This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg
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 3112515039375055744,2461147.6171,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112515039375055744 20260417.1171 13.64CV 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
target,2461147.6171,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.56CV 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
target,2461147.6171,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.51CV 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 3106277789090410496,2461147.6171,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106277789090410496 20260417.1171 13.59CV 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
target,2461147.6171,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.4533-02.0789,2461147.6171,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.4533-02.0789 20260417.1171 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114532097757533440,2461147.6171,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114532097757533440 20260417.1171 13.46CV 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 3108998839851392768,2461147.6171,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108998839851392768 20260417.1171 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4545-03.0133,2461147.6171,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4545-03.0133 20260417.1171 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6668-01.9250,2461147.6171,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6668-01.9250 20260417.1171 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112835443935349632,2461147.6171,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112835443935349632 20260417.1171 13.42CV 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 3112549914511382144,2461147.6171,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112549914511382144 20260417.1171 13.13CV 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 3102837412905531904,2461147.6171,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102837412905531904 20260417.1171 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6713+00.6013,2461147.6171,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6713+00.6013 20260417.1171 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112803528038358144,2461147.6171,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112803528038358144 20260417.1171 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112672888012933248,2461147.6171,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112672888012933248 20260417.1171 13.08CV 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 3125582872512184960,2461147.6171,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125582872512184960 20260417.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109012029688529536,2461147.6171,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109012029688529536 20260417.1171 13.06CV 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
target,2461147.6171,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.4965-00.6001,2461147.6171,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.4965-00.6001 20260417.1171 12.99CV 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
ATO J106.9991-01.5167,2461147.6171,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.9991-01.5167 20260417.1171 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7819-00.2754,2461147.6171,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.7819-00.2754 20260417.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1118-02.4298,2461147.6171,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1118-02.4298 20260417.1171 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109606113865803136,2461147.6171,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109606113865803136 20260417.1171 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3109005952316009984,2461147.6171,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109005952316009984 20260417.1171 12.74CV 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
ATO J105.1615-01.5148,2461147.6171,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1615-01.5148 20260417.1171 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3112074478812987264,2461147.6171,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112074478812987264 20260417.1171 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119497625408710400,2461147.6171,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119497625408710400 20260417.1171 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3112644713029544064,2461147.6171,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112644713029544064 20260417.1171 12.69CV 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 3112460441750884224,2461147.6171,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112460441750884224 20260417.1171 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.70CV 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
ATO J107.1974-03.7119,2461147.6171,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1974-03.7119 20260417.1171 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3502-00.8380,2461147.6171,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3502-00.8380 20260417.1171 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108734682183880576,2461147.6171,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108734682183880576 20260417.1171 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114694099624336256,2461147.6171,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114694099624336256 20260417.1171 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112640181842895232,2461147.6171,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112640181842895232 20260417.1171 12.45CV 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
ATO J105.8499-02.8303,2461147.6171,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.8499-02.8303 20260417.1171 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0658496-010628,2461147.6171,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0658496-010628 20260417.1171 12.45CV 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 3109471389332247552,2461147.6171,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109471389332247552 20260417.1171 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7305-03.0153,2461147.6171,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7305-03.0153 20260417.1171 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 3112992025564253184,2461147.6171,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112992025564253184 20260417.1171 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.15CV 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 J105.9536-03.3472,2461147.6171,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9536-03.3472 20260417.1171 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107979214615799680,2461147.6171,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107979214615799680 20260417.1171 12.01CV 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 J106.4621-02.0972,2461147.6171,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4621-02.0972 20260417.1171 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 3112231300951646592,2461147.6171,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112231300951646592 20260417.1171 12.06CV 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
ATO J103.6522-00.6011,2461147.6171,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6522-00.6011 20260417.1171 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 3109467884639416576,2461147.6171,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109467884639416576 20260417.1171 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
ATO J105.3280-03.1171,2461147.6171,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3280-03.1171 20260417.1171 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
ATO J107.2696-02.4769,2461147.6171,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2696-02.4769 20260417.1171 12.06CV 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 3101962171592322688,2461147.6171,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101962171592322688 20260417.1171 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
Gaia DR3 3108624627942178688,2461147.6171,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108624627942178688 20260417.1171 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065448.56+002321.1,2461147.6171,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065448.56+002321.1 20260417.1171 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
Gaia DR3 3125504223071142784,2461147.6171,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125504223071142784 20260417.1171 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109532137349277568,2461147.6171,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109532137349277568 20260417.1171 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 J104.2021+00.7657,2461147.6171,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2021+00.7657 20260417.1171 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112314039208032000,2461147.6171,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112314039208032000 20260417.1171 12.70CV 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
ATO J100.3363-00.8503,2461147.6171,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.3363-00.8503 20260417.1171 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
Gaia DR3 3115521344683433984,2461147.6171,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115521344683433984 20260417.1171 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3108690216381698304,2461147.6171,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108690216381698304 20260417.1171 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1999-01.8082,2461147.6171,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1999-01.8082 20260417.1171 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.69CV 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 3112121349793909632,2461147.6171,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112121349793909632 20260417.1171 12.95CV 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
target,2461147.6171,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 12.74CV 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
ATO J105.5594-03.0943,2461147.6171,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5594-03.0943 20260417.1171 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3112948251257159808,2461147.6171,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112948251257159808 20260417.1171 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113319370792417024,2461147.6171,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113319370792417024 20260417.1171 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3126153111029053568,2461147.6171,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126153111029053568 20260417.1171 12.82CV 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 J106.0676-03.0161,2461147.6171,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0676-03.0161 20260417.1171 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5787+00.4180,2461147.6171,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5787+00.4180 20260417.1171 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102653145931456000,2461147.6171,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102653145931456000 20260417.1171 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6739-02.7997,2461147.6171,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6739-02.7997 20260417.1171 12.74CV 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 3107920768701471488,2461147.6171,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107920768701471488 20260417.1171 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.3028-01.1286,2461147.6171,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.3028-01.1286 20260417.1171 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MGAB-V1900,2461147.6171,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MGAB-V1900 20260417.1171 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125637852391270784,2461147.6171,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125637852391270784 20260417.1171 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114733033507384064,2461147.6171,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114733033507384064 20260417.1171 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3042-01.5835,2461147.6171,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3042-01.5835 20260417.1171 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114460526421262848,2461147.6171,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114460526421262848 20260417.1171 13.08CV 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 3109297872654329344,2461147.6171,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109297872654329344 20260417.1171 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7477+00.2283,2461147.6171,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7477+00.2283 20260417.1171 12.99CV 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
ATO J104.7533-02.6015,2461147.6171,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7533-02.6015 20260417.1171 12.95CV 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 3108863080225629056,2461147.6171,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108863080225629056 20260417.1171 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125762818759969664,2461147.6171,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125762818759969664 20260417.1171 13.03CV 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 J102.9043-01.6544,2461147.6171,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9043-01.6544 20260417.1171 12.99CV 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
ATO J104.2307+00.9114,2461147.6171,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2307+00.9114 20260417.1171 13.08CV 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
ATO J106.5054-02.0639,2461147.6171,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5054-02.0639 20260417.1171 13.03CV 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 3109005849236806016,2461147.6171,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109005849236806016 20260417.1171 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3527+01.6546,2461147.6171,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.3527+01.6546 20260417.1171 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5059+00.7529,2461147.6171,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5059+00.7529 20260417.1171 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113219246514568576,2461147.6171,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260417.1171 13.13CV 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
target,2461147.6171,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.03CV 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 J105.4874+01.2254,2461147.6171,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.4874+01.2254 20260417.1171 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112503842401083904,2461147.6171,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112503842401083904 20260417.1171 13.03CV 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 3112223325200684160,2461147.6171,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112223325200684160 20260417.1171 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5973-05.9047,2461147.6171,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5973-05.9047 20260417.1171 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0837+00.8377,2461147.6171,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0837+00.8377 20260417.1171 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3335+01.2242,2461147.6171,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.3335+01.2242 20260417.1171 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112396051604609408,2461147.6171,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112396051604609408 20260417.1171 13.22CV 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 3107565214132271488,2461147.6171,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107565214132271488 20260417.1171 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.6630+01.9547,2461147.6171,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.6630+01.9547 20260417.1171 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7913+00.9506,2461147.6171,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.7913+00.9506 20260417.1171 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 17.1171 2461147.6171 13.44 07:02:14.11 -00:34:58.4
214.68248 2.13605 galactic Mon Second-epoch detections are separated by 2.7" and 4.9 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 3112609116339522816 | 07:02:14.11 -00:34:58.4 (user input) | 2021A&A...648A..44M | | (position from user input) (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 3112609116339522816,2461147.6171,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3112609116339522816 20260417.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6171,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.58CV 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
target,2461147.6171,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.54CV 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 J104.9413-02.3695,2461147.6171,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9413-02.3695 20260417.1171 13.51CV 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
target,2461147.6171,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1171 13.63CV 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
Date (UTC)
JD(UTC)
mag.
