an asteroid (will add it to exclusion list)
16:50:43.90 -30:56:36.7 -- not an asteroid (will add it to exclusion list)
16:11:29.63 -27:12:40.6 -- asteroid (will NOT add it to exclusion list)
16:47:04.16 -25:48:41.1 -- not an asteroid (will add it to exclusion list)
16:51:35.64 -29:55:36.7 -- not an asteroid (will add it to exclusion list)
16:53:15.95 -23:17:12.8 -- not an asteroid (will add it to exclusion list)
16:47:22.38 -30:41:08.3 -- not an asteroid (will add it to exclusion list)
16:49:07.80 -25:08:26.0 -- not an asteroid (will add it to exclusion list)
16:50:57.35 -26:46:44.2 -- not an asteroid (will add it to exclusion list)
15:50:03.55 -27:32:21.7 -- not an asteroid (will add it to exclusion list)
16:41:52.23 -23:10:25.4 -- not an asteroid (will add it to exclusion list)
16:49:14.55 -24:52:12.0 -- not an asteroid (will add it to exclusion list)
16:48:12.86 -24:15:55.7 -- asteroid (will NOT add it to exclusion list)
16:50:11.80 -22:54:53.5 -- not an asteroid (will add it to exclusion list)
16:51:44.42 -28:06:23.1 -- not an asteroid (will add it to exclusion list)
16:53:40.28 -23:59:48.6 -- asteroid (will NOT add it to exclusion list)
16:50:26.68 -21:25:56.3 -- not an asteroid (will add it to exclusion list)
16:53:25.14 -25:07:59.7 -- not an asteroid (will add it to exclusion list)
16:53:10.75 -25:41:37.8 -- not an asteroid (will add it to exclusion list)
16:53:03.34 -26:41:13.6 -- not an asteroid (will add it to exclusion list)
16:44:17.56 -22:06:56.7 -- not an asteroid (will add it to exclusion list)
15:56:21.89 -29:57:32.9 -- not an asteroid (will add it to exclusion list)
16:49:26.10 -22:10:24.6 -- not an asteroid (will add it to exclusion list)
16:45:41.32 -28:23:19.5 -- not an asteroid (will add it to exclusion list)
16:43:52.83 -25:04:31.2 -- not an asteroid (will add it to exclusion list)
15:49:28.26 -25:56:51.9 -- not an asteroid (will add it to exclusion list)
16:45:43.14 -26:19:30.8 -- not an asteroid (will add it to exclusion list)
15:50:58.03 -20:48:32.4 -- not an asteroid (will add it to exclusion list)
16:47:10.39 -22:36:47.2 -- not an asteroid (will add it to exclusion list)
16:26:48.51 -30:35:37.0 -- not an asteroid (will add it to exclusion list)
16:46:25.12 -25:57:10.1 -- not an asteroid (will add it to exclusion list)
16:44:17.35 -22:07:01.0 -- not an asteroid (will add it to exclusion list)
16:47:11.52 -31:07:37.1 -- not an asteroid (will add it to exclusion list)
16:48:29.27 -29:37:42.0 -- not an asteroid (will add it to exclusion list)
16:46:02.40 -22:04:22.4 -- not an asteroid (will add it to exclusion list)
16:21:15.09 -29:00:34.9 -- not an asteroid (will add it to exclusion list)
16:43:36.42 -28:35:42.0 -- not an asteroid (will add it to exclusion list)
16:50:16.55 -30:23:53.1 -- not an asteroid (will add it to exclusion list)
16:48:54.85 -22:51:09.3 -- not an asteroid (will add it to exclusion list)
16:21:15.35 -29:00:17.6 -- not an asteroid (will add it to exclusion list)
15:53:46.10 -27:16:25.1 -- not an asteroid (will add it to exclusion list)
16:42:25.84 -22:30:19.8 -- not an asteroid (will add it to exclusion list)
16:45:23.85 -26:22:16.2 -- not an asteroid (will add it to exclusion list)
16:02:18.90 -20:39:23.2 -- not an asteroid (will add it to exclusion list)
16:51:46.27 -22:28:36.5 -- not an asteroid (will add it to exclusion list)
16:03:43.99 -29:39:59.2 -- not an asteroid (will add it to exclusion list)
16:24:50.84 -31:02:24.8 -- not an asteroid (will add it to exclusion list)
16:51:28.12 -27:55:29.0 -- not an asteroid (will add it to exclusion list)
16:44:34.89 -24:54:56.8 -- not an asteroid (will add it to exclusion list)
16:41:01.84 -29:19:59.2 -- not an asteroid (will add it to exclusion list)
16:02:56.45 -30:30:55.1 -- not an asteroid (will add it to exclusion list)
16:35:56.46 -26:49:37.3 -- not an asteroid (will add it to exclusion list)
16:51:50.67 -22:18:52.1 -- not an asteroid (will add it to exclusion list)
16:02:47.56 -21:35:35.6 -- not an asteroid (will add it to exclusion list)
16:47:41.73 -26:13:54.6 -- not an asteroid (will add it to exclusion list)
16:51:44.11 -21:24:51.7 -- not an asteroid (will add it to exclusion list)
16:23:58.00 -26:39:22.5 -- not an asteroid (will add it to exclusion list)
16:48:41.84 -24:02:01.8 -- not an asteroid (will add it to exclusion list)
16:48:19.54 -22:20:22.5 -- not an asteroid (will add it to exclusion list)
16:40:41.60 -28:09:47.8 -- not an asteroid (will add it to exclusion list)
16:07:52.10 -26:57:35.6 -- not an asteroid (will add it to exclusion list)
16:53:02.49 -26:45:29.8 -- not an asteroid (will add it to exclusion list)
16:48:57.58 -28:48:19.0 -- not an asteroid (will add it to exclusion list)
16:52:46.80 -24:05:24.5 -- not an asteroid (will add it to exclusion list)
15:52:16.10 -20:33:54.5 -- not an asteroid (will add it to exclusion list)
16:19:12.54 -31:06:40.5 -- not an asteroid (will add it to exclusion list)
16:43:19.89 -27:50:23.8 -- not an asteroid (will add it to exclusion list)
16:42:14.64 -28:57:21.4 -- not an asteroid (will add it to exclusion list)
16:46:09.04 -25:26:40.9 -- not an asteroid (will add it to exclusion list)
16:52:23.70 -21:34:50.8 -- not an asteroid (will add it to exclusion list)
16:17:14.07 -21:58:16.4 -- not an asteroid (will add it to exclusion list)
16:50:30.49 -25:41:49.7 -- not an asteroid (will add it to exclusion list)
16:51:48.69 -28:49:04.8 -- not an asteroid (will add it to exclusion list)
16:34:10.65 -30:41:25.2 -- not an asteroid (will add it to exclusion list)
16:41:42.96 -30:41:04.3 -- not an asteroid (will add it to exclusion list)
16:42:47.42 -30:19:03.0 -- not an asteroid (will add it to exclusion list)
16:47:48.96 -27:16:00.3 -- not an asteroid (will add it to exclusion list)
16:51:49.38 -24:30:49.6 -- not an asteroid (will add it to exclusion list)
16:49:13.21 -29:25:16.6 -- not an asteroid (will add it to exclusion list)
16:50:15.44 -29:08:36.9 -- not an asteroid (will add it to exclusion list)
16:52:15.68 -22:40:30.2 -- not an asteroid (will add it to exclusion list)
16:39:12.14 -23:29:15.4 -- asteroid (will NOT add it to exclusion list)
15:54:49.42 -30:25:54.7 -- not an asteroid (will add it to exclusion list)
16:01:45.27 -28:21:33.0 -- asteroid (will NOT add it to exclusion list)
16:51:28.65 -28:14:26.0 -- not an asteroid (will add it to exclusion list)
16:40:20.92 -30:27:12.1 -- not an asteroid (will add it to exclusion list)
16:51:31.62 -26:38:49.8 -- not an asteroid (will add it to exclusion list)
16:44:32.91 -30:13:50.9 -- not an asteroid (will add it to exclusion list)
15:55:59.06 -27:23:29.9 -- not an asteroid (will add it to exclusion list)
16:21:41.99 -25:22:56.4 -- not an asteroid (will add it to exclusion list)
16:30:50.79 -26:38:04.3 -- not an asteroid (will add it to exclusion list)
16:46:11.16 -29:29:07.1 -- not an asteroid (will add it to exclusion list)
15:55:20.65 -27:31:47.7 -- not an asteroid (will add it to exclusion list)
16:03:29.05 -25:11:27.5 -- not an asteroid (will add it to exclusion list)
16:00:33.92 -27:50:41.7 -- not an asteroid (will add it to exclusion list)
16:27:10.40 -29:24:39.5 -- not an asteroid (will add it to exclusion list)
16:45:33.74 -29:20:02.2 -- not an asteroid (will add it to exclusion list)
16:51:58.95 -21:22:10.7 -- not an asteroid (will add it to exclusion list)
15:53:25.97 -29:39:59.3 -- not an asteroid (will add it to exclusion list)
16:52:00.09 -28:32:13.1 -- not an asteroid (will add it to exclusion list)
15:53:21.42 -21:06:10.6 -- not an asteroid (will add it to exclusion list)
16:04:17.61 -30:47:14.9 -- not an asteroid (will add it to exclusion list)