R.A. & Dec.(J2000)
X & Y (pix)
Image
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.0276-01.3052,2461147.6171,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0276-01.3052 20260417.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461147.61741014 17.04.2026 02:48:54.236 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 8 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): 29341
Objects passed selection criteria: 29233
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 21855.8
Average stars matched: 19827.8 (90.721 %)
Memory usage VmPeak: 131292 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 Thu Apr 16 21:56:54 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461147.61741014 17.04.2026 02:48:54.236 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 321
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 140 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): 220543
Objects passed selection criteria: 219913
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 170937
Average stars matched: 154648 (90.4706 %)
Memory usage VmPeak: 1963288 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 Thu Apr 16 22:00:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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: 2461147.61671826
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:27.544 -01:59:39.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:27.544 -01:59:39.08
Angular distance between the image centers 0.0655 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:27.010 -02:00:06.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:27.010 -02:00:06.33
Angular distance between the image centers 0.0670 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 06:51:27.544 -01:59:39.08
Second-epoch second image center 06:51:27.010 -02:00:06.33
Angular distance between the image centers 0.00789 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.FWe9zVkj9y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.gyBSNtUryj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits &> /tmp/tmp.ZcmHRA4FNZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits &> /tmp/tmp.DSsmwm1cZ4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.4 pix fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.5 mag. fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
14.4 mag. fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FWe9zVkj9y (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.gyBSNtUryj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZcmHRA4FNZ (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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2049, passed=22343
Got 22343 stars (including 20274 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 22343 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 920 matched stars entering correct_measured_positions(), 21859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 21861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 21861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 918 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.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.DSsmwm1cZ4 (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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1482, passed=16947
Got 16947 stars (including 15451 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 16947 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 16652 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 16653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 16653 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51877.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51877_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 51877_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:07.45 -01:28:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.331 3106909213700454528 099.53163508451 -01.46839862892 11.0128 10.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54245_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 54245_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:13.63 -02:21:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57420_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 57420_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:45.27 +00:41:47.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:27.544 -01:59:39.08 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:27.544 -01:59:39.08
Angular distance between the image centers 0.0655 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:27.010 -02:00:06.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:27.010 -02:00:06.33
Angular distance between the image centers 0.0670 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 06:51:27.544 -01:59:39.08
Second-epoch second image center 06:51:27.010 -02:00:06.33
Angular distance between the image centers 0.00789 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.YuR6KmfYVL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.p0vtAhL7f8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits &> /tmp/tmp.uD8f1Wwk3j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits &> /tmp/tmp.iWHI4fbXQr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 248 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
2.3 pix fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.8 mag. fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
13.7 mag. fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (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.YuR6KmfYVL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.p0vtAhL7f8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uD8f1Wwk3j (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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=23313, passed=168968
Got 168968 stars (including 145483 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 168968 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 166069 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 166070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 166070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 918 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.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.iWHI4fbXQr (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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=52, blended=17336, passed=138904
Got 138904 stars (including 121397 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 138904 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 137054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 137055 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 137055 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 928 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-47-54_20.00sec_-4.90C_LIGHT_0032.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.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_2026-04-16_CI_Mon-02-Q2b1x1_215217_TTUQ2b1x1_2202134_vKxuKaWg/wcs_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out283563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out287277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out303484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out283577.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out283686.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out300818.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out313822.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out318762.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out273991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325921.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 140s
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: 69s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283530_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283530_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283549_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283549_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283553_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283553_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283563_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283563_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:22.24 +00:33:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.074 3113590086878300544 102.84295080789 +00.56088917339 14.3448 13.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283564_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283564_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:56:53.33 -01:17:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.598 3112216423190217600 104.22228691627 -01.29910356997 14.5201 14.1883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283570_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283570_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:11.61 +00:50:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.762 3125567891665421568 101.54879744084 +00.83672062076 14.3349 13.7505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283577_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283577_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:25.52 -01:37:06.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283581_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283581_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283582_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283582_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283593_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283593_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283605_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283605_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:07.94 -02:49:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.999 3108017628802906752 106.78226834032 -02.81962839538 14.2695 13.2553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283614_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283614_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283625_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283625_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283658_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283658_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283661_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283661_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:10.25 +01:00:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.138 3125713821773344640 101.54272357930 +01.00410104796 14.2178 13.5838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283662_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283662_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:58.75 +00:11:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.694 3112759547573659008 106.49478838253 +00.18855727320 14.1112 13.5262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283663_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283663_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283680_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283680_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:16.35 -01:15:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.452 3112208589169679232 104.56840739062 -01.26417702453 14.3482 13.6695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283684_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283684_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283686_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283686_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:47.30 -00:37:51.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 283691_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283691_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:02:33.44 -01:58:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.683 3109049314307207680 105.63950162813 -01.96758727063 13.9169 13.