15:58:44.21 -21:46:42.4 -- not an asteroid (will add it to exclusion list)
16:52:50.85 -29:49:05.4 -- not an asteroid (will add it to exclusion list)
16:23:38.72 -25:46:45.0 -- not an asteroid (will add it to exclusion list)
16:32:46.15 -27:17:49.5 -- not an asteroid (will add it to exclusion list)
15:57:19.63 -21:00:25.4 -- not an asteroid (will add it to exclusion list)
16:51:59.57 -21:49:38.2 -- not an asteroid (will add it to exclusion list)
15:52:04.50 -21:11:00.6 -- not an asteroid (will add it to exclusion list)
16:53:18.90 -22:13:08.4 -- not an asteroid (will add it to exclusion list)
16:52:05.45 -21:46:49.2 -- not an asteroid (will add it to exclusion list)
15:57:37.63 -20:37:03.3 -- not an asteroid (will add it to exclusion list)
15:55:05.01 -29:58:22.0 -- not an asteroid (will add it to exclusion list)
16:51:05.22 -26:20:59.4 -- not an asteroid (will add it to exclusion list)
16:52:28.10 -24:31:50.9 -- not an asteroid (will add it to exclusion list)
16:50:04.08 -28:20:07.2 -- not an asteroid (will add it to exclusion list)
15:56:13.09 -23:17:57.5 -- not an asteroid (will add it to exclusion list)
16:44:36.51 -26:29:54.1 -- not an asteroid (will add it to exclusion list)
16:19:44.43 -28:59:29.8 -- not an asteroid (will add it to exclusion list)
16:13:08.91 -21:25:56.2 -- not an asteroid (will add it to exclusion list)
16:50:33.82 -22:21:20.6 -- not an asteroid (will add it to exclusion list)
16:23:42.41 -29:01:39.2 -- not an asteroid (will add it to exclusion list)
16:52:17.12 -22:30:35.4 -- not an asteroid (will add it to exclusion list)
16:52:30.19 -22:01:24.3 -- not an asteroid (will add it to exclusion list)
16:38:11.01 -25:53:54.7 -- not an asteroid (will add it to exclusion list)
16:31:27.14 -31:12:46.3 -- not an asteroid (will add it to exclusion list)
16:36:31.43 -27:21:34.2 -- not an asteroid (will add it to exclusion list)
16:52:23.00 -29:29:23.6 -- not an asteroid (will add it to exclusion list)
16:48:29.85 -24:53:56.9 -- not an asteroid (will add it to exclusion list)
16:36:31.05 -27:21:46.1 -- not an asteroid (will add it to exclusion list)
15:59:14.11 -28:41:19.5 -- not an asteroid (will add it to exclusion list)
16:50:24.00 -22:41:40.0 -- not an asteroid (will add it to exclusion list)
16:49:09.35 -25:23:43.8 -- not an asteroid (will add it to exclusion list)
16:45:02.13 -28:54:23.9 -- not an asteroid (will add it to exclusion list)
16:42:01.13 -30:49:13.3 -- not an asteroid (will add it to exclusion list)
16:24:30.94 -29:27:57.1 -- not an asteroid (will add it to exclusion list)
16:05:19.32 -30:42:02.3 -- not an asteroid (will add it to exclusion list)
16:48:44.76 -21:46:49.1 -- not an asteroid (will add it to exclusion list)
16:52:49.56 -21:55:47.7 -- not an asteroid (will add it to exclusion list)
16:03:31.22 -28:07:05.4 -- not an asteroid (will add it to exclusion list)
15:57:02.62 -21:08:35.9 -- not an asteroid (will add it to exclusion list)
16:52:28.93 -21:24:57.2 -- not an asteroid (will add it to exclusion list)
16:44:13.38 -22:52:49.5 -- not an asteroid (will add it to exclusion list)
15:59:26.63 -28:34:42.2 -- not an asteroid (will add it to exclusion list)
15:50:13.76 -29:38:23.2 -- not an asteroid (will add it to exclusion list)
15:48:22.29 -28:24:51.2 -- not an asteroid (will add it to exclusion list)
16:48:34.10 -24:50:18.3 -- not an asteroid (will add it to exclusion list)
15:52:57.93 -20:46:48.5 -- not an asteroid (will add it to exclusion list)
16:41:02.29 -27:26:49.2 -- not an asteroid (will add it to exclusion list)
16:39:14.52 -30:24:21.8 -- not an asteroid (will add it to exclusion list)
16:02:07.12 -28:54:34.3 -- not an asteroid (will add it to exclusion list)
16:46:51.19 -29:48:14.3 -- not an asteroid (will add it to exclusion list)
16:52:17.79 -28:19:33.9 -- not an asteroid (will add it to exclusion list)
16:41:58.85 -26:21:43.4 -- not an asteroid (will add it to exclusion list)
16:40:44.60 -31:05:26.1 -- not an asteroid (will add it to exclusion list)
16:48:47.88 -29:45:43.7 -- not an asteroid (will add it to exclusion list)
16:02:38.92 -25:41:54.2 -- not an asteroid (will add it to exclusion list)
15:52:50.84 -27:25:24.9 -- not an asteroid (will add it to exclusion list)
16:47:54.36 -28:09:24.7 -- not an asteroid (will add it to exclusion list)
16:07:01.00 -28:01:35.1 -- not an asteroid (will add it to exclusion list)
16:51:18.21 -25:10:26.1 -- not an asteroid (will add it to exclusion list)
16:45:07.48 -26:44:16.6 -- not an asteroid (will add it to exclusion list)
16:48:01.17 -25:41:15.8 -- not an asteroid (will add it to exclusion list)
16:53:35.91 -26:13:48.4 -- not an asteroid (will add it to exclusion list)
16:49:14.37 -27:19:36.7 -- not an asteroid (will add it to exclusion list)
16:23:17.83 -29:53:49.9 -- not an asteroid (will add it to exclusion list)
16:45:13.98 -28:20:12.5 -- not an asteroid (will add it to exclusion list)
15:57:02.38 -28:56:18.8 -- not an asteroid (will add it to exclusion list)
16:47:15.85 -29:54:43.8 -- not an asteroid (will add it to exclusion list)
16:36:50.02 -26:45:10.9 -- not an asteroid (will add it to exclusion list)
16:50:22.30 -28:32:21.1 -- not an asteroid (will add it to exclusion list)
16:47:41.78 -25:09:59.4 -- not an asteroid (will add it to exclusion list)
16:52:27.08 -25:54:30.4 -- not an asteroid (will add it to exclusion list)
16:44:43.62 -26:16:33.3 -- not an asteroid (will add it to exclusion list)
16:53:06.70 -29:42:18.7 -- not an asteroid (will add it to exclusion list)
16:47:10.40 -26:35:34.9 -- not an asteroid (will add it to exclusion list)
16:53:21.60 -29:48:56.7 -- not an asteroid (will add it to exclusion list)
16:49:08.47 -27:24:45.1 -- not an asteroid (will add it to exclusion list)
16:49:46.92 -22:57:17.9 -- not an asteroid (will add it to exclusion list)
16:50:11.85 -29:43:31.3 -- not an asteroid (will add it to exclusion list)
15:53:56.23 -29:50:40.8 -- not an asteroid (will add it to exclusion list)
15:58:10.89 -26:58:07.2 -- not an asteroid (will add it to exclusion list)
16:52:04.57 -28:59:34.4 -- not an asteroid (will add it to exclusion list)
16:46:18.58 -31:02:19.5 -- not an asteroid (will add it to exclusion list)
16:37:47.50 -27:20:55.0 -- not an asteroid (will add it to exclusion list)
16:33:01.34 -25:57:40.9 -- not an asteroid (will add it to exclusion list)
16:52:44.02 -26:36:32.6 -- not an asteroid (will add it to exclusion list)
16:52:51.23 -29:29:33.0 -- not an asteroid (will add it to exclusion list)
15:45:46.99 -28:52:51.0 -- not an asteroid (will add it to exclusion list)
16:27:12.77 -26:01:17.3 -- not an asteroid (will add it to exclusion list)
15:43:56.24 -29:08:47.0 -- not an asteroid (will add it to exclusion list)
16:38:24.19 -25:03:02.5 -- not an asteroid (will add it to exclusion list)
16:42:39.36 -28:55:45.7 -- not an asteroid (will add it to exclusion list)
16:51:21.99 -25:20:18.3 -- not an asteroid (will add it to exclusion list)
16:47:07.52 -29:00:50.9 -- not an asteroid (will add it to exclusion list)
16:52:42.70 -28:58:50.8 -- not an asteroid (will add it to exclusion list)
16:03:13.83 -28:26:08.0 -- not an asteroid (will add it to exclusion list)
15:51:52.27 -28:56:46.4 -- not an asteroid (will add it to exclusion list)
16:53:07.52 -29:51:08.5 -- not an asteroid (will add it to exclusion list)
16:51:55.89 -30:58:30.0 -- not an asteroid (will add it to exclusion list)
16:08:06.13 -28:47:30.5 -- not an asteroid (will add it to exclusion list)
16:43:07.58 -29:20:35.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