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283695_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283695_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283704_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283704_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283709_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283709_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:14.14 +01:58:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.939 3126023265576889088 100.80850983937 +01.97056968421 13.9412 12.9739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283712_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283712_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:00:56.32 -02:45:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.009 3108734201146971648 105.23495779642 -02.75744859106 14.2097 13.7986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283714_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283714_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:23.50 +01:30:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.897 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283743_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283743_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:41.45 -00:18:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.293 3112536071835919744 103.92280361080 -00.31443519720 13.6816 12.8260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283745_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283745_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283751_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283751_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283757_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283757_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:33.95 -00:32:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.492 3113254602686605824 103.39171426999 -00.53578205621 14.1855 13.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283761_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283761_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:56.60 -03:35:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.924 3102748425484967296 103.73601294796 -03.59011466135 13.6336 12.7576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283764_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283764_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:51.79 +01:20:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.554 3115367211199527296 105.46601850960 +01.33474391831 14.0347 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283769_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283769_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283775_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283775_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:53.26 +01:01:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.786 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283794_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283794_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283802_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283802_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283811_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283811_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:46.84 +01:14:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.507 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283816_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283816_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:24.98 +01:44:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283823_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283823_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:34.22 -01:25:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.551 3112199689997622912 104.39261774682 -01.42526029994 14.0127 13.7648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283824_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283824_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:42.33 -02:40:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.213 3108906583953732480 104.92678251199 -02.67257173606 13.7477 13.3167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283832_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283832_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283842_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283842_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283849_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283849_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:35:07.30 -03:03:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.918 3105134640594000512 098.78093694492 -03.05146524854 13.5639 12.6234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283856_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283856_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283873_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283873_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:52.43 +00:01:15.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 283878_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283878_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:30.29 +00:58:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.318 3125806726206403200 100.62650063837 +00.96875962341 13.6495 13.0741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283882_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283882_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283887_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283887_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283890_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283890_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283894_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283894_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283897_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283897_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 283898_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283898_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283905_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283905_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:23.65 -05:15:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.223 3101964366313335296 102.59896228734 -05.26153723479 13.5496 13.0347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283906_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283906_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283907_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:19.29 -01:29:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.145 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283908_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283908_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283913_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283913_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283919_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:52.25 -00:44:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.552 3109635113484885248 107.21776257479 -00.74292765116 13.7584 13.3194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283921_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283921_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283929_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:13.85 +00:50:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.769 3125567926025169792 101.55788835134 +00.84443176757 13.6372 12.9682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283931_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:48.94 -03:26:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.693 3108614766697925248 105.45408116604 -03.43935739421 13.6653 13.2764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283932_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283932_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:25.42 +02:12:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.483 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283936_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283936_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:43.48 +01:59:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.265 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283940_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283940_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:33.27 -02:33:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.541 3108788008498236544 106.63914543869 -02.56150533444 13.2692 12.5082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283944_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283944_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283948_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283948_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283957_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283957_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283958_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:11.83 -05:47:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.780 3053308713347183360 107.04941538548 -05.79453453280 13.2957 13.0950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283961_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283961_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:12.52 +00:51:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.914 3125567930324132096 101.55227975245 +00.85185603769 13.4133 12.9328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283962_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283962_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:22.81 +01:06:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.808 3125681313161965056 102.34535478729 +01.11030157285 13.3610 12.8932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283966_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283966_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:27.69 -01:45:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.030 3112044139160625024 104.36522484805 -01.75663240647 13.3959 12.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283969_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283969_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:19.55 +01:45:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.015 3126679394843801856 100.08151708014 +01.75936322406 12.9914 11.9342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283972_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283972_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:24.28 -01:19:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.904 3109389608855158656 107.10114566256 -01.33208361262 13.4700 13.3144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283976_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283976_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283981_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283981_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:33.09 +00:32:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.155 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283985_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283985_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283986_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283986_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283989_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 283989_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:08.14 -05:53:01.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284000_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:02.34 +01:07:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284002_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 284002_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284004_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 284004_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284005_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284005_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:04:36.64 -01:40:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284008_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 284008_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284014_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284014_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:49.61 -01:13:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.117 3112361520063852800 102.70670591074 -01.22782858409 12.8359 12.4507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284015_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284015_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:38.91 -05:59:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284019_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284019_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:50.69 +01:53:33.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284025_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284025_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:08.35 -01:38:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 3.500 3112051973180962560 104.53510192219 -01.64911575248 12.5679 12.0718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284027_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284027_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:35.58 +01:46:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284029_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284029_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:52.44 -06:12:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284030_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284030_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:11.70 -01:33:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284031_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284031_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:26.00 -01:50:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284032_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 284032_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:26.57 -00:54:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 286796_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 286796_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:40.15 -00:32:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 287277_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 287277_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:01.54 -00:05:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 1.023 3112865238129521920 104.75657781092 -00.08934525517 11.1791 10.2020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288602_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 288602_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:37.19 +00:26:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289288_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 289288_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:39.68 +00:25:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289904_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 289904_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:37.66 +00:43:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291001_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 291001_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:30.53 -01:04:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291329_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 291329_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:04:10.62 -03:14:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291994_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 291994_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:41.55 -00:33:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295093_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 295093_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:08.08 -04:35:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295792_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 295792_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:11.86 -02:15:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295816_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 295816_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:17.12 +02:00:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.610 3114765366020010752 106.57169428469 +02.00384672606 12.7577 12.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295974_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 295974_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:52.63 -01:19:04.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297009_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 297009_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:44.38 -00:31:38.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297731_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 297731_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298510_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 298510_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298817_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 298817_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:30.03 -04:07:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299153_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 299153_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299441_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 299441_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:09.42 -05:52:27.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299580_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 299580_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:37.42 -01:22:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.147 3109339379218885888 107.40665275024 -01.37683283674 13.0624 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299694_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 299694_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:02:23.05 +00:25:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.764 3113001715010265856 105.59586879156 +00.43145813945 12.8711 12.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299829_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 299829_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:28.45 -04:07:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299969_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 299969_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:37:58.47 -01:25:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300582_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 300582_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:54.21 +00:00:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.625 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300604_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 300604_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:00.15 -00:03:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300818_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 300818_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:02.54 -03:29:53.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301816_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 301816_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302835_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 302835_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:08.40 -03:35:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.190 3107717565213010816 107.03467099261 -03.58332209027 13.3745 13.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303095_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 303095_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:50.43 +01:35:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303484_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 303484_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:13.57 +01:34:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.819 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303770_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 303770_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:22.42 -03:06:03.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304009_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 304009_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:15.05 -05:59:31.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304271_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 304271_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304432_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 304432_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:44:36.08 +01:45:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305657_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 305657_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305871_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 305871_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:06.00 -00:02:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.318 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305942_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 305942_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305959_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 305959_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:02:19.44 -03:20:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.609 3108619920658643968 105.58111518078 -03.34490994692 13.4942 12.9329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305971_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 305971_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306148_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 306148_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306189_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 306189_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306476_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 306476_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:56:22.01 -00:53:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.774 3112424230887731712 104.09176485857 -00.88726742447 13.5854 13.1578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306621_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 306621_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:13.95 -00:06:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.467 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307045_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 307045_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307407_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 307407_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:57.66 -05:31:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.808 3101886477089103232 102.49047561547 -05.52980829634 13.5826 13.2799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307470_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 307470_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:48.46 +00:23:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.103 3113610294697190784 102.20183118370 +00.39122776001 13.6085 13.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307762_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 307762_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:23.30 -01:37:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.337 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307859_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 307859_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:47.32 +00:13:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.536 3113508143193552256 101.94725396759 +00.22585649620 13.6520 13.0798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308140_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 308140_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:35.91 +01:59:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308175_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 308175_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308547_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 308547_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308882_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 308882_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308945_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 308945_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309643_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 309643_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:00:53.23 +02:12:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.869 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309747_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 309747_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309805_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 309805_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:20.55 -00:31:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309951_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 309951_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310065_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310065_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310070_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 310070_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:33.26 +01:51:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310083_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310083_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310141_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 310141_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:23.99 -02:57:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.443 3102896172359569152 104.35008263573 -02.95190892558 13.8534 13.3648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310144_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310144_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310264_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310264_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310426_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310426_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310549_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310549_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310564_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 310564_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:26.88 -00:55:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.817 3112570461635443584 105.36207810215 -00.92448145232 13.7792 12.9935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310739_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310739_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310743_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 310743_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310902_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 310902_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:49.24 +00:27:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.319 3114279519319862400 107.20543385668 +00.45405634620 13.8903 13.