15:43:34.12 -28:17:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:46.25 -27:50:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:46.99 -28:00:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:43:56.24 -29:08:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:29.49 -26:37:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:46.19 -29:42:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:51.62 -30:12:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:44:54.08 -30:06:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:03.08 -29:12:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:07.91 -27:57:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:39.57 -27:45:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:45:46.99 -28:52:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:13.69 -28:27:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:16.16 -27:50:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:19.66 -27:13:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:39.62 -24:59:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:41.78 -26:10:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:46:51.43 -28:21:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:03.06 -25:44:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:13.46 -23:02:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:28.10 -24:09:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:32.84 -29:05:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:37.33 -22:29:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:38.45 -22:05:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:47:47.45 -27:18:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:11.82 -25:42:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:16.61 -28:18:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:22.29 -28:24:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:30.82 -24:25:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:35.33 -28:31:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:35.89 -27:11:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:48:44.45 -27:16:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:07.62 -30:12:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:10.22 -27:14:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:12.32 -23:31:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:25.39 -29:27:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:27.63 -27:46:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:28.26 -25:56:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:56.64 -25:22:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:49:58.93 -23:14:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:03.55 -27:32:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:09.06 -23:33:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:13.58 -26:44:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:13.76 -29:38:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:20.73 -21:17:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:26.53 -23:42:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:27.14 -21:40:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:28.72 -28:37:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:30.03 -29:11:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:50:58.03 -20:48:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:23.37 -21:43:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:36.51 -28:19:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:51:52.27 -28:56:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:04.50 -21:11:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:16.10 -20:33:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:38.30 -27:32:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:50.84 -27:25:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:52:57.93 -20:46:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:06.77 -29:13:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:07.65 -30:18:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:21.42 -21:06:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:25.97 -29:39:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:36.45 -27:49:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:42.53 -29:56:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:43.63 -29:10:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:46.10 -27:16:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
15:53:56.23 -29:50:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:54:26.43 -27:36:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:54:49.42 -30:25:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:54:53.43 -28:47:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:05.01 -29:58:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:07.43 -24:57:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:20.65 -27:31:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
15:55:59.06 -27:23:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:56:13.09 -23:17:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:56:21.89 -29:57:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:02.38 -28:56:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:02.62 -21:08:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:19.63 -21:00:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:57:37.63 -20:37:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
15:58:10.89 -26:58:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
15:58:44.21 -21:46:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:14.11 -28:41:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:25.19 -30:07:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
15:59:26.63 -28:34:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:00:10.44 -27:06:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:00:33.92 -27:50:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:01:03.66 -25:07:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:01:07.76 -27:36:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:07.12 -28:54:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:18.90 -20:39:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:38.92 -25:41:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:47.56 -21:35:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:02:56.45 -30:30:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:13.83 -28:26:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:29.05 -25:11:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:31.22 -28:07:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:43.99 -29:39:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:03:55.48 -24:32:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:04:10.16 -22:45:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:04:17.61 -30:47:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:05:19.32 -30:42:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:06:34.08 -29:10:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:07:01.00 -28:01:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:07:46.50 -30:41:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:07:52.10 -26:57:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:08:06.13 -28:47:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:10:05.64 -28:37:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:11:18.88 -23:42:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:23.58 -21:40:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:12:51.64 -24:45:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:13:08.91 -21:25:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:15:26.23 -21:10:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:15:49.28 -30:17:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:16:10.20 -28:21:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:17:14.07 -21:58:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:18:32.15 -28:19:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:12.54 -31:06:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:42.33 -25:34:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:44.43 -28:59:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:19:49.03 -22:17:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:20:22.29 -25:07:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:15.09 -29:00:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:15.35 -29:00:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:21:41.99 -25:22:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:54.64 -26:55:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:17.83 -29:53:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:35.43 -26:31:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:38.72 -25:46:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:42.41 -29:01:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:23:58.00 -26:39:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:16.86 -31:10:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:27.62 -29:35:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:30.94 -29:27:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:50.84 -31:02:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:26:48.51 -30:35:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:10.40 -29:24:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:27:12.77 -26:01:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:28:07.17 -26:26:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:18.48 -30:20:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:29:27.26 -27:33:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:30:50.79 -26:38:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:31:27.14 -31:12:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:32:46.15 -27:17:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:01.34 -25:57:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:52.07 -26:41:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:33:53.68 -28:12:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:10.65 -30:41:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:47.49 -28:43:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:35:56.46 -26:49:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:11.89 -31:01:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:31.05 -27:21:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:31.43 -27:21:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:36:50.02 -26:45:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:29.39 -28:31:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:35.07 -24:52:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:37:47.50 -27:20:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:11.01 -25:53:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:38:24.19 -25:03:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:12.36 -30:24:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:14.52 -30:24:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:22.04 -30:33:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:20.92 -30:27:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:41.60 -28:09:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:44.19 -30:29:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:40:44.60 -31:05:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:01.84 -29:19:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:02.29 -27:26:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:42.96 -30:41:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:52.23 -23:10:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:54.80 -31:12:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:58.85 -26:21:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:41:59.49 -29:44:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:01.13 -30:49:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:14.64 -28:57:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:25.84 -22:30:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:39.36 -28:55:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:47.42 -30:19:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:42:51.93 -30:17:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:07.58 -29:20:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:19.89 -27:50:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:36.42 -28:35:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:37.99 -30:11:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:38.83 -26:03:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:45.54 -30:06:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:46.00 -25:35:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:46.48 -25:13:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:43:52.83 -25:04:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:13.38 -22:52:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:17.35 -22:07:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:17.56 -22:06:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:32.91 -30:13:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:34.89 -24:54:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:36.51 -26:29:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:44:43.62 -26:16:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:02.13 -28:54:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:07.48 -26:44:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:13.98 -28:20:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:23.85 -26:22:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:33.74 -29:20:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:41.32 -28:23:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:45:43.14 -26:19:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:02.40 -22:04:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:09.04 -25:26:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:11.16 -29:29:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:15.63 -29:09:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:18.58 -31:02:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:20.11 -27:18:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:25.12 -25:57:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:51.19 -29:48:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:51.68 -31:01:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:52.02 -31:06:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:04.16 -25:48:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:07.52 -29:00:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:10.39 -22:36:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:10.40 -26:35:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:11.52 -31:07:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:15.85 -29:54:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:22.38 -30:41:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:41.73 -26:13:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:41.78 -25:09:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:42.42 -30:55:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:48.96 -27:16:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:51.76 -29:52:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:53.86 -31:06:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:47:54.36 -28:09:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:01.17 -25:41:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:13.17 -23:20:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:19.54 -22:20:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:29.27 -29:37:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:29.85 -24:53:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:34.10 -24:50:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:36.15 -26:02:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:41.84 -24:02:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:44.76 -21:46:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:47.88 -29:45:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:54.85 -22:51:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:57.44 -28:48:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:57.58 -28:48:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:58.98 -21:22:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:07.37 -23:11:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:07.80 -25:08:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:08.47 -27:24:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:09.35 -25:23:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:13.21 -29:25:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:14.37 -27:19:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:14.55 -24:52:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:20.97 -28:13:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:26.10 -22:10:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:46.92 -22:57:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:47.58 -22:57:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:49:47.93 -27:33:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:04.08 -28:20:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:08.90 -22:57:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:10.44 -29:57:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:11.80 -22:54:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:11.85 -29:43:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:15.44 -29:08:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:16.55 -30:23:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:22.30 -28:32:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:22.79 -28:32:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:24.00 -22:41:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:26.68 -21:25:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:27.52 -21:25:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:30.49 -25:41:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:33.82 -22:21:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:41.80 -24:34:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:43.90 -30:56:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:47.24 -25:20:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:57.35 -26:46:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:05.22 -26:20:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:07.46 -27:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:18.21 -25:10:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:21.99 -25:20:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:28.07 -25:27:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:28.12 -27:55:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:28.65 -28:14:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:31.62 -26:38:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:35.64 -29:55:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:44.11 -21:24:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:44.42 -28:06:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:46.27 -22:28:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:48.69 -28:49:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:49.38 -24:30:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:50.67 -22:18:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:54.48 -30:00:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:55.89 -30:58:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:56.57 -21:32:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:56.60 -21:19:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:58.95 -21:22:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:51:59.57 -21:49:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:00.09 -28:32:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:04.57 -28:59:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:05.45 -21:46:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:15.68 -22:40:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:17.12 -22:30:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:17.79 -28:19:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:20.76 -28:41:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:23.00 -29:29:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:23.70 -21:34:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:26.43 -28:44:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:27.08 -25:54:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:28.10 -24:31:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:28.93 -21:24:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:30.19 -22:01:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:32.87 -27:16:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:38.83 -21:45:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:42.70 -28:58:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:44.02 -26:36:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:46.80 -24:05:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:49.56 -21:55:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:50.85 -29:49:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:51.23 -29:29:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:00.64 -27:34:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:00.80 -25:21:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:02.11 -30:03:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:02.49 -26:45:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:03.34 -26:41:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:06.70 -29:42:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:07.37 -29:42:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:07.52 -29:51:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:10.75 -25:41:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:15.95 -23:17:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:18.90 -22:13:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:20.29 -30:49:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:21.60 -29:48:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:23.82 -25:20:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:24.81 -30:14:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:25.14 -25:07:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:53:35.91 -26:13:48.4 -- 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)
15:43:34.12 -28:17:14.9 -- not a known variable star
15:43:46.25 -27:50:10.6 -- a known variable star
15:43:46.99 -28:00:52.3 -- not a known variable star
15:43:56.24 -29:08:47.0 -- not a known variable star
15:44:29.49 -26:37:44.4 -- not a known variable star
15:44:46.19 -29:42:57.7 -- not a known variable star
15:44:51.62 -30:12:55.3 -- not a known variable star
15:44:54.08 -30:06:40.1 -- not a known variable star
15:45:03.08 -29:12:25.9 -- not a known variable star
15:45:07.91 -27:57:05.0 -- not a known variable star