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311017_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 311017_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:39:24.84 +00:07:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.716 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311715_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 311715_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:41:46.97 -00:16:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.545 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311970_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 311970_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:24.56 -03:02:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.402 3102885074164723584 104.60233457213 -03.04380600683 13.7588 13.5728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311987_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 311987_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:43.98 -06:16:28.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312601_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 312601_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312993_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 312993_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313030_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 313030_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:56:43.00 +02:11:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313278_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 313278_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313695_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 313695_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313784_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 313784_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313822_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 313822_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:04:04.92 -02:22:45.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313836_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 313836_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:04.03 +01:58:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313883_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 313883_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:02.88 +02:18:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314212_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 314212_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314233_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 314233_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314500_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 314500_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315242_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 315242_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315391_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 315391_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315463_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 315463_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315543_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 315543_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:36.91 -01:46:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.531 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315916_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 315916_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:41:20.89 -01:43:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.528 3106831942950099584 100.33652100745 -01.72233248144 13.6881 12.6456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316020_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 316020_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316359_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 316359_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316783_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 316783_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:39.53 -00:16:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.247 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316917_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 316917_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316931_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 316931_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317151_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 317151_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 317337_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 317337_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:04.46 -01:43:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.613 3109233104548149120 107.01874958326 -01.72878742697 13.9560 13.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317355_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 317355_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 317711_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 317711_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:51.24 -02:54:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.180 3108661530301553152 105.96319311778 -02.91418890016 13.9534 13.3027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317774_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 317774_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 317850_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 317850_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317885_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 317885_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:56.19 -04:43:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.866 3102055458280756864 103.48505444976 -04.73232095785 14.0018 13.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317971_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 317971_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318041_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 318041_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:56.80 -01:06:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.639 3112234943088845952 104.73669433005 -01.11373099072 13.8605 13.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318167_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 318167_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318762_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 318762_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:35.65 +01:13:54.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 318918_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 318918_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 318921_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 318921_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 319605_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 319605_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 319670_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 319670_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:06.94 +01:49:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 319875_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 319875_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 320302_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 320302_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 320363_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 320363_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 320499_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 320499_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320541_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 320541_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:58.37 -00:30:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.487 3119415711793096832 099.74273250352 -00.50489919050 13.6777 12.6099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320656_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 320656_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:22.39 +01:18:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.211 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320692_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 320692_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:20.29 -00:32:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.637 3112460617850838784 104.58465531557 -00.54491251100 14.1966 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320710_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 320710_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:34.53 +00:32:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.321 3113580985840503296 103.14371971951 +00.54139619495 14.0748 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320828_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 320828_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:54.08 +02:10:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 321987_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 321987_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:52.36 +01:12:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.421 3120620024919006848 099.71870063274 +01.20611895865 14.1237 13.6672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322110_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 322110_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:43.95 -05:54:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.231 3100366264824580480 102.18279250022 -05.90788495291 13.4790 12.3244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322235_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 322235_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:02.68 -00:42:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.346 3109627588701789184 106.76082783589 -00.70808447428 14.2295 13.7367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322555_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 322555_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 322764_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 322764_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 323091_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 323091_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:58.80 +00:22:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.610 3112953473937328256 104.99505493550 +00.36980486509 14.2939 13.9155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323587_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 323587_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:26.73 +01:30:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.552 3114673694239105408 107.11091176573 +01.50243433392 14.3921 13.6375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323875_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 323875_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323957_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 323957_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324002_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 324002_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:33:28.86 +01:58:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.268 3120965610869943424 098.36990336847 +01.97793607089 13.8185 12.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324093_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 324093_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 324189_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 324189_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:33.84 -00:46:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.880 3112262774476682112 104.89085647506 -00.77602993535 14.3279 13.8367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324412_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 324412_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:47.82 +00:29:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.396 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324767_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 324767_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:02:49.16 -00:17:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.771 3112668185029745152 105.70514144171 -00.29167765481 14.4099 13.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324875_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 324875_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 324981_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 324981_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 325462_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 325462_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:08.45 -00:01:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.065 3111232837019910656 107.03525090547 -00.03362767301 14.2683 13.7055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325491_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 325491_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:22.26 +01:17:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.897 3114662900981688192 106.84327005235 +01.28369138872 14.5265 14.0512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 325841_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 325841_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:17.14 -00:58:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.339 3112252500915149952 104.57109720795 -00.97245475897 14.8159 14.2813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 325843_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 325843_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:39.54 +01:45:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.215 3125969080270305920 101.66392389435 +01.75355861020 14.4022 13.7868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 325921_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 325921_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 326000_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 326000_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:36.89 -01:20:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.132 3109169023634641408 105.40423254432 -01.34721565378 14.6140 14.2329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:13.61 -02:21:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:45.28 +00:41:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 273991_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 273991_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:41:59.19 -01:11:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-16_21-48-54_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:00.68 +01:46:32.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 214s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:52:06.35 -01:18:23.5
06:54:46.91 -00:19:04.6
06:53:04.53 +00:38:05.7
07:04:36.12 +00:46:51.6
06:51:10.11 -01:42:53.6
06:51:28.46 +01:59:25.2
06:57:47.88 -02:04:27.4
07:05:41.60 +00:52:58.6
06:59:04.06 -02:15:16.8
07:05:46.64 -02:59:50.3
06:58:39.02 -01:55:24.1
06:59:09.81 -00:26:03.0
06:56:23.55 -00:01:50.1
06:53:30.50 -03:06:08.3
07:06:39.31 +00:36:40.1
07:03:36.85 -00:12:39.5
07:04:32.18 +00:11:22.2
07:02:23.52 -01:34:42.9
07:02:32.21 -00:13:11.1
06:43:45.73 +00:35:15.8
06:59:20.35 -02:01:16.1
07:01:12.63 -01:43:37.9
07:02:01.11 -00:36:17.0
07:07:56.27 -01:30:31.8
06:55:07.80 -00:16:30.4
07:05:05.63 -03:34:37.9
07:00:28.64 -02:26:03.3
07:08:31.22 -00:56:11.5
06:51:10.41 +01:05:59.0
06:59:42.02 -02:10:55.0
07:00:38.57 -01:30:51.5
06:55:18.36 -01:43:18.1
06:44:25.89 +00:03:22.6
06:59:24.64 -00:33:08.5
06:58:19.99 -00:33:18.7
06:55:03.12 -01:02:52.1
07:08:48.67 -03:43:00.6
06:57:23.16 -00:50:07.4
07:01:17.81 -02:42:57.6
07:07:06.84 +01:40:00.3
06:59:40.31 -00:39:48.7
07:03:24.00 -02:49:51.4
06:58:49.09 -01:06:27.0
07:05:18.09 -01:23:00.2
06:58:56.93 -03:00:42.9
07:01:04.28 +00:15:11.9
06:58:50.14 -01:53:11.9
07:03:47.13 -03:20:30.9
07:06:42.23 -03:09:14.7
07:05:50.98 -02:05:13.9
06:57:16.32 -00:59:40.6
06:54:34.38 -00:35:22.9
07:05:08.53 -01:31:34.2
07:01:19.05 -03:06:45.7
07:09:03.24 -02:29:06.4
06:51:06.52 -05:16:05.8
07:02:17.55 -03:14:35.0
06:54:48.31 +00:23:17.3
06:44:39.55 +00:10:07.2
07:03:04.31 -01:18:38.9
06:56:48.86 +00:46:31.1
06:55:27.05 -01:16:23.3
06:41:18.48 -00:51:04.3
07:05:33.64 +02:07:17.9
07:00:54.98 -03:04:10.8
07:04:50.30 -01:48:51.9
06:48:30.53 +00:57:45.0
06:56:11.66 -01:22:24.9
07:01:10.38 -01:01:15.8
07:02:14.49 -03:05:58.5
06:59:43.57 +00:17:09.6
06:54:59.72 +00:10:50.1
06:48:53.05 +01:49:28.7
07:04:16.72 -03:01:38.7
06:50:18.16 +00:24:40.8
06:57:05.86 -03:30:42.8
07:06:39.79 -02:47:34.6
07:07:40.43 -03:15:08.0
06:37:13.48 -01:07:58.0
06:46:50.54 +01:18:07.2
06:44:50.55 +01:05:43.5
07:05:58.21 +01:33:32.0
07:01:11.75 -01:35:20.0
07:09:21.52 +01:07:24.7
07:06:45.48 -01:30:49.3
06:50:59.44 +00:13:37.9
06:59:00.85 -02:36:04.0
07:04:51.48 -02:12:05.3
06:47:23.60 +01:25:42.6
06:51:34.20 -01:39:24.5
06:56:54.09 +00:54:12.7
07:05:59.00 -02:03:45.6
06:59:41.82 -02:11:38.2
06:49:27.61 +01:39:51.0
06:50:01.92 +00:45:47.4
06:50:41.37 -00:31:45.4
06:37:09.55 -01:09:02.1
07:01:55.99 +01:13:06.6
06:53:41.33 -00:33:49.2
06:57:11.43 -01:07:44.9
06:50:24.34 -05:53:57.9
07:04:19.82 +00:50:07.7
06:49:21.36 +01:13:44.9
06:53:08.11 -00:50:30.3
07:07:06.45 -04:13:53.0
06:38:39.09 +01:56:34.1
06:55:11.70 +00:56:23.9
07:02:14.11 -00:34:58.4
06:54:03.00 -00:10:55.4
06:54:24.96 -00:23:52.5
06:59:46.51 -02:22:13.9
06:47:18.91 +01:25:13.9
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:54:46.91 -00:19:04.6
06:53:04.53 +00:38:05.7
07:04:36.12 +00:46:51.6
06:51:10.11 -01:42:53.6
06:51:28.46 +01:59:25.2
06:57:47.88 -02:04:27.4
07:05:41.60 +00:52:58.6
06:59:04.06 -02:15:16.8
07:05:46.64 -02:59:50.3
06:58:39.02 -01:55:24.1
06:59:09.81 -00:26:03.0
06:56:23.55 -00:01:50.1
06:53:30.50 -03:06:08.3
07:06:39.31 +00:36:40.1
07:03:36.85 -00:12:39.5
07:04:32.18 +00:11:22.2
07:02:23.52 -01:34:42.9
07:02:32.21 -00:13:11.1
06:43:45.73 +00:35:15.8
06:59:20.35 -02:01:16.1
07:01:12.63 -01:43:37.9
07:02:01.11 -00:36:17.0
07:07:56.27 -01:30:31.8
06:55:07.80 -00:16:30.4
07:05:05.63 -03:34:37.9
07:00:28.64 -02:26:03.3
07:08:31.22 -00:56:11.5
06:51:10.41 +01:05:59.0
06:59:42.02 -02:10:55.0
07:00:38.57 -01:30:51.5
06:55:18.36 -01:43:18.1
06:44:25.89 +00:03:22.6
06:59:24.64 -00:33:08.5
06:58:19.99 -00:33:18.7
06:55:03.12 -01:02:52.1
07:08:48.67 -03:43:00.6
06:57:23.16 -00:50:07.4
07:01:17.81 -02:42:57.6
07:07:06.84 +01:40:00.3
06:59:40.31 -00:39:48.7
07:03:24.00 -02:49:51.4
06:58:49.09 -01:06:27.0
07:05:18.09 -01:23:00.2
06:58:56.93 -03:00:42.9
07:01:04.28 +00:15:11.9
06:58:50.14 -01:53:11.9
07:03:47.13 -03:20:30.9
07:06:42.23 -03:09:14.7
07:05:50.98 -02:05:13.9
06:57:16.32 -00:59:40.6
06:54:34.38 -00:35:22.9
07:05:08.53 -01:31:34.2
07:01:19.05 -03:06:45.7
07:09:03.24 -02:29:06.4
06:51:06.52 -05:16:05.8
07:02:17.55 -03:14:35.0
06:54:48.31 +00:23:17.3
06:44:39.55 +00:10:07.2
07:03:04.31 -01:18:38.9
06:56:48.86 +00:46:31.1
06:55:27.05 -01:16:23.3
06:41:18.48 -00:51:04.3
07:05:33.64 +02:07:17.9
07:00:54.98 -03:04:10.8
07:04:50.30 -01:48:51.9
06:48:30.53 +00:57:45.0
06:56:11.66 -01:22:24.9
07:01:10.38 -01:01:15.8
07:02:14.49 -03:05:58.5
06:59:43.57 +00:17:09.6
06:54:59.72 +00:10:50.1
06:48:53.05 +01:49:28.7
07:04:16.72 -03:01:38.7
06:50:18.16 +00:24:40.8
06:57:05.86 -03:30:42.8
07:06:39.79 -02:47:34.6
07:07:40.43 -03:15:08.0
06:37:13.48 -01:07:58.0
06:46:50.54 +01:18:07.2
06:44:50.55 +01:05:43.5
07:05:58.21 +01:33:32.0
07:01:11.75 -01:35:20.0
07:09:21.52 +01:07:24.7
07:06:45.48 -01:30:49.3
06:50:59.44 +00:13:37.9
06:59:00.85 -02:36:04.0
07:04:51.48 -02:12:05.3
06:47:23.60 +01:25:42.6
06:51:34.20 -01:39:24.5
06:56:54.09 +00:54:12.7
07:05:59.00 -02:03:45.6
06:59:41.82 -02:11:38.2
06:49:27.61 +01:39:51.0
06:50:01.92 +00:45:47.4
06:50:41.37 -00:31:45.4
06:37:09.55 -01:09:02.1
07:01:55.99 +01:13:06.6
06:53:41.33 -00:33:49.2
06:57:11.43 -01:07:44.9
06:50:24.34 -05:53:57.9
07:04:19.82 +00:50:07.7
06:49:21.36 +01:13:44.9
06:53:08.11 -00:50:30.3
07:07:06.45 -04:13:53.0
06:38:39.09 +01:56:34.1
06:55:11.70 +00:56:23.9
07:02:14.11 -00:34:58.4
06:54:03.00 -00:10:55.4
06:54:24.96 -00:23:52.5
06:59:46.51 -02:22:13.9
06:47:18.91 +01:25:13.9
06:52:06.35 -01:18:23.5
###################################################################################
06:54:46.91 -00:19:04.6 -- not an asteroid (will add it to exclusion list)
06:53:04.53 +00:38:05.7 -- not an asteroid (will add it to exclusion list)
07:04:36.12 +00:46:51.6 -- not an asteroid (will add it to exclusion list)
06:51:10.11 -01:42:53.6 -- not an asteroid (will add it to exclusion list)
06:51:28.46 +01:59:25.2 -- not an asteroid (will add it to exclusion list)
06:57:47.88 -02:04:27.4 -- not an asteroid (will add it to exclusion list)
07:05:41.60 +00:52:58.6 -- not an asteroid (will add it to exclusion list)
06:59:04.06 -02:15:16.8 -- not an asteroid (will add it to exclusion list)
07:05:46.64 -02:59:50.3 -- not an asteroid (will add it to exclusion list)
06:58:39.02 -01:55:24.1 -- not an asteroid (will add it to exclusion list)
06:59:09.81 -00:26:03.0 -- not an asteroid (will add it to exclusion list)
06:56:23.55 -00:01:50.1 -- not an asteroid (will add it to exclusion list)
06:53:30.50 -03:06:08.3 -- not an asteroid (will add it to exclusion list)
07:06:39.31 +00:36:40.1 -- not an asteroid (will add it to exclusion list)
07:03:36.85 -00:12:39.5 -- not an asteroid (will add it to exclusion list)
07:04:32.18 +00:11:22.2 -- not an asteroid (will add it to exclusion list)
07:02:23.52 -01:34:42.9 -- not an asteroid (will add it to exclusion list)
07:02:32.21 -00:13:11.1 -- not an asteroid (will add it to exclusion list)
06:43:45.73 +00:35:15.8 -- not an asteroid (will add it to exclusion list)
06:59:20.35 -02:01:16.1 -- not an asteroid (will add it to exclusion list)
07:01:12.63 -01:43:37.9 -- not an asteroid (will add it to exclusion list)
07:02:01.11 -00:36:17.0 -- not an asteroid (will add it to exclusion list)
07:07:56.27 -01:30:31.8 -- not an asteroid (will add it to exclusion list)
06:55:07.80 -00:16:30.4 -- not an asteroid (will add it to exclusion list)
07:05:05.63 -03:34:37.9 -- not an asteroid (will add it to exclusion list)
07:00:28.64 -02:26:03.3 -- not an asteroid (will add it to exclusion list)
07:08:31.22 -00:56:11.5 -- not an asteroid (will add it to exclusion list)
06:51:10.41 +01:05:59.0 -- not an asteroid (will add it to exclusion list)
06:59:42.02 -02:10:55.0 -- not an asteroid (will add it to exclusion list)
07:00:38.57 -01:30:51.5 -- not an asteroid (will add it to exclusion list)
06:55:18.36 -01:43:18.1 -- not an asteroid (will add it to exclusion list)
06:44:25.89 +00:03:22.6 -- not an asteroid (will add it to exclusion list)
06:59:24.64 -00:33:08.5 -- not an asteroid (will add it to exclusion list)
06:58:19.99 -00:33:18.7 -- not an asteroid (will add it to exclusion list)
06:55:03.12 -01:02:52.1 -- not an asteroid (will add it to exclusion list)
07:08:48.67 -03:43:00.6 -- not an asteroid (will add it to exclusion list)
06:57:23.16 -00:50:07.4 -- not an asteroid (will add it to exclusion list)