15:45:39.57 -27:45:32.5 -- not a known variable star
15:45:46.99 -28:52:51.0 -- not a known variable star
15:46:13.69 -28:27:47.4 -- not a known variable star
15:46:16.16 -27:50:46.9 -- not a known variable star
15:46:19.66 -27:13:14.2 -- not a known variable star
15:46:39.62 -24:59:07.4 -- not a known variable star
15:46:41.78 -26:10:08.5 -- not a known variable star
15:46:51.43 -28:21:58.1 -- not a known variable star
15:47:03.06 -25:44:33.7 -- not a known variable star
15:47:13.46 -23:02:44.4 -- a known variable star
15:47:28.10 -24:09:46.1 -- not a known variable star
15:47:32.84 -29:05:20.0 -- not a known variable star
15:47:37.33 -22:29:40.5 -- not a known variable star
15:47:38.45 -22:05:25.2 -- a known variable star
15:47:47.45 -27:18:21.4 -- not a known variable star
15:48:11.82 -25:42:19.6 -- not a known variable star
15:48:16.61 -28:18:26.7 -- not a known variable star
15:48:22.29 -28:24:51.2 -- not a known variable star
15:48:30.82 -24:25:40.0 -- not a known variable star
15:48:35.33 -28:31:41.6 -- not a known variable star
15:48:35.89 -27:11:31.0 -- not a known variable star
15:48:44.45 -27:16:29.7 -- not a known variable star
15:49:07.62 -30:12:46.9 -- not a known variable star
15:49:10.22 -27:14:31.1 -- not a known variable star
15:49:12.32 -23:31:25.0 -- not a known variable star
15:49:25.39 -29:27:58.5 -- not a known variable star
15:49:27.63 -27:46:20.6 -- not a known variable star
15:49:28.26 -25:56:51.9 -- not a known variable star
15:49:56.64 -25:22:14.1 -- a known variable star
15:49:58.93 -23:14:53.7 -- not a known variable star
15:50:03.55 -27:32:21.7 -- a known variable star
15:50:09.06 -23:33:22.9 -- a known variable star
15:50:13.58 -26:44:26.1 -- not a known variable star
15:50:13.76 -29:38:23.2 -- a known variable star
15:50:20.73 -21:17:01.1 -- a known variable star
15:50:26.53 -23:42:09.1 -- a known variable star
15:50:27.14 -21:40:20.2 -- not a known variable star
15:50:28.72 -28:37:06.5 -- not a known variable star
15:50:30.03 -29:11:38.0 -- not a known variable star
15:50:58.03 -20:48:32.4 -- not a known variable star
15:51:23.37 -21:43:04.6 -- a known variable star
15:51:36.51 -28:19:07.7 -- not a known variable star
15:51:52.27 -28:56:46.4 -- not a known variable star
15:52:04.50 -21:11:00.6 -- not a known variable star
15:52:16.10 -20:33:54.5 -- not a known variable star
15:52:38.30 -27:32:19.4 -- not a known variable star
15:52:50.84 -27:25:24.9 -- not a known variable star
15:52:57.93 -20:46:48.5 -- not a known variable star
15:53:06.77 -29:13:38.0 -- not a known variable star
15:53:07.65 -30:18:19.2 -- not a known variable star
15:53:21.42 -21:06:10.6 -- not a known variable star
15:53:25.97 -29:39:59.3 -- not a known variable star
15:53:36.45 -27:49:21.2 -- a known variable star
15:53:42.53 -29:56:33.4 -- not a known variable star
15:53:43.63 -29:10:22.3 -- not a known variable star
15:53:46.10 -27:16:25.1 -- a known variable star
15:53:56.23 -29:50:40.8 -- not a known variable star
15:54:26.43 -27:36:03.4 -- a known variable star
15:54:49.42 -30:25:54.7 -- not a known variable star
15:54:53.43 -28:47:47.8 -- a known variable star
15:55:05.01 -29:58:22.0 -- not a known variable star
15:55:07.43 -24:57:15.4 -- not a known variable star
15:55:20.65 -27:31:47.7 -- not a known variable star
15:55:59.06 -27:23:29.9 -- not a known variable star
15:56:13.09 -23:17:57.5 -- a known variable star
15:56:21.89 -29:57:32.9 -- not a known variable star
15:57:02.38 -28:56:18.8 -- a known variable star
15:57:02.62 -21:08:35.9 -- not a known variable star
15:57:19.63 -21:00:25.4 -- not a known variable star
15:57:37.63 -20:37:03.3 -- not a known variable star
15:58:10.89 -26:58:07.2 -- a known variable star
15:58:44.21 -21:46:42.4 -- not a known variable star
15:59:14.11 -28:41:19.5 -- not a known variable star
15:59:25.19 -30:07:27.5 -- not a known variable star
15:59:26.63 -28:34:42.2 -- not a known variable star
16:00:10.44 -27:06:36.6 -- not a known variable star
16:00:33.92 -27:50:41.7 -- not a known variable star
16:01:03.66 -25:07:15.5 -- not a known variable star
16:01:07.76 -27:36:05.5 -- not a known variable star
16:02:07.12 -28:54:34.3 -- not a known variable star
16:02:18.90 -20:39:23.2 -- not a known variable star
16:02:38.92 -25:41:54.2 -- a known variable star
16:02:47.56 -21:35:35.6 -- not a known variable star
16:02:56.45 -30:30:55.1 -- not a known variable star
16:03:13.83 -28:26:08.0 -- not a known variable star
16:03:29.05 -25:11:27.5 -- a known variable star
16:03:31.22 -28:07:05.4 -- not a known variable star
16:03:43.99 -29:39:59.2 -- not a known variable star
16:03:55.48 -24:32:34.5 -- not a known variable star
16:04:10.16 -22:45:50.0 -- not a known variable star
16:04:17.61 -30:47:14.9 -- not a known variable star
16:05:19.32 -30:42:02.3 -- a known variable star
16:06:34.08 -29:10:15.5 -- not a known variable star
16:07:01.00 -28:01:35.1 -- not a known variable star
16:07:46.50 -30:41:54.8 -- not a known variable star
16:07:52.10 -26:57:35.6 -- not a known variable star
16:08:06.13 -28:47:30.5 -- not a known variable star
16:10:05.64 -28:37:12.8 -- not a known variable star
16:11:18.88 -23:42:24.9 -- a known variable star
16:12:23.58 -21:40:12.9 -- a known variable star
16:12:51.64 -24:45:30.3 -- not a known variable star
16:13:08.91 -21:25:56.2 -- not a known variable star
16:15:26.23 -21:10:42.1 -- not a known variable star
16:15:49.28 -30:17:29.3 -- not a known variable star
16:16:10.20 -28:21:22.8 -- a known variable star
16:17:14.07 -21:58:16.4 -- not a known variable star
16:18:32.15 -28:19:41.4 -- a known variable star
16:19:12.54 -31:06:40.5 -- not a known variable star
16:19:42.33 -25:34:49.3 -- not a known variable star
16:19:44.43 -28:59:29.8 -- not a known variable star
16:19:49.03 -22:17:39.4 -- not a known variable star
16:20:22.29 -25:07:09.3 -- not a known variable star
16:21:15.09 -29:00:34.9 -- not a known variable star
16:21:15.35 -29:00:17.6 -- not a known variable star
16:21:41.99 -25:22:56.4 -- not a known variable star
16:22:54.64 -26:55:12.2 -- not a known variable star
16:23:17.83 -29:53:49.9 -- a known variable star
16:23:35.43 -26:31:39.8 -- a known variable star
16:23:38.72 -25:46:45.0 -- not a known variable star
16:23:42.41 -29:01:39.2 -- not a known variable star
16:23:58.00 -26:39:22.5 -- not a known variable star
16:24:16.86 -31:10:19.4 -- not a known variable star
16:24:27.62 -29:35:28.2 -- not a known variable star
16:24:30.94 -29:27:57.1 -- not a known variable star
16:24:50.84 -31:02:24.8 -- not a known variable star
16:26:48.51 -30:35:37.0 -- not a known variable star
16:27:10.40 -29:24:39.5 -- not a known variable star
16:27:12.77 -26:01:17.3 -- not a known variable star
16:28:07.17 -26:26:38.7 -- not a known variable star
16:29:18.48 -30:20:42.1 -- not a known variable star
16:29:27.26 -27:33:28.7 -- not a known variable star
16:30:50.79 -26:38:04.3 -- not a known variable star
16:31:27.14 -31:12:46.3 -- not a known variable star
16:32:46.15 -27:17:49.5 -- a known variable star
16:33:01.34 -25:57:40.9 -- not a known variable star
16:33:52.07 -26:41:24.5 -- not a known variable star
16:33:53.68 -28:12:39.2 -- not a known variable star
16:34:10.65 -30:41:25.2 -- not a known variable star
16:35:47.49 -28:43:59.3 -- not a known variable star
16:35:56.46 -26:49:37.3 -- not a known variable star
16:36:11.89 -31:01:26.4 -- a known variable star
16:36:31.05 -27:21:46.1 -- not a known variable star
16:36:31.43 -27:21:34.2 -- not a known variable star
16:36:50.02 -26:45:10.9 -- not a known variable star
16:37:29.39 -28:31:54.7 -- a known variable star
16:37:35.07 -24:52:43.0 -- not a known variable star