07:01:17.81 -02:42:57.6 -- not an asteroid (will add it to exclusion list)
07:07:06.84 +01:40:00.3 -- not an asteroid (will add it to exclusion list)
06:59:40.31 -00:39:48.7 -- not an asteroid (will add it to exclusion list)
07:03:24.00 -02:49:51.4 -- not an asteroid (will add it to exclusion list)
06:58:49.09 -01:06:27.0 -- not an asteroid (will add it to exclusion list)
07:05:18.09 -01:23:00.2 -- not an asteroid (will add it to exclusion list)
06:58:56.93 -03:00:42.9 -- not an asteroid (will add it to exclusion list)
07:01:04.28 +00:15:11.9 -- not an asteroid (will add it to exclusion list)
06:58:50.14 -01:53:11.9 -- not an asteroid (will add it to exclusion list)
07:03:47.13 -03:20:30.9 -- not an asteroid (will add it to exclusion list)
07:06:42.23 -03:09:14.7 -- not an asteroid (will add it to exclusion list)
07:05:50.98 -02:05:13.9 -- not an asteroid (will add it to exclusion list)
06:57:16.32 -00:59:40.6 -- not an asteroid (will add it to exclusion list)
06:54:34.38 -00:35:22.9 -- not an asteroid (will add it to exclusion list)
07:05:08.53 -01:31:34.2 -- not an asteroid (will add it to exclusion list)
07:01:19.05 -03:06:45.7 -- not an asteroid (will add it to exclusion list)
07:09:03.24 -02:29:06.4 -- not an asteroid (will add it to exclusion list)
06:51:06.52 -05:16:05.8 -- not an asteroid (will add it to exclusion list)
07:02:17.55 -03:14:35.0 -- not an asteroid (will add it to exclusion list)
06:54:48.31 +00:23:17.3 -- not an asteroid (will add it to exclusion list)
06:44:39.55 +00:10:07.2 -- not an asteroid (will add it to exclusion list)
07:03:04.31 -01:18:38.9 -- not an asteroid (will add it to exclusion list)
06:56:48.86 +00:46:31.1 -- not an asteroid (will add it to exclusion list)
06:55:27.05 -01:16:23.3 -- not an asteroid (will add it to exclusion list)
06:41:18.48 -00:51:04.3 -- not an asteroid (will add it to exclusion list)
07:05:33.64 +02:07:17.9 -- not an asteroid (will add it to exclusion list)
07:00:54.98 -03:04:10.8 -- not an asteroid (will add it to exclusion list)
07:04:50.30 -01:48:51.9 -- not an asteroid (will add it to exclusion list)
06:48:30.53 +00:57:45.0 -- not an asteroid (will add it to exclusion list)
06:56:11.66 -01:22:24.9 -- not an asteroid (will add it to exclusion list)
07:01:10.38 -01:01:15.8 -- not an asteroid (will add it to exclusion list)
07:02:14.49 -03:05:58.5 -- not an asteroid (will add it to exclusion list)
06:59:43.57 +00:17:09.6 -- not an asteroid (will add it to exclusion list)
06:54:59.72 +00:10:50.1 -- not an asteroid (will add it to exclusion list)
06:48:53.05 +01:49:28.7 -- not an asteroid (will add it to exclusion list)
07:04:16.72 -03:01:38.7 -- not an asteroid (will add it to exclusion list)
06:50:18.16 +00:24:40.8 -- not an asteroid (will add it to exclusion list)
06:57:05.86 -03:30:42.8 -- not an asteroid (will add it to exclusion list)
07:06:39.79 -02:47:34.6 -- not an asteroid (will add it to exclusion list)
07:07:40.43 -03:15:08.0 -- not an asteroid (will add it to exclusion list)
06:37:13.48 -01:07:58.0 -- not an asteroid (will add it to exclusion list)
06:46:50.54 +01:18:07.2 -- not an asteroid (will add it to exclusion list)
06:44:50.55 +01:05:43.5 -- not an asteroid (will add it to exclusion list)
07:05:58.21 +01:33:32.0 -- not an asteroid (will add it to exclusion list)
07:01:11.75 -01:35:20.0 -- not an asteroid (will add it to exclusion list)
07:09:21.52 +01:07:24.7 -- not an asteroid (will add it to exclusion list)
07:06:45.48 -01:30:49.3 -- not an asteroid (will add it to exclusion list)
06:50:59.44 +00:13:37.9 -- not an asteroid (will add it to exclusion list)
06:59:00.85 -02:36:04.0 -- not an asteroid (will add it to exclusion list)
07:04:51.48 -02:12:05.3 -- not an asteroid (will add it to exclusion list)
06:47:23.60 +01:25:42.6 -- not an asteroid (will add it to exclusion list)
06:51:34.20 -01:39:24.5 -- not an asteroid (will add it to exclusion list)
06:56:54.09 +00:54:12.7 -- not an asteroid (will add it to exclusion list)
07:05:59.00 -02:03:45.6 -- not an asteroid (will add it to exclusion list)
06:59:41.82 -02:11:38.2 -- not an asteroid (will add it to exclusion list)
06:49:27.61 +01:39:51.0 -- not an asteroid (will add it to exclusion list)
06:50:01.92 +00:45:47.4 -- not an asteroid (will add it to exclusion list)
06:50:41.37 -00:31:45.4 -- not an asteroid (will add it to exclusion list)
06:37:09.55 -01:09:02.1 -- not an asteroid (will add it to exclusion list)
07:01:55.99 +01:13:06.6 -- not an asteroid (will add it to exclusion list)
06:53:41.33 -00:33:49.2 -- not an asteroid (will add it to exclusion list)
06:57:11.43 -01:07:44.9 -- not an asteroid (will add it to exclusion list)
06:50:24.34 -05:53:57.9 -- not an asteroid (will add it to exclusion list)
07:04:19.82 +00:50:07.7 -- not an asteroid (will add it to exclusion list)
06:49:21.36 +01:13:44.9 -- not an asteroid (will add it to exclusion list)
06:53:08.11 -00:50:30.3 -- not an asteroid (will add it to exclusion list)
07:07:06.45 -04:13:53.0 -- not an asteroid (will add it to exclusion list)
06:38:39.09 +01:56:34.1 -- not an asteroid (will add it to exclusion list)
06:55:11.70 +00:56:23.9 -- not an asteroid (will add it to exclusion list)
07:02:14.11 -00:34:58.4 -- not an asteroid (will add it to exclusion list)
06:54:03.00 -00:10:55.4 -- not an asteroid (will add it to exclusion list)
06:54:24.96 -00:23:52.5 -- not an asteroid (will add it to exclusion list)
06:59:46.51 -02:22:13.9 -- not an asteroid (will add it to exclusion list)
06:47:18.91 +01:25:13.9 -- not an asteroid (will add it to exclusion list)
06:52:06.35 -01:18:23.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:37:09.55 -01:09:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:13.48 -01:07:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:39.09 +01:56:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:18.48 -00:51:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:45.73 +00:35:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:25.89 +00:03:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.55 +00:10:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.55 +01:05:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:50.54 +01:18:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:18.91 +01:25:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:23.60 +01:25:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:30.53 +00:57:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:53.05 +01:49:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:21.36 +01:13:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:27.61 +01:39:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:01.92 +00:45:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:18.16 +00:24:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:24.34 -05:53:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.37 -00:31:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.44 +00:13:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:06.52 -05:16:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.11 -01:42:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.41 +01:05:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.46 +01:59:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.20 -01:39:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.35 -01:18:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.53 +00:38:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:08.11 -00:50:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:30.50 -03:06:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.33 -00:33:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:03.00 -00:10:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:24.96 -00:23:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.38 -00:35:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:46.91 -00:19:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.31 +00:23:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:59.72 +00:10:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.12 -01:02:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:07.80 -00:16:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:11.70 +00:56:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:18.36 -01:43:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:27.05 -01:16:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:11.66 -01:22:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:23.55 -00:01:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:48.86 +00:46:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:54.09 +00:54:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:05.86 -03:30:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.43 -01:07:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.32 -00:59:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:23.16 -00:50:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.88 -02:04:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:19.99 -00:33:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.02 -01:55:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:49.09 -01:06:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.14 -01:53:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:56.93 -03:00:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.85 -02:36:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:04.06 -02:15:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:09.81 -00:26:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:20.35 -02:01:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:24.64 -00:33:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.31 -00:39:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:41.82 -02:11:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:42.02 -02:10:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:43.57 +00:17:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:46.51 -02:22:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:28.64 -02:26:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:38.57 -01:30:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:54.98 -03:04:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:04.28 +00:15:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.38 -01:01:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:11.75 -01:35:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:12.63 -01:43:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:17.81 -02:42:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.05 -03:06:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:55.99 +01:13:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:01.11 -00:36:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.11 -00:34:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.49 -03:05:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:17.55 -03:14:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.52 -01:34:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.21 -00:13:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.31 -01:18:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.00 -02:49:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.85 -00:12:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:47.13 -03:20:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.72 -03:01:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:19.82 +00:50:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:32.18 +00:11:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:36.12 +00:46:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:50.30 -01:48:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.48 -02:12:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:05.63 -03:34:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:08.53 -01:31:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.09 -01:23:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:33.64 +02:07:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.60 +00:52:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:46.64 -02:59:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.98 -02:05:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:58.21 +01:33:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:59.00 -02:03:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:39.31 +00:36:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:39.79 -02:47:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:42.23 -03:09:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.48 -01:30:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.45 -04:13:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.84 +01:40:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:40.43 -03:15:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:56.27 -01:30:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:31.22 -00:56:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.67 -03:43:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:03.24 -02:29:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.52 +01:07:24.7 -- 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)
06:37:09.55 -01:09:02.1 -- not a known variable star
06:37:13.48 -01:07:58.0 -- not a known variable star
06:38:39.09 +01:56:34.1 -- not a known variable star
06:41:18.48 -00:51:04.3 -- not a known variable star
06:43:45.73 +00:35:15.8 -- not a known variable star
06:44:25.89 +00:03:22.6 -- a known variable star
06:44:39.55 +00:10:07.2 -- a known variable star
06:44:50.55 +01:05:43.5 -- not a known variable star
06:46:50.54 +01:18:07.2 -- a known variable star
06:47:18.91 +01:25:13.9 -- not a known variable star
06:47:23.60 +01:25:42.6 -- a known variable star
06:48:30.53 +00:57:45.0 -- not a known variable star
06:48:53.05 +01:49:28.7 -- a known variable star
06:49:21.36 +01:13:44.9 -- not a known variable star
06:49:27.61 +01:39:51.0 -- not a known variable star
06:50:01.92 +00:45:47.4 -- not a known variable star
06:50:18.16 +00:24:40.8 -- not a known variable star
06:50:24.34 -05:53:57.9 -- not a known variable star
06:50:41.37 -00:31:45.4 -- not a known variable star
06:50:59.44 +00:13:37.9 -- not a known variable star
06:51:06.52 -05:16:05.8 -- a known variable star
06:51:10.11 -01:42:53.6 -- a known variable star
06:51:10.41 +01:05:59.0 -- not a known variable star
06:51:28.46 +01:59:25.2 -- not a known variable star
06:51:34.20 -01:39:24.5 -- not a known variable star
06:52:06.35 -01:18:23.5 -- not a known variable star
06:53:04.53 +00:38:05.7 -- not a known variable star
06:53:08.11 -00:50:30.3 -- a known variable star
06:53:30.50 -03:06:08.3 -- a known variable star
06:53:41.33 -00:33:49.2 -- a known variable star
06:54:03.00 -00:10:55.4 -- not a known variable star
06:54:24.96 -00:23:52.5 -- not a known variable star
06:54:34.38 -00:35:22.9 -- not a known variable star
06:54:46.91 -00:19:04.6 -- a known variable star
06:54:48.31 +00:23:17.3 -- a known variable star
06:54:59.72 +00:10:50.1 -- not a known variable star
06:55:03.12 -01:02:52.1 -- not a known variable star
06:55:07.80 -00:16:30.4 -- not a known variable star
06:55:11.70 +00:56:23.9 -- not a known variable star
06:55:18.36 -01:43:18.1 -- not a known variable star
06:55:27.05 -01:16:23.3 -- a known variable star
06:56:11.66 -01:22:24.9 -- not a known variable star
06:56:23.55 -00:01:50.1 -- a known variable star
06:56:48.86 +00:46:31.1 -- not a known variable star
06:56:54.09 +00:54:12.7 -- not a known variable star
06:57:05.86 -03:30:42.8 -- a known variable star
06:57:11.43 -01:07:44.9 -- a known variable star
06:57:16.32 -00:59:40.6 -- not a known variable star
06:57:23.16 -00:50:07.4 -- not a known variable star
06:57:47.88 -02:04:27.4 -- not a known variable star
06:58:19.99 -00:33:18.7 -- not a known variable star
06:58:39.02 -01:55:24.1 -- not a known variable star
06:58:49.09 -01:06:27.0 -- a known variable star
06:58:50.14 -01:53:11.9 -- not a known variable star
06:58:56.93 -03:00:42.9 -- not a known variable star
06:59:00.85 -02:36:04.0 -- not a known variable star
06:59:04.06 -02:15:16.8 -- not a known variable star
06:59:09.81 -00:26:03.0 -- a known variable star
06:59:20.35 -02:01:16.1 -- not a known variable star
06:59:24.64 -00:33:08.5 -- a known variable star
06:59:40.31 -00:39:48.7 -- not a known variable star
06:59:41.82 -02:11:38.2 -- not a known variable star
06:59:42.02 -02:10:55.0 -- a known variable star
06:59:43.57 +00:17:09.6 -- a known variable star
06:59:46.51 -02:22:13.9 -- not a known variable star
07:00:28.64 -02:26:03.3 -- not a known variable star
07:00:38.57 -01:30:51.5 -- not a known variable star
07:00:54.98 -03:04:10.8 -- not a known variable star
07:01:04.28 +00:15:11.9 -- a known variable star
07:01:10.38 -01:01:15.8 -- not a known variable star
07:01:11.75 -01:35:20.0 -- not a known variable star
07:01:12.63 -01:43:37.9 -- not a known variable star
07:01:17.81 -02:42:57.6 -- a known variable star
07:01:19.05 -03:06:45.7 -- not a known variable star
07:01:55.99 +01:13:06.6 -- not a known variable star
07:02:01.11 -00:36:17.0 -- not a known variable star
07:02:14.11 -00:34:58.4 -- not a known variable star
07:02:14.49 -03:05:58.5 -- not a known variable star
07:02:17.55 -03:14:35.0 -- not a known variable star
07:02:23.52 -01:34:42.9 -- not a known variable star
07:02:32.21 -00:13:11.1 -- not a known variable star
07:03:04.31 -01:18:38.9 -- not a known variable star
07:03:24.00 -02:49:51.4 -- not a known variable star
07:03:36.85 -00:12:39.5 -- not a known variable star
07:03:47.13 -03:20:30.9 -- not a known variable star
07:04:16.72 -03:01:38.7 -- not a known variable star
07:04:19.82 +00:50:07.7 -- not a known variable star
07:04:32.18 +00:11:22.2 -- a known variable star
07:04:36.12 +00:46:51.6 -- not a known variable star
07:04:50.30 -01:48:51.9 -- not a known variable star
07:04:51.48 -02:12:05.3 -- not a known variable star
07:05:05.63 -03:34:37.9 -- not a known variable star
07:05:08.53 -01:31:34.2 -- not a known variable star
07:05:18.09 -01:23:00.2 -- a known variable star
07:05:33.64 +02:07:17.9 -- not a known variable star
07:05:41.60 +00:52:58.6 -- a known variable star
07:05:46.64 -02:59:50.3 -- not a known variable star
07:05:50.98 -02:05:13.9 -- not a known variable star
07:05:58.21 +01:33:32.0 -- not a known variable star
07:05:59.00 -02:03:45.6 -- not a known variable star
07:06:39.31 +00:36:40.1 -- not a known variable star
07:06:39.79 -02:47:34.6 -- not a known variable star
07:06:42.23 -03:09:14.7 -- not a known variable star
07:06:45.48 -01:30:49.3 -- a known variable star
07:07:06.45 -04:13:53.0 -- not a known variable star
07:07:06.84 +01:40:00.3 -- not a known variable star
07:07:40.43 -03:15:08.0 -- a known variable star
07:07:56.27 -01:30:31.8 -- not a known variable star
07:08:31.22 -00:56:11.5 -- not a known variable star
07:08:48.67 -03:43:00.6 -- not a known variable star
07:09:03.24 -02:29:06.4 -- not a known variable star
07:09:21.52 +01:07:24.7 -- a known variable star
Found 83 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
112 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 112 (excluding asteroids and hot pixels, 83 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)2461147.61671826 -observatory V36
00:13:14.60 -01:25:53.3 Mercury (0.0mag)
03:14:07.01 +18:16:17.5 Venus (-3.9mag)
00:21:00.66 +01:12:48.5 Mars (1.2mag)
07:13:08.69 +22:45:23.2 Jupiter (-2.1mag)
00:29:40.66 +00:52:04.4 Saturn (0.9mag)
03:47:55.99 +19:48:14.0 Uranus (5.8mag)
00:10:59.14 -00:14:27.3 Neptune (7.8mag)
20:33:48.12 -22:52:39.2 Pluto (14.5mag)
01:11:30.79 +11:05:12.6 Moon (99.9mag)
-rw-r--r-- 1 apache apache 361 Apr 16 21:56 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461147.61671826:
07:13:04.75 +22:45:29.0 Io (5.8mag)
07:13:19.13 +22:44:59.0 Europa (5.9mag)
07:13:11.51 +22:45:10.0 Ganymede (5.4mag)
07:13:41.82 +22:44:11.6 Callisto (6.6mag)
07:16:25.94 +22:32:29.9 Himalia (15.3mag)
07:13:10.70 +22:45:20.7 Thebe (16.2mag)
07:16:38.74 +23:02:45.5 Elara (17.3mag)
07:12:06.14 +23:24:48.5 Pasiphae (17.4mag)
07:21:26.89 +22:43:30.9 Carme (18.5mag)
00:29:37.23 +00:52:32.2 Titan (8.8mag)
00:29:45.05 +00:52:03.3 Rhea (10.1mag)
00:29:18.84 +00:52:03.0 Iapetus (11.5mag)
00:29:44.82 +00:52:29.0 Hyperion (14.8mag)
00:31:16.66 +01:00:45.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 16 21:56 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461147.61671826:
15:43:19.70 -17:00:31.8 JWST
17:35:47.46 +38:48:53.0 Chandra
16:55:19.58 -51:36:55.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 16 21:56 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461147.61671826 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:26.59 -28:50:41.9 13.9mag P/2010 H2 (Vales)
05:07:32.61 -69:36:34.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:41.50 +31:26:42.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:19.07 +10:40:45.8 17.6mag C/2021 G2 (ATLAS)
23:10:30.90 +29:16:25.1 17.1mag C/2022 E2 (ATLAS)
04:30:32.43 +26:04:06.8 16.0mag C/2022 N2 (PANSTARRS)
09:03:40.26 +32:01:24.0 16.2mag C/2022 QE78 (ATLAS)
08:31:15.19 -00:02:09.2 17.3mag C/2022 R6 (PANSTARRS)
18:53:27.42 +18:37:32.6 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:18.44 -11:30:18.7 17.5mag P/2023 B1 (PANSTARRS)
09:07:07.93 -11:42:20.0 17.6mag C/2023 F3 (ATLAS)
21:55:19.01 +62:58:20.9 17.5mag C/2023 H5 (Lemmon)
19:18:12.45 -03:45:06.4 14.1mag C/2023 R1 (PANSTARRS)
21:30:02.98 +86:04:00.9 17.8mag C/2023 X2 (Lemmon)
06:18:26.40 +63:30:31.4 17.2mag C/2024 A1 (ATLAS)
05:15:39.13 +18:40:19.0 11.1mag C/2024 E1 (Wierzchos)
16:18:32.99 +06:34:23.5 17.4mag C/2024 G6 (ATLAS)
20:21:06.78 +15:34:44.5 14.6mag C/2024 J3 (ATLAS)
03:27:22.49 -22:12:59.6 16.3mag C/2024 T5 (ATLAS)
05:17:39.90 +45:00:58.2 17.7mag C/2025 J1 (Borisov)
13:34:12.83 +46:11:20.7 15.2mag C/2025 L1 (ATLAS)
03:27:03.12 -26:23:15.5 17.8mag C/2025 Q3 (ATLAS)
23:54:08.77 +18:10:06.1 8.4mag C/2025 R3 (PANSTARRS)
12:53:38.23 +03:04:47.9 17.4mag C/2025 Y1 (ATLAS)
03:36:44.14 +02:30:28.4 13.6mag C/2026 A1 (MAPS)
00:02:43.57 +37:25:18.5 14.6mag C/2026 B2 (Sun-Gao)
18:45:06.46 -09:39:31.8 11.8mag 10P/Tempel
14:58:47.45 +03:05:26.0 14.1mag 24P/Schaumasse
11:02:30.74 -01:29:26.6 15.7mag 29P/Schwassmann-Wachmann
18:01:15.44 -09:34:10.9 18.0mag 40P/Vaisala
10:37:32.37 -04:00:43.0 16.9mag 43P/Wolf-Harrington
01:50:24.15 +17:40:38.7 17.2mag 47P/Ashbrook-Jackson
07:12:50.31 +36:46:19.7 17.0mag 63P/Wild
23:30:28.51 -11:19:02.5 15.7mag 65P/Gunn
04:06:14.79 +21:38:07.9 15.9mag 76P/West-Kohoutek-Ikemura
01:08:02.84 +08:26:51.5 14.3mag 78P/Gehrels
23:06:22.02 -09:03:38.5 14.6mag 88P/Howell
02:13:34.30 +20:56:16.9 15.1mag 93P/Lovas
04:56:55.28 +32:20:47.4 16.2mag 123P/West-Hartley
08:29:41.99 +37:50:47.3 16.2mag 124P/Mrkos
02:34:56.66 +14:29:38.6 16.4mag 128P/Shoemaker-Holt
02:49:43.79 +14:37:42.2 17.5mag 131P/Mueller
01:32:03.30 +13:37:04.6 10.6mag 141P/Machholz
01:40:49.27 +05:17:30.9 10.6mag 141P-A/Machholz
00:25:35.72 +01:09:48.9 12.7mag 141P-D/Machholz
02:11:13.96 +07:03:05.9 17.8mag 141P-I/Machholz
01:05:29.75 -00:57:47.7 15.1mag 162P/SidingSpring
14:49:27.27 +00:02:38.8 17.7mag 210P/Christensen
21:42:02.55 -11:10:48.0 17.6mag 218P/LINEAR
17:16:48.97 -13:47:53.6 16.1mag 235P/LINEAR
05:36:54.08 +34:46:53.0 16.8mag 240P/NEAT
07:39:03.23 -05:02:51.7 17.7mag 242P/Spahr
22:19:41.97 -20:40:48.2 17.9mag 260P/McNaught
02:00:28.42 +20:44:26.4 18.0mag 295P/LINEAR
15:42:12.09 +07:03:47.2 17.5mag 391P/Kowalski
07:34:38.12 +21:22:08.4 17.7mag 450P/LONEOS
05:37:30.46 +44:58:03.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 16 21:56 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
17:21:59.44 -38:54:04.60 2026-04-14.4 15.15
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
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
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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 16 21:56 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:06:56.603 -64:55:52.46 AT 2026jcy 2026-04-09.11 18.906
08:27:06.222 -58:50:26.83 AT 2026jcx 2026-04-09.08 19.372
13:48:22.893 -31:10:42.12 AT 2026jcw 2026-04-09.08 19.95
17:39:28.750 +05:01:10.80 AT 2026jcv 2026-04-09.86 16.87
14:44:31.580 +71:55:25.90 AT 2026jcu 2026-04-09.47 17.9
12:39:27.288 -08:14:32.64 AT 2026jct 2026-04-09.53 20.16
14:15:21.948 -35:02:48.79 AT 2026jcs 2026-04-09.59 19.67
12:55:53.000 +08:04:22.00 AT 2026jcr 2026-04-09.62 22.1051
12:29:42.630 -28:00:38.18 AT 2026jcq 2026-04-09.56 18.99
13:00:14.826 -06:35:50.60 AT 2026jcp 2026-04-09.56 19.7
12:54:45.376 +09:10:41.41 AT 2026jco 2026-04-09.62 20.9256
13:25:12.570 -33:30:18.80 AT 2026jcn 2026-04-07.60 19.74
13:20:52.501 -35:57:03.67 AT 2026jcm 2026-04-07.60 20.01
12:07:08.367 +13:12:39.86 AT 2026jcl 2026-04-09.62 22.8073
12:11:43.063 +14:00:46.62 AT 2026jck 2026-04-09.62 21.8834
14:57:35.040 -17:11:22.89 AT 2026jcj 2026-04-09.58 19.52
15:09:26.181 -10:41:27.18 AT 2026jci 2026-04-09.45 20.2
18:22:34.467 +53:35:59.16 AT 2026jch 2026-04-05.40 19.7444
15:13:25.280 +39:43:46.60 AT 2026jcg 2026-03-30.81 21.1
17:32:02.830 +27:34:31.03 AT 2026jcf 2026-03-27.92 21.46
-rw-r--r-- 1 apache apache 30K Apr 16 21:56 tns_transients_list.txt