16:37:47.50 -27:20:55.0 -- a known variable star
16:38:11.01 -25:53:54.7 -- not a known variable star
16:38:24.19 -25:03:02.5 -- not a known variable star
16:39:12.36 -30:24:21.1 -- a known variable star
16:39:14.52 -30:24:21.8 -- a known variable star
16:39:22.04 -30:33:06.5 -- not a known variable star
16:40:20.92 -30:27:12.1 -- not a known variable star
16:40:41.60 -28:09:47.8 -- not a known variable star
16:40:44.19 -30:29:36.1 -- not a known variable star
16:40:44.60 -31:05:26.1 -- not a known variable star
16:41:01.84 -29:19:59.2 -- not a known variable star
16:41:02.29 -27:26:49.2 -- a known variable star
16:41:42.96 -30:41:04.3 -- not a known variable star
16:41:52.23 -23:10:25.4 -- not a known variable star
16:41:54.80 -31:12:09.5 -- a known variable star
16:41:58.85 -26:21:43.4 -- not a known variable star
16:41:59.49 -29:44:47.8 -- not a known variable star
16:42:01.13 -30:49:13.3 -- not a known variable star
16:42:14.64 -28:57:21.4 -- not a known variable star
16:42:25.84 -22:30:19.8 -- not a known variable star
16:42:39.36 -28:55:45.7 -- a known variable star
16:42:47.42 -30:19:03.0 -- a known variable star
16:42:51.93 -30:17:17.3 -- a known variable star
16:43:07.58 -29:20:35.2 -- not a known variable star
16:43:19.89 -27:50:23.8 -- not a known variable star
16:43:36.42 -28:35:42.0 -- not a known variable star
16:43:37.99 -30:11:07.0 -- not a known variable star
16:43:38.83 -26:03:37.7 -- not a known variable star
16:43:45.54 -30:06:17.2 -- not a known variable star
16:43:46.00 -25:35:49.2 -- not a known variable star
16:43:46.48 -25:13:34.2 -- not a known variable star
16:43:52.83 -25:04:31.2 -- not a known variable star
16:44:13.38 -22:52:49.5 -- not a known variable star
16:44:17.35 -22:07:01.0 -- a known variable star
16:44:17.56 -22:06:56.7 -- a known variable star
16:44:32.91 -30:13:50.9 -- a known variable star
16:44:34.89 -24:54:56.8 -- not a known variable star
16:44:36.51 -26:29:54.1 -- not a known variable star
16:44:43.62 -26:16:33.3 -- a known variable star
16:45:02.13 -28:54:23.9 -- a known variable star
16:45:07.48 -26:44:16.6 -- a known variable star
16:45:13.98 -28:20:12.5 -- not a known variable star
16:45:23.85 -26:22:16.2 -- not a known variable star
16:45:33.74 -29:20:02.2 -- not a known variable star
16:45:41.32 -28:23:19.5 -- not a known variable star
16:45:43.14 -26:19:30.8 -- not a known variable star
16:46:02.40 -22:04:22.4 -- not a known variable star
16:46:09.04 -25:26:40.9 -- not a known variable star
16:46:11.16 -29:29:07.1 -- a known variable star
16:46:15.63 -29:09:39.9 -- not a known variable star
16:46:18.58 -31:02:19.5 -- a known variable star
16:46:20.11 -27:18:39.2 -- not a known variable star
16:46:25.12 -25:57:10.1 -- not a known variable star
16:46:51.19 -29:48:14.3 -- a known variable star
16:46:51.68 -31:01:17.6 -- not a known variable star
16:46:52.02 -31:06:41.6 -- not a known variable star
16:47:04.16 -25:48:41.1 -- not a known variable star
16:47:07.52 -29:00:50.9 -- a known variable star
16:47:10.39 -22:36:47.2 -- not a known variable star
16:47:10.40 -26:35:34.9 -- not a known variable star
16:47:11.52 -31:07:37.1 -- not a known variable star
16:47:15.85 -29:54:43.8 -- a known variable star
16:47:22.38 -30:41:08.3 -- not a known variable star
16:47:41.73 -26:13:54.6 -- a known variable star
16:47:41.78 -25:09:59.4 -- a known variable star
16:47:42.42 -30:55:25.9 -- not a known variable star
16:47:48.96 -27:16:00.3 -- not a known variable star
16:47:51.76 -29:52:43.9 -- not a known variable star
16:47:53.86 -31:06:09.0 -- a known variable star
16:47:54.36 -28:09:24.7 -- a known variable star
16:48:01.17 -25:41:15.8 -- not a known variable star
16:48:13.17 -23:20:44.0 -- not a known variable star
16:48:19.54 -22:20:22.5 -- not a known variable star
16:48:29.27 -29:37:42.0 -- not a known variable star
16:48:29.85 -24:53:56.9 -- not a known variable star
16:48:34.10 -24:50:18.3 -- not a known variable star
16:48:36.15 -26:02:25.4 -- not a known variable star
16:48:41.84 -24:02:01.8 -- not a known variable star
16:48:44.76 -21:46:49.1 -- not a known variable star
16:48:47.88 -29:45:43.7 -- not a known variable star
16:48:54.85 -22:51:09.3 -- not a known variable star
16:48:57.44 -28:48:25.8 -- not a known variable star
16:48:57.58 -28:48:19.0 -- not a known variable star
16:48:58.98 -21:22:51.1 -- not a known variable star
16:49:07.37 -23:11:32.2 -- a known variable star
16:49:07.80 -25:08:26.0 -- a known variable star
16:49:08.47 -27:24:45.1 -- a known variable star
16:49:09.35 -25:23:43.8 -- a known variable star
16:49:13.21 -29:25:16.6 -- not a known variable star
16:49:14.37 -27:19:36.7 -- a known variable star
16:49:14.55 -24:52:12.0 -- not a known variable star
16:49:20.97 -28:13:29.4 -- not a known variable star
16:49:26.10 -22:10:24.6 -- not a known variable star
16:49:46.92 -22:57:17.9 -- a known variable star
16:49:47.58 -22:57:12.9 -- a known variable star
16:49:47.93 -27:33:22.9 -- not a known variable star
16:50:04.08 -28:20:07.2 -- not a known variable star
16:50:08.90 -22:57:21.4 -- not a known variable star
16:50:10.44 -29:57:32.8 -- a known variable star
16:50:11.80 -22:54:53.5 -- not a known variable star
16:50:11.85 -29:43:31.3 -- not a known variable star
16:50:15.44 -29:08:36.9 -- not a known variable star
16:50:16.55 -30:23:53.1 -- not a known variable star
16:50:22.30 -28:32:21.1 -- not a known variable star
16:50:22.79 -28:32:20.3 -- not a known variable star
16:50:24.00 -22:41:40.0 -- not a known variable star
16:50:26.68 -21:25:56.3 -- not a known variable star
16:50:27.52 -21:25:47.3 -- not a known variable star
16:50:30.49 -25:41:49.7 -- not a known variable star
16:50:33.82 -22:21:20.6 -- not a known variable star
16:50:41.80 -24:34:10.1 -- a known variable star
16:50:43.90 -30:56:36.7 -- not a known variable star
16:50:47.24 -25:20:34.5 -- not a known variable star
16:50:57.35 -26:46:44.2 -- a known variable star
16:51:05.22 -26:20:59.4 -- not a known variable star
16:51:07.46 -27:20:02.8 -- not a known variable star
16:51:18.21 -25:10:26.1 -- a known variable star
16:51:21.99 -25:20:18.3 -- not a known variable star
16:51:28.07 -25:27:43.8 -- a known variable star
16:51:28.12 -27:55:29.0 -- not a known variable star
16:51:28.65 -28:14:26.0 -- a known variable star
16:51:31.62 -26:38:49.8 -- not a known variable star
16:51:35.64 -29:55:36.7 -- not a known variable star
16:51:44.11 -21:24:51.7 -- not a known variable star
16:51:44.42 -28:06:23.1 -- not a known variable star
16:51:46.27 -22:28:36.5 -- not a known variable star
16:51:48.69 -28:49:04.8 -- a known variable star
16:51:49.38 -24:30:49.6 -- not a known variable star
16:51:50.67 -22:18:52.1 -- not a known variable star
16:51:54.48 -30:00:45.4 -- not a known variable star
16:51:55.89 -30:58:30.0 -- not a known variable star
16:51:56.57 -21:32:40.3 -- not a known variable star
16:51:56.60 -21:19:44.4 -- not a known variable star
16:51:58.95 -21:22:10.7 -- not a known variable star
16:51:59.57 -21:49:38.2 -- not a known variable star
16:52:00.09 -28:32:13.1 -- not a known variable star
16:52:04.57 -28:59:34.4 -- a known variable star
16:52:05.45 -21:46:49.2 -- not a known variable star
16:52:15.68 -22:40:30.2 -- not a known variable star
16:52:17.12 -22:30:35.4 -- not a known variable star
16:52:17.79 -28:19:33.9 -- not a known variable star
16:52:20.76 -28:41:48.4 -- a known variable star
16:52:23.00 -29:29:23.6 -- not a known variable star
16:52:23.70 -21:34:50.8 -- not a known variable star
16:52:26.43 -28:44:09.7 -- not a known variable star
16:52:27.08 -25:54:30.4 -- not a known variable star
16:52:28.10 -24:31:50.9 -- not a known variable star
16:52:28.93 -21:24:57.2 -- not a known variable star
16:52:30.19 -22:01:24.3 -- a known variable star
16:52:32.87 -27:16:35.1 -- a known variable star
16:52:38.83 -21:45:47.4 -- a known variable star
16:52:42.70 -28:58:50.8 -- a known variable star
16:52:44.02 -26:36:32.6 -- not a known variable star
16:52:46.80 -24:05:24.5 -- not a known variable star
16:52:49.56 -21:55:47.7 -- a known variable star
16:52:50.85 -29:49:05.4 -- not a known variable star
16:52:51.23 -29:29:33.0 -- a known variable star
16:53:00.64 -27:34:26.9 -- not a known variable star
16:53:00.80 -25:21:14.1 -- not a known variable star
16:53:02.11 -30:03:48.3 -- not a known variable star
16:53:02.49 -26:45:29.8 -- not a known variable star
16:53:03.34 -26:41:13.6 -- not a known variable star
16:53:06.70 -29:42:18.7 -- a known variable star
16:53:07.37 -29:42:10.4 -- a known variable star
16:53:07.52 -29:51:08.5 -- not a known variable star
16:53:10.75 -25:41:37.8 -- not a known variable star
16:53:15.95 -23:17:12.8 -- not a known variable star
16:53:18.90 -22:13:08.4 -- not a known variable star
16:53:20.29 -30:49:22.1 -- a known variable star
16:53:21.60 -29:48:56.7 -- not a known variable star
16:53:23.82 -25:20:45.7 -- a known variable star
16:53:24.81 -30:14:14.2 -- not a known variable star
16:53:25.14 -25:07:59.7 -- not a known variable star
16:53:35.91 -26:13:48.4 -- not a known variable star
Found 252 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
330 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 330 (excluding asteroids and hot pixels, 252 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461150.92596440 -observatory V36
00:31:37.19 +00:34:00.8 Mercury (-0.1mag)
03:30:28.55 +19:26:17.4 Venus (-3.9mag)
00:30:24.23 +02:14:34.4 Mars (1.2mag)
07:14:44.68 +22:42:41.0 Jupiter (-2.1mag)
00:31:08.37 +01:01:08.2 Saturn (0.9mag)
03:48:38.75 +19:50:30.0 Uranus (5.8mag)
00:11:24.69 -00:11:47.0 Neptune (7.8mag)
20:33:55.75 -22:52:52.5 Pluto (14.5mag)
04:34:02.76 +26:14:09.6 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 362 Apr 20 05:16 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461150.92596440:
07:14:46.97 +22:42:33.6 Io (5.8mag)
07:14:57.14 +22:42:13.2 Europa (5.9mag)
07:14:37.94 +22:43:01.9 Ganymede (5.4mag)
07:14:44.52 +22:42:31.9 Callisto (6.6mag)
07:17:52.68 +22:28:20.0 Himalia (15.4mag)
07:14:44.40 +22:42:43.8 Thebe (16.3mag)
07:18:09.39 +22:58:40.1 Elara (17.3mag)
07:13:55.63 +23:20:22.4 Pasiphae (17.4mag)
07:22:58.26 +22:41:06.9 Carme (18.5mag)
00:30:59.05 +01:01:21.1 Titan (8.8mag)
00:31:05.83 +01:01:14.5 Rhea (10.1mag)
00:30:42.11 +01:00:35.1 Iapetus (11.5mag)
00:31:00.35 +01:01:33.5 Hyperion (14.8mag)
00:32:41.64 +01:09:27.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 20 05:16 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461150.92596440:
15:55:30.48 -19:13:45.0 JWST
18:31:51.54 +27:01:41.0 Chandra
09:03:15.97 -51:35:07.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 20 05:16 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461150.92596440 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:35.55 -29:02:49.1 13.9mag P/2010 H2 (Vales)
05:10:00.08 -69:27:29.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:27.47 +31:28:07.5 17.2mag C/2017 K2 (PANSTARRS)
17:29:53.71 +11:03:56.8 17.6mag C/2021 G2 (ATLAS)
23:11:19.78 +29:24:36.6 17.1mag C/2022 E2 (ATLAS)
04:34:26.17 +26:09:20.5 16.1mag C/2022 N2 (PANSTARRS)
09:04:30.11 +32:01:52.8 16.3mag C/2022 QE78 (ATLAS)
08:31:51.26 +00:18:14.8 17.4mag C/2022 R6 (PANSTARRS)
18:52:33.95 +18:53:54.3 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:09.92 -11:27:22.9 17.5mag P/2023 B1 (PANSTARRS)
09:05:44.79 -11:11:20.0 17.7mag C/2023 F3 (ATLAS)
21:58:25.90 +63:10:29.0 17.5mag C/2023 H5 (Lemmon)
19:15:02.26 -03:49:00.4 14.1mag C/2023 R1 (PANSTARRS)
21:20:00.65 +86:31:59.1 17.8mag C/2023 X2 (Lemmon)
06:20:14.05 +63:30:01.8 17.2mag C/2024 A1 (ATLAS)
05:22:32.45 +19:40:57.4 11.3mag C/2024 E1 (Wierzchos)
16:16:19.15 +07:06:41.7 17.3mag C/2024 G6 (ATLAS)
20:21:54.68 +16:29:38.5 14.5mag C/2024 J3 (ATLAS)
03:30:23.49 -21:43:25.8 16.3mag C/2024 T5 (ATLAS)
05:20:32.09 +44:13:03.0 17.7mag C/2025 J1 (Borisov)
13:20:41.52 +48:00:16.4 15.4mag C/2025 L1 (ATLAS)
03:32:25.65 -26:55:19.1 17.9mag C/2025 Q3 (ATLAS)
00:36:03.77 +16:01:38.8 8.0mag C/2025 R3 (PANSTARRS)
12:52:13.41 +03:16:23.9 17.4mag C/2025 Y1 (ATLAS)
03:59:39.72 +02:14:24.5 14.5mag C/2026 A1 (MAPS)
00:11:53.77 +37:59:45.4 14.7mag C/2026 B2 (Sun-Gao)
18:51:31.86 -09:28:43.6 11.6mag 10P/Tempel
14:54:15.07 +02:43:05.5 14.4mag 24P/Schaumasse
11:01:42.87 -01:23:25.3 15.7mag 29P/Schwassmann-Wachmann
10:37:36.76 -03:46:05.3 17.0mag 43P/Wolf-Harrington
01:55:32.57 +18:14:09.2 17.3mag 47P/Ashbrook-Jackson
07:19:05.12 +36:02:56.8 17.0mag 63P/Wild
23:34:38.24 -10:55:38.0 15.7mag 65P/Gunn
04:15:14.84 +22:44:05.4 15.9mag 76P/West-Kohoutek-Ikemura
01:15:25.00 +09:05:32.1 14.3mag 78P/Gehrels
23:16:12.95 -08:04:54.6 14.7mag 88P/Howell
02:23:04.21 +21:47:49.3 15.1mag 93P/Lovas
05:03:18.27 +32:30:42.8 16.1mag 123P/West-Hartley
08:33:49.05 +36:19:17.9 16.2mag 124P/Mrkos
02:40:05.99 +14:51:26.9 16.4mag 128P/Shoemaker-Holt
02:56:15.06 +15:01:13.1 17.5mag 131P/Mueller
01:49:41.36 +14:41:13.8 10.5mag 141P/Machholz
01:57:55.40 +06:31:13.0 10.5mag 141P-A/Machholz
00:41:17.14 +02:18:17.8 12.3mag 141P-D/Machholz
02:28:30.27 +08:16:11.2 17.9mag 141P-I/Machholz
01:14:46.50 +00:42:28.3 15.0mag 162P/SidingSpring
14:43:37.08 +00:21:07.2 17.8mag 210P/Christensen
21:51:16.04 -10:23:25.4 17.7mag 218P/LINEAR
17:17:17.34 -13:23:40.9 16.1mag 235P/LINEAR
05:44:07.81 +35:00:26.5 16.8mag 240P/NEAT
07:40:48.00 -04:42:15.1 17.8mag 242P/Spahr
22:27:59.20 -19:46:07.3 17.8mag 260P/McNaught
02:07:20.14 +21:34:01.8 18.0mag 295P/LINEAR
15:40:47.91 +07:16:12.6 17.5mag 391P/Kowalski
07:36:01.08 +21:22:23.3 17.7mag 450P/LONEOS
05:42:24.90 +44:46:25.8 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 20 05:16 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
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
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
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
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
-rw-r--r-- 1 apache apache 5.8K Apr 20 05:16 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 20 05:16 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:24:19.761 -36:04:17.66 AT 2026jke 2026-04-06.51 19.98
11:16:25.694 -50:15:29.19 AT 2026jkd 2026-03-28.49 19.6
11:43:56.670 -49:03:17.42 AT 2026jkc 2026-04-12.46 19.35
11:38:21.891 -50:43:06.73 SN 2026jkb 2026-04-12.46 18.57
08:19:14.303 -28:43:36.53 AT 2026jka 2026-04-11.37 19.87
07:49:32.473 -24:44:26.65 AT 2026jjz 2026-04-12.39 18.98
14:44:18.498 -44:01:13.70 AT 2026jjy 2026-04-09.61 19.64
08:53:40.997 -38:26:31.85 AT 2026jjx 2026-03-23.40 20
12:26:02.763 -33:38:07.00 AT 2026jjw 2026-04-09.56 20.25
11:26:18.195 +19:38:31.94 AT 2026jjv 2026-04-06.91 19.81
11:33:29.132 -27:21:16.23 AT 2026jju 2026-04-12.45 19.32
12:15:03.964 -49:33:10.66 AT 2026jjt 2026-04-12.17 19.263
17:17:54.158 -75:07:32.46 AT 2026jjs 2026-04-12.30 19.194
08:35:23.434 +10:31:04.49 AT 2026jjr 2026-04-11.93 19.882
09:53:48.141 +08:12:51.52 AT 2026jjq 2026-04-11.92 20.219
12:47:33.422 +00:05:56.15 AT 2026jjp 2026-04-12.03 20.061
16:10:20.836 -68:49:59.48 AT 2026jjo 2026-04-12.26 19.161
18:36:22.563 -76:59:23.30 AT 2026jjn 2026-04-12.30 18.78
18:56:03.327 -40:52:01.58 AT 2026jjm 2026-04-12.35 18.51
16:42:43.663 -75:30:11.13 AT 2026jjl 2026-04-12.27 19.255
-rw-r--r-- 1 apache apache 30K Apr 20 05:16 tns_transients_list.txt
